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class="vector-toc-link" href="#Candidates_for_largest_exoplanets"> <div class="vector-toc-text"> 3 Candidates for largest exoplanets </div> </a> <button aria-controls="toc-Candidates_for_largest_exoplanets-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> Toggle Candidates for largest exoplanets subsection </button> <ul id="toc-Candidates_for_largest_exoplanets-sublist" class="vector-toc-list"> <li id="toc-Unconfirmed_exoplanets" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Unconfirmed_exoplanets"> <div class="vector-toc-text"> 3.1 Unconfirmed exoplanets </div> </a> <ul id="toc-Unconfirmed_exoplanets-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Exoplanets_with_uncertain_radii" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Exoplanets_with_uncertain_radii"> <div class="vector-toc-text"> 3.2 Exoplanets with uncertain radii </div> </a> <ul id="toc-Exoplanets_with_uncertain_radii-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Chronological_list_of_largest_exoplanets" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Chronological_list_of_largest_exoplanets"> <div class="vector-toc-text"> 4 Chronological list of largest exoplanets </div> </a> <ul id="toc-Chronological_list_of_largest_exoplanets-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-See_also" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#See_also"> <div class="vector-toc-text"> 5 See also </div> </a> <ul id="toc-See_also-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Notes" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Notes"> <div class="vector-toc-text"> 6 Notes </div> </a> <ul id="toc-Notes-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-References" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#References"> <div class="vector-toc-text"> 7 References </div> </a> <ul id="toc-References-sublist" class="vector-toc-list"> </ul> </li> </ul> </div> </div> </nav> </div> </div> <div class="mw-content-container"> <main id="content" class="mw-body"> <header class="mw-body-header vector-page-titlebar"> <nav aria-label="Contents" class="vector-toc-landmark"> <div id="vector-page-titlebar-toc" class="vector-dropdown vector-page-titlebar-toc vector-button-flush-left" > <input type="checkbox" id="vector-page-titlebar-toc-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-page-titlebar-toc" class="vector-dropdown-checkbox " aria-label="Toggle the table of contents" > <label id="vector-page-titlebar-toc-label" for="vector-page-titlebar-toc-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button 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srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif/368px-790106-0203_Voyager_58M_to_31M_reduced.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif 2x" data-file-width="390" data-file-height="400" /></a><figcaption><a href="/wiki/Jupiter" title="Jupiter">Jupiter</a> as seen by <a href="/wiki/Voyager_1" title="Voyager 1">Voyager 1</a> in 1979. It is the largest <a href="/wiki/Planet" title="Planet">planet</a> having its surface resolved<a href="#cite_note-8hZ77-1">[1]</a><a href="#cite_note-EKWXb-2">[2]</a><a href="#cite_note-UxcVg-3">[3]</a> and it is the largest <a href="/wiki/Planet" title="Planet">planet</a> in the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>.<a href="#cite_note-Ujyhy-4">[4]</a></figcaption></figure> Below is a list of the largest <a href="/wiki/Exoplanet" title="Exoplanet">exoplanets</a> so far discovered, in terms of physical size, ordered by radius. <meta property="mw:PageProp/toc" /> <div class="mw-heading mw-heading2"><h2 id="Limitations">Limitations</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=1" title="Edit section: Limitations">edit</a>]</div> This list of extrasolar objects may and will change over time due to diverging measurements published between scientific journals, varying methods used to examine these objects, and the notably difficult task of discovering extrasolar objects in general. These objects are not stars, and are quite small on a universal or even stellar scale. Then there is the fact that these objects might be <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarfs</a>, <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarfs</a>, or not exist at all. Because of this, this list only cites the most certain measurements to date and is prone to change. <div class="mw-heading mw-heading2"><h2 id="List">List</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=2" title="Edit section: List">edit</a>]</div> The sizes are listed in units of <a href="/wiki/Jupiter_radius" title="Jupiter radius">Jupiter radii</a> (<var>R</var>J, 71 492 km). This list is designed to include all planets that are larger than 1.7 times the size of <a href="/wiki/Jupiter" title="Jupiter">Jupiter</a>. Some well-known planets that are smaller than 1.7 <var>R</var>J (19.055 R🜨 or 121536.4 km) have been included for the sake of comparison. <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (classification) </caption> <tbody><tr> <td bgcolor="#FFF8DC" width="50px" style="text-align:center;">* </td> <th>Probably brown dwarfs (≳ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) (based on mass) </th></tr> <tr> <td bgcolor="#FFE8DC" width="50px" style="text-align:center;">† </td> <th>Probably sub-brown dwarfs (based on mass and location) </th></tr> <tr> <td bgcolor="#cff7c1" width="50px" style="text-align:center;">? </td> <th>Status uncertain </th></tr> <tr> <td style="text-align:center;">← </td> <th>Probably planets (≲ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) (based on mass) </th></tr> <tr> <td bgcolor="#CEE0F2" width="50px" style="text-align:center;">→ </td> <th>Planets with grazing transit, hindering radius determination </th></tr> <tr> <td bgcolor="pink" width="50px" style="text-align:center;"># </td> <th>Notable non-exoplanets reported for reference </th></tr> <tr> <td bgcolor="#e6e6e6" width="50px" style="text-align:center;">– </td> <th>Theoretical planet size restrictions </th></tr></tbody></table> </div> <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (illustration) </caption> <tbody><tr> <td style="border:5px ridge red;"> </td> <th>Artist's impression </th></tr> <tr> <td style="border:5px ridge yellow;"> </td> <th>Artist's size comparison </th></tr> <tr> <td style="border:5px ridge orange;"> </td> <th>Artist's impression and size comparison </th></tr> <tr> <td style="border:5px ridge blue;"> </td> <th>Direct imaging telescopic observation </th></tr> <tr> <td style="border:5px ridge cyan;"> </td> <th>Direct image size comparison </th></tr> <tr> <td style="border:5px ridge green;"> </td> <th>Composite image of direct observations </th></tr> <tr> <td 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.sticky-header>thead>tr:first-child,body.skin-timeless .mw-parser-output .sticky-header>caption+tbody>tr:first-child,body.skin-timeless .mw-parser-output .sticky-header>tbody:first-child>tr:first-child,body.skin-timeless .mw-parser-output .sticky-header-multi>thead{top:3.51em}}@media screen and (max-width:639px){body.skin-minerva .mw-parser-output .sticky-header,body.skin-minerva .mw-parser-output .sticky-header-multi,body.skin-monobook .mw-parser-output .sticky-header,body.skin-monobook .mw-parser-output .sticky-header-multi,body.skin-vector-legacy .mw-parser-output .sticky-header,body.skin-vector-legacy .mw-parser-output .sticky-header-multi,body.skin-vector-2022 .mw-parser-output .sticky-header,body.skin-vector-2022 .mw-parser-output .sticky-header-multi{display:table}body.skin-minerva .mw-parser-output .sticky-header>caption,body.skin-minerva .mw-parser-output .sticky-header-multi>caption{display:table-caption}}@media screen{html.skin-theme-clientpref-night body.skin-minerva .mw-parser-output .sticky-header-multi.wikitable{background-color:#101418}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os body.skin-minerva .mw-parser-output .sticky-header-multi.wikitable{background-color:#101418}}</style> <table class="wikitable sortable sticky-header"> <tbody><tr> <th class="unsortable">Illustration </th> <th>Name (Alternates) </th> <th data-sort-type="number">Radius (<a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>) </th> <th class="unsortable">Key </th> <th data-sort-type="number">Mass (<a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) </th> <th class="unsortable">Notes </th></tr> <tr style="background:pink;"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:The_Sun_in_white_light.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/The_Sun_in_white_light.jpg/112px-The_Sun_in_white_light.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/The_Sun_in_white_light.jpg/168px-The_Sun_in_white_light.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/The_Sun_in_white_light.jpg/224px-The_Sun_in_white_light.jpg 2x" data-file-width="3379" data-file-height="3379" /></a> </td> <td><a href="/wiki/Sun" title="Sun">Sun</a> (Sol) </td> <td data-sort-value="9.731">9.731 (1 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>)<a href="#cite_note-Prša-2016-5">[5]</a> <a href="/wiki/Solar_radius" title="Solar radius">(695 700 km)</a> </td> <td style="text-align:center;"># </td> <td data-sort-value="1047.569">1047.569 (1 <a href="/wiki/Solar_mass" title="Solar mass">M☉</a>)<a href="#cite_note-Prša-2016-5">[5]</a> <a href="/wiki/Solar_mass" title="Solar mass">(1.988 416 x 1030 kg)</a> </td> <td>The only star in the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>. Responsible for <a href="/wiki/Life" title="Life">life</a> on <a href="/wiki/Earth" title="Earth">Earth</a> and keeping the <a href="/wiki/Solar_System_planets" class="mw-redirect" title="Solar System planets">planets</a> on orbit. Age: 4.6 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a>.<a href="#cite_note-Bonanno-6">[6]</a> Reported for reference. </td></tr> <tr style="background:#e6e6e6"> <td> </td> <td>Maximum size of Planetary-mass Object </td> <td data-sort-value="8">8<a href="#cite_note-Chabrier-2014-7">[7]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="5">~ 5<a href="#cite_note-Chabrier-2014-7">[7]</a> </td> <td>Maximum theoretical size limit assumed for a ~ 5 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a> mass object right after formation, however, for 'arbitrary initial conditions'. </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge green; background: #000000; text-align:center;"><a href="/wiki/File:Proplyd_133-353_HST_F775W_image.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/0a/Proplyd_133-353_HST_F775W_image.jpg/112px-Proplyd_133-353_HST_F775W_image.jpg" decoding="async" width="112" height="69" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0a/Proplyd_133-353_HST_F775W_image.jpg/168px-Proplyd_133-353_HST_F775W_image.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0a/Proplyd_133-353_HST_F775W_image.jpg/224px-Proplyd_133-353_HST_F775W_image.jpg 2x" data-file-width="807" data-file-height="499" /></a> </td> <td><a href="/w/index.php?title=Proplyd_133-353&action=edit&redlink=1" class="new" title="Proplyd 133-353 (page does not exist)">Proplyd 133-353</a> </td> <td data-sort-value="7.82">< 7.82 ± 0.81<a href="#cite_note-Fang-2016-8">[8]</a><a href="#cite_note-L/Teff-9">[a]</a> (< 0.804 ± 0.083 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>) </td> <td style="text-align:center;">† </td> <td data-sort-value="13">≤ 13, 2–28<a href="#cite_note-Fang-2016-8">[8]</a> </td> <td>A <a href="/wiki/Rogue_planet#List" title="Rogue planet">candidate</a> <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>/<a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a> with a <a href="/wiki/Photoevaporation" title="Photoevaporation">photoevaporating</a> disk. It is located in the <a href="/wiki/Orion_Nebula" title="Orion Nebula">Orion Nebula Cluster</a>. At an age younger than 500 000 years, it is one of the youngest free-floating <a href="/wiki/Planetary-mass_object" title="Planetary-mass object">planetary-mass object</a> candidates known. More information about Proplyd 133-353 and estimates of its radius are available: <a href="#cite_note-13">[e]</a> </td></tr> <tr style="background:pink;"> <td style="border:5px ridge red; background:#5e2113; text-align:center;" rowspan="2"><a href="/wiki/File:2MASS_J05352184%E2%80%930546085.tif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/2MASS_J05352184%E2%80%930546085.tif/lossy-page1-112px-2MASS_J05352184%E2%80%930546085.tif.jpg" decoding="async" width="112" height="110" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/2MASS_J05352184%E2%80%930546085.tif/lossy-page1-168px-2MASS_J05352184%E2%80%930546085.tif.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/2MASS_J05352184%E2%80%930546085.tif/lossy-page1-224px-2MASS_J05352184%E2%80%930546085.tif.jpg 2x" data-file-width="1200" data-file-height="1175" /></a> </td> <td><a href="/wiki/2M0535-05" class="mw-redirect" title="2M0535-05">2M0535-05 A</a> (V2384 Orionis A) </td> <td data-sort-value="6.71">6.71 ± 0.11<a href="#cite_note-Gómez_Maqueo_Chew-2009-14">[9]</a> (0.690 ± 0.011 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="59.9">59.9 ± 3.5<a href="#cite_note-Gómez_Maqueo_Chew-2009-14">[9]</a> (0.0572 ± 0.0033 <a href="/wiki/Solar_mass" title="Solar mass">M☉</a>) </td> <td rowspan="2">First <a href="/wiki/Eclipsing_binary" class="mw-redirect" title="Eclipsing binary">eclipsing binary</a> <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a> system to be discovered, orbiting around 9.8 days.<a href="#cite_note-Stassun2006-15">[10]</a><a href="#cite_note-hubblesite2006-16">[11]</a> Age: ~1 <a href="/wiki/Million_years_ago" title="Million years ago">Myr</a>.<a href="#cite_note-:21-17">[12]</a> Reported for reference. </td></tr> <tr style="background:pink;"> <td><a href="/wiki/2M0535-05" class="mw-redirect" title="2M0535-05">2M0535-05 B</a> (V2384 Orionis B) </td> <td data-sort-value="5.25">5.25 ± 0.09<a href="#cite_note-Gómez_Maqueo_Chew-2009-14">[9]</a> (0.540 ± 0.009 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="38.3">38.3 ± 2.3<a href="#cite_note-Gómez_Maqueo_Chew-2009-14">[9]</a> (0.0366 ± 0.0022 <a href="/wiki/Solar_mass" title="Solar mass">M☉</a>) </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=KPNO-Tau-4&action=edit&redlink=1" class="new" title="KPNO-Tau-4 (page does not exist)">KPNO-Tau-4</a> </td> <td data-sort-value="4.1">4.1<a href="#cite_note-Kraus-2006-18">[13]</a><a href="#cite_note-l60e2-19">[14]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="10.51">10.5<a href="#cite_note-Kraus-2006-18">[13]</a> </td> <td>A member of Taurus-Auriga star-forming region.<a href="#cite_note-l60e2-19">[14]</a> </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:The_Sub-Stellar_Companion_to_GQ_Lupi.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/112px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg" decoding="async" width="112" height="93" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/168px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/224px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg 2x" data-file-width="1116" data-file-height="930" /></a> </td> <td><a href="/wiki/GQ_Lupi_b" title="GQ Lupi b">GQ Lupi b</a> (GQ Lup Ab, GQ Lup B) </td> <td data-sort-value="3.7">3.50+1.50 −1.03<a href="#cite_note-Seifahrt07-20">[15]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="20">20 ± 10;<a href="#cite_note-Sun-2024-21">[16]</a> 1 – 46 </td> <td>Second <a href="/wiki/Exoplanet" title="Exoplanet">exoplanet</a> to be directly imaged (after <a href="/wiki/2M1207_b" class="mw-redirect" title="2M1207 b">2M1207 b</a>). GQ Lupi b has a mass of 1 – 46 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>; in the higher half of this range, it may be classified as a young brown dwarf. It should not be confused with the star GQ Lup C (2MASS J15491331), 2400 AU away, sometimes referred to as GQ Lup B.<a href="#cite_note-Alcala2020-22">[17]</a> Other sources of the radius include: 3.7±0.7 <var>R</var>J<a href="#cite_note-Xuan-2024-23">[18]</a> and 3.77 <var>R</var>J.<a href="#cite_note-WDjss-24">[19]</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=2MASS_J0437%2B2331&action=edit&redlink=1" class="new" title="2MASS J0437+2331 (page does not exist)">2MASS J0437+2331</a> </td> <td data-sort-value="3.30">3.30<a href="#cite_note-:17-25">[20]</a><a href="#cite_note-L/Teff-9">[a]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="7.1">7.1 +1.1 −1.0<a href="#cite_note-:17-25">[20]</a> </td> <td>May be a <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a> or a <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a> </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Brown_dwarf_OTS_44_with_disc.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Brown_dwarf_OTS_44_with_disc.jpg/112px-Brown_dwarf_OTS_44_with_disc.jpg" decoding="async" width="112" height="90" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Brown_dwarf_OTS_44_with_disc.jpg/168px-Brown_dwarf_OTS_44_with_disc.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/8b/Brown_dwarf_OTS_44_with_disc.jpg/224px-Brown_dwarf_OTS_44_with_disc.jpg 2x" data-file-width="3000" data-file-height="2400" /></a> </td> <td><a href="/wiki/OTS_44" title="OTS 44">OTS 44</a> </td> <td data-sort-value="3.2">3.2 – 3.6<a href="#cite_note-Bonnefoy-2014-26">[21]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="11.51">11.5<a href="#cite_note-LVyQ3-27">[22]</a> </td> <td><a href="/wiki/Rogue_planet#List" title="Rogue planet">First discovered</a> <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>; very likely a <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a><a href="#cite_note-apj620_1_L51-28">[23]</a> or <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a>.<a href="#cite_note-joergens2013_AA558-29">[24]</a> It is surrounded by a circumstellar disk of dust and particles of rock and ice. The currently preferred radius estimate is done by SED modelling including substellar object and disk model.<a href="#cite_note-Bonnefoy-2014-26">[21]</a> </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:Brown_dwarf_2M_J044144_and_planet.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/d1/Brown_dwarf_2M_J044144_and_planet.jpg/112px-Brown_dwarf_2M_J044144_and_planet.jpg" decoding="async" width="112" height="70" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d1/Brown_dwarf_2M_J044144_and_planet.jpg/168px-Brown_dwarf_2M_J044144_and_planet.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d1/Brown_dwarf_2M_J044144_and_planet.jpg/224px-Brown_dwarf_2M_J044144_and_planet.jpg 2x" data-file-width="1000" data-file-height="628" /></a> </td> <td><a href="/wiki/2MASS_J0441%2B2301" title="2MASS J0441+2301">2M J044144 b</a> (2M0441+23 Bb) </td> <td data-sort-value="3.06">3.06<a href="#cite_note-Bowler-2015-30">[25]</a><a href="#cite_note-L/Teff-9">[a]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="9.8">9.8 ± 1.8<a href="#cite_note-Bowler-2015-30">[25]</a> </td> <td>Based on the mass ratio to <a href="/wiki/2MASS_J0441%2B2301" title="2MASS J0441+2301">2M J044145 A</a> (2M0441+23 Aa) of 200 +100 −50 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a> it is probably not a <a href="/wiki/Exoplanet" title="Exoplanet">planet</a> according to the exoplanet working definition.<a href="#cite_note-1YDdZ-31">[26]</a> </td></tr> <tr style="background:pink;"> <td style="border:5px ridge orange; background:#000000; text-align:center;"><a href="/wiki/File:Kapteyn%27s_Star_Comparison.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/17/Kapteyn%27s_Star_Comparison.jpg/112px-Kapteyn%27s_Star_Comparison.jpg" decoding="async" width="112" height="76" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/17/Kapteyn%27s_Star_Comparison.jpg/168px-Kapteyn%27s_Star_Comparison.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/17/Kapteyn%27s_Star_Comparison.jpg/224px-Kapteyn%27s_Star_Comparison.jpg 2x" data-file-width="536" data-file-height="363" /></a> </td> <td><a href="/wiki/Kapteyn%27s_Star" title="Kapteyn's Star">Kapteyn's Star</a> (HD 33793) </td> <td data-sort-value="2.83">2.83 ± 0.24<a href="#cite_note-Guinan-2016-32">[27]</a> (0.291 ± 0.025 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="294.4">294.4 ± 14.7<a href="#cite_note-Guinan-2016-32">[27]</a> (0.2810 ± 0.014 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td>The closest <a href="/wiki/Galactic_halo" title="Galactic halo">halo</a> star / <a href="/wiki/Red_dwarf" title="Red dwarf">red</a> <a href="/wiki/Subdwarf" title="Subdwarf">subdwarf</a>, at the distance of 12.82 ly (3.93 pc), and second-highest <a href="/wiki/Proper_motion" title="Proper motion">proper motion</a> of any stars of more than 8 <a href="/wiki/Arcseconds" class="mw-redirect" title="Arcseconds">arcseconds</a> per year (after the <a href="/wiki/Barnard%27s_Star" title="Barnard's Star">Barnard's Star</a>). Also the nearest star that orbits the <a href="/wiki/Milky_Way" title="Milky Way">galaxy</a> <a href="/wiki/Retrograde_motion" class="mw-redirect" title="Retrograde motion">backward</a>. Age: 11.5 +0.5 −1.5 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a>.<a href="#cite_note-Kapteyn-33">[28]</a> Reported for reference. </td></tr> <tr style="background:#cff7c1"> <td style="border:5px ridge blue; background: white; text-align:center;"><a href="/wiki/File:Subaru_AB_Aur_b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Subaru_AB_Aur_b.png/112px-Subaru_AB_Aur_b.png" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Subaru_AB_Aur_b.png/168px-Subaru_AB_Aur_b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/ea/Subaru_AB_Aur_b.png/224px-Subaru_AB_Aur_b.png 2x" data-file-width="3950" data-file-height="3950" /></a> </td> <td><a href="/wiki/AB_Aurigae_b" title="AB Aurigae b">AB Aurigae b</a> (AB Aur b) </td> <td data-sort-value="2.75">2.75<a href="#cite_note-Currie-2022-34">[29]</a> </td> <td style="text-align:center;">? </td> <td data-sort-value="20">20 (~ 4 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>)<a href="#cite_note-Ginski2022-35">[30]</a> < 130, 9 – 12 (1 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>)<a href="#cite_note-Currie-2022-34">[29]</a> </td> <td>Assuming a Hot-start evolutionary model and a planetary-mass, AB Aurigae b would be younger than 3 million years to have its observed large luminosity (and hence radius). This is inconsistent with the age of the host star, determined at 6.0 +2.5 −1.0 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>, and could imply delayed planet formation in the disk.<a href="#cite_note-hBkQl-36">[31]</a> Other system ages include 1 - 5 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>,<a href="#cite_note-Currie-2022-34">[29]</a> 4 ± 1 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a><a href="#cite_note-d9kt8-37">[32]</a> and 4 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>.<a href="#cite_note-38">[33]</a> Another source gives a higher mass of 20 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a> for an age of 4 <a href="/wiki/Megayear" class="mw-redirect" title="Megayear">Myr</a>, which is in the <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a> regime, arguing since gravitational instability of the disk (the preferred formation mechanism in the discovery publication)<a href="#cite_note-Currie-2022-34">[29]</a> operates on very short time scales the object might be as old as the central star <a href="/wiki/AB_Aurigae" title="AB Aurigae">AB Aur</a>.<a href="#cite_note-Ginski2022-35">[30]</a> Previously there was evidence that AB Aur b might not exist, such as its <a href="/wiki/Visible_spectrum" title="Visible spectrum">optical</a>/<a href="/wiki/Ultraviolet" title="Ultraviolet">UV</a> being consistent with that of scattered light<a href="#cite_note-Zhou-2023-39">[34]</a> and its accretion rate being disputed,<a href="#cite_note-QBogM-40">[35]</a> but more recent analyses weaken the latter dispute and confirm evidence favouring the existence of the protoplanet.<a href="#cite_note-41">[36]</a><a href="#cite_note-Dykes2024-42">[37]</a> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:DH_Tauri.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/112px-DH_Tauri.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/168px-DH_Tauri.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/224px-DH_Tauri.jpg 2x" data-file-width="503" data-file-height="503" /></a> </td> <td><a href="/wiki/DH_Tauri_b" class="mw-redirect" title="DH Tauri b">DH Tauri b</a> (DH Tau b) </td> <td data-sort-value="2.7">2.7 ± 0.8<a href="#cite_note-zhou2014-43">[38]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="11.1">11 ± 3<a href="#cite_note-zhou2014-43">[38]</a> </td> <td>First planet to have a confirmed <a href="/wiki/Circumplanetary_disk" title="Circumplanetary disk">circumplanetary disk</a>, detected with <a href="/wiki/Polarimetry" title="Polarimetry">polarimetry</a> at the <a href="/wiki/Very_Large_Telescope" title="Very Large Telescope">VLT</a>.<a href="#cite_note-:8-44">[39]</a> DH Tauri b has itself an <a href="/wiki/List_of_exomoon_candidates" title="List of exomoon candidates">exomoon candidate</a> orbiting it every 320 years, with about the same mass as Jupiter.<a href="#cite_note-:7-45">[40]</a> Other sources give the radii: 2.49 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a><a href="#cite_note-Bonnefoy-2014-26">[21]</a><a href="#cite_note-L/Teff-9">[a]</a> and 2.6 ± 0.6 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a><a href="#cite_note-Xuan-2024-23">[18]</a> and masses: 14.2 +2.4 −3.5 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>,<a href="#cite_note-:5-46">[41]</a> 17 ± 6 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>,<a href="#cite_note-:6-47">[42]</a> 12 ± 4 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a><a href="#cite_note-Xuan-2024-23">[18]</a> </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge yellow; background:#000000"><a href="/wiki/File:Exoplanet_Comparison_CT_Chamaeleontis_b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Exoplanet_Comparison_CT_Chamaeleontis_b.png/112px-Exoplanet_Comparison_CT_Chamaeleontis_b.png" decoding="async" width="112" height="52" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Exoplanet_Comparison_CT_Chamaeleontis_b.png/168px-Exoplanet_Comparison_CT_Chamaeleontis_b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0e/Exoplanet_Comparison_CT_Chamaeleontis_b.png/224px-Exoplanet_Comparison_CT_Chamaeleontis_b.png 2x" data-file-width="1040" data-file-height="480" /></a> </td> <td><a href="/wiki/CT_Chamaeleontis_b" class="mw-redirect" title="CT Chamaeleontis b">CT Chamaeleontis b</a> (CT Cha b) </td> <td data-sort-value="2.6">2.6+1.2 −0.2<a href="#cite_note-Bonnefoy-2014-26">[21]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="17">17 ± 6<a href="#cite_note-Schmidt-2008-48">[43]</a> </td> <td>Likely a brown dwarf. </td></tr> <tr style="background:pink;"> <td style="border:5px ridge purple; background:white; text-align:center;" rowspan="2"><a href="/wiki/File:CMDraLightCurve.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/c/cb/CMDraLightCurve.png/112px-CMDraLightCurve.png" decoding="async" width="112" height="73" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/cb/CMDraLightCurve.png/168px-CMDraLightCurve.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/cb/CMDraLightCurve.png/224px-CMDraLightCurve.png 2x" data-file-width="1500" data-file-height="975" /></a> </td> <td><a href="/wiki/CM_Draconis" title="CM Draconis">CM Draconis A</a> (Gliese 630.1A A, KOI-126A A) </td> <td data-sort-value="2.44">2.4437 ± 0.0002<a href="#cite_note-Martin2024-49">[44]</a> (0.251 13 ± 0.000 16 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="235.8">235.8 ± 0.3<a href="#cite_note-Martin2024-49">[44]</a> (0.225 07 ± 0.000 24 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td rowspan="2">One of the lightest stars with precisely measured masses and radii, orbiting around 1.268 days. Age: 4.1 ± 0.8 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a>.<a href="#cite_note-50">[45]</a> Reported for reference. </td></tr> <tr style="background:pink;"> <td><a href="/wiki/CM_Draconis" title="CM Draconis">CM Draconis B</a> (Gliese 630.1A B, KOI-126A B) </td> <td data-sort-value="2.31">2.3094 ± 0.0001<a href="#cite_note-Martin2024-49">[44]</a> (0.237 32 ± 0.000 14 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="220.2">220.2 ± 0.3<a href="#cite_note-Martin2024-49">[44]</a> (0.210 17 ± 0.000 28 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td></tr> <tr style="background:#CEE0F2"> <td> </td> <td><a href="/w/index.php?title=TOI-1408_b&action=edit&redlink=1" class="new" title="TOI-1408 b (page does not exist)">TOI-1408 b</a> </td> <td data-sort-value="2.23">2.23 ± 0.36 (25±4 <a href="/wiki/Earth_radius" title="Earth radius">R🜨</a>), 2.4 ± 0.5<a href="#cite_note-Korth-2024-51">[46]</a> </td> <td style="text-align:center;">→ </td> <td data-sort-value="1.86">1.86 ± 0.02<a href="#cite_note-Korth-2024-51">[46]</a> </td> <td>Grazing and very puffy hot Jupiter.<a href="#cite_note-Korth-2024-51">[46]</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=TWA_29&action=edit&redlink=1" class="new" title="TWA 29 (page does not exist)">TWA 29</a> </td> <td data-sort-value="2.222">2.222 +0.082 −0.081<a href="#cite_note-Hurt-2024-52">[47]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="6.6">6.6 +5.2 −2.9<a href="#cite_note-Hurt-2024-52">[47]</a> </td> <td> </td></tr> <tr style="background:#e6e6e6"> <td> </td> <td>Old <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> limit </td> <td data-sort-value="2.2">2.2<a href="#cite_note-limit-53">[48]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="0.0000000000000000001">> 0 </td> <td>Theoretical limit for <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiters</a> close to a star, that are limited by <a href="/wiki/Tidal_heating" title="Tidal heating">tidal heating</a>, resulting in 'runaway inflation' </td></tr> <tr> <td style="border:5px ridge orange; background:#000000;"><a href="/wiki/File:Comparison_XO-6.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/112px-Comparison_XO-6.png" decoding="async" width="112" height="86" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/168px-Comparison_XO-6.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/224px-Comparison_XO-6.png 2x" data-file-width="1400" data-file-height="1070" /></a> </td> <td><a href="/wiki/XO-6b" title="XO-6b">XO-6b</a> </td> <td data-sort-value="2.17">2.17 ± 0.2<a href="#cite_note-Saha2024-54">[49]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="4.47">4.47 ± 0.12<a href="#cite_note-Saha2024-54">[49]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=PSO_J077.1%2B24&action=edit&redlink=1" class="new" title="PSO J077.1+24 (page does not exist)">PSO J077.1+24</a> </td> <td data-sort-value="2.14">2.14<a href="#cite_note-:17-25">[20]</a><a href="#cite_note-L/Teff-9">[a]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="5.9">5.9 +0.9 −0.8<a href="#cite_note-:17-25">[20]</a> </td> <td><a href="/wiki/Rogue_planet" title="Rogue planet">Rogue planet</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=CAHA_Tau_1&action=edit&redlink=1" class="new" title="CAHA Tau 1 (page does not exist)">CAHA Tau 1</a> </td> <td data-sort-value="2.12">2.12<a href="#cite_note-Quanz-2010-55">[50]</a><a href="#cite_note-Encyclopaedia_of_exoplanetary_systems_/_exoplanet.eu-56">[51]</a><a href="#cite_note-L/Teff-9">[a]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="10.001">10 ± 5<a href="#cite_note-Quanz-2010-55">[50]</a><a href="#cite_note-Encyclopaedia_of_exoplanetary_systems_/_exoplanet.eu-56">[51]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:ROXs_42B_MUSE_IR.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/112px-ROXs_42B_MUSE_IR.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/168px-ROXs_42B_MUSE_IR.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/224px-ROXs_42B_MUSE_IR.jpg 2x" data-file-width="443" data-file-height="443" /></a> </td> <td><a href="/wiki/ROXs_42Bb" title="ROXs 42Bb">ROXs 42B b</a> </td> <td data-sort-value="2.105">2.10 ± 0.35<a href="#cite_note-Xuan-2024-23">[18]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="9">9 +6 −3,<a href="#cite_note-:12-57">[52]</a> 10 ± 4<a href="#cite_note-:13-58">[53]</a> </td> <td>Older estimates include 1.9 – 2.4, 1.3 – 4.7 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a><a href="#cite_note-DaemgenROX-59">[54]</a> and 2.43±0.18, 2.55±0.2 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>.<a href="#cite_note-:14-60">[55]</a> Other recent sources of masses include 3.2 – 27 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-Inglis2024-61">[56]</a> 13 ± 5 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-Xuan-2024-23">[18]</a> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:PDS_70.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/112px-PDS_70.jpg" decoding="async" width="112" height="95" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/168px-PDS_70.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/224px-PDS_70.jpg 2x" data-file-width="2000" data-file-height="1692" /></a> </td> <td><a href="/wiki/PDS_70#Protoplanetary_disk" title="PDS 70">PDS 70 b</a> </td> <td data-sort-value="2.09">2.09 +0.23 −0.31 – 2.72 +0.15 −0.17<a href="#cite_note-Wang2020-62">[57]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="3.2">3.2 +3.3 −1.6, 7.9 +4.9 −4.7, < 10 (2 σ), ≲ 15 (total)<a href="#cite_note-Wang_王-2021-63">[58]</a> </td> <td>Possibly the largest known exoplanet.<a href="#cite_note-limit-53">[48]</a> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:WASP-76_b_(2020).png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/b/b2/WASP-76_b_%282020%29.png/111px-WASP-76_b_%282020%29.png" decoding="async" width="111" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/b2/WASP-76_b_%282020%29.png/167px-WASP-76_b_%282020%29.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/b2/WASP-76_b_%282020%29.png/222px-WASP-76_b_%282020%29.png 2x" data-file-width="600" data-file-height="605" /></a> </td> <td><a href="/wiki/WASP-76b" title="WASP-76b">WASP-76b</a> </td> <td data-sort-value="2.083">2.083 +0.083 −0.063<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.92">0.92 ± 0.03<a href="#cite_note-12EET-65">[60]</a><a href="#cite_note-zy4wf-66">[61]</a> </td> <td>WASP-76b is suspected to have an <a href="/wiki/List_of_exomoon_candidates#Table" title="List of exomoon candidates">exo-Io candidate</a> due to the sodium being detected via <a href="/wiki/Absorption_spectroscopy" title="Absorption spectroscopy">absorption spectroscopy</a> around WASP-76b.<a href="#cite_note-Xqd9O-67">[62]</a> </td></tr> <tr> <td style="border:5px ridge purple; background:white;"><a href="/wiki/File:Transit_light_curve_of_Hat-P-67b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/112px-Transit_light_curve_of_Hat-P-67b.png" decoding="async" width="112" height="76" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/168px-Transit_light_curve_of_Hat-P-67b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/224px-Transit_light_curve_of_Hat-P-67b.png 2x" data-file-width="996" data-file-height="675" /></a> </td> <td><a href="/wiki/HAT-P-67b" class="mw-redirect" title="HAT-P-67b">HAT-P-67b</a> </td> <td data-sort-value="2.038">2.038+0.068 −0.038,<a href="#cite_note-Saha2024-54">[49]</a> 2.165 +0.024 −0.022<a href="#cite_note-HatP67-68">[f]</a><a href="#cite_note-Gully-Santiago-69">[63]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.418">0.418±0.012<a href="#cite_note-Saha2024-54">[49]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a>. Previously the largest known planet with an accurately and precisely measured radius,<a href="#cite_note-largest-70">[64]</a> though a new estimate revised its radius.<a href="#cite_note-Saha2024-54">[49]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HATS-15b&action=edit&redlink=1" class="new" title="HATS-15b (page does not exist)">HATS-15b</a> </td> <td data-sort-value="2.019">2.019 +0.202 −0.160<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="2.17">2.17 ± 0.15<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge blue; background:#000053; text-align:center;"><a href="/wiki/File:WISE1109-7734_(with_marker,_edited).png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/WISE1109-7734_%28with_marker%2C_edited%29.png/112px-WISE1109-7734_%28with_marker%2C_edited%29.png" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/WISE1109-7734_%28with_marker%2C_edited%29.png/168px-WISE1109-7734_%28with_marker%2C_edited%29.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/71/WISE1109-7734_%28with_marker%2C_edited%29.png/223px-WISE1109-7734_%28with_marker%2C_edited%29.png 2x" data-file-width="437" data-file-height="438" /></a> </td> <td><a href="/wiki/Cha_110913-773444" class="mw-redirect" title="Cha 110913-773444">Cha 110913-773444</a> (Cha 110913) </td> <td data-sort-value="2.05">2.0 – 2.1<a href="#cite_note-Bonnefoy-2014-26">[21]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="8.001">8 +7 −3<a href="#cite_note-IM4rM-71">[65]</a> </td> <td><a href="/wiki/Rogue_planet#List" title="Rogue planet">First confirmed</a> <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>. A rogue planet/<a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a> that is surrounded by a <a href="/wiki/Protoplanetary_disk" title="Protoplanetary disk">protoplanetary disk</a>. It is one of youngest free-floating substellar objects with 0.5–10 <a href="/wiki/Myr" class="mw-redirect" title="Myr">Myr</a>. The currently preferred radius estimate is done by SED modelling including substellar object and disk model.<a href="#cite_note-Bonnefoy-2014-26">[21]</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=CFHTWIR-Oph_90&action=edit&redlink=1" class="new" title="CFHTWIR-Oph 90 (page does not exist)">CFHTWIR-Oph 90</a> </td> <td data-sort-value="2.001">2.00 +0.09 −0.12;<a href="#cite_note-Bryan-2020-72">[66]</a> 3<a href="#cite_note-rilinger-73">[67]</a><a href="#cite_note-l7XWJ-74">[68]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="10.5">10.5<a href="#cite_note-rilinger-73">[67]</a> </td> <td>May be <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a> or <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=SSTB213_J041757_a&action=edit&redlink=1" class="new" title="SSTB213 J041757 a (page does not exist)">SSTB213 J041757 a</a> </td> <td data-sort-value="2">2<a href="#cite_note-75">[69]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="3.5">3.5<a href="#cite_note-76">[70]</a> </td> <td>In a binary with a smaller 1.7 <var>R</var>J <a href="#SSTB213_J041757b">planet</a>. </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:WASP-17b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/112px-WASP-17b.jpg" decoding="async" width="112" height="104" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/168px-WASP-17b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/224px-WASP-17b.jpg 2x" data-file-width="2030" data-file-height="1883" /></a> </td> <td><a href="/wiki/WASP-17b" title="WASP-17b">Ditsö̀</a> (WASP-17b) </td> <td data-sort-value="1.991">1.991 ± 0.081<a href="#cite_note-Bonomo-2017b-77">[71]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.512">0.512 ± 0.037<a href="#cite_note-Bonomo-2017b-77">[71]</a> </td> <td>Extremely low density of 0.08 g/cm3.<a href="#cite_note-:3-78">[72]</a> Possibly largest exoplanet at the time of discovery.<a href="#cite_note-:4-79">[73]</a> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Kepler-435b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/68/Kepler-435b.png/112px-Kepler-435b.png" decoding="async" width="112" height="104" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/68/Kepler-435b.png/168px-Kepler-435b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/68/Kepler-435b.png/224px-Kepler-435b.png 2x" data-file-width="373" data-file-height="348" /></a> </td> <td><a href="/w/index.php?title=Kepler-435b&action=edit&redlink=1" class="new" title="Kepler-435b (page does not exist)">Kepler-435b</a> </td> <td data-sort-value="1.99">1.99 ± 0.18<a href="#cite_note-Almenara-2015-80">[74]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.84">0.84 ± 0.15<a href="#cite_note-Almenara-2015-80">[74]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/b/bb/Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg/112px-Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg" decoding="async" width="112" height="75" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/bb/Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg/168px-Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/bb/Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg/224px-Artist%27s_impression_of_the_planet_OGLE-TR-L9b.jpg 2x" data-file-width="2000" data-file-height="1333" /></a> </td> <td><a href="/wiki/OGLE2-TR-L9b" title="OGLE2-TR-L9b">OGLE2-TR-L9b</a> </td> <td data-sort-value="1.958">1.958+0.174 −0.111<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="4.5">4.5±1.5<a href="#cite_note-Johns-64">[59]</a> </td> <td>First discovered planet orbiting a fast-rotating hot star, <a href="/wiki/OGLE2-TR-L9" title="OGLE2-TR-L9">OGLE2-TR-L9</a>.<a href="#cite_note-disc-81">[75]</a> </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge blue; background:#000053; text-align:center;"><a href="/wiki/File:CFHTWIR-Oph_98_AB_WFC3.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/112px-CFHTWIR-Oph_98_AB_WFC3.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/168px-CFHTWIR-Oph_98_AB_WFC3.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/224px-CFHTWIR-Oph_98_AB_WFC3.jpg 2x" data-file-width="456" data-file-height="456" /></a> </td> <td><a href="/wiki/CFHTWIR-Oph_98" class="mw-redirect" title="CFHTWIR-Oph 98">CFHTWIR-Oph 98 A</a> </td> <td data-sort-value="1.95">1.95+0.11 −0.10;<a href="#cite_note-Bryan-2020-72">[66]</a> 2.14<a href="#cite_note-rilinger-73">[67]</a><a href="#cite_note-Encyclopaedia_of_exoplanetary_systems_/_Exoplanet.eu-82">[76]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="15.4">15.4 ± 0.8;<a href="#cite_note-Fontanive-2020-83">[77]</a> 10.5<a href="#cite_note-rilinger-73">[67]</a> </td> <td>Either a <a href="/wiki/M-type_star" class="mw-redirect" title="M-type star">M-type</a> <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a> or <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a> with a sub-brown dwarf/<a href="/wiki/Exoplanet" title="Exoplanet">planet</a> companion <a href="/wiki/CFHTWIR-Oph_98_b" title="CFHTWIR-Oph 98 b">CFHTWIR-Oph 98 b</a>. Other sources of masses includes: 9.6 – 18.4 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-Fontanive-2020-83">[77]</a> </td></tr> <tr> <td> </td> <td><a href="/wiki/WASP-178b" title="WASP-178b">WASP-178b</a> (KELT-26 b) </td> <td data-sort-value="1.940">1.940 +0.060 −0.058<a href="#cite_note-Martínez-2020-84">[78]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.41">1.41 +0.43 −0.51<a href="#cite_note-Martínez-2020-84">[78]</a> </td> <td>An <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">ultra-hot Jupiter</a>. Initially, the planet's atmosphere was discovered having <a href="/wiki/Silicon_monoxide" title="Silicon monoxide">silicon monoxide</a>, making this exoplanet the first one to have the <a href="/wiki/Chemical_compound" title="Chemical compound">compound</a> on its atmosphere,<a href="#cite_note-Lothringer2022-85">[79]</a> now the atmosphere is more likely dominated by <a href="/wiki/Ionized" class="mw-redirect" title="Ionized">ionized</a> <a href="/wiki/Magnesium" title="Magnesium">magnesium</a> and <a href="/wiki/Iron" title="Iron">iron</a>.<a href="#cite_note-Damasceno2024-86">[80]</a> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:WASP-12b_a_Hot,_Carbon-Rich_Planet.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg/112px-WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg" decoding="async" width="112" height="84" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/29/WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg/168px-WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/29/WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg/224px-WASP-12b_a_Hot%2C_Carbon-Rich_Planet.jpg 2x" data-file-width="3200" data-file-height="2400" /></a> </td> <td><a href="/wiki/WASP-12b" title="WASP-12b">WASP-12b</a> </td> <td data-sort-value="1.937">1.937 ± 0.056<a href="#cite_note-WRrrL-87">[81]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.476">1.47 +0.076 −0.069<a href="#cite_note-collins-88">[82]</a> </td> <td>This planet is so close to its parent star that its tidal forces are distorting it into an egg-like shape. As of September 2017, it has been described as "black as asphalt", and as a "pitch black" hot Jupiter as it absorbs 94% of the starlight that reaches its surface. The planet will be destroyed in 3.16 ± 0.10 <a href="/wiki/Annum" class="mw-redirect" title="Annum">Ma</a> due to <a href="/wiki/Tidal_force" title="Tidal force">tidal interactions</a> between the planet and <a href="/wiki/WASP-12" title="WASP-12">WASP-12</a>.<a href="#cite_note-89">[83]</a><a href="#cite_note-90">[84]</a> WASP-12b is suspected to have <a href="/wiki/WASP-12b#Candidate_satellite" title="WASP-12b">one exomoon</a> due to a curve of change of shine of the planet observed regular variation of light.<a href="#cite_note-EytJY-91">[85]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=BD-14_3065_b&action=edit&redlink=1" class="new" title="BD-14 3065 b (page does not exist)">BD-14 3065 b</a> (TOI-4987 b) </td> <td data-sort-value="1.926">1.926 ± 0.094<a href="#cite_note-Šubjak-2024-92">[86]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="12.37">12.37 ± 0.92<a href="#cite_note-Šubjak-2024-92">[86]</a> </td> <td>Orbits the primary component, a subgiant star, of the triple star system. </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=KELT-19_Ab&action=edit&redlink=1" class="new" title="KELT-19 Ab (page does not exist)">KELT-19 Ab</a> </td> <td data-sort-value="1.91">1.91 ± 0.11<a href="#cite_note-Siverd-2017-93">[87]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="4.07">< 4.07 (3 σ)<a href="#cite_note-Siverd-2017-93">[87]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/112px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg" decoding="async" width="112" height="70" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/168px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/224px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg 2x" data-file-width="5000" data-file-height="3144" /></a> </td> <td><a href="/wiki/Dimidium" class="mw-redirect" title="Dimidium">Dimidium</a> (51 Peg b) </td> <td data-sort-value="1.9">1.9 ± 0.3<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.46">0.46 +0.06 −0.01<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td>First exoplanet to be discovered orbiting a <a href="/wiki/Main_sequence" title="Main sequence">main-sequence</a> star. Prototype <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiter</a>. </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:PIA21472_-_Hottest_Hot_Jupiter_Animation_(Artist%27s_Concept).gif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/95/PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif/112px-PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif" decoding="async" width="112" height="63" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/95/PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif/168px-PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/95/PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif/224px-PIA21472_-_Hottest_Hot_Jupiter_Animation_%28Artist%27s_Concept%29.gif 2x" data-file-width="960" data-file-height="540" /></a> </td> <td><a href="/wiki/KELT-9b" title="KELT-9b">KELT-9b</a> </td> <td data-sort-value="1.891">1.891 +0.061 −0.055<a href="#cite_note-lNqlN-95">[89]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="2.171">2.17 ± 0.56<a href="#cite_note-qYLMK-96">[90]</a> </td> <td>Hottest confirmed exoplanet known, with a temperature of 4050±180 <a href="/wiki/Kelvin" title="Kelvin">K</a> (3776.85 ± 180 <a href="/wiki/Celsius" title="Celsius">°C</a>; 6830.33 ± 324 <a href="/wiki/Fahrenheit" title="Fahrenheit">°F</a>).<a href="#cite_note-scottgaudi-97">[91]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=TOI-1518_b&action=edit&redlink=1" class="new" title="TOI-1518 b (page does not exist)">TOI-1518 b</a> </td> <td data-sort-value="1.875">1.875 ± 0.053<a href="#cite_note-Cabot-2021-98">[92]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="2.29999">< 2.3 (2 σ)<a href="#cite_note-Cabot-2021-98">[92]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HAT-P-70b&action=edit&redlink=1" class="new" title="HAT-P-70b (page does not exist)">HAT-P-70b</a> </td> <td data-sort-value="1.87">1.87 +0.15 −0.10<a href="#cite_note-Zhou-2019-99">[93]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="6.78">< 6.78 (3 σ)<a href="#cite_note-Zhou-2019-99">[93]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=2MASS_J1935-2846&action=edit&redlink=1" class="new" title="2MASS J1935-2846 (page does not exist)">2MASS J1935-2846</a> </td> <td data-sort-value="1.869">1.869 ± 0.053<a href="#cite_note-:18-100">[94]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="7.4">7.4 +6.3 −3.4<a href="#cite_note-:18-100">[94]</a> </td> <td>May be a <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a> or <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>. </td></tr> <tr style="background:#CEE0F2"> <td> </td> <td><a href="/w/index.php?title=HATS-23b&action=edit&redlink=1" class="new" title="HATS-23b (page does not exist)">HATS-23b</a> </td> <td data-sort-value="1.866">1.86 +0.30 −0.40<a href="#cite_note-Bento-2017-101">[95]</a> </td> <td style="text-align:center;">→ </td> <td data-sort-value="1.4702">1.470 ± 0.072<a href="#cite_note-Bento-2017-101">[95]</a> </td> <td>Grazing planet </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge blue; background:#000053; text-align:center;"><a href="/wiki/File:CFHTWIR-Oph_98_AB_WFC3.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/112px-CFHTWIR-Oph_98_AB_WFC3.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/168px-CFHTWIR-Oph_98_AB_WFC3.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/83/CFHTWIR-Oph_98_AB_WFC3.jpg/224px-CFHTWIR-Oph_98_AB_WFC3.jpg 2x" data-file-width="456" data-file-height="456" /></a> </td> <td><a href="/wiki/CFHTWIR-Oph_98_b" title="CFHTWIR-Oph 98 b">CFHTWIR-Oph 98 b</a> </td> <td data-sort-value="1.865">1.86 ± 0.05<a href="#cite_note-NASAExoplanetArchive-102">[96]</a><a href="#cite_note-Encyclopaedia_of_exoplanetary_systems_/_Exoplanet.eu-82">[76]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="7.8">7.8 +0.7 −0.8<a href="#cite_note-Fontanive-2020-83">[77]</a> </td> <td>May be a <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a>. Other sources of mass includes 4.1 – 11.6 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-Fontanive-2020-83">[77]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=KELT-8b&action=edit&redlink=1" class="new" title="KELT-8b (page does not exist)">KELT-8b</a> </td> <td data-sort-value="1.86">1.86 +0.18 −0.16<a href="#cite_note-Fulton-2015-103">[97]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.867">0.867 +0.065 −0.061<a href="#cite_note-Fulton-2015-103">[97]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=KPNO-Tau-12&action=edit&redlink=1" class="new" title="KPNO-Tau-12 (page does not exist)">KPNO-Tau-12</a> </td> <td data-sort-value="1.84">1.84,<a href="#cite_note-Kraus-2006-18">[13]</a> 2.22 +0.11 −0.17<a href="#cite_note-Bryan-2020-72">[66]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="11.5">11.5<a href="#cite_note-rilinger-73">[67]</a> </td> <td>A member of Taurus-Auriga star-forming region.<a href="#cite_note-Kraus-2006-18">[13]</a> </td></tr> <tr> <td style="border:5px ridge orange; background:#000000; text-align:center;"><a href="/wiki/File:TrES-4.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/112px-TrES-4.jpg" decoding="async" width="112" height="67" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/168px-TrES-4.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/224px-TrES-4.jpg 2x" data-file-width="750" data-file-height="450" /></a> </td> <td><a href="/wiki/TrES-4b" title="TrES-4b">TrES-4</a> (GSC 02620-00648 b) </td> <td data-sort-value="1.838">1.838 +0.240 −0.238<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.78">0.78 ± 0.19<a href="#cite_note-Stassun-2017-104">[98]</a> </td> <td>This planet has a density of 0.17 g/cm3,<a href="#cite_note-Johns-64">[59]</a> about that of <a href="/wiki/Balsa_wood" class="mw-redirect" title="Balsa wood">balsa wood</a>, less than Saturn's 0.7 g/cm3. </td></tr> <tr> <td> </td> <td><a href="/wiki/HAT-P-33b" title="HAT-P-33b">HAT-P-33b</a> </td> <td data-sort-value="1.827">1.827 ± 0.29,<a href="#cite_note-o5qXL-105">[99]</a> 1.85±0.49<a href="#cite_note-NASAExoplanetArchive-102">[96]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.72">0.72 +0.13 −0.12<a href="#cite_note-Wang2017-106">[100]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/wiki/HAT-P-32b" title="HAT-P-32b">HAT-P-32b</a> </td> <td data-sort-value="1.822">1.822 +0.350 −0.236<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.941">0.941 ± 0.166, 0.860 ± 0.164<a href="#cite_note-6LQQh-107">[101]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a>. </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-112px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-168px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-224px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg 2x" data-file-width="990" data-file-height="990" /></a> </td> <td><a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1 b</a> (YSES 1 b) </td> <td data-sort-value="1.821">1.82 ± 0.08<a href="#cite_note-vb0fx-108">[102]</a> – 3.0 +0.2 −0.7<a href="#cite_note-The_Extrasolar_Planet_Encyclopaedia-1995-109">[103]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="21.8">21.8 ± 3<a href="#cite_note-Wood-2023-110">[104]</a> </td> <td>Likely a <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a>; first <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a> to be directly observed having more than one exoplanet (along with <a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1 c</a>) found orbiting around <a href="/wiki/Solar_analog" title="Solar analog">sun-like</a> <a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1</a>,<a href="#cite_note-Ri9R7-111">[105]</a><a href="#cite_note-a5T6A-112">[106]</a> whose age is 27 <a href="/wiki/Year#SI_prefix_multipliers" title="Year">Myr</a>.<a href="#cite_note-Wood-2023-110">[104]</a> First exoplanet to have an isotope (<a href="/wiki/Carbon-13" title="Carbon-13">13C</a>) in its atmosphere.<a href="#cite_note-SA-20210714-113">[107]</a><a href="#cite_note-vb0fx-108">[102]</a> </td></tr> <tr style="background:pink;"> <td style="border:5px ridge green; background:#000000; text-align:center;"><a href="/wiki/File:Barnard2005.gif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/6c/Barnard2005.gif/112px-Barnard2005.gif" decoding="async" width="112" height="99" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/6c/Barnard2005.gif/168px-Barnard2005.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/6c/Barnard2005.gif/224px-Barnard2005.gif 2x" data-file-width="308" data-file-height="273" /></a> </td> <td><a href="/wiki/Barnard%27s_Star" title="Barnard's Star">Barnard's Star</a> </td> <td data-sort-value="1.82">1.82 ± 0.01<a href="#cite_note-Pineda-2021-114">[108]</a> (0.187 ± 0.001 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="168.7">168.7 +3.8 −3.7<a href="#cite_note-Pineda-2021-114">[108]</a> (0.1610 +0.0036 −0.0035 <a href="/wiki/Solar_mass" title="Solar mass">M☉</a>) </td> <td>Second nearest <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a> to the <a href="/wiki/Sun" title="Sun">Sun</a> at the distance of 5.97 ly (1.83 pc) and closest star in the <a href="/wiki/Northern_celestial_hemisphere" title="Northern celestial hemisphere">northern celestial hemisphere</a>. Also the highest <a href="/wiki/Proper_motion" title="Proper motion">proper motion</a> of any stars of 10.3 <a href="/wiki/Arcseconds" class="mw-redirect" title="Arcseconds">arcseconds</a> per year relative to the Sun. Has a planet, <a href="/wiki/Barnard_b" class="mw-redirect" title="Barnard b">Barnard's Star b / Barnard b</a>.<a href="#cite_note-opzKZ-115">[109]</a> Reported for reference. </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:CoRoT-1.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/3/34/CoRoT-1.jpg/112px-CoRoT-1.jpg" decoding="async" width="112" height="84" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/34/CoRoT-1.jpg/168px-CoRoT-1.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/34/CoRoT-1.jpg/224px-CoRoT-1.jpg 2x" data-file-width="4000" data-file-height="3000" /></a> </td> <td><a href="/wiki/CoRoT-1b" title="CoRoT-1b">CoRoT-1b</a> </td> <td data-sort-value="1.805">1.805 +0.132 −0.131<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.03">1.03 ± 0.12<a href="#cite_note-Johns-64">[59]</a> </td> <td>First exoplanet for which optical (as opposed to <a href="/wiki/HD_189733_b#Map_of_the_planet" title="HD 189733 b">infrared</a>) observations of phases were reported.<a href="#cite_note-116">[110]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WTS-2b&action=edit&redlink=1" class="new" title="WTS-2b (page does not exist)">WTS-2b</a> </td> <td data-sort-value="1.804">1.804 +0.144 −0.158<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.12">1.12 ± 0.16<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:UAndAb_full.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/20/UAndAb_full.jpg/112px-UAndAb_full.jpg" decoding="async" width="112" height="84" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/20/UAndAb_full.jpg/168px-UAndAb_full.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/20/UAndAb_full.jpg/224px-UAndAb_full.jpg 2x" data-file-width="4060" data-file-height="3045" /></a> </td> <td><a href="/wiki/Upsilon_Andromedae_b" title="Upsilon Andromedae b">Saffar</a> (υ And b) </td> <td data-sort-value="1.8">~ 1.8<a href="#cite_note-kNo8y-117">[111]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.70">1.70 +0.33 −0.24<a href="#cite_note-s9bfg-118">[112]</a> </td> <td>Radius estimated using the phase curve of reflected light. The planet orbits very close to its host star of 0.0595 <a href="/wiki/Astronomical_unit" title="Astronomical unit">AU</a>, completing an orbit in 4.617 <a href="/wiki/Day" title="Day">days</a>.<a href="#cite_note-9JjuK-119">[113]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HAT-P-40b&action=edit&redlink=1" class="new" title="HAT-P-40b (page does not exist)">HAT-P-40b</a> </td> <td data-sort-value="1.799">1.799 +0.237 −0.260<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.48">0.48 ± 0.13<a href="#cite_note-Johns-64">[59]</a> </td> <td>A very puffy hot Jupiter. </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WASP-122b&action=edit&redlink=1" class="new" title="WASP-122b (page does not exist)">WASP-122b</a> (KELT-14b) </td> <td data-sort-value="1.795">1.795 +0.107 −0.079<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.284">1.284 ± 0.032<a href="#cite_note-Turner-2016-120">[114]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=KELT-12b&action=edit&redlink=1" class="new" title="KELT-12b (page does not exist)">KELT-12b</a> </td> <td data-sort-value="1.79">1.79 +0.18 −0.17<a href="#cite_note-Stevens-2017-121">[115]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.95">0.95 ± 0.14<a href="#cite_note-Stevens-2017-121">[115]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:WASP-121b_01.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/e4/WASP-121b_01.jpg/112px-WASP-121b_01.jpg" decoding="async" width="112" height="90" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/e4/WASP-121b_01.jpg/168px-WASP-121b_01.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/e4/WASP-121b_01.jpg/224px-WASP-121b_01.jpg 2x" data-file-width="4500" data-file-height="3600" /></a> </td> <td><a href="/wiki/WASP-121b" title="WASP-121b">Tylos</a> (WASP-121b) </td> <td data-sort-value="1.773">1.773 +0.041 −0.033<a href="#cite_note-Bourrier2020-122">[116]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.157">1.157 ± 0.07<a href="#cite_note-Bourrier2020-122">[116]</a> </td> <td>First exoplanet found to contain water in an extrasolar planetary stratosphere. Tylos is suspected to have <a href="/wiki/WASP-121b#Possible_exomoon" title="WASP-121b">exo-Io candidate</a> due to the sodium being detected via <a href="/wiki/Absorption_spectroscopy" title="Absorption spectroscopy">absorption spectroscopy</a> around the planet.<a href="#cite_note-Hoeijmakers2020-123">[117]</a> </td></tr> <tr> <td> </td> <td><a href="/wiki/TOI-640_b" title="TOI-640 b">TOI-640 b</a> </td> <td data-sort-value="1.771">1.771 +0.060 −0.056<a href="#cite_note-Rodriguez-2021-124">[118]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.88">0.88 ± 0.16<a href="#cite_note-Rodriguez-2021-124">[118]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WASP-187b&action=edit&redlink=1" class="new" title="WASP-187b (page does not exist)">WASP-187b</a> </td> <td data-sort-value="1.766">1.766 ± 0.036<a href="#cite_note-Saha2024-54">[49]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.801">0.801 +0.084 −0.083<a href="#cite_note-Saha2024-54">[49]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WASP-94_Ab&action=edit&redlink=1" class="new" title="WASP-94 Ab (page does not exist)">WASP-94 Ab</a> </td> <td data-sort-value="1.761">1.761 +0.194 −0.191<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.5">0.5±0.13<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=TOI-2669b&action=edit&redlink=1" class="new" title="TOI-2669b (page does not exist)">TOI-2669b</a> </td> <td data-sort-value="1.76">1.76 ± 0.16<a href="#cite_note-Grunblatt-2022-125">[119]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.61">0.61 ± 0.19<a href="#cite_note-Grunblatt-2022-125">[119]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=WISE_J0528%2B0901&action=edit&redlink=1" class="new" title="WISE J0528+0901 (page does not exist)">WISE J0528+0901</a> </td> <td data-sort-value="1.752">1.752 +0.292 −0.195<a href="#cite_note-:19-126">[120]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="13.001">13 +3 −6<a href="#cite_note-:19-126">[120]</a> </td> <td><a href="/wiki/Brown_dwarf" title="Brown dwarf">Brown dwarf</a> or <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>. </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HATS-26b&action=edit&redlink=1" class="new" title="HATS-26b (page does not exist)">HATS-26b</a> </td> <td data-sort-value="1.75">1.75 ± 0.21<a href="#cite_note-Espinoza-2016-127">[121]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.650">0.650 ± 0.076<a href="#cite_note-Espinoza-2016-127">[121]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/wiki/Kepler-12b" title="Kepler-12b">Kepler-12b</a> </td> <td data-sort-value="1.7454">1.7454 +0.076 −0.072<a href="#cite_note-Berger-2018-128">[122]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.431">0.431 ± 0.041<a href="#cite_note-Fortney-2011-129">[123]</a> </td> <td>The least-irradiated of four <a href="/wiki/Hot_Jupiters" class="mw-redirect" title="Hot Jupiters">Hot Jupiters</a> experiencing a radius anomaly at the time of its discovery. </td></tr> <tr> <td> </td> <td><a href="/wiki/HAT-P-65b" class="mw-redirect" title="HAT-P-65b">HAT-P-65b</a> </td> <td data-sort-value="1.744">1.744 +0.165 −0.215<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.527">0.527 ± 0.083<a href="#cite_note-Hartman-2016-130">[124]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=2MASS_J2352-1100&action=edit&redlink=1" class="new" title="2MASS J2352-1100 (page does not exist)">2MASS J2352-1100</a> </td> <td data-sort-value="1.742">1.742 +0.035 −0.036<a href="#cite_note-:18-100">[94]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="12.4">12.4 +9.4 −5.5<a href="#cite_note-:18-100">[94]</a> </td> <td><a href="/wiki/Brown_dwarf" title="Brown dwarf">Brown dwarf</a> or <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>. </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=KELT-15b&action=edit&redlink=1" class="new" title="KELT-15b (page does not exist)">KELT-15b</a> </td> <td data-sort-value="1.741">1.74 ± 0.20<a href="#cite_note-Stassun-2017-104">[98]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.31">1.31 ± 0.43<a href="#cite_note-Stassun-2017-104">[98]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HAT-P-57b&action=edit&redlink=1" class="new" title="HAT-P-57b (page does not exist)">HAT-P-57b</a> </td> <td data-sort-value="1.74">1.74 ± 0.36<a href="#cite_note-Stassun-2017-104">[98]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.4101">1.41 ± 1.52<a href="#cite_note-Stassun-2017-104">[98]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WASP-93b&action=edit&redlink=1" class="new" title="WASP-93b (page does not exist)">WASP-93b</a> </td> <td data-sort-value="1.737">1.737 +0.121 −0.170<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.47">1.47 ± 0.29<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td style="border:5px ridge red; background:#222222; text-align:center"><a href="/wiki/File:UHJ_KELT-20b.webp" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/6e/UHJ_KELT-20b.webp/112px-UHJ_KELT-20b.webp.png" decoding="async" width="112" height="63" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/6e/UHJ_KELT-20b.webp/168px-UHJ_KELT-20b.webp.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/6e/UHJ_KELT-20b.webp/224px-UHJ_KELT-20b.webp.png 2x" data-file-width="2048" data-file-height="1152" /></a> </td> <td><a href="/wiki/KELT-20b" title="KELT-20b">KELT-20b</a> (MASCARA-2b) </td> <td data-sort-value="1.735">1.735 +0.07 −0.075,<a href="#cite_note-Lund-2017-131">[125]</a> 1.741 +0.069 −0.074<a href="#cite_note-NASAExoplanetArchive-102">[96]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="3.518">< 3.518 (3 σ)<a href="#cite_note-Lund-2017-131">[125]</a> </td> <td>An <a href="/wiki/Ultra-hot_Jupiter" class="mw-redirect" title="Ultra-hot Jupiter">ultra-hot Jupiter</a>. </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=WASP-82b&action=edit&redlink=1" class="new" title="WASP-82b (page does not exist)">WASP-82b</a> </td> <td data-sort-value="1.726">1.726+0.163 −0.195<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.17">1.17±0.20<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HAT-P-39b&action=edit&redlink=1" class="new" title="HAT-P-39b (page does not exist)">HAT-P-39b</a> </td> <td data-sort-value="1.712">1.712+0.140 −0.115<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.599">0.60±0.10<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/wiki/KELT-4Ab" title="KELT-4Ab">KELT-4Ab</a> </td> <td data-sort-value="1.706">1.706 +0.085 −0.076<a href="#cite_note-KELT-4Ab-132">[126]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.878">0.878 +0.070 −0.067<a href="#cite_note-KELT-4Ab-132">[126]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/wiki/WASP-79b" title="WASP-79b">WASP-79b</a> </td> <td data-sort-value="1.704">1.704 +0.195 −0.180<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.850">0.850 +0.180 −0.180<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=HAT-P-64b&action=edit&redlink=1" class="new" title="HAT-P-64b (page does not exist)">HAT-P-64b</a> </td> <td data-sort-value="1.703">1.703 ± 0.070<a href="#cite_note-Bakos-2021-133">[127]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.58">0.58 +0.18 −0.13<a href="#cite_note-Bakos-2021-133">[127]</a> </td> <td> </td></tr> <tr> <td> </td> <td><a href="/wiki/WASP-78b" class="mw-redirect" title="WASP-78b">WASP-78b</a> </td> <td data-sort-value="1.702">1.70 ± 0.04,<a href="#cite_note-wasp7879-134">[128]</a> 1.93 ± 0.45<a href="#cite_note-NASAExoplanetArchive-102">[96]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.89">0.89 ± 0.08<a href="#cite_note-wasp7879-134">[128]</a> </td> <td>This planet has likely undergone in the past a migration from the initial highly eccentric orbit.<a href="#cite_note-arN27-135">[129]</a> </td></tr> <tr> <td> </td> <td><a href="/w/index.php?title=Qatar-7b&action=edit&redlink=1" class="new" title="Qatar-7b (page does not exist)">Qatar-7b</a> </td> <td data-sort-value="1.701">1.70 ± 0.03<a href="#cite_note-NASAExoplanetArchive-102">[96]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.88">1.88 ± 0.25<a href="#cite_note-hZi7q-136">[130]</a> </td> <td> </td></tr> <tr style="background:#FFE8DC"> <td> </td> <td><a href="/w/index.php?title=SSTB213_J041757_b&action=edit&redlink=1" class="new" title="SSTB213 J041757 b (page does not exist)">SSTB213 J041757 b</a> </td> <td data-sort-value="1.70">1.70<a href="#cite_note-137">[131]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="1.50">1.50<a href="#cite_note-138">[132]</a> </td> <td>In a binary with a larger 2 <var>R</var>J <a href="#SSTB213_J041757_a">planet</a>. </td></tr> <tr> <td> </td> <td><a href="/wiki/CoRoT-17b" title="CoRoT-17b">CoRoT-17b</a> </td> <td data-sort-value="1.694">1.694 +0.139 −0.193<a href="#cite_note-Johns-64">[59]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="2.430">2.430 +0.300 −0.300<a href="#cite_note-Johns-64">[59]</a> </td> <td> </td></tr> <tr> <th colspan="6" style="background:#efefef" data-sort-value="1.699999">A few notable examples with radii below 1.7 <var>R</var>J (19.1 <a href="/wiki/Earth_radius" title="Earth radius"><var>R</var>🜨</a>). </th></tr> <tr> <td style="border:5px ridge orange; background:#000000; text-align:center;"><a href="/wiki/File:Exoplanet_Comparison_Kepler-7_b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/14/Exoplanet_Comparison_Kepler-7_b.png/112px-Exoplanet_Comparison_Kepler-7_b.png" decoding="async" width="112" height="52" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/14/Exoplanet_Comparison_Kepler-7_b.png/168px-Exoplanet_Comparison_Kepler-7_b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/14/Exoplanet_Comparison_Kepler-7_b.png/224px-Exoplanet_Comparison_Kepler-7_b.png 2x" data-file-width="1040" data-file-height="480" /></a> </td> <td><a href="/wiki/Kepler-7b" title="Kepler-7b">Kepler-7b</a> </td> <td data-sort-value="1.574">1.574 +0.075 −0.071<a href="#cite_note-Berger-2018-128">[122]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.433">0.433 +0.040 −0.041<a href="#cite_note-qGKCN-139">[133]</a> </td> <td>First exoplanet to have a crude map of cloud coverage.<a href="#cite_note-NASA-20130930-140">[134]</a><a href="#cite_note-MIT-20131002-141">[135]</a><a href="#cite_note-ArXiv-20130930-142">[136]</a> One of the first five <a href="/wiki/Exoplanets" class="mw-redirect" title="Exoplanets">exoplanets</a> to be confirmed by <a href="/wiki/NASA" title="NASA">NASA</a>'s <a href="/wiki/Kepler_space_telescope" title="Kepler space telescope">Kepler</a> spacecraft, within 34 days of Kepler's science operations.<a href="#cite_note-Latham2010-143">[137]</a> </td></tr> <tr style="background:pink;"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/95/New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg/112px-New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg" decoding="async" width="112" height="110" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/95/New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg/168px-New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/95/New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg/224px-New_shot_of_Proxima_Centauri%2C_our_nearest_neighbour.jpg 2x" data-file-width="604" data-file-height="592" /></a> </td> <td><a href="/wiki/Proxima_Centauri" title="Proxima Centauri">Proxima Centauri</a> (Alpha Centauri C) </td> <td data-sort-value="1.50">1.50 ± 0.04<a href="#cite_note-KervellaThévenin2017-144">[138]</a> (0.1542 ± 0.0045 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="127.9">127.9 ± 2.3<a href="#cite_note-KervellaThévenin2017-144">[138]</a> (0.1221 ± 0.0022 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td>The <a href="/wiki/List_of_nearest_stars" title="List of nearest stars">nearest</a> star and <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a> to the <a href="/wiki/Sun" title="Sun">Sun</a>, at a distance of 4.24 <a href="/wiki/Light-year" title="Light-year">ly</a> (1.30 <a href="/wiki/Parsec" title="Parsec">pc</a>), orbiting around <a href="/wiki/Alpha_Centauri" title="Alpha Centauri">Alpha Centauri</a> <a href="/wiki/Alpha_Centauri#Alpha_Centauri_AB_System" title="Alpha Centauri">AB System</a>, the <a href="/wiki/List_of_nearest_stars" title="List of nearest stars">nearest star system</a> to the Sun. Age: 4.85 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a>.<a href="#cite_note-ESO2003-145">[139]</a> Has a confirmed planet, <a href="/wiki/Proxima_Centauri_b" title="Proxima Centauri b">Proxima Centauri b</a>,<a href="#cite_note-1vpJT-146">[140]</a> a disputed planet, <a href="/wiki/Proxima_Centauri_c" title="Proxima Centauri c">Proxima Centauri c</a>,<a href="#cite_note-ArtigauCadieux2022-147">[141]</a> and a unconfirmed planet, <a href="/wiki/Proxima_Centauri_d" title="Proxima Centauri d">Proxima Centauri d</a>. Reported for reference. </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge blue; background:#000000;"><a href="/wiki/File:PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/e2/PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png/112px-PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png" decoding="async" width="112" height="69" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/e2/PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png/168px-PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/e2/PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png/224px-PSO_J318.5-22_image_from_the_Pan-STARRS1_telescope.png 2x" data-file-width="959" data-file-height="595" /></a> </td> <td><a href="/wiki/PSO_J318.5%E2%88%9222" title="PSO J318.5−22">PSO J318.5−22</a> (2MASS J2114-22) </td> <td data-sort-value="1.464">1.464 +0.009 −0.008<a href="#cite_note-:20-148">[142]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="8.3">8.3 ± 0.5<a href="#cite_note-:20-148">[142]</a> </td> <td>There is no consensus yet among astronomers whether PSO J318.5-22 should be referred to as a <a href="/wiki/Rogue_planet" title="Rogue planet">rogue planet</a>,<a href="#cite_note-gemini_confirm-149">[143]</a> as a <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a>,<a href="#cite_note-Vos_M.-150">[144]</a> or as a young <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a>.<a href="#cite_note-Faherty_Jacqueline-151">[145]</a> </td></tr> <tr> <td style="border:5px ridge green; background:#000000; text-align:center;"><a href="/wiki/File:Beta_Pictoris.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Beta_Pictoris.jpg/112px-Beta_Pictoris.jpg" decoding="async" width="112" height="72" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Beta_Pictoris.jpg/168px-Beta_Pictoris.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a9/Beta_Pictoris.jpg/224px-Beta_Pictoris.jpg 2x" data-file-width="3000" data-file-height="1929" /></a> </td> <td><a href="/wiki/Beta_Pictoris_b" title="Beta Pictoris b">Beta Pictoris b</a> (β Pic b) </td> <td data-sort-value="1.46">1.46 ± 0.01<a href="#cite_note-vbdKI-152">[146]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="11.729">11.729 +2.337 −2.135<a href="#cite_note-o5PbX-153">[147]</a> </td> <td>Found by <a href="/wiki/Direct_imaging" class="mw-redirect" title="Direct imaging">direct imaging</a>. Orbit of ~24 years soon to be fully observed since its first epoch from 2003. </td></tr> <tr> <td style="border:5px ridge purple; background:white; text-align:center;"><a href="/wiki/File:V376PegLightCurve.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/112px-V376PegLightCurve.png" decoding="async" width="112" height="73" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/168px-V376PegLightCurve.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/224px-V376PegLightCurve.png 2x" data-file-width="1500" data-file-height="975" /></a> </td> <td><a href="/wiki/HD_209458_b" title="HD 209458 b">HD 209458 b</a> ("Osiris") </td> <td data-sort-value="1.359">1.359 +0.016 −0.019<a href="#cite_note-Bonomo-2017a-154">[148]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.682">0.682 +0.014 −0.015<a href="#cite_note-Bonomo-2017a-154">[148]</a> </td> <td>First known <a href="/wiki/Transiting_exoplanet" class="mw-redirect" title="Transiting exoplanet">transiting exoplanet</a>, first precisely measured radius available, first to have its orbital speed measured, determining its mass directly,<a href="#cite_note-Ignas-155">[149]</a> and to have an <a href="/wiki/Atmosphere" title="Atmosphere">atmosphere</a>, containing evaporating <a href="/wiki/Hydrogen" title="Hydrogen">hydrogen</a>, and <a href="/wiki/Oxygen" title="Oxygen">oxygen</a> and <a href="/wiki/Carbon" title="Carbon">carbon</a>. First extrasolar <a href="/wiki/Gas_giant" title="Gas giant">gas giant</a> to have its superstorm measured. Nicknamed "<a href="/wiki/Osiris" title="Osiris">Osiris</a>". </td></tr> <tr style="background:pink;"> <td style="border:5px ridge green; background:#000000; text-align:center;"><a href="/wiki/File:Pleiades_and_Teide_1.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Pleiades_and_Teide_1.png/116px-Pleiades_and_Teide_1.png" decoding="async" width="116" height="130" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Pleiades_and_Teide_1.png/174px-Pleiades_and_Teide_1.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Pleiades_and_Teide_1.png/232px-Pleiades_and_Teide_1.png 2x" data-file-width="1500" data-file-height="1681" /></a> </td> <td><a href="/wiki/Teide_1" title="Teide 1">Teide 1</a> </td> <td data-sort-value="1.311">1.311 +0.120 −0.075<a href="#cite_note-:2-156">[150]</a> (0.1347 +0.0123 −0.0077 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="52">52 +15 −10<a href="#cite_note-:2-156">[150]</a> (0.0496 +0.0143 −0.0095 <a href="/wiki/Solar_mass" title="Solar mass">M☉</a>) </td> <td>One of the first two <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarfs</a> to be confirmed.<a href="#cite_note-RafaelRebolo2014-157">[151]</a><a href="#cite_note-158">[152]</a> Age: 70 – 140 <a href="/wiki/Million_years_ago" title="Million years ago">Myr</a>.<a href="#cite_note-159">[153]</a> Reported for reference. </td></tr> <tr> <td style="border:5px ridge purple; background:white; text-align:center;"><a href="/wiki/File:OGLE-TR-56_b_rv.pdf" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/b/ba/OGLE-TR-56_b_rv.pdf/page1-112px-OGLE-TR-56_b_rv.pdf.jpg" decoding="async" width="112" height="80" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/b/ba/OGLE-TR-56_b_rv.pdf/page1-168px-OGLE-TR-56_b_rv.pdf.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/b/ba/OGLE-TR-56_b_rv.pdf/page1-224px-OGLE-TR-56_b_rv.pdf.jpg 2x" data-file-width="1583" data-file-height="1125" /></a> </td> <td><a href="/wiki/OGLE-TR-56b" title="OGLE-TR-56b">OGLE-TR-56b</a> </td> <td data-sort-value="1.30">1.30 ± 0.05 </td> <td style="text-align:center;">← </td> <td data-sort-value="1.29">1.29 ± 0.12 </td> <td>First discovered exoplanet using the <a href="/wiki/Transit_method" class="mw-redirect" title="Transit method">transit method</a>.<a href="#cite_note-160">[154]</a> </td></tr> <tr> <td style="border:5px ridge red; background:#846000; text-align:center;"><a href="/wiki/File:TrES-2b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/3/3a/TrES-2b.png/112px-TrES-2b.png" decoding="async" width="112" height="75" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/3/3a/TrES-2b.png/168px-TrES-2b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/3/3a/TrES-2b.png/224px-TrES-2b.png 2x" data-file-width="3888" data-file-height="2592" /></a> </td> <td><a href="/wiki/TrES-2b" title="TrES-2b">TrES-2</a> (Kepler-1b) </td> <td data-sort-value="1.265">1.265 +0.054 −0.051<a href="#cite_note-Berger-2018-128">[122]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.199">1.199 ± 0.052<a href="#cite_note-Vk5eJ-161">[155]</a> </td> <td>Darkest known exoplanet due to an extremely low <a href="/wiki/Geometric_albedo" title="Geometric albedo">geometric albedo</a> of 0.0136, absorbing 99% of light. </td></tr> <tr style="background:pink;"> <td style="border:5px ridge yellow; background:black; text-align:center;"><a href="/wiki/File:1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/7e/1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png/112px-1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png" decoding="async" width="112" height="90" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/7e/1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png/168px-1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/7e/1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png/224px-1e8m_comparison_Saturn_Jupiter_OGLE-TR-122b_with_Uranus_Neptune_Sirius_B_Earth_Venus_no_transparency.png 2x" data-file-width="1280" data-file-height="1024" /></a> </td> <td><a href="/wiki/OGLE-TR-122B" class="mw-redirect" title="OGLE-TR-122B">OGLE-TR-122B</a> </td> <td data-sort-value="1.17">1.17 +0.23 −0.13<a href="#cite_note-xit-162">[156]</a> (0.120 +0.024 −0.013 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="96.38">96.4 ± 9.4 (0.092 ± 0.009 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td>Smallest eclipsing <a href="/wiki/Red_dwarf" title="Red dwarf">red dwarf</a> and smallest observationally measured diameter. First star with direct evidence to have its radius comparable with <a href="/wiki/Jupiter_radius" title="Jupiter radius">Jupiter's</a> (by transit).<a href="#cite_note-xit-162">[156]</a> Reported for reference. </td></tr> <tr style="background:pink;"> <td style="border:5px ridge red; background:black; text-align:center;"><a href="/wiki/File:Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/50/Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg/112px-Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg" decoding="async" width="112" height="90" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/50/Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg/168px-Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/50/Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg/224px-Artist%27s_view_of_planets_transiting_red_dwarf_star_in_TRAPPIST-1_system.jpg 2x" data-file-width="3000" data-file-height="2400" /></a> </td> <td><a href="/wiki/TRAPPIST-1" title="TRAPPIST-1">TRAPPIST-1</a> </td> <td data-sort-value="1.16">1.16 ± 0.01<a href="#cite_note-:25-163">[157]</a> (0.1192 ± 0.0013 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="94.1">94.1 ± 2.4<a href="#cite_note-:25-163">[157]</a> (0.0898 ± 0.0023 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td><a href="/wiki/List_of_exoplanet_extremes" title="List of exoplanet extremes">Coldest and smallest</a> known star hosting exoplanets.<a href="#cite_note-164">[158]</a> All <a href="/wiki/TRAPPIST-1#Planetary_system" title="TRAPPIST-1">7 exoplanets</a> are rocky planets, orbiting closer to the star than <a href="/wiki/Mercury#Orbit,_rotation,_and_longitude" class="mw-disambig" title="Mercury">Mercury</a>. Their low inclinations of planetary orbits relative to the system's <a href="/wiki/Ecliptic" title="Ecliptic">ecliptic</a> of less than 0.1 degrees make TRAPPIST-1 system the flattest <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a>.<a href="#cite_note-165">[159]</a> Age: 7.6 ± 2.2 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a>.<a href="#cite_note-166">[160]</a> Reported for reference. </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/80/Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg/112px-Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg" decoding="async" width="112" height="80" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/80/Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg/168px-Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/80/Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg/224px-Artist%E2%80%99s_impression_of_the_deep_blue_planet_HD_189733b.jpg 2x" data-file-width="4200" data-file-height="3000" /></a> </td> <td><a href="/wiki/HD_189733_b" title="HD 189733 b">HD 189733 b</a> </td> <td data-sort-value="1.138">1.138 ± 0.027<a href="#cite_note-:0-167">[161]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="1.123">1.123 ± 0.045<a href="#cite_note-:0-167">[161]</a> </td> <td>First exoplanet to have its <a href="/wiki/Heat_map" title="Heat map">thermal map</a> constructed,<a href="#cite_note-Knutson2007-168">[162]</a> its overall color (deep blue) determined,<a href="#cite_note-Berdyugina2011-169">[163]</a><a href="#cite_note-Evans2013-170">[164]</a> its transit viewed in the X-ray spectrum, and to have <a href="/wiki/Carbon_dioxide" title="Carbon dioxide">carbon dioxide</a> confirmed as being present in its atmosphere. Such the rich <a href="/wiki/Cobalt_blue" title="Cobalt blue">cobalt blue</a><a href="#cite_note-jz7Ys-171">[165]</a><a href="#cite_note-qWEUO-172">[166]</a> colour of HD 189733 b may be the result of <a href="/wiki/Rayleigh_scattering" title="Rayleigh scattering">Rayleigh scattering</a>. The wind can blow up to 8,700 km/h (5,400 mph) from the day side to the night side.<a href="#cite_note-h1pFg-173">[167]</a> </td></tr> <tr style="background:#FFE8DC"> <td style="border:5px ridge green; background:#000000; text-align:center;"><a href="/wiki/File:Primera_foto_planeta_extrasolar_ESO.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/12/Primera_foto_planeta_extrasolar_ESO.jpg/112px-Primera_foto_planeta_extrasolar_ESO.jpg" decoding="async" width="112" height="111" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/12/Primera_foto_planeta_extrasolar_ESO.jpg/168px-Primera_foto_planeta_extrasolar_ESO.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/12/Primera_foto_planeta_extrasolar_ESO.jpg/224px-Primera_foto_planeta_extrasolar_ESO.jpg 2x" data-file-width="778" data-file-height="772" /></a> </td> <td><a href="/wiki/2M1207b" title="2M1207b">2M1207 b</a> (TWA 27b) </td> <td data-sort-value="1.13">1.13<a href="#cite_note-Luhman-174">[168]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="5.5">5.5 ± 0.5<a href="#cite_note-Luhman-174">[168]</a> </td> <td>First directly imaged <a href="/wiki/Planetary-mass_object" title="Planetary-mass object">planetary body</a> to have its spectrum taken and first planet discovered orbiting a <a href="/wiki/2M1207" title="2M1207">brown dwarf</a>. Its mass is well below the limit for <a href="/wiki/Deuterium_fusion" title="Deuterium fusion">deuterium fusion</a> in brown dwarfs of 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>. This planet will shrink to a size slightly smaller than <a href="/wiki/Jupiter_radius" title="Jupiter radius">Jupiter</a> as it cools over the next few billion years. </td></tr> <tr style="background:pink;"> <td> </td> <td><a href="/wiki/2MASS_J0523%E2%88%921403" title="2MASS J0523−1403">2MASS J0523−1403</a> </td> <td data-sort-value="1.126">1.126 ± 0.063<a href="#cite_note-:26-175">[169]</a> (0.116 ± 0.006 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;"># </td> <td data-sort-value="67.54">67.54 ± 12.79<a href="#cite_note-filippazzo-176">[170]</a> (0.0644 ± 0.0122 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) or 103 ± 11<a href="#cite_note-:26-175">[169]</a> (0.0983 ± 0.0011 <a href="/wiki/Solar_mass" title="Solar mass"><var>M</var>☉</a>) </td> <td><a href="/wiki/List_of_coolest_stars" title="List of coolest stars">Coolest</a> <a href="/wiki/Main_sequence" title="Main sequence">main sequence</a> star with <a href="/wiki/Effective_temperature" title="Effective temperature">effective temperature</a> 1939 <a href="/wiki/Kelvin" title="Kelvin">K</a> (1665.85 <a href="/wiki/Celsius" title="Celsius">°C</a>; 3030.53 <a href="/wiki/Fahrenheit" title="Fahrenheit">°F</a>) and lightest <a href="/wiki/2MASS_J0523%E2%88%921403#Hydrogen_burning_limit" title="2MASS J0523−1403">hydrogen-fusing</a> star known.<a href="#cite_note-Dieterich_2013-177">[171]</a> Reported for reference. </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:WD_0806-661B_NIRCam.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/10/WD_0806-661B_NIRCam.jpg/112px-WD_0806-661B_NIRCam.jpg" decoding="async" width="112" height="93" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/10/WD_0806-661B_NIRCam.jpg/168px-WD_0806-661B_NIRCam.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/10/WD_0806-661B_NIRCam.jpg/224px-WD_0806-661B_NIRCam.jpg 2x" data-file-width="2421" data-file-height="2002" /></a> </td> <td><a href="/wiki/Ahra" class="mw-redirect" title="Ahra">Ahra</a> (WD 0806-661 b) </td> <td data-sort-value="1.12">1.12<a href="#cite_note-uP88O-178">[172]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="7">7 − 9<a href="#cite_note-Ahra_mass-179">[173]</a> </td> <td>Initially possibly formed closer to <a href="/wiki/WD_0806%E2%88%92661" title="WD 0806−661">Maru</a> (WD 0806−661), the planet or brown dwarf migrated further away as Maru reached the end of its life with current separation of about 2500 <a href="/wiki/Astronomical_unit" title="Astronomical unit">AU</a>. Might be considered an <a href="/wiki/Exoplanet" title="Exoplanet">exoplanet</a> or a <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a>, the <a href="/wiki/Brown_dwarf#Table_of_extremes" title="Brown dwarf">dimmest</a> <a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">sub-brown dwarf</a>. The <a href="/wiki/International_Astronomical_Union" title="International Astronomical Union">IAU</a> considers objects below the ~13 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a> limiting mass for <a href="/wiki/Deuterium_fusion" title="Deuterium fusion">deuterium fusion</a> that orbit stars (or <a href="/wiki/Stellar_remnants" class="mw-redirect" title="Stellar remnants">stellar remnants</a>) to be planets, regardless on how they formed.<a href="#cite_note-IAUplanetdef-180">[174]</a> At discovery in 2011 it was the coldest planetary-mass companion imaged caused by <a href="/wiki/WD_0806%E2%88%92661" title="WD 0806−661">Maru</a>'s age of 1.5–2.7 <a href="/wiki/Gigayear" class="mw-redirect" title="Gigayear">Gyr</a> and the first orbiting a single white dwarf.<a href="#cite_note-qmDOD-181">[175]</a> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:Coconuts-2b_unwise.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Coconuts-2b_unwise.png/112px-Coconuts-2b_unwise.png" decoding="async" width="112" height="108" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Coconuts-2b_unwise.png/168px-Coconuts-2b_unwise.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f3/Coconuts-2b_unwise.png/224px-Coconuts-2b_unwise.png 2x" data-file-width="900" data-file-height="864" /></a> </td> <td><a href="/wiki/COCONUTS-2_b" class="mw-redirect" title="COCONUTS-2 b">COCONUTS-2 b</a> (COCONUTS-2A b, L 34-26 b) </td> <td data-sort-value="1.11">1.11 +0.03 −0.04<a href="#cite_note-Zhang2024-182">[176]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="8">8 ± 2<a href="#cite_note-Zhang2024-182">[176]</a> </td> <td>Initially discovered as <a href="/wiki/Rogue_planet" title="Rogue planet">rogue</a> <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a> as WISEPA J075108.79−763449.6,<a href="#cite_note-COCONUTS-183">[177]</a> this planet has the longest known orbital period, orbiting around <a href="/wiki/L_34-26" class="mw-redirect" title="L 34-26">L 34-26</a> (COCONUTS-2A) at the distance of 7506 <a href="/wiki/Astronomical_unit" title="Astronomical unit">AU</a> with the duration of over 1 million years.<a href="#cite_note-uhnews-184">[178]</a> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-112px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-168px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f6/First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif/lossy-page1-224px-First_ever_image_of_a_multi-planet_system_around_a_Sun-like_star.tif.jpg 2x" data-file-width="990" data-file-height="990" /></a> </td> <td><a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1 c</a> (YSES 1 c) </td> <td data-sort-value="1.1">1.1 +0.06 −0.03<a href="#cite_note-Wood-2023-110">[104]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="7.2">7.2 ± 0.7<a href="#cite_note-Wood-2023-110">[104]</a> </td> <td>First <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a> to be directly observed having more than one exoplanet (along with <a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1 b</a>) found orbiting around <a href="/wiki/Solar_analog" title="Solar analog">sun-like</a> <a href="/wiki/TYC_8998-760-1" title="TYC 8998-760-1">TYC 8998-760-1</a>,<a href="#cite_note-Ri9R7-111">[105]</a><a href="#cite_note-a5T6A-112">[106]</a> whose age is 27 <a href="/wiki/Year#SI_prefix_multipliers" title="Year">Myr</a>.<a href="#cite_note-Wood-2023-110">[104]</a> </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge yellow; background:#000000; text-align:center;"><a href="/wiki/File:Exoplanet_Comparison_CoRoT-3_b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Exoplanet_Comparison_CoRoT-3_b.png/112px-Exoplanet_Comparison_CoRoT-3_b.png" decoding="async" width="112" height="52" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Exoplanet_Comparison_CoRoT-3_b.png/168px-Exoplanet_Comparison_CoRoT-3_b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1b/Exoplanet_Comparison_CoRoT-3_b.png/224px-Exoplanet_Comparison_CoRoT-3_b.png 2x" data-file-width="1040" data-file-height="480" /></a> </td> <td><a href="/wiki/CoRoT-3b" title="CoRoT-3b">CoRoT-3b</a> </td> <td data-sort-value="1.085">1.08 ± 0.05<a href="#cite_note-8YMrE-185">[179]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="21.66">21.66 ± 1.00<a href="#cite_note-Deleuil2008-186">[180]</a> </td> <td>Might be considered either a <a href="/wiki/Exoplanet" title="Exoplanet">planet</a> or a <a href="/wiki/Brown_dwarf" title="Brown dwarf">brown dwarf</a>, depending on the definition chosen for these terms. If the brown dwarf/planet limit is defined by mass regime using the <a href="/wiki/Deuterium_fusion" title="Deuterium fusion">deuterium burning</a> limit as the delimiter (i.e. 13 MJ), CoRoT-3b is a brown dwarf.<a href="#cite_note-3YVJQ-187">[181]</a> If formation is the criterion, CoRoT-3b may be a planet given that some models of planet formation predict that planets with masses up to 25–30 Jupiter masses can form via <a href="/wiki/Accretion_(astrophysics)" title="Accretion (astrophysics)">core accretion</a>.<a href="#cite_note-fny8Y-188">[182]</a> However, it is unclear which method of formation created CoRoT-3b. </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:Epsilon_Indi_Ab_(MIRI_Image).png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Epsilon_Indi_Ab_%28MIRI_Image%29.png/112px-Epsilon_Indi_Ab_%28MIRI_Image%29.png" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/Epsilon_Indi_Ab_%28MIRI_Image%29.png/168px-Epsilon_Indi_Ab_%28MIRI_Image%29.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/Epsilon_Indi_Ab_%28MIRI_Image%29.png/224px-Epsilon_Indi_Ab_%28MIRI_Image%29.png 2x" data-file-width="2160" data-file-height="2160" /></a> </td> <td><a href="/wiki/Epsilon_Indi_Ab" title="Epsilon Indi Ab">Epsilon Indi Ab</a> (ε Ind b) </td> <td data-sort-value="1.08">1.08<a href="#cite_note-Matthews2024-189">[183]</a><a href="#cite_note-L/Teff-9">[a]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="6.31">6.31 +0.60 −0.56<a href="#cite_note-Matthews2024-189">[183]</a> </td> <td>Nearest and coldest extrasolar planet directly imaged.<a href="#cite_note-JWSTImages2024-07-24-190">[184]</a> Second closest <a href="/wiki/Jovian_planet" class="mw-redirect" title="Jovian planet">Jovian exoplanet</a> to the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>, after <a href="/wiki/%CE%95_Eridani_b" class="mw-redirect" title="Ε Eridani b">AEgir</a> (ε Eridani b). </td></tr> <tr> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:Kepler-90_h_and_hypothetical_exomoon.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/fc/Kepler-90_h_and_hypothetical_exomoon.jpg/112px-Kepler-90_h_and_hypothetical_exomoon.jpg" decoding="async" width="112" height="60" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/fc/Kepler-90_h_and_hypothetical_exomoon.jpg/168px-Kepler-90_h_and_hypothetical_exomoon.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/fc/Kepler-90_h_and_hypothetical_exomoon.jpg/224px-Kepler-90_h_and_hypothetical_exomoon.jpg 2x" data-file-width="1600" data-file-height="857" /></a> </td> <td><a href="/wiki/Kepler-90h" title="Kepler-90h">Kepler-90h</a> </td> <td data-sort-value="1.01">1.01 ± 0.09<a href="#cite_note-NASAExoplanet-191">[185]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.639">0.639 ± 0.016<a href="#cite_note-Liang2020-192">[186]</a> </td> <td>Located in the <a href="/wiki/Kepler-90#Planetary_system" title="Kepler-90">Kepler-90 System</a> with eight known exoplanets, whose <a href="/wiki/Planetary_system#System_architectures" title="Planetary system">architecture</a> is similar to that of the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>, with <a href="/wiki/Rocky_planet" class="mw-redirect" title="Rocky planet">rocky planets</a> being closer to <a href="/wiki/Kepler-90" title="Kepler-90">Kepler-90</a> and <a href="/wiki/Gas_giant" title="Gas giant">gas giants</a> being more distant. This largest, most massive and outermost planet orbits every ~331.6 days at a separation of 1.01 <a href="/wiki/Astronomical_unit" title="Astronomical unit">AU</a> which is within the <a href="/wiki/Habitable_zone" title="Habitable zone">habitable zone</a> of <a href="/wiki/Kepler-90h#Habitability" title="Kepler-90h">Kepler-90</a> and thus could theoretically have a <a href="/wiki/Habitability_of_natural_satellites" title="Habitability of natural satellites">habitable</a> Earth-like <a href="/wiki/Exomoon" title="Exomoon">exomoon</a>. </td></tr> <tr style="background:pink;"> <td style="border:5px ridge cyan; background:#000000; text-align:center;"><a href="/wiki/File:Jupiter_Earth_Moon_Comparison.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/98/Jupiter_Earth_Moon_Comparison.png/112px-Jupiter_Earth_Moon_Comparison.png" decoding="async" width="112" height="84" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/98/Jupiter_Earth_Moon_Comparison.png/168px-Jupiter_Earth_Moon_Comparison.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/98/Jupiter_Earth_Moon_Comparison.png/224px-Jupiter_Earth_Moon_Comparison.png 2x" data-file-width="800" data-file-height="600" /></a> </td> <td><a href="/wiki/Jupiter" title="Jupiter">Jupiter</a> </td> <td data-sort-value="1">1 (11.209 <a href="/wiki/Earth_radius" title="Earth radius">R🜨</a>)<a href="#cite_note-Prša-2016-5">[5]</a> <a href="/wiki/Jupiter_radius" title="Jupiter radius">(71 492 km)</a> </td> <td style="text-align:center;"># </td> <td data-sort-value="1">1 (317.827 <a href="/wiki/Earth_mass" title="Earth mass">M🜨</a>)<a href="#cite_note-JPL_Planets-193">[187]</a> <a href="/wiki/Jupiter_mass" title="Jupiter mass">(1.898 125 × 1027 kg)</a> </td> <td><a href="/wiki/Jupiter#Formation_and_migration" title="Jupiter">Oldest</a>, largest and most massive <a href="/wiki/Solar_System_planets" class="mw-redirect" title="Solar System planets">planet</a> in the <a href="/wiki/Solar_System" title="Solar System">Solar System</a>;<a href="#cite_note-:1-194">[188]</a> this planet hosts <a href="/wiki/Moons_of_Jupiter" title="Moons of Jupiter">95 known moons</a> including the <a href="/wiki/Galilean_moons" title="Galilean moons">Galilean moons</a>. Reported for reference. </td></tr> <tr class="sortbottom"> <td colspan="6">For smaller exoplanets, see the <a href="/wiki/List_of_smallest_exoplanets" title="List of smallest exoplanets">list of smallest exoplanets</a> or other <a href="/wiki/Lists_of_planets" title="Lists of planets">lists of exoplanets</a>. </td></tr></tbody></table> <div class="mw-heading mw-heading2"><h2 id="Candidates_for_largest_exoplanets">Candidates for largest exoplanets</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=3" title="Edit section: Candidates for largest exoplanets">edit</a>]</div> <div class="mw-heading mw-heading3"><h3 id="Unconfirmed_exoplanets">Unconfirmed exoplanets</h3>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=4" title="Edit section: Unconfirmed exoplanets">edit</a>]</div> These planets are also larger than 1.7 times the size of the largest <a href="/wiki/Planet" title="Planet">planet</a> in the Solar System, <a href="/wiki/Jupiter" title="Jupiter">Jupiter</a>, but have yet to be confirmed or are disputed. <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (Classification) </caption> <tbody><tr> <td bgcolor="#FFF8DC" width="50px" style="text-align:center;">* </td> <th>Probably brown dwarfs (≳ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) (based on mass) </th></tr> <tr> <td style="text-align:center;">← </td> <th>Probably planets (≲ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) (based on mass) </th></tr> <tr> <td bgcolor="#FE9F9F" style="text-align:center;">‡ </td> <th>Unclassified object (unknown mass) </th></tr> <tr> <td bgcolor="#e6e6e6" width="50px" style="text-align:center;">– </td> <th>Theoretical planet size restrictions </th></tr></tbody></table> </div> <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (Illustration) </caption> <tbody><tr> <td style="border:5px ridge blue;"> </td> <th>Direct imaging telescopic observation </th></tr> <tr> <td style="border:5px ridge green;"> </td> <th>Composite image of direct observations </th></tr></tbody></table> </div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1253789634"> <table class="wikitable sortable sticky-header"> <tbody><tr> <th class="unsortable">Illustration </th> <th>Name (Alternates) (Status) </th> <th data-sort-type="number">Radius (<a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>) </th> <th class="unsortable">Key </th> <th data-sort-type="number">Mass (<a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) </th> <th class="unsortable">Notes </th></tr> <tr style="background:#e6e6e6"> <td> </td> <td>New born planet limit </td> <td data-sort-value="30">~ 30<a href="#cite_note-:16-195">[189]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="20">≤ 20 (≤ 13)<a href="#cite_note-:16-195">[189]</a> </td> <td>Theoretical size limit of a newly-formed exoplanet. </td></tr> <tr style="background:#e6e6e6"> <td> </td> <td>Young <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> limit </td> <td data-sort-value="20">~ 20<a href="#cite_note-:15-196">[190]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="10">≤ 10<a href="#cite_note-:15-196">[190]</a> </td> <td>Theoretical size limit of a newly-formed exoplanet that needed 104 – 105 (10000 – 100000) years to migrate close to the host star, but has not yet interacted with it beforehand. </td></tr> <tr> <td style="border:5px ridge green; background:white; text-align:center;"><a href="/wiki/File:FUOriLightCurve.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/ee/FUOriLightCurve.png/112px-FUOriLightCurve.png" decoding="async" width="112" height="73" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/ee/FUOriLightCurve.png/168px-FUOriLightCurve.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/ee/FUOriLightCurve.png/224px-FUOriLightCurve.png 2x" data-file-width="1500" data-file-height="975" /></a> </td> <td><a href="/wiki/FU_Orionis" title="FU Orionis">FU Orionis North b</a> (FU Ori b) <var>(unconfirmed)</var> </td> <td data-sort-value="10">~ 9.8<a href="#cite_note-:16-195">[189]</a> (~ 1.0 <a href="/wiki/Solar_radius" title="Solar radius">R☉</a>) </td> <td style="text-align:center;">← </td> <td data-sort-value="3">~ 3<a href="#cite_note-:16-195">[189]</a> </td> <td>Discovered using a variation of disk kinematics.<a href="#cite_note-197">[191]</a> Caused by <a href="/wiki/Tidal_disruption" class="mw-redirect" title="Tidal disruption">tidal disruption</a> and extreme evaporation the planet radius shrank from the beginning of the burst (14 <var>R</var>J) in 1937<a href="#cite_note-:15-196">[190]</a> to the present year by ~30 per cent and its mass is around half of its initial mass of 6 <var>M</var>J.<a href="#cite_note-:15-196">[190]</a><a href="#cite_note-:16-195">[189]</a> </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_174-179953_b&action=edit&redlink=1" class="new" title="UCAC4 174-179953 b (page does not exist)">UCAC4 174-179953 b</a> (unclassified) </td> <td>8.14 ± 0.40<a href="#cite_note-198">[192]</a> (0.84 <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a>) </td> <td style="text-align:center;">‡ </td> <td>Unknown </td> <td rowspan="4">May be unreliable. Object cannot be classified as brown dwarf or exoplanet without a mass estimate. </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=KIC_2437209_b&action=edit&redlink=1" class="new" title="KIC 2437209 b (page does not exist)">KIC 2437209 b</a> (2MASS 19205038+3743335 b) (unclassified) </td> <td>5.5 ± 1.0<a href="#cite_note-199">[193]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_220-040923_b&action=edit&redlink=1" class="new" title="UCAC4 220-040923 b (page does not exist)">UCAC4 220-040923 b</a> (unclassified) </td> <td>4.65 ± 0.20<a href="#cite_note-200">[194]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=Kepler-214_d&action=edit&redlink=1" class="new" title="Kepler-214 d (page does not exist)">Kepler-214 d</a> (KOI-693 d, 2MASS J18590116+4457217 d) (unclassified) </td> <td>3.5 ± 1.5<a href="#cite_note-201">[195]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr style="background:#FFF8DC"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:View_of_the_dust_disc_around_the_young_star_HD_100546.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/View_of_the_dust_disc_around_the_young_star_HD_100546.jpg/112px-View_of_the_dust_disc_around_the_young_star_HD_100546.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/52/View_of_the_dust_disc_around_the_young_star_HD_100546.jpg/168px-View_of_the_dust_disc_around_the_young_star_HD_100546.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/52/View_of_the_dust_disc_around_the_young_star_HD_100546.jpg/224px-View_of_the_dust_disc_around_the_young_star_HD_100546.jpg 2x" data-file-width="2000" data-file-height="2004" /></a> </td> <td><a href="/wiki/HD_100546_b" class="mw-redirect" title="HD 100546 b">HD 100546 b</a> (KR Mus b) (disputed) </td> <td data-sort-value="3.4">3.4<a href="#cite_note-elena-202">[196]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="25">25<a href="#cite_note-elena-202">[196]</a> </td> <td>Sometimes the initially reported 6.9+2.7 −2.9 <a href="/wiki/Jupiter_radius" title="Jupiter radius">RJ</a> for the emitting area due to the diffuse dust and gas envelope or debris disk surrounding the planet<a href="#cite_note-quanz2014-203">[197]</a> is confused with the actual radius. </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_223-042828_b&action=edit&redlink=1" class="new" title="UCAC4 223-042828 b (page does not exist)">UCAC4 223-042828 b</a> (unclassified) </td> <td>3.33 ± 0.50<a href="#cite_note-204">[198]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td> <td rowspan="11">May be unreliable. Object cannot be classified as brown dwarf or exoplanet without a mass estimate. </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_185-192986_b&action=edit&redlink=1" class="new" title="UCAC4 185-192986 b (page does not exist)">UCAC4 185-192986 b</a> (unclassified) </td> <td>3.3 ± 0.2<a href="#cite_note-205">[199]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_118-126574_b&action=edit&redlink=1" class="new" title="UCAC4 118-126574 b (page does not exist)">UCAC4 118-126574 b</a> (unclassified) </td> <td>3.12 ± 0.10<a href="#cite_note-206">[200]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_171-187216_b&action=edit&redlink=1" class="new" title="UCAC4 171-187216 b (page does not exist)">UCAC4 171-187216 b</a> (unclassified) </td> <td data-sort-value="2.751">2.75 ± 0.20<a href="#cite_note-207">[201]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=KOI-7073_b&action=edit&redlink=1" class="new" title="KOI-7073 b (page does not exist)">KOI-7073 b</a> (unclassified) </td> <td>2.699 +0.473 −0.794<a href="#cite_note-208">[202]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.0011">Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_175-188215_b&action=edit&redlink=1" class="new" title="UCAC4 175-188215 b (page does not exist)">UCAC4 175-188215 b</a> (unclassified) </td> <td>2.69 ± 0.50<a href="#cite_note-209">[203]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_116-118563_b&action=edit&redlink=1" class="new" title="UCAC4 116-118563 b (page does not exist)">UCAC4 116-118563 b</a> (unclassified) </td> <td>2.62 ± 0.10<a href="#cite_note-210">[204]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=KOI-974_b&action=edit&redlink=1" class="new" title="KOI-974 b (page does not exist)">KOI-974 b</a> (unclassified) </td> <td>2.51 ± 0.02<a href="#cite_note-211">[205]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=19g-2-01326_b&action=edit&redlink=1" class="new" title="19g-2-01326 b (page does not exist)">19g-2-01326 b</a> (unclassified) </td> <td>2.43<a href="#cite_note-212">[206]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TOI-1438_c&action=edit&redlink=1" class="new" title="TOI-1438 c (page does not exist)">TOI-1438 c</a> (unclassified) </td> <td>2.37 ± 0.17<a href="#cite_note-213">[207]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TOI-931_Ab&action=edit&redlink=1" class="new" title="TOI-931 Ab (page does not exist)">TOI-931 Ab</a> (unclassified) </td> <td>2.3571<a href="#cite_note-214">[208]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=SOI-2_b&action=edit&redlink=1" class="new" title="SOI-2 b (page does not exist)">SOI-2 b</a> (unclassified) </td> <td data-sort-value="2.22">2.22<a href="#cite_note-215">[209]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.001">Unknown </td> <td><a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a>, may be unreliable. Object cannot be classified as brown dwarf or exoplanet without a mass estimate. </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_332350266.01&action=edit&redlink=1" class="new" title="TIC 332350266.01 (page does not exist)">TIC 332350266.01</a> (unclassified) </td> <td>2.2143 +3.1823 −2.2143<a href="#cite_note-216">[210]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td> <td>May be unreliable. Object cannot be classified as brown dwarf or exoplanet without a mass estimate. </td></tr> <tr style="background:#e6e6e6"> <td> </td> <td>Old <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> limit </td> <td data-sort-value="2.2">2.2<a href="#cite_note-limit-53">[48]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="0.0000000000000000001">> 0 </td> <td>Theoretical limit for <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiters</a> close to a star, that are limited by <a href="/wiki/Tidal_heating" title="Tidal heating">tidal heating</a>, resulting in 'runaway inflation' </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_138664795.01&action=edit&redlink=1" class="new" title="TIC 138664795.01 (page does not exist)">TIC 138664795.01</a> (unclassified) </td> <td>2.1617 ± 0.1615<a href="#cite_note-217">[211]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td> <td rowspan="17">Object cannot be classified as brown dwarf or exoplanet without a mass estimate. </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_221-041868_b&action=edit&redlink=1" class="new" title="UCAC4 221-041868 b (page does not exist)">UCAC4 221-041868 b</a> (unclassified) </td> <td>2.1 ± 0.20<a href="#cite_note-218">[212]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TOI-496_b&action=edit&redlink=1" class="new" title="TOI-496 b (page does not exist)">TOI-496 b</a> (unclassified) </td> <td>2.050 +0.633 −0.285<a href="#cite_note-219">[213]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=19b1-02162_b&action=edit&redlink=1" class="new" title="19b1-02162 b (page does not exist)">19b1-02162 b</a> (unclassified) </td> <td>1.97<a href="#cite_note-220">[214]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=SOI-7_b&action=edit&redlink=1" class="new" title="SOI-7 b (page does not exist)">SOI-7 b</a> (unclassified) </td> <td data-sort-value="1.96">1.96<a href="#cite_note-221">[215]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.0009">Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_121-140615_b&action=edit&redlink=1" class="new" title="UCAC4 121-140615 b (page does not exist)">UCAC4 121-140615 b</a> (unclassified) </td> <td>1.94 ± 0.20<a href="#cite_note-222">[216]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_123-150641_b&action=edit&redlink=1" class="new" title="UCAC4 123-150641 b (page does not exist)">UCAC4 123-150641 b</a> (unclassified) </td> <td>1.93 ± 0.20<a href="#cite_note-223">[217]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_274508785.01&action=edit&redlink=1" class="new" title="TIC 274508785.01 (page does not exist)">TIC 274508785.01</a> (unclassified) </td> <td>1.9172 +2.3678 −1.9172<a href="#cite_note-224">[218]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=W74_b&action=edit&redlink=1" class="new" title="W74 b (page does not exist)">W74 b</a> (Gaia DR2 6045477635223138432 b) (unclassified) </td> <td>1.9<a href="#cite_note-225">[219]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_116307482.01&action=edit&redlink=1" class="new" title="TIC 116307482.01 (page does not exist)">TIC 116307482.01</a> (unclassified) </td> <td>1.8931 ± 1.4551<a href="#cite_note-226">[220]</a> </td> <td style="text-align:center;">‡ </td> <td>Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_122-142653_b&action=edit&redlink=1" class="new" title="UCAC4 122-142653 b (page does not exist)">UCAC4 122-142653 b</a> (unclassified) </td> <td>1.85 ± 0.10<a href="#cite_note-227">[221]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.0007">Unknown </td></tr> <tr bgcolor="FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_77173027.01&action=edit&redlink=1" class="new" title="TIC 77173027.01 (page does not exist)">TIC 77173027.01</a> (unclassified) </td> <td>1.8396 ± 1.115<a href="#cite_note-228">[222]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.0006">Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TOI-159_Ab&action=edit&redlink=1" class="new" title="TOI-159 Ab (page does not exist)">TOI-159 Ab</a> (unclassified) </td> <td data-sort-value="1.81">1.80 ± 0.77<a href="#cite_note-229">[223]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.0003">Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=TIC_82205179.01&action=edit&redlink=1" class="new" title="TIC 82205179.01 (page does not exist)">TIC 82205179.01</a> (TIC 82205179 b) (unclassified) </td> <td>1.76 ± 0.56<a href="#cite_note-230">[224]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="0.00009">Unknown </td></tr> <tr bgcolor="#FE9F9F"> <td> </td> <td><a href="/w/index.php?title=UCAC4_124-144273_b&action=edit&redlink=1" class="new" title="UCAC4 124-144273 b (page does not exist)">UCAC4 124-144273 b</a> (unclassified) </td> <td>1.71 ± 0.10<a href="#cite_note-231">[225]</a> </td> <td style="text-align:center;">‡ </td> <td data-sort-value="1.00007">Unknown </td></tr> </tbody></table> <div class="mw-heading mw-heading3"><h3 id="Exoplanets_with_uncertain_radii">Exoplanets with uncertain radii</h3>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=5" title="Edit section: Exoplanets with uncertain radii">edit</a>]</div> This list contains planets with uncertain radii that could be below or above the adopted cut-off of 1.7 <var>R</var>J, depending on the estimate. <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (classification) </caption> <tbody><tr> <td style="text-align:center;">← </td> <th>Probably planets (≲ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) (based on mass) </th></tr> <tr> <td bgcolor="#cff7c1" width="50px" style="text-align:center;">? </td> <th>Status uncertain </th></tr> <tr> <td bgcolor="#CEE0F2" width="50px" style="text-align:center;">→ </td> <th>Planets with grazing transit, hindering radius determination </th></tr></tbody></table> </div> <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (illustration) </caption> <tbody><tr> <td style="border:5px ridge blue;"> </td> <th>Direct imaging telescopic observation </th></tr> <tr> <td style="border:5px ridge green;"> </td> <th>Composite image of direct observations </th></tr></tbody></table> </div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1253789634"> <table class="wikitable sortable sticky-header"> <tbody><tr> <th class="unsortable">Illustration </th> <th>Name (Alternates) </th> <th data-sort-type="number">Radius (<a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>) </th> <th class="unsortable">Key </th> <th data-sort-type="number">Mass (<a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) </th> <th class="unsortable">Notes </th></tr> <tr style="background:#CEE0F2"> <td> </td> <td><a href="/w/index.php?title=TOI-3540_b&action=edit&redlink=1" class="new" title="TOI-3540 b (page does not exist)">TOI-3540 b</a> </td> <td data-sort-value="2.10">2.10, >1.44 (95% lower limit)<a href="#cite_note-Yee-2022-232">[226]</a> </td> <td style="text-align:center;">→ </td> <td data-sort-value="1.18">1.18 ± 0.14<a href="#cite_note-Yee-2022-232">[226]</a> </td> <td>Grazing planet </td></tr> <tr style="background:#CEE0F2"> <td> </td> <td><a href="/w/index.php?title=TOI-3807_b&action=edit&redlink=1" class="new" title="TOI-3807 b (page does not exist)">TOI-3807 b</a> </td> <td data-sort-value="2.00">2.00, >1.65 (95% lower limit)<a href="#cite_note-Yee-2023-233">[227]</a> </td> <td style="text-align:center;">→ </td> <td data-sort-value="1.04">1.04 +0.15 −0.14<a href="#cite_note-Yee-2023-233">[227]</a> </td> <td>Grazing planet </td></tr> <tr style="background:#CEE0F2"> <td> </td> <td><a href="/w/index.php?title=TOI-2193_Ab&action=edit&redlink=1" class="new" title="TOI-2193 Ab (page does not exist)">TOI-2193 Ab</a> </td> <td data-sort-value="1.77">1.77, >1.55 (95% lower limit)<a href="#cite_note-Yee-2022-232">[226]</a> </td> <td style="text-align:center;">→ </td> <td data-sort-value="0.94">0.94 ± 0.18<a href="#cite_note-Yee-2022-232">[226]</a> </td> <td>Grazing planet </td></tr> <tr> <th colspan="6" style="background:#efefef" data-sort-value="1.699999">Exoplanet(s) with radius(es) below 1.7 <var>R</var>J (19.1 <a href="/wiki/Earth_radius" title="Earth radius"><var>R</var>🜨</a>). </th></tr> <tr style="background:#cff7c1"> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:SR_12_C.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/112px-SR_12_C.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/168px-SR_12_C.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/224px-SR_12_C.jpg 2x" data-file-width="430" data-file-height="430" /></a> </td> <td><a href="/wiki/SR_12_(star)" title="SR 12 (star)">SR 12 c</a> (SR 12 (AB) c, SR 12 C) </td> <td data-sort-value="1.6">~ 1.6,<a href="#cite_note-:24-234">[228]</a> 2.38 +0.27 −0.32<a href="#cite_note-Bryan-2020-72">[66]</a> </td> <td style="text-align:center;">? </td> <td data-sort-value="11">11 ± 3<a href="#cite_note-:24-234">[228]</a> </td> <td>The planet is at the very edge of the <a href="/wiki/Deuterium_burning" class="mw-redirect" title="Deuterium burning">deuterium burning</a> limit. This object has a <a href="/wiki/Circumplanetary_disk" title="Circumplanetary disk">circumplanetary disk</a>, detected in <a href="/wiki/Submillimetre_astronomy" title="Submillimetre astronomy">sub-mm</a> with <a href="/wiki/Atacama_Large_Millimeter_Array" title="Atacama Large Millimeter Array">ALMA</a>.<a href="#cite_note-:11-235">[229]</a> Other sources of masses includes 14 +7 −8 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-:9-236">[230]</a> 12 – 15 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a><a href="#cite_note-:10-237">[231]</a> and 13 ± 2 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-Bryan-2020-72">[66]</a> </td></tr> <tr> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/11/The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg/112px-The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/11/The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg/168px-The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/11/The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg/224px-The_Star_AB_Pictoris_and_its_Companion_-_Phot-14d-05-normal.jpg 2x" data-file-width="800" data-file-height="798" /></a> </td> <td><a href="/wiki/AB_Pictoris_b" class="mw-redirect" title="AB Pictoris b">AB Pictoris b</a> (AB Pic b) </td> <td data-sort-value="1.57">1.57 ± 0.07 – 1.8 ± 0.3<a href="#cite_note-Palma-Bifani-2023-238">[232]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="10">10 ± 1<a href="#cite_note-Palma-Bifani-2023-238">[232]</a> </td> <td>Previously believed to be a likely brown dwarf, with mass estimates of 13−14 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a><a href="#cite_note-chauvin-239">[233]</a> to 70 MJ,<a href="#cite_note-neu05-240">[234]</a> its mass is now estimated to be 10±1 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>, with an age of 13+1.1 −0.6 million years.<a href="#cite_note-Palma2022-241">[235]</a> </td></tr> <tr> <td style="border:5px ridge green; background:#000000; text-align:center;"><a href="/wiki/File:PDS70c-CircumplanetaryDisk-20190711.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/68/PDS70c-CircumplanetaryDisk-20190711.jpg/112px-PDS70c-CircumplanetaryDisk-20190711.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/68/PDS70c-CircumplanetaryDisk-20190711.jpg/168px-PDS70c-CircumplanetaryDisk-20190711.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/68/PDS70c-CircumplanetaryDisk-20190711.jpg/224px-PDS70c-CircumplanetaryDisk-20190711.jpg 2x" data-file-width="1440" data-file-height="1440" /></a> </td> <td><a href="/wiki/PDS_70_c" class="mw-redirect" title="PDS 70 c">PDS 70 c</a> </td> <td data-sort-value="1.131">1.13 +0.56 −0.43 – 2.04 +0.61 −0.45<a href="#cite_note-Wang2020-62">[57]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="7.5">7.5 +4.7 −4.2<a href="#cite_note-Wang_王-2021-63">[58]</a> </td> <td>Second confirmed <a href="/wiki/Protoplanet" title="Protoplanet">protoplanet</a> in the <a href="/wiki/Planetary_system" title="Planetary system">planetary system</a> with the first two protoplanets. Has the first ever detected <a href="/wiki/Circumplanetary_disk" title="Circumplanetary disk">circumplanetary disk</a>, that was the second to be confirmed and was found using <a href="/wiki/Atacama_Large_Millimeter_Array" title="Atacama Large Millimeter Array">ALMA</a>.<a href="#cite_note-fdieh-242">[236]</a> Other sources of masses includes: 7.8 +5.0 −4.7 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>, ~1 − ~15 <var>M</var>J (total).<a href="#cite_note-Wang_王-2021-63">[58]</a> </td></tr></tbody></table> <div class="mw-heading mw-heading2"><h2 id="Chronological_list_of_largest_exoplanets">Chronological list of largest exoplanets</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=6" title="Edit section: Chronological list of largest exoplanets">edit</a>]</div> These exoplanets were the largest at the time of their discovery. <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (classification) </caption> <tbody><tr> <td bgcolor="#FFF8DC" width="50px" style="text-align:center;">* </td> <th>Later identified to be a probable brown dwarf or a star (≳ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) </th></tr> <tr> <td bgcolor="#CEF2E0" width="50px" style="text-align:center;">† </td> <th>Candidate for largest exoplanet (currently or in time span) </th></tr> <tr> <td bgcolor="#CEE0F2" width="50px" style="text-align:center;">→ </td> <th>Assumed largest exoplanet, while unconfirmed, later retracted or later confirmed </th></tr> <tr> <td style="text-align:center;">← </td> <th>Largest exoplanet (≲ 13 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) at the time </th></tr> <tr> <td bgcolor="#e6e6e6" width="50px" style="text-align:center;">– </td> <th>Largest confirmed exoplanet (in radius and mass), while discovered candidates might be larger </th></tr> <tr> <td bgcolor="pink" width="50px" style="text-align:center;"># </td> <th>Non-exoplanets reported for reference </th></tr></tbody></table> </div> <div style="display:inline-grid"> <table class="wikitable"> <caption>Key (illustration) </caption> <tbody><tr> <td style="border:5px ridge red;"> </td> <th>Artist's impression </th></tr> <tr> <td style="border:5px ridge yellow;"> </td> <th>Artist's size comparison </th></tr> <tr> <td style="border:5px ridge orange;"> </td> <th>Artist's impression and size comparison </th></tr> <tr> <td style="border:5px ridge cyan;"> </td> <th><a href="/wiki/Star_chart" title="Star chart">Star Chart / Star Map</a> </th></tr> <tr> <td style="border:5px ridge blue;"> </td> <th>Direct Imaging telescopic observation </th></tr> <tr> <td style="border:5px ridge green;"> </td> <th>Composite image of direct observations </th></tr> <tr> <td style="border:5px ridge purple;"> </td> <th>Transiting telescopic observation </th></tr></tbody></table> </div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1253789634"> <table class="wikitable sortable sticky-header"> <tbody><tr> <th data-sort-type="number">Years largest discovered </th> <th class="unsortable">Illustration </th> <th>Name (Alternates) </th> <th data-sort-type="number">Radius (<a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>) </th> <th class="unsortable">Key </th> <th data-sort-type="number">Mass (<a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>) </th> <th class="unsortable">Notes </th></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2024">2024 – present </td> <td style="border:5px ridge orange; background:#000000;"><a href="/wiki/File:Comparison_XO-6.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/112px-Comparison_XO-6.png" decoding="async" width="112" height="86" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/168px-Comparison_XO-6.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/224px-Comparison_XO-6.png 2x" data-file-width="1400" data-file-height="1070" /></a> </td> <td><a href="/wiki/XO-6b" title="XO-6b">XO-6b</a> </td> <td data-sort-value="2.171">2.17 ± 0.2<a href="#cite_note-Saha2024-54">[49]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="4.472">4.47 ± 0.12<a href="#cite_note-Saha2024-54">[49]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="2024">(2024 – present) </td> <td> </td> <td><a href="/w/index.php?title=TOI-1408_b&action=edit&redlink=1" class="new" title="TOI-1408 b (page does not exist)">TOI-1408 b</a> (BD+72 969 b) </td> <td data-sort-value="2.23">2.23 ± 0.36 (25±4 <a href="/wiki/Earth_radius" title="Earth radius">R🜨</a>), 2.4 ± 0.5<a href="#cite_note-Korth-2024-51">[46]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="1.86">1.86±0.02<a href="#cite_note-Korth-2024-51">[46]</a> </td> <td>Grazing and very puffy hot Jupiter.<a href="#cite_note-Korth-2024-51">[46]</a> Large size needs confirmation. </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="2020">(2020 – present) </td> <td style="border:5px ridge green; background:#000000;"><a href="/wiki/File:SR_12_C.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/112px-SR_12_C.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/168px-SR_12_C.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1e/SR_12_C.jpg/224px-SR_12_C.jpg 2x" data-file-width="430" data-file-height="430" /></a> </td> <td><a href="/wiki/SR_12_(star)" title="SR 12 (star)">SR 12 c</a> (SR 12 (AB) c, SR 12 C) </td> <td data-sort-value="2.38">2.38 +0.27 −0.32<a href="#cite_note-Bryan-2020-72">[66]</a> </td> <td style="text-align:center;">? </td> <td>13 ± 2<a href="#cite_note-Bryan-2020-72">[66]</a> </td> <td>The planet is at the very edge of the deuterium burning limit. Mass being below it needs confirmation. Other sources of masses includes 14 +7 −8 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-:9-236">[230]</a> 12 – 15 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-:10-237">[231]</a> </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="2018">(2018 – present) </td> <td style="border:5px ridge blue; background:#000000;"><a href="/wiki/File:PDS_70.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/112px-PDS_70.jpg" decoding="async" width="112" height="95" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/168px-PDS_70.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/224px-PDS_70.jpg 2x" data-file-width="2000" data-file-height="1692" /></a> </td> <td><a href="/wiki/PDS_70#Protoplanetary_disk" title="PDS 70">PDS 70 b</a> </td> <td>2.09 +0.23 −0.31 – 2.72 +0.15 −0.17,<a href="#cite_note-Wang2020-62">[57]</a> 2.7<a href="#cite_note-hBkQl-36">[31]</a> </td> <td style="text-align:center;">† </td> <td>3.2 +3.3 −1.6, 7.9 +4.9 −4.7, < 10 (2 σ), ≲ 15 (total)<a href="#cite_note-Wang_王-2021-63">[58]</a> </td> <td>Possibly the largest known exoplanet.<a href="#cite_note-limit-53">[48]</a> Multiple estimates give radii above 2 <var>R</var>J and below 3 <var>R</var>J.<a href="#cite_note-hBkQl-36">[31]</a><a href="#cite_note-Wang2020-62">[57]</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2017.2">2017 – 2024 </td> <td style="border:5px ridge purple; background:white;"><a href="/wiki/File:Transit_light_curve_of_Hat-P-67b.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/112px-Transit_light_curve_of_Hat-P-67b.png" decoding="async" width="112" height="76" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/168px-Transit_light_curve_of_Hat-P-67b.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/a0/Transit_light_curve_of_Hat-P-67b.png/224px-Transit_light_curve_of_Hat-P-67b.png 2x" data-file-width="996" data-file-height="675" /></a> </td> <td><a href="/wiki/HAT-P-67b" class="mw-redirect" title="HAT-P-67b">HAT-P-67b</a> </td> <td>2.085 +0.096 −0.071<a href="#cite_note-243">[237]</a> 2.165 +0.024 −0.022<a href="#cite_note-HatP67-68">[f]</a><a href="#cite_note-Gully-Santiago-69">[63]</a> </td> <td style="text-align:center;">– </td> <td>0.34 +0.25 −0.19<a href="#cite_note-Zhou-2017-244">[238]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a>. At discovery the largest known planet with an accurately and precisely measured radius.<a href="#cite_note-largest-70">[64]</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2017">2017 – 2017 </td> <td style="border:5px ridge orange; background:#000000;"><a href="/wiki/File:Comparison_XO-6.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/112px-Comparison_XO-6.png" decoding="async" width="112" height="86" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/168px-Comparison_XO-6.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Comparison_XO-6.png/224px-Comparison_XO-6.png 2x" data-file-width="1400" data-file-height="1070" /></a> </td> <td><a href="/wiki/XO-6b" title="XO-6b">XO-6b</a> </td> <td>2.07 ± 0.22<a href="#cite_note-zhao-245">[239]</a> </td> <td style="text-align:center;">– </td> <td>4.47 ± 0.12<a href="#cite_note-Saha2024-54">[49]</a> </td> <td>A very puffy <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2015">2015 – 2017 </td> <td style="border:5px ridge red; background:#000000;"><a href="/wiki/File:Profile_of_planet_51_Pegasi_b_(planet_only).jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/48/Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg/112px-Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/48/Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg/168px-Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/48/Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg/224px-Profile_of_planet_51_Pegasi_b_%28planet_only%29.jpg 2x" data-file-width="287" data-file-height="287" /></a> </td> <td><a href="/wiki/Dimidium" class="mw-redirect" title="Dimidium">Dimidium</a> (51 Peg b) </td> <td>1.9 ± 0.3<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="0.461">0.46 +0.06 −0.01<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td>First convincing exoplanet discovered orbiting a <a href="/wiki/Main_sequence" title="Main sequence">main-sequence</a> star. Prototype <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiter</a>. </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="2014">(2014 – 2024) </td> <td style="border:5px ridge blue; background:#000000;"><a href="/wiki/File:ROXs_42B_MUSE_IR.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/112px-ROXs_42B_MUSE_IR.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/168px-ROXs_42B_MUSE_IR.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/93/ROXs_42B_MUSE_IR.jpg/224px-ROXs_42B_MUSE_IR.jpg 2x" data-file-width="443" data-file-height="443" /></a> </td> <td><a href="/wiki/ROXs_42Bb" title="ROXs 42Bb">ROXs 42B b</a> </td> <td data-sort-value="2.43">2.43 ± 0.18 – 2.55 ± 0.2<a href="#cite_note-:14-60">[55]</a> 2.10 ± 0.35<a href="#cite_note-Xuan-2024-23">[18]</a> </td> <td style="text-align:center;">† </td> <td>9 +6 −3;<a href="#cite_note-:12-57">[52]</a> 10 ± 4<a href="#cite_note-:13-58">[53]</a> </td> <td>Large size needs confirmation. Other estimates include 1.9 – 2.4, 1.3 – 4.7 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>.<a href="#cite_note-DaemgenROX-59">[54]</a> Other recent sources of masses include 3.2 – 27 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-Inglis2024-61">[56]</a> 13 ± 5 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>.<a href="#cite_note-Xuan-2024-23">[18]</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2010">2010 – 2015 </td> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:WASP-17b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/112px-WASP-17b.jpg" decoding="async" width="112" height="104" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/168px-WASP-17b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/fd/WASP-17b.jpg/224px-WASP-17b.jpg 2x" data-file-width="2030" data-file-height="1883" /></a> </td> <td><a href="/wiki/WASP-17b" title="WASP-17b">Ditsö̀</a> (WASP-17b) </td> <td>1.74 +0.26 −0.23<a href="#cite_note-246">[240]</a> </td> <td style="text-align:center;">– </td> <td>0.512 ± 0.037<a href="#cite_note-Bonomo-2017b-77">[71]</a> </td> <td>Extremely low density of 0.08 g/cm3.<a href="#cite_note-:3-78">[72]</a> Possibly largest exoplanet at the time of discovery.<a href="#cite_note-:4-79">[73]</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2007">2007 – 2010 </td> <td style="border:5px ridge orange; background:#000000;"><a href="/wiki/File:TrES-4.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/112px-TrES-4.jpg" decoding="async" width="112" height="67" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/168px-TrES-4.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/df/TrES-4.jpg/224px-TrES-4.jpg 2x" data-file-width="750" data-file-height="450" /></a> </td> <td><a href="/wiki/TrES-4b" title="TrES-4b">TrES-4</a> (GSC 02620-00648 b) </td> <td>1.674 ± 0.094<a href="#cite_note-247">[241]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="0.78">0.78 ± 0.19<a href="#cite_note-Stassun-2017-104">[98]</a><a href="#cite_note-Johns-64">[59]</a> </td> <td>This planet has a density of 0.2 g/cm3, less than <a href="/wiki/Saturn#Internal_structure" title="Saturn">Saturn's</a> 0.7 g/cm3. </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="2006.5">(2006 – present) </td> <td style="border:5px ridge blue; background:#000000;"><a href="/wiki/File:DH_Tauri.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/112px-DH_Tauri.jpg" decoding="async" width="112" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/168px-DH_Tauri.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ac/DH_Tauri.jpg/224px-DH_Tauri.jpg 2x" data-file-width="503" data-file-height="503" /></a> </td> <td><a href="/wiki/DH_Tauri_b" class="mw-redirect" title="DH Tauri b">DH Tauri b</a> (DH Tau b) </td> <td data-sort-value="1.75">1.75<a href="#cite_note-:22-248">[242]</a><a href="#cite_note-:23-249">[243]</a><a href="#cite_note-L/Teff-9">[a]</a> 2.7 ± 0.8<a href="#cite_note-zhou2014-43">[38]</a> </td> <td style="text-align:center;">† </td> <td data-sort-value="11.5">11.5 +10.5 −3.1<a href="#cite_note-:22-248">[242]</a> </td> <td>Mass being below the deuterium burning limit needs confirmation. Temperature originally given as 2700 – 2800 K.<a href="#cite_note-:23-249">[243]</a> Other sources give the radii: 2.49 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>,<a href="#cite_note-Bonnefoy-2014-26">[21]</a><a href="#cite_note-L/Teff-9">[a]</a> 2.68 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>,<a href="#cite_note-Xuan-2020-250">[244]</a> and 2.6 ± 0.6 <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a><a href="#cite_note-Xuan-2024-23">[18]</a> and masses: 11 ± 3 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-zhou2014-43">[38]</a> 14.2 +2.4 −3.5 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a>,<a href="#cite_note-:5-46">[41]</a> 17 ± 6 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a><a href="#cite_note-:6-47">[42]</a> and 12 ± 4 <a href="/wiki/Jupiter_mass" title="Jupiter mass"><var>M</var>J</a><a href="#cite_note-Xuan-2024-23">[18]</a> </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="2006">2006 – 2007 </td> <td style="border:5px ridge red; background:black; text-align:center; margin:0 0 12px 0;"><a href="/wiki/File:Osiris_(HD209458b)_planet_illustration.jpeg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/8/84/Osiris_%28HD209458b%29_planet_illustration.jpeg/109px-Osiris_%28HD209458b%29_planet_illustration.jpeg" decoding="async" width="109" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/84/Osiris_%28HD209458b%29_planet_illustration.jpeg/164px-Osiris_%28HD209458b%29_planet_illustration.jpeg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/84/Osiris_%28HD209458b%29_planet_illustration.jpeg/218px-Osiris_%28HD209458b%29_planet_illustration.jpeg 2x" data-file-width="1380" data-file-height="1415" /></a> </td> <td><a href="/wiki/HD_209458_b" title="HD 209458 b">HD 209458 b</a> ("Osiris") </td> <td data-sort-value="1.275">1.27 ± 0.02<a href="#cite_note-251">[245]</a> </td> <td style="text-align:center;">– </td> <td data-sort-value="0.6825">0.682 +0.014 −0.015<a href="#cite_note-Bonomo-2017a-154">[148]</a> </td> <td>First known <a href="/wiki/Transiting_exoplanet" class="mw-redirect" title="Transiting exoplanet">transiting exoplanet</a>, first precisely measured planet available, first to have its orbital speed measured, determining its mass directly,<a href="#cite_note-Ignas-155">[149]</a> and to have an <a href="/wiki/Atmosphere" title="Atmosphere">atmosphere</a>, containing evaporating <a href="/wiki/Hydrogen" title="Hydrogen">hydrogen</a>, and <a href="/wiki/Oxygen" title="Oxygen">oxygen</a> and <a href="/wiki/Carbon" title="Carbon">carbon</a>. First extrasolar <a href="/wiki/Gas_giant" title="Gas giant">gas giant</a> to have its superstorm measured. Nicknamed "Osiris". </td></tr> <tr style="background:#FFF8DC"> <td data-sort-value="2005">(2005 – present) </td> <td style="border:5px ridge blue; background:#000000; text-align:center;"><a href="/wiki/File:The_Sub-Stellar_Companion_to_GQ_Lupi.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/112px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg" decoding="async" width="112" height="93" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/168px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/a/ad/The_Sub-Stellar_Companion_to_GQ_Lupi.jpg/224px-The_Sub-Stellar_Companion_to_GQ_Lupi.jpg 2x" data-file-width="1116" data-file-height="930" /></a> </td> <td><a href="/wiki/GQ_Lupi_b" title="GQ Lupi b">GQ Lupi b</a> (GQ Lup Ab, GQ Lup B) </td> <td data-sort-value="2">~ 2<a href="#cite_note-252">[246]</a> 3.50 +1.50 −1.03<a href="#cite_note-Seifahrt07-20">[15]</a> </td> <td style="text-align:center;">* </td> <td data-sort-value="1.001">1 – 46<a href="#cite_note-253">[247]</a> </td> <td>Second <a href="/wiki/Exoplanet" title="Exoplanet">exoplanet candidate</a> to be directly imaged (after <a href="/wiki/2M1207_b" class="mw-redirect" title="2M1207 b">2M1207 b</a>). </td></tr> <tr> <td data-sort-value="1999">1999 – 2006 </td> <td style="border:5px ridge purple; background:white; text-align:center;"><a href="/wiki/File:V376PegLightCurve.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/112px-V376PegLightCurve.png" decoding="async" width="112" height="73" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/168px-V376PegLightCurve.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2f/V376PegLightCurve.png/224px-V376PegLightCurve.png 2x" data-file-width="1500" data-file-height="975" /></a> </td> <td><a href="/wiki/HD_209458_b" title="HD 209458 b">HD 209458 b</a> ("Osiris") </td> <td>1.27 ± 0.02<a href="#cite_note-254">[248]</a> </td> <td style="text-align:center;">← </td> <td data-sort-value="0.682">0.682 +0.014 −0.015<a href="#cite_note-Bonomo-2017a-154">[148]</a> </td> <td>First known <a href="/wiki/Transiting_exoplanet" class="mw-redirect" title="Transiting exoplanet">transiting exoplanet</a>, first precisely measured radius available, first to have its orbital speed measured, determining its mass directly,<a href="#cite_note-Ignas-155">[149]</a> and to have an <a href="/wiki/Atmosphere" title="Atmosphere">atmosphere</a>, containing evaporating <a href="/wiki/Hydrogen" title="Hydrogen">hydrogen</a>, and <a href="/wiki/Oxygen" title="Oxygen">oxygen</a> and <a href="/wiki/Carbon" title="Carbon">carbon</a>. First extrasolar <a href="/wiki/Gas_giant" title="Gas giant">gas giant</a> to have its superstorm measured. Nicknamed "Osiris". </td></tr> <tr style="background:#CEF2E0"> <td data-sort-value="1996">(1995 – 1999) </td> <td style="border:5px ridge yellow; background:#000000;"><a href="/wiki/File:ExoplanetPopulations-20170616.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2e/ExoplanetPopulations-20170616.png/112px-ExoplanetPopulations-20170616.png" decoding="async" width="112" height="76" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2e/ExoplanetPopulations-20170616.png/168px-ExoplanetPopulations-20170616.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2e/ExoplanetPopulations-20170616.png/224px-ExoplanetPopulations-20170616.png 2x" data-file-width="4000" data-file-height="2700" /></a> </td> <td><a href="/wiki/List_of_exoplanets_discovered_before_2000" title="List of exoplanets discovered before 2000">various</a> </td> <td data-sort-value="1.01">Unknown </td> <td style="text-align:center;">† </td> <td data-sort-value="0.49"><a href="/wiki/HD_75289_b" title="HD 75289 b">0.49</a> – <a href="/wiki/HD_222582_b" title="HD 222582 b">8.37</a> </td> <td>About 20 – 25 <a href="/wiki/List_of_exoplanets_discovered_before_2000" title="List of exoplanets discovered before 2000">planets</a> were found within this time span via the <a href="/wiki/Doppler_spectroscopy" title="Doppler spectroscopy">radial velocity method</a>, none of them having radius measurements, especially shortly after their discoveries. As expected, Dimidium is larger than Poltergeist, whether one of the additional planets found till 1999 is larger than Dimidium is not clear to this day. </td></tr> <tr style="background:#e6e6e6"> <td data-sort-value="1995">1995 – 1999 </td> <td style="border:5px ridge red; background:#000000;" rowspan="2"><a href="/wiki/File:Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/112px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg" decoding="async" width="112" height="70" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/168px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/f7/Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg/224px-Artist_impression_of_the_exoplanet_51_Pegasi_b.jpg 2x" data-file-width="5000" data-file-height="3144" /></a> </td> <td><a href="/wiki/Dimidium" class="mw-redirect" title="Dimidium">Dimidium</a> (51 Peg b) </td> <td data-sort-value="1.025">Unknown </td> <td style="text-align:center;">– </td> <td>0.46 +0.06 −0.01<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td>First convincing exoplanet discovered orbiting a <a href="/wiki/Main_sequence" title="Main sequence">main-sequence</a> star. Prototype <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiter</a>. </td></tr> <tr> <td data-sort-value="1994">1995 – 1995 </td> <td><a href="/wiki/Dimidium" class="mw-redirect" title="Dimidium">Dimidium</a> (51 Peg b) </td> <td data-sort-value="1.02">Unknown </td> <td style="text-align:center;">← </td> <td>0.46 +0.06 −0.01<a href="#cite_note-Martins-2015-94">[88]</a> </td> <td>First convincing exoplanet discovered orbiting a <a href="/wiki/Main_sequence" title="Main sequence">main-sequence</a> star. Prototype <a href="/wiki/Hot_Jupiter" title="Hot Jupiter">hot Jupiter</a>. </td></tr> <tr style="background:#CEE0F2"> <td data-sort-value="1993">(1993 – 1999) </td> <td style="border:5px ridge red; background:#000000;"><a href="/wiki/File:Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/44/Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg/112px-Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg" decoding="async" width="112" height="84" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/44/Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg/168px-Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/44/Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg/224px-Artist%27s_impression_of_pulsar_planet_B1620-26c.jpg 2x" data-file-width="4000" data-file-height="3000" /></a> </td> <td><a href="/wiki/PSR_B1620%E2%88%9226_b" title="PSR B1620−26 b">PSR B1620−26 b</a> (PSR B1620-26 (AB) b, "Methuselah") </td> <td data-sort-value="1.001">Unknown </td> <td style="text-align:center;">→ </td> <td>2.5 ± 1<a href="#cite_note-Sigurdson-255">[249]</a> </td> <td>Likely larger than Poltergeist, but not confirmed as planet until 2003. First <a href="/wiki/Circumbinary_planet" title="Circumbinary planet">circumbinary planet</a>, first planet to be found in a <a href="/wiki/Globular_cluster" title="Globular cluster">globular cluster</a> and the oldest planet to be discovered (until 2020) at the age of 11.2–12.7 billion years old,<a href="#cite_note-Britt-256">[250]</a> hence the nickname, "Methuselah".<a href="#cite_note-Sigurdson-255">[249]</a><a href="#cite_note-STScI-257">[251]</a> </td></tr> <tr> <td data-sort-value="1992">1992 – 1995 </td> <td style="border:5px ridge red; background:#000000; text-align:center;"><a href="/wiki/File:PSR_B1257%2B12_B.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1a/PSR_B1257%2B12_B.jpg/112px-PSR_B1257%2B12_B.jpg" decoding="async" width="112" height="100" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1a/PSR_B1257%2B12_B.jpg/168px-PSR_B1257%2B12_B.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1a/PSR_B1257%2B12_B.jpg/224px-PSR_B1257%2B12_B.jpg 2x" data-file-width="450" data-file-height="400" /></a> </td> <td><a href="/wiki/PSR_B1257%2B12_c" class="mw-redirect" title="PSR B1257+12 c">Poltergeist</a> (PSR B1257+12 c) </td> <td data-sort-value="0.089">Unknown </td> <td style="text-align:center;">← </td> <td data-sort-value="0.0135">0.013 53 ± 0.000 63 (4.3 ± 0.2 <a href="/wiki/Earth_mass" title="Earth mass">M🜨</a>)<a href="#cite_note-nUpRl-258">[252]</a> </td> <td><a href="/wiki/List_of_exoplanets_discovered_before_2000" title="List of exoplanets discovered before 2000">First</a> confirmed planet ever discovered outside the <a href="/wiki/Solar_System" title="Solar System">Solar System</a> together with the less massive <a href="/wiki/PSR_B1257%2B12_A" title="PSR B1257+12 A">Draugr</a>, one of three <a href="/wiki/Pulsar_planet" title="Pulsar planet">pulsar planets</a> known to be orbiting the <a href="/wiki/Pulsar" title="Pulsar">pulsar</a> <a href="/wiki/PSR_B1257%2B12" title="PSR B1257+12">Lich</a>.<a href="#cite_note-vYZFq-259">[253]</a><a href="#cite_note-2LPxw-260">[254]</a> Unclear whether the planets are <a href="/wiki/Pulsar_planet#Formation" title="Pulsar planet">survivors or formed in a second round of planet formation</a> from the remnants of the <a href="/wiki/Supernova" title="Supernova">supernova</a> (see <a href="/wiki/Pulsar_planet" title="Pulsar planet">pulsar planets</a>). </td></tr> <tr style="background:#FFF8DC"> <td data-sort-value="1989">(1989 – 1992) </td> <td> </td> <td><a href="/wiki/HD_114762_b" title="HD 114762 b">HD 114762 b</a> ("Latham's Planet", HD 114762 Ab) </td> <td data-sort-value="1.05">Unknown </td> <td style="text-align:center;">* </td> <td data-sort-value="11.069">11.069 ± 0.063,<a href="#cite_note-wang-261">[255]</a> ~63.2<a href="#cite_note-Kane2012-262">[256]</a> </td> <td>Discovered in 1989 by Latham to have a minimum mass of 11.069 ± 0.063 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a> (at 90°) and a probable mass of approximately 63.2 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a> (at 10°),<a href="#cite_note-Kane2012-262">[256]</a> making the former planet the first to be spotted,<a href="#cite_note-first_exoplanet-263">[257]</a> and confirmed in 1991, it was thought to be the first discovered exoplanet until 2019 when it was confirmed to be a <a href="/wiki/Red_dwarf" title="Red dwarf">low-mass star</a> with the mass of 147.0 +39.3 −42.0 <a href="/wiki/Jupiter_mass" title="Jupiter mass">MJ</a>,<a href="#cite_note-2LAqC-264">[258]</a> making the <a href="/wiki/PSR_B1257%2B12_c" class="mw-redirect" title="PSR B1257+12 c">planet</a> above the first confirmed planet discovered ever. </td></tr> <tr style="background:#CEE0F2"> <td data-sort-value="1988">(1988 – 1992) </td> <td style="border:5px ridge cyan; background:white; text-align:center;"><a href="/wiki/File:Cepheus_constellation_map.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/6/69/Cepheus_constellation_map.png/92px-Cepheus_constellation_map.png" decoding="async" width="92" height="112" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/69/Cepheus_constellation_map.png/138px-Cepheus_constellation_map.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/69/Cepheus_constellation_map.png/184px-Cepheus_constellation_map.png 2x" data-file-width="2559" data-file-height="3119" /></a> </td> <td><a href="/wiki/Gamma_Cephei_Ab" title="Gamma Cephei Ab">Tadmor</a> (Gamma Cephei Ab) </td> <td data-sort-value="1.015">Unknown </td> <td style="text-align:center;">→ </td> <td>6.6 +2.3 −2.8<a href="#cite_note-1cbau-265">[259]</a> </td> <td>First evidence for exoplanet to receive later confirmation. First reported in 1988<a href="#cite_note-CikB8-266">[260]</a> (making it arguably the first true exoplanet discovered) and independently in 1989,<a href="#cite_note-LomZS-267">[261]</a> however, retracted in 1992<a href="#cite_note-oyrqA-268">[262]</a> due to the possibility that the stellar activity of the star mimics a planet not allowing a solid discovery claim and then finally confirmed in 2003.<a href="#cite_note-xAUtu-269">[263]</a> </td></tr> <tr style="background:pink;"> <td data-sort-value="-600">(<a href="/wiki/Jupiter#History" title="Jupiter">Antiquity</a> – 1992, 1988 or 1995) </td> <td style="border:5px ridge blue; background:#000000;"><a href="/wiki/File:Jupiter_New_Horizons.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Jupiter_New_Horizons.jpg/112px-Jupiter_New_Horizons.jpg" decoding="async" width="112" height="106" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Jupiter_New_Horizons.jpg/168px-Jupiter_New_Horizons.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Jupiter_New_Horizons.jpg/224px-Jupiter_New_Horizons.jpg 2x" data-file-width="579" data-file-height="549" /></a> </td> <td><a href="/wiki/Jupiter" title="Jupiter">Jupiter</a> </td> <td>1 (11.209 <a href="/wiki/Earth_radius" title="Earth radius">R🜨</a>)<a href="#cite_note-Prša-2016-5">[5]</a> <a href="/wiki/Jupiter_radius" title="Jupiter radius">(71 492 km)</a> </td> <td style="text-align:center;"># </td> <td>1 (317.827 <a href="/wiki/Earth_mass" title="Earth mass">M🜨</a>)<a href="#cite_note-JPL_Planets-193">[187]</a> <a href="/wiki/Jupiter_mass" title="Jupiter mass">(1.898 125 × 1027 kg)</a> </td> <td><a href="/wiki/Jupiter#Formation_and_migration" title="Jupiter">Oldest</a>, largest and most massive <a href="/wiki/Solar_System_planets" class="mw-redirect" title="Solar System planets">planet</a> in the <a href="/wiki/Solar_System" title="Solar System">Solar System</a><a href="#cite_note-:1-194">[188]</a> Observations date back to 7th or 8th century BC. Using an early telescope the <a href="/wiki/Galilean_moons" title="Galilean moons">Galilean moons</a> were discovered in 1610, the planet hosts <a href="/wiki/Moons_of_Jupiter" title="Moons of Jupiter">95 known moons</a>. Reported for reference. </td></tr> <tr class="sortbottom"> <td colspan="7">For earlier entries, see <a href="/wiki/Exoplanet#Early_speculations" title="Exoplanet">early speculations and discredited claims</a>. </td></tr></tbody></table> <div class="mw-heading mw-heading2"><h2 id="See_also">See also</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=7" title="Edit section: See also">edit</a>]</div> <ul><li><a href="/wiki/Lists_of_planets" title="Lists of planets">Lists of planets</a></li> <li><a href="/wiki/List_of_smallest_exoplanets" title="List of smallest exoplanets">List of smallest exoplanets</a></li> <li><a href="/wiki/List_of_largest_cosmic_structures" title="List of largest cosmic structures">List of largest cosmic structures</a></li> <li><a href="/wiki/List_of_largest_galaxies" title="List of largest galaxies">List of largest galaxies</a></li> <li><a href="/wiki/List_of_largest_nebulae" title="List of largest nebulae">List of largest nebulae</a></li> <li><a href="/wiki/List_of_largest_known_stars" class="mw-redirect" title="List of largest known stars">List of largest known stars</a></li> <li><a href="/wiki/Lists_of_astronomical_objects" title="Lists of astronomical objects">Lists of astronomical objects</a></li> <li><a href="/wiki/List_of_most_massive_stars" title="List of most massive stars">List of most massive stars</a></li></ul> <div class="mw-heading mw-heading2"><h2 id="Notes">Notes</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=8" title="Edit section: Notes">edit</a>]</div> <style data-mw-deduplicate="TemplateStyles:r1239543626">.mw-parser-output .reflist{margin-bottom:0.5em;list-style-type:decimal}@media screen{.mw-parser-output .reflist{font-size:90%}}.mw-parser-output .reflist .references{font-size:100%;margin-bottom:0;list-style-type:inherit}.mw-parser-output .reflist-columns-2{column-width:30em}.mw-parser-output .reflist-columns-3{column-width:25em}.mw-parser-output .reflist-columns{margin-top:0.3em}.mw-parser-output .reflist-columns ol{margin-top:0}.mw-parser-output .reflist-columns li{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .reflist-upper-alpha{list-style-type:upper-alpha}.mw-parser-output .reflist-upper-roman{list-style-type:upper-roman}.mw-parser-output .reflist-lower-alpha{list-style-type:lower-alpha}.mw-parser-output .reflist-lower-greek{list-style-type:lower-greek}.mw-parser-output .reflist-lower-roman{list-style-type:lower-roman}</style><div class="reflist reflist-lower-alpha"> <div class="mw-references-wrap"><ol class="references"> <li id="cite_note-L/Teff-9">^ <a href="#cite_ref-L/Teff_9-0">a</a> <a href="#cite_ref-L/Teff_9-1">b</a> <a href="#cite_ref-L/Teff_9-2">c</a> <a href="#cite_ref-L/Teff_9-3">d</a> <a href="#cite_ref-L/Teff_9-4">e</a> <a href="#cite_ref-L/Teff_9-5">f</a> <a href="#cite_ref-L/Teff_9-6">g</a> <a href="#cite_ref-L/Teff_9-7">h</a> <a href="#cite_ref-L/Teff_9-8">i</a> Based on the estimated temperature and luminosity via the <a href="/wiki/Stefan-Boltzmann_law" class="mw-redirect" title="Stefan-Boltzmann law">Stefan-Boltzmann law</a>. </li> <li id="cite_note-Info_1-10"><a href="#cite_ref-Info_1_10-0">^</a> Using PMS evolutionary models and a potential higher age of 1 Myr, the luminosity would be lower, and the planet would be smaller. However, this would require for the object to be closer as well, which is unlikely. Another distance estimate to the Orion Nebula Cluster would result in a luminosity 1.14 times lower and also a smaller radius.<a href="#cite_note-Fang-2016-8">[8]</a> </li> <li id="cite_note-Info_2-11"><a href="#cite_ref-Info_2_11-0">^</a> Instead of a photo-evaporating disk it may be an evaporating gaseous globule (EGG). If so, it has a mass of 2 - 28 <var>M</var>J.<a href="#cite_note-Fang-2016-8">[8]</a> </li> <li id="cite_note-Info_3-12"><a href="#cite_ref-Info_3_12-0">^</a> A calculated radius thus does not need to be the radius of the (dense) core. </li> <li id="cite_note-13"><a href="#cite_ref-13">^</a> <a href="#cite_note-Info_1-10">[b]</a> <a href="#cite_note-Info_2-11">[c]</a> <a href="#cite_note-Info_3-12">[d]</a> <a href="#cite_note-Fang-2016-8">[8]</a> </li> <li id="cite_note-HatP67-68">^ <a href="#cite_ref-HatP67_68-0">a</a> <a href="#cite_ref-HatP67_68-1">b</a> Calculated using Rp/R⋆ multiplied by R⋆. The value is later multiplied by (142984 km ÷ 1391400 km) to convert from <a href="/wiki/Solar_radius" title="Solar radius"><var>R</var>☉</a> to <a href="/wiki/Jupiter_radius" title="Jupiter radius"><var>R</var>J</a>. </li> </ol></div></div> <div class="mw-heading mw-heading2"><h2 id="References">References</h2>[<a href="/w/index.php?title=List_of_largest_exoplanets&action=edit&section=9" title="Edit section: References">edit</a>]</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r1239543626"><div class="reflist"> <div class="mw-references-wrap mw-references-columns"><ol class="references"> <li id="cite_note-8hZ77-1"><a href="#cite_ref-8hZ77_1-0">^</a> <style data-mw-deduplicate="TemplateStyles:r1238218222">.mw-parser-output cite.citation{font-style:inherit;word-wrap:break-word}.mw-parser-output .citation q{quotes:"\"""\"""'""'"}.mw-parser-output .citation:target{background-color:rgba(0,127,255,0.133)}.mw-parser-output .id-lock-free.id-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/6/65/Lock-green.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-limited.id-lock-limited a,.mw-parser-output .id-lock-registration.id-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/d/d6/Lock-gray-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .id-lock-subscription.id-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/a/aa/Lock-red-alt-2.svg")right 0.1em center/9px no-repeat}.mw-parser-output .cs1-ws-icon a{background:url("//upload.wikimedia.org/wikipedia/commons/4/4c/Wikisource-logo.svg")right 0.1em center/12px no-repeat}body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-free a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-limited a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-registration a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .id-lock-subscription a,body:not(.skin-timeless):not(.skin-minerva) .mw-parser-output .cs1-ws-icon a{background-size:contain;padding:0 1em 0 0}.mw-parser-output .cs1-code{color:inherit;background:inherit;border:none;padding:inherit}.mw-parser-output .cs1-hidden-error{display:none;color:var(--color-error,#d33)}.mw-parser-output .cs1-visible-error{color:var(--color-error,#d33)}.mw-parser-output .cs1-maint{display:none;color:#085;margin-left:0.3em}.mw-parser-output .cs1-kern-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right{padding-right:0.2em}.mw-parser-output .citation .mw-selflink{font-weight:inherit}@media screen{.mw-parser-output .cs1-format{font-size:95%}html.skin-theme-clientpref-night .mw-parser-output .cs1-maint{color:#18911f}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .cs1-maint{color:#18911f}}</style><cite class="citation web cs1"><a rel="nofollow" class="external text" href="https://science.nasa.gov/universe/exoplanets/observing-exoplanets-what-can-we-really-see/">"Observing Exoplanets: What Can We Really See?"</a>. 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href="/wiki/Template:Exoplanet" title="Template:Exoplanet"><abbr title="View this template">v</abbr></a></li><li class="nv-talk"><a href="/wiki/Template_talk:Exoplanet" title="Template talk:Exoplanet"><abbr title="Discuss this template">t</abbr></a></li><li class="nv-edit"><a href="/wiki/Special:EditPage/Template:Exoplanet" title="Special:EditPage/Template:Exoplanet"><abbr title="Edit this template">e</abbr></a></li></ul></div><div id="Exoplanets" style="font-size:114%;margin:0 4em">Exoplanets</div></th></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><a href="/wiki/Planet" title="Planet">Planet</a> <ul><li><a href="/wiki/Definition_of_planet" title="Definition of planet">Definition</a> <ul><li><a href="/wiki/IAU_definition_of_planet" title="IAU definition of planet">IAU</a></li></ul></li></ul></li> <li><a href="/wiki/Planetary_science" title="Planetary science">Planetary science</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;">Main topics</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Exoplanet" title="Exoplanet">Exoplanet</a></li> <li><a href="/wiki/Exoplanet_orbital_and_physical_parameters" title="Exoplanet orbital and physical parameters">Exoplanet orbital and physical parameters</a></li> <li><a href="/wiki/Methods_of_detecting_exoplanets" title="Methods of detecting exoplanets">Methods of detecting exoplanets</a></li> <li><a href="/wiki/Planetary_system" title="Planetary system">Planetary system</a></li> <li><a href="/wiki/Planet-hosting_star" title="Planet-hosting star">Planet-hosting stars</a></li></ul> </div></td><td class="noviewer navbox-image" rowspan="10" style="width:1px;padding:0 0 0 2px"><div><a href="/wiki/PDS_70" title="PDS 70"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/100px-PDS_70.jpg" decoding="async" width="100" height="85" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/150px-PDS_70.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/1/1c/PDS_70.jpg/200px-PDS_70.jpg 2x" data-file-width="2000" data-file-height="1692" /></a></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;">Sizes and <a href="/wiki/List_of_planet_types" title="List of planet types">types</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%;text-align:center;"><a href="/wiki/Terrestrial_planet" title="Terrestrial planet">Terrestrial</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Carbon_planet" title="Carbon planet">Carbon planet</a></li> <li><a href="/wiki/Coreless_planet" title="Coreless planet">Coreless planet</a></li> <li><a href="/wiki/Desert_planet" title="Desert planet">Desert planet</a></li> <li><a href="/wiki/Dwarf_planet" title="Dwarf planet">Dwarf planet</a></li> <li><a href="/wiki/Hycean_planet" title="Hycean planet">Hycean planet</a></li> <li><a href="/wiki/Ice_planet" title="Ice planet">Ice planet</a></li> <li><a href="/wiki/Iron_planet" title="Iron planet">Iron planet</a> (Super-Mercury)</li> <li><a href="/wiki/Lava_planet" title="Lava planet">Lava planet</a></li> <li><a href="/wiki/Ocean_world" title="Ocean world">Ocean world</a></li> <li><a href="/wiki/Mega-Earth" title="Mega-Earth">Mega-Earth</a></li> <li><a href="/wiki/Sub-Earth" title="Sub-Earth">Sub-Earth</a></li> <li><a href="/wiki/Super-Earth" title="Super-Earth">Super-Earth</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:center;"><a href="/wiki/Gas_giant" title="Gas giant">Gaseous</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Eccentric_Jupiter" title="Eccentric Jupiter">Eccentric Jupiter</a></li> <li><a href="/wiki/Mini-Neptune" title="Mini-Neptune">Mini-Neptune</a> (Gas dwarf)</li> <li><a href="/wiki/Helium_planet" title="Helium planet">Helium planet</a></li> <li><a href="/wiki/Hot_Jupiter" title="Hot Jupiter">Hot Jupiter</a></li> <li><a href="/wiki/Hot_Neptune" title="Hot Neptune">Hot Neptune</a></li> <li><a href="/wiki/Gas_giant" title="Gas giant">Gas giant</a></li> <li><a href="/wiki/Ice_giant" title="Ice giant">Ice giant</a></li> <li><a href="/wiki/Super-Jupiter" title="Super-Jupiter">Super-Jupiter</a></li> <li><a href="/wiki/Super-Neptune" title="Super-Neptune">Super-Neptune</a></li> <li><a href="/wiki/Super-puff" title="Super-puff">Super-puff</a></li> <li><a href="/wiki/Ultra-hot_Jupiter" class="mw-redirect" title="Ultra-hot Jupiter">Ultra-hot Jupiter</a></li> <li><a href="/wiki/Ultra-hot_Neptune" class="mw-redirect" title="Ultra-hot Neptune">Ultra-hot Neptune</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:center;">Other types</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Blanet" title="Blanet">Blanet</a></li> <li><a href="/wiki/Brown_dwarf" title="Brown dwarf">Brown dwarf</a></li> <li><a href="/wiki/Chthonian_planet" title="Chthonian planet">Chthonian planet</a></li> <li><a href="/wiki/Circumbinary_planet" title="Circumbinary planet">Circumbinary planet</a></li> <li><a href="/wiki/Circumtriple_planet" title="Circumtriple planet">Circumtriple planet</a></li> <li><a href="/wiki/Disrupted_planet" title="Disrupted planet">Disrupted planet</a></li> <li><a href="/wiki/Double_planet" title="Double planet">Double planet</a></li> <li><a href="/wiki/Ecumenopolis" title="Ecumenopolis">Ecumenopolis</a></li> <li><a href="/wiki/Eyeball_planet" title="Eyeball planet">Eyeball planet</a></li> <li><a href="/wiki/Giant_planet" title="Giant planet">Giant planet</a></li> <li><a href="/wiki/Mesoplanet" title="Mesoplanet">Mesoplanet</a></li> <li><a href="/wiki/Planetary-mass_object" title="Planetary-mass object">Planemo</a></li> <li><a href="/wiki/Brown_dwarf#Low-mass_brown_dwarfs_versus_high-mass_planets" title="Brown dwarf">Planet/Brown dwarf boundary</a></li> <li><a href="/wiki/Planetesimal" title="Planetesimal">Planetesimal</a></li> <li><a href="/wiki/Protoplanet" title="Protoplanet">Protoplanet</a></li> <li><a href="/wiki/Pulsar_planet" title="Pulsar planet">Pulsar planet</a></li> <li><a href="/wiki/Sub-brown_dwarf" title="Sub-brown dwarf">Sub-brown dwarf</a></li> <li><a href="/wiki/Sub-Neptune" title="Sub-Neptune">Sub-Neptune</a></li> <li><a href="/wiki/Toroidal_planet" title="Toroidal planet">Toroidal planet</a></li> <li><a href="/wiki/Ultra-cool_dwarf" title="Ultra-cool dwarf">Ultra-cool dwarf</a></li> <li><a href="/wiki/Ultra-short_period_planet" title="Ultra-short period planet">Ultra-short period planet (USP)</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Formation_and_evolution_of_the_Solar_System" title="Formation and evolution of the Solar System">Formation and evolution</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Accretion_(astrophysics)" title="Accretion (astrophysics)">Accretion</a></li> <li><a href="/wiki/Accretion_disk" title="Accretion disk">Accretion disk</a></li> <li><a href="/wiki/Asteroid_belt" title="Asteroid belt">Asteroid belt</a></li> <li><a href="/wiki/Circumplanetary_disk" title="Circumplanetary disk">Circumplanetary disk</a></li> <li><a href="/wiki/Circumstellar_disc" title="Circumstellar disc">Circumstellar disc</a></li> <li><a href="/wiki/Circumstellar_envelope" title="Circumstellar envelope">Circumstellar envelope</a></li> <li><a href="/wiki/Cosmic_dust" title="Cosmic dust">Cosmic dust</a></li> <li><a href="/wiki/Debris_disk" title="Debris disk">Debris disk</a></li> <li><a href="/wiki/Detached_object" title="Detached object">Detached object</a></li> <li><a href="/wiki/Disrupted_planet" title="Disrupted planet">Disrupted planet</a></li> <li><a href="/wiki/Accretion_disk#Excretion_disk" title="Accretion disk">Excretion disk</a></li> <li><a href="/wiki/Exozodiacal_dust" title="Exozodiacal dust">Exozodiacal dust</a></li> <li><a href="/wiki/Extraterrestrial_materials" title="Extraterrestrial materials">Extraterrestrial materials</a></li> <li><a href="/wiki/Extraterrestrial_sample_curation" title="Extraterrestrial sample curation">Extraterrestrial sample curation</a></li> <li><a href="/wiki/Giant-impact_hypothesis" title="Giant-impact hypothesis">Giant-impact hypothesis</a></li> <li><a href="/wiki/Gravitational_collapse" title="Gravitational collapse">Gravitational collapse</a></li> <li><a href="/wiki/Hills_cloud" title="Hills cloud">Hills cloud</a></li> <li><a href="/wiki/Exoplanet_interiors" title="Exoplanet interiors">Internal structure</a></li> <li><a href="/wiki/Interplanetary_dust_cloud" title="Interplanetary dust cloud">Interplanetary dust cloud</a></li> <li><a href="/wiki/Interplanetary_medium" title="Interplanetary medium">Interplanetary medium</a></li> <li><a href="/wiki/Interplanetary_space" class="mw-redirect" title="Interplanetary space">Interplanetary space</a></li> <li><a href="/wiki/Interstellar_cloud" title="Interstellar cloud">Interstellar cloud</a></li> <li><a href="/wiki/Interstellar_dust" class="mw-redirect" title="Interstellar dust">Interstellar dust</a></li> <li><a href="/wiki/Interstellar_medium" title="Interstellar medium">Interstellar medium</a></li> <li><a href="/wiki/Outer_space#Interstellar_space" title="Outer space">Interstellar space</a></li> <li><a href="/wiki/Kuiper_belt" title="Kuiper belt">Kuiper belt</a></li> <li><a href="/wiki/List_of_interstellar_and_circumstellar_molecules" title="List of interstellar and circumstellar molecules">List of interstellar and circumstellar molecules</a></li> <li><a href="/wiki/Stellar_collision#Formation_of_planets" title="Stellar collision">Merging stars</a></li> <li><a href="/wiki/Molecular_cloud" title="Molecular cloud">Molecular cloud</a></li> <li><a href="/wiki/Nebular_hypothesis" title="Nebular hypothesis">Nebular hypothesis</a></li> <li><a href="/wiki/Oort_cloud" title="Oort cloud">Oort cloud</a></li> <li><a href="/wiki/Outer_space" title="Outer space">Outer space</a></li> <li><a href="/wiki/Planetary_migration" title="Planetary migration">Planetary migration</a></li> <li><a href="/wiki/Planetary_system" title="Planetary system">Planetary system</a></li> <li><a href="/wiki/Planetesimal" title="Planetesimal">Planetesimal</a></li> <li><a href="/wiki/Nebular_hypothesis#Formation_of_planets" title="Nebular hypothesis">Planet formation</a></li> <li><a href="/wiki/Protoplanetary_disk" title="Protoplanetary disk">Protoplanetary disk</a></li> <li><a href="/wiki/Ring_system" title="Ring system">Ring system</a></li> <li><a href="/wiki/Rubble_pile" title="Rubble pile">Rubble pile</a></li> <li><a href="/wiki/Sample-return_mission" title="Sample-return mission">Sample-return mission</a></li> <li><a href="/wiki/Scattered_disc" title="Scattered disc">Scattered disc</a></li> <li><a href="/wiki/Star_formation" title="Star formation">Star formation</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Planetary_system" title="Planetary system">Systems</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Exocomet" title="Exocomet">Exocomet</a> <ul><li><a href="/wiki/Interstellar_comet" class="mw-redirect" title="Interstellar comet">Interstellar</a></li></ul></li> <li><a href="/wiki/Exomoon" title="Exomoon">Exomoon</a> <ul><li><a href="/wiki/Tidally_detached_exomoon" title="Tidally detached exomoon">Tidally detached</a></li></ul></li> <li><a href="/wiki/Rogue_planet" title="Rogue planet">Rogue planet</a></li> <li>Orbits <ul><li><a href="/wiki/Retrograde_and_prograde_motion#Exoplanets" title="Retrograde and prograde motion">Retrograde</a></li> <li><a href="/wiki/Co-orbital_configuration#Trojans" title="Co-orbital configuration">Trojan</a></li> <li><a href="/wiki/Orbital_resonance#Mean-motion_resonances_among_extrasolar_planets" title="Orbital resonance">Mean-motion resonances</a></li> <li><a href="/wiki/Titius%E2%80%93Bode_law#Lunar_systems_and_other_planetary_systems" title="Titius–Bode law">Titius–Bode law</a></li></ul></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Planetary_system#Planet-hosting_stars" title="Planetary system">Host stars</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/A-type_main-sequence_star#Planets" title="A-type main-sequence star">A</a></li> <li><a href="/wiki/B-type_main-sequence_star#Planets" title="B-type main-sequence star">B</a></li> <li><a href="/wiki/Binary_star#Planets" title="Binary star">Binary star</a></li> <li><a href="/wiki/Brown_dwarf#Planets_around_brown_dwarfs" title="Brown dwarf">Brown dwarfs</a></li> <li><a href="/wiki/F-type_main-sequence_star#Planets" title="F-type main-sequence star">F/Yellow-white dwarfs</a></li> <li><a href="/wiki/G-type_main-sequence_star#Planets" title="G-type main-sequence star">G/Yellow dwarfs</a></li> <li><a href="/wiki/Herbig_Ae/Be_star#Planets" title="Herbig Ae/Be star">Herbig Ae/Be</a></li> <li><a href="/wiki/K-type_main-sequence_star#Planets" title="K-type main-sequence star">K/Orange dwarfs</a></li> <li><a href="/wiki/Red_dwarf#Planets" title="Red dwarf">M/Red dwarfs</a></li> <li><a href="/wiki/Pulsar_planet" title="Pulsar planet">Pulsar</a></li> <li><a href="/wiki/Red_giant#Planets" title="Red giant">Red giant</a></li> <li><a href="/wiki/Subdwarf_B_star#Planetary_systems" title="Subdwarf B star">Subdwarf B</a></li> <li><a href="/wiki/Subgiant#Planets" title="Subgiant">Subgiant</a></li> <li><a href="/wiki/T_Tauri_star#Planets" title="T Tauri star">T Tauri</a></li> <li><a href="/wiki/White_dwarf#Debris_disks_and_planets" title="White dwarf">White dwarfs</a></li> <li><a href="/wiki/Yellow_giant#Planets" class="mw-redirect" title="Yellow giant">Yellow giants</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Methods_of_detecting_exoplanets" title="Methods of detecting exoplanets">Detection</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Astrometry" title="Astrometry">Astrometry</a></li> <li><a href="/wiki/Methods_of_detecting_exoplanets#Direct_imaging" title="Methods of detecting exoplanets">Direct imaging</a> <ul><li><a href="/wiki/List_of_directly_imaged_exoplanets" title="List of directly imaged exoplanets">list</a></li></ul></li> <li><a href="/wiki/Gravitational_microlensing" title="Gravitational microlensing">Microlensing</a> <ul><li><a href="/wiki/List_of_exoplanets_detected_by_microlensing" title="List of exoplanets detected by microlensing">list</a></li></ul></li> <li><a href="/wiki/Polarimetry" title="Polarimetry">Polarimetry</a></li> <li><a href="/wiki/Methods_of_detecting_exoplanets#Pulsar_timing" title="Methods of detecting exoplanets">Timing</a> <ul><li><a href="/wiki/List_of_exoplanets_detected_by_timing" title="List of exoplanets detected by timing">list</a></li></ul></li> <li><a href="/wiki/Doppler_spectroscopy" title="Doppler spectroscopy">Radial velocity</a> <ul><li><a href="/wiki/List_of_exoplanets_detected_by_radial_velocity" title="List of exoplanets detected by radial velocity">list</a></li></ul></li> <li><a href="/wiki/Methods_of_detecting_exoplanets#Transit_photometry" title="Methods of detecting exoplanets">Transit method</a> <ul><li><a href="/wiki/List_of_transiting_exoplanets" title="List of transiting exoplanets">list</a></li></ul></li> <li><a href="/wiki/Transit-timing_variation" title="Transit-timing variation">Transit-timing variation</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Planetary_habitability" title="Planetary habitability">Habitability</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Astrobiology" title="Astrobiology">Astrobiology</a></li> <li><a href="/wiki/Astrooceanography" class="mw-redirect" title="Astrooceanography">Astrooceanography</a></li> <li><a href="/wiki/Circumstellar_habitable_zone" class="mw-redirect" title="Circumstellar habitable zone">Circumstellar habitable zone</a></li> <li><a href="/wiki/Earth_analog" title="Earth analog">Earth analog</a></li> <li><a href="/wiki/Extraterrestrial_liquid_water" title="Extraterrestrial liquid water">Extraterrestrial liquid water</a></li> <li><a href="/wiki/Galactic_habitable_zone" title="Galactic habitable zone">Galactic habitable zone</a></li> <li><a href="/wiki/Habitability_of_binary_star_systems" title="Habitability of binary star systems">Habitability of binary star systems</a></li> <li><a href="/wiki/Habitability_of_F-type_main-sequence_star_systems" title="Habitability of F-type main-sequence star systems">Habitability of F-type main-sequence star systems</a></li> <li><a href="/wiki/Habitability_of_K-type_main-sequence_star_systems" title="Habitability of K-type main-sequence star systems">Habitability of K-type main-sequence star systems</a></li> <li><a href="/wiki/Habitability_of_natural_satellites" title="Habitability of natural satellites">Habitability of natural satellites</a></li> <li><a href="/wiki/Habitability_of_neutron_star_systems" title="Habitability of neutron star systems">Habitability of neutron star systems</a></li> <li><a href="/wiki/Habitability_of_red_dwarf_systems" title="Habitability of red dwarf systems">Habitability of red dwarf systems</a></li> <li><a href="/wiki/Habitability_of_yellow_dwarf_systems" title="Habitability of yellow dwarf systems">Habitability of yellow dwarf systems</a></li> <li><a href="/wiki/Habitable_zone_for_complex_life" title="Habitable zone for complex life">Habitable zone for complex life</a></li> <li><a href="/wiki/List_of_potentially_habitable_exoplanets" title="List of potentially habitable exoplanets">List of potentially habitable exoplanets</a></li> <li><a href="/wiki/Tholin" title="Tholin">Tholin</a></li> <li><a href="/wiki/Superhabitable_planet" class="mw-redirect" title="Superhabitable planet">Superhabitable planet</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;">Catalogues</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Catalog_of_Nearby_Habitable_Systems" title="Catalog of Nearby Habitable Systems">Nearby Habitable Systems</a></li> <li><a href="/wiki/Exoplanet_Data_Explorer" title="Exoplanet Data Explorer">Exoplanet Data Explorer</a></li> <li><a href="/wiki/Extrasolar_Planets_Encyclopaedia" title="Extrasolar Planets Encyclopaedia">Extrasolar Planets Encyclopaedia</a></li> <li><a href="/wiki/NASA_Exoplanet_Archive" title="NASA Exoplanet Archive">NASA Exoplanet Archive</a></li> <li><a href="/wiki/NASA_Star_and_Exoplanet_Database" title="NASA Star and Exoplanet Database">NASA Star and Exoplanet Database</a></li> <li><a href="/wiki/Open_Exoplanet_Catalogue" title="Open Exoplanet Catalogue">Open Exoplanet Catalogue</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;"><a href="/wiki/Lists_of_planets" title="Lists of planets">Lists</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li>Exoplanetary systems <ul><li><a href="/wiki/List_of_exoplanetary_host_stars" class="mw-redirect" title="List of exoplanetary host stars">Host stars</a></li> <li><a href="/wiki/List_of_multiplanetary_systems" title="List of multiplanetary systems">Multiplanetary systems</a></li> <li><a href="/wiki/List_of_stars_with_proplyds" title="List of stars with proplyds">Stars with proto-planetary discs</a></li></ul></li></ul> <ul><li><a href="/wiki/Lists_of_exoplanets" class="mw-redirect" title="Lists of exoplanets">Exoplanets</a> <ul><li><a href="/wiki/Discoveries_of_exoplanets" title="Discoveries of exoplanets">Discoveries</a></li> <li><a href="/wiki/List_of_exoplanet_extremes" title="List of exoplanet extremes">Extremes</a></li> <li><a href="/wiki/List_of_exoplanet_firsts" title="List of exoplanet firsts">Firsts</a></li> <li><a href="/wiki/List_of_nearest_exoplanets" title="List of nearest exoplanets">Nearest</a></li> <li><a class="mw-selflink selflink">Largest</a></li> <li><a href="/wiki/List_of_most_massive_exoplanets" class="mw-redirect" title="List of most massive exoplanets">Heaviest</a></li> <li><a href="/wiki/List_of_nearest_terrestrial_exoplanet_candidates" title="List of nearest terrestrial exoplanet candidates">Terrestrial candidates</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_by_the_Kepler_space_telescope" title="List of exoplanets discovered by the Kepler space telescope">Kepler</a> <ul><li><a href="/wiki/List_of_exoplanets_discovered_by_the_Kepler_space_telescope:_1%E2%80%93500" title="List of exoplanets discovered by the Kepler space telescope: 1–500">1–500</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_by_the_Kepler_space_telescope:_501%E2%80%931000" title="List of exoplanets discovered by the Kepler space telescope: 501–1000">501–1000</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_by_the_Kepler_space_telescope:_1001%E2%80%931500" title="List of exoplanets discovered by the Kepler space telescope: 1001–1500">1001–1500</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_by_the_Kepler_space_telescope:_1501%E2%80%932000" title="List of exoplanets discovered by the Kepler space telescope: 1501–2000">1501–2000</a></li></ul></li> <li><a href="/wiki/List_of_exoplanets_observed_during_Kepler%27s_K2_mission" title="List of exoplanets observed during Kepler's K2 mission">K2</a></li> <li><a href="/wiki/List_of_potentially_habitable_exoplanets" title="List of potentially habitable exoplanets">Potentially habitable</a></li> <li><a href="/wiki/List_of_proper_names_of_exoplanets" title="List of proper names of exoplanets">Proper names</a></li></ul></li></ul> <ul><li>Discovered exoplanets by year <ul><li><a href="/wiki/List_of_exoplanets_discovered_before_2000" title="List of exoplanets discovered before 2000">before 2000</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_between_2000%E2%80%932009" title="List of exoplanets discovered between 2000–2009">2000–2009</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2010" title="List of exoplanets discovered in 2010">2010</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2011" title="List of exoplanets discovered in 2011">2011</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2012" title="List of exoplanets discovered in 2012">2012</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2013" title="List of exoplanets discovered in 2013">2013</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2014" title="List of exoplanets discovered in 2014">2014</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2015" title="List of exoplanets discovered in 2015">2015</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2016" title="List of exoplanets discovered in 2016">2016</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2017" title="List of exoplanets discovered in 2017">2017</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2018" title="List of exoplanets discovered in 2018">2018</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2019" title="List of exoplanets discovered in 2019">2019</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2020" title="List of exoplanets discovered in 2020">2020</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2021" title="List of exoplanets discovered in 2021">2021</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2022" title="List of exoplanets discovered in 2022">2022</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2023" title="List of exoplanets discovered in 2023">2023</a></li> <li><a href="/wiki/List_of_exoplanets_discovered_in_2024" title="List of exoplanets discovered in 2024">2024</a></li></ul></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:right;">Other</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0"><div style="padding:0 0.25em"> <ul><li><a href="/wiki/Carl_Sagan_Institute" title="Carl Sagan Institute">Carl Sagan Institute</a></li> <li><a href="/wiki/Exoplanet_naming_convention" title="Exoplanet naming convention">Exoplanet naming convention</a></li> <li><a href="/wiki/Phase_curve_(astronomy)#Exoplanets" title="Phase curve (astronomy)">Exoplanet phase curves</a></li> <li><a href="/wiki/Exoplanetary_Circumstellar_Environments_and_Disk_Explorer" title="Exoplanetary Circumstellar Environments and Disk Explorer">Exoplanetary Circumstellar Environments and Disk Explorer</a></li> <li><a href="/wiki/Extragalactic_planet" title="Extragalactic planet">Extragalactic planet</a></li> <li><a href="/wiki/Extrasolar_planets_in_fiction" title="Extrasolar planets in fiction">Extrasolar planets in fiction</a></li> <li><a href="/wiki/Geodynamics_of_terrestrial_exoplanets" title="Geodynamics of terrestrial exoplanets">Geodynamics of terrestrial exoplanets</a></li> <li><a href="/wiki/Neptunian_desert" title="Neptunian desert">Neptunian desert</a></li> <li><a href="/wiki/Nexus_for_Exoplanet_System_Science" title="Nexus for Exoplanet System Science">Nexus for Exoplanet System Science</a></li> <li><a href="/wiki/Globular_cluster#Planets" title="Globular cluster">Planets in globular clusters</a></li> <li><a href="/wiki/Small_planet_radius_gap" title="Small planet radius gap">Small planet radius gap</a></li> <li><a href="/wiki/Sudarsky%27s_gas_giant_classification" title="Sudarsky's gas giant classification">Sudarsky's gas giant classification</a></li></ul> </div></td></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><a href="/wiki/Discoveries_of_exoplanets" title="Discoveries of exoplanets">Discoveries of exoplanets</a></li> <li><a href="/wiki/List_of_exoplanet_search_projects" title="List of exoplanet search projects">Search projects</a></li></ul> </div></td></tr></tbody></table></div>    </div><noscript><img src="https://login.wikimedia.org/wiki/Special:CentralAutoLogin/start?type=1x1&useformat=desktop" alt="" width="1" height="1" style="border: none; position: absolute;"></noscript> <div class="printfooter" data-nosnippet="">Retrieved from "<a dir="ltr" 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