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id="toc-mw-content-text" class="vector-toc-list-item vector-toc-level-1"> <a href="#" class="vector-toc-link"> <div class="vector-toc-text">序言</div> </a> </li> <li id="toc-歷史" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#歷史"> <div class="vector-toc-text"> 1 歷史 </div> </a> <ul id="toc-歷史-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-巴蒂金和布朗的假說" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#巴蒂金和布朗的假說"> <div class="vector-toc-text"> 2 巴蒂金和布朗的假說 </div> </a> <button aria-controls="toc-巴蒂金和布朗的假說-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> 开关巴蒂金和布朗的假說子章节 </button> <ul id="toc-巴蒂金和布朗的假說-sublist" class="vector-toc-list"> <li id="toc-軌道" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#軌道"> <div class="vector-toc-text"> 2.1 軌道 </div> </a> <ul id="toc-軌道-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-質量和半徑" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#質量和半徑"> <div class="vector-toc-text"> 2.2 質量和半徑 </div> </a> <ul id="toc-質量和半徑-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-起源" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#起源"> <div class="vector-toc-text"> 2.3 起源 </div> </a> <ul id="toc-起源-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-證據" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#證據"> <div class="vector-toc-text"> 2.4 證據 </div> </a> <ul id="toc-證據-sublist" class="vector-toc-list"> <li id="toc-觀測：高近日點天體的軌道群集" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#觀測：高近日點天體的軌道群集"> <div class="vector-toc-text"> 2.4.1 觀測：高近日點天體的軌道群集 </div> </a> <ul id="toc-觀測：高近日點天體的軌道群集-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-模擬：再現觀察到的群集" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#模擬：再現觀察到的群集"> <div class="vector-toc-text"> 2.4.2 模擬：再現觀察到的群集 </div> </a> <ul id="toc-模擬：再現觀察到的群集-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-動力學：第九行星如何改變極端海王星外天體的軌道" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#動力學：第九行星如何改變極端海王星外天體的軌道"> <div class="vector-toc-text"> 2.4.3 動力學：第九行星如何改變極端海王星外天體的軌道 </div> </a> <ul id="toc-動力學：第九行星如何改變極端海王星外天體的軌道-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-具有大半長軸的垂直軌道中的天體" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#具有大半長軸的垂直軌道中的天體"> <div class="vector-toc-text"> 2.4.4 具有大半長軸的垂直軌道中的天體 </div> </a> <ul id="toc-具有大半長軸的垂直軌道中的天體-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-高傾角天體的軌道" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#高傾角天體的軌道"> <div class="vector-toc-text"> 2.4.5 高傾角天體的軌道 </div> </a> <ul id="toc-高傾角天體的軌道-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-歐特雲和彗星" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#歐特雲和彗星"> <div class="vector-toc-text"> 2.4.6 歐特雲和彗星 </div> </a> <ul id="toc-歐特雲和彗星-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-2019年估計" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#2019年估計"> <div class="vector-toc-text"> 2.4.7 2019年估計 </div> </a> <ul id="toc-2019年估計-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-2021年估計" class="vector-toc-list-item vector-toc-level-3"> <a class="vector-toc-link" href="#2021年估計"> <div class="vector-toc-text"> 2.4.8 2021年估計 </div> </a> <ul id="toc-2021年估計-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-接受度" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#接受度"> <div class="vector-toc-text"> 2.5 接受度 </div> </a> <ul id="toc-接受度-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-備選假說" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#備選假說"> <div class="vector-toc-text"> 3 備選假說 </div> </a> <button aria-controls="toc-備選假說-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> 开关備選假說子章节 </button> <ul id="toc-備選假說-sublist" class="vector-toc-list"> <li id="toc-臨時或巧合的群集" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#臨時或巧合的群集"> <div class="vector-toc-text"> 3.1 臨時或巧合的群集 </div> </a> <ul id="toc-臨時或巧合的群集-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-大容量圓盤中的傾斜不穩定性" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#大容量圓盤中的傾斜不穩定性"> <div class="vector-toc-text"> 3.2 大容量圓盤中的傾斜不穩定性 </div> </a> <ul id="toc-大容量圓盤中的傾斜不穩定性-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-由一個巨大的圓盤牧養" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#由一個巨大的圓盤牧養"> <div class="vector-toc-text"> 3.3 由一個巨大的圓盤牧養 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aria-haspopup="true" data-event-name="ui.dropdown-p-lang-btn" class="vector-dropdown-checkbox mw-interlanguage-selector" aria-label="前往另一种语言写成的文章。60种语言可用" > <label id="p-lang-btn-label" for="p-lang-btn-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--action-progressive mw-portlet-lang-heading-60" aria-hidden="true" > 60种语言 </label> <div class="vector-dropdown-content"> <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li class="interlanguage-link interwiki-af mw-list-item"><a href="https://af.wikipedia.org/wiki/Planeet_Nege" title="Planeet Nege – 南非荷兰语" lang="af" hreflang="af" data-title="Planeet Nege" data-language-autonym="Afrikaans" data-language-local-name="南非荷兰语" class="interlanguage-link-target">Afrikaans</a></li><li class="interlanguage-link interwiki-ar mw-list-item"><a href="https://ar.wikipedia.org/wiki/%D8%A7%D9%84%D9%83%D9%88%D9%83%D8%A8_%D8%A7%D9%84%D8%AA%D8%A7%D8%B3%D8%B9" title="الكوكب التاسع – 阿拉伯语" lang="ar" hreflang="ar" data-title="الكوكب التاسع" data-language-autonym="العربية" data-language-local-name="阿拉伯语" class="interlanguage-link-target">العربية</a></li><li class="interlanguage-link interwiki-ast mw-list-item"><a href="https://ast.wikipedia.org/wiki/Planeta_Nueve" title="Planeta Nueve – 阿斯图里亚斯语" lang="ast" hreflang="ast" data-title="Planeta Nueve" data-language-autonym="Asturianu" data-language-local-name="阿斯图里亚斯语" class="interlanguage-link-target">Asturianu</a></li><li class="interlanguage-link interwiki-az mw-list-item"><a href="https://az.wikipedia.org/wiki/Doqquzuncu_Planet" title="Doqquzuncu Planet – 阿塞拜疆语" lang="az" hreflang="az" data-title="Doqquzuncu Planet" data-language-autonym="Azərbaycanca" data-language-local-name="阿塞拜疆语" class="interlanguage-link-target">Azərbaycanca</a></li><li class="interlanguage-link interwiki-azb mw-list-item"><a href="https://azb.wikipedia.org/wiki/%D8%AF%D9%88%D9%82%D9%82%D9%88%D8%B2%D9%88%D9%86%D8%AC%D9%88_%DA%AF%D8%B2%D9%8E%DA%AF%D9%86" title="دوققوزونجو گزَگن – South Azerbaijani" lang="azb" hreflang="azb" data-title="دوققوزونجو گزَگن" data-language-autonym="تۆرکجه" data-language-local-name="South Azerbaijani" class="interlanguage-link-target">تۆرکجه</a></li><li class="interlanguage-link interwiki-bn mw-list-item"><a href="https://bn.wikipedia.org/wiki/%E0%A6%A8%E0%A6%AC%E0%A6%AE_%E0%A6%97%E0%A7%8D%E0%A6%B0%E0%A6%B9" title="নবম গ্রহ – 孟加拉语" lang="bn" hreflang="bn" data-title="নবম গ্রহ" data-language-autonym="বাংলা" data-language-local-name="孟加拉语" class="interlanguage-link-target">বাংলা</a></li><li class="interlanguage-link interwiki-ca mw-list-item"><a href="https://ca.wikipedia.org/wiki/Nov%C3%A8_planeta" title="Novè planeta – 加泰罗尼亚语" lang="ca" hreflang="ca" data-title="Novè planeta" data-language-autonym="Català" data-language-local-name="加泰罗尼亚语" class="interlanguage-link-target">Català</a></li><li class="interlanguage-link interwiki-cs mw-list-item"><a href="https://cs.wikipedia.org/wiki/Dev%C3%A1t%C3%A1_planeta" title="Devátá planeta – 捷克语" lang="cs" hreflang="cs" data-title="Devátá planeta" data-language-autonym="Čeština" data-language-local-name="捷克语" class="interlanguage-link-target">Čeština</a></li><li class="interlanguage-link interwiki-da mw-list-item"><a href="https://da.wikipedia.org/wiki/Planet_x" title="Planet x – 丹麦语" lang="da" hreflang="da" data-title="Planet x" data-language-autonym="Dansk" data-language-local-name="丹麦语" class="interlanguage-link-target">Dansk</a></li><li class="interlanguage-link interwiki-de mw-list-item"><a href="https://de.wikipedia.org/wiki/Planet_Neun" title="Planet Neun – 德语" lang="de" hreflang="de" data-title="Planet Neun" data-language-autonym="Deutsch" data-language-local-name="德语" class="interlanguage-link-target">Deutsch</a></li><li class="interlanguage-link interwiki-diq mw-list-item"><a href="https://diq.wikipedia.org/wiki/Geyren%C4%B1ko_new%C4%B1n" title="Geyrenıko newın – Dimli" lang="diq" hreflang="diq" data-title="Geyrenıko newın" data-language-autonym="Zazaki" data-language-local-name="Dimli" class="interlanguage-link-target">Zazaki</a></li><li class="interlanguage-link interwiki-en badge-Q17559452 badge-recommendedarticle badge-Q17437796 badge-featuredarticle mw-list-item" title="推荐条目、典范条目"><a href="https://en.wikipedia.org/wiki/Planet_Nine" title="Planet Nine – 英语" lang="en" hreflang="en" data-title="Planet Nine" data-language-autonym="English" data-language-local-name="英语" class="interlanguage-link-target">English</a></li><li class="interlanguage-link interwiki-eo mw-list-item"><a href="https://eo.wikipedia.org/wiki/Planedo_Na%C5%AD" title="Planedo Naŭ – 世界语" lang="eo" hreflang="eo" data-title="Planedo Naŭ" data-language-autonym="Esperanto" data-language-local-name="世界语" class="interlanguage-link-target">Esperanto</a></li><li class="interlanguage-link interwiki-es mw-list-item"><a href="https://es.wikipedia.org/wiki/Planeta_Nueve" title="Planeta Nueve – 西班牙语" lang="es" hreflang="es" data-title="Planeta Nueve" data-language-autonym="Español" data-language-local-name="西班牙语" class="interlanguage-link-target">Español</a></li><li class="interlanguage-link interwiki-et mw-list-item"><a href="https://et.wikipedia.org/wiki/%C3%9Cheksas_planeet" title="Üheksas planeet – 爱沙尼亚语" lang="et" hreflang="et" data-title="Üheksas planeet" data-language-autonym="Eesti" data-language-local-name="爱沙尼亚语" class="interlanguage-link-target">Eesti</a></li><li class="interlanguage-link interwiki-eu mw-list-item"><a href="https://eu.wikipedia.org/wiki/Bederatzigarren_planeta" title="Bederatzigarren planeta – 巴斯克语" lang="eu" hreflang="eu" data-title="Bederatzigarren planeta" data-language-autonym="Euskara" data-language-local-name="巴斯克语" class="interlanguage-link-target">Euskara</a></li><li class="interlanguage-link interwiki-fa mw-list-item"><a href="https://fa.wikipedia.org/wiki/%D8%B3%DB%8C%D8%A7%D8%B1%D9%87_%DB%B9" title="سیاره ۹ – 波斯语" lang="fa" hreflang="fa" data-title="سیاره ۹" data-language-autonym="فارسی" data-language-local-name="波斯语" class="interlanguage-link-target">فارسی</a></li><li class="interlanguage-link interwiki-fi mw-list-item"><a href="https://fi.wikipedia.org/wiki/Planeetta_Yhdeks%C3%A4n" title="Planeetta Yhdeksän – 芬兰语" lang="fi" hreflang="fi" data-title="Planeetta Yhdeksän" data-language-autonym="Suomi" data-language-local-name="芬兰语" class="interlanguage-link-target">Suomi</a></li><li class="interlanguage-link interwiki-fr mw-list-item"><a href="https://fr.wikipedia.org/wiki/Plan%C3%A8te_Neuf" title="Planète Neuf – 法语" lang="fr" hreflang="fr" data-title="Planète Neuf" data-language-autonym="Français" data-language-local-name="法语" class="interlanguage-link-target">Français</a></li><li class="interlanguage-link interwiki-frr mw-list-item"><a href="https://frr.wikipedia.org/wiki/Planeet_9" title="Planeet 9 – 北弗里西亚语" lang="frr" hreflang="frr" data-title="Planeet 9" data-language-autonym="Nordfriisk" data-language-local-name="北弗里西亚语" class="interlanguage-link-target">Nordfriisk</a></li><li class="interlanguage-link interwiki-ga mw-list-item"><a href="https://ga.wikipedia.org/wiki/Pl%C3%A1in%C3%A9ad_Naoi" title="Pláinéad Naoi – 爱尔兰语" lang="ga" hreflang="ga" data-title="Pláinéad Naoi" data-language-autonym="Gaeilge" data-language-local-name="爱尔兰语" class="interlanguage-link-target">Gaeilge</a></li><li class="interlanguage-link interwiki-gl mw-list-item"><a href="https://gl.wikipedia.org/wiki/Planeta_Nove" title="Planeta Nove – 加利西亚语" lang="gl" hreflang="gl" data-title="Planeta Nove" data-language-autonym="Galego" data-language-local-name="加利西亚语" class="interlanguage-link-target">Galego</a></li><li class="interlanguage-link interwiki-he mw-list-item"><a href="https://he.wikipedia.org/wiki/%D7%9B%D7%95%D7%9B%D7%91_%D7%9C%D7%9B%D7%AA_%D7%AA%D7%A9%D7%99%D7%A2%D7%99_(%D7%9E%D7%A9%D7%95%D7%A2%D7%A8)" title="כוכב לכת תשיעי (משוער) – 希伯来语" lang="he" hreflang="he" data-title="כוכב לכת תשיעי (משוער)" data-language-autonym="עברית" data-language-local-name="希伯来语" class="interlanguage-link-target">עברית</a></li><li class="interlanguage-link interwiki-hi mw-list-item"><a href="https://hi.wikipedia.org/wiki/%E0%A4%A8%E0%A5%8C%E0%A4%B5%E0%A4%BE%E0%A4%82_%E0%A4%97%E0%A5%8D%E0%A4%B0%E0%A4%B9" title="नौवां ग्रह – 印地语" lang="hi" hreflang="hi" data-title="नौवां ग्रह" data-language-autonym="हिन्दी" data-language-local-name="印地语" class="interlanguage-link-target">हिन्दी</a></li><li class="interlanguage-link interwiki-hr mw-list-item"><a href="https://hr.wikipedia.org/wiki/Deveti_planet" title="Deveti planet – 克罗地亚语" lang="hr" hreflang="hr" data-title="Deveti planet" data-language-autonym="Hrvatski" data-language-local-name="克罗地亚语" class="interlanguage-link-target">Hrvatski</a></li><li class="interlanguage-link interwiki-hu mw-list-item"><a href="https://hu.wikipedia.org/wiki/Felt%C3%A9telezett_kilencedik_bolyg%C3%B3_a_Naprendszerben" title="Feltételezett kilencedik bolygó a Naprendszerben – 匈牙利语" lang="hu" hreflang="hu" data-title="Feltételezett kilencedik bolygó a Naprendszerben" data-language-autonym="Magyar" data-language-local-name="匈牙利语" class="interlanguage-link-target">Magyar</a></li><li class="interlanguage-link interwiki-hy mw-list-item"><a href="https://hy.wikipedia.org/wiki/%D4%BB%D5%B6%D5%B6%D5%A5%D6%80%D5%B8%D6%80%D5%A4_%D5%B4%D5%B8%D5%AC%D5%B8%D6%80%D5%A1%D5%AF" title="Իններորդ մոլորակ – 亚美尼亚语" lang="hy" hreflang="hy" data-title="Իններորդ մոլորակ" data-language-autonym="Հայերեն" data-language-local-name="亚美尼亚语" class="interlanguage-link-target">Հայերեն</a></li><li class="interlanguage-link interwiki-it badge-Q70893996 mw-list-item" title=""><a href="https://it.wikipedia.org/wiki/Pianeta_Nove" title="Pianeta Nove – 意大利语" lang="it" hreflang="it" data-title="Pianeta Nove" data-language-autonym="Italiano" data-language-local-name="意大利语" class="interlanguage-link-target">Italiano</a></li><li class="interlanguage-link interwiki-ja mw-list-item"><a href="https://ja.wikipedia.org/wiki/%E3%83%97%E3%83%A9%E3%83%8D%E3%83%83%E3%83%88%E3%83%BB%E3%83%8A%E3%82%A4%E3%83%B3" title="プラネット・ナイン – 日语" lang="ja" hreflang="ja" data-title="プラネット・ナイン" data-language-autonym="日本語" data-language-local-name="日语" class="interlanguage-link-target">日本語</a></li><li class="interlanguage-link interwiki-jbo mw-list-item"><a href="https://jbo.wikipedia.org/wiki/sozyplin" title="sozyplin – 逻辑语" lang="jbo" hreflang="jbo" data-title="sozyplin" data-language-autonym="La .lojban." data-language-local-name="逻辑语" class="interlanguage-link-target">La .lojban.</a></li><li class="interlanguage-link interwiki-kn mw-list-item"><a href="https://kn.wikipedia.org/wiki/%E0%B2%AA%E0%B3%8D%E0%B2%B2%E0%B2%BE%E0%B2%A8%E0%B3%86%E0%B2%9F%E0%B3%8D_%E0%B2%A8%E0%B3%88%E0%B2%A8%E0%B3%8D" title="ಪ್ಲಾನೆಟ್ ನೈನ್ – 卡纳达语" lang="kn" hreflang="kn" data-title="ಪ್ಲಾನೆಟ್ ನೈನ್" data-language-autonym="ಕನ್ನಡ" data-language-local-name="卡纳达语" class="interlanguage-link-target">ಕನ್ನಡ</a></li><li class="interlanguage-link interwiki-ko mw-list-item"><a href="https://ko.wikipedia.org/wiki/%EC%A0%9C9%ED%96%89%EC%84%B1" title="제9행성 – 韩语" lang="ko" hreflang="ko" data-title="제9행성" data-language-autonym="한국어" data-language-local-name="韩语" class="interlanguage-link-target">한국어</a></li><li class="interlanguage-link interwiki-la mw-list-item"><a href="https://la.wikipedia.org/wiki/Planeta_IX" title="Planeta IX – 拉丁语" lang="la" hreflang="la" data-title="Planeta IX" data-language-autonym="Latina" data-language-local-name="拉丁语" class="interlanguage-link-target">Latina</a></li><li class="interlanguage-link interwiki-lb mw-list-item"><a href="https://lb.wikipedia.org/wiki/Plan%C3%A9it_N%C3%A9ng" title="Planéit Néng – 卢森堡语" lang="lb" hreflang="lb" data-title="Planéit Néng" data-language-autonym="Lëtzebuergesch" data-language-local-name="卢森堡语" class="interlanguage-link-target">Lëtzebuergesch</a></li><li class="interlanguage-link interwiki-lv mw-list-item"><a href="https://lv.wikipedia.org/wiki/Dev%C4%ABt%C4%81_plan%C4%93ta" title="Devītā planēta – 拉脱维亚语" lang="lv" hreflang="lv" data-title="Devītā planēta" data-language-autonym="Latviešu" data-language-local-name="拉脱维亚语" class="interlanguage-link-target">Latviešu</a></li><li class="interlanguage-link interwiki-ml mw-list-item"><a href="https://ml.wikipedia.org/wiki/%E0%B4%AA%E0%B5%8D%E0%B4%B2%E0%B4%BE%E0%B4%A8%E0%B5%86%E0%B4%B1%E0%B5%8D%E0%B4%B1%E0%B5%8D_%E0%B4%A8%E0%B4%AF%E0%B5%BB" title="പ്ലാനെറ്റ് നയൻ – 马拉雅拉姆语" lang="ml" hreflang="ml" data-title="പ്ലാനെറ്റ് നയൻ" data-language-autonym="മലയാളം" data-language-local-name="马拉雅拉姆语" class="interlanguage-link-target">മലയാളം</a></li><li class="interlanguage-link interwiki-mr mw-list-item"><a href="https://mr.wikipedia.org/wiki/%E0%A4%A8%E0%A4%B5%E0%A4%B5%E0%A4%BE_%E0%A4%97%E0%A5%8D%E0%A4%B0%E0%A4%B9" title="नववा ग्रह – 马拉地语" lang="mr" hreflang="mr" data-title="नववा ग्रह" data-language-autonym="मराठी" data-language-local-name="马拉地语" class="interlanguage-link-target">मराठी</a></li><li class="interlanguage-link interwiki-ms mw-list-item"><a href="https://ms.wikipedia.org/wiki/Planet_9" title="Planet 9 – 马来语" lang="ms" hreflang="ms" data-title="Planet 9" data-language-autonym="Bahasa Melayu" data-language-local-name="马来语" class="interlanguage-link-target">Bahasa Melayu</a></li><li class="interlanguage-link interwiki-nl mw-list-item"><a href="https://nl.wikipedia.org/wiki/Planeet_negen" title="Planeet negen – 荷兰语" lang="nl" hreflang="nl" data-title="Planeet negen" data-language-autonym="Nederlands" data-language-local-name="荷兰语" class="interlanguage-link-target">Nederlands</a></li><li class="interlanguage-link interwiki-no mw-list-item"><a href="https://no.wikipedia.org/wiki/Planet_ni" title="Planet ni – 书面挪威语" lang="nb" hreflang="nb" data-title="Planet ni" data-language-autonym="Norsk bokmål" data-language-local-name="书面挪威语" class="interlanguage-link-target">Norsk bokmål</a></li><li class="interlanguage-link interwiki-pt mw-list-item"><a href="https://pt.wikipedia.org/wiki/Planeta_Nove" title="Planeta Nove – 葡萄牙语" lang="pt" hreflang="pt" data-title="Planeta Nove" data-language-autonym="Português" data-language-local-name="葡萄牙语" class="interlanguage-link-target">Português</a></li><li class="interlanguage-link interwiki-ro mw-list-item"><a href="https://ro.wikipedia.org/wiki/A_noua_planet%C4%83" title="A noua planetă – 罗马尼亚语" lang="ro" hreflang="ro" data-title="A noua planetă" data-language-autonym="Română" data-language-local-name="罗马尼亚语" class="interlanguage-link-target">Română</a></li><li class="interlanguage-link interwiki-ru mw-list-item"><a href="https://ru.wikipedia.org/wiki/%D0%94%D0%B5%D0%B2%D1%8F%D1%82%D0%B0%D1%8F_%D0%BF%D0%BB%D0%B0%D0%BD%D0%B5%D1%82%D0%B0" title="Девятая планета – 俄语" lang="ru" hreflang="ru" data-title="Девятая планета" data-language-autonym="Русский" data-language-local-name="俄语" class="interlanguage-link-target">Русский</a></li><li class="interlanguage-link interwiki-sco mw-list-item"><a href="https://sco.wikipedia.org/wiki/Planet_nine" title="Planet nine – 苏格兰语" lang="sco" hreflang="sco" data-title="Planet nine" data-language-autonym="Scots" data-language-local-name="苏格兰语" class="interlanguage-link-target">Scots</a></li><li class="interlanguage-link interwiki-sh mw-list-item"><a href="https://sh.wikipedia.org/wiki/Deveti_planet" title="Deveti planet – 塞尔维亚-克罗地亚语" lang="sh" hreflang="sh" data-title="Deveti planet" data-language-autonym="Srpskohrvatski / српскохрватски" data-language-local-name="塞尔维亚-克罗地亚语" class="interlanguage-link-target">Srpskohrvatski / српскохрватски</a></li><li class="interlanguage-link interwiki-simple mw-list-item"><a href="https://simple.wikipedia.org/wiki/Planet_9" title="Planet 9 – Simple English" lang="en-simple" hreflang="en-simple" data-title="Planet 9" data-language-autonym="Simple English" data-language-local-name="Simple English" class="interlanguage-link-target">Simple English</a></li><li class="interlanguage-link interwiki-sk mw-list-item"><a href="https://sk.wikipedia.org/wiki/Deviata_plan%C3%A9ta" title="Deviata planéta – 斯洛伐克语" lang="sk" hreflang="sk" data-title="Deviata planéta" data-language-autonym="Slovenčina" data-language-local-name="斯洛伐克语" class="interlanguage-link-target">Slovenčina</a></li><li class="interlanguage-link interwiki-sl mw-list-item"><a href="https://sl.wikipedia.org/wiki/Deveti_planet" title="Deveti planet – 斯洛文尼亚语" lang="sl" hreflang="sl" data-title="Deveti planet" data-language-autonym="Slovenščina" data-language-local-name="斯洛文尼亚语" class="interlanguage-link-target">Slovenščina</a></li><li class="interlanguage-link interwiki-sv mw-list-item"><a href="https://sv.wikipedia.org/wiki/Planet_Nio" title="Planet Nio – 瑞典语" lang="sv" hreflang="sv" data-title="Planet Nio" data-language-autonym="Svenska" data-language-local-name="瑞典语" class="interlanguage-link-target">Svenska</a></li><li class="interlanguage-link interwiki-sw mw-list-item"><a href="https://sw.wikipedia.org/wiki/Sayari_ya_Tisa" title="Sayari ya Tisa – 斯瓦希里语" lang="sw" hreflang="sw" data-title="Sayari ya Tisa" data-language-autonym="Kiswahili" data-language-local-name="斯瓦希里语" class="interlanguage-link-target">Kiswahili</a></li><li class="interlanguage-link interwiki-th mw-list-item"><a href="https://th.wikipedia.org/wiki/%E0%B8%94%E0%B8%B2%E0%B8%A7%E0%B9%80%E0%B8%84%E0%B8%A3%E0%B8%B2%E0%B8%B0%E0%B8%AB%E0%B9%8C%E0%B9%80%E0%B8%81%E0%B9%89%E0%B8%B2" title="ดาวเคราะห์เก้า – 泰语" lang="th" hreflang="th" data-title="ดาวเคราะห์เก้า" data-language-autonym="ไทย" data-language-local-name="泰语" class="interlanguage-link-target">ไทย</a></li><li class="interlanguage-link interwiki-tr mw-list-item"><a href="https://tr.wikipedia.org/wiki/Dokuzuncu_Gezegen" title="Dokuzuncu Gezegen – 土耳其语" lang="tr" hreflang="tr" data-title="Dokuzuncu Gezegen" data-language-autonym="Türkçe" data-language-local-name="土耳其语" class="interlanguage-link-target">Türkçe</a></li><li class="interlanguage-link interwiki-tt mw-list-item"><a href="https://tt.wikipedia.org/wiki/%D0%A2%D1%83%D0%B3%D1%8B%D0%B7%D1%8B%D0%BD%D1%87%D1%8B_%D0%BF%D0%BB%D0%B0%D0%BD%D0%B5%D1%82%D0%B0" title="Тугызынчы планета – 鞑靼语" lang="tt" hreflang="tt" data-title="Тугызынчы планета" data-language-autonym="Татарча / tatarça" data-language-local-name="鞑靼语" class="interlanguage-link-target">Татарча / tatarça</a></li><li class="interlanguage-link interwiki-uk mw-list-item"><a href="https://uk.wikipedia.org/wiki/%D0%94%D0%B5%D0%B2%27%D1%8F%D1%82%D0%B0_%D0%BF%D0%BB%D0%B0%D0%BD%D0%B5%D1%82%D0%B0" title="Дев'ята планета – 乌克兰语" lang="uk" hreflang="uk" data-title="Дев'ята планета" data-language-autonym="Українська" data-language-local-name="乌克兰语" class="interlanguage-link-target">Українська</a></li><li class="interlanguage-link interwiki-ur mw-list-item"><a href="https://ur.wikipedia.org/wiki/%D9%86%D9%88%D8%A7%DA%BA_%D8%B3%DB%8C%D8%A7%D8%B1%DB%81" title="نواں سیارہ – 乌尔都语" lang="ur" hreflang="ur" data-title="نواں سیارہ" data-language-autonym="اردو" data-language-local-name="乌尔都语" class="interlanguage-link-target">اردو</a></li><li class="interlanguage-link interwiki-vi mw-list-item"><a href="https://vi.wikipedia.org/wiki/H%C3%A0nh_tinh_th%E1%BB%A9_ch%C3%ADn" title="Hành tinh thứ chín – 越南语" lang="vi" hreflang="vi" data-title="Hành tinh thứ chín" data-language-autonym="Tiếng Việt" data-language-local-name="越南语" class="interlanguage-link-target">Tiếng Việt</a></li><li class="interlanguage-link interwiki-wuu mw-list-item"><a href="https://wuu.wikipedia.org/wiki/%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F" title="第九行星 – 吴语" lang="wuu" hreflang="wuu" data-title="第九行星" data-language-autonym="吴语" data-language-local-name="吴语" class="interlanguage-link-target">吴语</a></li><li class="interlanguage-link interwiki-zh-classical mw-list-item"><a href="https://zh-classical.wikipedia.org/wiki/%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F" title="第九行星 – 文言文" lang="lzh" hreflang="lzh" data-title="第九行星" data-language-autonym="文言" data-language-local-name="文言文" class="interlanguage-link-target">文言</a></li><li class="interlanguage-link interwiki-zh-min-nan mw-list-item"><a href="https://zh-min-nan.wikipedia.org/wiki/T%C4%93_9_he%CC%8Dk-chhe%E2%81%BF" title="Tē 9 he̍k-chheⁿ – 闽南语" lang="nan" hreflang="nan" data-title="Tē 9 he̍k-chheⁿ" data-language-autonym="閩南語 / Bân-lâm-gú" data-language-local-name="闽南语" class="interlanguage-link-target">閩南語 / Bân-lâm-gú</a></li><li 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.ambox-move{border-left-color:#9932cc!important}html.skin-theme-clientpref-os .mw-parser-output .ambox-protection{border-left-color:#a2a9b1!important}}</style><table class="box-Refimprove plainlinks metadata ambox ambox-content" role="presentation"><tbody><tr><td class="mbox-image"><div style="width:52px"><a href="/wiki/File:Tango-nosources.svg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Tango-nosources.svg/45px-Tango-nosources.svg.png" decoding="async" width="45" height="45" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Tango-nosources.svg/68px-Tango-nosources.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4e/Tango-nosources.svg/90px-Tango-nosources.svg.png 2x" data-file-width="48" data-file-height="48" /></a></div></td><td class="mbox-text"><div class="mbox-text-span">此條目需要补充更多<a href="/wiki/Wikipedia:%E5%88%97%E6%98%8E%E6%9D%A5%E6%BA%90" title="Wikipedia:列明来源">来源</a>。 (2024年3月22日) 请协助補充多方面<a href="/wiki/Wikipedia:%E5%8F%AF%E9%9D%A0%E6%9D%A5%E6%BA%90" title="Wikipedia:可靠来源">可靠来源</a>以<a class="external text" href="https://zh.wikipedia.org/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit">改善这篇条目</a>，<a href="/wiki/Wikipedia:%E5%8F%AF%E4%BE%9B%E6%9F%A5%E8%AF%81" class="mw-redirect" title="Wikipedia:可供查证">无法查证</a>的内容可能會因為<a href="/wiki/Template:Fact" class="mw-redirect" title="Template:Fact">异议提出</a>而被移除。 致使用者：请搜索一下条目的标题（来源搜索：<a rel="nofollow" class="external text" href="//www.google.com/search?&as_eq=wikipedia&q=%22%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F%22">"第九行星"</a> — <a rel="nofollow" class="external text" href="//www.google.com/search?q=%22%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F%22">网页</a>、<a rel="nofollow" class="external text" href="//www.google.com/search?tbm=nws&q=&as_src=-newswire+-wire+-presswire+-PR+-press+-release+-wikipedia&q=%22%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F%22">新闻</a>、<a rel="nofollow" class="external text" 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div.hatnote{padding-left:2em;margin-bottom:0.8em;margin-top:0.8em}.mw-parser-output .hatnote-notice-img::after{content:"\202f \202f \202f \202f "}.mw-parser-output .hatnote-notice-img-small::after{content:"\202f \202f "}.mw-parser-output .hatnote+link+.hatnote{margin-top:-0.5em}body.skin-minerva .mw-parser-output .hatnote-notice-img,body.skin-minerva .mw-parser-output .hatnote-notice-img-small{display:none}@media print{body.ns-0 .mw-parser-output .hatnote{display:none!important}}</style><div role="note" class="hatnote navigation-not-searchable"><a href="/wiki/Wikipedia:%E6%B6%88%E6%AD%A7%E4%B9%89" title="Wikipedia:消歧义"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/f/fb/Confusion_grey.svg/25px-Confusion_grey.svg.png" decoding="async" width="25" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/fb/Confusion_grey.svg/38px-Confusion_grey.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/fb/Confusion_grey.svg/50px-Confusion_grey.svg.png 2x" data-file-width="260" data-file-height="200" /></a>提示：此条目的主题不是<a href="/wiki/%E5%B8%95%E8%A5%BF%E7%93%A6%E5%B0%94%C2%B7%E7%BD%97%E5%A8%81%E5%B0%94" title="帕西瓦尔·罗威尔">帕西瓦爾·羅威爾</a>於1906年提出的<a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F" title="假設的海王星外行星">行星X</a>。</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r85100532" /><div role="note" class="hatnote navigation-not-searchable"><a href="/wiki/Wikipedia:%E6%B6%88%E6%AD%A7%E4%B9%89" title="Wikipedia:消歧义"><img alt="" src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5f/Disambig_gray.svg/25px-Disambig_gray.svg.png" decoding="async" width="25" height="19" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5f/Disambig_gray.svg/38px-Disambig_gray.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5f/Disambig_gray.svg/50px-Disambig_gray.svg.png 2x" data-file-width="220" data-file-height="168" /></a>此條目介紹的是於2014年首次提出的假想行星。关于曾被歸類為太陽系第九顆行星的矮行星，请见「<a href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F" title="冥王星">冥王星</a>」。关于其他用法，请见「<a href="/wiki/%E7%AC%AC%E4%B9%9D%E9%A1%86%E8%A1%8C%E6%98%9F" class="mw-disambig" title="第九顆行星">第九顆行星</a>」。</div> <style data-mw-deduplicate="TemplateStyles:r83732082">.mw-parser-output .infobox-subbox{padding:0;border:none;margin:-3px;width:auto;min-width:100%;font-size:100%;clear:none;float:none;background-color:transparent}.mw-parser-output .infobox-3cols-child{margin:auto}.mw-parser-output .infobox .navbar{font-size:100%}body.skin-minerva .mw-parser-output .infobox-header,body.skin-minerva .mw-parser-output .infobox-subheader,body.skin-minerva .mw-parser-output .infobox-above,body.skin-minerva .mw-parser-output .infobox-title,body.skin-minerva .mw-parser-output .infobox-image,body.skin-minerva .mw-parser-output .infobox-full-data,body.skin-minerva .mw-parser-output .infobox-below{text-align:center}@media screen{html.skin-theme-clientpref-night .mw-parser-output .infobox-full-data:not(.notheme)>div:not(.notheme)[style]{background:#1f1f23!important;color:#f8f9fa}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .infobox-full-data:not(.notheme) div:not(.notheme){background:#1f1f23!important;color:#f8f9fa}}html.skin-theme-clientpref-night .mw-parser-output .infobox td div:not(.notheme)[style]{background:transparent!important;color:var(--color-base,#202122)}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .infobox td div:not(.notheme)[style]{background:transparent!important;color:var(--color-base,#202122)}}html.skin-theme-clientpref-night .mw-parser-output .infobox td div.NavHead:not(.notheme)[style]{background:transparent!important}}@media screen and (prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .infobox td div.NavHead:not(.notheme)[style]{background:transparent!important}}@media(min-width:640px){body.skin--responsive .mw-parser-output .infobox-table{display:table!important}body.skin--responsive .mw-parser-output .infobox-table>caption{display:table-caption!important}body.skin--responsive .mw-parser-output .infobox-table>tbody{display:table-row-group}body.skin--responsive .mw-parser-output .infobox-table tr{display:table-row!important}body.skin--responsive .mw-parser-output .infobox-table th,body.skin--responsive .mw-parser-output .infobox-table td{padding-left:inherit;padding-right:inherit}}</style><table class="infobox"><caption class="infobox-title fn org">Planet Nine</caption><tbody><tr><td colspan="2" class="infobox-image"><a href="/wiki/File:Planet_nine_artistic_plain.png" class="mw-file-description" title="Planet Nine depicted as a dark sphere distant from the Sun with the Milky Way in the background."><img alt="Planet Nine depicted as a dark sphere distant from the Sun with the Milky Way in the background." src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5a/Planet_nine_artistic_plain.png/220px-Planet_nine_artistic_plain.png" decoding="async" width="220" height="147" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5a/Planet_nine_artistic_plain.png/330px-Planet_nine_artistic_plain.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5a/Planet_nine_artistic_plain.png/440px-Planet_nine_artistic_plain.png 2x" data-file-width="1920" data-file-height="1280" /></a><div class="infobox-caption"><div style="padding:0.1em 0;line-height:1.2em;">藝術家對第九行星的印象，它使銀河系中央黯然失色，遠處是太陽；海王星的軌道顯示為圍繞太陽的小橢圓（參見<a href="/wiki/File:Planet_nine_artistic_plain_labeled.png" title="File:Planet nine artistic plain labeled.png">帶標籤的版本</a>）</div></div></td></tr><tr><th colspan="2" class="infobox-header" style=""><a href="/wiki/%E8%BB%8C%E9%81%93%E5%8F%83%E6%95%B8" class="mw-redirect" title="軌道參數">軌道參數</a></th></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E6%8B%B1%E9%BB%9E" title="拱點">遠日點</a></th><td class="infobox-data" style="">560+260 −140 AU<a href="#cite_note-Brown_Batygin_2021z-1">[1]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E6%8B%B1%E9%BB%9E" title="拱點">近日點</a></th><td class="infobox-data" style="">340+80 −70 AU<a href="#cite_note-Brown_Batygin_2021z-1">[1]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">半長軸</a></th><td class="infobox-data" style="">460+160 −100 AU<a href="#cite_note-Brown_Batygin_2021z-1">[1]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">離心率</a></th><td class="infobox-data" style="">6999200000000000000♠0.2–6999500000000000000♠0.5<a href="#cite_note-P9H2019-2">[2]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%BD%A8%E9%81%93%E5%91%A8%E6%9C%9F" title="轨道周期">軌道週期</a></th><td class="infobox-data" style="">9,900+5,500 −3,100 yr<a href="#cite_note-3">[A]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%BB%8C%E9%81%93%E5%82%BE%E8%A7%92" title="軌道傾角">軌道傾角</a></th><td class="infobox-data" style="">16+5 −°<a href="#cite_note-Batygin2021-4">[3]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%BF%91%E5%BF%83%E9%BB%9E%E5%B9%85%E8%A7%92" title="近心點幅角">近日點參數</a></th><td class="infobox-data" style="">7000261799387799150♠150° (est.)<a href="#cite_note-TAJ201601-5">[4]</a></td></tr><tr><th colspan="2" class="infobox-header" style="">物理特徵</th></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%B3%AA%E9%87%8F" class="mw-redirect" title="質量">質量</a></th><td class="infobox-data" style="">6.3+2.3 −1.5 <a href="/wiki/%E5%9C%B0%E7%90%83%E8%B4%A8%E9%87%8F" title="地球质量">M🜨</a><a href="#cite_note-Brown_Batygin_2021z-1">[1]</a></td></tr><tr><th scope="row" class="infobox-label" style=""><a href="/wiki/%E8%A6%96%E6%98%9F%E7%AD%89" class="mw-redirect" title="視星等">視星等</a></th><td class="infobox-data" style="">~21<a href="#cite_note-Batygin2021-4">[3]</a></td></tr><tr><td colspan="2" class="infobox-below"><div class="reflist" style="list-style-type: decimal;"> </div></td></tr></tbody></table> 第九行星（英語：Planet Nine）是位於<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB#海王星外的区域" title="太阳系">太陽系外圍</a>的<a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E7%9A%84%E5%81%87%E8%A8%AD%E5%A4%A9%E9%AB%94%E5%88%97%E8%A1%A8" title="太陽系的假設天體列表">假想行星</a><a href="#cite_note-P9H2019-2">[2]</a><a href="#cite_note-TAJ201601-5">[4]</a>。它的引力效應可以解釋一組<a href="/wiki/%E6%A5%B5%E7%AB%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="極端海王星外天體">極端海王星外天體</a><a href="/wiki/%E8%BB%8C%E9%81%93" class="mw-disambig" title="軌道">軌道</a>的特殊聚集，這些天體位於<a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F" title="海王星">海王星</a>之外，繞太陽運行的平均距離是地球的250倍以上。這些極端海王星外天體往往在一個扇形區內最接近太陽，其軌道也有類似的傾斜。這些排列表明，一顆未被發現的行星可能正在引導已知最遙遠的<a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB" class="mw-redirect" title="太陽系">太陽系</a>天體的軌道<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-Sheppard2014-6">[5]</a><a href="#cite_note-fatty-7">[6]</a>。儘管如此，一些天文學家仍對這一結論提出了質疑，並斷言這是由於在一年中的大部分時間裏發現和跟踪這些天體的困難，因此是由於觀測偏差造成極端海王星外天體軌道的聚集<a href="#cite_note-TC-20200525-8">[7]</a>。 基於早期的估計，這顆假設的<a href="/wiki/%E8%B6%85%E7%B4%9A%E5%9C%B0%E7%90%83" class="mw-redirect" title="超級地球">超級地球</a>大小的行星的質量是地球的五到十倍，距離太陽的<a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">細長軌道</a>是地球的400到800倍。2021年，科學家對軌道的估計進行了改進，得出了較小的半長軸為380+140 −80 AU<a href="#cite_note-Batygin2021-4">[3]</a>。此後不久更新為460 +160 −100 AU<a href="#cite_note-Brown_Batygin_2021z-1">[1]</a>。<a href="/wiki/%E5%BA%B7%E6%96%AF%E5%9D%A6%E4%B8%81%C2%B7%E8%B2%9D%E8%92%82%E9%87%91" title="康斯坦丁·貝蒂金">康斯坦丁·貝蒂金</a>和<a href="/wiki/%E9%BA%A5%E5%85%8B%C2%B7%E5%B8%83%E6%9C%97" class="mw-redirect mw-disambig" title="麥克·布朗">麥克·布朗</a>提出，第九行星可能是一顆<a href="/wiki/%E5%B7%A8%E8%A1%8C%E6%98%9F" title="巨行星">巨行星</a>的<a href="/wiki/%E8%A1%8C%E6%98%9F%E6%A0%B8%E5%BF%83" title="行星核心">核心</a>，該行星在太陽系<a href="/wiki/%E6%98%9F%E9%9B%B2%E5%81%87%E8%AA%AA" title="星雲假說">起源</a>期間被木星從其原始軌道拋出。其他人提出這顆行星是從另一顆恆星<a href="/w/index.php?title=%E5%BC%95%E5%8A%9B%E6%8D%95%E7%8D%B2&action=edit&redlink=1" class="new" title="引力捕獲（页面不存在）">捕獲</a>的<a href="#cite_note-Mustill_etal_2016-9">[8]</a>，之前是一顆<a href="/wiki/%E6%98%9F%E9%9A%9B%E8%A1%8C%E6%98%9F" title="星際行星">星際行星</a>；或者它在遙遠的軌道上形成，並被一顆經過的恆星拉入偏心軌道<a href="#cite_note-TAJ201601-5">[4]</a>。 儘管<a href="/wiki/%E5%BB%A3%E5%9F%9F%E7%B4%85%E5%A4%96%E7%B7%9A%E5%B7%A1%E5%A4%A9%E6%8E%A2%E6%B8%AC%E8%A1%9B%E6%98%9F" title="廣域紅外線巡天探測衛星">廣域紅外線巡天探測衛星</a>（WISE）和<a href="/wiki/%E6%B3%9B%E6%98%9F%E8%AE%A1%E5%88%92" class="mw-redirect" title="泛星计划">泛星計劃</a>等巡天都沒有探測到第九行星，但它們並沒有排除在外太陽系中存在海王星直徑的天體<a href="#cite_note-bnb20160617-10">[9]</a><a href="#cite_note-Luhman2014-11">[10]</a>。過去的這些巡天探測第九行星的能力取決於它的位置和特徵。正在使用<a href="/wiki/%E5%BB%A3%E5%9F%9F%E7%B4%85%E5%A4%96%E7%B7%9A%E5%B7%A1%E5%A4%A9%E6%8E%A2%E6%B8%AC%E8%A1%9B%E6%98%9F#近地天體觀測" title="廣域紅外線巡天探測衛星">NEOWISE</a>和8米<a href="/wiki/%E6%98%B4%E6%98%9F%E5%9B%A2%E6%9C%9B%E8%BF%9C%E9%95%9C" title="昴星团望远镜">昴星團望遠鏡</a>對其餘區域進行進一步調查<a href="#cite_note-Meisner_etal_2017b-12">[11]</a><a href="#cite_note-sciencemag201601-13">[12]</a>。除非觀測到第九行星，否則它的存在純屬猜測。已經提出了幾種替代假設來解釋觀察到的<a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="海王星外天體">海王星外天體</a>（TNO）的聚集。 <meta property="mw:PageProp/toc" /> <div class="mw-heading mw-heading2"><h2 id="歷史">歷史</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=1" title="编辑章节：歷史">编辑</a>]</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r85100532" /><div role="note" class="hatnote navigation-not-searchable">参见：<a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F#遙遠物體的軌道" title="假設的海王星外行星">假設的海王星外行星 § 遙遠物體的軌道</a>和<a href="/wiki/%E7%8D%A8%E7%AB%8B%E5%A4%A9%E9%AB%94#軌道" title="獨立天體">獨立天體 § 軌道</a></div> 在1846年<a href="/w/index.php?title=%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%9A%84%E7%99%BC%E7%8F%BE&action=edit&redlink=1" class="new" title="海王星的發現（页面不存在）">海王星的發現</a>（英语：<a href="https://en.wikipedia.org/wiki/Discovery_of_Neptune" class="extiw" title="en:Discovery of Neptune">Discovery of Neptune</a>）之後，有相當多的猜測認為有可能另一顆行星存在於其軌道之外。其中最著名的理論預測了一顆遙遠行星的存在，這顆行星正在影響<a href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F" title="天王星">天王星</a>和<a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F" title="海王星">海王星</a>的軌道。經過廣泛的計算，<a href="/wiki/%E5%B8%95%E8%A5%BF%E7%93%A6%E7%88%BE%C2%B7%E7%BE%85%E5%A8%81%E7%88%BE" class="mw-redirect" title="帕西瓦爾·羅威爾">帕西瓦爾·羅威爾</a>預測了這顆假想的跨海王星行星的可能軌道和位置，並於1906年開始對其進行廣泛的蒐索。他將這個假想物體稱為「<a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F#歷史" title="假設的海王星外行星">X行星</a>」；這個名字之前曾被加布裏埃爾·達利特英語：Gabriel Dallet<a href="#cite_note-grosser-14">[13]</a><a href="#cite_note-tombaugh-15">[14]</a>。<a href="/wiki/%E5%85%8B%E8%8E%B1%E5%BE%B7%C2%B7%E6%B1%A4%E5%8D%9A" title="克莱德·汤博">克萊德·湯博</a>繼續了羅威爾的搜尋，並於1930年<a href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F#歷史" title="冥王星">發現冥王星</a>，但很快就被確定為太小，不符合羅威爾的X行星的資格<a href="#cite_note-Croswell1997-16">[15]</a>。1989年<a href="/wiki/%E6%97%85%E8%A1%8C%E8%80%852%E5%8F%B7" title="旅行者2号">航海家2號</a>飛越海王星後，天王星的預測軌道和觀測軌道之間的差異被確定是由於使用了以前不準確的海王星質量<a href="#cite_note-Browne_1993-17">[16]</a>。 通過軌道擾動等間接手段探測<a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F" title="假設的海王星外行星">海王星以外的行星</a>的嘗試可以追溯到發現冥王星之前。其中第一位是<a href="/w/index.php?title=%E5%96%AC%E6%B2%BB%C2%B7%E7%A6%8F%E5%B8%83%E6%96%AF_(%E7%A7%91%E5%AD%B8%E5%AE%B6)&action=edit&redlink=1" class="new" title="喬治·福布斯 (科學家)（页面不存在）">喬治·福布斯 (科學家)</a>（英语：<a href="https://en.wikipedia.org/wiki/George_Forbes_(scientist)" class="extiw" title="en:George Forbes (scientist)">George Forbes (scientist)</a>），他在1880年假設存在兩顆<a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F" title="假設的海王星外行星">跨海王星行星</a>。第一顆與太陽的平均距離或<a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">半長軸</a>為100 <a href="/wiki/%E5%A4%A9%E6%96%87%E5%96%AE%E4%BD%8D" title="天文單位">天文單位</a>（AU），是地球的100倍，第二顆將具有 300 AU 的半長軸。他的工作被認為與最近的第九行星理論相似，因為行星將負責幾個物體軌道的群集，在這種情況下，週期性<a href="/wiki/%E5%BD%97%E6%98%9F" title="彗星">彗星</a>的<a href="/wiki/%E8%BF%91%E6%97%A5%E9%BB%9E%E5%92%8C%E9%81%A0%E6%97%A5%E9%BB%9E" title="近日點和遠日點">遠日點</a>距離的群集接近100和300天文單位。這類似於<a href="/wiki/%E7%9F%AD%E5%91%A8%E6%9C%9F%E5%BD%97%E6%98%9F" title="短周期彗星">木星族彗星</a>在其軌道附近群集<a href="#cite_note-Millholland_Laughlin_2017-18">[17]</a><a href="#cite_note-Forbes_1880-19">[18]</a>。 2004年，發現軌道特殊的小行星<a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F90377" class="mw-redirect" title="小行星90377">賽德娜</a>，導致人們猜測它遇到了一個巨大的天體，而不是已知的任何行星之一。賽德娜的軌道是<a href="/wiki/%E7%8D%A8%E7%AB%8B%E5%A4%A9%E9%AB%94" title="獨立天體">獨立軌道</a>，<a href="/wiki/%E8%BF%91%E6%97%A5%E9%BB%9E" class="mw-redirect" title="近日點">近日點</a>距離為76天文單位，因此即使通過近日點時也不會受到海王星引力影響其軌跡的海王星外天體。有幾位作者提出，賽德娜是在遇到一個巨大的天體後進入這個軌道的，例如遙遠軌道上的未知行星，與形成太陽的<a href="/wiki/%E7%96%8F%E6%95%A3%E6%98%9F%E5%9C%98" class="mw-redirect" title="疏散星團">疏散星團</a>的成員，或後來經過太陽系附近的另一顆恆星<a href="#cite_note-spaceBrown-20">[19]</a><a href="#cite_note-iopsciencesedna-21">[20]</a>。2014年3月，在類似的軌道上發現了第二個近日點距離為80天文單位的<a href="/wiki/%E9%A1%9E%E5%A1%9E%E5%BE%B7%E5%A8%9C%E5%A4%A9%E9%AB%94#已知天體" class="mw-redirect" title="類塞德娜天體">類賽德娜天體</a>，<a href="/wiki/2012_VP113" title="2012 VP113">2012 VP113</a>，這再次引發了人們的猜測，即遙遠的太陽系中仍然存在一個未知的超級地球<a href="#cite_note-guardianSuperEarth-22">[21]</a><a href="#cite_note-searchformoreSedna-23">[22]</a>。 在2012年的一次會議上，羅德尼·戈麥斯（英語：Rodney Gomes）提出：一顆未被發現的行星負責一些軌道獨立的ETNO的軌道，並且有著巨大<a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">半長軸</a>的<a href="/wiki/%E5%8D%8A%E4%BA%BA%E9%A9%AC%E5%B0%8F%E8%A1%8C%E6%98%9F" title="半人马小行星">半人馬小行星</a>，而這些<a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E5%B0%8F%E5%A4%A9%E9%AB%94" title="太陽系小天體">太陽系小天體</a>們穿過巨行星的軌道<a href="#cite_note-llmysteries-24">[23]</a><a href="#cite_note-nosmokingGun-25">[24]</a>。擬議的海王星質量行星將位於遙遠（1500 AU）、偏心（<a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">離心率</a> 0.4）和傾斜（<a href="/wiki/%E8%BB%8C%E9%81%93%E5%82%BE%E8%A7%92" title="軌道傾角">傾角</a> ：40°）的軌道上。像第九行星一樣，它會導致半長軸大於300天文單位的物體的近日點振盪，將一些送入行星交叉軌道，而另一些則進入像賽德娜這樣的獨立軌道。戈麥斯、蘇亞雷斯（英語：Soares）和布拉瑟（英語：Brasser）在2015年發表了一篇文章，詳細介紹了他們的論點<a href="#cite_note-Gomes_2015-26">[25]</a>。 2014年，天文學家<a href="/wiki/%E4%B9%8D%E5%BE%B7%C2%B7%E7%89%B9%E9%AD%AF%E5%B8%8C%E7%95%A5" class="mw-redirect" title="乍德·特魯希略">查德·楚希羅</a>和<a href="/wiki/%E5%8F%B2%E8%80%83%E7%89%B9%C2%B7%E6%A1%91%E5%BE%B7%C2%B7%E9%9B%AA%E6%9F%8F" class="mw-redirect" title="史考特·桑德·雪柏">史考特·桑德·雪柏</a>注意到賽德娜和2012 VP113以及其它幾個ETNO的軌道相似。他們提出，一顆位於200至300天文單位之間圓形軌道上的未知行星正在擾亂它們的軌道<a href="#cite_note-Sheppard2014-6">[5]</a>。那年晚些時候，勞爾和卡洛斯·德拉富恩特·馬科斯認為，<a href="/wiki/%E8%BB%8C%E9%81%93%E5%85%B1%E6%8C%AF" class="mw-redirect" title="軌道共振">軌道共振</a>中的兩顆大質量行星是產生如此多軌道的相似性所必需的，當時已知有13顆獨立軌道的小行星<a href="#cite_note-Marcos_2014-27">[26]</a>。使用39顆ETNO的更大樣本，他們估計較近的行星的半長軸在300-400天文單位範圍內，離心率相對較低，傾角接近14度<a href="#cite_note-randomsearch-28">[27]</a>。 <div class="mw-heading mw-heading2"><h2 id="巴蒂金和布朗的假說">巴蒂金和布朗的假說</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=2" title="编辑章节：巴蒂金和布朗的假說">编辑</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Planet_nine_path_in_orion2.png" class="mw-file-description"><img alt="Starfield with hypothetical path of Planet Nine" src="//upload.wikimedia.org/wikipedia/commons/thumb/c/c5/Planet_nine_path_in_orion2.png/330px-Planet_nine_path_in_orion2.png" decoding="async" width="330" height="208" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/c/c5/Planet_nine_path_in_orion2.png/495px-Planet_nine_path_in_orion2.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/c/c5/Planet_nine_path_in_orion2.png/660px-Planet_nine_path_in_orion2.png 2x" data-file-width="2882" data-file-height="1814" /></a><figcaption>一條依據假想的第九行星遠日點推導出，由西向東穿過<a href="/wiki/%E7%8D%B5%E6%88%B6%E5%BA%A7" title="獵戶座">獵戶座</a>的路徑。它源自布朗的部落格上的意境構思<a href="#cite_note-findplanet9-29">[28]</a>。</figcaption></figure> 2016年初，加州理工學院的芭蒂金和布朗描述了第九行星如何解釋六個ETNO的相似軌道，並提出了該行星可能的軌道<a href="#cite_note-TAJ201601-5">[4]</a>。這個假說也可以解釋軌道<a href="/wiki/%E5%9E%82%E7%9B%B4" title="垂直">垂直</a>於<a href="/wiki/%E5%85%A7%E8%A1%8C%E6%98%9F" class="mw-redirect" title="內行星">內行星</a>的ETNOs<a href="#cite_note-TAJ201601-5">[4]</a>和其它有極端傾斜的小行星<a href="#cite_note-Batygin_Brown_high_inc-30">[29]</a>，並被作為對太陽<a href="/wiki/%E7%B9%9E%E5%9B%BA%E5%AE%9A%E8%BB%B8%E6%97%8B%E8%BD%89" title="繞固定軸旋轉">旋轉軸</a><a href="/wiki/%E8%BD%89%E8%BB%B8%E5%82%BE%E8%A7%92" title="轉軸傾角">傾斜</a>的解釋<a href="#cite_note-Gomes_Deienno_Morbidelli_2016-31">[30]</a>。 <div class="mw-heading mw-heading3"><h3 id="軌道">軌道</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=3" title="编辑章节：軌道">编辑</a>]</div> 最初假設第九行星以<a href="/wiki/%E6%A9%A2%E5%9C%93%E8%BB%8C%E9%81%93" title="橢圓軌道">橢圓軌道</a>繞太陽運行，偏心率為6999200000000000000♠0.2 to 0.5，其<a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">半長軸</a>估計為7013598391482800000♠400 to 800 AU<a href="#cite_note-32">[B]</a>，大約是海王星到太陽距離的13到26倍。這顆行星需要10,000到20,000年的時間才能繞太陽運行一個完整的軌道，並且它與地球軌道平面<a href="/wiki/%E9%BB%83%E9%81%93" class="mw-redirect" title="黃道">黃道</a>的傾角預計為6999261799387799150♠15° to 25°<a href="#cite_note-P9H2019-2">[2]</a><a href="#cite_note-NASA_PlanetX-33">[31]</a><a href="#cite_note-34">[C]</a>。遠日點，即或離太陽最遠的點，將位於<a href="/wiki/%E9%87%91%E7%89%9B%E5%BA%A7" title="金牛座">金牛座</a><a href="#cite_note-Brown_YouTube2017-35">[32]</a>，而近日點是離太陽最近的點，將位於<a href="/wiki/%E5%B7%A8%E8%9B%87%E5%BA%A7" title="巨蛇座">巨蛇座</a>（頭）、<a href="/wiki/%E8%9B%87%E5%A4%AB%E5%BA%A7" title="蛇夫座">蛇夫座</a>或<a href="/wiki/%E5%A4%A9%E7%A7%A4%E5%BA%A7" title="天秤座">天秤座</a><a href="#cite_note-B-BCharts-36">[33]</a><a href="#cite_note-Lemonick2016-37">[34]</a>。布朗認為，如果第九行星存在，那麼使用<a href="/wiki/%E9%87%8D%E5%8A%9B%E5%8A%A9%E6%8E%A8#奧伯特效應" title="重力助推">動力彈弓</a><a href="/wiki/%E8%BB%8C%E8%B7%A1" class="mw-redirect" title="軌跡">軌跡</a>可以在短短20年內到達它<a href="#cite_note-newscientist-38">[35]</a>。 <div class="mw-heading mw-heading3"><h3 id="質量和半徑">質量和半徑</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=4" title="编辑章节：質量和半徑">编辑</a>]</div> 據估計，這顆行星的質量是地球的5到10倍，半徑是地球的2到4倍<a href="#cite_note-P9H2019-2">[2]</a>。布朗認為，如果第九行星存在，它的質量足以在45億年（太陽系的年齡）裡<a href="/wiki/%E6%B8%85%E9%99%A4%E9%84%B0%E8%BF%91%E7%9A%84%E5%B0%8F%E5%A4%A9%E9%AB%94" title="清除鄰近的小天體">清除其軌道</a>，以它的引力支配著太陽系的外緣，這足以使它符合成為<a href="/wiki/%E8%A1%8C%E6%98%9F%E5%AE%9A%E7%BE%A9#IAU的定義" title="行星定義">行星的當前定義</a> <a href="#cite_note-lurking-39">[36]</a>。天文學家讓-呂克·瑪戈特（Jean-Luc Margot）也表示，第九行星符合它的標準，如果它被探測到，將有資格成為一顆行星<a href="#cite_note-Margot_2016-40">[37]</a><a href="#cite_note-Margot_2015-41">[38]</a>。 <div class="mw-heading mw-heading3"><h3 id="起源">起源</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=5" title="编辑章节：起源">编辑</a>]</div> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r85100532" /><div role="note" class="hatnote navigation-not-searchable">参见：<a href="/wiki/%E5%B0%BC%E6%96%AF%E6%A8%A1%E5%9E%8B" title="尼斯模型">尼斯模型</a>、<a href="/w/index.php?title=Five-planet_Nice_model&action=edit&redlink=1" class="new" title="Five-planet Nice model（页面不存在）">Five-planet Nice model</a>和<a href="/wiki/%E8%A1%8C%E6%98%9F%E9%81%B7%E7%A7%BB" title="行星遷移">行星遷移</a></div> 已經研究了第九行星的幾種可能起源，包括它從已知巨行星附近拋射，從另一顆恆星捕獲，以及「原位形成」。在他們最初的文章中，巴蒂金和布朗提出，第九行星在離太陽更近的地方形成，並在星雲時代與<a href="/wiki/%E6%9C%A8%E6%98%9F" title="木星">木星</a>或<a href="/wiki/%E5%9C%9F%E6%98%9F" title="土星">土星</a>近距離接觸後，被拋射到遙遠的偏心軌道<a href="#cite_note-TAJ201601-5">[4]</a>。然後，要麼是附近恆星的引力，要麼是來自<a href="/wiki/%E5%A4%AA%E9%99%BD%E6%98%9F%E9%9B%B2" title="太陽星雲">太陽星雲</a>的氣態殘餘物的拖曳<a href="#cite_note-Bromley_Kenyon_2016-42">[39]</a>降低了其軌道的偏心率。這個過程提高了它的近日點，使它不受其他行星的影響，處於一個非常寬闊但穩定的軌道上<a href="#cite_note-nytimes9thplanet-43">[40]</a><a href="#cite_note-caltechFAQ-44">[41]</a>。 據估計，這種情況發生的幾率僅為百分之幾<a href="#cite_note-Bailey_Fabrycky-45">[42]</a>。如果它沒有被扔進太陽系最遠的地方，第九行星可能會從<a href="/wiki/%E5%8E%9F%E8%A1%8C%E6%98%9F%E7%9B%A4" title="原行星盤">原行星盤</a>中吸積更多的質量，並發展成<a href="/wiki/%E6%B0%A3%E6%85%8B%E5%B7%A8%E8%A1%8C%E6%98%9F" title="氣態巨行星">氣態巨行星</a>或<a href="/wiki/%E5%86%B0%E5%B7%A8%E8%A1%8C%E6%98%9F" title="冰巨行星">冰巨行星</a>的核心<a href="#cite_note-lurking-39">[36]</a><a href="#cite_note-dl2018-46">[43]</a>。相對的，它的增長很早就停止了，使它的質量低於天王星或海王星<a href="#cite_note-Izidoro_etal_2015-47">[44]</a>。 來自巨大的<a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F" title="小行星">小行星</a>帶的<a href="/wiki/%E5%8B%95%E6%85%8B%E6%91%A9%E6%93%A6" title="動態摩擦">動態摩擦</a>也可能使第九行星被捕獲到一個穩定的軌道上。最近的模型表明，60–130<a href="/wiki/%E5%9C%B0%E7%90%83%E8%B4%A8%E9%87%8F" title="地球质量">M🜨</a>的小行星盤可能是在氣體從原行星盤的外部清除時形成的<a href="#cite_note-Carrera_etal_2017-48">[45]</a>。當第九行星穿過這個圓盤時，它的引力會改變單個物體的路徑，從而降低第九行星相對於它的速度。這將降低第九行星的離心率並穩定其軌道。如果這個圓盤有一個遙遠的內邊緣，即100–200<a href="/wiki/%E5%A4%A9%E6%96%87%E5%96%AE%E4%BD%8D" title="天文單位">{{{2}}}</a>，一顆遇到海王星的行星將有20%的幾率在與第九行星相似的軌道上被捕獲，如果內緣在200{{{2}}}，更有可能觀測到軌道的群集。與氣態星雲不同，小行星盤可能已經存在很長時間，因此可能允許後來的捕獲<a href="#cite_note-Eriksson_etal_2017-49">[46]</a>。 與另一顆恆星的相遇也可能改變遙遠行星的軌道，將其從圓形軌道轉變為偏心軌道。在這個距離上「原位」形成一顆行星需要一個非常巨大和廣泛的圓盤<a href="#cite_note-TAJ201601-5">[4]</a>，或者固體在消散的盤中向外漂移，形成一個狹窄的環，行星從這個環中吸積了十億年<a href="#cite_note-Kenyon_Bromley_2016-50">[47]</a>。如果一顆行星在太陽處於其原始星團中時，在如此遠的距離上形成，那麼它在高度偏心的軌道上與太陽保持束縛的概率約為10%<a href="#cite_note-Li_Adams_2016-51">[48]</a>。然而，當太陽仍然在它形成的疏散星團中時，任何延伸的圓盤都會受到經過的恆星引力破壞和光蒸發造成質量的損失<a href="#cite_note-P9H2019-2">[2]</a>。 第九行星可能是在太陽和另一顆恆星近距離接觸中，從太陽系外捕獲的。如果一顆行星在圍繞這顆恆星的遙遠軌道上，<a href="/w/index.php?title=%E6%AD%90%E6%8B%89%E4%B8%89%E9%AB%94%E5%95%8F%E9%A1%8C&action=edit&redlink=1" class="new" title="歐拉三體問題（页面不存在）">三體</a>在相遇期間的相互作用可能會改變行星的路徑，使其處於圍繞太陽的穩定軌道上。一顆起源於沒有木星質量行星系統中的行星，可能會在遙遠的偏心軌道上停留更長的時間，從而增加其被捕獲的機會<a href="#cite_note-Mustill_etal_2016-9">[8]</a>。更廣泛的可能軌道範圍將使它在相對低傾角軌道上被捕獲的幾率降低到1-2%<a href="#cite_note-Li_Adams_2016-51">[48]</a>。<a href="/w/index.php?title=Amir_Siraj&action=edit&redlink=1" class="new" title="Amir Siraj（页面不存在）">Amir Siraj</a>和<a href="/w/index.php?title=Avi_Loeb&action=edit&redlink=1" class="new" title="Avi Loeb（页面不存在）">Avi Loeb</a>發現，如果太陽曾經有一個遙遠的、質量相等的聯星伴星，那麼太陽奪取第九行星的幾率就會增加20倍<a href="#cite_note-Siraj_Loab_2020-52">[49]</a><a href="#cite_note-Passant_2020-53">[50]</a>。這個過程也可能發生在星際行星上，但它們被捕獲的可能性要小得多，只有0.05-0.10%被捕獲在類似於第九行星的軌道上<a href="#cite_note-Parker_etal_2017-54">[51]</a>。 <div class="mw-heading mw-heading3"><h3 id="證據">證據</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=6" title="编辑章节：證據">编辑</a>]</div> <style data-mw-deduplicate="TemplateStyles:r84265675">.mw-parser-output .hlist dl,.mw-parser-output .hlist ol,.mw-parser-output .hlist ul{margin:0;padding:0}.mw-parser-output .hlist dd,.mw-parser-output .hlist dt,.mw-parser-output .hlist li{margin:0;display:inline}.mw-parser-output .hlist.inline,.mw-parser-output .hlist.inline dl,.mw-parser-output .hlist.inline ol,.mw-parser-output .hlist.inline ul,.mw-parser-output .hlist dl dl,.mw-parser-output .hlist dl ol,.mw-parser-output .hlist dl ul,.mw-parser-output .hlist ol dl,.mw-parser-output .hlist ol ol,.mw-parser-output .hlist ol ul,.mw-parser-output .hlist ul dl,.mw-parser-output .hlist ul ol,.mw-parser-output .hlist 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.mw-parser-output .sidebar:not(.notheme) .sidebar-list-title,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-subgroup,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-pretitle,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-title,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-title-with-pretitle,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-heading,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-above,html.skin-theme-clientpref-os .mw-parser-output .sidebar:not(.notheme) .sidebar-below{background:inherit!important;color:inherit!important;border-color:#54595d!important}html.skin-theme-clientpref-os .mw-parser-output .sidebar a:not(.new):not(.mw-selflink):link{color:var(--color-progressive)!important}}@media print{body.ns-0 .mw-parser-output .sidebar{display:none!important}}</style><table class="sidebar nomobile nowraplinks" style="width: auto;"><caption class="sidebar-outer-title"><a href="/wiki/%E9%81%A0%E8%B7%9D%E5%B0%8F%E8%A1%8C%E6%98%9F" title="遠距小行星">遠距小行星</a>的種類</caption><tbody><tr><td class="sidebar-content" style="text-align: left;"> <ul><li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%85%A7%E5%A4%A9%E9%AB%94" title="海王星內天體">海王星內天體</a> <ul><li><a href="/wiki/%E5%8D%8A%E4%BA%BA%E9%A9%AC%E5%B0%8F%E8%A1%8C%E6%98%9F" title="半人马小行星">半人马小行星</a></li> <li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%89%B9%E6%B4%9B%E4%BC%8A" title="海王星特洛伊">海王星特洛伊</a></li></ul></li> <li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="海王星外天體">海王星外天體</a>（TNOs）‡ <ul><li><a href="/wiki/%E6%9F%AF%E4%BC%8A%E4%BC%AF%E5%B8%A6" title="柯伊伯带">古柏帶天體</a>（KBOs） <ul><li><a href="/wiki/%E5%82%B3%E7%B5%B1%E5%8F%A4%E6%9F%8F%E5%B8%B6%E5%A4%A9%E9%AB%94" title="傳統古柏帶天體">傳統古柏帶天體</a>（QB1天體，cubewanos）</li> <li><a href="/wiki/%E5%85%B1%E6%8C%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="共振海王星外天體">共振海王星外天體</a> <ul><li><a href="/wiki/%E5%86%A5%E6%97%8F%E5%B0%8F%E5%A4%A9%E9%AB%94" title="冥族小天體">冥族小天體</a>（與海王星2:3共振）</li></ul></li></ul></li> <li><a href="/wiki/%E9%9B%A2%E6%95%A3%E7%9B%A4" title="離散盤">離散盤天體</a> <ul><li><a href="/wiki/%E5%85%B1%E6%8C%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="共振海王星外天體">共振離散盤天體</a></li></ul></li> <li><a href="/wiki/%E7%8D%A8%E7%AB%8B%E5%A4%A9%E9%AB%94" title="獨立天體">獨立天體</a></li> <li><a href="/wiki/%E6%A5%B5%E7%AB%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="極端海王星外天體">極端海王星外天體</a></li> <li><a href="/wiki/%E9%A1%9E%E5%A1%9E%E5%BE%B7%E5%A8%9C%E5%A4%A9%E9%AB%94" class="mw-redirect" title="類塞德娜天體">類塞德娜天體</a></li> <li><a href="/wiki/%E5%A5%A5%E5%B0%94%E7%89%B9%E4%BA%91" title="奥尔特云">歐特雲天體</a>（ICO/OCOs）</li></ul></li></ul></td> </tr><tr><td class="sidebar-below" style="font-weight: normal;"> ‡  註：在海王星外的<a href="/wiki/%E7%9F%AE%E8%A1%8C%E6%98%9F" title="矮行星">矮行星</a>都屬於 "<a href="/wiki/%E9%A1%9E%E5%86%A5%E7%9F%AE%E8%A1%8C%E6%98%9F" title="類冥矮行星">類冥矮行星</a>"</td></tr><tr><td class="sidebar-navbar" style="line-height:1.6"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84265675" /><style data-mw-deduplicate="TemplateStyles:r84244141">.mw-parser-output .navbar{display:inline;font-weight:normal}.mw-parser-output .navbar-collapse{float:left;text-align:left}.mw-parser-output .navbar-boxtext{word-spacing:0}.mw-parser-output .navbar ul{display:inline-block;white-space:nowrap;line-height:inherit}.mw-parser-output .navbar-brackets::before{margin-right:-0.125em;content:"[ "}.mw-parser-output .navbar-brackets::after{margin-left:-0.125em;content:" ]"}.mw-parser-output .navbar li{word-spacing:-0.125em}.mw-parser-output .navbar a>span,.mw-parser-output .navbar a>abbr{text-decoration:inherit}.mw-parser-output .navbar-mini abbr{font-variant:small-caps;border-bottom:none;text-decoration:none;cursor:inherit}.mw-parser-output .navbar-ct-full{font-size:110%;margin:0 8em}.mw-parser-output .navbar-ct-mini{font-size:110%;margin:0 5em}html.skin-theme-clientpref-night .mw-parser-output .navbar li a abbr{color:var(--color-base)!important}@media(prefers-color-scheme:dark){html.skin-theme-clientpref-os .mw-parser-output .navbar li a abbr{color:var(--color-base)!important}}@media print{.mw-parser-output .navbar{display:none!important}}</style><div class="navbar plainlinks hlist navbar-mini"><ul><li class="nv-view"><a href="/wiki/Template:Distant_minor_planets_sidebar" title="Template:Distant minor planets sidebar"><abbr title="查看该模板">查</abbr></a></li><li class="nv-talk"><a href="/wiki/Template_talk:Distant_minor_planets_sidebar" title="Template talk:Distant minor planets sidebar"><abbr title="讨论该模板">论</abbr></a></li><li class="nv-edit"><a href="/wiki/Special:%E7%BC%96%E8%BE%91%E9%A1%B5%E9%9D%A2/Template:Distant_minor_planets_sidebar" title="Special:编辑页面/Template:Distant minor planets sidebar"><abbr title="编辑该模板">编</abbr></a></li></ul></div></td></tr></tbody></table> 第九行星的引力影響可以解釋太陽系的四個特點<a href="#cite_note-Brennan_2017-55">[52]</a>： <ul><li>極端海王星外天體軌道的群集；</li> <li>像<a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F90377" class="mw-redirect" title="小行星90377">賽德娜</a>這樣的天體的高近日點，它們是<a href="/wiki/%E7%8D%A8%E7%AB%8B%E5%A4%A9%E9%AB%94" title="獨立天體">獨立</a>，不受海王星的影響；</li> <li>極端海王星外天體的高傾角，其軌道大致垂直於八顆已知行星的軌道；</li> <li>半長軸小於100 AU的高傾角<a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="海王星外天體">海王星外天體</a>（TNO）。</li></ul> 第九行星最初被提出來解釋軌道的群集，通過一種機制來解釋像賽德娜這樣的天體的高近日點。其中一些天體演變成垂直軌道是出乎意料的，但發現與先前觀察到的天體相匹配。後來發現，當其它行星被納入模擬時，一些具有垂直軌道的物體的軌道會向較小的半長軸方向演化。儘管已經為這些特性提供了許多其它機制，但第九行星的引力影響是唯一可以解釋所有四種現象的機制。然而，第九行星的引力也會增加穿過其軌道的其它物體的傾角，這可能會留下<a href="/wiki/%E9%9B%A2%E6%95%A3%E7%9B%A4" title="離散盤">離散盤的物體</a><a href="#cite_note-Kaib_etal_2019-56">[53]</a>，即在海王星之外軌道運行，半長軸大於50天文單位的天體，以及傾角分佈比觀測到的更寬的<a href="/wiki/%E7%9F%AD%E5%91%A8%E6%9C%9F%E5%BD%97%E6%98%9F" title="短周期彗星">短週期彗星</a><a href="#cite_note-Nesvorny_etal_2017-57">[54]</a>。在此之前，第九行星被假設為太陽自轉軸相對於行星軌道傾斜 6 度的原因<a href="#cite_note-Stirone_sun_tilt-58">[55]</a>，但最近對其預測軌道和質量的更新將這種偏移限制在〜1度<a href="#cite_note-P9H2019-2">[2]</a>。 <div class="mw-heading mw-heading4"><h4 id="觀測：高近日點天體的軌道群集">觀測：高近日點天體的軌道群集</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=7" title="编辑章节：觀測：高近日點天體的軌道群集">编辑</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Orbit1.svg" class="mw-file-description"><img alt="天體的軌道顯示為與黃道相交的傾斜橢圓。" src="//upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Orbit1.svg/260px-Orbit1.svg.png" decoding="async" width="260" height="234" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Orbit1.svg/390px-Orbit1.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/eb/Orbit1.svg/520px-Orbit1.svg.png 2x" data-file-width="555" data-file-height="500" /></a><figcaption>該圖說明瞭天體的真實異常、近心點的論點、升交點的經度和傾角。</figcaption></figure> 特魯希略和謝潑德最早描述了具有大半長軸的海王星外天體軌道的群集，他們注意到賽德娜和類賽德娜的2012 VP113軌道之間的相似性。如果沒有第九行星的存在，這些軌道應該是隨機分佈的，沒有偏好任何方向。經過進一步分析，特魯希略和謝潑德觀察到，近日點大於7012448793612100000♠30 AU且半長軸大於7013224396806050000♠150 AU的12個海王星外天體的<a href="/wiki/%E8%BF%91%E5%BF%83%E9%BB%9E%E5%B9%85%E8%A7%92" title="近心點幅角">近日點參數</a>聚集在零度附近，這意味著當它們最接近太陽時，它們會升至黃道上方。特魯希略和謝潑德提出，這種排列是由海王星以外的一顆巨大的未知行星通過<a href="/wiki/%E5%8F%A4%E5%9C%A8%E6%A9%9F%E5%88%B6" title="古在機制">古在機制</a>引起的<a href="#cite_note-Sheppard2014-6">[5]</a>。對於具有相似半長軸的物體，古在機制會將其近日點的論點限制在接近0度或180度。這種限制允許具有偏心和傾斜軌道的物體避免靠近行星，因為它們會在距離太陽最近和最遠的點之間穿過行星軌道的平面，並在它們遠高於或低於其軌道時穿過行星的軌道<a href="#cite_note-Marcos_2014-27">[26]</a><a href="#cite_note-KopanyasKozai-59">[56]</a>。特魯希略和謝潑德關於這些物體如何通過古在機制對齊的假設，已被進一步的分析和證據所取代<a href="#cite_note-TAJ201601-5">[4]</a>。 巴蒂金和布朗試圖反駁特魯希略和謝潑德提出的機制，還檢查了具有大半長軸的海王星外天體的軌道<a href="#cite_note-TAJ201601-5">[4]</a>。在排除了特魯希略和謝潑德的原始分析中由於接近海王星而不穩定，或受到海王星<a href="/wiki/%E8%BB%8C%E9%81%93%E5%85%B1%E6%8C%AF" class="mw-redirect" title="軌道共振">平均運動共振</a>影響的物體後，巴蒂金和布朗確定其餘六個物體的近日點論點（賽德娜、2012 VP113、<a href="/w/index.php?title=%E5%B0%8F%E8%A1%8C%E6%98%9F474640&action=edit&redlink=1" class="new" title="小行星474640（页面不存在）">小行星474640</a>（英语：<a href="https://en.wikipedia.org/wiki/474640_Alicanto" class="extiw" title="en:474640 Alicanto">474640 Alicanto</a>）、<a href="/w/index.php?title=2010_GB174&action=edit&redlink=1" class="new" title="2010 GB174（页面不存在）">2010 GB174</a>、<a href="/w/index.php?title=(148209)_2000_CR105&action=edit&redlink=1" class="new" title="(148209) 2000 CR105（页面不存在）">2000 CR105</a>、和<a href="/w/index.php?title=(445473)_2010_VZ98&action=edit&redlink=1" class="new" title="(445473) 2010 VZ98（页面不存在）">2010 VZ98</a>）被群集在一起，大約在7000555014702134197♠318°±8°。這一發現與古在機制如何傾向於將軌道與近日點在0°或180°的論點對齊不一致<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-60">[D]</a>。 <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Planet_Nine_animation.gif" class="mw-file-description"><img alt="動畫圖從內行星和外行星的軌道縮小到最外層物體的大幅擴展軌道，這些天體指向螢幕的左側。第九行星的假想軌道顯示為一條虛線。" src="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Planet_Nine_animation.gif/260px-Planet_Nine_animation.gif" decoding="async" width="260" height="195" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/09/Planet_Nine_animation.gif/390px-Planet_Nine_animation.gif 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/09/Planet_Nine_animation.gif/520px-Planet_Nine_animation.gif 2x" data-file-width="640" data-file-height="480" /></a><figcaption>六個遙遠的海王星外天體之間的軌道相關性導致了這一假設。（參見：<a href="/wiki/File:Planet_Nine_-_black_background.png" title="File:Planet Nine - black background.png">最終幀軌道</a>。）</figcaption></figure> 巴蒂金和布朗還發現，半長軸大於250 AU和近日點超過30 AU的六個ETNO的軌道（賽德娜、2012 VP113、Alicanto、2010 GB174、<a href="/w/index.php?title=2007_TG422&action=edit&redlink=1" class="new" title="2007 TG422（页面不存在）">2007 TG422</a>、和<a href="/w/index.php?title=2013_RF98&action=edit&redlink=1" class="new" title="2013 RF98（页面不存在）">2013 RF98</a>），它們在空間上與它們的近日點方向大致相同，導致它們的<a href="/wiki/%E8%BF%91%E5%BF%83%E9%BB%9E%E7%B6%93%E5%BA%A6" title="近心點經度">近日點黃經</a>的群集，這是它們最接近太陽的位置。這六個天體的軌道也相對於<a href="/wiki/%E9%BB%84%E9%81%93%E5%B9%B3%E9%9D%A2" class="mw-redirect" title="黄道平面">黃道</a>的軌道傾斜，並且大約<a href="/wiki/%E5%85%B1%E9%9D%A2" title="共面">共面</a>，產生了它們的<a href="/wiki/%E5%8D%87%E4%BA%A4%E9%BB%9E%E9%BB%83%E7%B6%93" title="升交點黃經">升交點黃經</a>的群集，即它們各自通過黃道上升的方向。他們確定這種對齊組合是偶然的只有0.007%的可能性<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-cbcRadio-61">[57]</a><a href="#cite_note-planetaryblog201601-62">[58]</a>。這六個天體是通過六架望遠鏡的六次不同調查發現的。這使得群集不太可能是由於觀察偏差造成的，例如將望遠鏡指向天空的特定部分。觀測到的群集應該在幾億年後被抹去，因為近日點和升交點的位置發生了變化，或者<a href="/wiki/%E9%80%B2%E5%8B%95" title="進動">恆星進動</a>，由於它們的半長軸和偏心率不同，它們以不同的速率變化<a href="#cite_note-63">[E]</a>。這表明群集不可能是由於遙遠的過去的事件造成的<a href="#cite_note-TAJ201601-5">[4]</a>，例如，一顆路過的恆星<a href="#cite_note-Hands_etal_2019-64">[59]</a>，並且很可能由繞太陽運行物體的引力場維持<a href="#cite_note-TAJ201601-5">[4]</a>。 六顆天體中的兩顆（2013 RF98和Alicanto）也具有非常相似的軌道和光譜<a href="#cite_note-gtcres-65">[60]</a><a href="#cite_note-binary-ScienceDaily-66">[61]</a>。這導致了一種建議，即它們是在與遙遠物體相遇時在遠日點附近被破壞的<a href="/wiki/%E9%9B%99%E5%B0%8F%E8%A1%8C%E6%98%9F" title="雙小行星">聯星天體</a>。聯星的破壞需要相對近距離的相遇，但這在離太陽很遠的地方變得不太可能<a href="#cite_note-Marcos_binary_disruption-67">[62]</a>。 在後來的一篇文章中，特魯希略和謝潑德指出了近日點的經度與半長軸大於150天文單位的海王星外天體的近日點幅角之間的相關性。近日點經度為 0–120° 的近日點參數在280° 到360° 之間，近日點經度在180° 和 340° 之間的參數在0° 和40° 之間。該相關性的統計學意義為99.99%。他們認為，這種相關性是由於這些物體的軌道通過其軌道上方或下方來避免接近大質量行星<a href="#cite_note-trujillo20160912-68">[63]</a>。 卡洛斯和勞爾·德拉富恩特·馬科斯在2017年的一篇文章中指出，到ETNO升交點的距離分佈，以及半人馬小行星和具有大半長軸的彗星的距離分佈可能是<a href="/wiki/%E9%9B%99%E5%B3%B0%E5%88%86%E5%B8%83" title="雙峰分布">雙峰</a>。他們認為這是由於ETNO避免接近半長軸為300-400天文單位的行星<a href="#cite_note-nodes-69">[64]</a><a href="#cite_note-nodes_phys.org-70">[65]</a>。隨著數據的增加（40個物件），ETNO的相互節點距離分佈顯示出最短的相互升交點和降交點距離之間存在統計學上的顯著不對稱性，這可能不是由於觀測偏差，而可能是外部擾動的結果<a href="#cite_note-nodes2-71">[66]</a><a href="#cite_note-nodes3-72">[67]</a>。 <style data-mw-deduplicate="TemplateStyles:r70089473/mw-parser-output/.tmulti">.mw-parser-output .tmulti .thumbinner{display:flex;flex-direction:column}.mw-parser-output .tmulti .trow{display:flex;flex-direction:row;clear:left;flex-wrap:wrap;width:100%;box-sizing:border-box}.mw-parser-output .tmulti .tsingle{margin:1px;float:left}.mw-parser-output .tmulti .theader{clear:both;font-weight:bold;text-align:center;align-self:center;background-color:transparent;width:100%}.mw-parser-output .tmulti .thumbcaption{background-color:transparent}.mw-parser-output .tmulti .text-align-left{text-align:left}.mw-parser-output .tmulti .text-align-right{text-align:right}.mw-parser-output .tmulti .text-align-center{text-align:center}@media all and (max-width:720px){.mw-parser-output .tmulti .thumbinner{width:100%!important;box-sizing:border-box;max-width:none!important;align-items:center}.mw-parser-output .tmulti .trow{justify-content:center}.mw-parser-output .tmulti .tsingle{float:none!important;max-width:100%!important;box-sizing:border-box;text-align:center}.mw-parser-output .tmulti .tsingle .thumbcaption{text-align:left}.mw-parser-output .tmulti .trow>.thumbcaption{text-align:center}}</style><div class="thumb tmulti tleft"><div class="thumbinner" style="width:667px;max-width:667px"><div class="trow"><div class="theader">極端海王星外天體繞軌道運行</div></div><div class="trow"><div class="tsingle" style="width:414px;max-width:414px"><div class="thumbimage" style="height:214px;overflow:hidden"><a href="/wiki/File:Planet_nine-etnos_now-new3.png" class="mw-file-description"><img alt="極端海王星外天體和第九行星的軌道" src="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/Planet_nine-etnos_now-new3.png/412px-Planet_nine-etnos_now-new3.png" decoding="async" width="412" height="215" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/9/93/Planet_nine-etnos_now-new3.png/618px-Planet_nine-etnos_now-new3.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/9/93/Planet_nine-etnos_now-new3.png/824px-Planet_nine-etnos_now-new3.png 2x" data-file-width="1709" data-file-height="891" /></a></div><div class="thumbcaption">六個原始軌道和<a href="/wiki/%E6%A5%B5%E7%AB%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="極端海王星外天體">八顆額外的極端海王星外天體</a>，其近日點附近的當前位置為紫色，假設的第九行星軌道為綠色</div></div><div class="tsingle" style="width:249px;max-width:249px"><div class="thumbimage" style="height:214px;overflow:hidden"><a href="/wiki/File:Planet_nine-etnos_now-close-new.png" class="mw-file-description"><img alt="極端海王星外天體和行星軌道的特寫" src="//upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Planet_nine-etnos_now-close-new.png/247px-Planet_nine-etnos_now-close-new.png" decoding="async" width="247" height="214" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Planet_nine-etnos_now-close-new.png/371px-Planet_nine-etnos_now-close-new.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/2/2d/Planet_nine-etnos_now-close-new.png/494px-Planet_nine-etnos_now-close-new.png 2x" data-file-width="1028" data-file-height="892" /></a></div><div class="thumbcaption">13顆極端海王星外天體當前位置的特寫視圖</div></div></div></div></div> <div style="clear:both;"></div> <div class="mw-heading mw-heading4"><h4 id="模擬：再現觀察到的群集">模擬：再現觀察到的群集</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=8" title="编辑章节：模擬：再現觀察到的群集">编辑</a>]</div> 極端海王星外天體軌道的群集和近日點的升高在包括第九行星在內的模擬中再現。在巴蒂金和布朗進行的模擬中，以隨機方向開始的半長軸高達550 AU的離散盤天體群被雕刻成空間受限軌道的近似<a href="/wiki/%E5%85%B1%E7%B7%9A" class="mw-disambig" title="共線">共線</a>和共面群的高度偏心軌道上。這使得大多數天體的近日點指向相似的方向，並且天體的軌道具有相似的傾斜度。這些天體中有許多進入了像賽德娜這樣的高近日點軌道，出乎意料的是，有些進入了垂直軌道。巴蒂金和布朗後來注意到這些軌道以前被觀測到過<a href="#cite_note-TAJ201601-5">[4]</a>。 在他們最初的分析中，巴蒂金和布朗發現，在使用10個地球質量的模擬中，最好的再現前六個極端海王星外天體的軌道分佈{{efn-ua|巴蒂金和布朗提供了質量的一個數量級估計。 <ul><li>如果「M」等於0.1地球質量，那麼動力學演化將以異常緩慢的速度進行，太陽系的壽命可能不足以進行所需的軌道雕刻。</li> <li>如果「M」等於1地球質量，那麼長壽命拱點的反對齊軌道確實會發生，但不穩定軌道的移除將發生在比太陽系當前演化更長的時間尺度上。因此，即使它們會表現出對特定拱點方向的偏好，它們也不會像數據那樣表現出真正的侷限性。</li> <li>他們還指出，「M」大於10地球質量意味著半長軸更長。因此，他們估計該天體的質量可能在5到15M🜨。位於以下軌道的行星：<a href="#cite_note-73">[F]</a></li> <li><a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">半長軸</a>「a」 ≈ 7014104718509490000♠700 AU（<a href="/wiki/%E8%BD%A8%E9%81%93%E5%91%A8%E6%9C%9F" title="轨道周期">軌道週期</a> 7001.5=18,520 年）</li> <li><a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">離心率</a> 「e」 ≈ 0.6，（<a href="/wiki/%E8%BF%91%E6%97%A5%E9%BB%9E" class="mw-redirect" title="近日點">近日點</a> ≈ 7013418874037960000♠280 AU， <a href="/wiki/%E9%81%A0%E6%97%A5%E9%BB%9E" class="mw-redirect" title="遠日點">遠日點</a> ≈ 7014167549615184000♠1,120 AU）</li> <li><a href="/wiki/%E8%BB%8C%E9%81%93%E5%82%BE%E8%A7%92" title="軌道傾角">傾角</a>「i」 ≈ 對<a href="/wiki/%E9%BB%83%E9%81%93" class="mw-redirect" title="黃道">黃道</a>傾角30°</li> <li><a href="/wiki/%E5%8D%87%E4%BA%A4%E9%BB%9E%E9%BB%83%E7%B6%93" title="升交點黃經">升交點黃經</a>「Ω」 ≈ 7000174532925199433♠100°.<a href="#cite_note-74">[G]</a></li> <li><a href="/wiki/%E8%BF%91%E5%BF%83%E9%BB%9E%E5%B9%85%E8%A7%92" title="近心點幅角">近心點幅角</a>「ω」 ≈ 140° 和<a href="/wiki/%E8%BF%91%E5%BF%83%E9%BB%9E%E7%B6%93%E5%BA%A6" title="近心點經度">近心點經度</a>「ω」= 7000418879020478640♠240°<a href="#cite_note-P9_where_are_you_P1-75">[68]</a>。</li></ul> 第九行星的這些參數對海王星外天體產生了不同的模擬效果。半長軸大於250天文單位的天體與第九行星強烈反對齊，近日點與第九行星的近日點相對。半長軸在150 AU到250 天文單位之間的天體與第九行星弱對齊，近日點與第九行星的近日點方向相同。半長軸小於150天文單位的天體幾乎沒有受到影響<a href="#cite_note-bnb20160617-10">[9]</a>。模擬還顯示，半長軸大於7013373994676750000♠250 AU，如果它們的偏心度較低，就可以有穩定、對齊的軌道。這些天體尚待觀察<a href="#cite_note-TAJ201601-5">[4]</a>。 還研究了第九行星的其它可能軌道，其半長軸在7013598391482800000♠400 AU和7014224396806050000♠1500 AU之間，離心率高達0.8，軌道傾角範圍很廣。這些軌道產生了不同的結果。巴蒂金和布朗發現，如果第九行星有更高的傾角，極端海王星外天體的軌道更有可能有類似的傾角，但反對齊也會减少<a href="#cite_note-bnb20160617-10">[9]</a>。Becker等人的模擬表明，如果第九行星的離心率較小，它們的軌道會更穩定，但在離心率較高的情况下，反對齊的可能性更大<a href="#cite_note-Becker_etal_2017-76">[69]</a>。勞勒等人發現，如果第九行星的軌道是圓形的，那麼與第九行星發生軌道共振時捕獲的天體會更小，到達高傾角軌道的天體也會更少<a href="#cite_note-Lawler_etal_2016-77">[70]</a>。Cáceres等人的研究表明，如果第九行星的近日點軌道較低，極端海王星外天體的軌道會更好地對齊，但其近日點需要高於90 AU<a href="#cite_note-Caceres_etal_2018-78">[71]</a>。巴蒂金等人後來的研究發現，更高的離心率軌道降低了極端海王星外天體軌道的平均傾斜<a href="#cite_note-P9H2019-2">[2]</a>。雖然第九行星的軌道參數和質量有很多可能的組合，但沒有一種替代模擬能更好地預測觀測到的原始極端海王星外天體的排列。更多遙遠太陽系天體的發現將使天文學家能够對這顆假設行星的軌道做出更準確的預測。這些也可能為第九行星假說提供進一步的支持或反駁<a href="#cite_note-discoveryDeBrief-79">[72]</a><a href="#cite_note-thestarKateAllen-80">[73]</a>。 包括巨行星遷移在內的模擬導致極端海王星外天體軌道的排列較弱<a href="#cite_note-Nesvorny_etal_2017-57">[54]</a>。對齊的方向也發生了變化，隨著半長軸的增加，從更對齊變為反對齊，隨著近日點距離的增加，也從反對齊變為對齊。後者將導致螺線管的軌道與大多數其它極端海王星外天體相反<a href="#cite_note-Kaib_etal_2019-56">[53]</a>。 <div class="mw-heading mw-heading4"><h4 id="動力學：第九行星如何改變極端海王星外天體的軌道"><span id=".E5.8B.95.E5.8A.9B.E5.AD.B8.EF.BC.9A.E7.AC.AC.E4.B9.9D.E8.A1.8C.E6.98.9F.E5.A6.82.E4.BD.95.E6.94.B9.E8.AE.8A.E6.A5.B5.E7.AB.AF.E6.B5.B7.E7.8E.8B.E6.98.9F.E5.A4.96.E5.A4.A9.E9.AB.94.E7.9A.84.E8.BB.8C.E9.81.93">動力學：第九行星如何改變極端海王星外天體的軌道</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=9" title="编辑章节：動力學：第九行星如何改變極端海王星外天體的軌道">编辑</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png" class="mw-file-description"><img alt="對齊的軌道在抛物線黑線的兩側顯示為紅色輪廓線，而反對齊的軌道則在抛物線內顯示為藍色輪廓線。" src="//upload.wikimedia.org/wikipedia/commons/thumb/8/81/Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png/260px-Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png" decoding="async" width="260" height="196" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/8/81/Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png/390px-Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/8/81/Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png/520px-Secular_evolution_of_eTNOs_induced_by_Planet_Nine.png 2x" data-file-width="814" data-file-height="614" /></a><figcaption>第九行星對半長軸為250天文單位的極端海王星外天體誘導的長期演化<a href="#cite_note-Beust_2016-81">[74]</a><a href="#cite_note-Batygin_Morbidelli_2017-82">[75]</a>。藍色：反對齊排列，紅色：對齊排列，綠色：亞穩的，橙色：迴圈的。黑線上方的是交叉軌道<a href="#cite_note-83">[H]</a></figcaption></figure> <link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r85100532" /><div role="note" class="hatnote navigation-not-searchable">主条目：<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F%E5%B0%8D%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94%E7%9A%84%E5%BD%B1%E9%9F%BF&action=edit&redlink=1" class="new" title="第九行星對海王星外天體的影響（页面不存在）">第九行星對海王星外天體的影響</a></div> 第九行星通過一系列效應改變了極端海王星外天體的軌道。在很長的時間尺度上，第九行星對極端海王星外天體的軌道施加<a href="/wiki/%E5%8A%9B%E7%9F%A9" title="力矩">力矩</a>，該力矩隨其軌道與第九行星的對齊而變化。由此產生的<a href="/wiki/%E8%A7%92%E5%8B%95%E9%87%8F" class="mw-redirect" title="角動量">角動量</a>交換導致近日點上升，將它們置於類似塞德納的軌道上，然後下降，在數億年後使它們回到原來的軌道。當它們的離心率很小時，它們的近日點方向的運動也會反轉，使物體保持反對齊，見圖上的藍色曲線，或對齊的紅色曲線。在較短的時間尺度上，與第九行星的運動共振提供了相位保護，通過略微改變天體的半長軸來穩定它們的軌道，使它們的軌道與第九行星同步，並防止近距離接近。海王星和其他巨行星的引力，以及第九行星軌道的傾斜，減弱了這種保護。這導致了天體在共振之間跳躍時，半長軸的<a href="/wiki/%E6%B7%B7%E6%B2%8C%E7%90%86%E8%AB%96" class="mw-redirect" title="混沌理論">混沌</a>變化，包括百萬年時間尺度上的高階共振，如27:17<a href="#cite_note-Batygin_Morbidelli_2017-82">[75]</a>。如果極端海王星外天體和第九行星都在傾斜軌道上，那麼平均運動共振對於它們的生存可能不是必要的<a href="#cite_note-Li_etal_2018-84">[76]</a>。天體的軌道極點圍繞太陽系<a href="/w/index.php?title=%E6%8B%89%E6%99%AE%E6%8B%89%E6%96%AF%E5%B9%B3%E9%9D%A2&action=edit&redlink=1" class="new" title="拉普拉斯平面（页面不存在）">拉普拉斯平面</a>（英语：<a href="https://en.wikipedia.org/wiki/Laplace_plane" class="extiw" title="en:Laplace plane">Laplace plane</a>）的極點進動。在大的半長軸上，拉普拉斯平面向第九行星軌道的平面彎曲。這導致極端海王星外天體的軌道極點平均向一側傾斜，並且使其升交點的經度群集<a href="#cite_note-Batygin_Morbidelli_2017-82">[75]</a>。 <div class="mw-heading mw-heading4"><h4 id="具有大半長軸的垂直軌道中的天體">具有大半長軸的垂直軌道中的天體</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=10" title="编辑章节：具有大半長軸的垂直軌道中的天體">编辑</a>]</div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/File:Planet_nine_TNO_orbits.svg" class="mw-file-description"><img alt="第九行星的軌道指向頂部，而群集的彗星則指向底部。" src="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Planet_nine_TNO_orbits.svg/330px-Planet_nine_TNO_orbits.svg.png" decoding="async" width="330" height="186" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/77/Planet_nine_TNO_orbits.svg/495px-Planet_nine_TNO_orbits.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/77/Planet_nine_TNO_orbits.svg/660px-Planet_nine_TNO_orbits.svg.png 2x" data-file-width="512" data-file-height="288" /></a><figcaption>其中五顆軌道高度傾斜（幾乎垂直於黃道）天體的軌道在這裡顯示為青色橢圓，假設的第九行星為橙色。</figcaption></figure> 第九行星可以將極端海王星外天體送入大致垂直於黃道的軌道<a href="#cite_note-extremeTech-85">[77]</a><a href="#cite_note-Siegel-86">[78]</a>。已經觀測到幾個傾角大於50°、半長軸大於250 AU的天體<a href="#cite_note-mpc-6-87">[79]</a>。當一些低傾角的極端海王星外天體在到達低離心率軌道時與第九行星形成<a href="/wiki/%E9%95%B7%E6%9C%9F%E5%85%B1%E6%8C%AF" title="長期共振">長期共振</a>時，就會產生這些軌道。共振導致它們的離心率和傾角增加，將極端海王星外天體輸送到具有低近日點的垂直軌道上，在那裡它們更容易被觀測到。然後，極端海王星外天體演變成具有較低離心率的<a href="/wiki/%E9%A0%86%E8%A1%8C%E5%92%8C%E9%80%86%E8%A1%8C" title="順行和逆行">逆行</a>軌道，之後它們經過第二階段的高離心率垂直軌道，然後返回低離心率和傾斜軌道。與第九行星的長期共振涉及軌道參數和近日點經度的<a href="/wiki/%E7%B7%9A%E6%80%A7%E7%B5%84%E5%90%88" class="mw-redirect" title="線性組合">線性組合</a>：Δϖ – 2ω。與谷在機制不同，這種共振導致物體在幾乎垂直的軌道上達到最大離心率。在巴蒂金和莫比德利進行的模擬中，這種進化相對常見，38%的穩定物體至少經歷過一次<a href="#cite_note-Batygin_Morbidelli_2017-82">[75]</a>。當它們到達低近日點時，這些天體的近日點論點群集在第九行星的附近或對面，它們的昇交點經度群集在距離第九行星任一方向90°左右<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-Li_etal_2018-84">[76]</a>。這與觀測結果大致一致，這些觀測結果的差異歸因於與已知巨行星的遙遠相遇<a href="#cite_note-TAJ201601-5">[4]</a>。 <div class="mw-heading mw-heading4"><h4 id="高傾角天體的軌道">高傾角天體的軌道</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=11" title="编辑章节：高傾角天體的軌道">编辑</a>]</div> 半長軸小於100天文單位的高傾角極端海王星外天體族群可能是由第九行星和其它巨行星的共同作用產生的。進入垂直軌道的極端海王星外天體的近日點足够小，其軌道可以與海王星或其他巨行星的軌道相交。與其中一顆行星的相遇可以將極端海王星外天體的半長軸降低到100 AU以下，在那裡，物體的軌道不再由第九行星控制，使其軌道類似<a href="/w/index.php?title=2008_KV42&action=edit&redlink=1" class="new" title="2008 KV42（页面不存在）">2008 KV42</a>。預測這些天體中壽命最長的天體軌道分佈是不均勻的。大多數軌道的近日點在5 AU到35 AU之間，傾角在110°以下；在一個幾乎沒有天體的間隙之外，將是其它傾斜度接近150°和近10 AU的物體<a href="#cite_note-Batygin_Brown_high_inc-30">[29]</a>。以前有人提出這些物體起源於<a href="/wiki/%E6%AD%90%E7%89%B9%E9%9B%B2" class="mw-redirect" title="歐特雲">歐特雲</a><a href="#cite_note-Brasser_etal_2012-88">[80]</a>。歐特雲是理論上在2,000到200,000天文單位的距離上圍繞太陽的冰星子<a href="#cite_note-Williams_OortCloud-89">[81]</a>。然而，在沒有第九行星的模擬中，歐特雲產生的數量與觀測結果相比不足<a href="#cite_note-Kaib_etal_2019-56">[53]</a>。一些高傾角的海王星外天體可能會變成<a href="/w/index.php?title=514107_Ka%C3%AFepaoka%C3%AFawela&action=edit&redlink=1" class="new" title="514107 Kaïepaokaïawela（页面不存在）">逆行的木星特洛伊</a> <a href="#cite_note-Kohne_Batygin_2020-90">[82]</a>。 <div class="mw-heading mw-heading4"><h4 id="歐特雲和彗星">歐特雲和彗星</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=12" title="编辑章节：歐特雲和彗星">编辑</a>]</div> 第九行星將改變彗星的來源區和傾角分佈。在<a href="/wiki/%E5%B0%BC%E6%96%AF%E6%A8%A1%E5%9E%8B" title="尼斯模型">尼斯模型</a>描述的巨行星遷移的模擬中，當包括第九行星時，<a href="/wiki/%E6%AD%90%E7%89%B9%E9%9B%B2" class="mw-redirect" title="歐特雲">歐特雲</a>中捕獲的物體較少。其它天體將被捕獲在由第九行星動態控制的天體雲中。這顆第九行星雲由極端海王星外天體和垂直天體組成，將天體的半長軸範圍,從200天文單位延伸到3000天文單位，並包含大約0.3-0.4個地球質量<a href="#cite_note-Nesvorny_etal_2017-57">[54]</a><a href="#cite_note-Lawler_etal_2016-77">[70]</a>。當第九行星雲中天體的近日點下降到足以與其它的行星相遇時，一些天體會分散到進入太陽系內部的軌道上，在那裡它們可以成為彗星被觀測到。如果第九行星存在，將大約佔<a href="/wiki/%E5%BD%97%E6%98%9F#短週期" title="彗星">哈雷型彗星</a>數量的三分之一。與第九行星的相互作用也會增加穿過其軌道的離散盤天體的軌道傾角<a href="#cite_note-Kaib_etal_2019-56">[53]</a>。<a href="/wiki/%E5%BD%97%E6%98%9F#短週期" title="彗星">木星族彗星</a>也比觀測到的具有更廣泛的傾角分佈<a href="#cite_note-Nesvorny_etal_2017-57">[54]</a><a href="#cite_note-Gibbs_IEEE-91">[83]</a>。最近對第九行星較小質量和離心率的估計將減少其對這些傾角的影響<a href="#cite_note-P9H2019-2">[2]</a>。 <div class="mw-heading mw-heading4"><h4 id="2019年估計">2019年估計</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=13" title="编辑章节：2019年估計">编辑</a>]</div> 2019年2月，符合半長軸超過250天文單位的原始假設的極端海王星外天體總數已增加到14個<a href="#cite_note-P9H2019-2">[2]</a>： <ul><li>半長軸400–500 AU;</li> <li>軌道離心率 0.15–0.3;</li> <li>軌道傾角〜 20°;</li> <li>質量約為地球質量的5倍。</li></ul> <div class="mw-heading mw-heading4"><h4 id="2021年估計">2021年估計</h4>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=14" title="编辑章节：2021年估計">编辑</a>]</div> 2021年8月，巴蒂金和布朗重新分析了與極端海王星外天體觀測相關的數據，同時考慮了觀測偏差，他們發現在某些方向上觀測的可能性比其他方向更大。他們表示，觀察到的軌道群集「在99.6%的置信水準下仍然很重要」<a href="#cite_note-Batygin2021-4">[3]</a>。將觀測偏差與數值模擬相結合，他們預測了第九行星的特徵<a href="#cite_note-Batygin2021-4">[3]</a>： <ul><li>半長軸380+140 −80 AU（300–520 AU）;</li> <li>近日點300+85 −60 AU (240–385 AU);</li> <li>軌道傾角 16+5 −° (11°–21°);</li> <li>質量6.2+2.2 −1.3地球質量（8.4M⊕–4.9M⊕）。</li></ul> <div class="mw-heading mw-heading3"><h3 id="接受度">接受度</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=15" title="编辑章节：接受度">编辑</a>]</div> 巴蒂金在解釋為他和布朗的研究文章開發的模擬結果時很謹慎，他說：「在第九行星被相機捕捉到之前，它不算是真實的。我們現在所擁有的只是一個回聲。」<a href="#cite_note-TomLevensonAtlantic-92">[84]</a>。2016年，布朗認為第九行星存在的幾率約為90%<a href="#cite_note-lurking-39">[36]</a>。<a href="/w/index.php?title=%E6%A0%BC%E9%9B%B7%E6%88%88%E9%87%8C%C2%B7%E5%8B%9E%E5%85%8B%E6%9E%97&action=edit&redlink=1" class="new" title="格雷戈里·勞克林（页面不存在）">格雷戈里·勞克林</a>（英语：<a href="https://en.wikipedia.org/wiki/Greg_Laughlin" class="extiw" title="en:Greg Laughlin">Greg Laughlin</a>）是為數不多的提前知道這篇文章的研究人員之一，他給出了68.3%的估計<a href="#cite_note-fatty-7">[6]</a>。其他持懷疑態度的科學家需要更多的數據來分析額外的古柏帶天體或通過照片確認的最終證據<a href="#cite_note-vergeSlamDunkandWaterTightEvidence-93">[85]</a><a href="#cite_note-thestarKateAllen-80">[73]</a><a href="#cite_note-scantEvidence-94">[86]</a>。布朗，雖然承認懷疑論者的觀點，但仍然認為有足夠的數據來尋找新行星<a href="#cite_note-pbsBrown-95">[87]</a>。 第九行星假說得到了幾位天文學家和學者的支援。2016年1月，美國國家航空暨太空總署科學任務局局長<a href="/w/index.php?title=%E5%90%89%E5%A7%86%C2%B7%E6%A0%BC%E6%9E%97&action=edit&redlink=1" class="new" title="吉姆·格林（页面不存在）">吉姆·格林</a>（英语：<a href="https://en.wikipedia.org/wiki/James_L._Green" class="extiw" title="en:James L. Green">James L. Green</a>）說：「現在的證據比以前更有力。」<a href="#cite_note-popsci-96">[88]</a>。但格林也警告說，對於觀測到遙遠的極端海王星外天體的運動，還有其它可能的解釋，並引用<a href="/wiki/%E5%8D%A1%E5%B0%94%C2%B7%E8%90%A8%E6%A0%B9" title="卡尔·萨根">卡爾·薩根</a>的話說：「非比尋常的索賠需要非比尋常的證據。」<a href="#cite_note-lurking-39">[36]</a>。<a href="/wiki/%E9%BA%BB%E7%9C%81%E7%90%86%E5%B7%A5%E5%AD%B8%E9%99%A2" class="mw-redirect" title="麻省理工學院">麻省理工學院</a>教授<a href="/w/index.php?title=%E6%B9%AF%E7%91%AA%E6%96%AF%C2%B7%E8%90%8A%E6%96%87%E6%A3%AE&action=edit&redlink=1" class="new" title="湯瑪斯·萊文森（页面不存在）">湯瑪斯·萊文森</a>（英语：<a href="https://en.wikipedia.org/wiki/Tom_Levenson" class="extiw" title="en:Tom Levenson">Tom Levenson</a>）得出結論，就目前而言，第九行星似乎是目前已知的關於太陽系外圍區域唯一能令多數人滿意的解釋<a href="#cite_note-TomLevensonAtlantic-92">[84]</a>。天文學家<a href="/w/index.php?title=%E4%BA%9E%E6%AD%B7%E5%B1%B1%E5%BE%B7%E7%BE%85%C2%B7%E8%8E%AB%E6%AF%94%E5%BE%B7%E5%88%A9_(%E5%A4%A9%E6%96%87%E5%AD%B8%E5%AE%B6)&action=edit&redlink=1" class="new" title="亞歷山德羅·莫比德利 (天文學家)（页面不存在）">亞歷山德羅·莫比德利 (天文學家)</a>（英语：<a href="https://en.wikipedia.org/wiki/Alessandro_Morbidelli" class="extiw" title="en:Alessandro Morbidelli">Alessandro Morbidelli</a>）在《天文學雜誌》（The Astronomical Journal）上評論了這篇研究文章，他對此表示贊同，他說：「我看不出巴蒂金和布朗還能提任何其它的解釋。」<a href="#cite_note-fatty-7">[6]</a><a href="#cite_note-lurking-39">[36]</a>。 天文學家雷努·瑪律霍特拉（Renu Malhotra）仍然對第九行星無所知，但她指出，她和她的同事們發現，極端海王星外天體的軌道似乎以一種難以解釋的方式傾斜。她說：「我們看到的翹曲量簡直太瘋狂了，對我來說，這是迄今為止我遇到的關於第九行星最有趣的證據。」<a href="#cite_note-sciamGiantGhost-97">[89]</a>。 其他專家則持不同程度的懷疑態度。美國天體物理學家伊桑·西格爾（Ethan Siegel）此前曾推測行星可能是在早期動力學不穩定期間從太陽系中噴射出來的，他對太陽系中是否存在未被發現的行星持懷疑態度<a href="#cite_note-Siegel-86">[78]</a><a href="#cite_note-Siegel_2015-98">[90]</a>。在2018年的一篇文章中，他討論了一項沒有發現極端海王星外天體軌道群集證據的調查，他認為先前觀察到的群集可能是觀測偏差的結果，並聲稱大多數科學家認為第九行星不存在<a href="#cite_note-Siegel_2018a-99">[91]</a>。行星科學家<a href="/w/index.php?title=%E5%93%88%E7%88%BE%C2%B7%E8%90%8A%E7%B6%AD%E6%A3%AE&action=edit&redlink=1" class="new" title="哈爾·萊維森（页面不存在）">哈爾·萊維森</a>（英语：<a href="https://en.wikipedia.org/wiki/Harold_F._Levison" class="extiw" title="en:Harold F. Levison">Harold F. Levison</a>）認為，拋射出的天體最終進入歐特雲內部的幾率只有2%左右，並推測如果一個天體進入了穩定的軌道，那麼許多天體一定已經被拋過了歐特雲<a href="#cite_note-skyntelescopePlanetX-100">[92]</a>。 2020年，根據<a href="/w/index.php?title=%E5%A4%96%E5%A4%AA%E9%99%BD%E7%B3%BB%E8%B5%B7%E6%BA%90%E8%AA%BF%E6%9F%A5&action=edit&redlink=1" class="new" title="外太陽系起源調查（页面不存在）">外太陽系起源調查</a>（英语：<a href="https://en.wikipedia.org/wiki/Outer_Solar_System_Origins_Survey" class="extiw" title="en:Outer Solar System Origins Survey">Outer Solar System Origins Survey</a>）和<a href="/wiki/%E6%9A%97%E8%83%BD%E9%87%8F%E5%B7%A1%E5%A4%A9" title="暗能量巡天">暗能量巡天</a>的結果，對第九行星假說產生了進一步的懷疑，OSSOS記錄了800多個跨海王星天體，暗能量調查發現了316個新天體<a href="#cite_note-Bernardinelli_2020a-101">[93]</a>。這兩項調查都調整了觀測偏差，並得出結論：在觀察到的物體中，沒有群集的證據<a href="#cite_note-Lawler2020-102">[94]</a>。作者進一步解釋說，幾乎所有天體的軌道都可以用物理現象來解釋，而不是像布朗和巴蒂金所提出的第九顆行星那樣<a href="#cite_note-Lawler2021-103">[95]</a>。其中一項研究的作者薩曼莎·勞勒（Samantha Lawler）表示，布朗和巴蒂金提出的第九行星假說「經不起詳細的觀察」，指出800個天體的樣本相較於少得多的14個樣本，量要大得多，而基於上述天體的結論性研究「為時過早」。她進一步解釋說，這些極端軌道的現象可能是由於海王星在太陽系歷史早期向外遷移時的引力掩星造成的<a href="#cite_note-Universetoday_2020-104">[96]</a>。 <div class="mw-heading mw-heading2"><h2 id="備選假說">備選假說</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=16" title="编辑章节：備選假說">编辑</a>]</div> <div class="mw-heading mw-heading3"><h3 id="臨時或巧合的群集">臨時或巧合的群集</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=17" title="编辑章节：臨時或巧合的群集">编辑</a>]</div> 外太陽系調查（OSSOS）的結果表明，觀測到的群集是觀測偏差和小數統計相結合的結果。OSSOS是對具有已知偏差的外太陽系的良好特徵調查，觀測到八顆半長軸大於150天文單位的天體，其軌道方向很寬廣。在考慮了調查的觀測偏差後，沒有看到和Sheppard確定的近日點（ω）群集論點的證據，<a href="#cite_note-106">[I]</a>半長軸最大的天體的軌道方向在統計學上與隨機性一致<a href="#cite_note-Shankman_etal_2017-105">[97]</a><a href="#cite_note-Siegel_2018b-107">[98]</a>。佩德羅·伯納迪內利（Pedro Bernardinelli）和他的同事們還發現，暗能量巡天發現的極端海王星外天體的軌道元素沒有顯示出群集的證據。然而，他們也指出，天空覆蓋率和發現的天體數量不足以表明沒有第九行星<a href="#cite_note-Ratner_2020-108">[99]</a><a href="#cite_note-Bernardelli_2020b-109">[100]</a>。當這兩項調查與特魯希略和謝潑德的調查相結合時，也發現了類似的結果<a href="#cite_note-Napier_etal_2021-110">[101]</a>。這些結果與邁克·布朗對先前觀察到的極端海王星外天體中發現偏差的分析不同。他發現，在考慮了觀測偏差之後，如果10個已知極端海王星外天體的實際分佈均勻，則只有1.2%的時間可以觀察到近日點經度的群集。當與觀察到的近日點參數群集的幾率相結合時，概率為0.025%<a href="#cite_note-Brown_discovery_biases-111">[102]</a>。布朗和巴蒂金後來對14個極端海王星外天體的發現偏差進行了分析，確定觀測到的近日點經度和軌道極點位置群集的概率為0.2%<a href="#cite_note-Brown_Batygin_2019-112">[103]</a>。 對在第九行星影響下演化的15個已知天體的模擬也揭示了與觀測結果的差異。科里·尚克曼（Cory Shankman）和他的同事們將第九行星納入了對15個半長軸大於150天文單位、近日點大於30天文單位的天體的許多複製（具有相似軌道的天體）的模擬中<a href="#cite_note-113">[J]</a>。雖然他們觀察到半長軸大於250天文單位的天體軌道與第九行星相反的軌道對齊，但沒有看到近日點論點的群集。他們的模擬還表明，極端海王星外天體的近日點上升和下降是平穩的，使許多極端海王星外天體的近日點距離在50 AU和70 AU之間，而這些天體沒有被觀測到，並預測還會有許多其它未觀測到的天體<a href="#cite_note-Shankman_etal_2016_10-114">[104]</a>。其中包括一個大型高傾角天體，由於大多數觀測結果都是小傾角，這些天體會被遺漏<a href="#cite_note-Lawler_etal_2016-77">[70]</a>，以及大量近日點是如此遙遠的天體，以至於它們太微弱而無法觀察到。許多天體在遇到其它巨行星後也能被驅逐出太陽系。大量未觀測到的種群和許多天體的丟失導致尚克曼等人估計原始種群的質量是地球質量的數十倍，這就要求在太陽系早期噴出更大的質量<a href="#cite_note-115">[K]</a>。尚克曼等人得出結論，第九行星的存在不太可能，目前觀察到的現有極端海王星外天體的排列是一種暫時現象，隨著更多天體被探測到，這種現象將消失<a href="#cite_note-sciamGiantGhost-97">[89]</a><a href="#cite_note-Shankman_etal_2016_10-114">[104]</a>。 <div class="mw-heading mw-heading3"><h3 id="大容量圓盤中的傾斜不穩定性">大容量圓盤中的傾斜不穩定性</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=18" title="编辑章节：大容量圓盤中的傾斜不穩定性">编辑</a>]</div> 安-瑪麗·馬迪根（Ann-Marie Madigan）和邁克爾·麥考特（Michael McCourt）假設，在遙遠的大質量帶（假設稱為Zderic-Madigan或ZM帶）中，<a href="/w/index.php?title=%E5%82%BE%E8%A7%92%E4%B8%8D%E7%A9%A9%E5%AE%9A%E6%80%A7&action=edit&redlink=1" class="new" title="傾角不穩定性（页面不存在）">傾角不穩定性</a>（英语：<a href="https://en.wikipedia.org/wiki/Inclination_instability" class="extiw" title="en:Inclination instability">Inclination instability</a>）負責極端海王星外天體近日點論點的對齊<a href="#cite_note-Madigan_McCourt_2016-116">[105]</a>。在這種具有高離心率軌道的粒子盤中可能發生傾角不穩定性（<a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">e</a> > 0.6）圍繞一個中心天體，如太陽。這個圓盤的自重力會導致它的自發組織，增加物體的傾斜度並對齊近日點的論點，將其形成一個在原始平面上方或下方的圓錐體<a href="#cite_note-Madigan_etal_2018-117">[106]</a>。這個過程需要更長的時間和足夠大的圓盤質量，大約需要十億年的時間，1-10 地球質量盤<a href="#cite_note-Madigan_McCourt_2016-116">[105]</a>。安-瑪麗·馬迪根認為，一些已經發現的海王星外天體，如<a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F90377" class="mw-redirect" title="小行星90377">90377 塞德納</a>和<a href="/wiki/2012_VP113" title="2012 VP113">2012 VP113</a>可能是這個圓盤的成員<a href="#cite_note-:0-118">[107]</a>。如果是這樣的話，該地區可能會有數千個類似的天體<a href="#cite_note-:0-118">[107]</a>。邁克·布朗（Mike Brown）認為第九行星是一個更可能的解釋，並指出目前的調查還沒有揭示出足夠大的離散盤來產生「傾角不穩定性」<a href="#cite_note-spaceplanet9-119">[108]</a><a href="#cite_note-planet9ornot-120">[109]</a>。在包括小行星盤自重力在內的太陽系尼斯模型模擬中，沒有發生傾角不穩定。取而代之的是，模擬產生了物體軌道的快速進動，並且大多數天體在太短的時間尺度上被拋射出來，以至於發生了傾角不穩定<a href="#cite_note-Fan_Batygin_2017-121">[110]</a>。2020年，馬迪根及其同事表明，傾角不穩定性需要20地球質量存在於一個半長軸為幾百天文單位的天體盤中<a href="#cite_note-Skibba2020-122">[111]</a>。該圓盤中的傾角不穩定性也可以再現極端海王星外天體的近日點距離中觀察到的間隙<a href="#cite_note-Zderic_etal_2020-123">[112]</a>，以及在給定足夠時間的傾斜不穩定性後觀察到的近端排列<a href="#cite_note-Zderic_Madigan_2020-124">[113]</a><a href="#cite_note-Zedric_etal_2021-125">[114]</a>。截至2022年的模擬表明，<a href="/wiki/%E8%96%87%E6%8B%89%C2%B7%E9%AD%AF%E8%B3%93%E5%A4%A9%E6%96%87%E5%8F%B0" title="薇拉·魯賓天文台">薇拉·魯賓天文台</a>的時空遺產調查（LSST，Legacy Survey of Space and Time）專案在2024年開始數據收集時，應該能夠提供支援或反對 ZM 帶的有力證據<a href="#cite_note-:0-118">[107]</a>。 <div class="mw-heading mw-heading3"><h3 id="由一個巨大的圓盤牧養">由一個巨大的圓盤牧養</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=19" title="编辑章节：由一個巨大的圓盤牧養">编辑</a>]</div> 安特拉尼克·塞菲利安（Antranik Sefilian）和吉哈德·圖馬（Jihad Touma）提出，中等離心率海王星外天體的大質量圓盤是極端海王星外天體經度聚集的原因。這個圓盤將包含10個地球質量的海王星外天體，它們的軌道對齊，半長軸隨著它們的離心率從零到0.165的增加而增加。圓盤的引力效應將抵消巨行星驅動的向前進動，從而保持其單個物體的軌道方向。具有高離心率天體的軌道，例如觀測到的極端海王星外天體，如果它們的軌道與這個圓盤反對齊，則具有大致固定的方位或近日點經度，將是穩定的<a href="#cite_note-Seilian_Touma_2019-126">[115]</a>。儘管布朗認為所提出的圓盤可以解釋觀測到的極端海王星外天體的聚集，但他發現圓盤能够存活在太陽系的整個年齡中是不可能的<a href="#cite_note-Patel_2019-127">[116]</a>。巴蒂金認為古柏帶的質量不足以解釋圓盤的形成，並問道：「為什麼原行星盤會在30天文單位附近結束，並在100天文單位以上重新開始<a href="#cite_note-Dvorsky_2019-128">[117]</a>？」 <div class="mw-heading mw-heading3"><h3 id="處於較低離心率軌道的行星">處於較低離心率軌道的行星</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=20" title="编辑章节：處於較低離心率軌道的行星">编辑</a>]</div> <table class="wikitable sortable" style="text-align:center; float:right;"> <caption>建議的諧振對象 <a href="/wiki/%E5%8D%8A%E9%95%B7%E8%BB%B8" title="半長軸">a</a> > 150 AU, <a href="/wiki/%E8%BF%91%E6%97%A5%E9%BB%9E" class="mw-redirect" title="近日點">q</a> > 40 AU<a href="#cite_note-Malhotra_Volk_Wang-129">[118]</a> </caption> <tbody><tr> <th>天體</th> <th><a href="/wiki/%E8%BD%A8%E9%81%93%E5%91%A8%E6%9C%9F" title="轨道周期">質心週期</a> （年）</th> <th>比率 </th></tr> <tr> <td><a href="/w/index.php?title=2013_GP136&action=edit&redlink=1" class="new" title="2013 GP136（页面不存在）">2013 GP136</a></td> <td>1,830</td> <td>9:1 </td></tr> <tr> <td><a href="/wiki/2000_CR105" class="mw-redirect" title="2000 CR105">2000 CR105</a></td> <td>3,304</td> <td>5:1 </td></tr> <tr> <td><a href="/wiki/2012_VP113" title="2012 VP113">2012 VP113</a></td> <td>4,300</td> <td>4:1 </td></tr> <tr> <td><a href="/w/index.php?title=%E5%B0%8F%E8%A1%8C%E6%98%9F474640&action=edit&redlink=1" class="new" title="小行星474640（页面不存在）">474640 Alicanto</a></td> <td>5,900</td> <td>3:1 </td></tr> <tr> <td><a href="/w/index.php?title=2010_GB174&action=edit&redlink=1" class="new" title="2010 GB174（页面不存在）">2010 GB174</a></td> <td>6,500</td> <td>5:2 </td></tr> <tr> <td><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F90377" class="mw-redirect" title="小行星90377">賽德娜</a></td> <td>≈ 11,400</td> <td>3:2 </td></tr> <tr> <th>假想的行星</th> <th>≈ 17,000</th> <th>1:1（根據定義） </th></tr></tbody></table> 第九行星假說包括一組關於行星質量和軌道的預測。另一種假設是預測一顆具有不同軌道參數的行星。雷努·馬爾霍特拉（Renu Malhotra）、凱瑟琳·沃爾克（Kathryn Volk）和王向育（Xianyu Wang）提出，軌道週期最長的四個獨立天體，即近日點距離超過7012598391482800000♠40 AU，和半長軸大於 7013373994676750000♠250 AU，與一顆假設行星的平均運動共振為「n」：1或「n」：2。其它兩顆半長軸大於7013224396806050000♠150 AU的天體，也有可能與這顆行星產生共振。他們提出的行星可能位於離心率較低、低傾角的軌道上，<a href="/wiki/%E8%BB%8C%E9%81%93%E9%9B%A2%E5%BF%83%E7%8E%87" title="軌道離心率">離心率（e）</a>  < 0.18和<a href="/wiki/%E8%BB%8C%E9%81%93%E5%82%BE%E8%A7%92" title="軌道傾角">傾角（i）</a> ≈ 11°。在這種情況下，要求離心率受到避免2010 GB174接近行星的限制。如果極端海王星外天體處於第三類週期軌道<a href="#cite_note-131">[L]</a>，由於它們的近日點論點的平動增强了它們的穩定性，這顆行星可能處於更高傾角的軌道上，具有<a href="/wiki/%E8%BB%8C%E9%81%93%E5%82%BE%E8%A7%92" title="軌道傾角">i</a> ≈ 48°。不同於巴蒂金和布朗，馬爾霍特拉、沃爾克和王沒有具體說明大多數遙遠的獨立天體的軌道會與這顆大質量行星反對齊<a href="#cite_note-Malhotra_Volk_Wang-129">[118]</a><a href="#cite_note-Malhotra_TED_2017-132">[120]</a>。 <div class="mw-heading mw-heading3"><h3 id="古在機制導致的對齊">古在機制導致的對齊</h3>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=21" title="编辑章节：古在機制導致的對齊">编辑</a>]</div> 特魯希略和謝潑德在2014年認為，一顆位於圓形軌道上的大質量行星的平均距離為7013299195741400000♠200 AU和7013448793612100000♠300 AU負責12顆具有大的半長軸的海王星外天體的近日點論點的聚集。特魯希略和謝潑德確定了12顆海王星外天體軌道的近日點論點接近零度的聚集，其中近日點大於7012448793612100000♠30 AU和半長軸大於7013224396806050000♠150 AU<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-Sheppard2014-6">[5]</a>。之後的數值模擬表明，近日點的論點應該以不同的速度流通，使其在數十億年後隨機化，他們提出，一顆位於數百天文單位圓形軌道上的大質量行星是造成這種聚集的原因<a href="#cite_note-Sheppard2014-6">[5]</a><a href="#cite_note-sciencenews-133">[121]</a>。這顆大質量的行星將導致海王星外天體近日點的擺動大約在0°或180° 通過<a href="/wiki/%E5%8F%A4%E5%9C%A8%E6%A9%9F%E5%88%B6" title="古在機制">古在機制</a>，使它們的軌道在離行星最近和最遠的近日點和遠日點附近穿過行星軌道的平面<a href="#cite_note-Sheppard2014-6">[5]</a><a href="#cite_note-Marcos_2014-27">[26]</a>。在數值模擬中，包括圓形低傾角軌道上的2–15個地球質量體，7013299195741400000♠200 AU和7013448793612100000♠300 AU賽德娜和2012VP113的近旋面爭論在0°左右校準了數十億年（儘管沒有近日點較小的天體），並在1,500天文單位的高傾角軌道上與海王星質量天體一起經歷了一段時間的平衡<a href="#cite_note-Sheppard2014-6">[5]</a>。另一個過程，比如一顆經過的恆星，將被要求解釋180°附近沒有近日點論據的天體<a href="#cite_note-TAJ201601-5">[4]</a><a href="#cite_note-136">[M]</a> <div class="mw-heading mw-heading2"><h2 id="反響">反響</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=22" title="编辑章节：反響">编辑</a>]</div> 美國<a href="/w/index.php?title=%E5%A4%AA%E7%A9%BA%E7%B8%BD%E7%BD%B2%E8%A1%8C%E6%98%9F%E7%A7%91%E5%AD%B8%E9%83%A8&action=edit&redlink=1" class="new" title="太空總署行星科學部（页面不存在）">太空總署行星科學部</a>主任<a href="/w/index.php?title=%E5%90%89%E5%A7%86%C2%B7%E6%A0%BC%E6%9E%97&action=edit&redlink=1" class="new" title="吉姆·格林（页面不存在）">吉姆·格林</a>支持麥克·布朗的說法，他認為“現在的證據比之前更強”。但格林警告說，對遙遠<a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="海王星外天體">海王星外天體</a>觀察到的運動有其他的可能性，並引用<a href="/wiki/%E5%8D%A1%E5%B0%94%C2%B7%E8%90%A8%E6%A0%B9" title="卡尔·萨根">卡爾·薩根</a>的話「非凡的主張需要非凡的證據」。 湯姆·萊文森得出的結論是「就目前而言，第九行星似乎是現在所知道的太陽系外圍區域唯一令人滿意的解釋」。亞歷山德羅·莫爾比德利（Alessandro Morbidelli）評論《<a href="/wiki/%E5%A4%A9%E6%96%87%E6%9C%9F%E5%88%8A" title="天文期刊">天文期刊</a>》的研究文章時表示同意，他說「我看不到其他解釋可以取代貝提金和布朗所提出的」。 美國天體物理學家<a href="/wiki/%E4%BC%8A%E6%A3%AE%C2%B7%E8%A5%BF%E6%A0%BC%E7%88%BE" title="伊森·西格爾">伊森·西格爾</a>對太陽系中存在尚未發現的行星持懷疑態度，但他推測太陽系至少有一顆超級地球，這種星球在其他行星系統中很常見，但尚未在太陽系中被發現。超級地球在太陽系早期的動力不穩定期間可能已經從太陽系中彈出。行星科學家哈爾·萊維森（Hal Levison）認為被彈出太陽系的超級地球最終落入奧爾特雲的可能性僅為2％左右，並推測如果該星球進入穩定的軌道，許多物體必須被拋出奧爾特雲。 天文學家預計，第九行星的發現將有助於人類理解太陽系和其他行星系統形成的過程，了解太陽系的非比尋常——因為其缺乏位於地球與海王星質量之間的行星。 <div class="mw-heading mw-heading2"><h2 id="註解">註解</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=23" title="编辑章节：註解">编辑</a>]</div> <div class="reflist" style="list-style-type: upper-alpha;"> <ol class="references"> <li id="cite_note-3"><a href="#cite_ref-3">^</a> 據布朗和巴蒂金估計，截至2021年，第九行星的半長軸在360至620天文單位之間；這意味著這顆行星的軌道週期介於6,800（3601.5）至15,400（6201.5）年。 </li> <li id="cite_note-32"><a href="#cite_ref-32">^</a> 從400 AU延伸到1,000 AU的一系列半長軸在模擬中產生了觀察到的群集<a href="#cite_note-bnb20160617-10">[9]</a>。 </li> <li id="cite_note-34"><a href="#cite_ref-34">^</a> 《紐約客》將第九行星的平均軌道距離納入視角，顯然暗指該雜誌最著名的漫畫之一：「<a href="/w/index.php?title=%E5%BE%9E%E7%AC%AC%E4%B9%9D%E5%A4%A7%E9%81%93%E7%9C%8B%E4%B8%96%E7%95%8C&action=edit&redlink=1" class="new" title="從第九大道看世界（页面不存在）">從第九大道看世界</a>（英语：<a href="https://en.wikipedia.org/wiki/View_of_the_World_from_9th_Avenue" class="extiw" title="en:View of the World from 9th Avenue">View of the World from 9th Avenue</a>）」：「如果太陽在<a href="/wiki/%E7%AC%AC%E4%BA%94%E5%A4%A7%E9%81%93" title="第五大道">第五大道</a>，地球在西邊一個街區，木星將在<a href="/w/index.php?title=%E8%A5%BF%E9%82%8A%E9%AB%98%E9%80%9F%E5%85%AC%E8%B7%AF&action=edit&redlink=1" class="new" title="西邊高速公路（页面不存在）">西邊高速公路</a>上，冥王星將在<a href="/w/index.php?title=%E6%96%B0%E6%BE%A4%E8%A5%BF%E5%B7%9E%E8%92%99%E7%89%B9%E5%85%8B%E9%9B%B7%E7%88%BE&action=edit&redlink=1" class="new" title="新澤西州蒙特克雷爾（页面不存在）">新澤西州蒙特克雷爾</a>，而新行星將在<a href="/wiki/%E5%85%8B%E5%88%A9%E5%A4%AB%E8%98%AD" class="mw-redirect" title="克利夫蘭">克利夫蘭</a>附近的某個地方<a href="#cite_note-fatty-7">[6]</a>。」 </li> <li id="cite_note-60"><a href="#cite_ref-60">^</a> 有兩種類型的保護機制是可能的<a href="#cite_note-KopanyasKozai-59">[56]</a>： <ol><li>對於「a」和「e」值使得它們只能在近日點（或遠日點）附近遇到行星的天體，這種相遇可以通過高傾角和「ω」大約90°或270°的天體來阻止（即使相遇發生，由於相對速度相對較高，它們也不會對小行星的軌道產生太大影響）。</li> <li>當「ω」在0°或180°左右振盪，並且小行星的半長軸接近擾動行星的半長軸時，另一種機制是可行的：在這種情況下°節點交叉總是遠離行星本身，發生在近日點和遠日點附近，前提是偏心率足夠高並且行星的軌道幾乎是圓形的。</li></ol> </li> <li id="cite_note-63"><a href="#cite_ref-63">^</a> 對於具有較大半長軸和傾角以及較小偏心率的物體，進動速率較慢： <math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle {\dot {\varpi }}={\frac {3}{4}}{\sqrt {\frac {GM}{a^{3}}}}{\frac {1}{(1-e^{2})^{2}}}\sum _{k=5}^{8}{\frac {m_{k}a_{k}^{2}}{Ma^{2}}}cos^{2}(i)}"> <semantics> <mrow class="MJX-TeXAtom-ORD"> <mstyle displaystyle="true" scriptlevel="0"> <mrow class="MJX-TeXAtom-ORD"> <mrow class="MJX-TeXAtom-ORD"> <mover> <mi>ϖ</mi> <mo>˙</mo> </mover> </mrow> </mrow> <mo>=</mo> <mrow class="MJX-TeXAtom-ORD"> <mfrac> <mn>3</mn> <mn>4</mn> </mfrac> </mrow> <mrow class="MJX-TeXAtom-ORD"> <msqrt> <mfrac> <mrow> <mi>G</mi> <mi>M</mi> </mrow> <msup> <mi>a</mi> <mrow class="MJX-TeXAtom-ORD"> <mn>3</mn> </mrow> </msup> </mfrac> </msqrt> </mrow> <mrow class="MJX-TeXAtom-ORD"> <mfrac> <mn>1</mn> <mrow> <mo stretchy="false">(</mo> <mn>1</mn> <mo>−</mo> <msup> <mi>e</mi> <mrow class="MJX-TeXAtom-ORD"> <mn>2</mn> </mrow> </msup> <msup> <mo stretchy="false">)</mo> <mrow class="MJX-TeXAtom-ORD"> <mn>2</mn> </mrow> </msup> </mrow> </mfrac> </mrow> <munderover> <mo>∑</mo> <mrow class="MJX-TeXAtom-ORD"> <mi>k</mi> <mo>=</mo> <mn>5</mn> </mrow> <mrow class="MJX-TeXAtom-ORD"> <mn>8</mn> </mrow> </munderover> <mrow class="MJX-TeXAtom-ORD"> <mfrac> <mrow> <msub> <mi>m</mi> <mrow class="MJX-TeXAtom-ORD"> <mi>k</mi> </mrow> </msub> <msubsup> <mi>a</mi> <mrow class="MJX-TeXAtom-ORD"> <mi>k</mi> </mrow> <mrow class="MJX-TeXAtom-ORD"> <mn>2</mn> </mrow> </msubsup> </mrow> <mrow> <mi>M</mi> <msup> <mi>a</mi> <mrow class="MJX-TeXAtom-ORD"> <mn>2</mn> </mrow> </msup> </mrow> </mfrac> </mrow> <mi>c</mi> <mi>o</mi> <msup> <mi>s</mi> <mrow class="MJX-TeXAtom-ORD"> <mn>2</mn> </mrow> </msup> <mo stretchy="false">(</mo> <mi>i</mi> <mo stretchy="false">)</mo> </mstyle> </mrow> <annotation encoding="application/x-tex">{\displaystyle {\dot {\varpi }}={\frac {3}{4}}{\sqrt {\frac {GM}{a^{3}}}}{\frac {1}{(1-e^{2})^{2}}}\sum _{k=5}^{8}{\frac {m_{k}a_{k}^{2}}{Ma^{2}}}cos^{2}(i)}</annotation> </semantics> </math><img src="https://wikimedia.org/api/rest_v1/media/math/render/svg/74cca8c45124d14485188ad3a6ee2dea0ba57fd4" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -3.171ex; width:41.594ex; height:7.509ex;" alt="{\displaystyle {\dot {\varpi }}={\frac {3}{4}}{\sqrt {\frac {GM}{a^{3}}}}{\frac {1}{(1-e^{2})^{2}}}\sum _{k=5}^{8}{\frac {m_{k}a_{k}^{2}}{Ma^{2}}}cos^{2}(i)}" /> 此處的<math xmlns="http://www.w3.org/1998/Math/MathML" alttext="{\displaystyle m_{k}a_{k}}"> <semantics> <mrow class="MJX-TeXAtom-ORD"> <mstyle displaystyle="true" scriptlevel="0"> <msub> <mi>m</mi> <mrow class="MJX-TeXAtom-ORD"> <mi>k</mi> </mrow> </msub> <msub> <mi>a</mi> <mrow class="MJX-TeXAtom-ORD"> <mi>k</mi> </mrow> </msub> </mstyle> </mrow> <annotation encoding="application/x-tex">{\displaystyle m_{k}a_{k}}</annotation> </semantics> </math><img src="https://wikimedia.org/api/rest_v1/media/math/render/svg/d2cc81a84bff6241b6f7b7aa07e93b6f1d37394f" class="mwe-math-fallback-image-inline mw-invert skin-invert" aria-hidden="true" style="vertical-align: -0.671ex; width:5.448ex; height:2.009ex;" alt="{\displaystyle m_{k}a_{k}}" />是行星木星穿過海王星的質量和半長軸。 </li> <li id="cite_note-73"><a href="#cite_ref-73">^</a> 括弧中的計算值。 </li> <li id="cite_note-74"><a href="#cite_ref-74">^</a> 6個天體的升交點的平均經度約為102°。在後來發表的一篇部落格中，巴蒂金和布朗將他們對升交點經度的估計限制為7000164060949687467♠94°。 </li> <li id="cite_note-83"><a href="#cite_ref-83">^</a> 文章中的類似圖形在伯斯特（Beust）<a href="#cite_note-Beust_2016-81">[74]</a>、巴蒂金和莫比德利（Morbidelli）的文章中<a href="#cite_note-Batygin_Morbidelli_2017-82">[75]</a>。圖是哈密頓（Hamiltonian）繪的，顯示了具有相等能量的軌道偏心率和取向的組合。如果沒有與第九行星近距離相遇，這將改變軌道的能量，那麼隨著軌道的演變，天體的<a href="/wiki/%E8%BB%8C%E9%81%93%E6%A0%B9%E6%95%B8" title="軌道根數">軌道根數</a>將保持在其中一條曲線上。 </li> <li id="cite_note-106"><a href="#cite_ref-106">^</a> 在具有半長軸大於150 AU>的八個天體中，OSSOS發現了三個具有Trojillo和Sheppard（2014）先前確定的星團之外的近日點（ω）參數<a href="#cite_note-Sheppard2014-6">[5]</a>：<a href="/w/index.php?title=2015_GT50&action=edit&redlink=1" class="new" title="2015 GT50（页面不存在）">2015 GT50</a>、<a href="/w/index.php?title=2015_KH163&action=edit&redlink=1" class="new" title="2015 KH163（页面不存在）">2015 KH163</a>、和 <a href="/w/index.php?title=2013_UT15&action=edit&redlink=1" class="new" title="2013 UT15（页面不存在）">2013 UT15</a><a href="#cite_note-Shankman_etal_2017-105">[97]</a>。 </li> <li id="cite_note-113"><a href="#cite_ref-113">^</a> 所有 15 個軌道演化圖的連結包含在文章的檔案版本中. </li> <li id="cite_note-115"><a href="#cite_ref-115">^</a> 尚克曼等人估計，這個群體的質量是地球質量的幾十倍，需要從巨行星附近噴出數百到數千個地球質量才能保留下來。在尼斯模型中，估計有20-50個地球質量被噴射出來，在巨行星形成過程中，也有相當大的質量從它們附近噴出。 </li> <li id="cite_note-131"><a href="#cite_ref-131">^</a> 在平均運動共振中，這通常被稱為（也許是錯誤的）<a href="/wiki/%E5%8F%A4%E5%9C%A8%E6%A9%9F%E5%88%B6" title="古在機制">古在機制</a><a href="#cite_note-Malhotra_2017-130">[119]</a>。 </li> <li id="cite_note-136"><a href="#cite_ref-136">^</a> 假設這些天體的軌道元素沒有改變，Jílková等人提出，與路過的恆星相遇可能有助於獲得這些天體–被他們稱為類賽德娜天體（與q > 30 和a > 150的<a href="/wiki/%E6%A5%B5%E7%AB%AF%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="極端海王星外天體">極端海王星外天體</a>）。他們還預測，「類賽德娜天體」區域有930個星子，內歐特雲通過同樣的遭遇獲得了約440個星子<a href="#cite_note-JilkovaSednito-134">[122]</a><a href="#cite_note-stealingsedna-135">[123]</a>。 </li> </ol></div> <div id="references-NoteFoot"></div> <div class="mw-heading mw-heading2"><h2 id="相關條目">相關條目</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=24" title="编辑章节：相關條目">编辑</a>]</div> <ul><li><a href="/wiki/%E5%81%87%E8%A8%AD%E7%9A%84%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E8%A1%8C%E6%98%9F" title="假設的海王星外行星">假設的海王星外行星</a></li> <li><a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E7%9A%84%E5%81%87%E8%A8%AD%E5%A4%A9%E9%AB%94%E5%88%97%E8%A1%A8#行星" title="太陽系的假設天體列表">太陽系的假設天體列表</a></li> <li><a href="/wiki/%E5%A0%A4%E5%96%80_(%E5%81%87%E6%83%B3%E8%A1%8C%E6%98%9F)" title="堤喀 (假想行星)">堤喀</a></li> <li><a href="/wiki/%E6%B6%85%E5%A2%A8%E8%A5%BF%E6%96%AF%E6%98%9F" title="涅墨西斯星">涅墨西斯星</a>（復仇女神）</li> <li><a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E5%BD%A2%E6%88%90%E8%88%87%E6%BC%94%E5%8C%96%E5%81%87%E8%AA%AA%E7%9A%84%E6%AD%B7%E5%8F%B2" title="太陽系形成與演化假說的歷史">太陽系形成與演化假說的歷史</a></li> <li><a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E7%9A%84%E5%81%87%E8%A8%AD%E5%A4%A9%E9%AB%94%E5%88%97%E8%A1%A8" title="太陽系的假設天體列表">太陽系的假設天體列表</a></li> <li><a href="/wiki/%E5%B0%BC%E6%AF%94%E9%B2%81%E7%A2%B0%E6%92%9E#第九行星" title="尼比鲁碰撞">尼比鲁碰撞#第九行星</a></li> <li><a href="/wiki/%E7%A5%9D%E8%9E%8D%E6%98%9F" title="祝融星">祝融星</a></li></ul> <div class="mw-heading mw-heading2"><h2 id="參考資料">參考資料</h2>[<a href="/w/index.php?title=%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&action=edit&section=25" title="编辑章节：參考資料">编辑</a>]</div> <div class="reflist columns references-column-width" style="-moz-column-width: 30em; -webkit-column-width: 30em; column-width: 30em; list-style-type: decimal;"> <ol class="references"> <li id="cite_note-Brown_Batygin_2021z-1">^ <a href="#cite_ref-Brown_Batygin_2021z_1-0">1.0</a> <a href="#cite_ref-Brown_Batygin_2021z_1-1">1.1</a> <a href="#cite_ref-Brown_Batygin_2021z_1-2">1.2</a> <a href="#cite_ref-Brown_Batygin_2021z_1-3">1.3</a> <a href="#cite_ref-Brown_Batygin_2021z_1-4">1.4</a> <cite class="citation journal">Brown, Michael E.; Batygin, Konstantin. A search for Planet Nine using the Zwicky Transient Facility public archive. The Astronomical Journal. 31 January 2022, 163 (2): 102. <a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2022AJ....163..102B">Bibcode:2022AJ....163..102B</a>. <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:239768690">S2CID 239768690</a>. <a rel="nofollow" class="external text" href="//arxiv.org/abs/2110.13117">arXiv:2110.13117</a> <img alt="可免费查阅" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" width="9" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813" />. <a rel="nofollow" class="external text" href="https://doi.org/10.3847%2F1538-3881%2Fac32dd">doi:10.3847/1538-3881/ac32dd</a> <img alt="可免费查阅" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" width="9" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813" />.</cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=A+search+for+Planet+Nine+using+the+Zwicky+Transient+Facility+public+archive&rft.au=Batygin%2C+Konstantin&rft.aufirst=Michael+E.&rft.aulast=Brown&rft.date=2022-01-31&rft.genre=article&rft.issue=2&rft.jtitle=The+Astronomical+Journal&rft.pages=102&rft.volume=163&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A239768690&rft_id=info%3Aarxiv%2F2110.13117&rft_id=info%3Abibcode%2F2022AJ....163..102B&rft_id=info%3Adoi%2F10.3847%2F1538-3881%2Fac32dd&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-P9H2019-2">^ <a href="#cite_ref-P9H2019_2-0">2.0</a> <a href="#cite_ref-P9H2019_2-1">2.1</a> <a href="#cite_ref-P9H2019_2-2">2.2</a> <a href="#cite_ref-P9H2019_2-3">2.3</a> <a href="#cite_ref-P9H2019_2-4">2.4</a> <a href="#cite_ref-P9H2019_2-5">2.5</a> <a href="#cite_ref-P9H2019_2-6">2.6</a> <a href="#cite_ref-P9H2019_2-7">2.7</a> <a href="#cite_ref-P9H2019_2-8">2.8</a> <cite class="citation journal">Batygin, Konstantin; Adams, Fred C.; Brown, Michael E.; Becker, Juliette C. The Planet Nine Hypothesis. <a href="/w/index.php?title=Physics_Reports&action=edit&redlink=1" class="new" title="Physics Reports（页面不存在）">Physics Reports</a>. 2019, 805: 1–53. <a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2019PhR...805....1B">Bibcode:2019PhR...805....1B</a>. <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:119248548">S2CID 119248548</a>. <a rel="nofollow" class="external text" href="//arxiv.org/abs/1902.10103">arXiv:1902.10103</a> <img alt="可免费查阅" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" width="9" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813" />. <a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.physrep.2019.01.009">doi:10.1016/j.physrep.2019.01.009</a>.</cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=The+Planet+Nine+Hypothesis&rft.au=Adams%2C+Fred+C.&rft.au=Becker%2C+Juliette+C.&rft.au=Brown%2C+Michael+E.&rft.aufirst=Konstantin&rft.aulast=Batygin&rft.date=2019&rft.genre=article&rft.jtitle=Physics+Reports&rft.pages=1-53&rft.volume=805&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A119248548&rft_id=info%3Aarxiv%2F1902.10103&rft_id=info%3Abibcode%2F2019PhR...805....1B&rft_id=info%3Adoi%2F10.1016%2Fj.physrep.2019.01.009&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-Batygin2021-4">^ <a href="#cite_ref-Batygin2021_4-0">3.0</a> <a href="#cite_ref-Batygin2021_4-1">3.1</a> <a href="#cite_ref-Batygin2021_4-2">3.2</a> <a href="#cite_ref-Batygin2021_4-3">3.3</a> <a href="#cite_ref-Batygin2021_4-4">3.4</a> <cite class="citation journal"><a href="/w/index.php?title=Michael_E._Brown&action=edit&redlink=1" class="new" title="Michael E. Brown（页面不存在）">Brown, Michael E.</a>; <a href="/wiki/Konstantin_Batygin" class="mw-redirect" title="Konstantin Batygin">Batygin, Konstantin</a>. The Orbit of Planet Nine. The Astronomical Journal. 2021-08-26, 162 (5): 219. <a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2021AJ....162..219B">Bibcode:2021AJ....162..219B</a>. <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:230196275">S2CID 230196275</a>. <a rel="nofollow" class="external text" href="//arxiv.org/abs/2108.09868">arXiv:2108.09868</a> <img alt="可免费查阅" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" width="9" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813" />. <a rel="nofollow" class="external text" href="https://doi.org/10.3847%2F1538-3881%2Fac2056">doi:10.3847/1538-3881/ac2056</a> <img alt="可免费查阅" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" width="9" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813" />.</cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=The+Orbit+of+Planet+Nine&rft.au=Batygin%2C+Konstantin&rft.aufirst=Michael+E.&rft.aulast=Brown&rft.date=2021-08-26&rft.genre=article&rft.issue=5&rft.jtitle=The+Astronomical+Journal&rft.pages=219&rft.volume=162&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A230196275&rft_id=info%3Aarxiv%2F2108.09868&rft_id=info%3Abibcode%2F2021AJ....162..219B&rft_id=info%3Adoi%2F10.3847%2F1538-3881%2Fac2056&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-TAJ201601-5">^ <a href="#cite_ref-TAJ201601_5-0">4.00</a> <a href="#cite_ref-TAJ201601_5-1">4.01</a> <a href="#cite_ref-TAJ201601_5-2">4.02</a> <a href="#cite_ref-TAJ201601_5-3">4.03</a> <a href="#cite_ref-TAJ201601_5-4">4.04</a> <a href="#cite_ref-TAJ201601_5-5">4.05</a> <a href="#cite_ref-TAJ201601_5-6">4.06</a> <a href="#cite_ref-TAJ201601_5-7">4.07</a> <a href="#cite_ref-TAJ201601_5-8">4.08</a> <a href="#cite_ref-TAJ201601_5-9">4.09</a> <a href="#cite_ref-TAJ201601_5-10">4.10</a> <a href="#cite_ref-TAJ201601_5-11">4.11</a> <a href="#cite_ref-TAJ201601_5-12">4.12</a> <a href="#cite_ref-TAJ201601_5-13">4.13</a> <a href="#cite_ref-TAJ201601_5-14">4.14</a> <a href="#cite_ref-TAJ201601_5-15">4.15</a> <a href="#cite_ref-TAJ201601_5-16">4.16</a> <a href="#cite_ref-TAJ201601_5-17">4.17</a> <a href="#cite_ref-TAJ201601_5-18">4.18</a> <a href="#cite_ref-TAJ201601_5-19">4.19</a> <cite class="citation journal"><a href="/wiki/Konstantin_Batygin" class="mw-redirect" title="Konstantin Batygin">Batygin, Konstantin</a>; <a href="/w/index.php?title=Michael_E._Brown&action=edit&redlink=1" class="new" title="Michael E. 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Universe Today. 10 August 2015 [25 February 2019]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20180123211102/https://www.universetoday.com/32522/oort-cloud/">存档</a>于23 January 2018）.</cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=What+is+the+Oort+Cloud%3F&rft.aufirst=Matt&rft.aulast=Williams&rft.date=2015-08-10&rft.genre=unknown&rft.jtitle=Universe+Today&rft_id=https%3A%2F%2Fwww.universetoday.com%2F32522%2Foort-cloud%2F&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-Kohne_Batygin_2020-90"><a href="#cite_ref-Kohne_Batygin_2020_90-0">^</a> <cite class="citation journal">Köhne, Tobias; Batygin, Konstantin. On the Dynamical Origins of Retrograde Jupiter Trojans and their Connection to High-Inclination TNOs. 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Wayt. <a rel="nofollow" class="external text" href="https://spectrum.ieee.org/aerospace/satellites/is-there-a-giant-planet-lurking-beyond-pluto">Is There a Giant Planet Lurking Beyond Pluto?</a>. <a href="/wiki/IEEE_Spectrum" class="mw-redirect" title="IEEE Spectrum">IEEE Spectrum</a>. August 2017 [1 August 2017]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20170801005216/https://spectrum.ieee.org/aerospace/satellites/is-there-a-giant-planet-lurking-beyond-pluto">存档</a>于1 August 2017）.</cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=Is+There+a+Giant+Planet+Lurking+Beyond+Pluto%3F&rft.aufirst=W.+Wayt&rft.aulast=Gibbs&rft.date=2017-08&rft.genre=unknown&rft.jtitle=IEEE+Spectrum&rft_id=https%3A%2F%2Fspectrum.ieee.org%2Faerospace%2Fsatellites%2Fis-there-a-giant-planet-lurking-beyond-pluto&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-TomLevensonAtlantic-92">^ <a href="#cite_ref-TomLevensonAtlantic_92-0">84.0</a> <a href="#cite_ref-TomLevensonAtlantic_92-1">84.1</a> <cite class="citation magazine">Levenson, Thomas. <a rel="nofollow" class="external text" href="https://www.theatlantic.com/science/archive/2016/01/a-new-planet-or-a-red-herring/42681">A New Planet or a Red Herring?</a>. <a href="/wiki/The_Atlantic" class="mw-redirect" title="The Atlantic">The Atlantic</a>. 25 January 2016 [18 July 2016]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20211019195840/https://www.theatlantic.com/politics/archive/2007/06/the-capitolist/42681/">存档</a>于19 October 2021）. <q><a href="/w/index.php?title=Template:-%27&action=edit&redlink=1" class="new" title="Template:-'（页面不存在）">Template:-'</a>We plotted the real data on top of the model' Batyagin recalls, and they fell 'exactly where they were supposed to be.' That was, he said, the epiphany. 'It was a dramatic moment. This thing I thought could disprove it turned out to be the strongest evidence for Planet Nine.'</q></cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=A+New+Planet+or+a+Red+Herring%3F&rft.aufirst=Thomas&rft.aulast=Levenson&rft.date=2016-01-25&rft.genre=article&rft.jtitle=The+Atlantic&rft_id=https%3A%2F%2Fwww.theatlantic.com%2Fscience%2Farchive%2F2016%2F01%2Fa-new-planet-or-a-red-herring%2F42681&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-vergeSlamDunkandWaterTightEvidence-93"><a href="#cite_ref-vergeSlamDunkandWaterTightEvidence_93-0">^</a> <cite class="citation news">Grush, Loren. <a rel="nofollow" class="external text" href="https://www.theverge.com/2016/1/20/10801824/ninth-planet-x-discovered-evidence">Our Solar System May Have a Ninth Planet After All – but Not All Evidence Is in (We Still Haven't Seen It Yet)</a>. <a href="/wiki/The_Verge" title="The Verge">The Verge</a>. 20 January 2016 [18 July 2016]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20160729141120/http://www.theverge.com/2016/1/20/10801824/ninth-planet-x-discovered-evidence">存档</a>于29 July 2016）. <q>The statistics do sound promising, at first. The researchers say there's a 1 in 15,000 chance that the movements of these objects are coincidental and don't indicate a planetary presence at all. ... 'When we usually consider something as clinched and air tight, it usually has odds with a much lower probability of failure than what they have,' says Sara Seager, a planetary scientist at MIT. For a study to be a slam dunk, the odds of failure are usually 1 in 1,744,278. ... But researchers often publish before they get the slam-dunk odds, in order to avoid getting scooped by a competing team, Seager says. Most outside experts agree that the researchers' models are strong. And Neptune was originally detected in a similar fashion—by researching observed anomalies in the movement of Uranus. Additionally, the idea of a large planet at such a distance from the Sun isn't actually that unlikely, according to Bruce Macintosh, a planetary scientist at Stanford University.</q></cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=Our+Solar+System+May+Have+a+Ninth+Planet+After+All+%E2%80%93+but+Not+All+Evidence+Is+in+%28We+Still+Haven%27t+Seen+It+Yet%29&rft.aufirst=Loren&rft.aulast=Grush&rft.date=2016-01-20&rft.genre=article&rft.jtitle=The+Verge&rft_id=https%3A%2F%2Fwww.theverge.com%2F2016%2F1%2F20%2F10801824%2Fninth-planet-x-discovered-evidence&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-scantEvidence-94"><a href="#cite_ref-scantEvidence_94-0">^</a> <cite class="citation magazine">Crocket, Christopher. <a rel="nofollow" class="external text" href="https://www.sciencenews.org/article/computer-simulations-heat-hunt-planet-nine">Computer Simulations Heat up Hunt for Planet Nine</a>. <a href="/w/index.php?title=Science_News&action=edit&redlink=1" class="new" title="Science News（页面不存在）">Science News</a>. 31 January 2016 [7 February 2016]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20160206211941/https://www.sciencenews.org/article/computer-simulations-heat-hunt-planet-nine">存档</a>于6 February 2016）. <q><a href="/w/index.php?title=Template:-%27&action=edit&redlink=1" class="new" title="Template:-'（页面不存在）">Template:-'</a>It's exciting and very compelling work,' says Meg Schwamb, a planetary scientist at Academia Sinica in Taipei, Taiwan. But only six bodies lead the way to the putative planet. 'Whether that's enough is still a question.'</q></cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=Computer+Simulations+Heat+up+Hunt+for+Planet+Nine&rft.aufirst=Christopher&rft.aulast=Crocket&rft.date=2016-01-31&rft.genre=article&rft.jtitle=Science+News&rft_id=https%3A%2F%2Fwww.sciencenews.org%2Farticle%2Fcomputer-simulations-heat-hunt-planet-nine&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-pbsBrown-95"><a href="#cite_ref-pbsBrown_95-0">^</a> <cite class="citation news"><a rel="nofollow" class="external text" href="https://www.pbs.org/newshour/bb/we-cant-see-this-possible-9th-planet-but-we-feel-its-presence/">We Can't See This Possible 9th Planet, but We Feel Its Presence</a>. <a href="/wiki/PBS_NewsHour" class="mw-redirect" title="PBS NewsHour">PBS NewsHour</a>. 22 January 2016 [18 July 2016]. （原始内容<a rel="nofollow" class="external text" href="https://web.archive.org/web/20160722042941/http://www.pbs.org/newshour/bb/we-cant-see-this-possible-9th-planet-but-we-feel-its-presence/">存档</a>于22 July 2016）. <q><a href="/w/index.php?title=Template:-%27&action=edit&redlink=1" class="new" title="Template:-'（页面不存在）">Template:-'</a>Right now, any good scientist is going to be skeptical, because it's a pretty big claim. And without the final evidence that it's real, there is always that chance that it's not. So, everybody should be skeptical. But I think it's time to mount this search. I mean, we like to think of it as, we have provided the treasure map of where this ninth planet is, and we have done the starting gun, and now it's a race to actually point your telescope at the right spot in the sky and make that discovery of planet nine.' —Mike Brown</q></cite><span title="ctx_ver=Z39.88-2004&rfr_id=info%3Asid%2Fzh.wikipedia.org%3A%E7%AC%AC%E4%B9%9D%E8%A1%8C%E6%98%9F&rft.atitle=We+Can%27t+See+This+Possible+9th+Planet%2C+but+We+Feel+Its+Presence&rft.date=2016-01-22&rft.genre=article&rft.jtitle=PBS+NewsHour&rft_id=https%3A%2F%2Fwww.pbs.org%2Fnewshour%2Fbb%2Fwe-cant-see-this-possible-9th-planet-but-we-feel-its-presence%2F&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal" class="Z3988">  </li> <li id="cite_note-popsci-96"><a href="#cite_ref-popsci_96-0">^</a> <cite class="citation web">Fecht, Sarah. <a rel="nofollow" class="external text" href="http://www.popsci.com/could-there-really-be-9th-planet-that-we-didnt-know-about">Can There Really Be a Planet in Our Solar 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src="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/12px-Commons-logo.svg.png" decoding="async" width="12" height="16" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/18px-Commons-logo.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/4a/Commons-logo.svg/24px-Commons-logo.svg.png 2x" data-file-width="1024" data-file-height="1376" /> <a href="/wiki/%E7%BB%B4%E5%9F%BA%E5%85%B1%E4%BA%AB%E8%B5%84%E6%BA%90" title="维基共享资源">维基共享资源</a>上的相關多媒體資源：<a href="https://commons.wikimedia.org/wiki/Category:Planet_Nine" class="extiw" title="commons:Category:Planet Nine">第九行星</a></li> <li><a rel="nofollow" class="external text" href="http://findplanetnine.blogspot.com/">The Search for Planet Nine</a> （<a rel="nofollow" class="external text" href="//web.archive.org/web/20171124104719/http://findplanetnine.blogspot.com/">页面存档备份</a>，存于<a href="/wiki/%E4%BA%92%E8%81%94%E7%BD%91%E6%A1%A3%E6%A1%88%E9%A6%86" title="互联网档案馆">互联网档案馆</a>） – Blog by Brown and Batygin</li> <li><a rel="nofollow" class="external text" href="https://solarsystem.nasa.gov/planets/hypothetical-planet-x/in-depth/">Hypothetical Planet X</a> （<a rel="nofollow" class="external text" href="//web.archive.org/web/20191019012033/https://solarsystem.nasa.gov/planets/hypothetical-planet-x/in-depth/">页面存档备份</a>，存于<a href="/wiki/%E4%BA%92%E8%81%94%E7%BD%91%E6%A1%A3%E6%A1%88%E9%A6%86" title="互联网档案馆">互联网档案馆</a>） – NASA Planetary Science Division</li></ul> <div class="navbox-styles"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84265675" /><style data-mw-deduplicate="TemplateStyles:r84261037">.mw-parser-output .navbox{box-sizing:border-box;border:1px solid #a2a9b1;width:100%;clear:both;font-size:88%;text-align:center;padding:1px;margin:1em auto 0}.mw-parser-output .navbox .navbox{margin-top:0}.mw-parser-output .navbox+.navbox,.mw-parser-output .navbox+.navbox-styles+.navbox{margin-top:-1px}.mw-parser-output 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title="土星环" /><area href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F" shape="circle" coords="418,18,12" alt="天王星" title="天王星" /><area href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" shape="circle" coords="427,10,6" alt="天王星的卫星" title="天王星的卫星" /><area href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F%E7%8E%AF" shape="rect" coords="408,4,429,34" alt="天王星环" title="天王星环" /><area href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F" shape="circle" coords="462,18,12" alt="海王星" title="海王星" /><area href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" shape="circle" coords="471,10,3" alt="海王星的卫星" title="海王星的卫星" /><area href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%8E%AF" shape="rect" coords="441,9,485,28" alt="海王星环" title="海王星环" /><area href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F" shape="circle" coords="504,18,8" alt="冥王星" title="冥王星" /><area href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" shape="circle" coords="510,13,3" alt="冥王星的卫星" title="冥王星的卫星" /><area href="/wiki/%E5%A6%8A%E7%A5%9E%E6%98%9F" shape="circle" coords="534,18,8" alt="妊神星" title="妊神星" /><area href="/wiki/%E5%A6%8A%E7%A5%9E%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" shape="circle" coords="540,13,3" alt="妊神星的卫星" title="妊神星的卫星" /><area href="/wiki/%E9%B8%9F%E7%A5%9E%E6%98%9F" shape="circle" coords="567,18,8" alt="鸟神星" title="鸟神星" /><area href="/wiki/%E6%9F%AF%E4%BC%8A%E4%BC%AF%E5%B8%A6" shape="rect" coords="490,0,580,35" alt="柯伊伯带" title="柯伊伯带" /><area href="/wiki/%E9%98%8B%E7%A5%9E%E6%98%9F" shape="circle" coords="596,18,8" alt="阋神星" title="阋神星" /><area href="/wiki/%E9%98%8B%E5%8D%AB%E4%B8%80" shape="circle" coords="602,13,3" alt="阋卫一" title="阋卫一" /><area href="/wiki/%E9%9B%A2%E6%95%A3%E7%9B%A4" shape="rect" coords="581,0,610,35" alt="離散盤" title="離散盤" /><area href="/wiki/%E5%A5%A5%E5%B0%94%E7%89%B9%E4%BA%91" shape="rect" coords="623,0,640,35" alt="山形云" title="山形云" /><area href="/wiki/%E5%A5%A5%E5%B0%94%E7%89%B9%E4%BA%91" shape="rect" coords="641,0,666,35" alt="奥尔特云" title="奥尔特云" /></map><figcaption></figcaption></figure></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align: center"><a href="/wiki/%E5%A4%AA%E9%98%B3" title="太阳">太阳</a> • <a href="/wiki/%E5%A4%AA%E9%99%BD%E5%9C%88" title="太陽圈">太陽圈</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><td colspan="2" class="navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th id="行星" scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E8%A1%8C%E6%98%9F" title="行星">行星</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E6%B0%B4%E6%98%9F" title="水星">水星</a></li> <li><a href="/wiki/%E9%87%91%E6%98%9F" title="金星">金星</a></li> <li><a href="/wiki/%E5%9C%B0%E7%90%83" title="地球">地球</a> <ul><li><a href="/wiki/%E6%9C%88%E7%90%83" title="月球">月球</a></li></ul></li> <li><a href="/wiki/%E7%81%AB%E6%98%9F" title="火星">火星</a> <ul><li><a href="/wiki/%E7%81%AB%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" class="mw-redirect" title="火星的卫星">火卫</a></li></ul></li> <li><a href="/wiki/%E6%9C%A8%E6%98%9F" title="木星">木星</a> <ul><li><a href="/wiki/%E6%9C%A8%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="木星的卫星">木衛</a></li> <li><a href="/wiki/%E6%9C%A8%E6%98%9F%E7%8E%AF" class="mw-redirect" title="木星环">木星环</a></li></ul></li> <li><a href="/wiki/%E5%9C%9F%E6%98%9F" title="土星">土星</a> <ul><li><a href="/wiki/%E5%9C%9F%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="土星的卫星">土卫</a></li> <li><a href="/wiki/%E5%9C%9F%E6%98%9F%E7%8E%AF" class="mw-redirect" title="土星环">土星环</a></li></ul></li> <li><a href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F" title="天王星">天王星</a> <ul><li><a href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="天王星的卫星">天卫</a></li> <li><a href="/wiki/%E5%A4%A9%E7%8E%8B%E6%98%9F%E7%8E%AF" class="mw-redirect" title="天王星环">天王星环</a></li></ul></li> <li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F" title="海王星">海王星</a> <ul><li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="海王星的卫星">海卫</a></li> <li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%8E%AF" class="mw-redirect" title="海王星环">海王星环</a></li></ul></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E7%9F%AE%E8%A1%8C%E6%98%9F" title="矮行星">矮行星</a></th><td class="navbox-list-with-group navbox-list navbox-even hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E7%A9%80%E7%A5%9E%E6%98%9F" title="穀神星">穀神星</a></li> <li><a href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F" title="冥王星">冥王星</a> <ul><li><a href="/wiki/%E5%86%A5%E7%8E%8B%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" class="mw-redirect" title="冥王星的卫星">冥卫</a></li></ul></li> <li><a href="/wiki/%E5%A6%8A%E7%A5%9E%E6%98%9F" title="妊神星">妊神星</a> <ul><li><a href="/wiki/%E5%A6%8A%E7%A5%9E%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="妊神星的卫星">妊卫</a></li></ul></li> <li><a href="/wiki/%E9%B8%9F%E7%A5%9E%E6%98%9F" title="鸟神星">鸟神星</a> <ul><li><a href="/wiki/S/2015_(136472)_1" title="S/2015 (136472) 1">鳥卫一</a></li></ul></li> <li><a href="/wiki/%E9%98%8B%E7%A5%9E%E6%98%9F" title="阋神星">阋神星</a> <ul><li><a href="/wiki/%E9%98%8B%E5%8D%AB%E4%B8%80" title="阋卫一">阋卫一</a></li></ul></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><td colspan="2" class="navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th id="太阳系小天体" scope="row" class="navbox-group" style="width:1%;padding: 0.35em; text-align: center"><a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E5%B0%8F%E5%A4%A9%E9%AB%94" title="太陽系小天體">太阳系 小天体</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F" title="小行星">小行星</a> （<a href="/wiki/%E5%BE%AE%E5%9E%8B%E8%A1%8C%E6%98%9F" title="微型行星">微型行星</a>）</th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th id="小行星族" scope="row" class="navbox-group" style="width:1%"><a href="/wiki/Category:%E5%B0%8F%E8%A1%8C%E6%98%9F%E6%97%8F" title="Category:小行星族">小行星族</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E7%A5%9D%E8%9E%8D%E5%9E%8B%E5%B0%8F%E8%A1%8C%E6%98%9F" title="祝融型小行星">祝融型小行星</a></li> <li><a href="/wiki/%E8%BF%91%E5%9C%B0%E5%A4%A9%E4%BD%93" title="近地天体">近地小行星</a></li> <li><a href="/wiki/%E4%B8%BB%E5%B0%8F%E8%A1%8C%E6%98%9F%E5%B8%B6" title="主小行星帶">主小行星帶</a></li> <li><a href="/wiki/%E7%89%B9%E6%B4%9B%E4%BC%8A%E5%A4%A9%E4%BD%93" title="特洛伊天体">特洛伊天体</a> <ul><li><a href="/wiki/%E6%9C%A8%E6%98%9F%E7%89%B9%E6%B4%9B%E4%BC%8A" title="木星特洛伊">木星特洛伊</a></li> <li><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E7%89%B9%E6%B4%9B%E4%BC%8A" title="海王星特洛伊">海王星特洛伊</a></li></ul></li> <li><a href="/wiki/%E5%B8%8C%E5%B0%94%E8%BE%BE%E6%97%8F" title="希尔达族">希尔达族</a></li> <li><a href="/wiki/%E5%8D%8A%E4%BA%BA%E9%A9%AC%E5%B0%8F%E8%A1%8C%E6%98%9F" title="半人马小行星">半人马小行星</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F%E8%A1%9B%E6%98%9F" title="小行星衛星">小行星衛星</a></li> <li><a href="/wiki/%E6%B5%81%E6%98%9F%E4%BD%93" title="流星体">流星体</a></li> <li><a href="/wiki/%E6%99%BA%E7%A5%9E%E6%98%9F" title="智神星">小行星2智神星</a></li> <li><a href="/wiki/%E5%A9%9A%E7%A5%9E%E6%98%9F" title="婚神星">小行星3婚神星</a></li> <li><a href="/wiki/%E7%81%B6%E7%A5%9E%E6%98%9F" title="灶神星">小行星4灶神星</a></li> <li><a href="/wiki/%E5%81%A5%E7%A5%9E%E6%98%9F" title="健神星">小行星10健神星</a></li></ul> </div></td></tr><tr><td colspan="2" class="navbox-list navbox-even hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em">另见：<a href="/wiki/%E5%80%BC%E5%BE%97%E9%97%9C%E6%B3%A8%E7%9A%84%E5%B0%8F%E8%A1%8C%E6%98%9F%E5%88%97%E8%A1%A8" title="值得關注的小行星列表">小行星列表</a>。</div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E6%B5%B7%E7%8E%8B%E6%98%9F%E5%A4%96%E5%A4%A9%E9%AB%94" title="海王星外天體">海王星 外天体</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th id="古柏带" scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E6%9F%AF%E4%BC%8A%E4%BC%AF%E5%B8%A6" title="柯伊伯带">古柏带</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"></div><table class="nowraplinks navbox-subgroup" style="border-spacing:0"><tbody><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E5%86%A5%E6%97%8F%E5%B0%8F%E5%A4%A9%E9%AB%94" title="冥族小天體">冥族小天體</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E4%BA%A1%E7%A5%9E%E6%98%9F" title="亡神星">小行星90482亡神星</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F28978" title="小行星28978">小行星28978伊克西翁</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E5%82%B3%E7%B5%B1%E5%8F%A4%E6%9F%8F%E5%B8%B6%E5%A4%A9%E9%AB%94" title="傳統古柏帶天體">傳統古柏帶天體</a></th><td class="navbox-list-with-group navbox-list navbox-even hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F55637" title="小行星55637">小行星55637</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F20000" title="小行星20000">小行星20000伐罗那</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F15760" title="小行星15760">小行星15760</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F55636" title="小行星55636">小行星55636</a></li> <li><a href="/wiki/%E5%88%9B%E7%A5%9E%E6%98%9F" title="创神星">小行星50000创神星</a></li> <li><a href="/wiki/%E9%9B%A8%E7%A5%9E%E6%98%9F" title="雨神星">小行星38628雨神星</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F55565" title="小行星55565">小行星55565</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E9%9B%A2%E6%95%A3%E7%9B%A4" title="離散盤">離散盤</a></th><td class="navbox-list-with-group navbox-list navbox-odd hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F84522" title="小行星84522">小行星84522</a></li> <li><a href="/wiki/2004_XR190" class="mw-redirect" title="2004 XR190">2004 XR190</a></li> <li><a href="/wiki/%E5%B0%8F%E8%A1%8C%E6%98%9F90377" class="mw-redirect" title="小行星90377">小行星90377賽德娜</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E5%BD%97%E6%98%9F" title="彗星">彗星</a></th><td class="navbox-list-with-group navbox-list navbox-even hlist" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E5%91%A8%E6%9C%9F%E5%BD%97%E6%98%9F%E5%88%97%E8%A1%A8" class="mw-redirect" title="周期彗星列表">周期彗星</a>和<a href="/wiki/%E9%9D%9E%E9%80%B1%E6%9C%9F%E5%BD%97%E6%98%9F%E5%88%97%E8%A1%A8" title="非週期彗星列表">非周期彗星</a></li> <li><a href="/wiki/%E8%BE%BE%E6%91%A9%E5%85%8B%E5%9E%8B%E5%B0%8F%E8%A1%8C%E6%98%9F" title="达摩克型小行星">达摩克型小行星</a></li> <li><a href="/wiki/%E5%86%85%E5%A5%A5%E5%B0%94%E7%89%B9%E4%BA%91" title="内奥尔特云">内欧特云</a></li> <li><a href="/wiki/%E5%A5%A5%E5%B0%94%E7%89%B9%E4%BA%91" title="奥尔特云">欧特云</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr></tbody></table><div></div></td></tr></tbody></table><div></div></td></tr><tr><td class="navbox-abovebelow" colspan="2" style="font-size: smaller"><div>另见：<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB%E7%9A%84%E5%BD%A2%E6%88%90%E4%B8%8E%E6%BC%94%E5%8C%96" title="太阳系的形成与演化">太阳系的形成与演化</a>、<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB%E5%A4%A9%E4%BD%93%E5%8F%91%E7%8E%B0%E6%97%B6%E9%97%B4%E5%88%97%E8%A1%A8" title="太阳系天体发现时间列表">太阳系天体发现时间列表</a>、<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB%E5%A4%A9%E4%BD%93%E5%88%97%E8%A1%A8" title="太阳系天体列表">轨道列表</a>和<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB%E5%A4%A9%E4%BD%93%E5%A4%A7%E5%B0%8F%E5%88%97%E8%A1%A8" title="太阳系天体大小列表">大小列表</a>、<a href="/wiki/%E5%A4%AA%E9%99%BD%E7%B3%BB%E7%9A%84%E5%81%87%E8%A8%AD%E5%A4%A9%E9%AB%94%E5%88%97%E8%A1%A8" title="太陽系的假設天體列表">太陽系的假設天體列表</a>、<a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB%E6%A8%A1%E5%9E%8B" title="太阳系模型">太阳系模型</a>，以及<a href="/wiki/Portal:%E5%A4%AA%E9%98%B3%E7%B3%BB" title="Portal:太阳系">太阳系主题</a></div></td></tr></tbody></table></div> <div class="navbox-styles"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84265675" /><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84261037" /></div><div role="navigation" class="navbox" aria-labelledby="2016年太空活動" style="padding:3px"><table class="nowraplinks hlist mw-collapsible autocollapse navbox-inner" style="border-spacing:0;background:transparent;color:inherit"><tbody><tr><th scope="col" class="collapsible-title navbox-title" colspan="3"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84265675" /><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r84244141" /><div class="navbar plainlinks hlist navbar-mini"><ul><li class="nv-view"><a href="/wiki/Template:2016%E5%B9%B4%E5%A4%AA%E7%A9%BA%E6%B4%BB%E5%8A%A8" title="Template:2016年太空活动"><abbr title="查看该模板">查</abbr></a></li><li class="nv-talk"><a href="/wiki/Template_talk:2016%E5%B9%B4%E5%A4%AA%E7%A9%BA%E6%B4%BB%E5%8A%A8" title="Template talk:2016年太空活动"><abbr title="讨论该模板">论</abbr></a></li><li class="nv-edit"><a href="/wiki/Special:%E7%BC%96%E8%BE%91%E9%A1%B5%E9%9D%A2/Template:2016%E5%B9%B4%E5%A4%AA%E7%A9%BA%E6%B4%BB%E5%8A%A8" title="Special:编辑页面/Template:2016年太空活动"><abbr title="编辑该模板">编</abbr></a></li></ul></div><div id="2016年太空活動" style="font-size:110%;margin:0 5em">2016年太空活動</div></th></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><div style="float: left;"> « <a href="/wiki/Template:2015%E5%B9%B4%E5%A4%AA%E7%A9%BA%E6%B4%BB%E5%8B%95" title="Template:2015年太空活動">2015</a> </div> <div style="float: right;"><a href="/wiki/Template:2017%E5%B9%B4%E5%A4%AA%E7%A9%BA%E6%B4%BB%E5%8A%A8" title="Template:2017年太空活动">2017</a> » </div></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/2016%E5%B9%B4%E8%88%AA%E5%A4%A9%E6%B4%BB%E5%8A%A8%E5%88%97%E8%A1%A8" title="2016年航天活动列表">太空探測器發射</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E7%81%AB%E6%98%9F%E5%BE%AE%E9%87%8F%E6%B0%A3%E9%AB%94%E4%BB%BB%E5%8B%99%E8%A1%9B%E6%98%9F" title="火星微量氣體任務衛星">火星微量氣體任務衛星</a>（火星繞行衛星；2016年3月發射）</li> <li><a href="/wiki/%E7%9E%B3_(%E4%BA%BA%E9%80%A0%E8%A1%9B%E6%98%9F)" title="瞳 (人造衛星)">瞳</a>（X射線觀測衛星；2016年2月發射）</li> <li><a href="/wiki/%E6%96%AF%E5%9F%BA%E4%BA%9E%E5%B8%95%E9%9B%B7%E5%88%A9EDM%E7%99%BB%E9%99%B8%E5%99%A8" title="斯基亞帕雷利EDM登陸器">斯基亞帕雷利EDM登陸器</a>（火星登陸器；2016年3月發射）</li> <li><a href="/wiki/OSIRIS-REx" title="OSIRIS-REx">OSIRIS-REx</a>（小行星研究和採樣返回任務；2016年9月發射）</li></ul> </div></td><td class="noviewer navbox-image" rowspan="7" style="width:1px;padding:0px 0px 0px 2px;padding-left: 0.5em;"><div><a href="/wiki/File:JUNO_-_PIA13746.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5b/JUNO_-_PIA13746.jpg/100px-JUNO_-_PIA13746.jpg" decoding="async" width="100" height="83" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/5b/JUNO_-_PIA13746.jpg/150px-JUNO_-_PIA13746.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/5b/JUNO_-_PIA13746.jpg/200px-JUNO_-_PIA13746.jpg 2x" data-file-width="4800" data-file-height="4000" /></a> <a href="/wiki/File:Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg/100px-Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg" decoding="async" width="100" height="141" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/7/71/Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg/150px-Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/71/Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg/200px-Artist%E2%80%99s_impression_of_the_ultracool_dwarf_star_TRAPPIST-1_from_the_surface_of_one_of_its_planets.jpg 2x" data-file-width="3535" data-file-height="5000" /></a></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%"><a href="/wiki/%E6%92%9E%E6%93%8A%E4%BA%8B%E4%BB%B6" title="撞擊事件">撞擊事件</a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=DN160822_03&action=edit&redlink=1" class="new" title="DN160822 03（页面不存在）">DN160822 03</a>（英语：<a href="https://en.wikipedia.org/wiki/DN160822_03" class="extiw" title="en:DN160822 03">DN160822 03</a>）</li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">選擇的<a href="/wiki/%E8%BF%91%E5%9C%B0%E5%A4%A9%E4%BD%93" title="近地天体">近地天体</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=2016%E5%B9%B4%E9%A3%9B%E6%8E%A0%E5%9C%B0%E7%90%83%E7%9A%84%E5%B0%8F%E8%A1%8C%E6%98%9F%E5%88%97%E8%A1%A8&action=edit&redlink=1" class="new" title="2016年飛掠地球的小行星列表（页面不存在）">飛掠地球的小行星</a>（英语：<a href="https://en.wikipedia.org/wiki/List_of_asteroid_close_approaches_to_Earth_in_2016" class="extiw" title="en:List of asteroid close approaches to Earth in 2016">List of asteroid close approaches to Earth in 2016</a>）</li> <li><a href="/w/index.php?title=(85990)_1999_JV6&action=edit&redlink=1" class="new" title="(85990) 1999 JV6（页面不存在）">(85990) 1999 JV6</a></li> <li><a href="/wiki/1994_WR12" title="1994 WR12">1994 WR12</a></li> <li><a href="/w/index.php?title=2013_TX68&action=edit&redlink=1" class="new" title="2013 TX68（页面不存在）">2013 TX68</a></li> <li><a href="/w/index.php?title=2016_EU85&action=edit&redlink=1" class="new" title="2016 EU85（页面不存在）">2016 EU85</a></li> <li><a href="/w/index.php?title=469219_%E6%8C%AF%E7%9B%AA%E5%A4%A9%E6%98%9F&action=edit&redlink=1" class="new" title="469219 振盪天星（页面不存在）">469219 振盪天星</a></li> <li><a href="/w/index.php?title=2016_PQ&action=edit&redlink=1" class="new" title="2016 PQ（页面不存在）">2016 PQ</a>（英语：<a href="https://en.wikipedia.org/wiki/2016_PQ" class="extiw" title="en:2016 PQ">2016 PQ</a>）</li> <li><a href="/w/index.php?title=(164121)_2003_YT1&action=edit&redlink=1" class="new" title="(164121) 2003 YT1（页面不存在）">(164121) 2003 YT1</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">行星</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 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/2016%E5%B9%B4%E5%8F%91%E7%8E%B0%E7%9A%84%E7%B3%BB%E5%A4%96%E8%A1%8C%E6%98%9F%E5%88%97%E8%A1%A8" title="2016年发现的系外行星列表">太陽系外行星</a> <a href="/wiki/Category:2016%E5%B9%B4%E5%8F%91%E7%8E%B0%E7%9A%84%E7%B3%BB%E5%A4%96%E8%A1%8C%E6%98%9F" title="分類:2016年發現的系外行星"><img alt="2016年發現的系外行星列表" src="//upload.wikimedia.org/wikipedia/commons/thumb/4/48/Folder_Hexagonal_Icon.svg/15px-Folder_Hexagonal_Icon.svg.png" decoding="async" width="15" height="13" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/4/48/Folder_Hexagonal_Icon.svg/23px-Folder_Hexagonal_Icon.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/4/48/Folder_Hexagonal_Icon.svg/30px-Folder_Hexagonal_Icon.svg.png 2x" data-file-width="36" data-file-height="31" /></a></th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=%E5%AE%A4%E5%A5%B3%E5%BA%A738b&action=edit&redlink=1" class="new" title="室女座38b（页面不存在）">室女座38b</a>（英语：<a href="https://en.wikipedia.org/wiki/38_Virginis_b" class="extiw" title="en:38 Virginis b">38 Virginis b</a>）</li> <li><a href="/wiki/%E5%B7%A8%E8%9F%B9%E5%BA%A755e" title="巨蟹座55e">巨蟹座55e</a>的大氣層組成成分</li> <li><a href="/wiki/%E8%91%9B%E5%88%A9%E6%96%AF536b" title="葛利斯536b">格利泽536b</a></li> <li><a href="/wiki/2MASS_J2126%E2%80%938140" title="2MASS J2126–8140">JMASS J2126-8140</a></li> <li><a href="/wiki/2MASS_J1119%E2%80%931137" title="2MASS J1119–1137">2MASS J1119–1137</a></li> <li><a href="/wiki/BD%2B20594b" title="BD+20594b">BD+20594b</a></li> <li><a href="/w/index.php?title=Pr0211_c&action=edit&redlink=1" class="new" title="Pr0211 c（页面不存在）">Pr0211 c</a>（英语：<a href="https://en.wikipedia.org/wiki/Pr0211_c" class="extiw" title="en:Pr0211 c">Pr0211 c</a>）</li> <li><a href="/wiki/TRAPPIST-1" title="TRAPPIST-1">TRAPPIST-1</a> <ul><li><a href="/wiki/TRAPPIST-1b" title="TRAPPIST-1b">b</a></li> <li><a href="/w/index.php?title=TRAPPIST-1c&action=edit&redlink=1" class="new" title="TRAPPIST-1c（页面不存在）">c</a>（英语：<a href="https://en.wikipedia.org/wiki/TRAPPIST-1c" class="extiw" title="en:TRAPPIST-1c">TRAPPIST-1c</a>）</li> <li><a href="/wiki/TRAPPIST-1d" title="TRAPPIST-1d">d</a></li></ul></li> <li><a href="/w/index.php?title=%E9%95%B7%E8%9B%87%E5%BA%A7TWb&action=edit&redlink=1" class="new" title="長蛇座TWb（页面不存在）">長蛇座TWb</a>（英语：<a href="https://en.wikipedia.org/wiki/TW_Hydrae_b" class="extiw" title="en:TW Hydrae b">TW Hydrae b</a>）</li> <li><a href="/w/index.php?title=%E5%85%8B%E5%8D%9C%E5%8B%9220g&action=edit&redlink=1" class="new" title="克卜勒20g（页面不存在）">开普勒20g</a>（英语：<a href="https://en.wikipedia.org/wiki/Kepler-20g" class="extiw" title="en:Kepler-20g">Kepler-20g</a>）</li> <li><a href="/w/index.php?title=%E5%85%8B%E5%8D%9C%E5%8B%9256d&action=edit&redlink=1" class="new" title="克卜勒56d（页面不存在）">开普勒56d</a>（英语：<a href="https://en.wikipedia.org/wiki/Kepler-56d" class="extiw" title="en:Kepler-56d">Kepler-56d</a>）</li> <li><a href="/w/index.php?title=%E5%85%8B%E5%8D%9C%E5%8B%92737b&action=edit&redlink=1" class="new" title="克卜勒737b（页面不存在）">开普勒737b</a>（英语：<a href="https://en.wikipedia.org/wiki/Kepler-737b" class="extiw" title="en:Kepler-737b">Kepler-737b</a>）</li> <li><a href="/wiki/%E5%85%8B%E5%8D%9C%E5%8B%921229b" title="克卜勒1229b">开普勒1229b</a></li> <li><a href="/w/index.php?title=%E5%85%8B%E5%8D%9C%E5%8B%921520b&action=edit&redlink=1" class="new" title="克卜勒1520b（页面不存在）">开普勒1520b</a>（英语：<a href="https://en.wikipedia.org/wiki/Kepler-1520b" class="extiw" title="en:Kepler-1520b">Kepler-1520b</a>）</li> <li><a href="/wiki/%E5%85%8B%E5%8D%9C%E5%8B%921625b" title="克卜勒1625b">开普勒1625b</a></li> <li><a href="/wiki/%E5%85%8B%E5%8D%9C%E5%8B%921638b" title="克卜勒1638b">开普勒1638b</a></li> <li><a href="/wiki/%E5%85%8B%E5%8D%9C%E5%8B%921647b" title="克卜勒1647b">开普勒1647b</a></li> <li><a href="/wiki/OGLE-2007-BLG-349(AB)b" title="OGLE-2007-BLG-349(AB)b">OGLE-2007-BLG-349(AB)b</a></li> <li><a href="/wiki/%E6%AF%94%E9%84%B0%E6%98%9Fb" title="比鄰星b">比鄰星b</a></li> <li><a href="/wiki/%E9%87%91%E7%89%9B%E5%BA%A7V830b" title="金牛座V830b">金牛座V830b</a></li> <li><a href="/w/index.php?title=%E5%8D%A1%E9%81%943b&action=edit&redlink=1" class="new" title="卡達3b（页面不存在）">卡塔尔3b</a>（英语：<a href="https://en.wikipedia.org/wiki/Qatar-3b" class="extiw" title="en:Qatar-3b">Qatar-3b</a>）</li> <li><a href="/w/index.php?title=%E5%8D%A1%E9%81%944b&action=edit&redlink=1" class="new" title="卡達4b（页面不存在）">卡塔尔4b</a>（英语：<a href="https://en.wikipedia.org/wiki/Qatar-4b" class="extiw" title="en:Qatar-4b">Qatar-4b</a>）</li> <li><a href="/w/index.php?title=%E5%8D%A1%E9%81%945b&action=edit&redlink=1" class="new" title="卡達5b（页面不存在）">卡塔尔5b</a>（英语：<a href="https://en.wikipedia.org/wiki/Qatar-5b" class="extiw" title="en:Qatar-5b">Qatar-5b</a>）</li> <li><a href="/wiki/K2-33b" title="K2-33b">K2-33b</a></li> <li><a href="/wiki/K2-72" title="K2-72">K2-72</a> <ul><li><a href="/w/index.php?title=K2-72b&action=edit&redlink=1" class="new" title="K2-72b（页面不存在）">b</a>（英语：<a href="https://en.wikipedia.org/wiki/K2-72b" class="extiw" title="en:K2-72b">K2-72b</a>）</li> <li><a href="/wiki/K2-72c" title="K2-72c">c</a></li> <li><a href="/w/index.php?title=K2-72d&action=edit&redlink=1" class="new" title="K2-72d（页面不存在）">d</a>（英语：<a href="https://en.wikipedia.org/wiki/K2-72d" class="extiw" title="en:K2-72d">K2-72d</a>）</li> <li><a href="/wiki/K2-72e" title="K2-72e">e</a></li></ul></li> <li><a href="/wiki/HIP_41378" title="HIP 41378">HIP 41378</a> <ul><li><a href="/wiki/HIP_41378_b" title="HIP 41378 b">b</a></li> <li><a href="/wiki/HIP_41378_c" title="HIP 41378 c">c</a></li> <li><a href="/wiki/HIP_41378_d" title="HIP 41378 d">d</a></li> <li><a href="/wiki/HIP_41378_e" title="HIP 41378 e">e</a></li> <li><a href="/wiki/HIP_41378_f" title="HIP 41378 f">f</a></li></ul></li> <li><a href="/w/index.php?title=HD_19467_B&action=edit&redlink=1" class="new" title="HD 19467 B（页面不存在）">HD 19467 b</a>（英语：<a href="https://en.wikipedia.org/wiki/HD_19467_B" class="extiw" title="en:HD 19467 B">HD 19467 B</a>）</li> <li><a href="/w/index.php?title=HD_164922_c&action=edit&redlink=1" class="new" title="HD 164922 c（页面不存在）">HD 164922 c</a>（英语：<a href="https://en.wikipedia.org/wiki/HD_164922_c" class="extiw" title="en:HD 164922 c">HD 164922 c</a>）</li> <li><a href="/wiki/KELT-9b" title="KELT-9b">KELT-9b</a></li> <li><a href="/wiki/KELT-11b" title="KELT-11b">KELT-11b</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align: center;"><a href="/wiki/%E5%A4%AA%E9%98%B3%E7%B3%BB" title="太阳系">太阳系</a></th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a class="mw-selflink selflink">第九行星</a></li></ul> </div></td></tr></tbody></table><div></div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">发现</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=IDCS_J1426.5%2B3508&action=edit&redlink=1" class="new" title="IDCS J1426.5+3508（页面不存在）">IDCS 1426</a>（英语：<a href="https://en.wikipedia.org/wiki/IDCS_J1426.5%2B3508" class="extiw" title="en:IDCS J1426.5+3508">IDCS J1426.5+3508</a>）</li> <li><a href="/wiki/BOSS%E9%95%B7%E5%9F%8E" title="BOSS長城">BOSS長城</a></li> <li><a href="/wiki/GN-z11" title="GN-z11">GN-z11</a></li> <li><a href="/wiki/SDSS_J1240%2B6710" title="SDSS J1240+6710">SDSS J1240+6710</a></li> <li><a href="/w/index.php?title=%E5%B7%A8%E7%88%B5%E5%BA%A72%E7%9F%AE%E6%98%9F%E7%B3%BB&action=edit&redlink=1" class="new" title="巨爵座2矮星系（页面不存在）">巨爵座2</a>（英语：<a href="https://en.wikipedia.org/wiki/Crater_2_dwarf_galaxy" class="extiw" title="en:Crater 2 dwarf galaxy">Crater 2 dwarf galaxy</a>）</li> <li><a href="/wiki/(471325)_2011_KT19" title="(471325) 2011 KT19">2011 KT19</a></li> <li><a href="/wiki/GW150914" title="GW150914">GW150914</a> （首次观测引力波，在2015年发现）</li> <li><a href="/wiki/GW151226" title="GW151226">GW151226</a>（在2015年发现）</li> <li><a href="/wiki/2015_RR245" title="2015 RR245">2015 RR245</a>（在2015年发现）</li> <li><a href="/w/index.php?title=GRB_160625B&action=edit&redlink=1" class="new" title="GRB 160625B（页面不存在）">GRB 160625B</a>（英语：<a href="https://en.wikipedia.org/wiki/GRB_160625B" class="extiw" title="en:GRB 160625B">GRB 160625B</a>）</li> <li><a href="/wiki/2014_UZ224" title="2014 UZ224">2014 UZ224</a>（在2014年发现）</li> <li><a href="/w/index.php?title=WISE_J080822.18-644357.3&action=edit&redlink=1" class="new" title="WISE J080822.18-644357.3（页面不存在）">WISE J080822.18-644357.3</a>（英语：<a href="https://en.wikipedia.org/wiki/WISE_J080822.18-644357.3" class="extiw" title="en:WISE J080822.18-644357.3">WISE J080822.18-644357.3</a>）</li> <li><a href="/wiki/%E5%AE%A4%E5%A5%B3%E5%BA%A7_%E2%85%A0" title="室女座 Ⅰ">室女座 Ⅰ</a></li> <li><a href="/wiki/HD_131399_Ab" title="HD 131399 Ab">HD 131399 Ab</a></li> <li><a href="/wiki/%E6%9C%A8%E6%98%9F%E7%9A%84%E5%8D%AB%E6%98%9F" title="木星的卫星">木星的卫星</a> <ul><li><a href="/wiki/%E6%9C%A8%E8%A1%9B%E4%BA%94%E5%8D%81%E5%9B%9B" title="木衛五十四">54</a></li> <li><a href="/wiki/%E6%9C%A8%E8%A1%9B%E5%85%AD%E5%8D%81%E4%BA%8C" title="木衛六十二">62</a></li> <li><a href="/w/index.php?title=S/2016_J_3&action=edit&redlink=1" class="new" title="S/2016 J 3（页面不存在）">S/2016 J 3</a>（英语：<a href="https://en.wikipedia.org/wiki/S/2016_J_3" class="extiw" title="en:S/2016 J 3">S/2016 J 3</a>）</li> <li><a href="/wiki/S/2016_J_4" title="S/2016 J 4">S/2016 J 4</a></li></ul></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">彗星</th><td class="navbox-list-with-group navbox-list navbox-odd" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=252P/%E6%9E%97%E5%B0%BC%E7%88%BE%E5%BD%97%E6%98%9F&action=edit&redlink=1" class="new" title="252P/林尼爾彗星（页面不存在）">252P/林尼爾彗星</a>（英语：<a href="https://en.wikipedia.org/wiki/252P/LINEAR" class="extiw" title="en:252P/LINEAR">252P/LINEAR</a>）</li> <li><a href="/w/index.php?title=P/2016_BA14&action=edit&redlink=1" class="new" title="P/2016 BA14（页面不存在）">P/2016 BA14</a>（英语：<a href="https://en.wikipedia.org/wiki/P/2016_BA14_(PanSTARRS)" class="extiw" title="en:P/2016 BA14 (PanSTARRS)">P/2016 BA14 (PanSTARRS)</a>）</li> <li><a href="/w/index.php?title=53P/%E8%8C%83%C2%B7%E6%AF%94%E6%96%AF%E5%B8%83%E6%B4%9B%E5%85%8B%E5%BD%97%E6%98%9F&action=edit&redlink=1" class="new" title="53P/范·比斯布洛克彗星（页面不存在）">53P/范·比斯布洛克彗星</a>（英语：<a href="https://en.wikipedia.org/wiki/53P/Van_Biesbroeck" class="extiw" title="en:53P/Van Biesbroeck">53P/Van Biesbroeck</a>）</li> <li><a href="/w/index.php?title=C/2016_R2&action=edit&redlink=1" class="new" title="C/2016 R2（页面不存在）">C/2016 R2</a>（英语：<a href="https://en.wikipedia.org/wiki/C/2016_R2_(PanSTARRS)" class="extiw" title="en:C/2016 R2 (PanSTARRS)">C/2016 R2 (PanSTARRS)</a>）</li> <li><a href="/wiki/%E7%BB%B4%E5%B0%94%E7%89%B9%E4%BA%8C%E5%8F%B7%E5%BD%97%E6%98%9F" title="维尔特二号彗星">维尔特二号彗星</a></li> <li><a href="/wiki/%E5%9D%A6%E6%99%AE%E5%B0%941%E5%8F%B7%E5%BD%97%E6%98%9F" title="坦普尔1号彗星">坦普尔1号彗星</a></li> <li><a href="/wiki/%E4%B8%B2%E7%94%B0%E5%BD%97%E6%98%9F" title="串田彗星">串田彗星</a></li> <li><a href="/w/index.php?title=%E6%B2%83%E5%B0%94%E5%A4%AB-%E5%93%88%E7%81%B5%E9%A1%BF%E5%BD%97%E6%98%9F&action=edit&redlink=1" class="new" title="沃尔夫-哈灵顿彗星（页面不存在）">沃尔夫-哈灵顿彗星</a>（英语：<a href="https://en.wikipedia.org/wiki/43P/Wolf%E2%80%93Harrington" class="extiw" title="en:43P/Wolf–Harrington">43P/Wolf–Harrington</a>）</li> <li><a href="/wiki/%E6%9C%AC%E7%94%B0-%E5%A7%86%E5%B0%94%E7%A7%91%E6%96%AF-%E5%B8%95%E4%BC%8A%E6%9D%9C%E8%8E%8E%E7%A7%91%E5%A8%83%E5%BD%97%E6%98%9F" title="本田-姆尔科斯-帕伊杜莎科娃彗星">本田-姆尔科斯-帕伊杜莎科娃彗星</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%">太空探索</th><td class="navbox-list-with-group navbox-list navbox-even" style="width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/%E6%9C%B1%E8%AF%BA%E5%8F%B7" title="朱诺号">朱诺号</a>（进入<a href="/wiki/%E6%9C%A8%E6%98%9F" title="木星">木星</a>轨道；2016年7月）</li> <li><a href="/wiki/%E7%BE%85%E5%A1%9E%E5%A1%94%E8%99%9F" title="羅塞塔號">羅塞塔號</a>／<a href="/wiki/%E8%8F%B2%E8%90%8A%E7%99%BB%E9%99%B8%E5%99%A8" title="菲萊登陸器">菲萊登陸器</a>（任务结束于<a href="/wiki/%E6%A5%9A%E7%95%99%E8%8E%AB%E5%A4%AB-%E6%A0%BC%E6%8B%89%E5%B8%8C%E9%96%80%E5%85%8B%E5%BD%97%E6%98%9F" class="mw-redirect" title="楚留莫夫-格拉希門克彗星">67P/彗星</a>；2016年9月）</li> <li><a href="/wiki/%E6%96%AF%E5%9F%BA%E4%BA%9E%E5%B8%95%E9%9B%B7%E5%88%A9EDM%E7%99%BB%E9%99%B8%E5%99%A8" title="斯基亞帕雷利EDM登陸器">斯基亞帕雷利EDM登陸器</a>（登陸<a href="/wiki/%E7%81%AB%E6%98%9F" title="火星">火星</a>；2016年10月）</li></ul> </div></td></tr><tr><td class="navbox-abovebelow" colspan="3"><div> <ul><li><img src="//upload.wikimedia.org/wikipedia/commons/thumb/e/e0/Symbol_question.svg/16px-Symbol_question.svg.png" decoding="async" width="16" height="16" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/e/e0/Symbol_question.svg/23px-Symbol_question.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/e/e0/Symbol_question.svg/31px-Symbol_question.svg.png 2x" data-file-width="180" data-file-height="185" /> <a href="/wiki/Category:2015%E5%B9%B4%E5%A4%AA%E7%A9%BA" title="Category:2015年太空">Category:2015年太空</a> — <a href="/wiki/Category:2016%E5%B9%B4%E5%A4%AA%E7%A9%BA" title="Category:2016年太空">Category:2016年太空</a> — <a href="/wiki/Category:2017%E5%B9%B4%E5%A4%AA%E7%A9%BA" title="Category:2017年太空">Category:2017年太空</a></li></ul> </div></td></tr></tbody></table></div> <style data-mw-deduplicate="TemplateStyles:r84365013">.mw-parser-output .portal-bar{font-size:88%;font-weight:bold;display:flex;justify-content:center;align-items:baseline}.mw-parser-output .portal-bar-bordered{padding:0 2em;background-color:#fdfdfd;border:1px solid #a2a9b1;clear:both;margin:1em auto 0}.mw-parser-output .portal-bar-unbordered{padding:0 1.7em;margin-left:0}.mw-parser-output .portal-bar-content{display:flex;flex-flow:row wrap;flex:0 1 auto;padding:0.15em 0;column-gap:1em;align-items:baseline;margin:0;list-style:none}.mw-parser-output .portal-bar-item{display:inline-block;margin:0.15em 0.2em;min-height:24px;line-height:24px}@media screen and (max-width:768px){.mw-parser-output .portal-bar{font-size:88%;font-weight:bold;display:flex;flex-flow:column wrap;align-items:baseline}.mw-parser-output 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