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class="vector-menu-content-list"> <li id="pt-sitesupport-2" class="user-links-collapsible-item mw-list-item user-links-collapsible-item"><a data-mw="interface" href="//donate.wikimedia.org/wiki/Special:FundraiserRedirector?utm_source=donate&utm_medium=sidebar&utm_campaign=C13_bs.wikipedia.org&uselang=bs" class=""><span>Donacije</span></a> </li> <li id="pt-createaccount-2" class="user-links-collapsible-item mw-list-item user-links-collapsible-item"><a data-mw="interface" href="/w/index.php?title=Posebno:Napravi_ra%C4%8Dun&returnto=Raspr%C5%A1eni+disk" title="Predlažemo vam da napravite račun i prijavite se; međutim, to nije obavezno" class=""><span>Napravi korisnički račun</span></a> </li> <li id="pt-login-2" class="user-links-collapsible-item mw-list-item user-links-collapsible-item"><a data-mw="interface" href="/w/index.php?title=Posebno:Korisni%C4%8Dka_prijava&returnto=Raspr%C5%A1eni+disk" title="Predlažemo vam da se prijavite, iako to nije obavezno [o]" accesskey="o" class=""><span>Prijavi me</span></a> </li> </ul> </div> </div> </div> <div id="vector-user-links-dropdown" class="vector-dropdown vector-user-menu vector-button-flush-right vector-user-menu-logged-out" title="Više opcija" > <input type="checkbox" id="vector-user-links-dropdown-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-user-links-dropdown" class="vector-dropdown-checkbox " aria-label="Lični alati" > <label id="vector-user-links-dropdown-label" for="vector-user-links-dropdown-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--icon-only " aria-hidden="true" ><span class="vector-icon mw-ui-icon-ellipsis mw-ui-icon-wikimedia-ellipsis"></span> <span class="vector-dropdown-label-text">Lični alati</span> </label> <div class="vector-dropdown-content"> <div id="p-personal" class="vector-menu mw-portlet mw-portlet-personal user-links-collapsible-item" 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decoding=\"async\" width=\"40\" height=\"43\" class=\"mw-file-element\" srcset=\"//upload.wikimedia.org/wikipedia/commons/thumb/7/71/Wikipedia_Asian_Month_Logo.svg/60px-Wikipedia_Asian_Month_Logo.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/7/71/Wikipedia_Asian_Month_Logo.svg/80px-Wikipedia_Asian_Month_Logo.svg.png 2x\" data-file-width=\"512\" data-file-height=\"555\" /\u003E\u003C/a\u003E\u003C/span\u003E\u003C/td\u003E\u003Ctd class=\"mbox-text\"\u003EOd 1. do 30. novembra 2024. učestvujte u projektu \u003Ca href=\"/wiki/Wikipedia:Azijski_mjesec/2024.\" title=\"Wikipedia:Azijski mjesec/2024.\"\u003E\"Azijski mjesec\"\u003C/a\u003E.\u003C/td\u003E\u003C/tr\u003E\u003C/tbody\u003E\u003C/table\u003E\u003C/div\u003E\u003C/div\u003E\u003C/div\u003E\u003C/div\u003E";}}());</script></div> </div> <div class="vector-column-start"> <div class="vector-main-menu-container"> <div id="mw-navigation"> <nav id="mw-panel" class="vector-main-menu-landmark" aria-label="Sajt"> <div 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id="mw-panel-toc-list"> <li 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">Početak</div> </a> </li> <li id="toc-Otkriće" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Otkriće"> <div class="vector-toc-text"> <span class="vector-toc-numb">1</span> <span>Otkriće</span> </div> </a> <ul id="toc-Otkriće-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Podjele_transneptunskog_prostora" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Podjele_transneptunskog_prostora"> <div class="vector-toc-text"> <span class="vector-toc-numb">2</span> <span>Podjele transneptunskog prostora</span> </div> </a> <button aria-controls="toc-Podjele_transneptunskog_prostora-sublist" class="cdx-button cdx-button--weight-quiet cdx-button--icon-only vector-toc-toggle"> <span class="vector-icon mw-ui-icon-wikimedia-expand"></span> <span>Uključi/isključi podsekciju Podjele transneptunskog prostora</span> </button> <ul id="toc-Podjele_transneptunskog_prostora-sublist" class="vector-toc-list"> <li id="toc-Raspršeni_disk_naspram_Kuiperovog_pojasa" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Raspršeni_disk_naspram_Kuiperovog_pojasa"> <div class="vector-toc-text"> <span class="vector-toc-numb">2.1</span> <span>Raspršeni disk naspram Kuiperovog pojasa</span> </div> </a> <ul id="toc-Raspršeni_disk_naspram_Kuiperovog_pojasa-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Odvojeni_objekti" class="vector-toc-list-item vector-toc-level-2"> <a class="vector-toc-link" href="#Odvojeni_objekti"> <div class="vector-toc-text"> <span class="vector-toc-numb">2.2</span> <span>Odvojeni objekti</span> </div> </a> <ul id="toc-Odvojeni_objekti-sublist" class="vector-toc-list"> </ul> </li> </ul> </li> <li id="toc-Orbite" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Orbite"> <div class="vector-toc-text"> <span class="vector-toc-numb">3</span> <span>Orbite</span> </div> </a> <ul id="toc-Orbite-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Formiranje" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Formiranje"> <div class="vector-toc-text"> <span class="vector-toc-numb">4</span> <span>Formiranje</span> </div> </a> <ul id="toc-Formiranje-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Sasr+tav" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Sasr+tav"> <div class="vector-toc-text"> <span class="vector-toc-numb">5</span> <span>Sasr+tav</span> </div> </a> <ul id="toc-Sasr+tav-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Komete" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Komete"> <div class="vector-toc-text"> <span class="vector-toc-numb">6</span> <span>Komete</span> </div> </a> <ul id="toc-Komete-sublist" class="vector-toc-list"> </ul> </li> <li id="toc-Reference" class="vector-toc-list-item vector-toc-level-1 vector-toc-list-item-expanded"> <a class="vector-toc-link" href="#Reference"> <div class="vector-toc-text"> <span class="vector-toc-numb">7</span> <span>Reference</span> </div> </a> <ul id="toc-Reference-sublist" class="vector-toc-list"> </ul> </li> </ul> </div> </div> </nav> </div> </div> <div class="mw-content-container"> <main id="content" class="mw-body"> <header class="mw-body-header vector-page-titlebar"> <nav aria-label="Sadržaj" class="vector-toc-landmark"> <div id="vector-page-titlebar-toc" class="vector-dropdown vector-page-titlebar-toc vector-button-flush-left" > <input type="checkbox" id="vector-page-titlebar-toc-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-vector-page-titlebar-toc" class="vector-dropdown-checkbox " aria-label="Uključi/isključi sadržaj" > <label id="vector-page-titlebar-toc-label" for="vector-page-titlebar-toc-checkbox" class="vector-dropdown-label cdx-button cdx-button--fake-button cdx-button--fake-button--enabled cdx-button--weight-quiet cdx-button--icon-only " aria-hidden="true" ><span class="vector-icon mw-ui-icon-listBullet mw-ui-icon-wikimedia-listBullet"></span> <span class="vector-dropdown-label-text">Uključi/isključi sadržaj</span> </label> <div class="vector-dropdown-content"> <div id="vector-page-titlebar-toc-unpinned-container" class="vector-unpinned-container"> </div> </div> </div> </nav> <h1 id="firstHeading" class="firstHeading mw-first-heading"><span class="mw-page-title-main">Raspršeni disk</span></h1> <div id="p-lang-btn" class="vector-dropdown mw-portlet mw-portlet-lang" > <input type="checkbox" id="p-lang-btn-checkbox" role="button" aria-haspopup="true" data-event-name="ui.dropdown-p-lang-btn" class="vector-dropdown-checkbox mw-interlanguage-selector" aria-label="Idi na članak na drugom jeziku. Dostupno na 60 jezika" > <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" ><span class="vector-icon mw-ui-icon-language-progressive mw-ui-icon-wikimedia-language-progressive"></span> <span class="vector-dropdown-label-text">60 jezika</span> </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/Verstrooide_skyf" title="Verstrooide skyf – afrikans" lang="af" hreflang="af" data-title="Verstrooide skyf" data-language-autonym="Afrikaans" data-language-local-name="afrikans" class="interlanguage-link-target"><span>Afrikaans</span></a></li><li class="interlanguage-link interwiki-ar mw-list-item"><a href="https://ar.wikipedia.org/wiki/%D9%82%D8%B1%D8%B5_%D9%85%D8%AA%D9%81%D8%B1%D9%82" title="قرص متفرق – arapski" lang="ar" hreflang="ar" data-title="قرص متفرق" data-language-autonym="العربية" data-language-local-name="arapski" class="interlanguage-link-target"><span>العربية</span></a></li><li class="interlanguage-link interwiki-be mw-list-item"><a href="https://be.wikipedia.org/wiki/%D0%A0%D0%B0%D1%81%D1%81%D0%B5%D1%8F%D0%BD%D1%8B_%D0%B4%D1%8B%D1%81%D0%BA" title="Рассеяны дыск – bjeloruski" lang="be" hreflang="be" data-title="Рассеяны дыск" data-language-autonym="Беларуская" data-language-local-name="bjeloruski" class="interlanguage-link-target"><span>Беларуская</span></a></li><li class="interlanguage-link interwiki-be-x-old mw-list-item"><a href="https://be-tarask.wikipedia.org/wiki/%D0%A0%D0%B0%D1%81%D1%8C%D1%81%D0%B5%D1%8F%D0%BD%D1%8B_%D0%B4%D1%8B%D1%81%D0%BA" title="Расьсеяны дыск – Belarusian (Taraškievica orthography)" lang="be-tarask" hreflang="be-tarask" data-title="Расьсеяны дыск" data-language-autonym="Беларуская (тарашкевіца)" data-language-local-name="Belarusian (Taraškievica orthography)" class="interlanguage-link-target"><span>Беларуская (тарашкевіца)</span></a></li><li class="interlanguage-link interwiki-bg mw-list-item"><a href="https://bg.wikipedia.org/wiki/%D0%A0%D0%B0%D0%B7%D1%80%D0%B5%D0%B4%D0%B5%D0%BD_%D0%B4%D0%B8%D1%81%D0%BA" title="Разреден диск – bugarski" lang="bg" hreflang="bg" data-title="Разреден диск" data-language-autonym="Български" data-language-local-name="bugarski" class="interlanguage-link-target"><span>Български</span></a></li><li class="interlanguage-link interwiki-ca mw-list-item"><a href="https://ca.wikipedia.org/wiki/Disc_dispers" title="Disc dispers – katalonski" lang="ca" hreflang="ca" data-title="Disc dispers" data-language-autonym="Català" data-language-local-name="katalonski" class="interlanguage-link-target"><span>Català</span></a></li><li class="interlanguage-link interwiki-ckb mw-list-item"><a href="https://ckb.wikipedia.org/wiki/%D8%AF%DB%8C%D8%B3%DA%A9%DB%8C_%D8%A8%DA%B5%D8%A7%D9%88" title="دیسکی بڵاو – centralnokurdski" lang="ckb" hreflang="ckb" data-title="دیسکی بڵاو" data-language-autonym="کوردی" data-language-local-name="centralnokurdski" class="interlanguage-link-target"><span>کوردی</span></a></li><li class="interlanguage-link interwiki-cs badge-Q17437796 badge-featuredarticle mw-list-item" title="istaknuti članak"><a href="https://cs.wikipedia.org/wiki/Rozpt%C3%BDlen%C3%BD_disk" title="Rozptýlený disk – češki" lang="cs" hreflang="cs" data-title="Rozptýlený disk" data-language-autonym="Čeština" data-language-local-name="češki" class="interlanguage-link-target"><span>Čeština</span></a></li><li class="interlanguage-link interwiki-cy mw-list-item"><a href="https://cy.wikipedia.org/wiki/Y_Ddisgen_Wasgaredig" title="Y Ddisgen Wasgaredig – velški" lang="cy" hreflang="cy" data-title="Y Ddisgen Wasgaredig" data-language-autonym="Cymraeg" data-language-local-name="velški" class="interlanguage-link-target"><span>Cymraeg</span></a></li><li class="interlanguage-link interwiki-de mw-list-item"><a href="https://de.wikipedia.org/wiki/Scattered_Disk_Object" title="Scattered Disk Object – njemački" lang="de" hreflang="de" data-title="Scattered Disk Object" data-language-autonym="Deutsch" data-language-local-name="njemački" class="interlanguage-link-target"><span>Deutsch</span></a></li><li class="interlanguage-link interwiki-el mw-list-item"><a href="https://el.wikipedia.org/wiki/%CE%91%CE%BD%CF%84%CE%B9%CE%BA%CE%B5%CE%AF%CE%BC%CE%B5%CE%BD%CE%BF_%CE%B4%CE%B9%CE%B1%CF%83%CE%BA%CE%BF%CF%81%CF%80%CE%B9%CF%83%CE%BC%CE%AD%CE%BD%CE%BF%CF%85_%CE%B4%CE%AF%CF%83%CE%BA%CE%BF%CF%85" title="Αντικείμενο διασκορπισμένου δίσκου – grčki" lang="el" hreflang="el" data-title="Αντικείμενο διασκορπισμένου δίσκου" data-language-autonym="Ελληνικά" data-language-local-name="grčki" class="interlanguage-link-target"><span>Ελληνικά</span></a></li><li class="interlanguage-link interwiki-en badge-Q17437796 badge-featuredarticle mw-list-item" title="istaknuti članak"><a href="https://en.wikipedia.org/wiki/Scattered_disc" title="Scattered disc – engleski" lang="en" hreflang="en" data-title="Scattered disc" data-language-autonym="English" data-language-local-name="engleski" class="interlanguage-link-target"><span>English</span></a></li><li class="interlanguage-link interwiki-eo mw-list-item"><a href="https://eo.wikipedia.org/wiki/Disa_disko" title="Disa disko – esperanto" lang="eo" hreflang="eo" data-title="Disa disko" data-language-autonym="Esperanto" data-language-local-name="esperanto" class="interlanguage-link-target"><span>Esperanto</span></a></li><li class="interlanguage-link interwiki-es mw-list-item"><a href="https://es.wikipedia.org/wiki/Disco_disperso" title="Disco disperso – španski" lang="es" hreflang="es" data-title="Disco disperso" data-language-autonym="Español" data-language-local-name="španski" class="interlanguage-link-target"><span>Español</span></a></li><li class="interlanguage-link interwiki-eu mw-list-item"><a href="https://eu.wikipedia.org/wiki/Disko_sakabanatua" title="Disko sakabanatua – baskijski" lang="eu" hreflang="eu" data-title="Disko sakabanatua" data-language-autonym="Euskara" data-language-local-name="baskijski" class="interlanguage-link-target"><span>Euskara</span></a></li><li class="interlanguage-link interwiki-fa mw-list-item"><a href="https://fa.wikipedia.org/wiki/%D8%AF%DB%8C%D8%B3%DA%A9_%D9%BE%D8%B1%D8%A7%DA%A9%D9%86%D8%AF%D9%87" title="دیسک پراکنده – perzijski" lang="fa" hreflang="fa" data-title="دیسک پراکنده" data-language-autonym="فارسی" data-language-local-name="perzijski" class="interlanguage-link-target"><span>فارسی</span></a></li><li class="interlanguage-link interwiki-fi mw-list-item"><a href="https://fi.wikipedia.org/wiki/Hajanainen_kiekko" title="Hajanainen kiekko – finski" lang="fi" hreflang="fi" data-title="Hajanainen kiekko" data-language-autonym="Suomi" data-language-local-name="finski" class="interlanguage-link-target"><span>Suomi</span></a></li><li class="interlanguage-link interwiki-fr mw-list-item"><a href="https://fr.wikipedia.org/wiki/Disque_des_objets_%C3%A9pars" title="Disque des objets épars – francuski" lang="fr" hreflang="fr" data-title="Disque des objets épars" data-language-autonym="Français" data-language-local-name="francuski" class="interlanguage-link-target"><span>Français</span></a></li><li class="interlanguage-link interwiki-gl mw-list-item"><a href="https://gl.wikipedia.org/wiki/Disco_disperso" title="Disco disperso – galicijski" lang="gl" hreflang="gl" data-title="Disco disperso" data-language-autonym="Galego" data-language-local-name="galicijski" class="interlanguage-link-target"><span>Galego</span></a></li><li class="interlanguage-link interwiki-gn mw-list-item"><a href="https://gn.wikipedia.org/wiki/Apu%27a_ha%27e%C3%B1o" title="Apu'a ha'eño – gvarani" lang="gn" hreflang="gn" data-title="Apu'a ha'eño" data-language-autonym="Avañe'ẽ" data-language-local-name="gvarani" class="interlanguage-link-target"><span>Avañe'ẽ</span></a></li><li class="interlanguage-link interwiki-he mw-list-item"><a href="https://he.wikipedia.org/wiki/%D7%94%D7%93%D7%99%D7%A1%D7%A7_%D7%94%D7%9E%D7%A4%D7%95%D7%96%D7%A8" title="הדיסק המפוזר – hebrejski" lang="he" hreflang="he" data-title="הדיסק המפוזר" data-language-autonym="עברית" data-language-local-name="hebrejski" class="interlanguage-link-target"><span>עברית</span></a></li><li class="interlanguage-link interwiki-hi mw-list-item"><a href="https://hi.wikipedia.org/wiki/%E0%A4%AC%E0%A4%BF%E0%A4%96%E0%A4%B0%E0%A4%BE_%E0%A4%9A%E0%A4%95%E0%A5%8D%E0%A4%B0" title="बिखरा चक्र – hindi" lang="hi" hreflang="hi" data-title="बिखरा चक्र" data-language-autonym="हिन्दी" data-language-local-name="hindi" class="interlanguage-link-target"><span>हिन्दी</span></a></li><li class="interlanguage-link interwiki-hu mw-list-item"><a href="https://hu.wikipedia.org/wiki/Sz%C3%B3rt_korong" title="Szórt korong – mađarski" lang="hu" hreflang="hu" data-title="Szórt korong" data-language-autonym="Magyar" data-language-local-name="mađarski" class="interlanguage-link-target"><span>Magyar</span></a></li><li class="interlanguage-link interwiki-hy mw-list-item"><a href="https://hy.wikipedia.org/wiki/%D5%91%D6%80%D5%BE%D5%A1%D5%AE_%D5%BD%D5%AF%D5%A1%D5%BE%D5%A1%D5%BC%D5%A1%D5%AF" title="Ցրված սկավառակ – armenski" lang="hy" hreflang="hy" data-title="Ցրված սկավառակ" data-language-autonym="Հայերեն" data-language-local-name="armenski" class="interlanguage-link-target"><span>Հայերեն</span></a></li><li class="interlanguage-link interwiki-id mw-list-item"><a href="https://id.wikipedia.org/wiki/Piringan_tersebar" title="Piringan tersebar – indonezijski" lang="id" hreflang="id" data-title="Piringan tersebar" data-language-autonym="Bahasa Indonesia" data-language-local-name="indonezijski" class="interlanguage-link-target"><span>Bahasa Indonesia</span></a></li><li class="interlanguage-link interwiki-it mw-list-item"><a href="https://it.wikipedia.org/wiki/Disco_diffuso" title="Disco diffuso – italijanski" lang="it" hreflang="it" data-title="Disco diffuso" data-language-autonym="Italiano" data-language-local-name="italijanski" class="interlanguage-link-target"><span>Italiano</span></a></li><li class="interlanguage-link interwiki-ja mw-list-item"><a href="https://ja.wikipedia.org/wiki/%E6%95%A3%E4%B9%B1%E5%86%86%E7%9B%A4%E5%A4%A9%E4%BD%93" title="散乱円盤天体 – japanski" lang="ja" hreflang="ja" data-title="散乱円盤天体" data-language-autonym="日本語" data-language-local-name="japanski" class="interlanguage-link-target"><span>日本語</span></a></li><li class="interlanguage-link interwiki-kab mw-list-item"><a href="https://kab.wikipedia.org/wiki/A%E1%B9%ADebsi_yettuzuzren" title="Aṭebsi yettuzuzren – kabile" lang="kab" hreflang="kab" data-title="Aṭebsi yettuzuzren" data-language-autonym="Taqbaylit" data-language-local-name="kabile" class="interlanguage-link-target"><span>Taqbaylit</span></a></li><li class="interlanguage-link interwiki-ko mw-list-item"><a href="https://ko.wikipedia.org/wiki/%EC%82%B0%EB%9E%80%EC%9B%90%EB%B0%98" title="산란원반 – korejski" lang="ko" hreflang="ko" data-title="산란원반" data-language-autonym="한국어" data-language-local-name="korejski" class="interlanguage-link-target"><span>한국어</span></a></li><li class="interlanguage-link interwiki-la mw-list-item"><a href="https://la.wikipedia.org/wiki/Corpora_transneptuniana_dispersa" title="Corpora transneptuniana dispersa – latinski" lang="la" hreflang="la" data-title="Corpora transneptuniana dispersa" data-language-autonym="Latina" data-language-local-name="latinski" class="interlanguage-link-target"><span>Latina</span></a></li><li class="interlanguage-link interwiki-lb mw-list-item"><a href="https://lb.wikipedia.org/wiki/Scattered_disk_object" title="Scattered disk object – luksemburški" lang="lb" hreflang="lb" data-title="Scattered disk object" data-language-autonym="Lëtzebuergesch" data-language-local-name="luksemburški" class="interlanguage-link-target"><span>Lëtzebuergesch</span></a></li><li class="interlanguage-link interwiki-lmo mw-list-item"><a href="https://lmo.wikipedia.org/wiki/Disch_Sparnegat" title="Disch Sparnegat – lombardski" lang="lmo" hreflang="lmo" data-title="Disch Sparnegat" data-language-autonym="Lombard" data-language-local-name="lombardski" class="interlanguage-link-target"><span>Lombard</span></a></li><li class="interlanguage-link interwiki-lv mw-list-item"><a href="https://lv.wikipedia.org/wiki/Izklied%C4%93tais_disks" title="Izkliedētais disks – latvijski" lang="lv" hreflang="lv" data-title="Izkliedētais disks" data-language-autonym="Latviešu" data-language-local-name="latvijski" class="interlanguage-link-target"><span>Latviešu</span></a></li><li class="interlanguage-link interwiki-mk mw-list-item"><a href="https://mk.wikipedia.org/wiki/%D0%A0%D0%B0%D1%81%D0%B5%D0%B0%D0%BD_%D0%94%D0%B8%D1%81%D0%BA" title="Расеан Диск – makedonski" lang="mk" hreflang="mk" data-title="Расеан Диск" data-language-autonym="Македонски" data-language-local-name="makedonski" class="interlanguage-link-target"><span>Македонски</span></a></li><li class="interlanguage-link interwiki-ms mw-list-item"><a href="https://ms.wikipedia.org/wiki/Cakera_terserak" title="Cakera terserak – malajski" lang="ms" hreflang="ms" data-title="Cakera terserak" data-language-autonym="Bahasa Melayu" data-language-local-name="malajski" class="interlanguage-link-target"><span>Bahasa Melayu</span></a></li><li class="interlanguage-link interwiki-nl mw-list-item"><a href="https://nl.wikipedia.org/wiki/Scattered_disk_object" title="Scattered disk object – nizozemski" lang="nl" hreflang="nl" data-title="Scattered disk object" data-language-autonym="Nederlands" data-language-local-name="nizozemski" class="interlanguage-link-target"><span>Nederlands</span></a></li><li class="interlanguage-link interwiki-nn mw-list-item"><a href="https://nn.wikipedia.org/wiki/Den_spreidde_skiva" title="Den spreidde skiva – norveški (Nynorsk)" lang="nn" hreflang="nn" data-title="Den spreidde skiva" data-language-autonym="Norsk nynorsk" data-language-local-name="norveški (Nynorsk)" class="interlanguage-link-target"><span>Norsk nynorsk</span></a></li><li class="interlanguage-link interwiki-no mw-list-item"><a href="https://no.wikipedia.org/wiki/Den_spredte_skiven" title="Den spredte skiven – norveški (Bokmal)" lang="nb" hreflang="nb" data-title="Den spredte skiven" data-language-autonym="Norsk bokmål" data-language-local-name="norveški (Bokmal)" class="interlanguage-link-target"><span>Norsk bokmål</span></a></li><li class="interlanguage-link interwiki-pl badge-Q17437796 badge-featuredarticle mw-list-item" title="istaknuti članak"><a href="https://pl.wikipedia.org/wiki/Dysk_rozproszony" title="Dysk rozproszony – poljski" lang="pl" hreflang="pl" data-title="Dysk rozproszony" data-language-autonym="Polski" data-language-local-name="poljski" class="interlanguage-link-target"><span>Polski</span></a></li><li class="interlanguage-link interwiki-pnb mw-list-item"><a href="https://pnb.wikipedia.org/wiki/%DA%A9%DA%BE%D9%84%D8%B1%DB%8C%D8%A7_%DA%86%DA%BE%D9%86%D8%A7" title="کھلریا چھنا – Western Punjabi" lang="pnb" hreflang="pnb" data-title="کھلریا چھنا" data-language-autonym="پنجابی" data-language-local-name="Western Punjabi" class="interlanguage-link-target"><span>پنجابی</span></a></li><li class="interlanguage-link interwiki-ps mw-list-item"><a href="https://ps.wikipedia.org/wiki/%D9%88%DB%8C%D8%B4%D9%84%DB%8C_%D8%AF%DB%8C%D8%B3%DA%A9" title="ویشلی دیسک – paštu" lang="ps" hreflang="ps" data-title="ویشلی دیسک" data-language-autonym="پښتو" data-language-local-name="paštu" class="interlanguage-link-target"><span>پښتو</span></a></li><li class="interlanguage-link interwiki-pt mw-list-item"><a href="https://pt.wikipedia.org/wiki/Disco_disperso" title="Disco disperso – portugalski" lang="pt" hreflang="pt" data-title="Disco disperso" data-language-autonym="Português" data-language-local-name="portugalski" class="interlanguage-link-target"><span>Português</span></a></li><li class="interlanguage-link interwiki-ro mw-list-item"><a href="https://ro.wikipedia.org/wiki/Discul_%C3%AEmpr%C4%83%C8%99tiat" title="Discul împrăștiat – rumunski" lang="ro" hreflang="ro" data-title="Discul împrăștiat" data-language-autonym="Română" data-language-local-name="rumunski" class="interlanguage-link-target"><span>Română</span></a></li><li class="interlanguage-link interwiki-ru mw-list-item"><a href="https://ru.wikipedia.org/wiki/%D0%A0%D0%B0%D1%81%D1%81%D0%B5%D1%8F%D0%BD%D0%BD%D1%8B%D0%B9_%D0%B4%D0%B8%D1%81%D0%BA" title="Рассеянный диск – ruski" lang="ru" hreflang="ru" data-title="Рассеянный диск" data-language-autonym="Русский" data-language-local-name="ruski" class="interlanguage-link-target"><span>Русский</span></a></li><li class="interlanguage-link interwiki-sh mw-list-item"><a href="https://sh.wikipedia.org/wiki/Rasejani_disk" title="Rasejani disk – srpskohrvatski" lang="sh" hreflang="sh" data-title="Rasejani disk" data-language-autonym="Srpskohrvatski / српскохрватски" data-language-local-name="srpskohrvatski" class="interlanguage-link-target"><span>Srpskohrvatski / српскохрватски</span></a></li><li class="interlanguage-link interwiki-simple mw-list-item"><a href="https://simple.wikipedia.org/wiki/Scattered_disc" title="Scattered disc – Simple English" lang="en-simple" hreflang="en-simple" data-title="Scattered disc" data-language-autonym="Simple English" data-language-local-name="Simple English" class="interlanguage-link-target"><span>Simple English</span></a></li><li class="interlanguage-link interwiki-sk mw-list-item"><a href="https://sk.wikipedia.org/wiki/Rozpt%C3%BDlen%C3%BD_disk" title="Rozptýlený disk – slovački" lang="sk" hreflang="sk" data-title="Rozptýlený disk" data-language-autonym="Slovenčina" data-language-local-name="slovački" class="interlanguage-link-target"><span>Slovenčina</span></a></li><li class="interlanguage-link interwiki-sl mw-list-item"><a href="https://sl.wikipedia.org/wiki/Razpr%C5%A1eni_disk" title="Razpršeni disk – slovenski" lang="sl" hreflang="sl" data-title="Razpršeni disk" data-language-autonym="Slovenščina" data-language-local-name="slovenski" class="interlanguage-link-target"><span>Slovenščina</span></a></li><li class="interlanguage-link interwiki-sr mw-list-item"><a href="https://sr.wikipedia.org/wiki/%D0%A0%D0%B0%D1%81%D0%B5%D1%98%D0%B0%D0%BD%D0%B8_%D0%B4%D0%B8%D1%81%D0%BA" title="Расејани диск – srpski" lang="sr" hreflang="sr" data-title="Расејани диск" data-language-autonym="Српски / srpski" data-language-local-name="srpski" class="interlanguage-link-target"><span>Српски / srpski</span></a></li><li class="interlanguage-link interwiki-sv mw-list-item"><a href="https://sv.wikipedia.org/wiki/Scattered_disc" title="Scattered disc – švedski" lang="sv" hreflang="sv" data-title="Scattered disc" data-language-autonym="Svenska" data-language-local-name="švedski" class="interlanguage-link-target"><span>Svenska</span></a></li><li class="interlanguage-link interwiki-th mw-list-item"><a href="https://th.wikipedia.org/wiki/%E0%B9%81%E0%B8%96%E0%B8%9A%E0%B8%AB%E0%B8%B4%E0%B8%99%E0%B8%81%E0%B8%A3%E0%B8%B0%E0%B8%88%E0%B8%B2%E0%B8%A2" title="แถบหินกระจาย – tajlandski" lang="th" hreflang="th" data-title="แถบหินกระจาย" data-language-autonym="ไทย" data-language-local-name="tajlandski" class="interlanguage-link-target"><span>ไทย</span></a></li><li class="interlanguage-link interwiki-tr mw-list-item"><a href="https://tr.wikipedia.org/wiki/Da%C4%9F%C4%B1n%C4%B1k_disk" title="Dağınık disk – turski" lang="tr" hreflang="tr" data-title="Dağınık disk" data-language-autonym="Türkçe" data-language-local-name="turski" class="interlanguage-link-target"><span>Türkçe</span></a></li><li class="interlanguage-link interwiki-tt mw-list-item"><a href="https://tt.wikipedia.org/wiki/%D0%A7%D3%99%D1%87%D0%B5%D0%BB%D0%B3%D3%99%D0%BD_%D0%B4%D0%B8%D1%81%D0%BA" title="Чәчелгән диск – tatarski" lang="tt" hreflang="tt" data-title="Чәчелгән диск" data-language-autonym="Татарча / tatarça" data-language-local-name="tatarski" class="interlanguage-link-target"><span>Татарча / tatarça</span></a></li><li class="interlanguage-link interwiki-uk mw-list-item"><a href="https://uk.wikipedia.org/wiki/%D0%A0%D0%BE%D0%B7%D1%81%D1%96%D1%8F%D0%BD%D0%B8%D0%B9_%D0%B4%D0%B8%D1%81%D0%BA" title="Розсіяний диск – ukrajinski" lang="uk" hreflang="uk" data-title="Розсіяний диск" data-language-autonym="Українська" data-language-local-name="ukrajinski" class="interlanguage-link-target"><span>Українська</span></a></li><li class="interlanguage-link interwiki-vi mw-list-item"><a href="https://vi.wikipedia.org/wiki/%C4%90%C4%A9a_ph%C3%A2n_t%C3%A1n" title="Đĩa phân tán – vijetnamski" lang="vi" hreflang="vi" data-title="Đĩa phân tán" data-language-autonym="Tiếng Việt" data-language-local-name="vijetnamski" class="interlanguage-link-target"><span>Tiếng Việt</span></a></li><li class="interlanguage-link interwiki-wuu mw-list-item"><a href="https://wuu.wikipedia.org/wiki/%E7%A6%BB%E6%95%A3%E7%9B%98" title="离散盘 – Wu kineski" lang="wuu" hreflang="wuu" data-title="离散盘" data-language-autonym="吴语" data-language-local-name="Wu kineski" class="interlanguage-link-target"><span>吴语</span></a></li><li class="interlanguage-link interwiki-xmf mw-list-item"><a href="https://xmf.wikipedia.org/wiki/%E1%83%9B%E1%83%9D%E1%83%A0%E1%83%A6%E1%83%95%E1%83%90%E1%83%A4%E1%83%98%E1%83%9A%E1%83%98_%E1%83%93%E1%83%98%E1%83%A1%E1%83%99%E1%83%98" title="მორღვაფილი დისკი – Mingrelian" lang="xmf" hreflang="xmf" data-title="მორღვაფილი დისკი" data-language-autonym="მარგალური" data-language-local-name="Mingrelian" class="interlanguage-link-target"><span>მარგალური</span></a></li><li class="interlanguage-link interwiki-zh mw-list-item"><a href="https://zh.wikipedia.org/wiki/%E9%9B%A2%E6%95%A3%E7%9B%A4" title="離散盤 – kineski" lang="zh" hreflang="zh" data-title="離散盤" data-language-autonym="中文" data-language-local-name="kineski" class="interlanguage-link-target"><span>中文</span></a></li><li class="interlanguage-link interwiki-zh-min-nan mw-list-item"><a href="https://zh-min-nan.wikipedia.org/wiki/S%C3%A0n-lo%C4%81n_%C3%AE%E2%81%BF-po%C3%A2%E2%81%BF" title="Sàn-loān îⁿ-poâⁿ – Minnan" lang="nan" hreflang="nan" data-title="Sàn-loān îⁿ-poâⁿ" data-language-autonym="閩南語 / Bân-lâm-gú" data-language-local-name="Minnan" class="interlanguage-link-target"><span>閩南語 / Bân-lâm-gú</span></a></li><li class="interlanguage-link interwiki-zh-yue mw-list-item"><a href="https://zh-yue.wikipedia.org/wiki/%E9%BB%83%E9%81%93%E9%9B%A2%E6%95%A3%E5%A4%A9%E9%AB%94" title="黃道離散天體 – kantonski" lang="yue" hreflang="yue" data-title="黃道離散天體" data-language-autonym="粵語" data-language-local-name="kantonski" class="interlanguage-link-target"><span>粵語</span></a></li> </ul> <div class="after-portlet after-portlet-lang"><span class="wb-langlinks-edit wb-langlinks-link"><a href="https://www.wikidata.org/wiki/Special:EntityPage/Q180380#sitelinks-wikipedia" title="Uredi međujezičke linkove" class="wbc-editpage">Uredi veze</a></span></div> </div> </div> </div> </header> <div class="vector-page-toolbar"> <div class="vector-page-toolbar-container"> <div id="left-navigation"> <nav aria-label="Imenski prostori"> <div id="p-associated-pages" class="vector-menu vector-menu-tabs mw-portlet mw-portlet-associated-pages" > <div class="vector-menu-content"> <ul class="vector-menu-content-list"> <li id="ca-nstab-main" class="selected vector-tab-noicon mw-list-item"><a href="/wiki/Raspr%C5%A1eni_disk" title="Prikaži stranicu sa sadržajem [c]" accesskey="c"><span>Stranica</span></a></li><li id="ca-talk" class="new vector-tab-noicon mw-list-item"><a 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id="contentSub"><div id="mw-content-subtitle"></div></div> <div id="mw-content-text" class="mw-body-content"><div class="mw-content-ltr mw-parser-output" lang="bs" dir="ltr"><figure typeof="mw:File/Thumb"><a href="/wiki/Datoteka:Eris_and_dysnomia2.jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/5b/Eris_and_dysnomia2.jpg/300px-Eris_and_dysnomia2.jpg" decoding="async" width="300" height="298" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/5/5b/Eris_and_dysnomia2.jpg 1.5x" data-file-width="386" data-file-height="384" /></a><figcaption><a href="/wiki/Erida_(patuljasta_planeta)" title="Erida (patuljasta planeta)">Erida</a>, najveći poznati objekat raspršenog diska (u sredini) i njegov mjesec <a href="/w/index.php?title=Dysnomia&action=edit&redlink=1" class="new" title="Dysnomia (stranica ne postoji)">Dysnomia</a> (lijevo od objekta)</figcaption></figure> <p><b>Raspršeni disk</b> ili <b>rasuti disk</b> (<a href="/wiki/Engleski_jezik" title="Engleski jezik">engleski</a>: <span lang="en"><i>scattered-disc objects</i></span>, SDO) jest udaljeni disk oko zvijezde u <a href="/wiki/Sun%C4%8Dev_sistem" title="Sunčev sistem">Sunčevom sistemu</a> koji je rijetko naseljen ledenim <a href="/w/index.php?title=Mala_tijela_Sun%C4%8Devig_sistema&action=edit&redlink=1" class="new" title="Mala tijela Sunčevig sistema (stranica ne postoji)">malim tijelima Sunčevog sistema</a>, koja su podskup šire porodice <a href="/wiki/Transneptunsko_tijelo" title="Transneptunsko tijelo">transneptunskih objekata</a>. Objekti rasutih diskova imaju orbitalne ekscentricitete u rasponu od 0,8, nagiba do 40° i perihelije veće od 30 astronomskih jedinica (4,5×109 km; 2,8×109 milja). Smatra se da su ove ekstremne orbite rezultat gravitacionog "rasipanja" <a href="/wiki/Plinoviti_div" title="Plinoviti div">plinovitih divova</a>, a objekti su i dalje podložni perturbaciji planete <a href="/wiki/Neptun" title="Neptun">Neptuna</a>. </p><p>Iako se najbliži objekti raspršenog diska približavaju <a href="/wiki/Sunce" title="Sunce">Suncu</a> na oko 30-35 AJ, njihove orbite mogu se protezati i dalje od 100 AJ. Ovo čini rasute objekte među najhladnijim i najudaljenijim objektima u Sunčevom sistemu.<sup id="cite_ref-1" class="reference"><a href="#cite_note-1"><span class="cite-bracket">[</span>1<span class="cite-bracket">]</span></a></sup> Unutrašnji dio raspršenog diska preklapa se s područjem orbitalnih objekata u obliku torusa koji se tradicionalno naziva <a href="/wiki/Kuiperov_pojas" title="Kuiperov pojas">Kuiperov pojas</a>,<sup id="cite_ref-Morbidelli2008_2-0" class="reference"><a href="#cite_note-Morbidelli2008-2"><span class="cite-bracket">[</span>2<span class="cite-bracket">]</span></a></sup> ali njegove vanjske granice sežu mnogo dalje od Sunca i dalje iznad i ispod ekliptike od samog Kuiperovog pojasa. </p><p>Zbog njegove nestabilne prirode, astronomi sada smatraju da je rasuti disk mjesto nastanka većine periodičnih kometa u Sunčevom sistemu, pri čemu su <a href="/wiki/Kentauri" title="Kentauri">kentauri</a>, populacija ledenih tijela između <a href="/wiki/Jupiter" title="Jupiter">Jupitera</a> i <a href="/wiki/Neptun" title="Neptun">Neptuna</a>, međufaza u migraciji objekta iz raspršenog diska u unutrašnji Sunčev sistem.<sup id="cite_ref-Horner2004a_3-0" class="reference"><a href="#cite_note-Horner2004a-3"><span class="cite-bracket">[</span>3<span class="cite-bracket">]</span></a></sup> Na kraju, perturbacije sa <a href="/wiki/Divovske_planete" title="Divovske planete">divovskih planeta</a> šalju takve objekte prema Suncu, pretvarajući ih u periodične komete. Smatra se da su mnogi objekti predloženog <a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortovog oblaka</a> nastali u rasutom disku. <a href="/wiki/Odvojeni_objekt" title="Odvojeni objekt">Odvojeni objekti</a> se ne razlikuju znacajno od rasutih diskova, a neki se, kao što je <a href="/w/index.php?title=Sedna&action=edit&redlink=1" class="new" title="Sedna (stranica ne postoji)">Sedna</a>, ponekad smatraju uključenima u ovu grupu. </p> <meta property="mw:PageProp/toc" /> <div class="mw-heading mw-heading2"><h2 id="Otkriće"><span id="Otkri.C4.87e"></span>Otkriće</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=1" title="Uredi odlomak "Otkriće"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=1" title="Edit section's source code: Otkriće"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <p>Tradicionalno, uređaji poput <a href="/w/index.php?title=Komparator_treptaja&action=edit&redlink=1" class="new" title="Komparator treptaja (stranica ne postoji)">komparatora treptaja</a> korišteni su u astronomiji za otkrivanje objekata u Sunčevom sistemu, jer bi se ovi objekti kretali između dvije ekspozicije - to je uključivalo dugotrajne korake poput ekspozicije i razvijanja fotografskih ploča ili filmova, a ljudi su zatim koristili komparator treptanja za ručno otkrivanje potencijalnih objekata. Tokom 1980-ih, upotreba kamera zasnovanih na <a href="/w/index.php?title=CCD_senzor&action=edit&redlink=1" class="new" title="CCD senzor (stranica ne postoji)">CCD</a>-u u teleskopima omogućila je direktnu proizvodnju elektronskih slika koje su se zatim mogle lako digitalizirati i prenijeti u digitalne slike. Budući da je CCD hvatao više svjetla od filma (oko 90% naspram 10% ulaznog svjetla) i da se treptanje sada moglo obaviti na podesivom kompjuterskom ekranu, istraživanja su omogućila veću propusnost. Rezultat je bio poplava novih otkrića: preko hiljadu <a href="/wiki/Transneptunsko_tijelo" title="Transneptunsko tijelo">transneptunskih objekata</a> je otkriveno između 1992. i 2006.<sup id="cite_ref-4" class="reference"><a href="#cite_note-4"><span class="cite-bracket">[</span>4<span class="cite-bracket">]</span></a></sup> </p><p>Prvi objekat rasutih diskova (SDO) koji je prepoznat kao takav bio je <a href="/w/index.php?title=TL66&action=edit&redlink=1" class="new" title="TL66 (stranica ne postoji)">TL<sub>66</sub></a> iz 1996.<sup id="cite_ref-5" class="reference"><a href="#cite_note-5"><span class="cite-bracket">[</span>5<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-Davies1_6-0" class="reference"><a href="#cite_note-Davies1-6"><span class="cite-bracket">[</span>6<span class="cite-bracket">]</span></a></sup> koji su prvobitno identifikovali astronomi sa sedištem u <a href="/w/index.php?title=Mauna_Kei&action=edit&redlink=1" class="new" title="Mauna Kei (stranica ne postoji)">Mauna Kei</a> na <a href="/wiki/Havaji" title="Havaji">Havajima</a> 1996. Još tri su identifikovana istim istraživanjem 1999: <a href="/w/index.php?title=1999_CV118&action=edit&redlink=1" class="new" title="1999 CV118 (stranica ne postoji)">1999 CV<sub>118</sub></a>, <a href="/w/index.php?title=1999_CY118&action=edit&redlink=1" class="new" title="1999 CY118 (stranica ne postoji)">1999 CY<sub>118</sub></a> i <a href="/w/index.php?title=1999_CF119&action=edit&redlink=1" class="new" title="1999 CF119 (stranica ne postoji)">1999 CF<sub>119</sub></a>.<sup id="cite_ref-jewitt2000_7-0" class="reference"><a href="#cite_note-jewitt2000-7"><span class="cite-bracket">[</span>7<span class="cite-bracket">]</span></a></sup> Prvi otkriveni objekat koji je trenutno klasifikovan kao SDO bio je <a href="/w/index.php?title=TL8&action=edit&redlink=1" class="new" title="TL8 (stranica ne postoji)">TL<sub>8</sub></a> iz 1995, koji je pronašao <a href="/w/index.php?title=Spacewatch&action=edit&redlink=1" class="new" title="Spacewatch (stranica ne postoji)">Spacewatch</a>.<sup id="cite_ref-8" class="reference"><a href="#cite_note-8"><span class="cite-bracket">[</span>8<span class="cite-bracket">]</span></a></sup> </p><p>Od 2011, identifikovano je preko 200 SDO-a,<sup id="cite_ref-MPC_9-0" class="reference"><a href="#cite_note-MPC-9"><span class="cite-bracket">[</span>9<span class="cite-bracket">]</span></a></sup> uključujući <a href="/w/index.php?title=G%C7%83k%C3%BAn%C7%81%CA%BCh%C3%B2md%C3%ADm%C3%A0&action=edit&redlink=1" class="new" title="Gǃkúnǁʼhòmdímà (stranica ne postoji)">Gǃkúnǁʼhòmdímà</a> (otkrili Schwamb, Brown i Rabinowitz), <a href="/w/index.php?title=Gonggong&action=edit&redlink=1" class="new" title="Gonggong (stranica ne postoji)">Gonggong</a> (Schwamb, Brown i Rabinowitz)<sup id="cite_ref-10" class="reference"><a href="#cite_note-10"><span class="cite-bracket">[</span>10<span class="cite-bracket">]</span></a></sup> 2002. <a href="/w/index.php?title=TC302&action=edit&redlink=1" class="new" title="TC302 (stranica ne postoji)">TC<sub>302</sub></a> (NEAT, Trujill i Rabinowitz),<sup id="cite_ref-11" class="reference"><a href="#cite_note-11"><span class="cite-bracket">[</span>11<span class="cite-bracket">]</span></a></sup> <a href="/w/index.php?title=Sedna&action=edit&redlink=1" class="new" title="Sedna (stranica ne postoji)">Sedna</a> (Brown, Trujillo i Rabinowitz)<sup id="cite_ref-12" class="reference"><a href="#cite_note-12"><span class="cite-bracket">[</span>12<span class="cite-bracket">]</span></a></sup> i <a href="/w/index.php?title=474640_Alicanto&action=edit&redlink=1" class="new" title="474640 Alicanto (stranica ne postoji)">474640 Alicanto</a> (<a href="/w/index.php?title=Deep_Ecliptic_Survey&action=edit&redlink=1" class="new" title="Deep Ecliptic Survey (stranica ne postoji)">Deep Ecliptic Survey</a>).<sup id="cite_ref-13" class="reference"><a href="#cite_note-13"><span class="cite-bracket">[</span>13<span class="cite-bracket">]</span></a></sup> Iako se pretpostavlja da je broj objekata u Kuiperovom pojasu i raspršenom, disku približno jednak, pristranost posmatranja zbog njihove veće udaljenosti znači da je do danas uočeno mnogo manje SDO.<sup id="cite_ref-dynam_14-0" class="reference"><a href="#cite_note-dynam-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="Podjele_transneptunskog_prostora">Podjele transneptunskog prostora</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=2" title="Uredi odlomak "Podjele transneptunskog prostora"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=2" title="Edit section's source code: Podjele transneptunskog prostora"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure typeof="mw:File/Thumb"><a href="/wiki/Datoteka:TheKuiperBelt_Projections_100AU_Classical_SDO.svg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/5/58/TheKuiperBelt_Projections_100AU_Classical_SDO.svg/210px-TheKuiperBelt_Projections_100AU_Classical_SDO.svg.png" decoding="async" width="210" height="210" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/5/58/TheKuiperBelt_Projections_100AU_Classical_SDO.svg/315px-TheKuiperBelt_Projections_100AU_Classical_SDO.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/5/58/TheKuiperBelt_Projections_100AU_Classical_SDO.svg/420px-TheKuiperBelt_Projections_100AU_Classical_SDO.svg.png 2x" data-file-width="480" data-file-height="480" /></a><figcaption>Ekscentricitet i nagib populacije Raspršenih diskova u poređenju sa <a href="/w/index.php?title=Klasi%C4%8Dni_objekti_Kuiperovog_pojasa&action=edit&redlink=1" class="new" title="Klasični objekti Kuiperovog pojasa (stranica ne postoji)">klasičnim</a> i 5:2 <a href="/w/index.php?title=Rezonantni_objekti_Kuiperovog_pojasa&action=edit&redlink=1" class="new" title="Rezonantni objekti Kuiperovog pojasa (stranica ne postoji)">rezonantnim objektima Kuiperovog pojasa</a></figcaption></figure> <p>Poznati transneptunski objekti se često dijele na dvije subpopulacije: <a href="/wiki/Kuiperov_pojas" title="Kuiperov pojas">Kuiperov pojas</a> i Raspršeni disk.<sup id="cite_ref-MorbidBrown_15-0" class="reference"><a href="#cite_note-MorbidBrown-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup> Pretpostavljena je hipoteza o trećem rezervoaru transneptunskih objekata, <a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortovom oblaku</a>, iako nisu izvršena nikakva potvrđena direktna zapažanja Oortovog oblaka.<sup id="cite_ref-Morbidelli2008_2-1" class="reference"><a href="#cite_note-Morbidelli2008-2"><span class="cite-bracket">[</span>2<span class="cite-bracket">]</span></a></sup> Neki istraživači dalje sugerišu prijelazni prostor između raspršenog diska i unutrašnjeg Oortovog oblaka, naseljen "odvojenim objektima".<sup id="cite_ref-gomes_16-0" class="reference"><a href="#cite_note-gomes-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading3"><h3 id="Raspršeni_disk_naspram_Kuiperovog_pojasa"><span id="Raspr.C5.A1eni_disk_naspram_Kuiperovog_pojasa"></span>Raspršeni disk naspram Kuiperovog pojasa</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=3" title="Uredi odlomak "Raspršeni disk naspram Kuiperovog pojasa"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=3" title="Edit section's source code: Raspršeni disk naspram Kuiperovog pojasa"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <p>Kuiperov pojas je relativno debeo torus (ili "krofna") prostora, koji se proteže od oko 30 do 50 AJ<sup id="cite_ref-17" class="reference"><a href="#cite_note-17"><span class="cite-bracket">[</span>17<span class="cite-bracket">]</span></a></sup> koji se sastoji od dvije glavne populacije objekata Kuiperovog pojasa (<a href="/wiki/Engleski_jezik" title="Engleski jezik">engleski</a>: <span lang="en"><i>Kuiper Belt Objects, KBOs</i></span>): <a href="/w/index.php?title=Klasi%C4%8Dni_objekti_Kuiperovog_pojasa&action=edit&redlink=1" class="new" title="Klasični objekti Kuiperovog pojasa (stranica ne postoji)">klasični objekti Kuiperovog pojasa</a> (ili "cubewanos" ), koji leže u orbitama koje Neptun ne dira, i <a href="/w/index.php?title=Rezonantni_objekti_Kuiperovog_pojasa&action=edit&redlink=1" class="new" title="Rezonantni objekti Kuiperovog pojasa (stranica ne postoji)">rezonantni objekti Kuiperovog pojasa</a>; one koje je Neptun zaključao u precizan orbitalni omjer kao što je 2:3 (objekat se okreće dvaput za svake tri Neptunove orbite) i 1:2 (objekat se okreće jednom za svake dvije Neptunove orbite). Ovi omjeri, zvani orbitalne rezonanse, omogućavaju KBO-ima da opstanu u regijama koje bi Neptunov gravitacijski uticaj inače rasčistio tokom trajanja Sunčevog sistema, budući da objekti nikada nisu dovoljno blizu Neptuna da bi se raspršili njegovom gravitacijom. Oni u rezonansi 2:3 poznati su kao "<a href="/wiki/Plutini" title="Plutini">plutini</a>", jer je <a href="/wiki/Pluton" title="Pluton">Pluton</a> najveći član njihove grupe, dok su oni u rezonanciji 1:2 poznati kao "twotinos". </p><p>Za razliku od Kuiperovog pojasa, populaciju raspršenih diskova može poremetiti Neptun.<sup id="cite_ref-dynam2_18-0" class="reference"><a href="#cite_note-dynam2-18"><span class="cite-bracket">[</span>18<span class="cite-bracket">]</span></a></sup> Objekti raspršenog diska dolaze u gravitacijski domet Neptuna na svom najbližem približavanju (~30 AJ), ali njihove najveće udaljenosti dostižu višestruko više.<sup id="cite_ref-gomes_16-1" class="reference"><a href="#cite_note-gomes-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> Tekuća istraživanja<sup id="cite_ref-horner2003_19-0" class="reference"><a href="#cite_note-horner2003-19"><span class="cite-bracket">[</span>19<span class="cite-bracket">]</span></a></sup> sugerišu da <a href="/wiki/Kentauri" title="Kentauri">kentauri</a>, klasa ledenih planetoida koji kruže između <a href="/wiki/Jupiter" title="Jupiter">Jupitera</a> i <a href="/wiki/Neptun" title="Neptun">Neptuna</a>, mogu jednostavno biti SDO koje je Neptun bacio u unutrašnje domete Sunčevog sistema, što ih čini "cis-neptunskim" umjesto transneptunskim razbacanim objektima.<sup id="cite_ref-20" class="reference"><a href="#cite_note-20"><span class="cite-bracket">[</span>20<span class="cite-bracket">]</span></a></sup> Neki objekti, poput <a href="/w/index.php?title=(29981)_1999_TD10&action=edit&redlink=1" class="new" title="(29981) 1999 TD10 (stranica ne postoji)">(29981) 1999 TD<sub>10</sub></a>, zamagljuju razliku,<sup id="cite_ref-21" class="reference"><a href="#cite_note-21"><span class="cite-bracket">[</span>21<span class="cite-bracket">]</span></a></sup> a <a href="/wiki/Centar_za_male_planete" title="Centar za male planete">Centar za male planete</a> (MPC), koji službeno katalogizira sve transneptunske objekte, sada zajedno navodi kentaure i SDO.<sup id="cite_ref-MPC_9-1" class="reference"><a href="#cite_note-MPC-9"><span class="cite-bracket">[</span>9<span class="cite-bracket">]</span></a></sup> </p><p>MPC, međutim, pravi jasnu razliku između Kuiperovog pojasa i Raspršenog diska, odvajajući te objekte u stabilnim orbitama (Kuiperov pojas) od onih u rasutim orbitama (Raspršeni disk i Kentauri).<sup id="cite_ref-MPC_9-2" class="reference"><a href="#cite_note-MPC-9"><span class="cite-bracket">[</span>9<span class="cite-bracket">]</span></a></sup> Međutim, razlika između Kuiperovog pojasa i Raspršenog diska nije jasna i mnogi astronomi ne vide rasuti disk kao zasebnu populaciju već kao spoljašnji region Kajperovog pojasa. Drugi termin koji se koristi je "razbacani objekt Kuiperovog pojasa" (ili SKBO) za tijela rasutog diska.<sup id="cite_ref-22" class="reference"><a href="#cite_note-22"><span class="cite-bracket">[</span>22<span class="cite-bracket">]</span></a></sup> </p><p>Morbidelli i Brown predlažu da je razlika između objekata u Kuiperovom pojasu i objekata rasutih diskova u tome što se potonja tijela "prenose u velikoj poluosi bliskim i udaljenim susretima s Neptunom",<sup id="cite_ref-MorbidBrown_15-1" class="reference"><a href="#cite_note-MorbidBrown-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup> ali prva nisu iskusila tako bliske susreti. Ovo razgraničenje je neadekvatno (kako oni primjećuju) u odnosu na starost Sunčevog sistema, budući da tijela "zarobljena u rezonansama" mogu "preći iz faze raspršenja u fazu ne-raspršenja (i obrnuto) više puta."<sup id="cite_ref-MorbidBrown_15-2" class="reference"><a href="#cite_note-MorbidBrown-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup> transneptunski objekti bi mogli da putuju naprijed-nazad između Kuiperovog pojasa i rasutog diska tokom vremena. Stoga su umjesto objekata odabrali da definišu regije, a ne objekte, definirajući rasuti disk kao "područje orbitalnog prostora koje mogu posjetiti tijela koja su naišla na Neptun" unutar radijusa <a href="/w/index.php?title=Hill_sfera&action=edit&redlink=1" class="new" title="Hill sfera (stranica ne postoji)">Hill sfere</a>, a Kuiperov pojas kao njegov "komplement ... u a > 30 AU regiji"; region Sunčevog sistema naseljen objektima sa velikim poluosama većim od 30 AJ.<sup id="cite_ref-MorbidBrown_15-3" class="reference"><a href="#cite_note-MorbidBrown-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading3"><h3 id="Odvojeni_objekti">Odvojeni objekti</h3><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=4" title="Uredi odlomak "Odvojeni objekti"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=4" title="Edit section's source code: Odvojeni objekti"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <p><a href="/wiki/Centar_za_male_planete" title="Centar za male planete">Centar za male planete</a> klasifikuje transneptunski objekat <a href="/w/index.php?title=90377_Sedna&action=edit&redlink=1" class="new" title="90377 Sedna (stranica ne postoji)">90377 Sedna</a> kao objekat raspršenog diska. Njegov pronalazač <a href="/w/index.php?title=Michael_E._Brown&action=edit&redlink=1" class="new" title="Michael E. Brown (stranica ne postoji)">Michael E. Brown</a> predložio je umjesto toga da ga treba smatrati unutrašnjim objektom <a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortovog oblaka</a>, a ne članom <a class="mw-selflink selflink">raspršenog diska</a>, jer je, s perihelijskom udaljenosti od 76 AJ, previše udaljen da bi bio pod utjecajem gravitacijske privlačnosti. vanjskih planeta.<sup id="cite_ref-Sedna_23-0" class="reference"><a href="#cite_note-Sedna-23"><span class="cite-bracket">[</span>23<span class="cite-bracket">]</span></a></sup> Prema ovoj definiciji, objekat sa perihelom većim od 40 AJ može se klasifikovati kao izvan raspršenog diska.<sup id="cite_ref-Kobe_24-0" class="reference"><a href="#cite_note-Kobe-24"><span class="cite-bracket">[</span>24<span class="cite-bracket">]</span></a></sup> </p><p>Sedna nije jedini takav objekt: <a href="/w/index.php?title=(148209)_2000_CR105&action=edit&redlink=1" class="new" title="(148209) 2000 CR105 (stranica ne postoji)">(148209) 2000 CR<sub>105</sub></a> (otkriven prije Sedne) i <a href="/w/index.php?title=474640_Alicanto&action=edit&redlink=1" class="new" title="474640 Alicanto (stranica ne postoji)">474640 Alicanto</a> imaju perihel koji je previše udaljen od Neptuna da bi na njih mogao utjecati. To je dovelo do rasprave među astronomima o novom skupu malih planeta, nazvanom prošireni rasuti disk (E-SDO).<sup id="cite_ref-25" class="reference"><a href="#cite_note-25"><span class="cite-bracket">[</span>25<span class="cite-bracket">]</span></a></sup> <a href="/w/index.php?title=2000_CR105&action=edit&redlink=1" class="new" title="2000 CR105 (stranica ne postoji)">2000 CR<sub>105</sub></a> može biti i unutrašnji Oortov oblak ili (vjerovatnije) prelazni objekat između raspršenog diska i unutrašnjeg Oortovog oblaka. U skorije vrijeme, ovi objekti su se nazivali "razdvojeni",<sup id="cite_ref-Jewitt2006_26-0" class="reference"><a href="#cite_note-Jewitt2006-26"><span class="cite-bracket">[</span>26<span class="cite-bracket">]</span></a></sup> ili <a href="/w/index.php?title=Udaljeni_odvojeni_objekti&action=edit&redlink=1" class="new" title="Udaljeni odvojeni objekti (stranica ne postoji)">udaljeni odvojeni objekti</a> (<a href="/wiki/Engleski_jezik" title="Engleski jezik">engleski</a>: <span lang="en"><i>Distant Detached Objects, DDO</i></span>).<sup id="cite_ref-Gomez_2006_27-0" class="reference"><a href="#cite_note-Gomez_2006-27"><span class="cite-bracket">[</span>27<span class="cite-bracket">]</span></a></sup> </p><p>Ne postoje jasne granice između raspršenih i odvojenih regija.<sup id="cite_ref-Kobe_24-1" class="reference"><a href="#cite_note-Kobe-24"><span class="cite-bracket">[</span>24<span class="cite-bracket">]</span></a></sup> Gomes i drugi definišu SDO-ove kao one koji imaju "visoko ekscentrične orbite, perihelije iza Neptuna i polu-velike ose izvan rezonanse 1:2." Prema ovoj definiciji, svi udaljeni odvojeni objekti su SDO.<sup id="cite_ref-gomes_16-2" class="reference"><a href="#cite_note-gomes-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> Pošto se orbite odvojenih objekata ne mogu proizvesti rasijavanjem Neptuna, predloženi su alternativni mehanizmi sijanja, uključujući zvijezdu u prolazu<sup id="cite_ref-Morbidelli2004_28-0" class="reference"><a href="#cite_note-Morbidelli2004-28"><span class="cite-bracket">[</span>28<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-29" class="reference"><a href="#cite_note-29"><span class="cite-bracket">[</span>29<span class="cite-bracket">]</span></a></sup> ili udaljeni objekat veličine planete.[28] Alternativno, sugerisano je da su ovi objekti uhvaćeni sa <a href="/wiki/Zvijezda" title="Zvijezda">zvijezde</a> u prolazu.<sup id="cite_ref-Gomez_2006_27-1" class="reference"><a href="#cite_note-Gomez_2006-27"><span class="cite-bracket">[</span>27<span class="cite-bracket">]</span></a></sup> </p><p>Šema koju je uveo izvještaj iz 2005. iz <a href="/w/index.php?title=Deep_Ecliptic_Survey&action=edit&redlink=1" class="new" title="Deep Ecliptic Survey (stranica ne postoji)">Deep Ecliptic Survey</a> J. L. Elliott i drugi razlikuje dvije kategorije: raspršeni-blizu (tj. tipični SDO) i raspršeni-prošireni (tj. odvojeni objekti).<sup id="cite_ref-DES_Elliot2006_30-0" class="reference"><a href="#cite_note-DES_Elliot2006-30"><span class="cite-bracket">[</span>30<span class="cite-bracket">]</span></a></sup> Objekti u blizini raspršenih su oni čije su orbite nerezonantne, ne-planetarne orbite koje se ukrštaju i imaju <a href="/w/index.php?title=Tisserandov_parametar&action=edit&redlink=1" class="new" title="Tisserandov parametar (stranica ne postoji)">Tisserandov parametar</a> (u odnosu na Neptun) manji od 3.<sup id="cite_ref-DES_Elliot2006_30-1" class="reference"><a href="#cite_note-DES_Elliot2006-30"><span class="cite-bracket">[</span>30<span class="cite-bracket">]</span></a></sup> Objekti raspršenog proširenja imaju Tisserandov parametar (u odnosu na Neptun) veći od 3 i imaju vremenski prosječni ekscentricitet veći od 0,2.<sup id="cite_ref-DES_Elliot2006_30-2" class="reference"><a href="#cite_note-DES_Elliot2006-30"><span class="cite-bracket">[</span>30<span class="cite-bracket">]</span></a></sup> </p><p>Alternativna klasifikacija, koju su uveli B. J. Gladman, B. G. Marsden i C. Van Laerhoven 2007, koristi integraciju orbite od 10 miliona godina umjesto Tisserandovog parametra.<sup id="cite_ref-ArizonaBook_Gladman2007_31-0" class="reference"><a href="#cite_note-ArizonaBook_Gladman2007-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup> Objekat se kvalifikuje kao SDO ako njegova orbita nije rezonantna, ima veliku poluosu ne veću od 2000 AJ, i, tokom integracije, njegova velika poluosa pokazuje ekskurziju od 1,5 AJ ili više.<sup id="cite_ref-ArizonaBook_Gladman2007_31-1" class="reference"><a href="#cite_note-ArizonaBook_Gladman2007-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup> Gladman i drugi predlažu termin raspršujući disk objekt da bi se naglasila ova današnja mobilnost.<sup id="cite_ref-ArizonaBook_Gladman2007_31-2" class="reference"><a href="#cite_note-ArizonaBook_Gladman2007-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup> Ako objekt nije SDO prema gornjoj definiciji, ali je ekscentricitet njegove orbite veći od 0,240, on se klasifikuje kao odvojeni TNO.<sup id="cite_ref-ArizonaBook_Gladman2007_31-3" class="reference"><a href="#cite_note-ArizonaBook_Gladman2007-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup> (Objekti sa manjim ekscentricitetom smatraju se klasičnim.) U ovoj šemi, disk se proteže od orbite Neptuna do 2000 AJ, regije koji se naziva unutrašnji Oortov oblak. </p> <div class="mw-heading mw-heading2"><h2 id="Orbite">Orbite</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=5" title="Uredi odlomak "Orbite"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=5" title="Edit section's source code: Orbite"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure class="mw-halign-right" typeof="mw:File/Thumb"><a href="/wiki/Datoteka:KBOs_and_resonances.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/05/KBOs_and_resonances.png/660px-KBOs_and_resonances.png" decoding="async" width="660" height="288" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/05/KBOs_and_resonances.png/990px-KBOs_and_resonances.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/05/KBOs_and_resonances.png/1320px-KBOs_and_resonances.png 2x" data-file-width="13860" data-file-height="6044" /></a><figcaption>Distribucija <a href="/wiki/Transneptunsko_tijelo" title="Transneptunsko tijelo">transneptunskih objekata</a>, sa velikom poluosom na horizontalnoj i nagibom na vertikalnoj osi. Objekti Raspršenog diska su prikazani sivom bojom, objekti koji su u rezonansi sa Neptunom crvenom bojom. <a href="/wiki/Klasi%C4%8Dni_objekt_Kuiperovog_pojasa" title="Klasični objekt Kuiperovog pojasa">Klasični objekt Kuiperovog pojasa</a> (cubewanos) i sednoidi su plavi, odnosno žuti..</figcaption></figure> <p>Raspršeni disk je vrlo dinamično okruženje.<sup id="cite_ref-dynam_14-1" class="reference"><a href="#cite_note-dynam-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup> Budući da ih <a href="/wiki/Neptun" title="Neptun">Neptun</a> još uvijek može poremetiti, orbite SDO-a su uvijek u opasnosti od poremećaja; bilo da bude poslani van u <a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortov oblak</a> ili unutra u populaciju <a href="/wiki/Kentauri" title="Kentauri">kentaura</a> i na kraju u Jupiterovu porodicu kometa.<sup id="cite_ref-dynam_14-2" class="reference"><a href="#cite_note-dynam-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup> Iz tog razloga Gladman i drugi radije nazivaju regiju diskom za raspršivanje, a ne raspršenim.<sup id="cite_ref-ArizonaBook_Gladman2007_31-4" class="reference"><a href="#cite_note-ArizonaBook_Gladman2007-31"><span class="cite-bracket">[</span>31<span class="cite-bracket">]</span></a></sup> Za razliku od objekata <a href="/wiki/Kuiperov_pojas" title="Kuiperov pojas">Kuiperovog pojasa</a> (KBO), orbite objekata raspršenih diskova mogu biti nagnuti do 40° od <a href="/wiki/Ekliptika" title="Ekliptika">ekliptike</a>.<sup id="cite_ref-Bertoldi_Altenhoff_et_al._2006_32-0" class="reference"><a href="#cite_note-Bertoldi_Altenhoff_et_al._2006-32"><span class="cite-bracket">[</span>32<span class="cite-bracket">]</span></a></sup> </p><p>SDO su tipično okarakterizirane orbitama sa srednjim i visokim <a href="/wiki/Ekscentricitet" title="Ekscentricitet">ekscentricitetima</a> sa velikom poluosom većom od 50 AJ, ali njihova <a href="/wiki/Perihel" title="Perihel">perihelija</a> ih dovodi pod utjecaj Neptuna.<sup id="cite_ref-tjl2000_33-0" class="reference"><a href="#cite_note-tjl2000-33"><span class="cite-bracket">[</span>33<span class="cite-bracket">]</span></a></sup> Imati perihel od otprilike 30 AJ je jedna od definišnih karakteristika raspršenih objekata, jer omogućava Neptunu da izvrši svoj gravitacijski uticaj.<sup id="cite_ref-jewitt2000_7-1" class="reference"><a href="#cite_note-jewitt2000-7"><span class="cite-bracket">[</span>7<span class="cite-bracket">]</span></a></sup> </p><p>Klasični objekti (<a href="/wiki/Klasi%C4%8Dni_objekt_Kuiperovog_pojasa" title="Klasični objekt Kuiperovog pojasa">cubewano</a>) se veoma razlikuju od raspršenih objekata: više od 30% svih cubewano je na niskim nagibima, skoro kružnim orbitama čiji ekscentriciteti dostižu maksimum od 0,25.<sup id="cite_ref-Levison2003_34-0" class="reference"><a href="#cite_note-Levison2003-34"><span class="cite-bracket">[</span>34<span class="cite-bracket">]</span></a></sup> Klasični predmeti posjeduju ekscentricitete u rasponu od 0,2 do 0,8. Iako su nagibi raspršenih objekata slični ekstremnijim KBO-ovima, vrlo mali broj rasutih objekata ima orbite tako bliže ekliptici kao i većina KBO populacije.<sup id="cite_ref-dynam_14-3" class="reference"><a href="#cite_note-dynam-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup> </p><p>Iako su kretanja u rasutom disku nasumična, oni imaju tendenciju da slijede slične smjerove, što znači da SDO mogu postati zarobljeni u privremenim rezonancijama s Neptunom. Primjeri mogućih rezonantnih orbita unutar raspršenog diska uključuju 1:3, 2:7, 3:11, 5:22 i 4:79.<sup id="cite_ref-gomes_16-3" class="reference"><a href="#cite_note-gomes-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="Formiranje">Formiranje</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=6" title="Uredi odlomak "Formiranje"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=6" title="Edit section's source code: Formiranje"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure typeof="mw:File/Thumb"><a href="/wiki/Datoteka:Lhborbits.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Lhborbits.png/400px-Lhborbits.png" decoding="async" width="400" height="134" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Lhborbits.png/600px-Lhborbits.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Lhborbits.png/800px-Lhborbits.png 2x" data-file-width="1360" data-file-height="454" /></a><figcaption>Simulacija koja prikazuje vanjske planete i Kuiperov pojas: a) Prije rezonanse Jupiter/Saturn 2:1 b) Rasipanje objekata Kuiperovog pojasa u Sunčev sistem nakon orbitalnog pomaka Neptuna c) Nakon izbacivanja tijela Kuiperovog pojasa od strane Jupitera</figcaption></figure> <p>Raspršeni disk je još uvijek slabo shvaćen: još uvijek nije predložen model formiranja Kuiperovog pojasa i raspršenog diska koji bi objasnio sva njihova uočena svojstva.<sup id="cite_ref-MorbidBrown_15-4" class="reference"><a href="#cite_note-MorbidBrown-15"><span class="cite-bracket">[</span>15<span class="cite-bracket">]</span></a></sup> </p><p>Prema savremenim modelima, raspršeni disk je nastao kada su objekti iz Kuiperovog pojasa (KBO) bili "raspršeni" u ekscentrične i nagnute orbite gravitacionom interakcijom sa Neptunom i drugim vanjskim planetama.<sup id="cite_ref-Duncan_Levison_1997_35-0" class="reference"><a href="#cite_note-Duncan_Levison_1997-35"><span class="cite-bracket">[</span>35<span class="cite-bracket">]</span></a></sup> Količina vremena za ovaj proces ostaje neizvjesna. Jedna hipoteza procjenjuje period jednak cijeloj starosti <a href="/wiki/Sun%C4%8Dev_sistem" title="Sunčev sistem">Sunčevog sistema</a>;<sup id="cite_ref-36" class="reference"><a href="#cite_note-36"><span class="cite-bracket">[</span>36<span class="cite-bracket">]</span></a></sup> druga pretpostavlja da se raspršivanje dogodilo relativno brzo, tokom Neptunove rane epohe migracije.<sup id="cite_ref-shuffle_37-0" class="reference"><a href="#cite_note-shuffle-37"><span class="cite-bracket">[</span>37<span class="cite-bracket">]</span></a></sup> </p><p>Modeli za kontinuirano formiranje kroz doba Sunčevog sistema ilustriraju da pri slabim rezonansama unutar Kuiperovog pojasa (kao što je 5:7 ili 8:1), ili na granicama jačih rezonansi, objekti mogu razviti slabe orbitalne nestabilnosti tokom miliona godina. Rezonansa 4:7 posebno ima veliku nestabilnost. KBO se također mogu pomjeriti u nestabilne orbite bliskim prolaskom masivnih objekata ili sudarima. Tokom vremena, raspršeni disk bi se postepeno formirao od ovih izolovanih događaja.<sup id="cite_ref-gomes_16-4" class="reference"><a href="#cite_note-gomes-16"><span class="cite-bracket">[</span>16<span class="cite-bracket">]</span></a></sup> </p><p>Računarske simulacije su također sugerisale brže i ranije formiranje raspršenog diska. Moderne teorije pokazuju da se ni <a href="/wiki/Uran" title="Uran">Uran</a> ni <a href="/wiki/Neptun" title="Neptun">Neptun</a> nisu mogli formirati <a href="/wiki/In_situ" title="In situ">in situ</a> izvan <a href="/wiki/Saturn" title="Saturn">Saturna</a>, jer je na tom rasponu postojalo premalo primordijalne materije da bi proizvela objekte tako velike mase. Umjesto toga, ove planete i Saturn su se možda formirali bliže <a href="/wiki/Jupiter" title="Jupiter">Jupiteru</a>, ali su odbačeni vani tokom rane evolucije Sunčevog sistema, možda kroz razmjenu ugaonog momenta sa raspršenim objektima.<sup id="cite_ref-migration_38-0" class="reference"><a href="#cite_note-migration-38"><span class="cite-bracket">[</span>38<span class="cite-bracket">]</span></a></sup> Jednom kada su se orbite Jupitera i Saturna pomaknule u rezonansu 2:1 (dvije orbite Jupitera za svaku orbitu Saturna), njihova kombinovana <a href="/wiki/Gravitacija" title="Gravitacija">gravitacijska sila</a> poremetila je orbite Urana i Neptuna, šaljući Neptun u privremeni "haos" proto-Kuipera pojasa.<sup id="cite_ref-shuffle_37-1" class="reference"><a href="#cite_note-shuffle-37"><span class="cite-bracket">[</span>37<span class="cite-bracket">]</span></a></sup> Kako je Neptun putovao prema van, raspršio je mnoge <a href="/wiki/Transneptunsko_tijelo" title="Transneptunsko tijelo">transneptunske objekte</a> u više i ekscentrične orbite.<sup id="cite_ref-Duncan_Levison_1997_35-1" class="reference"><a href="#cite_note-Duncan_Levison_1997-35"><span class="cite-bracket">[</span>35<span class="cite-bracket">]</span></a></sup><sup id="cite_ref-39" class="reference"><a href="#cite_note-39"><span class="cite-bracket">[</span>39<span class="cite-bracket">]</span></a></sup> Ovaj model navodi da je 90% ili više objekata u raspršenom disku možda "promovisano u ove ekscentrične orbite Neptunovim rezonansama tokom epohe migracije... [zbog toga] raspršeni disk možda nije toliko raspršen."<sup id="cite_ref-migration_38-1" class="reference"><a href="#cite_note-migration-38"><span class="cite-bracket">[</span>38<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="Sasr+tav"><span id="Sasr.2Btav"></span>Sasr+tav</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=7" title="Uredi odlomak "Sasr+tav"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=7" title="Edit section's source code: Sasr+tav"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure typeof="mw:File/Thumb"><a href="/wiki/Datoteka:2003_UB313_near-infrared_spectrum.png" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/2003_UB313_near-infrared_spectrum.png/200px-2003_UB313_near-infrared_spectrum.png" decoding="async" width="200" height="211" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/2003_UB313_near-infrared_spectrum.png/300px-2003_UB313_near-infrared_spectrum.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/d/d6/2003_UB313_near-infrared_spectrum.png/400px-2003_UB313_near-infrared_spectrum.png 2x" data-file-width="514" data-file-height="541" /></a><figcaption>Infracrveni spektri Eride i Plutona, naglašavajući njihove zajedničke linije apsorpcije metana</figcaption></figure> <p>Raštrkani objekti, kao i drugi transneptunski objekti, imaju malu gustoću i uglavnom se sastoje od smrznutih isparljivih materija kao što su <a href="/wiki/Voda" title="Voda">voda</a> i <a href="/wiki/Metan" title="Metan">metan</a>.<sup id="cite_ref-dynam3_40-0" class="reference"><a href="#cite_note-dynam3-40"><span class="cite-bracket">[</span>40<span class="cite-bracket">]</span></a></sup> Spektralna analiza odabranog Kuiperovog pojasa i raspršenih objekata otkrila je znakove sličnih spojeva. I Pluton i Erida, na primjer, pokazuju tragove metana.<sup id="cite_ref-methane_41-0" class="reference"><a href="#cite_note-methane-41"><span class="cite-bracket">[</span>41<span class="cite-bracket">]</span></a></sup> </p><p>Astronomi su prvobitno pretpostavili da će čitava transneptunska populacija pokazati sličnu crvenu boju površine, jer se mislilo da potječu iz istog područja i da su podvrgnuti istim fizičkim procesima.<sup id="cite_ref-dynam3_40-1" class="reference"><a href="#cite_note-dynam3-40"><span class="cite-bracket">[</span>40<span class="cite-bracket">]</span></a></sup> Konkretno, očekivalo se da će SDO imati velike količine površinskog metana, hemijski promijenjenog u <a href="/wiki/Tolini" title="Tolini">toline</a> sunčevom svjetlošću. Ovo bi apsorbiralo plavo svjetlo, stvarajući crvenkastu nijansu.<sup id="cite_ref-dynam3_40-2" class="reference"><a href="#cite_note-dynam3-40"><span class="cite-bracket">[</span>40<span class="cite-bracket">]</span></a></sup> Većina <a href="/w/index.php?title=Klasi%C4%8Dni_objekati_Kuiperovog_pojasa&action=edit&redlink=1" class="new" title="Klasični objekati Kuiperovog pojasa (stranica ne postoji)">klasičnih objekata</a> prikazuje ovu boju, ali raspršeni objekti ne; umjesto toga, imaju bijeli ili sivkasti izgled.<sup id="cite_ref-dynam3_40-3" class="reference"><a href="#cite_note-dynam3-40"><span class="cite-bracket">[</span>40<span class="cite-bracket">]</span></a></sup> </p><p>Jedno od objašnjenja je izloženost bijelih podzemnih slojeva udarima; drugi je da veća udaljenost raspršenih objekata od <a href="/wiki/Sunce" title="Sunce">Sunca</a> stvara gradijent kompozicije, analogan gradijentu sastava zemaljskih i plinovitih <a href="/wiki/Divovske_planete" title="Divovske planete">divovskih planeta</a>.<sup id="cite_ref-dynam3_40-4" class="reference"><a href="#cite_note-dynam3-40"><span class="cite-bracket">[</span>40<span class="cite-bracket">]</span></a></sup> <a href="/w/index.php?title=Michael_E._Brown&action=edit&redlink=1" class="new" title="Michael E. Brown (stranica ne postoji)">Michael E. Brown</a>, otkrivač raspršenog objekta <a href="/wiki/Erida_(patuljasta_planeta)" title="Erida (patuljasta planeta)">Erida</a>, sugeriše da bi njegova bljeđa boja mogla biti zato što je, na trenutnoj udaljenosti od Sunca, njegova atmosfera metana zaleđena na cijeloj površini, stvarajući sloj sjajnog bijelog leda debljine nekoliko centimetara. S druge strane, <a href="/wiki/Pluton" title="Pluton">Pluton</a> bi, budući da je bliži Suncu, bio dovoljno topao da bi se metan zaledio samo na hladnije regije s visokim albedom, ostavljajući regije sa niskim albedom prekrivene tolinom bez leda.<sup id="cite_ref-methane_41-1" class="reference"><a href="#cite_note-methane-41"><span class="cite-bracket">[</span>41<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="Komete">Komete</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=8" title="Uredi odlomak "Komete"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=8" title="Edit section's source code: Komete"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <figure class="mw-default-size" typeof="mw:File/Thumb"><a href="/wiki/Datoteka:Tempel_1_(PIA02127).jpg" class="mw-file-description"><img src="//upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Tempel_1_%28PIA02127%29.jpg/220px-Tempel_1_%28PIA02127%29.jpg" decoding="async" width="220" height="220" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Tempel_1_%28PIA02127%29.jpg/330px-Tempel_1_%28PIA02127%29.jpg 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/0/0f/Tempel_1_%28PIA02127%29.jpg/440px-Tempel_1_%28PIA02127%29.jpg 2x" data-file-width="500" data-file-height="500" /></a><figcaption><a href="/w/index.php?title=Tempel_1&action=edit&redlink=1" class="new" title="Tempel 1 (stranica ne postoji)">Tempel 1</a>, kometa porodice Jupiter</figcaption></figure> <p>U početku se smatralo da je Kuiperov pojas izvor <a href="/wiki/Kometa" title="Kometa">kometa</a> <a href="/wiki/Ekliptika" title="Ekliptika">ekliptike</a> <a href="/wiki/Sun%C4%8Dev_sistem" title="Sunčev sistem">Sunčevog sistema</a>. Međutim, studije regije od 1992. pokazale su da su orbite unutar Kuiperovog pojasa relativno stabilne i da ekliptičke komete potiču iz raspršenog diska, gdje su orbite općenito manje stabilne.<sup id="cite_ref-42" class="reference"><a href="#cite_note-42"><span class="cite-bracket">[</span>42<span class="cite-bracket">]</span></a></sup> </p><p>Komete se mogu slobodno podijeliti u dvije kategorije: kratkoperiodične i dugoperiodične – za koje se smatra da potječu iz <a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortovog oblaka</a>. Dvije glavne kategorije kratkoperiodičnih kometa su <a href="/w/index.php?title=Komete_Jupiterove_porodice&action=edit&redlink=1" class="new" title="Komete Jupiterove porodice (stranica ne postoji)">komete Jupiterove porodice</a> (JFC) i <a href="/w/index.php?title=Komete_Halleyjevog_tipa&action=edit&redlink=1" class="new" title="Komete Halleyjevog tipa (stranica ne postoji)">komete Halleyjevog tipa</a>.<sup id="cite_ref-dynam_14-4" class="reference"><a href="#cite_note-dynam-14"><span class="cite-bracket">[</span>14<span class="cite-bracket">]</span></a></sup> Smatra se da su komete Halley tipa, koje su nazvane po svom prototipu, <a href="/wiki/Halleyjeva_kometa" title="Halleyjeva kometa">Halleyjeva kometa</a>, nastale u Oortovom oblaku, ali da su uvučene u unutrašnji Sunčev sistem gravitacijom <a href="/wiki/Divovske_planete" title="Divovske planete">Divovskih planeta</a>,<sup id="cite_ref-matter_43-0" class="reference"><a href="#cite_note-matter-43"><span class="cite-bracket">[</span>43<span class="cite-bracket">]</span></a></sup> dok se smatra da su JFC da je nastao u raspršenom disku.<sup id="cite_ref-dynam2_18-1" class="reference"><a href="#cite_note-dynam2-18"><span class="cite-bracket">[</span>18<span class="cite-bracket">]</span></a></sup> Smatra se da su <a href="/wiki/Kentauri" title="Kentauri">kentauri</a> dinamički posredni stepen između raspršenog diska i porodice Jupiter.<sup id="cite_ref-horner2003_19-1" class="reference"><a href="#cite_note-horner2003-19"><span class="cite-bracket">[</span>19<span class="cite-bracket">]</span></a></sup> </p><p>Postoje mnoge razlike između SDO-a i JFC-a, iako su mnoge komete iz porodice Jupiter možda nastale u raspršenom disku. Iako kentauri dijele crvenkastu ili neutralnu boju s mnogim SDO, njihova jezgra su plava, što ukazuje na fundamentalnu hemijsku ili fizičku razliku.<sup id="cite_ref-matter_43-1" class="reference"><a href="#cite_note-matter-43"><span class="cite-bracket">[</span>43<span class="cite-bracket">]</span></a></sup> Jedna hipoteza je da se jezgra kometa ponovo pojavljuju na površini kako se približavaju Suncu pomoću podzemnih materijala koji naknadno zatrpavaju stariji materijal.<sup id="cite_ref-matter_43-2" class="reference"><a href="#cite_note-matter-43"><span class="cite-bracket">[</span>43<span class="cite-bracket">]</span></a></sup> </p> <div class="mw-heading mw-heading2"><h2 id="Reference">Reference</h2><span class="mw-editsection"><span class="mw-editsection-bracket">[</span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&veaction=edit&section=9" title="Uredi odlomak "Reference"" class="mw-editsection-visualeditor"><span>uredi</span></a><span class="mw-editsection-divider"> | </span><a href="/w/index.php?title=Raspr%C5%A1eni_disk&action=edit&section=9" title="Edit section's source code: Reference"><span>uredi izvor</span></a><span class="mw-editsection-bracket">]</span></span></div> <style data-mw-deduplicate="TemplateStyles:r3312388">.mw-parser-output .reflist{font-size:90%;margin-bottom:0.5em;list-style-type:decimal}.mw-parser-output .reflist .references{font-size:100%;margin-bottom:0;list-style-type:inherit}.mw-parser-output .reflist-columns-2{column-width:30em}.mw-parser-output .reflist-columns-3{column-width:25em}.mw-parser-output .reflist-columns{margin-top:0.3em}.mw-parser-output .reflist-columns ol{margin-top:0}.mw-parser-output .reflist-columns li{page-break-inside:avoid;break-inside:avoid-column}.mw-parser-output .reflist-upper-alpha{list-style-type:upper-alpha}.mw-parser-output .reflist-upper-roman{list-style-type:upper-roman}.mw-parser-output .reflist-lower-alpha{list-style-type:lower-alpha}.mw-parser-output .reflist-lower-greek{list-style-type:lower-greek}.mw-parser-output .reflist-lower-roman{list-style-type:lower-roman}</style><div class="reflist"> <div class="mw-references-wrap mw-references-columns"><ol class="references"> <li id="cite_note-1"><span class="mw-cite-backlink"><b><a href="#cite_ref-1">^</a></b></span> <span class="reference-text">Maggie Masetti. 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(October 16–18, 2005). <a rel="nofollow" class="external text" href="http://webarchive.loc.gov/all/20061012062457/http://www.ciw.edu/sheppard/pub/Sheppard06smallbodies.pdf">"Small Bodies in the Outer Solar System"</a> <span class="cs1-format">(PDF)</span>. <i>New Horizons in Astronomy: Frank N. Bash Symposium 2005</i>. Austin, Texas: Astronomical Society of the Pacific. str. 3–14. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/1-58381-220-2" title="Posebno:Knjižni izvori/1-58381-220-2"><bdi>1-58381-220-2</bdi></a>. Arhivirano s <a rel="nofollow" class="external text" href="http://www.ciw.edu/sheppard/pub/Sheppard06smallbodies.pdf">originala</a> <span class="cs1-format">(PDF)</span>, 12. 10. 2006<span class="reference-accessdate">. Pristupljeno 14. 8. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=conference&rft.atitle=Small+Bodies+in+the+Outer+Solar+System&rft.btitle=New+Horizons+in+Astronomy%3A+Frank+N.+Bash+Symposium+2005&rft.place=Austin%2C+Texas&rft.pages=3-14&rft.pub=Astronomical+Society+of+the+Pacific&rft.date=2005-10-16%2F2005-10-18&rft.isbn=1-58381-220-2&rft.aulast=Sheppard&rft.aufirst=Scott+S.&rft_id=http%3A%2F%2Fwww.ciw.edu%2Fsheppard%2Fpub%2FSheppard06smallbodies.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-5"><span class="mw-cite-backlink"><b><a href="#cite_ref-5">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFLuuMarsdenJewitt1997" class="citation journal cs1">Luu, Jane X.; Marsden, Brian G.; Jewitt, David C. (5. 6. 1997). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20070812095854/http://www.ifa.hawaii.edu/faculty/jewitt/papers/TL66_1996/TL66.pdf">"A new dynamical class of object in the outer Solar System"</a> <span class="cs1-format">(PDF)</span>. <i>Nature</i>. <b>387</b> (6633): 573–575. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/1997Natur.387..573L">1997Natur.387..573L</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2F42413">10.1038/42413</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4370529">4370529</a>. Arhivirano s <a rel="nofollow" class="external text" href="http://www2.ess.ucla.edu/~jewitt/papers/TL66_1996/TL66.pdf">originala</a> <span class="cs1-format">(PDF)</span>, 12. 8. 2007<span class="reference-accessdate">. Pristupljeno 2. 8. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=A+new+dynamical+class+of+object+in+the+outer+Solar+System&rft.volume=387&rft.issue=6633&rft.pages=573-575&rft.date=1997-06-05&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4370529%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1038%2F42413&rft_id=info%3Abibcode%2F1997Natur.387..573L&rft.aulast=Luu&rft.aufirst=Jane+X.&rft.au=Marsden%2C+Brian+G.&rft.au=Jewitt%2C+David+C.&rft_id=http%3A%2F%2Fwww2.ess.ucla.edu%2F~jewitt%2Fpapers%2FTL66_1996%2FTL66.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Davies1-6"><span class="mw-cite-backlink"><b><a href="#cite_ref-Davies1_6-0">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFDavies2001" class="citation book cs1">Davies, John Keith (2001). <span class="cs1-lock-registration" title="Potrebna besplatna registracija"><a rel="nofollow" class="external text" href="https://archive.org/details/beyondplutoexplo00davi/page/111"><i>Beyond Pluto: Exploring the Outer Limits of the Solar System</i></a></span>. Cambridge University Press. str. <a rel="nofollow" class="external text" href="https://archive.org/details/beyondplutoexplo00davi/page/111">111</a>. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/978-0-521-80019-8" title="Posebno:Knjižni izvori/978-0-521-80019-8"><bdi>978-0-521-80019-8</bdi></a><span class="reference-accessdate">. Pristupljeno 2. 7. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=book&rft.btitle=Beyond+Pluto%3A+Exploring+the+Outer+Limits+of+the+Solar+System&rft.pages=111&rft.pub=Cambridge+University+Press&rft.date=2001&rft.isbn=978-0-521-80019-8&rft.aulast=Davies&rft.aufirst=John+Keith&rft_id=https%3A%2F%2Farchive.org%2Fdetails%2Fbeyondplutoexplo00davi%2Fpage%2F111&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-jewitt2000-7"><span class="mw-cite-backlink">^ <a href="#cite_ref-jewitt2000_7-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-jewitt2000_7-1"><sup><i><b>b</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFJewitt2009" class="citation web cs1"><a href="/wiki/David_C._Jewitt" title="David C. Jewitt">Jewitt, David C.</a> (August 2009). <a rel="nofollow" class="external text" href="http://www2.ess.ucla.edu/~jewitt/kb/kb-scattered.html">"Scattered Kuiper Belt Objects (SKBOs)"</a>. Institute for Astronomy<span class="reference-accessdate">. Pristupljeno <span class="nowrap">2010-01-23</span></span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Scattered+Kuiper+Belt+Objects+%28SKBOs%29&rft.pub=Institute+for+Astronomy&rft.date=2009-08&rft.aulast=Jewitt&rft.aufirst=David+C.&rft_id=http%3A%2F%2Fwww2.ess.ucla.edu%2F~jewitt%2Fkb%2Fkb-scattered.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-8"><span class="mw-cite-backlink"><b><a href="#cite_ref-8">^</a></b></span> <span class="reference-text">Schmadel, Lutz D. (2003); <i>Dictionary of Minor Planet Names</i> (5th rev. and enlarged ed. edition). Berlin: Springer. Page 925 (Appendix 10). Also see McFadden, Lucy-Ann; Weissman, Paul & Johnson, Torrence (1999). <i>Encyclopedia of the Solar System</i>. San Diego: Academic Press. Page 218.</span> </li> <li id="cite_note-MPC-9"><span class="mw-cite-backlink">^ <a href="#cite_ref-MPC_9-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-MPC_9-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-MPC_9-2"><sup><i><b>c</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFIAU:_Minor_Planet_Center2011" class="citation web cs1">IAU: Minor Planet Center (3. 1. 2011). <a rel="nofollow" class="external text" href="http://www.minorplanetcenter.org/iau/lists/Centaurs.html">"List Of Centaurs and Scattered-Disk Objects"</a>. Central Bureau for Astronomical Telegrams, Harvard-Smithsonian Center for Astrophysics<span class="reference-accessdate">. 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Minor Planet Center<span class="reference-accessdate">. Pristupljeno 25. 10. 2010</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Discovery+Circumstances%3A+Numbered+Minor+Planets&rft.pub=Minor+Planet+Center&rft.date=2007-05-01&rft.au=Staff&rft_id=http%3A%2F%2Fwww.minorplanetcenter.org%2Fiau%2Flists%2FNumberedMPs.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-12"><span class="mw-cite-backlink"><b><a href="#cite_ref-12">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite class="citation web cs1"><a rel="nofollow" class="external text" href="http://www.minorplanetcenter.org/iau/lists/NumberedMPs090001.html">"Discovery Circumstances: Numbered Minor Planets (90001)-(95000)"</a>. Minor Planet Center<span class="reference-accessdate">. Pristupljeno 25. 10. 2010</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Discovery+Circumstances%3A+Numbered+Minor+Planets+%2890001%29-%2895000%29&rft.pub=Minor+Planet+Center&rft_id=http%3A%2F%2Fwww.minorplanetcenter.org%2Fiau%2Flists%2FNumberedMPs090001.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-13"><span class="mw-cite-backlink"><b><a href="#cite_ref-13">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFMarc_W._Buie2007" class="citation web cs1"><a href="/w/index.php?title=Marc_W._Buie&action=edit&redlink=1" class="new" title="Marc W. Buie (stranica ne postoji)">Marc W. Buie</a> (8. 11. 2007). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20100818145946/http://www.boulder.swri.edu/~buie/kbo/astrom/04VN112.html">"Orbit Fit and Astrometric record for 04VN112"</a>. SwRI (Space Science Department). Arhivirano s <a rel="nofollow" class="external text" href="http://www.boulder.swri.edu/~buie/kbo/astrom/04VN112.html">originala</a>, 18. 8. 2010<span class="reference-accessdate">. Pristupljeno 17. 7. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Orbit+Fit+and+Astrometric+record+for+04VN112&rft.pub=SwRI+%28Space+Science+Department%29&rft.date=2007-11-08&rft.au=Marc+W.+Buie&rft_id=http%3A%2F%2Fwww.boulder.swri.edu%2F~buie%2Fkbo%2Fastrom%2F04VN112.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-dynam-14"><span class="mw-cite-backlink">^ <a href="#cite_ref-dynam_14-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-dynam_14-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-dynam_14-2"><sup><i><b>c</b></i></sup></a> <a href="#cite_ref-dynam_14-3"><sup><i><b>d</b></i></sup></a> <a href="#cite_ref-dynam_14-4"><sup><i><b>e</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFLevisonDonnes2007" class="citation book cs1">Levison, Harold F.; Donnes, Luke (2007). <a rel="nofollow" class="external text" href="http://astropolis.pl/index.php?app=core">"Comet Populations and Cometary Dynamics"</a>. u Adams McFadden, Lucy Ann; Weissman, Paul Robert; Johnson, Torrence V. (ured.). <a rel="nofollow" class="external text" href="https://archive.org/details/encyclopediaofso0000unse_u6d1/page/575"><i>Encyclopedia of the Solar System</i></a> (2nd izd.). Amsterdam; Boston: Academic Press. str. <a rel="nofollow" class="external text" href="https://archive.org/details/encyclopediaofso0000unse_u6d1/page/575">575–588</a>. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/978-0-12-088589-3" title="Posebno:Knjižni izvori/978-0-12-088589-3"><bdi>978-0-12-088589-3</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Comet+Populations+and+Cometary+Dynamics&rft.btitle=Encyclopedia+of+the+Solar+System&rft.place=Amsterdam%3B+Boston&rft.pages=575-588&rft.edition=2nd&rft.pub=Academic+Press&rft.date=2007&rft.isbn=978-0-12-088589-3&rft.aulast=Levison&rft.aufirst=Harold+F.&rft.au=Donnes%2C+Luke&rft_id=http%3A%2F%2Fastropolis.pl%2Findex.php%3Fapp%3Dcore&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-MorbidBrown-15"><span class="mw-cite-backlink">^ <a href="#cite_ref-MorbidBrown_15-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-MorbidBrown_15-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-MorbidBrown_15-2"><sup><i><b>c</b></i></sup></a> <a href="#cite_ref-MorbidBrown_15-3"><sup><i><b>d</b></i></sup></a> <a href="#cite_ref-MorbidBrown_15-4"><sup><i><b>e</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFMorbidelliBrown2004" class="citation book cs1">Morbidelli, Alessandro; Brown, Michael E. (2004-11-01). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20090621084121/http://www.lpi.usra.edu/books/CometsII/7004.pdf">"The Kuiper Belt and the Primordial Evolution of the Solar System"</a> <span class="cs1-format">(PDF)</span>. u M. C. Festou; H. U. Keller; H. A. Weaver (ured.). <i>Comets II</i>. Tucson (AZ): University of Arizona Press. str. 175–91. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/978-0-8165-2450-1" title="Posebno:Knjižni izvori/978-0-8165-2450-1"><bdi>978-0-8165-2450-1</bdi></a>. <a href="/wiki/OCLC_(identifikator)" class="mw-redirect" title="OCLC (identifikator)">OCLC</a> <a rel="nofollow" class="external text" href="//www.worldcat.org/oclc/56755773">56755773</a>. Arhivirano s originala 2009-06-21<span class="reference-accessdate">. Pristupljeno <span class="nowrap">2008-07-27</span></span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=The+Kuiper+Belt+and+the+Primordial+Evolution+of+the+Solar+System&rft.btitle=Comets+II&rft.place=Tucson+%28AZ%29&rft.pages=175-91&rft.pub=University+of+Arizona+Press&rft.date=2004-11-01&rft_id=info%3Aoclcnum%2F56755773&rft.isbn=978-0-8165-2450-1&rft.aulast=Morbidelli&rft.aufirst=Alessandro&rft.au=Brown%2C+Michael+E.&rft_id=http%3A%2F%2Fwww.lpi.usra.edu%2Fbooks%2FCometsII%2F7004.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span><span class="cs1-maint citation-comment">CS1 održavanje: bot: nepoznat status originalnog URL-a (<a href="/wiki/Kategorija:CS1_odr%C5%BEavanje:_bot:_nepoznat_status_originalnog_URL-a" title="Kategorija:CS1 održavanje: bot: nepoznat status originalnog URL-a">link</a>)</span></span> </li> <li id="cite_note-gomes-16"><span class="mw-cite-backlink">^ <a href="#cite_ref-gomes_16-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-gomes_16-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-gomes_16-2"><sup><i><b>c</b></i></sup></a> <a href="#cite_ref-gomes_16-3"><sup><i><b>d</b></i></sup></a> <a href="#cite_ref-gomes_16-4"><sup><i><b>e</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFGomesFernandezGallardoBrunini2008" class="citation web cs1">Gomes, Rodney S.; Fernandez, Julio A.; Gallardo, Tabare; Brunini, Adrian (2008). <a rel="nofollow" class="external text" href="http://www.fisica.edu.uy/~gallardo/scatdisk.pdf">"The Scattered Disk: Origins, Dynamics and End States"</a> <span class="cs1-format">(PDF)</span>. <i>Universidad de la Republica, Uruguay</i><span class="reference-accessdate">. Pristupljeno 10. 8. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=Universidad+de+la+Republica%2C+Uruguay&rft.atitle=The+Scattered+Disk%3A+Origins%2C+Dynamics+and+End+States&rft.date=2008&rft.aulast=Gomes&rft.aufirst=Rodney+S.&rft.au=Fernandez%2C+Julio+A.&rft.au=Gallardo%2C+Tabare&rft.au=Brunini%2C+Adrian&rft_id=http%3A%2F%2Fwww.fisica.edu.uy%2F~gallardo%2Fscatdisk.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-17"><span class="mw-cite-backlink"><b><a href="#cite_ref-17">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFDe_SanctisCapriaCoradini2001" class="citation journal cs1">De Sanctis, M. C.; Capria, M. T.; Coradini, A. (2001). <a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F320385">"Thermal Evolution and Differentiation of Edgeworth-Kuiper Belt Objects"</a>. <i>The Astronomical Journal</i>. <b>121</b> (5): 2792–2799. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2001AJ....121.2792D">2001AJ....121.2792D</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F320385">10.1086/320385</a></span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astronomical+Journal&rft.atitle=Thermal+Evolution+and+Differentiation+of+Edgeworth-Kuiper+Belt+Objects&rft.volume=121&rft.issue=5&rft.pages=2792-2799&rft.date=2001&rft_id=info%3Adoi%2F10.1086%2F320385&rft_id=info%3Abibcode%2F2001AJ....121.2792D&rft.aulast=De+Sanctis&rft.aufirst=M.+C.&rft.au=Capria%2C+M.+T.&rft.au=Coradini%2C+A.&rft_id=%2F%2Fdoi.org%2F10.1086%252F320385&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-dynam2-18"><span class="mw-cite-backlink">^ <a href="#cite_ref-dynam2_18-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-dynam2_18-1"><sup><i><b>b</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFMorbidelliLevison2007" class="citation book cs1">Morbidelli, Alessandro; Levison, Harold F. (2007). <a rel="nofollow" class="external text" href="https://archive.org/details/encyclopediaofso0000unse_u6d1/page/589">"Kuiper Belt Dynamics"</a>. u Lucy-Ann Adams McFadden; Paul Robert Weissman; Torrence V. Johnson (ured.). <i>Encyclopedia of the Solar System</i> (2nd izd.). Amsterdam; Boston: Academic Press. str. <a rel="nofollow" class="external text" href="https://archive.org/details/encyclopediaofso0000unse_u6d1/page/589">589–604</a>. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/978-0-12-088589-3" title="Posebno:Knjižni izvori/978-0-12-088589-3"><bdi>978-0-12-088589-3</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=Kuiper+Belt+Dynamics&rft.btitle=Encyclopedia+of+the+Solar+System&rft.place=Amsterdam%3B+Boston&rft.pages=589-604&rft.edition=2nd&rft.pub=Academic+Press&rft.date=2007&rft.isbn=978-0-12-088589-3&rft.aulast=Morbidelli&rft.aufirst=Alessandro&rft.au=Levison%2C+Harold+F.&rft_id=https%3A%2F%2Farchive.org%2Fdetails%2Fencyclopediaofso0000unse_u6d1%2Fpage%2F589&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-horner2003-19"><span class="mw-cite-backlink">^ <a href="#cite_ref-horner2003_19-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-horner2003_19-1"><sup><i><b>b</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFHornerEvansBaileyAsher2003" class="citation journal cs1">Horner, J.; Evans, N. W.; Bailey, Mark E.; Asher, D. J. (2003). "The Populations of Comet-like Bodies in the Solar System". <i>Monthly Notices of the Royal Astronomical Society</i>. <b>343</b> (4): 1057–1066. <a href="/w/index.php?title=ArXiv_(identifikator)&action=edit&redlink=1" class="new" title="ArXiv (identifikator) (stranica ne postoji)">arXiv</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="//arxiv.org/abs/astro-ph/0304319">astro-ph/0304319</a></span>. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2003MNRAS.343.1057H">2003MNRAS.343.1057H</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1046%2Fj.1365-8711.2003.06714.x">10.1046/j.1365-8711.2003.06714.x</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:2822011">2822011</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Monthly+Notices+of+the+Royal+Astronomical+Society&rft.atitle=The+Populations+of+Comet-like+Bodies+in+the+Solar+System&rft.volume=343&rft.issue=4&rft.pages=1057-1066&rft.date=2003&rft_id=info%3Aarxiv%2Fastro-ph%2F0304319&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A2822011%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1046%2Fj.1365-8711.2003.06714.x&rft_id=info%3Abibcode%2F2003MNRAS.343.1057H&rft.aulast=Horner&rft.aufirst=J.&rft.au=Evans%2C+N.+W.&rft.au=Bailey%2C+Mark+E.&rft.au=Asher%2C+D.+J.&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-20"><span class="mw-cite-backlink"><b><a href="#cite_ref-20">^</a></b></span> <span class="reference-text">Remo notes that Cis-Neptunian bodies "include terrestrial and large gaseous planets, planetary moons, asteroids, and main-belt comets within Neptune's orbit." (Remo 2007)</span> </li> <li id="cite_note-21"><span class="mw-cite-backlink"><b><a href="#cite_ref-21">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFSilber1999" class="citation web cs1">Silber, Kenneth (1999). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20050921034710/http://www.space.com/scienceastronomy/solarsystem/centaur_disc_991111.html">"New Object in Solar System Defies Categories"</a>. <i>space.com</i>. Arhivirano s <a rel="nofollow" class="external text" href="http://www.space.com/scienceastronomy/solarsystem/centaur_disc_991111.html">originala</a>, 21. 9. 2005<span class="reference-accessdate">. Pristupljeno 12. 8. 2008</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=space.com&rft.atitle=New+Object+in+Solar+System+Defies+Categories&rft.date=1999&rft.aulast=Silber&rft.aufirst=Kenneth&rft_id=http%3A%2F%2Fwww.space.com%2Fscienceastronomy%2Fsolarsystem%2Fcentaur_disc_991111.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-22"><span class="mw-cite-backlink"><b><a href="#cite_ref-22">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFJewitt2008" class="citation web cs1">Jewitt, David C. (2008). <a rel="nofollow" class="external text" href="http://www2.ess.ucla.edu/~jewitt/kb/big_kbo.html">"The 1000 km Scale KBOs"</a><span class="reference-accessdate">. Pristupljeno 23. 1. 2010</span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=The+1000+km+Scale+KBOs&rft.date=2008&rft.aulast=Jewitt&rft.aufirst=David+C.&rft_id=http%3A%2F%2Fwww2.ess.ucla.edu%2F~jewitt%2Fkb%2Fbig_kbo.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Sedna-23"><span class="mw-cite-backlink"><b><a href="#cite_ref-Sedna_23-0">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFBrown" class="citation web cs1">Brown, Michael E. <a rel="nofollow" class="external text" href="http://www.gps.caltech.edu/~mbrown/sedna/">"Sedna (The coldest most distant place known in the solar system; possibly the first object in the long-hypothesized Oort cloud)"</a>. California Institute of Technology, Department of Geological Sciences<span class="reference-accessdate">. Pristupljeno <span class="nowrap">2008-07-02</span></span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=unknown&rft.btitle=Sedna+%28The+coldest+most+distant+place+known+in+the+solar+system%3B+possibly+the+first+object+in+the+long-hypothesized+Oort+cloud%29&rft.pub=California+Institute+of+Technology%2C+Department+of+Geological+Sciences&rft.aulast=Brown&rft.aufirst=Michael+E.&rft_id=http%3A%2F%2Fwww.gps.caltech.edu%2F~mbrown%2Fsedna%2F&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Kobe-24"><span class="mw-cite-backlink">^ <a href="#cite_ref-Kobe_24-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-Kobe_24-1"><sup><i><b>b</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFLykawkaMukai2007" class="citation journal cs1">Lykawka, Patryk Sofia; Mukai, Tadashi (2007). "Dynamical classification of trans-Neptunian objects: Probing their origin, evolution, and interrelation". <i>Icarus</i>. Kobe. <b>189</b> (1): 213–232. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2007Icar..189..213L">2007Icar..189..213L</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2007.01.001">10.1016/j.icarus.2007.01.001</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=Dynamical+classification+of+trans-Neptunian+objects%3A+Probing+their+origin%2C+evolution%2C+and+interrelation&rft.volume=189&rft.issue=1&rft.pages=213-232&rft.date=2007&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2007.01.001&rft_id=info%3Abibcode%2F2007Icar..189..213L&rft.aulast=Lykawka&rft.aufirst=Patryk+Sofia&rft.au=Mukai%2C+Tadashi&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-25"><span class="mw-cite-backlink"><b><a href="#cite_ref-25">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFGladman" class="citation web cs1">Gladman, Brett J. <a rel="nofollow" class="external text" href="http://www.obs-nice.fr/gladman/cr105.html">"Evidence for an Extended Scattered Disk?"</a>. <i>Observatoire de la Cote d'Azur</i><span class="reference-accessdate">. Pristupljeno <span class="nowrap">2008-08-02</span></span>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=unknown&rft.jtitle=Observatoire+de+la+Cote+d%27Azur&rft.atitle=Evidence+for+an+Extended+Scattered+Disk%3F&rft.aulast=Gladman&rft.aufirst=Brett+J.&rft_id=http%3A%2F%2Fwww.obs-nice.fr%2Fgladman%2Fcr105.html&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Jewitt2006-26"><span class="mw-cite-backlink"><b><a href="#cite_ref-Jewitt2006_26-0">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFJewittDelsanti2006" class="citation book cs1"><a href="/wiki/David_C._Jewitt" title="David C. Jewitt">Jewitt, David C.</a>; Delsanti, A. (2006). "The Solar System Beyond The Planets". <a rel="nofollow" class="external text" href="http://www2.ess.ucla.edu/~jewitt/papers/2006/DJ06.pdf"><i>Solar System Update : Topical and Timely Reviews in Solar System Sciences</i></a> <span class="cs1-format">(PDF)</span>. Springer-Praxis Ed. <a href="/wiki/ISBN_(identifikator)" class="mw-redirect" title="ISBN (identifikator)">ISBN</a> <a href="/wiki/Posebno:Knji%C5%BEni_izvori/978-3-540-26056-1" title="Posebno:Knjižni izvori/978-3-540-26056-1"><bdi>978-3-540-26056-1</bdi></a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Abook&rft.genre=bookitem&rft.atitle=The+Solar+System+Beyond+The+Planets&rft.btitle=Solar+System+Update+%3A+Topical+and+Timely+Reviews+in+Solar+System+Sciences&rft.pub=Springer-Praxis+Ed.&rft.date=2006&rft.isbn=978-3-540-26056-1&rft.aulast=Jewitt&rft.aufirst=David+C.&rft.au=Delsanti%2C+A.&rft_id=http%3A%2F%2Fwww2.ess.ucla.edu%2F~jewitt%2Fpapers%2F2006%2FDJ06.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Gomez_2006-27"><span class="mw-cite-backlink">^ <a href="#cite_ref-Gomez_2006_27-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-Gomez_2006_27-1"><sup><i><b>b</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFGomesMateseLissauer2006" class="citation journal cs1">Gomes, Rodney S.; Matese, John J.; Lissauer, Jack J. (October 2006). "A distant planetary-mass solar companion may have produced distant detached objects". <i>Icarus</i>. <b>184</b> (2): 589–601. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2006Icar..184..589G">2006Icar..184..589G</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1016%2Fj.icarus.2006.05.026">10.1016/j.icarus.2006.05.026</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Icarus&rft.atitle=A+distant+planetary-mass+solar+companion+may+have+produced+distant+detached+objects&rft.volume=184&rft.issue=2&rft.pages=589-601&rft.date=2006-10&rft_id=info%3Adoi%2F10.1016%2Fj.icarus.2006.05.026&rft_id=info%3Abibcode%2F2006Icar..184..589G&rft.aulast=Gomes&rft.aufirst=Rodney+S.&rft.au=Matese%2C+John+J.&rft.au=Lissauer%2C+Jack+J.&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-Morbidelli2004-28"><span class="mw-cite-backlink"><b><a href="#cite_ref-Morbidelli2004_28-0">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFMorbidelliLevison2004" class="citation journal cs1">Morbidelli, Alessandro; Levison, Harold F. (November 2004). <a rel="nofollow" class="external text" href="https://archive.org/details/sim_astronomical-journal_2004-11_128_5/page/2564">"Scenarios for the Origin of the Orbits of the Trans-Neptunian Objects 2000 CR<sub>105</sub> and 2003 VB<sub>12</sub>"</a>. <i>The Astronomical Journal</i>. <b>128</b> (5): 2564–2576. <a href="/w/index.php?title=ArXiv_(identifikator)&action=edit&redlink=1" class="new" title="ArXiv (identifikator) (stranica ne postoji)">arXiv</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="//arxiv.org/abs/astro-ph/0403358">astro-ph/0403358</a></span>. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2004AJ....128.2564M">2004AJ....128.2564M</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F424617">10.1086/424617</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:119486916">119486916</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astronomical+Journal&rft.atitle=Scenarios+for+the+Origin+of+the+Orbits+of+the+Trans-Neptunian+Objects+2000+CR%3Csub%3E105%3C%2Fsub%3E+and+2003+VB%3Csub%3E12%3C%2Fsub%3E&rft.volume=128&rft.issue=5&rft.pages=2564-2576&rft.date=2004-11&rft_id=info%3Aarxiv%2Fastro-ph%2F0403358&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A119486916%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1086%2F424617&rft_id=info%3Abibcode%2F2004AJ....128.2564M&rft.aulast=Morbidelli&rft.aufirst=Alessandro&rft.au=Levison%2C+Harold+F.&rft_id=https%3A%2F%2Farchive.org%2Fdetails%2Fsim_astronomical-journal_2004-11_128_5%2Fpage%2F2564&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-29"><span class="mw-cite-backlink"><b><a href="#cite_ref-29">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFPfalznerBhandareVinckeLacerda2018" class="citation journal cs1">Pfalzner, Susanne; Bhandare, Asmita; Vincke, Kirsten; Lacerda, Pedro (2018-08-09). <a rel="nofollow" class="external text" href="https://doi.org/10.3847%2F1538-4357%2Faad23c">"Outer Solar System Possibly Shaped by a Stellar Fly-by"</a>. <i>The Astrophysical Journal</i>. <b>863</b> (1): 45. <a href="/w/index.php?title=ArXiv_(identifikator)&action=edit&redlink=1" class="new" title="ArXiv (identifikator) (stranica ne postoji)">arXiv</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="//arxiv.org/abs/1807.02960">1807.02960</a></span>. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2018ApJ...863...45P">2018ApJ...863...45P</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="https://doi.org/10.3847%2F1538-4357%2Faad23c">10.3847/1538-4357/aad23c</a></span>. <a href="/wiki/ISSN_(identifikator)" class="mw-redirect" title="ISSN (identifikator)">ISSN</a> <a rel="nofollow" class="external text" href="//www.worldcat.org/issn/1538-4357">1538-4357</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:119197960">119197960</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astrophysical+Journal&rft.atitle=Outer+Solar+System+Possibly+Shaped+by+a+Stellar+Fly-by&rft.volume=863&rft.issue=1&rft.pages=45&rft.date=2018-08-09&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A119197960%23id-name%3DS2CID&rft_id=info%3Abibcode%2F2018ApJ...863...45P&rft_id=info%3Aarxiv%2F1807.02960&rft.issn=1538-4357&rft_id=info%3Adoi%2F10.3847%2F1538-4357%2Faad23c&rft.aulast=Pfalzner&rft.aufirst=Susanne&rft.au=Bhandare%2C+Asmita&rft.au=Vincke%2C+Kirsten&rft.au=Lacerda%2C+Pedro&rft_id=%2F%2Fdoi.org%2F10.3847%252F1538-4357%252Faad23c&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-DES_Elliot2006-30"><span class="mw-cite-backlink">^ <a href="#cite_ref-DES_Elliot2006_30-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-DES_Elliot2006_30-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-DES_Elliot2006_30-2"><sup><i><b>c</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFElliotKernClancy2005" class="citation journal cs1">Elliot, J. 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Dynamical Classification, the Kuiper Belt Plane, and the Core Population"</a>. <i>The Astronomical Journal</i>. <b>129</b> (2): 1117–1162. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2005AJ....129.1117E">2005AJ....129.1117E</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<span class="cs1-lock-free" title="Slobodno dostupno"><a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F427395">10.1086/427395</a></span>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:19385887">19385887</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astronomical+Journal&rft.atitle=The+Deep+Ecliptic+Survey%3A+A+Search+for+Kuiper+Belt+Objects+and+Centaurs.+II.+Dynamical+Classification%2C+the+Kuiper+Belt+Plane%2C+and+the+Core+Population&rft.volume=129&rft.issue=2&rft.pages=1117-1162&rft.date=2005&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A19385887%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1086%2F427395&rft_id=info%3Abibcode%2F2005AJ....129.1117E&rft.aulast=Elliot&rft.aufirst=J.+L.&rft.au=Kern%2C+S.+D.&rft.au=Clancy%2C+K.+B.&rft_id=%2F%2Fdoi.org%2F10.1086%252F427395&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-ArizonaBook_Gladman2007-31"><span class="mw-cite-backlink">^ <a href="#cite_ref-ArizonaBook_Gladman2007_31-0"><sup><i><b>a</b></i></sup></a> <a href="#cite_ref-ArizonaBook_Gladman2007_31-1"><sup><i><b>b</b></i></sup></a> <a href="#cite_ref-ArizonaBook_Gladman2007_31-2"><sup><i><b>c</b></i></sup></a> <a href="#cite_ref-ArizonaBook_Gladman2007_31-3"><sup><i><b>d</b></i></sup></a> <a href="#cite_ref-ArizonaBook_Gladman2007_31-4"><sup><i><b>e</b></i></sup></a></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFGladmanMarsdenVan_Laerhoven2008" class="citation book cs1"><a href="/w/index.php?title=Brett_J._Gladman&action=edit&redlink=1" class="new" title="Brett J. 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(2 February 2006). <a rel="nofollow" class="external text" href="https://archive.org/details/sim_nature-uk_2006-02-02_439_7076/page/563">"The trans-Neptunian object <span class="nowrap">UB<sub>313</sub></span> is larger than Pluto"</a>. <i>Nature</i>. <b>439</b> (7076): 563–564. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2006Natur.439..563B">2006Natur.439..563B</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1038%2Fnature04494">10.1038/nature04494</a>. <a href="/wiki/PMID_(identifikator)" class="mw-redirect" title="PMID (identifikator)">PMID</a> <a rel="nofollow" class="external text" href="//pubmed.ncbi.nlm.nih.gov/16452973">16452973</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:4369483">4369483</a>.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=Nature&rft.atitle=The+trans-Neptunian+object+%3Cspan+class%3D%22nowrap%22%3EUB%3Csub%3E313%3C%2Fsub%3E%3C%2Fspan%3E+is+larger+than+Pluto&rft.volume=439&rft.issue=7076&rft.pages=563-564&rft.date=2006-02-02&rft_id=info%3Adoi%2F10.1038%2Fnature04494&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A4369483%23id-name%3DS2CID&rft_id=info%3Apmid%2F16452973&rft_id=info%3Abibcode%2F2006Natur.439..563B&rft.aulast=Bertoldi&rft.aufirst=F.&rft.au=Altenhoff%2C+W.&rft.au=Weiss%2C+A.&rft.au=Menten%2C+K.+M.&rft.au=Thum%2C+C.&rft_id=https%3A%2F%2Farchive.org%2Fdetails%2Fsim_nature-uk_2006-02-02_439_7076%2Fpage%2F563&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> <li id="cite_note-tjl2000-33"><span class="mw-cite-backlink"><b><a href="#cite_ref-tjl2000_33-0">^</a></b></span> <span class="reference-text"><link rel="mw-deduplicated-inline-style" href="mw-data:TemplateStyles:r3303350"><cite id="CITEREFTrujilloJewittLuu2000" class="citation journal cs1">Trujillo, Chadwick A.; <a href="/wiki/David_C._Jewitt" title="David C. 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(2001). <a rel="nofollow" class="external text" href="https://web.archive.org/web/20200503023241/http://pdfs.semanticscholar.org/9b63/4b7bf2b08f6bafae8bbe61fec60d36de6346.pdf">"From Kuiper Belt Object to Cometary Nucleus: The Missing Ultrared Matter"</a> <span class="cs1-format">(PDF)</span>. <i>The Astronomical Journal</i>. <b>123</b> (2): 1039–1049. <a href="/wiki/Bibcode_(identifikator)" class="mw-redirect" title="Bibcode (identifikator)">Bibcode</a>:<a rel="nofollow" class="external text" href="https://ui.adsabs.harvard.edu/abs/2002AJ....123.1039J">2002AJ....123.1039J</a>. <a href="/wiki/Doi_(identifikator)" class="mw-redirect" title="Doi (identifikator)">doi</a>:<a rel="nofollow" class="external text" href="https://doi.org/10.1086%2F338692">10.1086/338692</a>. <a href="/wiki/S2CID_(identifikator)" class="mw-redirect" title="S2CID (identifikator)">S2CID</a> <a rel="nofollow" class="external text" href="https://api.semanticscholar.org/CorpusID:122240711">122240711</a>. Arhivirano s <a rel="nofollow" class="external text" href="http://pdfs.semanticscholar.org/9b63/4b7bf2b08f6bafae8bbe61fec60d36de6346.pdf">originala</a> <span class="cs1-format">(PDF)</span>, 2020-05-03.</cite><span title="ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.jtitle=The+Astronomical+Journal&rft.atitle=From+Kuiper+Belt+Object+to+Cometary+Nucleus%3A+The+Missing+Ultrared+Matter&rft.volume=123&rft.issue=2&rft.pages=1039-1049&rft.date=2001&rft_id=https%3A%2F%2Fapi.semanticscholar.org%2FCorpusID%3A122240711%23id-name%3DS2CID&rft_id=info%3Adoi%2F10.1086%2F338692&rft_id=info%3Abibcode%2F2002AJ....123.1039J&rft.aulast=Jewitt&rft.aufirst=David+C.&rft_id=http%3A%2F%2Fpdfs.semanticscholar.org%2F9b63%2F4b7bf2b08f6bafae8bbe61fec60d36de6346.pdf&rfr_id=info%3Asid%2Fbs.wikipedia.org%3ARaspr%C5%A1eni+disk" class="Z3988"></span></span> </li> </ol></div></div> <div role="navigation" class="navbox" aria-labelledby="Sunčev_sistem" 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="navbox-title" colspan="2" style="text-align:center;"><style data-mw-deduplicate="TemplateStyles:r3312386">.mw-parser-output .navbar{display:inline;font-size:88%;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-mini abbr{font-variant:small-caps;border-bottom:none;text-decoration:none;cursor:inherit}.mw-parser-output .navbar-ct-full{font-size:114%;margin:0 7em}.mw-parser-output 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title="Uredi šablon" style="text-align:center;;;background:none transparent;border:none;box-shadow:none;padding:0;">u</abbr></a></li></ul></div><div id="Sunčev_sistem" style="font-size:114%;margin:0 4em"><a href="/wiki/Sun%C4%8Dev_sistem" title="Sunčev sistem">Sunčev sistem</a></div></th></tr><tr><td class="navbox-abovebelow" colspan="2" style="text-align:center;"><div id="*_Sunce_*_Merkur_*_Venera_*_Zemlja_*_Mars_*_Cerera_*_Jupiter_*_Saturn_*_Uran_*_Neptun_*_Pluton_*_Haumea_*_Makemake_*_Erida"><figure class="mw-default-size noresize" typeof="mw:File"><span><img src="//upload.wikimedia.org/wikipedia/commons/b/b8/Solar_System_Template_Final.png" decoding="async" width="666" height="36" class="mw-file-element" data-file-width="666" data-file-height="36" usemap="#ImageMap_17fe26ea7fa9c552" /></span><map name="ImageMap_17fe26ea7fa9c552"><area href="/wiki/Sunce" shape="rect" coords="0,0,90,35" alt="Sunce" title="Sunce" /><area href="/wiki/Merkur_(planeta)" shape="circle" coords="112,18,6" alt="Merkur" title="Merkur" /><area href="/wiki/Venera" shape="circle" coords="153,18,8" alt="Venera" title="Venera" /><area href="/wiki/Mjesec" shape="circle" coords="204,10,4" alt="Mjesec" title="Mjesec" /><area href="/wiki/Zemlja_(planeta)" shape="circle" coords="195,18,8" alt="Zemlja" title="Zemlja" /><area href="/wiki/Mars" shape="circle" coords="233,18,8" alt="Mars" title="Mars" /><area href="/wiki/Sateliti_Marsa" shape="circle" coords="241,13,3" alt="Fobos i Deimos" title="Fobos i Deimos" /><area href="/wiki/Asteroidni_pojas" shape="rect" coords="256,0,288,35" alt="Glavni asteroidni pojas" title="Glavni asteroidni pojas" /><area href="/wiki/Jupiter" shape="circle" coords="316,19,15" alt="Jupiter" title="Jupiter" /><area href="/wiki/Sateliti_Jupitera" shape="circle" coords="329,6,6" alt="Sateliti Jupitera" title="Sateliti Jupitera" /><area href="/wiki/Jupiterovi_prstenovi" shape="rect" coords="298,18,335,20" alt="Jupiterovi prstenovi" title="Jupiterovi prstenovi" /><area href="/wiki/Uran" shape="circle" coords="418,18,12" alt="Uran" title="Uran" /><area href="/wiki/Prirodni_sateliti_Urana" shape="circle" coords="427,10,6" alt="Prirodni sateliti Urana" title="Prirodni sateliti Urana" /><area href="/wiki/Uranovi_prstenovi" shape="rect" coords="408,4,429,34" alt="Uranovi prstenovi" title="Uranovi prstenovi" /><area href="/wiki/Neptun" shape="circle" coords="462,18,12" alt="Neptun" title="Neptun" /><area href="/wiki/Prirodni_sateliti_Neptune" shape="circle" coords="471,10,3" alt="Prirodni sateliti Neptune" title="Prirodni sateliti Neptune" /><area href="/wiki/Neptunovi_prstenovi" shape="rect" coords="441,9,485,28" alt="Neptunovi prstenovi" title="Neptunovi prstenovi" /><area href="/wiki/Pluton" shape="circle" coords="504,18,8" alt="Pluton" title="Pluton" /><area href="/wiki/Prirodni_sateliti_Plutona" shape="circle" coords="510,13,3" alt="Prirodni sateliti Plutona" title="Prirodni sateliti Plutona" /><area href="/wiki/Haumea" shape="circle" coords="534,18,8" alt="Haumea" title="Haumea" /><area href="/wiki/Prirodni_sateliti_Haumea" shape="circle" coords="540,13,3" alt="Prirodni sateliti Haumea" title="Prirodni sateliti Haumea" /><area href="/wiki/Makemake" shape="circle" coords="567,18,8" alt="Makemake" title="Makemake" /><area href="/wiki/Kuiperov_pojas" shape="rect" coords="490,0,580,35" alt="Kuiperov pojas" title="Kuiperov pojas" /><area href="/wiki/Eris_(patuljasta_planeta)" shape="circle" coords="596,18,8" alt="Eris" title="Eris" /><area href="/wiki/Dysnomia_(mjesec)" shape="circle" coords="602,13,3" alt="Dysnomia" title="Dysnomia" /><area href="/wiki/Raspr%C5%A1eni_disk" shape="rect" coords="581,0,610,35" alt="Raspršeni disk" title="Raspršeni disk" /><area href="/wiki/Hillsov_oblak" shape="rect" coords="623,0,640,35" alt="Hillsov oblak" title="Hillsov oblak" /><area href="/wiki/Oortov_oblak" shape="rect" coords="641,0,666,35" alt="Oortov oblak" title="Oortov oblak" /></map><figcaption></figcaption></figure> <ul><li><a href="/wiki/Sunce" title="Sunce">Sunce</a></li> <li><a href="/wiki/Merkur" title="Merkur">Merkur</a></li> <li><a href="/wiki/Venera" title="Venera">Venera</a></li> <li><a href="/wiki/Zemlja_(planeta)" title="Zemlja (planeta)">Zemlja</a></li> <li><a href="/wiki/Mars" title="Mars">Mars</a></li> <li><i><a href="/wiki/Cerera_(patuljasta_planeta)" title="Cerera (patuljasta planeta)">Cerera</a></i></li> <li><a href="/wiki/Jupiter" title="Jupiter">Jupiter</a></li> <li><a href="/wiki/Saturn" title="Saturn">Saturn</a></li> <li><a href="/wiki/Uran" title="Uran">Uran</a></li> <li><a href="/wiki/Neptun" title="Neptun">Neptun</a></li> <li><i><a href="/wiki/Pluton" title="Pluton">Pluton</a></i></li> <li><i><a href="/wiki/Haumea" title="Haumea">Haumea</a></i></li> <li><i><a href="/wiki/Makemake" title="Makemake">Makemake</a></i></li> <li><i><a href="/wiki/Erida_(patuljasta_planeta)" title="Erida (patuljasta planeta)">Erida</a></i></li></ul></div></td></tr><tr><td colspan="2" class="navbox-list navbox-odd" style="width:100%;padding:0px;background:transparent;color:inherit;"><div style="padding:0px;"><table cellspacing="0" class="navbox-columns-table" style="text-align:left;width:100%;"><tbody><tr style="vertical-align:top;"><td style="padding:0px;;;;width:50%;"><div> </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/Planet" class="mw-redirect" title="Planet">Planetarij</a></th><td class="navbox-list navbox-even" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/Dvostruka_planeta" title="Dvostruka planeta">Dvostruka planeta</a></li> <li><a href="/wiki/Patuljasta_planeta" title="Patuljasta planeta">Patuljasta planeta</a></li> <li><a href="/wiki/Divovske_planete" title="Divovske planete">Divovske planete</a></li> <li><a href="/wiki/Plinoviti_div" title="Plinoviti div">Plinoviti div</a></li> <li><a href="/wiki/Ledeni_div" title="Ledeni div">Ledeni div</a></li> <li><a href="/w/index.php?title=Planetarni_sistem&action=edit&redlink=1" class="new" title="Planetarni sistem (stranica ne postoji)">Planetarni sistem</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:center;"><a href="/wiki/Planetarni_prsten" title="Planetarni prsten">Prstenovi</a></th><td class="navbox-list navbox-odd" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=Jupiterovi_prsteni&action=edit&redlink=1" class="new" title="Jupiterovi prsteni (stranica ne postoji)">Jupiterovi</a></li> <li><a href="/wiki/Saturnovi_prstenovi" title="Saturnovi prstenovi">Saturnovi</a> <span style="font-size:90%;">(<a href="/w/index.php?title=Prstenovi_Rhea&action=edit&redlink=1" class="new" title="Prstenovi Rhea (stranica ne postoji)">Rhean</a>)</span></li> <li><a href="/w/index.php?title=Uranovi_prstenovi&action=edit&redlink=1" class="new" title="Uranovi prstenovi (stranica ne postoji)">Uranovi</a></li> <li><a href="/w/index.php?title=Neptunovi_prsteni&action=edit&redlink=1" class="new" title="Neptunovi prsteni (stranica ne postoji)">Neptunovi</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align:center;"><a href="/wiki/Prirodni_satelit" title="Prirodni satelit">Mjeseci</a></th><td class="navbox-list navbox-even" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/Mjesec_(satelit)" title="Mjesec (satelit)">Zemljin <span style="font-size:90%;">(Mjesec / <i>Luna</i></span></a></li> <li><span style="font-size:90%;"><a href="/w/index.php?title=Drugi_sateliti_Zemlje&action=edit&redlink=1" class="new" title="Drugi sateliti Zemlje (stranica ne postoji)">drugi)</a></span></li> <li><a href="/wiki/Marsovi_prirodni_sateliti" title="Marsovi prirodni sateliti">Marsovi</a></li> <li><a href="/wiki/Jupiterovi_prirodni_sateliti" title="Jupiterovi prirodni sateliti">Jupiterovi</a></li> <li><a href="/wiki/Saturnovi_prirodni_sateliti" title="Saturnovi prirodni sateliti">Saturnovi</a></li> <li><a href="/wiki/Uranovi_prirodni_sateliti" title="Uranovi prirodni sateliti">Uranovi</a></li> <li><a href="/wiki/Neptunovi_prirodni_sateliti" title="Neptunovi prirodni sateliti">Neptunovi</a></li> <li><a href="/wiki/Plutonovi_prirodni_sateliti" class="mw-redirect" title="Plutonovi prirodni sateliti">Plutonovi</a></li> <li><a href="/w/index.php?title=Sateliti_Haumea&action=edit&redlink=1" class="new" title="Sateliti Haumea (stranica ne postoji)">Haumea-e</a></li> <li><a href="/w/index.php?title=Dysnomia_(satelit)&action=edit&redlink=1" class="new" title="Dysnomia (satelit) (stranica ne postoji)">Eridian</a></li></ul> </div></td></tr></tbody></table><div> </div></td><td style="border-left:2px solid #fdfdfd;padding:0px;;;;width:50%;"><div> </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/Mala_tijela_Sun%C4%8Devog_sistema" title="Mala tijela Sunčevog sistema">SSSB</a></th><td class="navbox-list navbox-odd" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/wiki/Meteoroidi" title="Meteoroidi">Meteoroidi</a></li> <li><a href="/wiki/Male_planete" title="Male planete">Male planete</a></li> <li><a href="/wiki/Asteroidi" title="Asteroidi">Asteroidi</a></li> <li><a href="/wiki/Asteroidni_pojas" title="Asteroidni pojas">Asteroidni pojas</a></li> <li><a href="/wiki/Kentauri" title="Kentauri">Kentauri</a></li> <li><a href="/w/index.php?title=Trans-Neptunski_objekt&action=edit&redlink=1" class="new" title="Trans-Neptunski objekt (stranica ne postoji)">TNO</a></li> <li><a href="/wiki/Kuiperov_pojas" title="Kuiperov pojas">Kuiperov pojas</a></li> <li><a class="mw-selflink selflink">Raspršeni disk</a></li> <li><a href="/wiki/Kometa" title="Kometa">Komete</a></li> <li><a href="/wiki/Oortov_oblak" title="Oortov oblak">Oortov oblak</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align: center;">Spiskovi</th><td class="navbox-list navbox-even" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=Spisak_objekata_Sun%C4%8Devog_sistema&action=edit&redlink=1" class="new" title="Spisak objekata Sunčevog sistema (stranica ne postoji)">Objekti Sunčevog sistema</a> (<a href="/w/index.php?title=Spisak_objekata_Sun%C4%8Devog_sistema_po_veli%C4%8Dini&action=edit&redlink=1" class="new" title="Spisak objekata Sunčevog sistema po veličini (stranica ne postoji)">po veličini</a>)</li> <li><a href="/w/index.php?title=Spisak_malih_planeta&action=edit&redlink=1" class="new" title="Spisak malih planeta (stranica ne postoji)">Male planete</a></li></ul> </div></td></tr><tr><th scope="row" class="navbox-group" style="width:1%;text-align: center;"><span typeof="mw:File"><span title="Portal"><img alt="Portal" src="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/Portal-puzzle.svg/16px-Portal-puzzle.svg.png" decoding="async" width="16" height="14" class="mw-file-element" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/f/fd/Portal-puzzle.svg/24px-Portal-puzzle.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/f/fd/Portal-puzzle.svg/32px-Portal-puzzle.svg.png 2x" data-file-width="32" data-file-height="28" /></span></span> <a href="/wiki/Wikipedia:Portal" title="Wikipedia:Portal">Portali</a></th><td class="navbox-list navbox-odd" style="text-align:left;border-left-width:2px;border-left-style:solid;width:100%;padding:0px"><div style="padding:0em 0.25em"> <ul><li><a href="/w/index.php?title=Portal:Sun%C4%8Dev_sistem&action=edit&redlink=1" class="new" title="Portal:Sunčev sistem (stranica ne postoji)">Sunčev sistem</a></li> <li><a href="/wiki/Portal:Astronomija" title="Portal:Astronomija">Astronomija</a></li> <li><a href="/w/index.php?title=Portal:Prou%C4%8Davanje_Zemlje&action=edit&redlink=1" class="new" title="Portal:Proučavanje Zemlje (stranica ne postoji)">Proučavanje Zemlje</a></li> <li><a href="/w/index.php?title=Portal:Mars&action=edit&redlink=1" class="new" title="Portal:Mars (stranica ne postoji)">Mars</a></li> <li><a href="/w/index.php?title=Portal:Uran&action=edit&redlink=1" class="new" title="Portal:Uran (stranica ne postoji)">Uran</a></li> <li><a href="/w/index.php?title=Portal:Kosmologija&action=edit&redlink=1" class="new" title="Portal:Kosmologija (stranica ne postoji)">Kosmologija</a></li></ul> </div></td></tr></tbody></table><div> </div></td></tr></tbody></table></div></td></tr><tr><td class="navbox-abovebelow" colspan="2" style="text-align:center;;padding:0.4em;line-height:1.25em;"><div><a href="/wiki/Zemlja_(planeta)" title="Zemlja (planeta)">Zemlja</a> <span style="font-size:115%;">→</span> <a href="/wiki/Sun%C4%8Dev_sistem" title="Sunčev sistem">Sunčev sistem</a> <span style="font-size:115%;">→</span> <a href="/wiki/Lokalni_me%C4%91uzvjezdani_oblak" title="Lokalni međuzvjezdani oblak">Lokalni međuzvjezdani oblak</a> <span style="font-size:115%;">→</span> <a href="/wiki/Lokalni_mjehur" title="Lokalni mjehur">Lokalni mjehur</a> <span style="font-size:115%;">→</span> <a href="/wiki/Gouldov_pojas" title="Gouldov pojas">Gouldov pojas</a> <span style="font-size:115%;">→</span> <a href="/wiki/Orionova_ruka" title="Orionova ruka">Orionova ruka</a> <span style="font-size:115%;">→</span> <a href="/wiki/Mlije%C4%8Dni_put" title="Mliječni put">Mliječni put</a> <span 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