{"id":49581,"date":"2026-10-29T10:18:04","date_gmt":"2026-10-29T08:18:04","guid":{"rendered":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/10\/29\/gok-bilimciler-plutonun-otesinde-olasi-bir-cuce-gezegen-kesfetti\/"},"modified":"2026-10-29T10:18:04","modified_gmt":"2026-10-29T08:18:04","slug":"gok-bilimciler-plutonun-otesinde-olasi-bir-cuce-gezegen-kesfetti","status":"publish","type":"post","link":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/10\/29\/gok-bilimciler-plutonun-otesinde-olasi-bir-cuce-gezegen-kesfetti\/","title":{"rendered":"G\u00f6k bilimciler Pl\u00fcton&#039;un \u00f6tesinde olas\u0131 bir c\u00fcce gezegen ke\u015ffetti"},"content":{"rendered":"<p><\/p>\n<div>\n<p>&#13;<br \/>\n\tBu bulgu, \u015eili&#8217;de 2 bin 682 metre y\u00fcksekli\u011findeki bir da\u011f\u0131n zirvesinde yer alan ve d\u00fcnyan\u0131n en b\u00fcy\u00fck dijital kameras\u0131na ev sahipli\u011fi yapan yeni teleskop Vera C. Rubin G\u00f6zlemevi taraf\u0131ndan yap\u0131lan tespitlerin bir sonucu olarak ortaya \u00e7\u0131kt\u0131.<\/p>\n<p>&#13;<br \/>\n\tTeleskop 2025 y\u0131l\u0131nda faaliyete ge\u00e7ti ve her \u00fc\u00e7 g\u00fcnde bir t\u00fcm g\u00f6ky\u00fcz\u00fcn\u00fc g\u00f6r\u00fcnt\u00fcleyebiliyor.<\/p>\n<p>&#13;<br \/>\n\tSmithsonian&#8217;da k\u0131demli astrofizik\u00e7i ve Harvard \u00dcniversitesinde astronomi \u00f6\u011fretim g\u00f6revlisi olan Matthew Holman, Rubin taraf\u0131ndan 2026 y\u0131l\u0131n\u0131n ba\u015flar\u0131nda toplanan verileri taramak ve hareket eden nesnelere ait milyarlarca tespiti incelemek i\u00e7in ortakla\u015fa geli\u015ftirdi\u011fi bir bilgisayar program\u0131n\u0131 \u00e7al\u0131\u015ft\u0131rd\u0131.<\/p>\n<p>&#13;<br \/>\n\tED138 ortaya \u00e7\u0131kt\u0131\u011f\u0131nda ilk tepkisinin heyecanl\u0131 bir inan\u00e7s\u0131zl\u0131k oldu\u011funu s\u00f6yleyen Holman, bilgisayar program\u0131nda bir hata olup olmad\u0131\u011f\u0131n\u0131 hemen kontrol etti\u011fini belirtti.<\/p>\n<p>&#13;<br \/>\n\tG\u00f6zlemi do\u011frulamak i\u00e7in ayn\u0131 zamanda Rubin Operasyonlar\u0131 ekip \u00fcyesi olan Holman, Rubin G\u00fcne\u015f Sistemi ba\u015f bilim insan\u0131 ve Washington \u00dcniversitesi astronomi b\u00f6l\u00fcm\u00fcnde profes\u00f6r olan meslekta\u015f\u0131 Mario Juric ile birlikte \u00e7al\u0131\u015ft\u0131.<\/p>\n<p>&#13;<br \/>\n\tJuric, Rubin&#8217;in katalo\u011funda ED138 ile ilgili daha fazla g\u00f6zlem arad\u0131 ve mart 2026&#8217;ya kadar uzanan 20 ek g\u00f6zlem buldu. Sonunda ara\u015ft\u0131rmac\u0131lar, di\u011fer kaynaklar\u0131 kullanarak nesnenin y\u00f6r\u00fcngesini 10 y\u0131l geriye d\u00f6n\u00fck olarak \u00e7izmeyi ba\u015fard\u0131. Ancak Holman, ED138&#8217;in hen\u00fcz resmi olarak bir c\u00fcce gezegen olmad\u0131\u011f\u0131 konusunda uyararak \u015fu an i\u00e7in hala bir aday oldu\u011funu, fiziksel olarak ne kadar b\u00fcy\u00fck oldu\u011funu ger\u00e7ekten bilmeleri gerekti\u011fini ve bunun muhtemelen birka\u00e7 ay s\u00fcrece\u011fini s\u00f6yledi.<\/p>\n<h2>&#13;<br \/>\n\tED138&#8217;in \u00f6zellikleri ortaya \u00e7\u0131kt\u0131<\/h2>\n<p>&#13;<br \/>\n\tED138&#8217;in \u00e7ap\u0131n\u0131n 600 ile 1500 kilometre aras\u0131nda oldu\u011fu tahmin ediliyor. Bu boyut onu tan\u0131nan c\u00fcce gezegenlerin en k\u00fc\u00e7\u00fc\u011f\u00fc olan Ceres&#8217;ten daha b\u00fcy\u00fck yap\u0131yor. \u015eu anda g\u00fcne\u015fin etraf\u0131nda yakla\u015f\u0131k 46 astronomik birim mesafede d\u00f6n\u00fcyor. Her bir birim D\u00fcnya ile g\u00fcne\u015f aras\u0131ndaki ortalama mesafeyi temsil ediyor. Bu da ED138&#8217;in Pl\u00fcton&#8217;dan daha uzakta oldu\u011fu ve ayn\u0131 zamanda g\u00fcne\u015fin etraf\u0131nda Nept\u00fcn&#8217;den daha uzak bir mesafede d\u00f6nen nesne s\u0131n\u0131f\u0131 olan Nept\u00fcn \u00f6tesi bir nesne oldu\u011fu anlam\u0131na geliyor.<\/p>\n<p>&#13;<br \/>\n\tHolman&#8217;a g\u00f6re, gece g\u00f6ky\u00fcz\u00fcnde \u00e7\u0131plak g\u00f6zle g\u00f6r\u00fclemeyen ED138, nereye bakacaklar\u0131n\u0131 bildikleri takdirde ger\u00e7ekten yetenekli amat\u00f6rlerin g\u00f6rebilece\u011fi kadar parlak bir yap\u0131ya sahip.<\/p>\n<p>&#13;<br \/>\n\tHolman, bilim insanlar\u0131n\u0131n ED138&#8217;i daha \u00f6nce ke\u015ffetmemesinin nedenlerinden birinin g\u00fcney yar\u0131m k\u00fcrede bulunmas\u0131 ve bu nedenle kuzey yar\u0131m k\u00fcreden g\u00f6zlemlenmesinin \u00e7ok zor olmas\u0131 oldu\u011funu kaydetti. Bunun nesneyi bulabilecek t\u00fcm teleskop setlerini zaten eledi\u011fini ve g\u00fcney yar\u0131m k\u00fcrede g\u00f6ky\u00fcz\u00fcn\u00fc ara\u015ft\u0131ran \u00e7ok fazla teleskop bulunmad\u0131\u011f\u0131n\u0131 s\u00f6yledi.<\/p>\n<p>&#13;<br \/>\n\tED138&#8217;in gizli kalmas\u0131n\u0131 sa\u011flayan bir di\u011fer fakt\u00f6r ise galaksimizle ayn\u0131 d\u00fczlemde yer almas\u0131 oldu. Holman, nesnenin son 20 y\u0131ld\u0131r bizim bak\u0131\u015f a\u00e7\u0131m\u0131za g\u00f6re Samanyolu boyunca kendi yolunda ilerledi\u011fini a\u00e7\u0131klad\u0131. \u0130nsanlar\u0131n genellikle Samanyolu&#8217;nda bir \u015feyler aramad\u0131\u011f\u0131n\u0131, \u00e7\u00fcnk\u00fc hareket eden nesneleri bulman\u0131n \u00e7ok zor oldu\u011fu kadar \u00e7ok y\u0131ld\u0131z bulundu\u011funu belirtti.<\/p>\n<p>&#13;<br \/>\n\tYeni c\u00fcce gezegen aday\u0131, Rubin teleskobunun tespit etti\u011fi ve b\u00fcy\u00fck \u00f6l\u00e7\u00fcde asteroitler ile \u00e7ok daha k\u00fc\u00e7\u00fck Nept\u00fcn \u00f6tesi nesnelerden olu\u015fan b\u00fcy\u00fcyen listesine kat\u0131ld\u0131. Holman&#8217;a g\u00f6re, ED138 boyutlar\u0131nda birka\u00e7 nesne daha bulunabilir ve Rubin eninde sonunda onlar\u0131 da tespit edebilir.<\/p>\n<p>&#13;<br \/>\n\tBelfast Queen&#8217;s \u00dcniversitesinde astrofizik okutman\u0131 ve Rubin G\u00fcne\u015f Sistemi Operasyonlar\u0131 ekibi \u00fcyesi Megan Schwamb bir e-postada, Rubin G\u00f6zlemevinin g\u00fcne\u015f sistemini yeni derinliklere kadar envanterleyerek i\u015fini ger\u00e7ekten iyi yapt\u0131\u011f\u0131n\u0131 belirtti. Devreye alma g\u00f6zlemlerinin ba\u015flar\u0131nda b\u00f6yle bir nesne bulmas\u0131na \u015fa\u015f\u0131rd\u0131\u011f\u0131n\u0131 s\u00f6yleyen Schwamb, bunun bu y\u0131lki beklentileri aras\u0131nda olmad\u0131\u011f\u0131n\u0131 ifade etti. Schwamb, Rubin&#8217;in h\u0131z, derinlik ve g\u00f6ky\u00fcz\u00fc kapsam\u0131 kombinasyonunun \u00f6n\u00fcm\u00fczdeki on y\u0131lda ve \u00f6zellikle \u00f6n\u00fcm\u00fczdeki birka\u00e7 y\u0131l i\u00e7inde g\u00fcne\u015f sistemine bak\u0131\u015f a\u00e7\u0131m\u0131z\u0131 nas\u0131l de\u011fi\u015ftirece\u011fini g\u00f6sterdi\u011fini ekledi.<\/p>\n<h2>&#13;<br \/>\n\tBir d\u00fcnya olarak d\u00fc\u015f\u00fcn\u00fcn<\/h2>\n<p>&#13;<br \/>\n\tUluslararas\u0131 Astronomi Birli\u011fi 2006 y\u0131l\u0131nda g\u00fcne\u015fin etraf\u0131nda d\u00f6nen, \u00e7o\u011funlukla yuvarlak olan ve y\u00f6r\u00fcngesini benzer b\u00fcy\u00fckl\u00fckteki nesnelerden temizleyecek kadar b\u00fcy\u00fck olan bir nesne olarak tan\u0131mlad\u0131\u011f\u0131 yeni bir gezegen tan\u0131m\u0131n\u0131 kabul etti.<\/p>\n<p>&#13;<br \/>\n\tBilim insanlar\u0131, son \u015fart\u0131 yerine getirmedi\u011fi i\u00e7in Pl\u00fcton&#8217;un stat\u00fcs\u00fcn\u00fc d\u00fc\u015f\u00fcrme y\u00f6n\u00fcnde tart\u0131\u015fmal\u0131 bir karar ald\u0131 ve g\u00fcne\u015f sistemimiz dokuz gezegenden sekiz gezegene d\u00fc\u015ft\u00fc. Ayn\u0131 zamanda, Pl\u00fcton ve benzerleri, g\u00fcne\u015fin etraf\u0131nda d\u00f6nen ancak kendi y\u00f6r\u00fcngelerindeki enkaz\u0131 temizleyecek kadar b\u00fcy\u00fck olmayan neredeyse yuvarlak nesneler olan c\u00fcce gezegenler olarak bilinmeye ba\u015fland\u0131.<\/p>\n<p>&#13;<br \/>\n\tED138 yeni bir c\u00fcce gezegen olarak do\u011frulan\u0131rsa, g\u00f6k bilimciler ona \u00f6nce kal\u0131c\u0131 bir numara, ard\u0131ndan da ger\u00e7ek bir isim verecek. Ancak bu s\u00fcre\u00e7 zaman alabilir ve ismi tam olarak kimin se\u00e7ece\u011fine dair detaylar hen\u00fcz belirsizli\u011fini koruyor.<\/p>\n<p>&#13;<br \/>\n\t\u0130nsanlar\u0131n kendisine \u015fimdiden baz\u0131 \u00f6neriler e-postas\u0131 g\u00f6nderdi\u011fini ve bunlardan baz\u0131lar\u0131n\u0131n halihaz\u0131rda di\u011fer nesneler taraf\u0131ndan al\u0131nd\u0131\u011f\u0131n\u0131 s\u00f6yleyen Holman, s\u00fcrecin e\u011flenceli olaca\u011f\u0131n\u0131, kendisinin de bir \u015feyler \u00f6nerebilece\u011fini ancak bunun \u00e7ok b\u00fcy\u00fck bir proje oldu\u011fu i\u00e7in fazla umutlanmad\u0131\u011f\u0131n\u0131 belirtti.<\/p>\n<p>&#13;<br \/>\n\tED138&#8217;in ke\u015ffinde yer almayan Yeni Zelanda&#8217;daki Canterbury \u00dcniversitesi do\u00e7enti Michele Bannister, bulgunun kendi alanlar\u0131 i\u00e7in \u00f6nemli oldu\u011funu s\u00f6yledi. G\u00fcne\u015f sisteminin k\u00fc\u00e7\u00fck d\u00fcnyalar\u0131n\u0131 inceleyen Bannister, nesnenin Nept\u00fcn \u00f6tesi bir nesne olmas\u0131 ve fiziksel olarak olduk\u00e7a b\u00fcy\u00fck olmas\u0131na ra\u011fmen \u00e7\u0131plak g\u00f6zle g\u00f6r\u00fclemeyecek kadar s\u00f6n\u00fck kalmas\u0131 nedeniyle bilimsel olarak ger\u00e7ekten harika oldu\u011funu ifade etti.<\/p>\n<p>&#13;<br \/>\n\tNesnenin boyutunun tam da onun bir d\u00fcnya oldu\u011funu d\u00fc\u015f\u00fcnmeye ba\u015flayabilece\u011fimiz aral\u0131kta oldu\u011funu s\u00f6zlerine ekleyen Bannister, art\u0131k di\u011fer teleskoplar\u0131n da onun hakk\u0131nda daha fazla bilgi edinmek i\u00e7in bayra\u011f\u0131 devralaca\u011f\u0131n\u0131 belirtti.<\/p>\n<p>&#13;<br \/>\n\tBannister, oraya bir <a href=\"https:\/\/www.trthaber.com\/etiket\/uzay\/\" target=\"_blank\">uzay<\/a> arac\u0131 g\u00f6nderilmesi halinde Pl\u00fcton gibi bir nitrojen buzuluna sahip oldu\u011funun g\u00f6r\u00fclebilece\u011fini ve bunu g\u00f6rmenin harika olaca\u011f\u0131n\u0131 s\u00f6yledi. Bannister \u015fu anda tek bildiklerinin nesnenin b\u00fcy\u00fck oldu\u011fu y\u00f6n\u00fcnde oldu\u011funu, fiziksel \u00f6zelliklerinin ger\u00e7ekte ne oldu\u011fu hakk\u0131nda geri kalan her \u015feyin bir s\u00fcreli\u011fine spek\u00fclasyondan ibaret olaca\u011f\u0131n\u0131 kaydetti.<\/p>\n<\/p><\/div>\n","protected":false},"excerpt":{"rendered":"<p>&#13; Bu bulgu, \u015eili&#8217;de 2 bin 682 metre y\u00fcksekli\u011findeki bir da\u011f\u0131n zirvesinde yer alan ve d\u00fcnyan\u0131n en b\u00fcy\u00fck dijital kameras\u0131na ev sahipli\u011fi yapan yeni teleskop Vera C. Rubin G\u00f6zlemevi taraf\u0131ndan yap\u0131lan tespitlerin bir sonucu olarak ortaya \u00e7\u0131kt\u0131. &#13; Teleskop 2025 y\u0131l\u0131nda faaliyete ge\u00e7ti ve her \u00fc\u00e7 g\u00fcnde bir t\u00fcm g\u00f6ky\u00fcz\u00fcn\u00fc g\u00f6r\u00fcnt\u00fcleyebiliyor. &#13; Smithsonian&#8217;da k\u0131demli astrofizik\u00e7i [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":47028,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jnews-multi-image_gallery":[],"jnews_single_post":[],"jnews_primary_category":[],"jnews_social_meta":[],"jnews_override_counter":[],"footnotes":""},"categories":[2],"tags":[],"class_list":["post-49581","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v28.8 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>G\u00f6k bilimciler Pl\u00fcton&#039;un \u00f6tesinde olas\u0131 bir c\u00fcce gezegen ke\u015ffetti - Kuzeyin Sesi<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/kuzeyinsesi.org\/index.php\/2026\/10\/29\/gok-bilimciler-plutonun-otesinde-olasi-bir-cuce-gezegen-kesfetti\/\" \/>\n<meta property=\"og:locale\" content=\"tr_TR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"G\u00f6k bilimciler Pl\u00fcton&#039;un \u00f6tesinde olas\u0131 bir c\u00fcce gezegen ke\u015ffetti - Kuzeyin Sesi\" \/>\n<meta property=\"og:description\" content=\"&#013; Bu bulgu, \u015eili&#8217;de 2 bin 682 metre y\u00fcksekli\u011findeki bir da\u011f\u0131n zirvesinde yer alan ve d\u00fcnyan\u0131n en b\u00fcy\u00fck dijital kameras\u0131na ev sahipli\u011fi yapan yeni teleskop Vera C. 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