\n
\n\tLondra Queen Mary \u00dcniversitesinden ara\u015ft\u0131rmac\u0131lar, bir gezegenin geriye do\u011fru y\u00f6r\u00fcngesini belirlemeye yard\u0131mc\u0131 oldu. Bu ke\u015fif, gezegen sistemlerinin nas\u0131l olu\u015ftu\u011funa ve evrimle\u015fti\u011fine dair ipu\u00e7lar\u0131 sunabilir.<\/p>\n
\n\tBir y\u0131ld\u0131z ve gezegenleri d\u00f6nen ayn\u0131 gaz ve toz diskinden olu\u015ftu\u011funda, gezegenlerin y\u0131ld\u0131z\u0131n d\u00f6n\u00fc\u015f y\u00f6n\u00fcnde hareket etmesi bekleniyor.<\/p>\n
\n\tAncak g\u00f6k bilimciler, Nept\u00fcn b\u00fcy\u00fckl\u00fc\u011f\u00fcndeki GJ 3090 b gezegeninin y\u0131ld\u0131z\u0131n\u0131n etraf\u0131nda ters y\u00f6nde hareket etti\u011fini ke\u015ffetti.<\/p>\n
\n\tGezegenin ev sahibi olan M c\u00fccesi, galaksimizdeki y\u0131ld\u0131zlar\u0131n \u00e7o\u011funlu\u011funu olu\u015fturan k\u00fc\u00e7\u00fck ve so\u011fuk y\u0131ld\u0131zlardan biri olarak biliniyor. GJ 3090 b, bu t\u00fcr bir y\u0131ld\u0131z\u0131n etraf\u0131nda geriye do\u011fru y\u00f6r\u00fcnge izleyen bilinen ilk gezegen oldu.<\/p>\n
\n\tBu durum, gezegenin b\u00f6ylesine al\u0131\u015f\u0131lmad\u0131k bir rotay\u0131 nas\u0131l edindi\u011fine dair sorular\u0131 g\u00fcndeme getirdi.<\/p>\n
\n\tUluslararas\u0131 bir ekip, y\u00f6r\u00fcngenin \u00fc\u00e7 boyutlu y\u00f6nelimini \u00f6l\u00e7mek i\u00e7in \u0131\u015f\u0131\u011f\u0131 dalga boylar\u0131na ay\u0131ran bir ara\u00e7 olan yak\u0131n k\u0131z\u0131l\u00f6tesi spektrograf\u0131ndan (NIRPS) elde edilen y\u00fcksek \u00e7\u00f6z\u00fcn\u00fcrl\u00fckl\u00fc g\u00f6zlemleri kulland\u0131. Ekip, yakla\u015f\u0131k 136 derecelik bir y\u00f6r\u00fcnge e\u011fikli\u011fi hesaplad\u0131.<\/p>\n
\n\tY\u0131ld\u0131z\u0131n d\u00f6n\u00fc\u015f ekseni ile gezegenin y\u00f6r\u00fcnge ekseni aras\u0131ndaki bu a\u00e7\u0131, gezegenin geriye do\u011fru y\u00f6r\u00fcngede d\u00f6nd\u00fc\u011f\u00fcn\u00fc do\u011frulad\u0131.<\/p>\n
\n\tLondra Queen Mary \u00dcniversitesinden ara\u015ft\u0131rman\u0131n ba\u015fyazar\u0131 Dr. Andrew Winter, “Bu dikkat \u00e7ekici bir gezegen sistemi \u00e7\u00fcnk\u00fc gezegen sadece y\u0131ld\u0131z\u0131na g\u00f6re e\u011fik de\u011fil, ayn\u0131 zamanda ters y\u00f6nde y\u00f6r\u00fcngede d\u00f6n\u00fcyor. Bu durum, b\u00f6ylesine al\u0131\u015f\u0131lmad\u0131k bir y\u00f6r\u00fcngenin nas\u0131l olu\u015fmu\u015f olabilece\u011fi sorusunu hemen ak\u0131llara getiriyor” dedi.<\/p>\n
\n\tGeriye do\u011fru y\u00f6r\u00fcnge do\u011fu\u015ftan m\u0131 miras kald\u0131?<\/h2>\n
\n\tAstronomy & Astrophysics Letters dergisinde yay\u0131mlanan ara\u015ft\u0131rma, GJ 3090 b’nin al\u0131\u015f\u0131lmad\u0131k y\u00f6r\u00fcngesini y\u0131ld\u0131z\u0131n sistemin olu\u015fumunun erken d\u00f6nemlerinde edindi\u011fi materyalden miras al\u0131p almad\u0131\u011f\u0131n\u0131 inceliyor.<\/p>\n
\n\tCenevre \u00dcniversitesinden Dr. \u00d6\u011fretim \u00dcyesi Vincent Bourrier, “Bir gezegen sisteminin farkl\u0131 y\u00f6nelimli ikinci bir diskten yeniden in\u015fa edilebilece\u011fi fikri \u00f6zellikle heyecan verici. Bu, gen\u00e7 bir y\u0131ld\u0131z\u0131n etraf\u0131ndaki ortam\u0131n, gezegenlerinin mimarisini belirlemede bekledi\u011fimizden \u00e7ok daha b\u00fcy\u00fck bir rol oynayabilece\u011fini g\u00f6steriyor” ifadesini kulland\u0131.<\/p>\n
\n\tBu senaryoya g\u00f6re, y\u0131ld\u0131z \u00e7evresinden orijinal diskine g\u00f6re e\u011fik olan ba\u015fka bir gaz ve toz diski edindi. Yeni edinilen bu materyalden olu\u015fan gezegenler s\u00f6z konusu y\u00f6nelimi miras alm\u0131\u015f olabilir. Bu durumda GJ 3090 b’nin geriye do\u011fru y\u00f6r\u00fcngesi, rotas\u0131n\u0131 a\u00e7\u0131klamak i\u00e7in daha sonra ya\u015fanacak \u015fiddetli bir kar\u015f\u0131la\u015fmaya gerek kalmadan, ba\u015flang\u0131c\u0131na dair kan\u0131tlar\u0131 koruyacak.<\/p>\n
\n\tDev bir yolda\u015f\u0131n izine rastlanmad\u0131<\/h2>\n
\n\tK\u00fctle \u00e7ekimsel etkile\u015fimler, bir gezegenin y\u00f6r\u00fcngesini tersine \u00e7evirmenin ba\u015fka bir yolunu sunuyor.<\/p>\n
\n\tYeterince b\u00fcy\u00fck bir d\u0131\u015f gezegen veya yolda\u015f bir y\u0131ld\u0131z, zamanla y\u00f6r\u00fcngeyi bozarak dramatik bir \u015fekilde e\u011febiliyor.<\/p>\n
\n\tBu t\u00fcr etkile\u015fimler genellikle ters y\u00f6nl\u00fc gezegenleri a\u00e7\u0131klamak i\u00e7in kullan\u0131l\u0131yor. Bu nedenle ara\u015ft\u0131rmac\u0131lar, GJ 3090 sisteminde a\u015f\u0131r\u0131 e\u011fikli\u011fi kolayca a\u00e7\u0131klayabilecek kadar b\u00fcy\u00fck, birbirinden uzak bir yolda\u015f y\u0131ld\u0131z veya d\u0131\u015f gezegen arad\u0131.<\/p>\n
\n\tCenevre \u00dcniversitesinden doktora \u00f6\u011frencisi Yann Carteret, “Gezegeni b\u00f6ylesine a\u015f\u0131r\u0131 bir y\u00f6r\u00fcngeye zorlam\u0131\u015f olabilecek t\u00fcrden dev bir yolda\u015f arad\u0131k ancak buna dair bir kan\u0131t bulamad\u0131k. Bu durum, sistemin bu al\u0131\u015f\u0131lmad\u0131k mimariyi nas\u0131l edindi\u011fi konusunda farkl\u0131 d\u00fc\u015f\u00fcnmemiz gerekebilece\u011fini g\u00f6steriyor” diye konu\u015ftu.<\/p>\n
\n\tGJ 3090 b, g\u00f6k bilimcilerin \u00fc\u00e7 boyutlu y\u00f6r\u00fcnge e\u011fikli\u011fini \u00f6l\u00e7t\u00fckleri bir M c\u00fccesinin etraf\u0131ndaki en k\u00fc\u00e7\u00fck gezegen olma \u00f6zelli\u011fini ta\u015f\u0131yor. Bu \u00f6l\u00e7\u00fcm, yak\u0131n k\u0131z\u0131l\u00f6tesi g\u00f6zlemlerin ara\u015ft\u0131rmac\u0131lar\u0131n bu yayg\u0131n y\u0131ld\u0131zlar\u0131n etraf\u0131ndaki gezegen y\u00f6r\u00fcngelerini incelemesine nas\u0131l yard\u0131mc\u0131 olabilece\u011fini g\u00f6steriyor.<\/p>\n
\n\tSistemin yanl\u0131\u015f hizalanm\u0131\u015f ikinci bir diskten olu\u015fup olu\u015famayaca\u011f\u0131n\u0131 test etmek ve di\u011fer gezegen sistemlerinin benzer \u015fekilde a\u015f\u0131r\u0131 y\u00f6r\u00fcnge d\u00fczenlemelerine sahip olup olmad\u0131\u011f\u0131n\u0131 belirlemek i\u00e7in daha fazla g\u00f6zlem yap\u0131lmas\u0131 gerekecek.<\/p>\n<\/p><\/div>\n","protected":false},"excerpt":{"rendered":"
Londra Queen Mary \u00dcniversitesinden ara\u015ft\u0131rmac\u0131lar, bir gezegenin geriye do\u011fru y\u00f6r\u00fcngesini belirlemeye yard\u0131mc\u0131 oldu. Bu ke\u015fif, gezegen sistemlerinin nas\u0131l olu\u015ftu\u011funa ve evrimle\u015fti\u011fine dair ipu\u00e7lar\u0131 sunabilir.
Bir y\u0131ld\u0131z ve gezegenleri d\u00f6nen ayn\u0131 gaz ve toz diskinden olu\u015ftu\u011funda, gezegenlerin y\u0131ld\u0131z\u0131n d\u00f6n\u00fc\u015f y\u00f6n\u00fcnde hareket etmesi bekleniyor.
Ancak g\u00f6k bilimciler, Nept\u00fcn b\u00fcy\u00fckl\u00fc\u011f\u00fcndeki GJ 3090 b gezegeninin y\u0131ld\u0131z\u0131n\u0131n […]<\/p>\n","protected":false},"author":1,"featured_media":37956,"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-47361","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya"],"yoast_head":"\n
Tuhaf gezegen geriye do\u011fru d\u00f6n\u00fcyor: Bilim insanlar\u0131 nedenini bilmiyor - 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\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/\" \/>\n<meta property=\"og:locale\" content=\"tr_TR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Tuhaf gezegen geriye do\u011fru d\u00f6n\u00fcyor: Bilim insanlar\u0131 nedenini bilmiyor - Kuzeyin Sesi\" \/>\n<meta property=\"og:description\" content=\"
Londra Queen Mary \u00dcniversitesinden ara\u015ft\u0131rmac\u0131lar, bir gezegenin geriye do\u011fru y\u00f6r\u00fcngesini belirlemeye yard\u0131mc\u0131 oldu. Bu ke\u015fif, gezegen sistemlerinin nas\u0131l olu\u015ftu\u011funa ve evrimle\u015fti\u011fine dair ipu\u00e7lar\u0131 sunabilir.
Bir y\u0131ld\u0131z ve gezegenleri d\u00f6nen ayn\u0131 gaz ve toz diskinden olu\u015ftu\u011funda, gezegenlerin y\u0131ld\u0131z\u0131n d\u00f6n\u00fc\u015f y\u00f6n\u00fcnde hareket etmesi bekleniyor.
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Kuzeyin Sesi","robots":{"index":"index","follow":"follow","max-snippet":"max-snippet:-1","max-image-preview":"max-image-preview:large","max-video-preview":"max-video-preview:-1"},"canonical":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/","og_locale":"tr_TR","og_type":"article","og_title":"Tuhaf gezegen geriye do\u011fru d\u00f6n\u00fcyor: Bilim insanlar\u0131 nedenini bilmiyor - Kuzeyin Sesi","og_description":"
Londra Queen Mary \u00dcniversitesinden ara\u015ft\u0131rmac\u0131lar, bir gezegenin geriye do\u011fru y\u00f6r\u00fcngesini belirlemeye yard\u0131mc\u0131 oldu. Bu ke\u015fif, gezegen sistemlerinin nas\u0131l olu\u015ftu\u011funa ve evrimle\u015fti\u011fine dair ipu\u00e7lar\u0131 sunabilir.
Bir y\u0131ld\u0131z ve gezegenleri d\u00f6nen ayn\u0131 gaz ve toz diskinden olu\u015ftu\u011funda, gezegenlerin y\u0131ld\u0131z\u0131n d\u00f6n\u00fc\u015f y\u00f6n\u00fcnde hareket etmesi bekleniyor.
Ancak g\u00f6k bilimciler, Nept\u00fcn b\u00fcy\u00fckl\u00fc\u011f\u00fcndeki GJ 3090 b gezegeninin y\u0131ld\u0131z\u0131n\u0131n […]","og_url":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/","og_site_name":"Kuzeyin Sesi","article_publisher":"https:\/\/www.facebook.com\/kuzeyinsesii","article_published_time":"2026-09-28T06:12:03+00:00","og_image":[{"url":"https:\/\/trthaberstatic.cdn.wp.trt.com.tr\/resimler\/2432000\/gezegen-2433418.jpg","type":"","width":"","height":""}],"author":"Kuzeyin Sesi","twitter_card":"summary_large_image","twitter_creator":"@kuzeyinsesii","twitter_site":"@kuzeyinsesii","twitter_misc":{"Yazan:":"Kuzeyin Sesi","Tahmini okuma s\u00fcresi":"4 dakika"},"schema":{"@context":"https:\/\/schema.org","@graph":[{"@type":"Article","@id":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/#article","isPartOf":{"@id":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/"},"author":{"name":"Kuzeyin Sesi","@id":"https:\/\/kuzeyinsesi.org\/#\/schema\/person\/9f859689cdf01485597712386e37f5aa"},"headline":"Tuhaf gezegen geriye do\u011fru d\u00f6n\u00fcyor: Bilim insanlar\u0131 nedenini bilmiyor","datePublished":"2026-09-28T06:12:03+00:00","mainEntityOfPage":{"@id":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/"},"wordCount":761,"commentCount":0,"image":{"@id":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/#primaryimage"},"thumbnailUrl":"https:\/\/kuzeyinsesi.org\/wp-content\/uploads\/2026\/05\/gezegen-2433418.jpg","articleSection":["D\u00fcnya"],"inLanguage":"tr","potentialAction":[{"@type":"CommentAction","name":"Comment","target":["https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/#respond"]}]},{"@type":"WebPage","@id":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/","url":"https:\/\/kuzeyinsesi.org\/index.php\/2026\/09\/28\/tuhaf-gezegen-geriye-dogru-donuyor-bilim-insanlari-nedenini-bilmiyor\/","name":"Tuhaf gezegen geriye do\u011fru d\u00f6n\u00fcyor: Bilim insanlar\u0131 nedenini bilmiyor - 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