{"id":40080,"date":"2026-05-29T14:06:17","date_gmt":"2026-05-29T11:06:17","guid":{"rendered":"https:\/\/haberkuzey.com\/index.php\/2026\/05\/29\/uzayda-kurallari-yikan-kesif-galaksisinden-daha-buyuk-kara-delik-bulundu\/"},"modified":"2026-05-29T14:06:17","modified_gmt":"2026-05-29T11:06:17","slug":"uzayda-kurallari-yikan-kesif-galaksisinden-daha-buyuk-kara-delik-bulundu","status":"publish","type":"post","link":"https:\/\/haberkuzey.com\/index.php\/2026\/05\/29\/uzayda-kurallari-yikan-kesif-galaksisinden-daha-buyuk-kara-delik-bulundu\/","title":{"rendered":"Uzayda kurallar\u0131 y\u0131kan ke\u015fif: Galaksisinden daha b\u00fcy\u00fck kara delik bulundu"},"content":{"rendered":"<div>\n<p>&#13;<br \/>\n\tKe\u015fif, evrenin hen\u00fcz \u015fimdiki ya\u015f\u0131n\u0131n y\u00fczde 5&#8217;indeyken var olan ve &#8220;K\u00fc\u00e7\u00fck K\u0131rm\u0131z\u0131 Nokta&#8221; (Little Red Dot) olarak s\u0131n\u0131fland\u0131r\u0131lan &#8220;Abell2744-QSO1&#8221; adl\u0131 s\u0131ra d\u0131\u015f\u0131 bir g\u00f6k cisminin incelenmesiyle yap\u0131ld\u0131.<\/p>\n<p>&#13;<br \/>\n\tNormal \u015fartlarda sadece bin 300 \u0131\u015f\u0131k y\u0131l\u0131 geni\u015fli\u011findeki bu k\u00fc\u00e7\u00fck yap\u0131y\u0131 detayl\u0131ca incelemek imkans\u0131zken, &#8220;Pandora\u2019n\u0131n K\u00fcmesi&#8221; olarak da bilinen devasa galaksi k\u00fcmesi Abell 2744\u2019\u00fcn yaratt\u0131\u011f\u0131 k\u00fctle\u00e7ekimsel merceklenme etkisi devreye girdi.<\/p>\n<p>&#13;<br \/>\n\tUzay-zaman\u0131 b\u00fckerek bu uzak yap\u0131y\u0131 dev bir b\u00fcy\u00fcte\u00e7 gibi b\u00fcy\u00fcten ve g\u00f6ky\u00fcz\u00fcnde \u00fc\u00e7 ayr\u0131 kopya halinde g\u00f6r\u00fcnt\u00fcleyen bu do\u011fal fenomen, teleskobun nesneyi do\u011frudan analiz etmesini sa\u011flad\u0131.<\/p>\n<p><\/p>\n<h2>&#13;<br \/>\n\tKlasik olu\u015fum senaryolar\u0131 ge\u00e7ersiz kald\u0131<\/h2>\n<p>&#13;<br \/>\n\tCambridge \u00dcniversitesi Kavli Kozmoloji Enstit\u00fcs\u00fc&#8217;nden Ignas Juod\u017ebalis ve Roberto Maiolino liderli\u011findeki uluslararas\u0131 ekip, teleskobun NIRSpec enstr\u00fcman\u0131n\u0131 kullanarak kara deli\u011fin \u00e7evresindeki gaz \u00fczerindeki k\u00fctle\u00e7ekimsel etkisini haritaland\u0131rd\u0131. Yap\u0131lan do\u011frudan \u00f6l\u00e7\u00fcmler, kara deli\u011fin k\u00fctlesinin tahmin edilenden 10 milyon kat daha fazla, yani tam 50 milyon g\u00fcne\u015f k\u00fctlesi oldu\u011funu ortaya koydu.<\/p>\n<p>&#13;<br \/>\n\tDaha da \u00e7arp\u0131c\u0131 olan\u0131, bu devasa yap\u0131n\u0131n i\u00e7inde bulundu\u011fu galaksinin toplam k\u00fctlesinin en az \u00fc\u00e7te ikisini (yakla\u015f\u0131k y\u00fczde 66) tek ba\u015f\u0131na olu\u015fturmas\u0131yd\u0131. G\u00fcn\u00fcm\u00fcz evrenindeki galaksilerde merkezi kara delikler ev sahibi galaksinin k\u00fctlesinin yaln\u0131zca \u00e7ok k\u00fc\u00e7\u00fck bir kesrini olu\u015ftururken, bu nesnenin galaksinin kendisinden bile daha b\u00fcy\u00fck bir k\u00fctle pay\u0131na sahip olmas\u0131 teorileri alt\u00fcst etti.<\/p>\n<h2>&#13;<br \/>\n\t&#8220;\u00c7\u0131plak bir kara delik&#8221; ile kar\u015f\u0131 kar\u015f\u0131yay\u0131z<\/h2>\n<p>&#13;<br \/>\n\tAstrofizik d\u00fcnyas\u0131nda kabul g\u00f6ren klasik teoriye g\u00f6re, devasa bir y\u0131ld\u0131z \u00f6mr\u00fcn\u00fcn sonuna gelip \u00e7\u00f6ker, ard\u0131ndan bu k\u00fc\u00e7\u00fck kara delik \u00e7evresindeki maddeleri yutarak ve di\u011fer kara deliklerle birle\u015ferek zamanla s\u00fcper k\u00fctleli hale gelirdi.<\/p>\n<p>&#13;<br \/>\n\tYani \u00f6nce galaksiler ve y\u0131ld\u0131zlar olu\u015fur, kara delikler onlardan beslenerek b\u00fcy\u00fcrd\u00fc. Ancak bu yeni sistemde gaz bile\u015fiminin neredeyse tamamen saf hidrojen ve helyumdan olu\u015ftu\u011fu, oksijen gibi y\u0131ld\u0131z art\u0131\u011f\u0131 a\u011f\u0131r elementlerin oran\u0131n\u0131n G\u00fcne\u015f\u2019inkinden y\u00fczde 0,5 daha az oldu\u011fu tespit edildi. Ara\u015ft\u0131rmac\u0131lar, bu yap\u0131y\u0131 y\u0131ld\u0131z s\u00fcre\u00e7lerinden \u00f6nce meydana gelmi\u015f &#8220;neredeyse tamamen \u00e7\u0131plak bir kara delik&#8221; olarak tan\u0131ml\u0131yor.<\/p>\n<h2>&#13;<br \/>\n\tAstrofizikte yeni bir d\u00f6nem ba\u015fl\u0131yor<\/h2>\n<p>&#13;<br \/>\n\tNature ve Monthly Notices of the Royal Astronomical Society dergilerinde yay\u0131mlanan iki ayr\u0131 makaleyle duyurulan bu ke\u015fif, evrenin ilk b\u00fcy\u00fck yap\u0131lar\u0131n\u0131n tahmin edilenin aksine galaksiler de\u011fil, do\u011frudan devasa kara delikler olabilece\u011fini g\u00f6steriyor.<\/p>\n<p>&#13;<br \/>\n\tUzmanlar, bu bulgunun kara deliklerin olu\u015fum ve b\u00fcy\u00fcme senaryolar\u0131n\u0131n tamamen yeniden yaz\u0131lmas\u0131n\u0131 gerektiren bir paradigma de\u011fi\u015fimi oldu\u011funu belirtiyor. Maddenin y\u0131ld\u0131z \u00e7\u00f6k\u00fc\u015f\u00fc a\u015famas\u0131ndan ge\u00e7meden, B\u00fcy\u00fck Patlama sonras\u0131ndaki do\u011frudan yo\u011funluk farklar\u0131yla kendi i\u00e7ine \u00e7\u00f6kerek bu devasa &#8220;ilksel&#8221; yap\u0131lar\u0131 olu\u015fturmu\u015f olma ihtimali, \u00f6n\u00fcm\u00fczdeki on y\u0131l\u0131n en b\u00fcy\u00fck kozmik ara\u015ft\u0131rma ba\u015fl\u0131klar\u0131ndan biri olmaya aday g\u00f6r\u00fcn\u00fcyor.<\/p>\n<\/p><\/div>\n","protected":false},"excerpt":{"rendered":"<p>&#13; Ke\u015fif, evrenin hen\u00fcz \u015fimdiki ya\u015f\u0131n\u0131n y\u00fczde 5&#8217;indeyken var olan ve &#8220;K\u00fc\u00e7\u00fck K\u0131rm\u0131z\u0131 Nokta&#8221; (Little Red Dot) olarak s\u0131n\u0131fland\u0131r\u0131lan &#8220;Abell2744-QSO1&#8221; adl\u0131 s\u0131ra d\u0131\u015f\u0131 bir g\u00f6k cisminin incelenmesiyle yap\u0131ld\u0131. &#13; Normal \u015fartlarda sadece bin 300 \u0131\u015f\u0131k y\u0131l\u0131 geni\u015fli\u011findeki bu k\u00fc\u00e7\u00fck yap\u0131y\u0131 detayl\u0131ca incelemek imkans\u0131zken, &#8220;Pandora\u2019n\u0131n K\u00fcmesi&#8221; olarak da bilinen devasa galaksi k\u00fcmesi Abell 2744\u2019\u00fcn yaratt\u0131\u011f\u0131 k\u00fctle\u00e7ekimsel [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":40081,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jnews-multi-image_gallery":[],"jnews_single_post":[],"jnews_primary_category":[],"footnotes":""},"categories":[2],"tags":[],"class_list":["post-40080","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.7 - 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