{"id":49121,"date":"2018-12-09T22:05:05","date_gmt":"2018-12-09T20:05:05","guid":{"rendered":"https:\/\/osr.org\/?p=49121\/"},"modified":"2018-12-09T22:05:05","modified_gmt":"2018-12-09T20:05:05","slug":"hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi","status":"publish","type":"post","link":"https:\/\/osr.org\/tr\/blog\/astronomi\/hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi\/","title":{"rendered":"Hubble, &#8216;g\u00fclen y\u00fcz&#8217; galaksi k\u00fcmesini ortaya \u00e7\u0131kard\u0131"},"content":{"rendered":"<p>NASA\/ESA Hubble Uzay Teleskobu&#8217;nun Geni\u015f Alan Kameras\u0131 3 (WFC3) ile \u00e7ekilen bu g\u00f6r\u00fcnt\u00fc resmi olarak SDSS J0952 + 3434 bilinen bir g\u00f6kada k\u00fcmesini g\u00f6steriyor. Ancak, bir g\u00f6kada k\u00fcmesi g\u00fclen y\u00fcze benzeyen galaksilerden olu\u015fuyor.<br \/>\nG\u00f6r\u00fcnt\u00fc, geni\u015f \u0131\u015f\u0131k yay\u0131n\u0131n \u00fcst\u00fcnde iki sar\u0131 renkli damlay\u0131 ortaya koyuyor.<br \/>\nNASA, &#8216;a\u011f\u0131z&#8217; \u0131\u015f\u0131\u011f\u0131n bir hilesi taraf\u0131ndan yarat\u0131ld\u0131\u011f\u0131n\u0131 s\u00f6yl\u00fcyor.<br \/>\nHubble bu g\u00f6r\u00fcnt\u00fcy\u00fc yeni y\u0131ld\u0131zlar\u0131n kozmos boyunca nas\u0131l yay\u0131ld\u0131\u011f\u0131n\u0131 anlamak i\u00e7in kullanacak.<br \/>\nNASA, &#8216;WFC3, benzeri g\u00f6r\u00fclmemi\u015f bir \u00e7\u00f6z\u00fcn\u00fcrl\u00fckte uzak g\u00f6kadalar\u0131 g\u00f6rebiliyor. Bunlar\u0131n i\u00e7inde yer alan y\u0131ld\u0131z olu\u015fum b\u00f6lgelerini bulmak ve incelemek i\u00e7in yeterince y\u00fcksek.&#8221; dedi.<br \/>\nY\u0131ld\u0131zlar devasa gaz bulutlar\u0131 i\u00e7inde do\u011farlar. Bu devasa bulutlar ya da y\u0131ld\u0131zlar yer\u00e7ekimi alt\u0131nda \u00e7\u00f6kerek yeni y\u0131ld\u0131zlara d\u00f6n\u00fc\u015fecek tohumlar haline gelir. Bilim adamlar\u0131 farkl\u0131 y\u0131ld\u0131z kre\u015flerinin parlakl\u0131\u011f\u0131n\u0131, b\u00fcy\u00fckl\u00fc\u011f\u00fcn\u00fc ve olu\u015fum oranlar\u0131n\u0131 analiz ederek yeni do\u011fmu\u015f bir y\u0131ld\u0131z\u0131n olu\u015fumuna yol a\u00e7abilecek s\u00fcre\u00e7ler hakk\u0131nda daha fazla \u015fey \u00f6\u011frenmeyi umuyor. Farkl\u0131 galaksiler i\u00e7inde bunlarla \u00e7al\u0131\u015fmak, evrendeki zaman ve mekanda farkl\u0131 noktalarda y\u0131ld\u0131z olu\u015fumu hakk\u0131nda bilgi verecek.<\/p>\n<h2><span style=\"color: #15acdf\">Y\u0131d\u0131zlar ve galaksi k\u00fcmeleri <\/span><\/h2>\n<p>G\u00f6k ada k\u00fcmesi ya da galaksi k\u00fcmesi, k\u00fctle \u00e7ekimi sayesinde birbirlerine ba\u011fl\u0131 y\u00fczden fazla g\u00f6k adan\u0131n olu\u015fturdu\u011fu k\u00fcmedir. G\u00f6k ada say\u0131s\u0131 100\u2019\u00fcn alt\u0131nda oldu\u011fu zaman bu topluluklara, gruplar ve k\u00fcmeler aras\u0131ndaki s\u0131n\u0131rlar belirgin olmasa da, g\u00f6k ada grubu denir. G\u00f6k ada k\u00fcmeleri bi\u00e7imleriyle (\u00f6zel, k\u00fcresel, simetrik, vs.) da\u011f\u0131l\u0131mlar\u0131yla veya (birka\u00e7 bine \u00e7\u0131kabilen) g\u00f6k ada say\u0131lar\u0131yla nitelenirler. 10 milyar y\u0131l \u00f6nce olu\u015ftuklar\u0131 san\u0131lmaktad\u0131r.<\/p>\n<p>G\u00f6k ada k\u00fcmelerinin bir araya gelmesiyle olu\u015fan k\u00fcmeler toplulu\u011funa ise \u00fcst k\u00fcme ya da s\u00fcper k\u00fcme (\u0130ng. super cluster) ad\u0131 verilir. G\u00f6k ada k\u00fcmeleri istikrarl\u0131 yap\u0131lar olup k\u00fcmenin k\u00fctle\u00e7ekimsel etkisinden ka\u00e7amazlar. G\u00f6k ada k\u00fcmelerinin Evren&#8217;deki da\u011f\u0131l\u0131m\u0131 homojen de\u011fildir; kimi b\u00f6lgelerde s\u0131kl\u0131k g\u00f6sterirlerken kimi b\u00f6lgelerde seyrektirler. G\u00f6k adalar\u0131n yakla\u015f\u0131k % 90\u2019\u0131 bir k\u00fcmeye ya da bir \u00fcst k\u00fcmeye dahildir. G\u00f6k adam\u0131z Samanyolu, 30 kadar g\u00f6k ada i\u00e7eren yerel gruba (\u0130ng. local group) dahil olup bu yerel grup da bir s\u00fcper k\u00fcmeye dahildir.<\/p>\n<p>G\u00f6k ada k\u00fcmeleri, s\u0131cakl\u0131\u011f\u0131 107K ila 108 K aras\u0131nda de\u011fi\u015fen ve yo\u011funlu\u011fu \u00e7ok az (par\u00e7ac\u0131k say\u0131s\u0131 cm\u00b3 ba\u015f\u0131na 10\u22123 ila 10\u22122) olan ve X \u0131\u015f\u0131nlar\u0131 yayan bir gaz i\u00e7erirler. G\u00f6k ada k\u00fcmelerinin toplam k\u00fctleleri 1014 ila 1015 G\u00fcne\u015f k\u00fctlesi aras\u0131nda, yar\u0131\u00e7aplar\u0131 ise 2 ila 10 Mpc aras\u0131nda de\u011fi\u015fir.<\/p>\n<h2><span style=\"color: #15acdf\">G\u00f6k adalar ve y\u0131ld\u0131zlar<\/span><\/h2>\n<p>Galaksi veya g\u00f6k ada, k\u00fctle \u00e7ekimi kuvvetiyle birbirine ba\u011fl\u0131 y\u0131ld\u0131zlar, y\u0131ld\u0131zlararas\u0131 gaz, toz ve plazman\u0131n meydana getirdi\u011fi y\u0131ld\u0131zlararas\u0131 madde ve \u015fimdilik pek anla\u015f\u0131lamam\u0131\u015f karanl\u0131k maddeden olu\u015fan sistemdir. Tipik galaksiler 10 milyon (c\u00fcce galaksi) ile bir trilyon (dev galaksi) aras\u0131ndaki miktarlarda y\u0131ld\u0131z i\u00e7erirle ve bir galaksinin i\u00e7erdi\u011fi y\u0131ld\u0131zlar\u0131n hepsi o galaksinin k\u00fctle merkezini eksen alan y\u00f6r\u00fcngelerde d\u00f6ner. Galaksiler \u00e7e\u015fitli \u00e7oklu y\u0131ld\u0131z sistemlerini, y\u0131ld\u0131z k\u00fcmelerini ve \u00e7e\u015fitli nebulalar\u0131 da i\u00e7erebilirler. \u00c7evresinde gezegenler ve asteroitler gibi \u00e7e\u015fitli kozmik cisimler d\u00f6nen G\u00fcne\u015f, Samanyolu Galaksisi&#8217;ndeki y\u0131ld\u0131zlardan yaln\u0131zca biridir.<\/p>\n<p>Bir sanat\u00e7\u0131 taraf\u0131ndan haz\u0131rlanan Samanyolu Galaksisi. \u0130ki ana spiral kol \u00e7ekirdekteki \u00e7ubuk olu\u015fumunun u\u00e7lar\u0131ndan \u00e7\u0131kmaktad\u0131r. G\u00fcne\u015f kollardan birinde yer almaktad\u0131r.<br \/>\nTarihsel olarak galaksiler g\u00f6zle g\u00f6r\u00fclen \u015fekillerine g\u00f6re s\u0131n\u0131flanm\u0131\u015flard\u0131r. Bu s\u0131n\u0131flamada s\u0131k kar\u015f\u0131la\u015f\u0131lan bi\u00e7imlerden biri, \u0131\u015f\u0131k profili elips \u015fekilli olan eliptik galaksidir. Sarmal galaksiler, tozlu ve k\u0131vr\u0131ml\u0131 kollar\u0131 olan disk \u015fekilli yap\u0131lard\u0131r.<\/p>\n<p>D\u00fczensiz ya da ola\u011fan d\u0131\u015f\u0131 bi\u00e7imli galaksiler ise &#8220;tuhaf galaksiler&#8221; olarak bilinir ve tipik olarak, kom\u015fu galaksilerin k\u00fctle \u00e7ekimine ba\u011fl\u0131 bi\u00e7im bozulmas\u0131yla olu\u015furlar. Birbirlerine yak\u0131n galaksilerin aras\u0131ndaki bu t\u00fcr etkile\u015fimlerle s\u00f6z konusu galaksiler birle\u015febilece\u011fi gibi, y\u0131ld\u0131z olu\u015fumu olaylar\u0131nda &#8220;patlama&#8221; diye adland\u0131r\u0131labilecek \u00f6l\u00e7\u00fcde fazla art\u0131\u015flar\u0131n tetiklenmesiyle y\u0131ld\u0131z patlama galaksileri (\u0130ng., starburst galaxy) de geli\u015febilir. Ayr\u0131ca, d\u00fczenli bir yap\u0131ya sahip olmayan k\u00fc\u00e7\u00fck galaksilerden de d\u00fcz<\/p>\n","protected":false},"excerpt":{"rendered":"<p>NASA\/ESA Hubble Uzay Teleskobu&#8217;nun Geni\u015f Alan Kameras\u0131 3 (WFC3) ile \u00e7ekilen bu g\u00f6r\u00fcnt\u00fc resmi olarak SDSS J0952 + 3434 bilinen bir g\u00f6kada k\u00fcmesini g\u00f6steriyor. Ancak, bir g\u00f6kada k\u00fcmesi g\u00fclen y\u00fcze benzeyen galaksilerden olu\u015fuyor. G\u00f6r\u00fcnt\u00fc, geni\u015f \u0131\u015f\u0131k yay\u0131n\u0131n \u00fcst\u00fcnde iki sar\u0131 renkli damlay\u0131 ortaya koyuyor. NASA, &#8216;a\u011f\u0131z&#8217; \u0131\u015f\u0131\u011f\u0131n bir hilesi taraf\u0131ndan yarat\u0131ld\u0131\u011f\u0131n\u0131 s\u00f6yl\u00fcyor. Hubble bu g\u00f6r\u00fcnt\u00fcy\u00fc [&hellip;]<\/p>\n","protected":false},"author":23,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":""},"categories":[506],"tags":[],"class_list":["post-49121","post","type-post","status-publish","format-standard","hentry","category-astronomi"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v26.7 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Hubble, &#039;g\u00fclen y\u00fcz&#039; galaksi k\u00fcmesini ortaya \u00e7\u0131kard\u0131 - Online Star Register<\/title>\n<meta name=\"description\" content=\"Hubble, &#039;g\u00fclen g\u00f6kada k\u00fcmesinin&#039; yeni bir g\u00f6r\u00fcnt\u00fcs\u00fcn\u00fc ortaya \u00e7\u0131kard\u0131.\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/osr.org\/tr\/blog\/astronomi\/hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi\/\" \/>\n<meta property=\"og:locale\" content=\"tr_TR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Hubble, &#039;g\u00fclen y\u00fcz&#039; galaksi k\u00fcmesini ortaya \u00e7\u0131kard\u0131 - Online Star Register\" \/>\n<meta property=\"og:description\" content=\"Hubble, &#039;g\u00fclen g\u00f6kada k\u00fcmesinin&#039; yeni bir g\u00f6r\u00fcnt\u00fcs\u00fcn\u00fc ortaya \u00e7\u0131kard\u0131.\" \/>\n<meta property=\"og:url\" content=\"https:\/\/osr.org\/tr\/blog\/astronomi\/hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi\/\" \/>\n<meta property=\"og:site_name\" content=\"Online Star Register\" \/>\n<meta property=\"article:published_time\" content=\"2018-12-09T20:05:05+00:00\" \/>\n<meta name=\"author\" content=\"Hatice Utkan Ozden\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"Hatice Utkan Ozden\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"4 minutes\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\n\t    \"@context\": \"https:\/\/schema.org\",\n\t    \"@graph\": [\n\t        {\n\t            \"@type\": \"Article\",\n\t            \"@id\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi\/#article\",\n\t            \"isPartOf\": {\n\t                \"@id\": \"https:\/\/osr.org\/tr\/blog\/astronomi\/hubble-gulen-yuz-galaksi-kumesini-ortaya-cikardi\/\"\n\t            },\n\t            \"author\": {\n\t                \"name\": \"Hatice Utkan Ozden\",\n\t                \"@id\": \"https:\/\/osr.org\/tr\/#\/schema\/person\/ef86e8c767dff5d728379a636d34a85a\"\n\t            },\n\t            \"headline\": \"Hubble, &#8216;g\u00fclen y\u00fcz&#8217; 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