{"id":147,"date":"2026-08-21T12:02:06","date_gmt":"2026-08-21T12:02:06","guid":{"rendered":"https:\/\/baharkilic.org\/?p=147"},"modified":"2026-08-21T13:40:42","modified_gmt":"2026-08-21T13:40:42","slug":"hubble-gozuyle-centaurus-a","status":"publish","type":"post","link":"https:\/\/baharkilic.org\/?p=147","title":{"rendered":"Hubble g\u00f6z\u00fcyle Centaurus A"},"content":{"rendered":"<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;NASA\/ESA Hubble uzay teleskobuyla Centaurus A galaksisinin yak\u0131n &ccedil;ekimlerini i&ccedil;eren muhte\u015fem&nbsp;g&ouml;r&uuml;nt&uuml;ler elde edildi. Hubble&rsquo;a eklenen son model Wide Field Camera-3 aparat\u0131 sayesinde, galaksinin ak\u0131 i&ccedil;eren dinamik bir g&ouml;r&uuml;nt&uuml;s&uuml; elde edildi.<\/span><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp;<strong>NGC 5128<\/strong> olarak da bilnen Centaurus A,&nbsp; karanl\u0131k maddeden meydana gelen &ccedil;arp\u0131c\u0131 toz \u015feritleriyle &uuml;nl&uuml;d&uuml;r. Bu galaksi hakk\u0131nda \u015fimdiye kadar elde edilen en detayl\u0131 g&ouml;r&uuml;nt&uuml;ler, Wide Field Camera 3 kameras\u0131yla &ccedil;al\u0131\u015fan Hubble teleskobuyla elde edildi. &Ccedil;oklu dalga boyu i&ccedil;eren bu g&ouml;r&uuml;nt&uuml;lerde, galaksinin bu tozlu k\u0131s\u0131mlar\u0131n\u0131n daha &ouml;nce hi&ccedil; g&ouml;r&uuml;lmemi\u015f ayr\u0131nt\u0131lar\u0131 ortaya &ccedil;\u0131kt\u0131.<\/span><span style=\"color: #000000;\">&nbsp;<\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;G&ouml;r&uuml;nen spektrumdaki &ouml;zeliklerin yan\u0131 s\u0131ra, gen&ccedil; y\u0131ld\u0131zlardan gelen ultraviyole \u0131\u015f\u0131k ve yak\u0131n k\u0131z\u0131l &ouml;tesi \u0131\u015f\u0131k da g&ouml;r&uuml;lmektedir, bu da toz taraf\u0131ndan perdelenen ayr\u0131nt\u0131lar\u0131n bir k\u0131sm\u0131n\u0131 g&ouml;rmemizi sa\u011flar.<\/span><\/p>\n<p><span style=\"color: #000000;\"><img loading=\"lazy\" decoding=\"async\" src=\"\/image.axd?picture=2011%2f6%2fcentaurus+a.jpg\" alt=\"centaurus\" width=\"430\" height=\"453\" \/><\/span><\/p>\n<p><span style=\"color: #000000;\"><strong><span style=\"font-family: verdana, geneva; font-size: small;\">Resim:<\/span><\/strong><em><span style=\"font-family: verdana, geneva; font-size: small;\"> (Credit: NASA, ESA, and the Hubble Heritage (STScI\/AURA)-ESA\/Hubble Collaboration. Acknowledgment: R. O&rsquo;Connell (University of Virginia)<\/span><\/em><\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;Centaurus A&rsquo;y\u0131 boylu boyunca kesen koyu toz \u015feridi, y\u0131ld\u0131zs\u0131z bir ortama de\u011fil, beli &ouml;l&ccedil;&uuml;de bir y\u0131ld\u0131z \u0131\u015f\u0131\u011f\u0131na i\u015faret eder. I\u015f\u0131k ge&ccedil;irmeyen bulutlar, g&ouml;r&uuml;nen \u0131\u015f\u0131\u011f\u0131n bize ula\u015fmas\u0131n\u0131 engeller. Hubble, bu resimde, k&ouml;\u015feler aras\u0131ndan ge&ccedil;en hattaki bu tozsu bulutlara odaklanm\u0131\u015ft\u0131r. Kara temelli teleskoplarla elde edilen geni\u015f a&ccedil;\u0131l\u0131 g&ouml;r&uuml;nt&uuml;lerde bu \u015ferit, b&uuml;t&uuml;n galaksi boyunca uzanmaktad\u0131r.<\/span><span style=\"color: #000000;\">&nbsp;<\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;Gaz ve toz diskinin, b&uuml;k&uuml;lm&uuml;\u015f gibi g&ouml;r&uuml;nen \u015fekli, ge&ccedil;mi\u015fte Centaurus A&rsquo;n\u0131n ba\u015fka bir galaksiyle &ccedil;arp\u0131\u015f\u0131p birle\u015fmi\u015f olabilece\u011fini d&uuml;\u015f&uuml;nd&uuml;r&uuml;yor. Bu olay\u0131n yaratt\u0131\u011f\u0131&nbsp; \u015fok dalgalar\u0131, Hidrojen gaz\u0131n\u0131n&nbsp; ergimesiyle y\u0131ld\u0131z olu\u015fumunun yo\u011fun b&ouml;lgelerini ate\u015flemi\u015ftir. Bu olay, Hubble teleskobunun yak\u0131n &ccedil;ekimli foto\u011fraf\u0131nda g&ouml;r&uuml;len s\u0131n\u0131r (d\u0131\u015f) b&ouml;lgelerinde ve k\u0131rm\u0131z\u0131 lekelerde belirgindir.<\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;Galaksinin yo\u011fun &ccedil;ekirde\u011finin merkezinde, y&uuml;ksek oranda aktif bir s&uuml;per k&uuml;tleli kara delik bulunur. G&uuml;&ccedil;l&uuml; r&ouml;lativist jetler, b&uuml;y&uuml;k miktarda radyo ve X \u0131\u015f\u0131n\u0131 kaynakl\u0131 radyasyon yayar, ancak bunlar bu foto\u011frafta g&ouml;r&uuml;nmez &ccedil;&uuml;nk&uuml; Hubble optik, ultraviyole ve k\u0131z\u0131l &ouml;tesi dalga boylar\u0131n\u0131 inceleyecek \u015fekilde tasarlanm\u0131\u015ft\u0131r.<\/span><span style=\"color: #000000;\">&nbsp;<\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp; &nbsp;Sadece 11 milyon \u0131\u015f\u0131k y\u0131l\u0131 uzakl\u0131kta olan Centaurus A , g&ouml;receli olarak bize yak\u0131n bir galaksidir. Sadece yak\u0131n de\u011fil, ayn\u0131 zamanda parlakt\u0131r da. Bu &ouml;zelli\u011fiyle, g&uuml;ney yar\u0131mk&uuml;rede ya\u015fayan amat&ouml;r astronomlar i&ccedil;in &ccedil;ok &ccedil;ekici bir inceleme alan\u0131 olu\u015fturur. (G&uuml;ney yar\u0131mk&uuml;rede Centaurus A a&ccedil;\u0131k&ccedil;a g&ouml;r&uuml;nmektedir.) Y\u0131ld\u0131zbilimciler, d&uuml;rb&uuml;nle bile galaksiyi inceleyebilir.&nbsp;<\/span><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">Ancak sadece Hubble Uzay Teleskobuyla bu kadar ayr\u0131nt\u0131 ortaya &ccedil;\u0131km\u0131\u015ft\u0131r, hem de bu derece e\u015fsiz bir netlik ve &ccedil;&ouml;z&uuml;n&uuml;rl&uuml;kle. Hubble&rsquo;\u0131n y&ouml;r&uuml;ngedeki konumu sayesinde, atmosfer taraf\u0131ndan gizlenen ultraviyole dalga boylar\u0131 izlenebilir.<\/span><\/p>\n<p><span style=\"color: #000000;\">&nbsp;<\/span><\/p>\n<p><span style=\"color: #000000;\"><span style=\"font-family: verdana, geneva; font-size: small;\">&nbsp; <strong>&nbsp;Makale kayna\u011f\u0131:<\/strong> <\/span><span style=\"font-family: verdana, geneva; font-size: small;\"><em><a href=\"https:\/\/esahubble.org\/\" target=\"_blank\">ESA\/Hubble Information Centre<\/a><\/em>&#8216;dan elde edilen bilgilerin \u0131\u015f\u0131\u011f\u0131nda <em><a href=\"http:\/\/www.sciencedaily.com\/releases\/2011\/06\/110616092645.htm\" target=\"_blank\">ScienceDaily<\/a><\/em>&nbsp;ekibi taraf\u0131ndan yaz\u0131lm\u0131\u015ft\u0131r.<\/span><\/span><\/p>\n<p><span style=\"color: #000000;\"><span style=\"font-family: verdana, geneva; font-size: small;\"><strong>&nbsp; &nbsp;&Ccedil;eviri:<\/strong> felis agnosticus<\/span><\/span><\/p>\n<p><span style=\"font-family: verdana, geneva; font-size: small; color: #000000;\">&nbsp;<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>&nbsp; &nbsp;NASA\/ESA Hubble uzay teleskobuyla Centaurus A galaksisinin yak\u0131n &ccedil;ekimlerini i&ccedil;eren muhte\u015fem&nbsp;g&ouml;r&uuml;nt&uuml;ler elde edildi. Hubble&rsquo;a eklenen son model Wide Field Camera-3 aparat\u0131 sayesinde, galaksinin ak\u0131 i&ccedil;eren dinamik bir g&ouml;r&uuml;nt&uuml;s&uuml; elde edildi.&nbsp;NGC 5128 olarak da bilnen Centaurus A,&nbsp; karanl\u0131k maddeden meydana gelen &ccedil;arp\u0131c\u0131 toz \u015feritleriyle &uuml;nl&uuml;d&uuml;r. Bu galaksi hakk\u0131nda \u015fimdiye kadar elde edilen en detayl\u0131 g&ouml;r&uuml;nt&uuml;ler, [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[3],"tags":[],"class_list":["post-147","post","type-post","status-publish","format-standard","hentry","category-bilim"],"_links":{"self":[{"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/posts\/147","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/baharkilic.org\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=147"}],"version-history":[{"count":1,"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/posts\/147\/revisions"}],"predecessor-version":[{"id":412,"href":"https:\/\/baharkilic.org\/index.php?rest_route=\/wp\/v2\/posts\/147\/revisions\/412"}],"wp:attachment":[{"href":"https:\/\/baharkilic.org\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=147"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/baharkilic.org\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=147"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/baharkilic.org\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=147"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}