{"id":5364,"date":"2025-12-12T00:07:56","date_gmt":"2025-12-11T21:07:56","guid":{"rendered":"https:\/\/www.ikizler.org\/?p=5364"},"modified":"2025-12-25T00:09:08","modified_gmt":"2025-12-24T21:09:08","slug":"sh-2-185-gamma-cassiopeia-nebula","status":"publish","type":"post","link":"http:\/\/www.ikizler.org\/index.php\/2025\/12\/12\/sh-2-185-gamma-cassiopeia-nebula\/","title":{"rendered":"Sh 2-185\u00a0 Gamma Cassiopeia Nebula"},"content":{"rendered":"\n<figure class=\"wp-block-gallery has-nested-images columns-default is-cropped wp-block-gallery-1 is-layout-flex wp-block-gallery-is-layout-flex\">\n<figure class=\"wp-block-image size-large\"><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"1000\" height=\"702\" data-id=\"5365\" src=\"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?resize=1000%2C702&#038;ssl=1\" alt=\"\" class=\"wp-image-5365\" srcset=\"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?w=1000 1000w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?resize=300%2C211 300w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?resize=768%2C539 768w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?resize=892%2C626 892w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?resize=480%2C337 480w\" sizes=\"auto, (max-width: 1000px) 100vw, 1000px\" \/><\/figure>\n<\/figure>\n\n\n\n<p><strong>Sh 2-185,&nbsp;<\/strong><a href=\"https:\/\/en.wikipedia.org\/wiki\/Cassiopeia_(constellation)\">kuzey tak\u0131my\u0131ld\u0131z\u0131 Cassiopeia&#8217;da<\/a>&nbsp;bulunan devasa y\u0131ld\u0131z sistemi Gamma Cassiopeiae (\u03b3 Cas)&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Constellation\">merkezli<\/a>&nbsp;bir&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Gamma_Cassiopeiae\">H<\/a>&nbsp;II&nbsp;b\u00f6lgesidir&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/H_II_region\">.<\/a>&nbsp;1959&#8217;da&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Stewart_Sharpless\">Stewart Sharpless taraf\u0131ndan yay\u0131nlanan ikinci&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Sharpless_catalog\"><em>H II B\u00f6lgeleri Katalo\u011fu&#8217;na<\/em><\/a>&nbsp;dahil edilmi\u015ftir&nbsp;.&nbsp;&nbsp;Sh 2-185, G\u00fcne\u015f&#8217;ten yakla\u015f\u0131k 10.500&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">\u0131\u015f\u0131k y\u0131l\u0131<\/a>&nbsp;(3,23&nbsp;&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Parsec#Parsecs_and_kiloparsecs\">kpc<\/a>&nbsp;) uzakl\u0131kta yer almaktad\u0131r.&nbsp;&nbsp;B\u00f6lge bir toz kabu\u011fuyla \u00e7evrilidir&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Young_stellar_object\">&nbsp;ve gen\u00e7 y\u0131ld\u0131z nesnelerinin<\/a>&nbsp;karakteristik \u00f6zelli\u011fi olan birka\u00e7 k\u0131z\u0131l\u00f6tesi nokta kayna\u011f\u0131 sergiler&nbsp;.&nbsp;<\/p>\n\n\n\n<p>Bu H II b\u00f6lgesi,&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Reflection_nebula\">yans\u0131ma<\/a>&nbsp;ve&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Emission_nebula\">emisyon bulutsular\u0131<\/a>&nbsp;IC 59 ve IC 63&#8217;\u00fc i\u00e7erir.&nbsp;&nbsp;Her iki bulutsunun da kuyruklu y\u0131ld\u0131z \u015feklinde bir yap\u0131s\u0131 vard\u0131r ve IC 63, ikisi aras\u0131nda daha parlak olan\u0131d\u0131r.&nbsp;&nbsp;\u0130ki bulutsunun g\u00f6r\u00fcn\u00fcm\u00fcndeki farkl\u0131l\u0131k, \u03b3 Cas&#8217;tan olan fiziksel uzakl\u0131klar\u0131n\u0131n bir sonucudur. IC 63, iyi tan\u0131mlanm\u0131\u015f bir iyonizasyon cephesi sergilerken, bu IC 59&#8217;da yoktur.&nbsp;&nbsp;Bulutsular,&nbsp;G\u00fcne\u015f&#8217;e en yak\u0131n&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Photodissociation_region\">fotodisosyasyon b\u00f6lgeleridir .&nbsp;<\/a><\/p>\n\n\n\n<p><a href=\"https:\/\/en.wikipedia.org\/wiki\/Max_Wolf\">Bu bulutsu, Alman g\u00f6kbilimci Max Wolf<\/a>&nbsp;taraf\u0131ndan 30 Aral\u0131k 1893&#8217;te&nbsp;ke\u015ffedildi&nbsp;&nbsp;ve 1895&#8217;te&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/J._L._E._Dreyer\">JLE Dreyer&#8217;in<\/a>&nbsp;Bulutsular&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Index_Catalogue_of_Nebulae\"><em>\u0130ndeks Katalo\u011fu&#8217;na<\/em><\/a>&nbsp;eklendi&nbsp;&nbsp;A\u00e7\u0131sal boyutu \u015fu kadard\u0131r:10&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Minute_of_arc\">\u2032<\/a>&nbsp;ve k\u00fc\u00e7\u00fck bir teleskopla g\u00f6r\u00fclebilir.&nbsp;&nbsp;D\u00fcnya perspektifinden bak\u0131ld\u0131\u011f\u0131nda, IC 59, \u03b3 Cas&#8217;\u0131n \u00f6n\u00fcnde konumlanm\u0131\u015ft\u0131r ve y\u0131ld\u0131za en yak\u0131n ucu 13,5 \u0131\u015f\u0131k y\u0131l\u0131 (4,15 pc) uzakl\u0131kta yer almaktad\u0131r. Bu, \u03b3 Cas taraf\u0131ndan \u015fekillendirilen bir&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Photodissociation_region\">fotodissosiasyon b\u00f6lgesidir<\/a>&nbsp;. Y\u0131ld\u0131zdan gelen \u0131\u015f\u0131k, bulutsudan D\u00fcnya&#8217;ya do\u011fru 17\u00b0&#8217;lik bir a\u00e7\u0131yla sa\u00e7\u0131lmaktad\u0131r.&nbsp;<\/p>\n\n\n\n<p>Bulutsunun ucu \u03b3 Cas&#8217;a en yak\u0131n nokta olarak kabul edilse de, en yo\u011fun UV radyasyonu bat\u0131daki i\u00e7b\u00fckey y\u00fczeyden al\u0131nmaktad\u0131r. Bu nedenle u\u00e7, bulutunun geri kalan\u0131ndan y\u0131ld\u0131za daha uzakta olabilir. Bu bulutsunun daha s\u0131cak bile\u015feninin ortalama s\u0131cakl\u0131\u011f\u0131 \u015f\u00f6yledir:675&nbsp;\u00b1&nbsp;49 K&nbsp;, so\u011futucu bile\u015fen ise150&nbsp;\u00b1&nbsp;34 K&nbsp;.<\/p>\n\n\n\n<p>Kaynak: <a href=\"https:\/\/en.wikipedia.org\/\">https:\/\/en.wikipedia.org\/<\/a><\/p>\n\n\n\n<p>Foto\u011fraf: U\u011fur \u0130K\u0130ZLER<br>Tarih: 12.12.2025<br>Saat: 00:01 &#8211; 01:45<br>Yer: Mudanya &#8211; Bursa 40.36023 \u00b0 N &#8211; 28.90191 \u00b0 E<\/p>\n\n\n\n<p>Optik : El yap\u0131m\u0131 Newton teleskop 150 mm f\/4.57<\/p>\n\n\n\n<p>TeleVue Paracorr Coma Corrector<\/p>\n\n\n\n<p>Kundak: El yap\u0131m\u0131 kundak<br>Kamera : Canon EOS 6D Full Spectrum Modified<\/p>\n\n\n\n<p>Otomatik takip: PHD, Bower mirror lens&nbsp; 500 mm f\/6.3- ZWO ASI 120 MC-S<\/p>\n\n\n\n<p>ISO: 1600<\/p>\n\n\n\n<p>Poz: Light&nbsp; 60 x 90 sn. \u2013 Dark 30 \u2013 Flat 20 \u2013 Bias 25<\/p>\n\n\n\n<p>Yaz\u0131l\u0131m: Pix\u0130nsight 1.8, Photoshop CC 2015<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Sh 2-185,&nbsp;kuzey tak\u0131my\u0131ld\u0131z\u0131 Cassiopeia&#8217;da&nbsp;bulunan devasa y\u0131ld\u0131z sistemi Gamma Cassiopeiae (\u03b3 Cas)&nbsp;merkezli&nbsp;bir&nbsp;H&nbsp;II&nbsp;b\u00f6lgesidir&nbsp;.&nbsp;1959&#8217;da&nbsp;Stewart Sharpless taraf\u0131ndan yay\u0131nlanan ikinci&nbsp;H II B\u00f6lgeleri Katalo\u011fu&#8217;na&nbsp;dahil edilmi\u015ftir&nbsp;.&nbsp;&nbsp;Sh 2-185, G\u00fcne\u015f&#8217;ten yakla\u015f\u0131k 10.500&nbsp;\u0131\u015f\u0131k y\u0131l\u0131&nbsp;(3,23&nbsp;&nbsp;kpc&nbsp;) uzakl\u0131kta yer almaktad\u0131r.&nbsp;&nbsp;B\u00f6lge bir toz kabu\u011fuyla \u00e7evrilidir&nbsp;&nbsp;ve gen\u00e7 y\u0131ld\u0131z nesnelerinin&nbsp;karakteristik \u00f6zelli\u011fi olan birka\u00e7 k\u0131z\u0131l\u00f6tesi nokta kayna\u011f\u0131 sergiler&nbsp;.&nbsp; Bu H II b\u00f6lgesi,&nbsp;yans\u0131ma&nbsp;ve&nbsp;emisyon bulutsular\u0131&nbsp;IC 59 ve IC 63&#8217;\u00fc i\u00e7erir.&nbsp;&nbsp;Her iki bulutsunun da kuyruklu&#8230;<\/p>\n","protected":false},"author":1,"featured_media":5365,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[22,10],"tags":[],"class_list":["post-5364","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-bulutsular","category-derin-uzay","wpcat-22-id","wpcat-10-id"],"jetpack_featured_media_url":"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2025\/12\/Gamma_Cassiopeia.jpg?fit=1000%2C702","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5364","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/comments?post=5364"}],"version-history":[{"count":1,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5364\/revisions"}],"predecessor-version":[{"id":5366,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5364\/revisions\/5366"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media\/5365"}],"wp:attachment":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media?parent=5364"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/categories?post=5364"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/tags?post=5364"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}