{"id":4381,"date":"2023-06-20T20:57:00","date_gmt":"2023-06-20T17:57:00","guid":{"rendered":"http:\/\/www.ikizler.org\/?p=4381"},"modified":"2023-09-29T20:59:31","modified_gmt":"2023-09-29T17:59:31","slug":"m81-m82-bode-ve-puro-gokadalari","status":"publish","type":"post","link":"https:\/\/www.ikizler.org\/index.php\/2023\/06\/20\/m81-m82-bode-ve-puro-gokadalari\/","title":{"rendered":"M81 \u2013 M82 Bode ve Puro G\u00f6kadalar\u0131"},"content":{"rendered":"\n<figure class=\"wp-block-gallery columns-1 is-cropped wp-block-gallery-1 is-layout-flex wp-block-gallery-is-layout-flex\"><ul class=\"blocks-gallery-grid\"><li class=\"blocks-gallery-item\"><figure><img data-recalc-dims=\"1\" loading=\"lazy\" decoding=\"async\" width=\"1000\" height=\"657\" src=\"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?resize=1000%2C657\" alt=\"\" data-id=\"4382\" data-full-url=\"http:\/\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg\" data-link=\"http:\/\/www.ikizler.org\/?attachment_id=4382\" class=\"wp-image-4382\" srcset=\"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?w=1000&amp;ssl=1 1000w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?resize=300%2C197&amp;ssl=1 300w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?resize=768%2C505&amp;ssl=1 768w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?resize=892%2C586&amp;ssl=1 892w, https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?resize=480%2C315&amp;ssl=1 480w\" sizes=\"auto, (max-width: 1000px) 100vw, 1000px\" \/><\/figure><\/li><\/ul><\/figure>\n\n\n\n<p><strong>Messier 81<\/strong>&nbsp;(ayr\u0131ca&nbsp;NGC 3031&nbsp;veya&nbsp;Bode G\u00f6kadas\u0131&nbsp;olarak da bilinir ),&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Ursa_Major\">B\u00fcy\u00fck Ay\u0131&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Constellation\">tak\u0131my\u0131ld\u0131z\u0131<\/a>&nbsp;y\u00f6n\u00fcnde yakla\u015f\u0131k&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/1_E22_m\">12 milyon&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">\u0131\u015f\u0131ky\u0131l\u0131<\/a>&nbsp;uzakl\u0131kta bulunan&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Grand_design_spiral_galaxy\">b\u00fcy\u00fck tasar\u0131ml\u0131 sarmal g\u00f6kadad\u0131r<\/a>&nbsp;.&nbsp;29,44&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Parsec#Parsecs_and_kiloparsecs\">kiloparsek<\/a>&nbsp;(96.000&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">\u0131\u015f\u0131ky\u0131l\u0131<\/a>&nbsp;)&nbsp;\u00e7ap\u0131ndad\u0131r.&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Milky_Way\">&nbsp;Samanyolu<\/a>&nbsp;galaksisine g\u00f6receli yak\u0131nl\u0131\u011f\u0131 , b\u00fcy\u00fck boyutu ve&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Active_galactic_nucleus\">aktif galaktik \u00e7ekirde\u011fi (70 milyon&nbsp;<\/a>g\u00fcne\u015f &nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Supermassive_black_hole\">&nbsp;k\u00fctleli kara deli\u011fi<\/a>&nbsp;bar\u0131nd\u0131rmas\u0131&nbsp;nedeniyle&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Astronomer\">, Messier 81 profesyonel g\u00f6kbilimciler<\/a>&nbsp;taraf\u0131ndan kapsaml\u0131 bir \u015fekilde incelenmi\u015ftir&nbsp;.&nbsp;Galaksinin b\u00fcy\u00fck boyutu ve nispeten y\u00fcksek parlakl\u0131\u011f\u0131 da onu&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Amateur_astronomy\">amat\u00f6r g\u00f6kbilimciler<\/a>&nbsp;i\u00e7in pop\u00fcler bir hedef haline getiriyor .&nbsp;&nbsp;\u015eubat 2022&#8217;nin sonlar\u0131nda g\u00f6kbilimciler, M81&#8217;in tekrarlanan&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Fast_radio_burst\">h\u0131zl\u0131 radyo patlamas\u0131 olan&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Fast_radio_burst#FRB_20200120E\">FRB 20200120E&#8217;nin<\/a>&nbsp;kayna\u011f\u0131 olabilece\u011fini bildirdi&nbsp;.<\/p>\n\n\n\n<p>Messier 81 ilk olarak 31 Aral\u0131k 1774&#8217;te&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Johann_Elert_Bode\">Johann Elert Bode<\/a>&nbsp;taraf\u0131ndan ke\u015ffedildi.&nbsp;&nbsp;Bu nedenle bazen &#8220;Bode Galaksisi&#8221; olarak da an\u0131l\u0131r.&nbsp;1779&#8217;da&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Pierre_M%C3%A9chain\">Pierre M\u00e9chain<\/a>&nbsp;ve&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Charles_Messier\">Charles Messier<\/a>&nbsp;, Bode&#8217;un nesnesini yeniden tan\u0131mlad\u0131lar ve dolay\u0131s\u0131yla onu&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_object\">Messier Katalo\u011funda<\/a>&nbsp;listelediler .&nbsp;<\/p>\n\n\n\n<p><strong>Messier 82<\/strong>&nbsp;(ayr\u0131ca&nbsp;NGC 3034&nbsp;,&nbsp;Puro G\u00f6kadas\u0131&nbsp;veya&nbsp;M82&nbsp;olarak da bilinir ),&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Ursa_Major\">B\u00fcy\u00fck Ay\u0131&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Constellation\">tak\u0131my\u0131ld\u0131z\u0131<\/a>&nbsp;y\u00f6n\u00fcnde&nbsp;yakla\u015f\u0131k 12 milyon&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">\u0131\u015f\u0131ky\u0131l\u0131 uzakl\u0131kta bulunan&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Starburst_galaxy\">, y\u0131ld\u0131zlarla dolu bir g\u00f6kadad\u0131r<\/a>&nbsp;.&nbsp;12,52&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Parsec#Parsecs_and_kiloparsecs\">kiloparsek<\/a>&nbsp;(40.800&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Light-year\">\u0131\u015f\u0131ky\u0131l\u0131<\/a>&nbsp;)&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Galaxy#Isophotal_diameter\"> \u00e7ap\u0131yla<\/a>&nbsp;M81&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/M81_Group\">Grubunun<\/a>&nbsp;ikinci en b\u00fcy\u00fck \u00fcyesidir .&nbsp;&nbsp;Samanyolu&#8217;ndan&nbsp;yakla\u015f\u0131k be\u015f kat&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Luminosity#Astronomy\">daha parlakt\u0131r<\/a>&nbsp;ve merkez b\u00f6lgesi yakla\u015f\u0131k y\u00fcz kat daha parlakt\u0131r.&nbsp;&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Starburst_region\">Y\u0131ld\u0131z patlamas\u0131 aktivitesinin kom\u015fu galaksi&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_81\">M81<\/a>&nbsp;ile etkile\u015fim sonucu tetiklendi\u011fi d\u00fc\u015f\u00fcn\u00fcl\u00fcyor&nbsp;.&nbsp;D\u00fcnya&#8217;ya en yak\u0131n y\u0131ld\u0131z patlamas\u0131 galaksilerinden biri olan M82, bu galaksi tipinin prototip \u00f6rne\u011fidir.&nbsp;&nbsp;Bir&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Type_Ia_supernova\">tip Ia s\u00fcpernova olan&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/SN_2014J\">SN 2014J<\/a>&nbsp;, 21 Ocak 2014&#8217;te galakside ke\u015ffedildi.&nbsp;&nbsp;2014 y\u0131l\u0131nda, M82&#8217;yi incelerken bilim insanlar\u0131,&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/M82_X-2\">M82 olarak adland\u0131r\u0131lan, \u015fimdiye kadar bilinen en parlak pulsar\u0131 ke\u015ffettiler.&nbsp;<\/a><a href=\"https:\/\/en.wikipedia.org\/wiki\/M82_X-2\">X-2<\/a>&nbsp;.<\/p>\n\n\n\n<p>M82,&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Messier_81\">M81<\/a>&nbsp;ile birlikte 1774&#8217;te&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Johann_Elert_Bode\">Johann Elert Bode<\/a>&nbsp;taraf\u0131ndan ke\u015ffedildi. &nbsp;Bunu &#8220;bulutsu bir yama&#8221; olarak tan\u0131mlad\u0131, bu&nbsp;di\u011ferinden yakla\u015f\u0131k&nbsp;3 derece uzakta \u201c \u00e7ok soluk ve uzun \u015fekilli \u201c&nbsp; 1779&#8217;da&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Pierre_M%C3%A9chain\">Pierre M\u00e9chain<\/a>&nbsp;ba\u011f\u0131ms\u0131z olarak her iki nesneyi de yeniden ke\u015ffetti ve bunlar\u0131&nbsp;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Charles_Messier\">Charles Messier&#8217;e<\/a>&nbsp;bildirdi , o da bunlar\u0131 katalo\u011funa ekledi.<\/p>\n\n\n\n<p>Kaynak: <a href=\"https:\/\/wikipedia.org\">https:\/\/wikipedia.org<\/a><\/p>\n\n\n\n<p>Foto\u011fraf: U\u011fur \u0130K\u0130ZLER<br>Tarih: 20.06.2023<br>Saat: 01:12 &#8211; 03:10<br>Yer: Mudanya &#8211; Bursa 40.36023 \u00b0 N &#8211; 28.90191 \u00b0 E<\/p>\n\n\n\n<p>Optik (G\u00f6r\u00fcnt\u00fcleme): El yap\u0131m\u0131 Newton teleskop 150 mm f\/4.57<\/p>\n\n\n\n<p>TeleVue Paracorr Coma Corrector<br>Kundak: El yap\u0131m\u0131 kundak<br>Kamera (G\u00f6r\u00fcnt\u00fcleme): 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; 100 x 60 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>Messier 81&nbsp;(ayr\u0131ca&nbsp;NGC 3031&nbsp;veya&nbsp;Bode G\u00f6kadas\u0131&nbsp;olarak da bilinir ),&nbsp;B\u00fcy\u00fck Ay\u0131&nbsp;tak\u0131my\u0131ld\u0131z\u0131&nbsp;y\u00f6n\u00fcnde yakla\u015f\u0131k&nbsp;12 milyon&nbsp;\u0131\u015f\u0131ky\u0131l\u0131&nbsp;uzakl\u0131kta bulunan&nbsp;b\u00fcy\u00fck tasar\u0131ml\u0131 sarmal g\u00f6kadad\u0131r&nbsp;.&nbsp;29,44&nbsp;kiloparsek&nbsp;(96.000&nbsp;\u0131\u015f\u0131ky\u0131l\u0131&nbsp;)&nbsp;\u00e7ap\u0131ndad\u0131r.&nbsp;&nbsp;Samanyolu&nbsp;galaksisine g\u00f6receli yak\u0131nl\u0131\u011f\u0131 , b\u00fcy\u00fck boyutu ve&nbsp;aktif galaktik \u00e7ekirde\u011fi (70 milyon&nbsp;g\u00fcne\u015f &nbsp;&nbsp;k\u00fctleli kara deli\u011fi&nbsp;bar\u0131nd\u0131rmas\u0131&nbsp;nedeniyle&nbsp;, Messier 81 profesyonel g\u00f6kbilimciler&nbsp;taraf\u0131ndan kapsaml\u0131 bir \u015fekilde incelenmi\u015ftir&nbsp;.&nbsp;Galaksinin b\u00fcy\u00fck boyutu ve nispeten y\u00fcksek parlakl\u0131\u011f\u0131 da onu&nbsp;amat\u00f6r g\u00f6kbilimciler&nbsp;i\u00e7in pop\u00fcler bir hedef haline getiriyor .&nbsp;&nbsp;\u015eubat 2022&#8217;nin sonlar\u0131nda g\u00f6kbilimciler, M81&#8217;in tekrarlanan&nbsp;h\u0131zl\u0131&#8230;<\/p>\n","protected":false},"author":1,"featured_media":4382,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[25],"tags":[],"class_list":["post-4381","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-gokadalar","wpcat-25-id"],"jetpack_featured_media_url":"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M81-M82_1000x657.jpg?fit=1000%2C657&ssl=1","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4381","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/comments?post=4381"}],"version-history":[{"count":1,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4381\/revisions"}],"predecessor-version":[{"id":4383,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4381\/revisions\/4383"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media\/4382"}],"wp:attachment":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media?parent=4381"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/categories?post=4381"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/tags?post=4381"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}