{"id":5339,"date":"2025-10-20T23:36:00","date_gmt":"2025-10-20T20:36:00","guid":{"rendered":"https:\/\/www.ikizler.org\/?p=5339"},"modified":"2025-12-25T00:25:17","modified_gmt":"2025-12-24T21:25:17","slug":"m16-kartal-ve-m17-omega-bulutsulari","status":"publish","type":"post","link":"https:\/\/www.ikizler.org\/index.php\/2025\/10\/20\/m16-kartal-ve-m17-omega-bulutsulari\/","title":{"rendered":"M16 Kartal ve M17 Omega Bulutsular\u0131"},"content":{"rendered":"\n
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\"\"<\/figure>\n<\/figure>\n\n\n\n

Kartal Bulutsusu<\/strong> ( Massier 16<\/strong> veya M16<\/strong> ve NGC 6611<\/strong> olarak kataloglanm\u0131\u015ft\u0131r ve ayr\u0131ca Y\u0131ld\u0131z Krali\u00e7esi Bulutsusu olarak <\/strong>da bilinir), <\/a>Jean-Philippe de Cheseaux<\/a> taraf\u0131ndan 1745-46’da ke\u015ffedilen Y\u0131lan tak\u0131my\u0131ld\u0131z\u0131ndaki<\/a> gen\u00e7 bir a\u00e7\u0131k <\/a>y\u0131ld\u0131z<\/a> k\u00fcmesidir . Hem “Kartal” hem de “Y\u0131ld\u0131z Krali\u00e7esi”, bulutsunun merkezine yak\u0131n karanl\u0131k sil\u00fcetin g\u00f6rsel izlenimlerine at\u0131fta bulunur,  bu alan Hubble Uzay Teleskobu<\/a> taraf\u0131ndan g\u00f6r\u00fcnt\u00fclenen ” Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131<\/a> ” olarak \u00fcnlenmi\u015ftir . Bulutsu,<\/a> yukar\u0131da bahsedilen Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131 da dahil olmak \u00fczere birka\u00e7 aktif y\u0131ld\u0131z olu\u015fturan <\/a>gaz ve toz<\/a> b\u00f6lgesi i\u00e7erir. Kartal Bulutsusu, Samanyolu’nun Yay <\/a>Kolu’nda<\/a> yer al\u0131r.<\/p>\n\n\n\n

Kartal Bulutsusu, IC 4703<\/strong> olarak kataloglanan da\u011f\u0131n\u0131k bir emisyon bulutsusu<\/a> veya H II b\u00f6lgesidir<\/a> . Aktif y\u0131ld\u0131z olu\u015fumunun ger\u00e7ekle\u015fti\u011fi bu b\u00f6lge yakla\u015f\u0131k 5700 \u0131\u015f\u0131k y\u0131l\u0131 uzakl\u0131ktad\u0131r. <\/a>Bulutsunun<\/a> kuzeydo\u011fu kesiminde g\u00f6r\u00fclebilen bir gaz sivri ucu yakla\u015f\u0131k 9,5 \u0131\u015f\u0131k y\u0131l\u0131 veya yakla\u015f\u0131k 90 trilyon kilometre uzunlu\u011fundad\u0131r. <\/a><\/p>\n\n\n\n

Bulutsu ile ili\u015fkili k\u00fcme, \u00e7o\u011funlukla S\u00fctunlar\u0131n kuzeybat\u0131s\u0131ndaki molek\u00fcler buluttaki bir bo\u015flukta yo\u011funla\u015fm\u0131\u015f yakla\u015f\u0131k 8100 y\u0131ld\u0131za sahiptir.  En parlak y\u0131ld\u0131z (HD 168076), iyi bir d\u00fcrb\u00fcnle kolayca g\u00f6r\u00fclebilen +8,24’l\u00fck bir g\u00f6r\u00fcn\u00fcr kadire<\/a> sahiptir . Asl\u0131nda, bir O3,5V y\u0131ld\u0131z<\/a> ve bir O7,5V arkada\u015f\u0131ndan olu\u015fan bir ikili y\u0131ld\u0131zd\u0131r<\/a> .  Bu y\u0131ld\u0131z\u0131n k\u00fctlesi yakla\u015f\u0131k 80 g\u00fcne\u015f k\u00fctlesi ve <\/a>G\u00fcne\u015f’in<\/a> 1 milyon kat\u0131na kadar bir parlakl\u0131\u011fa sahiptir . K\u00fcmenin ya\u015f\u0131n\u0131n 1-2 milyon y\u0131l oldu\u011fu tahmin edilmektedir. <\/p>\n\n\n\n

Tan\u0131mlay\u0131c\u0131 isimler, g\u00fcneydo\u011fudan merkezi \u0131\u015f\u0131kl\u0131 alana do\u011fru y\u00fckselen merkezi s\u00fctunun \u015feklinin izlenimlerini yans\u0131tmaktad\u0131r. “Y\u0131ld\u0131z Krali\u00e7esi Bulutsusu” ad\u0131, Robert Burnham Jr.<\/a> taraf\u0131ndan , merkezi s\u00fctunun sil\u00fcet halinde g\u00f6sterilen Y\u0131ld\u0131z Krali\u00e7esi olarak nitelendirilmesini yans\u0131tacak \u015fekilde ortaya at\u0131lm\u0131\u015ft\u0131r.<\/p>\n\n\n\n

M 17 Omega Bulutsusu<\/p>\n\n\n\n

Omega Bulutsusu, <\/strong>Yay tak\u0131my\u0131ld\u0131z\u0131ndaki<\/a> bir H II b\u00f6lgesidir<\/a> . 1745 y\u0131l\u0131nda Philippe Loys de Ch\u00e9seaux<\/a> taraf\u0131ndan ke\u015ffedilmi\u015ftir. Charles <\/a>Messier 1764 y\u0131l\u0131nda kataloglam\u0131\u015ft\u0131r. <\/a>Samanyolu’nun<\/a> en zengin y\u0131ld\u0131z alanlar\u0131ndan baz\u0131lar\u0131na sahiptir ve Yay tak\u0131my\u0131ld\u0131z\u0131n\u0131n kuzeydeki \u00fc\u00e7te ikilik k\u0131sm\u0131nda yer al\u0131r. Bu \u00f6zellik ayr\u0131ca Ku\u011fu Bulutsusu<\/strong> , \u0130\u015faret Bulutsusu<\/strong> , Istakoz Bulutsusu<\/strong> ve At Nal\u0131 Bulutsusu<\/strong> olarak da bilinir ve Messier 17<\/strong> veya M17<\/strong> veya NGC 6618<\/strong> olarak kataloglanm\u0131\u015ft\u0131r .<\/p>\n\n\n\n

Omega Bulutsusu, D\u00fcnya’dan<\/a> 5.000 ila 6.000 \u0131\u015f\u0131k y\u0131l\u0131<\/a> uzakl\u0131kta olup yakla\u015f\u0131k 15 \u0131\u015f\u0131k y\u0131l\u0131 \u00e7ap\u0131ndad\u0131r. Bu bulutsunun bir par\u00e7as\u0131 olan <\/a>y\u0131ld\u0131zlararas\u0131 madde<\/a> bulutu yakla\u015f\u0131k 40 \u0131\u015f\u0131k y\u0131l\u0131 \u00e7ap\u0131ndad\u0131r ve 30.000 g\u00fcne\u015f k\u00fctlesine sahiptir. Omega Bulutsusu’nun toplam k\u00fctlesi<\/a> tahmini 800 g\u00fcne\u015f k\u00fctlesidir<\/a> .<\/p>\n\n\n\n

Galaksimizin en parlak ve en b\u00fcy\u00fck y\u0131ld\u0131z olu\u015fum b\u00f6lgelerinden biri olarak kabul edilir. Yerel geometrisi, Orion Bulutsusu’na<\/a> benzer, ancak \u00f6nden de\u011fil kenardan bak\u0131larak g\u00f6r\u00fcl\u00fcr. <\/p>\n\n\n\n

A\u00e7\u0131k k\u00fcme<\/a> NGC 6618, bulutsunun i\u00e7ine g\u00f6m\u00fcl\u00fcd\u00fcr ve bu s\u0131cak, gen\u00e7 y\u0131ld\u0131zlardan gelen <\/a>radyasyon<\/a> nedeniyle bulutsunun gazlar\u0131n\u0131n<\/a> parlamas\u0131na neden olur ; ancak bulutsudaki ger\u00e7ek y\u0131ld\u0131z say\u0131s\u0131 \u00e7ok daha y\u00fcksektir – 800’e kadar, 100’\u00fc B9’dan \u00f6nceki spektral tipte ve 9’u <\/a>O spektral tipte<\/a> art\u0131 d\u0131\u015f b\u00f6lgelerinde olu\u015fum halinde binden fazla y\u0131ld\u0131z.  En gen\u00e7 k\u00fcmelerden biridir. <\/p>\n\n\n\n

Bulutsunun g\u00fcneydo\u011fu kesiminde yer alan parlak mavi de\u011fi\u015fken y\u0131ld\u0131z<\/a> HD 168607’nin genellikle onunla ili\u015fkili oldu\u011fu varsay\u0131l\u0131r; yak\u0131n kom\u015fusu olan mavi <\/a>dev y\u0131ld\u0131z <\/a>HD 168625<\/a> de \u00f6yle olabilir.<\/p>\n\n\n\n

Yay <\/a>bulutsusundaki<\/a> Omega Bulutsusu olan M17’nin Ku\u011fu k\u0131sm\u0131, bir berber dire\u011fine<\/a> benzetilmektedir . <\/p>\n\n\n\n

Kaynak: https:\/\/en.wikipedia.org<\/a><\/p>\n\n\n\n

Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 20.10.2025
Saat: 20:38 – 21:43
Yer: Mudanya – Bursa 40.36023 \u00b0 N – 28.90191 \u00b0 E<\/p>\n\n\n\n

Canon Extender EF 2x III<\/p>\n\n\n\n

Optik : Canon EF 70-200mm f\/2.8L IS II USM  ( 400 mm-f\/5.6 )<\/p>\n\n\n\n

Kundak: El yap\u0131m\u0131 kundak
Kamera : Canon EOS 6D Full Spectrum Modified<\/p>\n\n\n\n

Otomatik takip: PHD, Bower mirror lens  500 mm f\/6.3- ZWO ASI 120 MC-S<\/p>\n\n\n\n

ISO: 1600<\/p>\n\n\n\n

Poz: Light  40 x 90 sn. \u2013 Dark 30 \u2013 Flat 20 \u2013 Bias 25<\/p>\n\n\n\n

Yaz\u0131l\u0131m: Pix\u0130nsight 1.8, Photoshop CC 2015<\/p>\n","protected":false},"excerpt":{"rendered":"

Kartal Bulutsusu ( Massier 16 veya M16 ve NGC 6611 olarak kataloglanm\u0131\u015ft\u0131r ve ayr\u0131ca Y\u0131ld\u0131z Krali\u00e7esi Bulutsusu olarak da bilinir), Jean-Philippe de Cheseaux taraf\u0131ndan 1745-46’da ke\u015ffedilen Y\u0131lan tak\u0131my\u0131ld\u0131z\u0131ndaki gen\u00e7 bir a\u00e7\u0131k y\u0131ld\u0131z k\u00fcmesidir . Hem “Kartal” hem de “Y\u0131ld\u0131z Krali\u00e7esi”, bulutsunun merkezine yak\u0131n karanl\u0131k sil\u00fcetin g\u00f6rsel izlenimlerine at\u0131fta bulunur,  bu alan Hubble Uzay Teleskobu taraf\u0131ndan g\u00f6r\u00fcnt\u00fclenen ” Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131 ” olarak \u00fcnlenmi\u015ftir . Bulutsu, yukar\u0131da bahsedilen Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131 da dahil olmak \u00fczere birka\u00e7 aktif y\u0131ld\u0131z olu\u015fturan gaz ve toz b\u00f6lgesi i\u00e7erir. Kartal Bulutsusu, Samanyolu’nun Yay Kolu’nda yer al\u0131r….<\/p>\n","protected":false},"author":1,"featured_media":5340,"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-5339","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\/M16_M17.jpg?fit=1000%2C668&ssl=1","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5339","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=5339"}],"version-history":[{"count":1,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5339\/revisions"}],"predecessor-version":[{"id":5341,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/5339\/revisions\/5341"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media\/5340"}],"wp:attachment":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media?parent=5339"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/categories?post=5339"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/tags?post=5339"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}