{"id":3788,"date":"2025-10-10T09:09:00","date_gmt":"2025-10-10T06:09:00","guid":{"rendered":"http:\/\/www.ikizler.org\/?p=3788"},"modified":"2025-12-25T00:25:38","modified_gmt":"2025-12-24T21:25:38","slug":"m-16-kartal-bulutsusu","status":"publish","type":"post","link":"https:\/\/www.ikizler.org\/index.php\/2025\/10\/10\/m-16-kartal-bulutsusu\/","title":{"rendered":"M 16 – Kartal Bulutsusu"},"content":{"rendered":"\n
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Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 10.10.2025
Saat: 20:06 – 20:56
Yer: Mudanya – Bursa 40.36023 \u00b0 N – 28.90191 \u00b0 E<\/p>\n\n\n\n

Optik : El yap\u0131m\u0131 Newton teleskop 150 mm f\/4.57<\/p>\n\n\n\n

Kundak: El yap\u0131m\u0131 kundak
TeleVue Paracorr Coma Corrector<\/p>\n\n\n\n

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  42 x 60 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\n\n\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

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

Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 18.06.2025
Saat: 01:36 – 04:05
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  127 x 60 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\n\n\n

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\"\"<\/figure>\n<\/figure>\n\n\n\n

M 16 \u2013 Kartal Bulutsusu<\/p>\n\n\n\n

Kartal Bulutsusu (Katalogda Messier 16 veya M16 ve NGC 6611 ve ayr\u0131ca Y\u0131ld\u0131z Krali\u00e7e Bulutsusu olarak da bilinir), Jean-Philippe de Cheseaux taraf\u0131ndan 1745-46’da ke\u015ffedilen Serpens tak\u0131my\u0131ld\u0131z\u0131nda bulunan gen\u00e7 bir a\u00e7\u0131k y\u0131ld\u0131z k\u00fcmesidir. Hem “Kartal” hem de “Y\u0131ld\u0131z Krali\u00e7esi”, Hubble Uzay Teleskobu taraf\u0131ndan g\u00f6r\u00fcnt\u00fclenen “Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131” olarak \u00fcnlenen bir alan olan bulutsunun merkezine yak\u0131n karanl\u0131k siluetin g\u00f6rsel izlenimlerini ifade eder. 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\n\n\n

Kartal Bulutsusu, IC 4703 olarak kataloglanan da\u011f\u0131n\u0131k salma bulutsusu veya H II b\u00f6lgesinin bir par\u00e7as\u0131d\u0131r. Aktif ak\u0131m y\u0131ld\u0131z olu\u015fumunun bu b\u00f6lgesi yakla\u015f\u0131k 5700 \u0131\u015f\u0131ky\u0131l\u0131 uzakl\u0131ktad\u0131r. Kuzeydo\u011fu kesimde nebuladan \u00e7\u0131kt\u0131\u011f\u0131 g\u00f6r\u00fclebilen bir gaz kulesi yakla\u015f\u0131k 9,5 \u0131\u015f\u0131ky\u0131l\u0131 veya yakla\u015f\u0131k 90 trilyon kilometre uzunlu\u011fundad\u0131r.<\/p>\n\n\n\n

Bulutsu ile ili\u015fkili k\u00fcme, \u00e7o\u011funlukla S\u00fctunlar\u0131n kuzey bat\u0131s\u0131ndaki molek\u00fcler buluttaki bir bo\u015flukta yo\u011funla\u015fan 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 kadir kadirdir. Asl\u0131nda bir O3.5V y\u0131ld\u0131z\u0131 ve bir O7.5V yolda\u015f\u0131ndan olu\u015fan ikili bir y\u0131ld\u0131zd\u0131r. Bu y\u0131ld\u0131z\u0131n k\u00fctlesi yakla\u015f\u0131k 80 g\u00fcne\u015f k\u00fctlesi ve G\u00fcne\u015f’inkinin 1 milyon kat\u0131 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 ayd\u0131nl\u0131k alana do\u011fru y\u00fckselen merkezi s\u00fctunun \u015feklinin izlenimlerini yans\u0131t\u0131r. “Y\u0131ld\u0131z Krali\u00e7e Bulutsusu” ad\u0131, Robert Burnham, Jr. taraf\u0131ndan tan\u0131t\u0131ld\u0131 ve merkez s\u00fctunu siluette g\u00f6sterilen Y\u0131ld\u0131z Krali\u00e7e olarak nitelendirmesini yans\u0131tt\u0131.<\/p>\n\n\n\n

Jeff Hester ve Paul Scowen taraf\u0131ndan 1995 y\u0131l\u0131nda Hubble Uzay Teleskobu kullan\u0131larak \u00fcretilen g\u00f6r\u00fcnt\u00fcler, bulutsu i\u00e7indeki s\u00fcre\u00e7lerin bilimsel olarak anla\u015f\u0131lmas\u0131n\u0131 b\u00fcy\u00fck \u00f6l\u00e7\u00fcde geli\u015ftirdi. Bunlardan biri, geni\u015f bir y\u0131ld\u0131z olu\u015fum b\u00f6lgesini betimleyen “Yarat\u0131l\u0131\u015f S\u00fctunlar\u0131” olarak \u00fcnlendi. K\u00fc\u00e7\u00fck karanl\u0131k ceplerinin \u00f6ny\u0131ld\u0131zlar oldu\u011funa inan\u0131l\u0131yor. S\u00fctun yap\u0131s\u0131, 2005 y\u0131l\u0131nda Spitzer Uzay Teleskobu ile g\u00f6r\u00fcnt\u00fclenen Cassiopeia’n\u0131n Ruh Bulutsusu’ndaki \u00e7ok daha b\u00fcy\u00fck bir \u00f6rne\u011fe benzemektedir, ayn\u0131 \u015fekilde “Y\u0131ld\u0131z Yarat\u0131m\u0131 S\u00fctunlar\u0131” olarak nitelendirilmi\u015ftir. veya “Y\u0131ld\u0131z Olu\u015fumunun S\u00fctunlar\u0131”. Bir ma\u011faran\u0131n taban\u0131ndan \u00e7\u0131k\u0131nt\u0131 yapan dikitlere benzeyen bu s\u00fctunlar, yeni y\u0131ld\u0131zlar i\u00e7in kulu\u00e7ka makinesi g\u00f6revi g\u00f6ren y\u0131ld\u0131zlararas\u0131 hidrojen gaz\u0131 ve tozdan olu\u015fur. S\u00fctunlar\u0131n i\u00e7inde ve y\u00fczeylerinde g\u00f6kbilimciler, YUMURTA (“Buharla\u015fan Gaz K\u00fcreleri”) ad\u0131 verilen daha yo\u011fun gaz d\u00fc\u011f\u00fcmleri veya k\u00fcrecikleri buldular. Bunlar\u0131n baz\u0131lar\u0131n\u0131n i\u00e7inde y\u0131ld\u0131zlar olu\u015fuyor.<\/p>\n\n\n\n

Chandra g\u00f6zlemevinden al\u0131nan X-\u0131\u015f\u0131n\u0131 g\u00f6r\u00fcnt\u00fcleri, Hubble’\u0131n “S\u00fctunlar” g\u00f6r\u00fcnt\u00fcs\u00fcyle kar\u015f\u0131la\u015ft\u0131r\u0131ld\u0131\u011f\u0131nda, X-\u0131\u015f\u0131n\u0131 kaynaklar\u0131n\u0131n (gen\u00e7 y\u0131ld\u0131zlardan gelen) s\u00fctunlarla \u00f6rt\u00fc\u015fmedi\u011fini, aksine bulutsuyu rastgele noktalad\u0131\u011f\u0131n\u0131 g\u00f6stermi\u015ftir. S\u00fctunlar\u0131n EGG’lerindeki herhangi bir \u00f6ny\u0131ld\u0131z hen\u00fcz X-\u0131\u015f\u0131nlar\u0131 yayacak kadar s\u0131cak de\u011fil.[kaynak belirtilmeli]<\/p>\n\n\n\n

Spitzer Uzay Teleskobu’ndan elde edilen kan\u0131tlar, ba\u015flang\u0131\u00e7ta M16’daki s\u00fctunlar\u0131n “ge\u00e7mi\u015f bir s\u00fcpernova” taraf\u0131ndan tehdit edilebilece\u011fini \u00f6ne s\u00fcrd\u00fc. Spitzer taraf\u0131ndan 2007’de g\u00f6zlemlenen s\u0131cak gaz, onlar\u0131n zaten – b\u00fcy\u00fck olas\u0131l\u0131kla – 8.000 ila 9.000 y\u0131l \u00f6nce patlayan bir s\u00fcpernova taraf\u0131ndan rahats\u0131z edildi\u011fini \u00f6ne s\u00fcrd\u00fc. Uzakl\u0131k nedeniyle, ana \u0131\u015f\u0131k patlamas\u0131 1.000 ila 2.000 y\u0131l \u00f6nce k\u0131sa bir s\u00fcre i\u00e7in D\u00fcnya’ya ula\u015fm\u0131\u015f olacakt\u0131. Daha yava\u015f hareket eden, kuramsalla\u015ft\u0131r\u0131lm\u0131\u015f bir \u015fok dalgas\u0131n\u0131n bulutsunun i\u00e7inden ge\u00e7mesi birka\u00e7 bin y\u0131l alacak ve hassas s\u00fctunlar\u0131 havaya u\u00e7uracakt\u0131. Bununla birlikte, 2014 y\u0131l\u0131nda s\u00fctunlar Hubble taraf\u0131ndan hem g\u00f6r\u00fcn\u00fcr \u0131\u015f\u0131kta hem de k\u0131z\u0131l\u00f6tesi \u0131\u015f\u0131kta ikinci kez g\u00f6r\u00fcnt\u00fclendi. 20 y\u0131l sonraki g\u00f6r\u00fcnt\u00fcler, s\u00fctunlar i\u00e7inde meydana gelen buharla\u015fma h\u0131z\u0131n\u0131n yeni ve ayr\u0131nt\u0131l\u0131 bir hesab\u0131n\u0131 sa\u011flad\u0131. \u0130\u00e7lerinde hi\u00e7bir s\u00fcpernova kan\u0131tlanmam\u0131\u015ft\u0131r ve bir \u015fekilde hala var olduklar\u0131 ve en az 100.000 y\u0131l daha ortaya \u00e7\u0131kacaklar\u0131 tahmin edilmektedir.<\/p>\n\n\n\n

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

Obje Ad\u0131: M 16 \u2013 Kartal Bulutsusu<\/p>\n\n\n\n

Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 20.07.2022
Saat: 00:46 – 03:04
Yer: Mudanya – Bursa 40.36023 \u00b0 N – 28.90191 \u00b0 E<\/p>\n\n\n\n

Optik (G\u00f6r\u00fcnt\u00fcleme): El yap\u0131m\u0131 Newton teleskop 150 mm f\/4.57<\/p>\n\n\n\n

TeleVue Paracorr Coma Corrector
Kundak: El yap\u0131m\u0131 kundak
Kamera (G\u00f6r\u00fcnt\u00fcleme): Canon EOS 6D Beader Astro Conversion Filter 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: 2000<\/p>\n\n\n\n

Poz: Light  90 x 60 sn. \u2013 Dark 30 \u2013 Flat 20 \u2013 Bias 25 Yaz\u0131l\u0131m: Pix\u0130nsight 1.8, Photoshop CC 2015<\/p>\n","protected":false},"excerpt":{"rendered":"

Foto\u011fraf: U\u011fur \u0130K\u0130ZLERTarih: 10.10.2025Saat: 20:06 – 20:56Yer: Mudanya – Bursa 40.36023 \u00b0 N – 28.90191 \u00b0 E Optik : El yap\u0131m\u0131 Newton teleskop 150 mm f\/4.57 Kundak: El yap\u0131m\u0131 kundakTeleVue Paracorr Coma Corrector Kamera : Canon EOS 6D Full Spectrum Modified Otomatik takip: PHD, Bower mirror lens  500 mm f\/6.3- ZWO ASI 120 MC-S ISO:…<\/p>\n","protected":false},"author":1,"featured_media":5322,"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-3788","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\/06\/M16.jpg?fit=1000%2C685&ssl=1","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/3788","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=3788"}],"version-history":[{"count":3,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/3788\/revisions"}],"predecessor-version":[{"id":5324,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/3788\/revisions\/5324"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media\/5322"}],"wp:attachment":[{"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media?parent=3788"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/categories?post=3788"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/tags?post=3788"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}