{"id":4416,"date":"2025-08-31T21:37:00","date_gmt":"2025-08-31T18:37:00","guid":{"rendered":"http:\/\/www.ikizler.org\/?p=4416"},"modified":"2025-12-25T00:27:18","modified_gmt":"2025-12-24T21:27:18","slug":"m-33-triangulum-gokadasi","status":"publish","type":"post","link":"http:\/\/www.ikizler.org\/index.php\/2025\/08\/31\/m-33-triangulum-gokadasi\/","title":{"rendered":"M 33 – Triangulum G\u00f6kadas\u0131"},"content":{"rendered":"\n
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\u00dc\u00e7gen G\u00f6kadas\u0131,<\/strong> D\u00fcnya’dan 2,73<\/a> milyon \u0131\u015f\u0131k y\u0131l\u0131<\/a> (\u0131y) uzakl\u0131kta, \u00dc\u00e7gen tak\u0131my\u0131ld\u0131z\u0131nda<\/a> bulunan sarmal<\/a> bir g\u00f6kadad\u0131r. Messier<\/strong><\/a> 33<\/strong> veya NGC<\/strong><\/a> 598<\/strong> olarak kataloglanm\u0131\u015ft\u0131r . 18,74 kiloparsek<\/a> (61.100 \u0131\u015f\u0131k y\u0131l\u0131<\/a> ) D \u00dc\u00e7gen G\u00f6kadas\u0131, <\/a>Andromeda G\u00f6kadas\u0131<\/a> ve Samanyolu’nun ard\u0131ndan <\/a>Yerel Grup<\/a> g\u00f6kadalar\u0131n\u0131n \u00fc\u00e7\u00fcnc\u00fc b\u00fcy\u00fck \u00fcyesidir.<\/p>\n\n\n\n

Galaksi, Macellan tipi<\/a> bir sarmal galaksi olan B\u00fcy\u00fck Macellan Bulutu’ndan<\/a> sonra Yerel Grup’taki<\/a> en k\u00fc\u00e7\u00fck ikinci sarmal galaksidir . ve gece g\u00f6ky\u00fcz\u00fcnde birbirlerine olan yak\u0131nl\u0131klar\u0131 nedeniyle Andromeda Galaksisi’nin<\/a> bir uydusu oldu\u011funa veya ikincisine geri d\u00f6nd\u00fc\u011f\u00fcne inan\u0131lmaktad\u0131r . Ayr\u0131ca bir H II <\/a>\u00e7ekirde\u011fine<\/a> sahiptir.<\/p>\n\n\n\n

I\u015f\u0131k kirlili\u011fi<\/a> olmayan ola\u011fan\u00fcst\u00fc iyi g\u00f6r\u00fcnt\u00fcleme ko\u015fullar\u0131 alt\u0131nda , \u00dc\u00e7gen G\u00f6kadas\u0131 baz\u0131 ki\u015filer taraf\u0131ndan tamamen karanl\u0131\u011fa adapte olmu\u015f \u00e7\u0131plak g\u00f6zle<\/a> g\u00f6r\u00fclebilir ; bu izleyicilere g\u00f6re, b\u00fcy\u00fctme olmadan g\u00f6r\u00fclebilen en uzak kal\u0131c\u0131 varl\u0131kt\u0131r ve Andromeda G\u00f6kadas\u0131 Messier 31’den yakla\u015f\u0131k yar\u0131 yar\u0131ya daha yak\u0131nd\u0131r. Fiziksel kapsam\u0131 nedeniyle, b\u00fcy\u00fctme olmadan bile y\u0131ld\u0131z benzeri bir noktadan ziyade da\u011f\u0131n\u0131k veya geni\u015flemi\u015f bir nesnedir.<\/p>\n\n\n\n

Optik yard\u0131m olmadan g\u00f6zlemlenebilirli\u011fi, karanl\u0131k, a\u00e7\u0131k ve \u015feffaf bir g\u00f6ky\u00fcz\u00fc alt\u0131nda derin k\u0131rsal alanlarda do\u011frudan g\u00f6r\u00fc\u015f kullanan ki\u015filer taraf\u0131ndan nispeten kolayca g\u00f6r\u00fclebilmesinden, iyi g\u00f6r\u00fcnt\u00fcleme ko\u015fullar\u0131 alt\u0131nda s\u0131\u011f k\u0131rsal alanlarda banliy\u00f6lerin \u00f6tesindeki yerlerdeki g\u00f6zlemciler taraf\u0131ndan \u00e7evrilmi\u015f g\u00f6r\u00fc\u015f\u00fcn kullan\u0131lmas\u0131n\u0131 gerektirmesine kadar de\u011fi\u015fir. <\/a>Bortle Karanl\u0131k G\u00f6ky\u00fcz\u00fc \u00d6l\u00e7e\u011fi’nin<\/a> referans nesnelerinden biridir.<\/p>\n\n\n\n

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

Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 31.08.2025
Saat: 01:13 – 03:59
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

TeleVue Paracorr Coma Corrector<\/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: 3200<\/p>\n\n\n\n

Poz: Light  247 x 30 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

\u00dc\u00e7gen G\u00f6kadas\u0131, \u00dc\u00e7gen tak\u0131my\u0131ld\u0131z\u0131 <\/a>y\u00f6n\u00fcnde<\/a> , D\u00fcnya’dan 2,73 milyon \u0131\u015f\u0131k y\u0131l\u0131  uzakl\u0131kta bulunan <\/a>sarmal<\/a> bir g\u00f6kadad\u0131r . Messier<\/a> 33 veya NGC ( <\/a>Yeni Genel Katalog)<\/em><\/a> 598 olarak kataloglanm\u0131\u015ft\u0131r . 18,74 kiloparseklik<\/a> (61.100 \u0131\u015f\u0131ky\u0131l\u0131<\/a> ) \u00e7ap\u0131yla \u00dc\u00e7gen G\u00f6kadas\u0131, Yerel G\u00f6kada Grubu’nun <\/a>Andromeda G\u00f6kadas\u0131<\/a> ve Samanyolu’nun<\/a> ard\u0131ndan \u00fc\u00e7\u00fcnc\u00fc en b\u00fcy\u00fck \u00fcyesidir .<\/p>\n\n\n\n

Galaksi, Yerel Gruptaki en k\u00fc\u00e7\u00fck sarmal g\u00f6kadad\u0131r (her ne kadar daha k\u00fc\u00e7\u00fck olan B\u00fcy\u00fck<\/a> ve K\u00fc\u00e7\u00fck Macellan Bulutlar\u0131<\/a> Samanyolu ile kar\u015f\u0131la\u015fmadan \u00f6nce sarmallar olmu\u015f olsalar da) ve Andromeda Galaksisinin bir uydusu ya da onun D\u00fcnya’ya geri d\u00f6nmekte oldu\u011funa inan\u0131lmaktad\u0131r. \u0130kincisi etkile\u015fimleri, h\u0131zlar\u0131  ve gece g\u00f6ky\u00fcz\u00fcnde birbirlerine yak\u0131nl\u0131klar\u0131 nedeniyle. Ayn\u0131 zamanda bir H II <\/a>\u00e7ekirde\u011fine<\/a> sahiptir . <\/p>\n\n\n\n

I\u015f\u0131k kirlili\u011finin<\/a> olmad\u0131\u011f\u0131 son derece iyi g\u00f6r\u00fcnt\u00fcleme ko\u015fullar\u0131 alt\u0131nda , \u00dc\u00e7gen G\u00f6kadas\u0131 baz\u0131 ki\u015filer taraf\u0131ndan tamamen karanl\u0131\u011fa uyarlanm\u0131\u015f \u00e7\u0131plak<\/a> g\u00f6zle g\u00f6r\u00fclebilmektedir.  Bu izleyicilere g\u00f6re, b\u00fcy\u00fctme olmadan g\u00f6r\u00fclebilen en uzak kal\u0131c\u0131 varl\u0131kt\u0131r ve Messier 31, Andromeda Galaksisi’nin yakla\u015f\u0131k yar\u0131s\u0131 kadard\u0131r. Fiziksel boyutundan dolay\u0131 b\u00fcy\u00fct\u00fclmese bile y\u0131ld\u0131z benzeri bir nokta yerine da\u011f\u0131n\u0131k veya uzat\u0131lm\u0131\u015f bir nesnedir.<\/p>\n\n\n\n

Optik yard\u0131m olmadan g\u00f6zlemlenebilirli\u011fi, karanl\u0131k, a\u00e7\u0131k, \u015feffaf bir g\u00f6ky\u00fcz\u00fc alt\u0131nda derin k\u0131rsal b\u00f6lgelerde do\u011frudan g\u00f6r\u00fc\u015f kullanan insanlar taraf\u0131ndan nispeten kolay g\u00f6r\u00fclebilmesinden , banliy\u00f6lerin \u00f6tesinde, s\u0131\u011f k\u0131rsal alanlardaki iyi g\u00f6r\u00fcnt\u00fcleme ko\u015fullar\u0131 alt\u0131nda yerlerdeki g\u00f6zlemciler taraf\u0131ndan \u00f6nlenmi\u015f g\u00f6r\u00fc\u015f\u00fcn<\/a> kullan\u0131lmas\u0131n\u0131 gerektirmesine kadar de\u011fi\u015fir.  Bortle Karanl\u0131k G\u00f6ky\u00fcz\u00fc \u00d6l\u00e7e\u011finin<\/a> referans nesnelerinden biridir .<\/p>\n\n\n\n

Crumey<\/a> , M33’\u00fcn toplam g\u00f6r\u00fcnen V-b\u00fcy\u00fckl\u00fc\u011f\u00fcn\u00fcn 5,72 olmas\u0131na ra\u011fmen, yakla\u015f\u0131k 6,6 etkili g\u00f6rsel b\u00fcy\u00fckl\u00fc\u011f\u00fcne sahip oldu\u011funu g\u00f6stermi\u015ftir; bu, g\u00f6r\u00fcn\u00fcrl\u00fck i\u00e7in bir \u00f6nko\u015fulun, g\u00f6zlemcinin y\u0131ld\u0131zlar\u0131 en az\u0131ndan bu son rakam kadar s\u00f6n\u00fck g\u00f6rebilmesi oldu\u011fu anlam\u0131na gelir.  Bu, \u00e7ok karanl\u0131k bir yerde bile bir\u00e7ok insan\u0131n g\u00f6rebilece\u011finden daha s\u00f6n\u00fckt\u00fcr. <\/p>\n\n\n\n

Galaksi ba\u011f\u0131ms\u0131z olarak Charles Messier<\/a> taraf\u0131ndan 25-26 A\u011fustos 1764 gecesi ke\u015ffedildi. Bulutsular ve Y\u0131ld\u0131z K\u00fcmeleri Katalo\u011fu’nda<\/em> (1771) 33 numaral\u0131 nesne olarak yay\u0131nland\u0131 ; dolay\u0131s\u0131yla M33 ad\u0131.  William Herschel, kapsaml\u0131 bulutsu katalo\u011funu derlerken, Messier taraf\u0131ndan tan\u0131mlanan nesnelerin \u00e7o\u011funu dahil etmemeye dikkat etti.  Ancak M33 bir istisnayd\u0131 ve bu nesneyi 11 Eyl\u00fcl 1784’te H V-17 olarak kataloglad\u0131.<\/p>\n\n\n\n

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

Foto\u011fraf: U\u011fur \u0130K\u0130ZLER
Tarih: 26.09.2023
Saat: 03:10 – 05:48
Yer: Mudanya – Bursa 40.36023 \u00b0 N – 28.90191 \u00b0 E<\/p>\n\n\n\n

Optik (G\u00f6r\u00fcnt\u00fcleme): EF 70-200mm f\/2.8L IS II USM  ( 200 mm-f\/2.8 )<\/p>\n\n\n\n

Canon Extender EF 2x III ( 400 mm f\/5.6 )<\/p>\n\n\n\n

Kundak: El yap\u0131m\u0131 kundak
Kamera (G\u00f6r\u00fcnt\u00fcleme): 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: 3200<\/p>\n\n\n\n

Poz: Light  116 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","protected":false},"excerpt":{"rendered":"

\u00dc\u00e7gen G\u00f6kadas\u0131, D\u00fcnya’dan 2,73 milyon \u0131\u015f\u0131k y\u0131l\u0131 (\u0131y) uzakl\u0131kta, \u00dc\u00e7gen tak\u0131my\u0131ld\u0131z\u0131nda bulunan sarmal bir g\u00f6kadad\u0131r. Messier 33 veya NGC 598 olarak kataloglanm\u0131\u015ft\u0131r . 18,74 kiloparsek (61.100 \u0131\u015f\u0131k y\u0131l\u0131 ) D \u00dc\u00e7gen G\u00f6kadas\u0131, Andromeda G\u00f6kadas\u0131 ve Samanyolu’nun ard\u0131ndan Yerel Grup g\u00f6kadalar\u0131n\u0131n \u00fc\u00e7\u00fcnc\u00fc b\u00fcy\u00fck \u00fcyesidir. Galaksi, Macellan tipi bir sarmal galaksi olan B\u00fcy\u00fck Macellan Bulutu’ndan sonra Yerel Grup’taki en k\u00fc\u00e7\u00fck ikinci sarmal galaksidir . ve gece g\u00f6ky\u00fcz\u00fcnde birbirlerine olan yak\u0131nl\u0131klar\u0131 nedeniyle Andromeda Galaksisi’nin bir uydusu oldu\u011funa veya ikincisine geri d\u00f6nd\u00fc\u011f\u00fcne inan\u0131lmaktad\u0131r . Ayr\u0131ca bir H II \u00e7ekirde\u011fine sahiptir. I\u015f\u0131k kirlili\u011fi olmayan ola\u011fan\u00fcst\u00fc iyi g\u00f6r\u00fcnt\u00fcleme ko\u015fullar\u0131 alt\u0131nda , \u00dc\u00e7gen…<\/p>\n","protected":false},"author":1,"featured_media":4417,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[10,25],"tags":[],"class_list":["post-4416","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-derin-uzay","category-gokadalar","wpcat-10-id","wpcat-25-id"],"jetpack_featured_media_url":"https:\/\/i0.wp.com\/www.ikizler.org\/wp-content\/uploads\/2023\/09\/M33_Triangulum_Galaksy_1000x691.jpg?fit=1000%2C691","jetpack_sharing_enabled":true,"_links":{"self":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4416","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=4416"}],"version-history":[{"count":2,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4416\/revisions"}],"predecessor-version":[{"id":5317,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/posts\/4416\/revisions\/5317"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media\/4417"}],"wp:attachment":[{"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/media?parent=4416"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/categories?post=4416"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/www.ikizler.org\/index.php\/wp-json\/wp\/v2\/tags?post=4416"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}