Sarmal yap\u0131s\u0131yla dikkat \u00e7eken Messier 77, merkezindeki aktif \u00e7ekirde\u011fi nedeniyle astronomlar aras\u0131nda uzun s\u00fcredir \u00f6zel bir ilgi g\u00f6r\u00fcyor. Galaksinin parlak kalbinde, k\u00fctlesi G\u00fcne\u015f’in 8 milyon kat\u0131na ula\u015fan bir s\u00fcper k\u00fctleli kara delik bulunuyor. Kara deli\u011fin \u00e7evresinde d\u00f6nen gaz, a\u015f\u0131r\u0131 \u0131s\u0131narak ola\u011fan\u00fcst\u00fc yo\u011funlukta \u0131\u015f\u0131ma yap\u0131yor. Webb’in orta k\u0131z\u0131l\u00f6tesi enstr\u00fcman\u0131, bu b\u00f6lgenin daha \u00f6nce hi\u00e7 bu denli net g\u00f6r\u00fclmemi\u015f ayr\u0131nt\u0131lar\u0131n\u0131 yakalad\u0131.<\/p>\n\n\n\n
Messier 77, hem g\u00f6rece yak\u0131n konumu hem de g\u00f6zlemlenebilir \u00f6zellikleri a\u00e7\u0131s\u0131ndan aktif galaksi \u00e7ekirdeklerini incelemek i\u00e7in ideal bir laboratuvar niteli\u011fi ta\u015f\u0131yor. Webb’in k\u0131z\u0131l\u00f6tesi duyarl\u0131l\u0131\u011f\u0131, toz bulutlar\u0131n\u0131n ard\u0131na gizlenmi\u015f bu yap\u0131lar\u0131 g\u00f6r\u00fcn\u00fcr \u0131\u015f\u0131k teleskoplar\u0131n\u0131n ula\u015famad\u0131\u011f\u0131 bir netlikte ortaya koyuyor.<\/p>\n\n\n\n
2021’de f\u0131rlat\u0131lan Webb, evrenin en uzak k\u00f6\u015felerinden g\u00fcne\u015f sistemimizin gezegenlerine kadar geni\u015f bir yelpazede \u00e7\u0131\u011f\u0131r a\u00e7an g\u00f6zlemler yapmay\u0131 s\u00fcrd\u00fcr\u00fcyor.<\/p>\n\n\n\n
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