File:Supernova SN 2017eaw in a galaxy NGC 6946.png

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English: A supernova in a galaxy NGC 6946 "Fireworks" (marked by dashes). Its brightness on the peak was comparable with the total brightness of the whole galaxy. This is the tenth supernova in this galaxy observed during the last 100 years. Insets: evolution of a visible color of the supernova: from bluish at early stages to reddish at later stage. Other stars in the image belong to our Milky Way galaxy.
Українська: Наднова у галактиці NGC 6946 "Фейєрверк" (відмічена рисками). Яскравість наднової (результату гравітаційного колапсу масивної зірки, що витратила термоядерне паливо) на піку яскравості порівняна з яскравістю всієї галактики. Це десята наднова в цій галактиці за 100 років спостережень. Врізки: зміна видимого кольору наднової: з блакитного відтінку на початку до червонуватого на кінцевих стадіях. Інші зірки на зображенні належать до нашої Галактики -- Чумацького Шляху. Фотографія отримана за допомогою телескопа-рефлектора діаметром 150мм f/5 на екваторіальному монтуванні з трекінгом і цифрової дзеркальної камери. Київ.
English: A supernova in a galaxy NGC 6946 "Fireworks" (marked by dashes). Its brightness on the peak was comparable with the total brightness of the whole galaxy. Other stars in the image belong to our Milky Way galaxy. This is the tenth supernova in this galaxy observed during the last 100 years. Insets: evolution of a visible color of the supernova: from bluish at early stages to reddish at later stage. The picture was taken using 150/750 Newtonian on motorized equatorial mount and DSLR camera.
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Author Mpyat2
Camera location50° 22′ 54.61″ N, 30° 37′ 35.4″ E Kartographer map based on OpenStreetMap.View this and other nearby images on: OpenStreetMapinfo

The picture was taken using SkyWatcher 150/750 Newtonian on EQ5 mount with motor drives with Canon EOS600D as an imaging camera.

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current19:29, 4 November 2017Thumbnail for version as of 19:29, 4 November 2017700 × 1,000 (1.03 MB)Mpyat2 (talk | contribs)User created page with UploadWizard

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