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You entered: stellar evolution
![Планетарная туманность Эйбелл 7](https://images.astronet.ru/pubd/2022/05/23/0001833729/Abell_7-2022-02-20-HOO-1024.preview.jpg)
20.05.2022
Very faint planetary nebula Abell 7 is some 1,800 light-years distant, just south of Orion in planet Earth's skies in the constellation Lepus, The Hare. Surrounded by Milky Way stars and near...
![Остаток сверхновой Кеплера](https://images.astronet.ru/pubd/2004/10/08/0001199863/kepler_stsci_cg1.preview.jpg)
8.10.2004
Light from the stellar explosion that created this energized cosmic cloud was first seen on planet Earth in October 1604, a mere four hundred years ago. The supernova produced a bright new star in early 17th century skies within the constellation Ophiucus.
![Молодые звезды и пылевые туманности в Тельце](https://images.astronet.ru/pubd/2017/03/31/0001379220/LBN782ProcessedLRv1-2_1024.preview.jpg)
29.03.2017
This complex of dusty nebulae lingers along the edge of the Taurus molecular cloud, a mere 450 light-years distant. Stars are forming on the cosmic scene. Composed from almost 40 hours of image data...
![Туманность Ожерелье](https://images.astronet.ru/pubd/2010/11/03/0001247963/necklace_corradi900c.preview.jpg)
2.11.2010
The small constellation Sagitta sports this large piece of cosmic jewelry, dubbed the Necklace Nebula. The newly discovered example of a ring-shaped planetary nebula is about 15,000 light-years distant. Its bright ring with pearls of glowing gas is half a light-year across.
![Фи Персея: двойная звезда](https://images.astronet.ru/pubd/2003/08/18/0001192446/phiper_bpounds_big.preview.jpg)
11.12.1997
It's clear who is the biggest star in this binary system. Based on recent results, this artist's vision of the double star Phi Persei, 720 light years away, shows a bright, rapidly rotating massive star surrounded by a disk of gas. A small companion star orbits 100 million miles away.
![Двойная звезда φ Персея](https://images.astronet.ru/pubd/2006/11/12/0001217704/phiper_bpounds_big.preview.jpg)
2.10.1999
It's clear who is the biggest star in this binary system. Based on recent results, this artist's vision of the double star Phi Persei, 720 light years away, shows a bright, rapidly rotating massive star surrounded by a disk of gas. A small companion star orbits 100 million miles away.
![Остаток сверхновой Кеплера в рентгеновских лучах](https://images.astronet.ru/pubd/2007/01/16/0001220314/keplersnr_chandra.preview.jpg)
15.01.2007
What caused this mess? Some type of star exploded to create the unusually shaped nebula known as Kepler's supernova remnant, but which type? Light from the stellar explosion that created this energized cosmic cloud was first seen on planet Earth in October 1604, a mere four hundred years ago.
![Остаток сверхновой Кеплера в рентгеновских лучах](https://images.astronet.ru/pubd/2013/05/15/0001287429/keplersnr_chandra_960.preview.jpg)
15.05.2013
What caused this mess? Some type of star exploded to create the unusually shaped nebula known as Kepler's supernova remnant, but which type? Light from the stellar explosion that created this energized cosmic cloud was first seen on planet Earth in October 1604, a mere four hundred years ago.
![Медленный танец галактик NGC 5394 и 5395](https://images.astronet.ru/pubd/2020/03/04/0001626317/NGC5394n5_gemini_960.preview.jpg)
3.03.2020
If you like slow dances, then this may be one for you. A single turn in this dance takes several hundred million years. Two galaxies, NGC 5394 and NGC 5395, slowly whirl about each other in a gravitational interaction that sets off a flourish of sparks in the form of new stars.
![Кольцевая туманность вокруг WR 134](https://images.astronet.ru/pubd/2024/05/31/0001930720/NebulousRealmofWR134_1024.preview.png)
30.05.2024
Made with narrowband filters, this cosmic snapshot covers a field of view over twice as wide as the full Moon within the boundaries of the constellation Cygnus. It highlights the bright edge of a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas.
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