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You entered: NGC catalog
![Молодые звезды NGC 346](https://images.astronet.ru/pubd/2005/11/17/0001209555/ngc346_hst_l78.preview.jpg)
17.11.2005
Star cluster NGC 346 is embedded in the largest star forming region in the Small Magellanic Cloud, some 210,000 light-years distant. The massive stars of NGC 346 are short lived, but very energetic.
![NGC 869 & NGC 884: двойное звездное скопление](https://images.astronet.ru/pubd/2003/06/21/0001191061/ngc869_as.preview.jpg)
29.01.1997
Most star clusters are singularly impressive. But open clusters NGC 869 and NGC 884 are doubly impressive. Also known as "h and chi Persei", this rare double cluster, shown above, is bright enough to be seen from a dark location without even binoculars.
![Галактика Арп 94](https://images.astronet.ru/pubd/2013/10/09/0001294241/NGC3227_crawford950.preview.jpg)
9.10.2013
This telescopic snapshot records a cosmic moment in the tumultuous lives of large spiral galaxy NGC 3227 and smaller elliptical NGC 3226. Catching them in the middle of an ongoing gravitational dance, the sensitive imaging also follows faint tidal star streams flung from the galaxies in their repeated close encounters.
![NGC 869 и NGC 884: двойное рассеянное скопление](https://images.astronet.ru/pubd/2003/12/02/0001195433/doublecluster_fulbright.preview.jpg)
2.12.2003
Most star clusters are singularly impressive. Open clusters NGC 869 and NGC 884, however, are doubly impressive. Also known as "h and chi Persei", this unusual double cluster, shown above, is bright enough to be seen from a dark location without even binoculars.
![NGC 869 и NGC 884: двойное рассеянное скопление](https://images.astronet.ru/pubd/2005/10/11/0001208510/doublecluster_davis.preview.jpg)
11.10.2005
Most star clusters are singularly impressive. Open clusters NGC 869 and NGC 884, however, are doubly impressive. Also known as "h and chi Persei", this unusual double cluster, shown above, is bright enough to be seen from a dark location without even binoculars.
![Комета Хартли пролетает мимо двойного звёздного скопления](https://images.astronet.ru/pubd/2010/10/26/0001247801/hartleydouble_eder.preview.jpg)
26.10.2010
Most star clusters are singularly impressive. Open clusters NGC 869 and NGC 884, however, are doubly impressive. Also known as "h and chi Persei", this unusual double cluster, shown above, is bright enough to be seen from a dark location without even binoculars.
![NGC 6559: к востоку от Лагуны](https://images.astronet.ru/pubd/2021/10/07/0001769837/NGC6559Sartori1024.preview.jpg)
7.10.2021
Slide your telescope just east of the Lagoon Nebula to find this alluring field of view in the rich starfields of the constellation Sagittarius toward the central Milky Way. Of course the Lagoon nebula is also known as M8, the eighth object listed in Charles Messier's famous catalog of bright nebulae and star clusters.
![Арп 81: 100 миллионов лет спустя](https://images.astronet.ru/pubd/2003/12/11/0001195551/arp81_keel_c2.preview.jpg)
11.12.2003
From planet Earth, we view this strongly interacting pair of galaxies, cataloged as Arp 81, as they were only about 100 million years after their mutual closest approach. The havoc wreaked by gravity during...
![M8: туманность Лагуна](https://images.astronet.ru/pubd/2013/08/18/0001291989/M8_rural_hiresBobillo950.preview.jpg)
17.08.2013
This beautiful cosmic cloud is a popular stop on telescopic tours of the constellation Sagittarius. Eighteenth century cosmic tourist Charles Messier cataloged the bright nebula as M8. Modern day astronomers recognize the Lagoon Nebula as an active stellar nursery about 5,000 light-years distant, in the direction of the center of our Milky Way Galaxy.
![Пекулярная пара галактик Арп 87](https://images.astronet.ru/pubd/2007/11/01/0001224199/arp87web_c800.preview.jpg)
1.11.2007
A cosmic bridge of stars, gas, and dust stretches for over 75,000 light-years and joins this peculiar pair of galaxies cataloged as Arp 87. The bridge is strong evidence that these two immense star systems have passed close to each other and experienced violent tides induced by mutual gravity.
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