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You entered: NGC 300
![Шаровое скопление NGC 2419](https://images.astronet.ru/pubd/2009/01/23/0001232938/ngc2419a7_hammar_c800.preview.jpg)
23.01.2009
Of three objects prominent in this thoughtful telescopic image, a view toward the stealthy constellation Lynx, two (the spiky ones) are nearby stars. The third is the remote globular star cluster NGC 2419, at distance of nearly 300,000 light-years.
![NGC 520: сталкивающиеся галактики](https://images.astronet.ru/pubd/2021/09/07/0001760243/NGC520_HubbleOstling_960.preview.jpg)
7.09.2021
Is this one galaxy or two? The jumble of stars, gas, and dust that is NGC 520 is now thought to incorporate the remains of two separate disk galaxies. A defining component...
![NGC 247 с друзьями](https://images.astronet.ru/pubd/2020/01/16/0001599738/NGC247hager_1024.preview.jpg)
16.01.2020
About 70,000 light-years across, NGC 247 is a spiral galaxy smaller than our Milky Way. Measured to be only 11 million light-years distant it is nearby though. Tilted nearly edge-on as seen from our perspective, it dominates this telescopic field of view toward the southern constellation Cetus.
![Большая туманность в Киле](https://images.astronet.ru/pubd/2019/05/07/0001468820/CarinaWideField_Willasch_1080.preview.jpg)
7.05.2019
What's happening in the center of the Carina Nebula? Stars are forming, dying, and leaving an impressive tapestry of dark dusty filaments. The entire Carina Nebula, cataloged as NGC 3372, spans over 300 light years and lies about 8,500 light-years away in the constellation of Carina.
![В центре туманности Киля](https://images.astronet.ru/pubd/2024/02/05/0001919695/Carina_Taylor_960.preview.jpg)
5.02.2024
What's happening in the core of the Carina Nebula? Stars are forming, dying, and leaving an impressive tapestry of dark dusty filaments. The entire Carina Nebula, cataloged as NGC 3372, spans over 300 light years and lies about 8,500 light-years away in the constellation of Carina.
![NGC 4676: когда сталкиваются мыши](https://images.astronet.ru/pubd/2015/02/01/0001331704/mice_hubble_1080.preview.jpg)
31.01.2015
These two mighty galaxies are pulling each other apart. Known as the "Mice" because they have such long tails, each spiral galaxy has likely already passed through the other. The long tails are created by the relative difference between gravitational pulls on the near and far parts of each galaxy.
![Облака туманности Киля](https://images.astronet.ru/pubd/2016/05/16/0001362754/EtaCore_Ebersole_960.preview.jpg)
16.05.2016
What forms lurk in the mists of the Carina Nebula? The dark ominous figures are actually molecular clouds, knots of molecular gas and dust so thick they have become opaque. In comparison, however, these clouds are typically much less dense than Earth's atmosphere.
![Облака туманности Киля](https://images.astronet.ru/pubd/2021/05/03/0001737607/EtaCore_Ebersole_960.preview.jpg)
2.05.2021
What forms lurk in the mists of the Carina Nebula? The dark ominous figures are actually molecular clouds, knots of molecular gas and dust so thick they have become opaque. In comparison, however, these clouds are typically much less dense than Earth's atmosphere.
![Эллиптическая галактика NGC 1132](https://images.astronet.ru/pubd/2008/02/13/0001226181/ngc1132_hcst.preview.jpg)
13.02.2008
NGC 1132 is one smooth galaxy -- but how did it form? As an elliptical galaxy, NGC 1132 has little dust and gas, and few stars have formed in it recently. Although many elliptical galaxies are in clusters of galaxies, NGC 1132 appears as a large, isolated galaxy toward the constellation of the River (Eridanus).
![NGC 4676: столкновение "мышек"](https://images.astronet.ru/pubd/2004/06/12/0001198383/ngc4676_hst_c1.preview.jpg)
12.06.2004
These two mighty galaxies are pulling each other apart. Known as "The Mice" because they have such long tails, each spiral galaxy has likely already passed through the other. They will probably collide again and again until they coalesce.
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