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Keywords: LMC, Tarantula Nebula, 30 Doradus
![Туманность Тарантул](https://images.astronet.ru/pubd/2006/01/06/0001210818/tarantula_moore_fr1.preview.jpg)
5.01.2006
First cataloged as a star, 30 Doradus is actually an immense star forming region in nearby galaxy The Large Magellanic Cloud. The region's spidery appearance is responsible for its popular name, the Tarantula Nebula, except that this tarantula is about 1,000 light-years across, and 180,000 light-years away in the southern constellation Dorado.
![Большое Магелланово Облако в инфракрасном свете](https://images.astronet.ru/pubd/2006/09/04/0001216127/lmc_spitzer.preview.jpg)
4.09.2006
Where does dust collect in galaxies? To help find out, a team of researchers took the most detailed image ever of gas clouds and dust in the neighboring Large Magellanic Cloud (LMC) galaxy.
![В центре области звездообразования 30 Золотой Рыбы](https://images.astronet.ru/pubd/2002/08/26/0001179350/30doradus_hst_big.preview.gif)
24.05.1996
In the center of 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. The center of this cluster, known as R136, is boxed in the upper right portion of the above picture.
![Комплекс N44](https://images.astronet.ru/pubd/2008/03/27/0001227002/N44NNBWeb2_goldman_c800.preview.jpg)
26.03.2008
A truly giant complex of emission nebulae, N44 is about 1,000 light-years across. It shines in southern skies as a denizen of our neighboring galaxy, the Large Magellanic Cloud, 170,000 light-years away.
![Туманность N44F, принесенная ветром](https://images.astronet.ru/pubd/2004/08/19/0001199347/n44f_hst_c1.preview.jpg)
19.08.2004
A fast and powerful wind from a hot young star has created this stunning bubble-shaped nebula poised on the end of a bright filament of hydrogen gas. Cataloged as N44F, the cosmic windblown bubble is seen at the left of this Hubble Space Telescope image.
![Газовый поток от Магеллановых Облаков](https://images.astronet.ru/pubd/2004/08/09/0001198905/lmcstream_csiro_big.preview.jpg)
26.08.1998
Spanning the sky behind the majestic Clouds of Magellan is an unusual stream of gas: the Magellanic Stream. The origin of this gas might hold a clue to origin and fate of our Milky Way's most famous satellite galaxies: the LMC and the SMC.
![Тарантул](https://images.astronet.ru/pubd/2003/06/24/0001191221/tarantula2_saao.preview.jpg)
4.06.1997
NGC 2070 is an immense star forming region in a nearby galaxy known as the Large Magellanic Cloud. Its spidery appearance is responsible for its popular name, "The Tarantula Nebula", except that this tarantula is about 1,000 light-years across, and 165,000 light-years away in the southern constellation Dorado.
![Звездное "буйство" в области звездообразования 30 Золотой Рыбы](https://images.astronet.ru/pubd/2002/08/26/0001179349/30doradus_aat.preview.gif)
23.05.1996
The largest, most violent star forming region known in the whole Local Group of galaxies lies in our neighboring galaxy the LMC. Were 30 Doradus at the distance of the Orion Nebula -- a local star forming region -- it would take up fully half the sky.
![30 Золотой Рыбы: зона Тарантула](https://images.astronet.ru/pubd/2005/12/12/0001210188/tarantula_ctio.preview.jpg)
11.12.2005
The Tarantula Nebula is more than 1,000 light-years across - a giant emission nebula within our neighboring galaxy the Large Magellanic Cloud. Inside this cosmic arachnid lies a central young cluster of massivestars, cataloged as R136, whose intense radiation and strong winds have helped energize the nebular glow and shape the spidery filaments.
![R136: массивные звезды 30 Золотой Рыбы](https://images.astronet.ru/pubd/2005/12/11/0001210181/tarantula_hst.preview.jpg)
10.12.2005
In the center of star-forming region 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. These stars, known as the star cluster R136, and part of the surrounding nebula are captured here in this gorgeous visible-light image from the Hubble Space Telescope.
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