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You entered: 30 Doradus
![Новые звезды в области 30 Золотой Рыбы](https://images.astronet.ru/pubd/2006/11/12/0001217705/30dor_details_big.preview.jpg)
1.10.1999
Compare these matched Hubble Space Telescope views (visible-light on top; infrared on bottom) of a region in the star-forming 30 Doradus Nebula. Find the numbered arrows in the infrared image which identify newborn massive stars. For example, arrows 1 and 5 both point to compact clusters of bright young stars.
![Звездное скопление R136](https://images.astronet.ru/pubd/2007/05/07/0001221916/r136_hst.preview.jpg)
6.05.2007
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.
![Звездное скопление R136](https://images.astronet.ru/pubd/2016/01/24/0001354600/30dor_hubble_960.preview.jpg)
24.01.2016
In the center of star-forming region 30 Doradus lies a huge cluster containing some of the largest, hottest, and most massive stars known. These stars, known collectively as star cluster R136, were captured in the featured image in visible light by the Wide Field Camera 3 in 2009 peering through the Hubble Space Telescope.
![Звёздное скопление R136](https://images.astronet.ru/pubd/2012/07/30/0001268424/30dor_hst_960.preview.jpg)
29.07.2012
In the center of star-forming region 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. These stars, known collectively as star cluster R136, were captured above in visible light by the newly installed Wide Field Camera peering though the recently refurbished Hubble Space Telescope.
![Звездное скопление R136](https://images.astronet.ru/pubd/2009/12/21/0001237484/30dor_hst.preview.jpg)
21.12.2009
In the center of star-forming region 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. These stars, known collectively as star cluster R136, were captured above in visible light by the newly installed Wide Field Camera peering though the recently refurbished Hubble Space Telescope.
![Туманность Тарантул: вид в телескоп Spitzer](https://images.astronet.ru/pubd/2004/02/02/0001196426/tarantula_spitzer.preview.jpg)
2.02.2004
In the heart of monstrous Tarantula Nebula lies one of the most unusual star clusters. Known as NGC 2070 or R136, it is home to a great number of hot young stars. The energetic light from these stars continually ionizes nebula gas, while their energetic particle wind blows bubbles and defines intricate filaments.
![Звездное скопление R136](https://images.astronet.ru/pubd/2001/08/31/0001170568/30Doradus_hst.preview.jpg)
30.07.2001
In the center of star-forming region 30 Doradus lies a huge cluster of the largest, hottest, most massive stars known. Known as R136, the cluster's energetic stars are breaking out of the cocoon of gas and dust from which they formed.
!["Щупальца" туманности Тарантул](https://images.astronet.ru/pubd/2004/12/28/0001201609/tarantula_eso.preview.jpg)
28.12.2004
The Tarantula Nebula is a giant emission nebula within our neighboring galaxy the Large Magellanic Cloud. Inside this cosmic arachnid lies a huge central young cluster of massive stars, cataloged as R136 and partially visible on the upper right.
![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.
![В сердце Тарантула](https://images.astronet.ru/pubd/2006/11/12/0001217668/tarantula_btc_big.preview.jpg)
27.10.1999
In the heart of monstrous Tarantula Nebula lies one of the most unusual star clusters. Known as NGC 2070 or R136, it is home to a great number of hot young stars. The energetic light from these stars continually ionizes nebula gas, while their energetic particle wind blows bubbles and defines intricate filaments.
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