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Keywords: M 8, Lagoon Nebula
![Выброс из галактики М87](https://images.astronet.ru/pubd/2001/03/15/0001166660/m87jet_hst_big.preview.jpg)
6.07.2000
What's causing a huge jet to emanate from the center of galaxy M87? Although the unusual jet was first noticed early in the twentieth century, the exact cause is still debated. The above recently released picture taken by the Hubble Space Telescope shows clear details, however.
![Оживленный центр туманности Лагуна](https://images.astronet.ru/pubd/2020/06/01/0001663585/LagoonCenter_HubbleGravinese_960.preview.jpg)
1.06.2020
The center of the Lagoon Nebula is a whirlwind of spectacular star formation. Visible near the image center, at least two long funnel-shaped clouds, each roughly half a light-year long, have been formed by extreme stellar winds and intense energetic starlight. A tremendously bright nearby star, Hershel 36, lights the area.
![Центр туманности Лагуна в инфракрасном свете](https://images.astronet.ru/pubd/2021/03/19/0001730684/M8_HLA_F125wF160w_Nachman1024.preview.jpg)
19.03.2021
Stars fill this infrared view, spanning 4 light-years across the center of the Lagoon Nebula. Visible light images show the glowing gas and obscuring dust clouds that dominate the scene. But this infrared image...
![Южный утес в Лагуне](https://images.astronet.ru/pubd/2021/05/16/0001739510/M8_rim2geminicrop600.preview.jpg)
15.05.2021
Undulating bright ridges and dusty clouds cross this close-up of the nearby star forming region M8, also known as the Lagoon Nebula. A sharp, false-color composite of narrow band visible and broad band near-infrared...
![Туманность Лагуна без звезд](https://images.astronet.ru/pubd/2022/09/13/0001848832/LagoonStarFree_Dhar_960.preview.jpg)
8.08.2022
Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent, cosmic depths of the Lagoon Nebula. Also known as M8, the bright star forming region is about 5,000 light-years distant.
![Триплет в Стрельце](https://images.astronet.ru/pubd/2021/04/26/0001736421/M8-M20_GabrielSantos_APOD1024.preview.jpg)
26.04.2021
These three bright nebulae are often featured on telescopic tours of the constellation Sagittarius and the crowded starfields of the central Milky Way. In fact, 18th century cosmic tourist Charles Messier cataloged two of them; M8, the large nebula below and right of center, and colorful M20 near the top of the frame.
![Триплет в Стрельце](https://images.astronet.ru/pubd/2017/07/30/0001386982/TOA1-M8M20-SL-DCP01andB600-09-Final7-Cc1024.preview.jpg)
27.07.2017
These three bright nebulae are often featured on telescopic tours of the constellation Sagittarius and the crowded starfields of the central Milky Way. In fact, 18th century cosmic tourist Charles Messier cataloged two of them; M8, the large nebula above and left of center, and colorful M20 near the bottom of the frame.
![В центре туманности Лагуна](https://images.astronet.ru/pubd/2017/05/22/0001383347/lagoon_hubble_960.preview.jpg)
21.05.2017
The center of the Lagoon Nebula is a whirlwind of spectacular star formation. Visible on the lower left, at least two long funnel-shaped clouds, each roughly half a light-year long, have been formed by extreme stellar winds and intense energetic starlight. The tremendously bright nearby star, Hershel 36, lights the area.
![Туманность Лагуна в линиях водорода, серы и кислорода](https://images.astronet.ru/pubd/2016/01/05/0001352879/LagoonHSO_Nemcik_960.preview.jpg)
5.01.2016
The majestic Lagoon Nebula is filled with hot gas and the home for many young stars. Spanning 100 light years across while lying only about 5000 light years distant, the Lagoon Nebula is so big and bright that it can be seen without a telescope toward the constellation of the Archer (Sagittarius).
![Широкая и глубокая Лагуна](https://images.astronet.ru/pubd/2016/09/09/0001368872/M8-8-25-16-webMillerWalker1024.preview.jpg)
9.09.2016
Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent, cosmic depths of the Lagoon Nebula. Also known as M8, the bright star forming region is about 5,000 light-years distant.
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