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Credit & Copyright: C. R. O'Dell
(Vanderbilt)
et al.,
L. Bianchi
(JHU)
et al.,
Hubble Heritage Team,
NASA
Explanation:
How did stars form in the early universe?
Astronomers are gaining insight by studying
NGC 6822, a nearby galaxy classified as
irregular by modern standards but appearing more typical of
galaxies billions of years ago.
Inspection of NGC 6822 shows several bright star groups,
including two dubbed
Hubble-X and Hubble-V.
Pictured above, the
Hubble Space Telescope has resolved
Hubble V into the energetic stars
that are lighting up the surrounding gas.
Each star in the central dense knot of
Hubble V shines brighter than 100,000
Suns.
The Hubble V gas cloud spans about 200
light years and lies about 1.5 million light-years away toward the
constellation
Sagittarius.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: Hubble V - NGC 6822 - star formation
Publications with words: Hubble V - NGC 6822 - star formation
See also:
- NGC 1893 and the Tadpoles of IC 410
- Star Factory Messier 17
- APOD: 2023 August 28 Á Star Formation in the Pacman Nebula
- APOD: 2023 July 10 Á Stars, Dust and Nebula in NGC 6559
- NGC 1333: Stellar Nursery in Perseus
- APOD: 2023 March 21 Á Dark Nebulae and Star Formation in Taurus
- The Tadpole Nebula in Gas and Dust