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Star Forming Region Hubble-V

Star Forming Region Hubble-V

Credit & copyright: Credit: C. R. O'Dell ( Vanderbilt ) et al. , L. Bianchi ( JHU ) et al. , Hubble Heritage Team , NASA

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 Sun s. 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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