Image:Triangulum.nebula.full.jpg
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NGC 604 is an H II region inside the Triangulum Galaxy. It was discovered by William Herschel on September 11, 1784. It is one of the largest H II regions in the Local Group of galaxies; at the galaxy's estimated distance of 2.4 million light-years its longest diameter is roughly 700 light-years (200 + parsecs), over 20 times the size of the visible portion of the Orion Nebula. Over 6300 times more luminous than the Orion Nebula, if it were at the same distance it would outshine Venus. Like all emission nebulae, its gas is ionized by a cluster of massive stars at its center.(*)
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| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 08:10, 26 April 2005 | 1,127×1,201 (2.42 MB) | Aarchiba | (Emission nebula NGC 604 lies in a spiral arm of galaxy M33, 2.7 million light-years away in the constellation Triangulum. This is a site where stars are being born. Though such nebulae are common in galaxies, this one is particularly large, nearl) |
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- Hydrogen
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- Stellar evolution
- H II region
- NGC 604
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