Sculptor Dwarf Galaxy
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Sculptor Dwarf Elliptical Galaxy | |
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Observation data (J2000 epoch) | |
Constellation | Sculptor |
Right ascension | 01h 00m 09.3s[1] |
Declination | −33° 42′ 33″[1] |
Redshift | 110 ± 1 km/s[1] |
Distance | 290 ± 30 kly (90 ± 10 kpc)[2][3] |
Type | E[1] |
Apparent dimensions (V) | 39′.8 × 30′.9[1] |
Apparent magnitude (V) | 10.1[1] |
Other designations | |
Sculptor Dwarf Spheroidal,[1] PGC 3589,[1] MCG-06-03-015 | |
The Sculptor Dwarf Galaxy (also called the Sculptor Dwarf Elliptical Galaxy or the Sculptor Dwarf Spheroidal Galaxy) is a dwarf spheroidal galaxy that is a satellite of the Milky Way. The galaxy lies within the constellation Sculptor. It was discovered in 1937 by Harlow Shapley using the 24-inch Bruce refractor at Boyden Observatory.[4][5] The galaxy is located about 290,000 light-years away from the Solar System. The Sculptor Dwarf contains only 4 percent of the carbon and other heavy elements in our own galaxy, the Milky Way, making it similar to primitive galaxies seen at the edge of the universe.[6]
Metallicity
The metallicity of Sculptor dwarf appears to be broken up into two distinct groups, one with [Fe/H] = -2.3 and the other with [Fe/H] = -1.5.[7] Similar to many of the other Local Group galaxies, the older metal-poor segment appears more extended than the younger metal-rich segment.[8]
Gallery
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Sculptor Dwarf Galaxy taken by the 2.2-meter MPG/ESO telescope.[9]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Lua error in package.lua at line 80: module 'strict' not found.
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- ↑ Shapley, H., (1938) Harvard Bull. 908.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Astronomers Detect Dust Around a Primitive Star, Shedding New Light on Universe’s Origins Newswise, Retrieved on January 19, 2008.
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External links
- The Sculptor Dwarf Galaxy on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates: 01h 00m 09.3s, −33° 42′ 33″
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