Canes Venatici Dwarf Galaxy
From Wikipedia, the free encyclopedia
Galaxy | List of galaxies |
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Observation data (Epoch J2000) |
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Constellation | Canes Venatici |
Right ascension | 13h 28m 03.5s[1] |
Declination | +33° 33′ 21″[1] |
Redshift | |
Distance | 640 kly (196 kpc)[citation needed] |
Type | dSph |
Apparent dimensions (V) | |
Apparent magnitude (V) | 13.9V[1] |
Notable features | |
Other designations | |
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The Canes Venatici Dwarf (CVn dSph) is the most distant satellite galaxy of the Milky Way as of 2006. It is a dwarf spheroidal galaxy in the Canes Venatici constellation, lying 640,000 light-years away. The galaxy is approximately 6000 light-years across and very faint.
[edit] External links
- The Universe within 500000 light-years The Satellite Galaxies (Atlas of the Universe)
- Two New Galaxies Orbiting the Milky Way (Ken Croswell) April 19, 2006
- Strange satellite galaxies revealed around Milky Way Kimm Groshong (New Scientist) 17:00 24 April 2006
- New Milky Way companions found: SDSS-II first to view two dim dwarf galaxies (SDSS) May 8, 2006
- Astronomers Find Two New Milky Way Companions (SpaceDaily) May 10, 2006
[edit] References
Galactic Core: Center of the Milky Way |