Canes Venatici Dwarf Galaxy

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Canes Venatici Dwarf
Galaxy List of galaxies
Observation data
(Epoch J2000)
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
CVn dSph[1]

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

[edit] References

  1. ^ a b c d NASA/IPAC Extragalactic Database. Results for CVn dSph. Retrieved on 2006-11-26.
The Milky Way
v  d  e

Galactic Core: Center of the Milky Way
Spiral Arms: Carina Arm | Crux Arm | Cygnus Arm | Norma Arm | Orion Arm | Perseus Arm | Sagittarius Arm | Scutum Arm
Location: Universe | Virgo Supercluster | Local Group
Satellite galaxies: Boötes Dwarf | Canes Venatici Dwarf | Canis Major Dwarf Galaxy | Carina Dwarf | Draco Dwarf | Fornax Dwarf | Large Magellanic Cloud | Leo I | Leo II | Sag DEG | Sculptor Dwarf Galaxy | Sextans Dwarf | Small Magellanic Cloud | Ursa Major Dwarf | Ursa Minor Dwarf | Virgo Stellar Stream