Andromeda XVIII | |
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DSS image of Andromeda XVIII | |
Observation data (J2000 epoch) | |
Constellation | Andromeda |
Right ascension | 00h 02m 14.5s[1] |
Declination | +45° 05′ 20″[1] |
Helio radial velocity | −326.2 ± 2.7[2] |
Distance | 4,420 ± 290 kly (1,355 ± 88 kpc) |
Group or cluster | Local Group |
Apparent magnitude (V) | 15.50 ± 0.24[3] |
Absolute magnitude (V) | −10.41 ± 0.28[3] |
Characteristics | |
Type | dG[1] |
Mass | 4.2×106 ± 0.3×106[3] M☉ |
Half-light radius (physical) | 325 ± 24[2] |
Other designations | |
PGC 5056918[4] |
Andromeda XVIII, discovered in 2008, is a dwarf spheroidal galaxy (has no rings, low luminosity, much dark matter, little gas or dust), which is a satellite of the Andromeda Galaxy (M31). It is one of the 14 known dwarf galaxies orbiting M31. It was announced in 2010 that the orbiting galaxies lie close to a plane running through M31's center.[citation needed]
Original source: https://en.wikipedia.org/wiki/Andromeda XVIII.
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