From Handwiki | Pegasus Dwarf Spheroidal Galaxy | |
|---|---|
![]() Hubble Space Telescope image of Pegasus Dwarf Spheroidal Galaxy | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 23h 51m 46.3s[1] |
| Declination | +24° 34′ 57″[1] |
| Redshift | −354 ± 3 km/s[1] |
| Distance | 2.7 ± 0.1 Mly (820 ± 20 kpc)[2][3] |
| Apparent magnitude (V) | 14.2[1] |
| Characteristics | |
| Type | dSph[2] |
| Apparent size (V) | 4.0′ × 2.0′[1] |
| Other designations | |
| Pegasus II,[1] Andromeda VI,[1] Peg dSph,[1] KKH 99,[1] PGC 2807158 | |
The Pegasus Dwarf Spheroidal (also known as Andromeda VI or Peg dSph for short) is a dwarf spheroidal galaxy about 2.7 million light-years away in the constellation Pegasus. The Pegasus Dwarf is a member of the Local Group and a satellite galaxy of the Andromeda Galaxy (M31).
The Pegasus Dwarf Spheroidal is a galaxy with mainly metal-poor stellar populations.[4] Its metallicity is [Fe/H] ≃ −1.3.[5] It is located at the right ascension 23h51m46.30s and declination +24d34m57.0s in the equatorial coordinate system (epoch J2000.0), and in a distance of 820 ± 20 kpc from Earth and a distance of 294 ± 8 kpc[a] from the Andromeda Galaxy.
The galaxy was discovered in 1999[6] by various authors on the Second Palomar Observatory Sky Survey (POSS II) films.[7]
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Categories: [Dwarf spheroidal galaxies] [Principal Galaxies Catalogue objects] [Local Group] [Low surface brightness galaxies] [Andromeda Subgroup] [Pegasus (constellation)]