RS Persei is a red supergiant variable star located in the Double Cluster in Perseus.
Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
RS Persei
 RS Persei is the red star closest to the centre of NGC 884, the right hand cluster (north is down). |
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Perseus |
Right ascension |
2h 22m 24.288s[1] |
Declination |
+57° 0.6′ 34.08″[1] |
Apparent magnitude (V) |
7.82-10.0[2] |
Characteristics |
Spectral type |
M4Iab[3] |
Variable type |
SRc[2] |
Astrometry |
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Radial velocity (Rv) | −38.0±2[4] km/s |
Proper motion (μ) | RA: −0.371±0.137[5] mas/yr Dec.: −0.931±0.165[5] mas/yr |
Parallax (π) | 0.6437 ± 0.0822[5] mas |
Distance | 2,345±55[6] pc |
Absolute magnitude (MV) | −6.18[7] |
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Details[6] |
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Mass | 12-15 M☉ |
Radius | 770±30 R☉ |
Luminosity | 77,600+9,500 −8,400 L☉ |
Surface gravity (log g) | −0.2±0.05 cgs |
Temperature | 3,470±90 K |
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Other designations |
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RS Per, HD 14488, BD +56°583, 2MASS J02222428+5706340, AAVSO 0215+56A |
Database references |
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SIMBAD | data |
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