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31 Persei
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31 Persei
31 Persei
Location of 31 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 03h 19m 07.63796s[1]
Declination 50° 05′ 41.8724″[1]
Apparent magnitude (V) 5.05[2]
Characteristics
Spectral type B5V[3]
U−B color index −0.53[4]
B−V color index −0.06[4]
Astrometry
Radial velocity (Rv)−1.60[5] km/s
Proper motion (μ) RA: +23.580[1] mas/yr
Dec.: −23.322[1] mas/yr
Parallax (π)5.8399±0.1792 mas[1]
Distance560 ± 20 ly
(171 ± 5 pc)
Absolute magnitude (MV)−1.44[6]
Details
Mass4.647[7] M
Radius3.4[8] R
Luminosity950[6] L
Temperature15,301[6] K
Metallicity [Fe/H]0.00[9] dex
Rotational velocity (v sin i)260[10] km/s
Age234[11] Myr
Other designations
31 Per, BD+49°902, GC 3945, HD 20418, HIP 15444, HR 989, SAO 38714[12]
Database references
SIMBADdata

31 Persei is a single[13] star in the northern constellation of Perseus. It is visible to the naked eye as a dim, blue-white hued point of light with an apparent visual magnitude of 5.05.[2] This star is located around 172 parsecs (560 ly) away from the Sun,[14] and it is drifting closer with a radial velocity of −1.6 km/s.[5] It is likely a member of the Alpha Persei Cluster.[15]

This object is a massive B-type main-sequence star with a stellar classification of B5V[3] and it is currently generating energy through hydrogen fusion at its core. It is around 234[9] million years old and is spinning rapidly with a projected rotational velocity of 260 km/s.[10] The star has 4.6[7] times the mass of the Sun and about 3.4[8] times the radius of the Sun. It is radiating 950[6] times the luminosity of the Sun from its photosphere at an effective temperature of 15,301 K.[6]

References

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