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Star in the constellation Perseus From Wikipedia, the free encyclopedia
36 Persei is a solitary,[8] variable star located 121 light years away from the Sun in the northern constellation of Perseus. It is visible to the naked eye as a dim, yellow-white hued point of light with a baseline apparent visual magnitude of 5.32.[2] The star is drifting closer to the Sun with a heliocentric radial velocity of −47.5 km/s,[4] and may come as close as 36.6 light-years in 661,000 years.[5]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Perseus |
Right ascension | 03h 32m 26.25886s[1] |
Declination | 46° 03′ 24.7029″[1] |
Apparent magnitude (V) | 5.32[2] |
Characteristics | |
Spectral type | F4III[3] |
U−B color index | −0.02[2] |
B−V color index | +0.41[2] |
Astrometry | |
Radial velocity (Rv) | −47.5[4] km/s |
Proper motion (μ) | RA: −52.829[1] mas/yr Dec.: −74.915[1] mas/yr |
Parallax (π) | 26.9895 ± 0.1053 mas[1] |
Distance | 120.8 ± 0.5 ly (37.1 ± 0.1 pc) |
Absolute magnitude (MV) | 2.50[5] |
Details | |
Mass | 1.50[4] M☉ |
Radius | 2.28+0.13 −0.09[1] R☉ |
Luminosity | 8.585±0.042[1] L☉ |
Surface gravity (log g) | 3.94[4] cgs |
Temperature | 6,546+126 −176[1] K |
Metallicity [Fe/H] | −0.17[4] dex |
Rotational velocity (v sin i) | 28.0[6] km/s |
Age | 2.20[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
The stellar classification of 36 Persei is F4III,[3] matching an aging giant star that has used up its core hydrogen. This object is used by astronomers as a spectral standard for stars with a similar class.[9] The star is a suspected variable of unknown type, ranging in visual magnitude from 5.29 down to 5.33,[10] and is a source of X-ray emission.[11] The star is 2.2[4] billion years old with a projected rotational velocity of 28 km/s.[6] It has an estimated 1.5[4] times the mass of the Sun and has not yet expanded significantly, having 2.3[1] times the Sun's girth. The star is radiating 8.6[1] times the luminosity of the Sun from its photosphere at an effective temperature of 6,546 [1]
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