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54 Persei

Star in the constellation Perseus From Wikipedia, the free encyclopedia

54 Persei is a single[10] star in the northern constellation of Perseus. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.93.[2] The star is located approximately 220 light years away based on parallax, but is drifting closer with a radial velocity of −27 km/s.[5]

Quick facts Constellation, Right ascension ...
54 Persei
Location of 54 Persei (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Perseus
Right ascension 04h 20m 24.63885s[1]
Declination 34° 34 00.2033[1]
Apparent magnitude (V) 4.93[2]
Characteristics
Spectral type G8+ IIIb[3]
U−B color index +0.69[4]
B−V color index +0.95[4]
Astrometry
Radial velocity (Rv)−26.82[5] km/s
Proper motion (μ) RA: −25.046[1] mas/yr
Dec.: −6.420[1] mas/yr
Parallax (π)14.8484±0.1993 mas[1]
Distance220 ± 3 ly
(67.3 ± 0.9 pc)
Absolute magnitude (MV)0.80[6]
Details[7]
Mass2.57±0.10 M
Radius9.37±0.22 R
Luminosity50.7±2.0 L
Surface gravity (log g)2.93±0.03 cgs
Temperature5,036±32 K
Metallicity [Fe/H]+0.11±0.10 dex
Rotational velocity (v sin i)1.8[8] km/s
Age580±90 Myr
Other designations
54 Per, BD+34°860, FK5 158, GC 5235, HD 27348, HIP 20252, HR 1343, SAO 57171, CCDM J04204+3435A, WDS J04204+3434A[9]
Database references
SIMBADdata
Close

This is an aging giant star with a stellar classification of G8+ IIIb,[3] a star that has exhausted the supply of hydrogen at its core and expanded to more than nine times the girth of the Sun. It is around 580 million years old with 2.6 times the mass of the Sun. The star is radiating 51 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,036 K.[7] It has one distant visual companion, designated component B, at an angular separation of 93 and magnitude 13.0.[11]

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