Nu Persei

Yellow-white hued star in the constellation Perseus From Wikipedia, the free encyclopedia

ν Persei, Latinized as Nu Persei, is a single[13] star and a suspected variable in the northern constellation of Perseus. It has a yellow-white hue and is visible to the naked eye with an apparent visual magnitude of 3.80.[2] This object is located approximately 560 light-years from the Sun based on parallax[1] but is drifting closer with a radial velocity of −12 km/s.[5]

Right ascension03h 45m 11.63204s[1]
Declination+42° 34 42.7829[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Nu Persei
Location of ν Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 03h 45m 11.63204s[1]
Declination +42° 34 42.7829[1]
Apparent magnitude (V) 3.80[2]
Characteristics
Spectral type F5II[3]
U−B color index +0.28[2]
B−V color index +0.42[2]
Variable type suspected[4]
Astrometry
Radial velocity (Rv)−12.10[5] km/s
Proper motion (μ) RA: −14.45[1] mas/yr
Dec.: +2.53[1] mas/yr
Parallax (π)5.86±0.22 mas[1]
Distance560 ± 20 ly
(171 ± 6 pc)
Absolute magnitude (MV)−2.39[6]
Details
Mass5.01[7] M
Radius20.62+1.72
−1.76
[8] R
Luminosity603.6±41.2[8] L
Surface gravity (log g)3.04[9] cgs
Temperature6,300+287
−158
[8] K
Metallicity [Fe/H]+0.41[9] dex
Rotational velocity (v sin i)48.9[10] km/s
Age109[11] Myr
Other designations
ν Per, 41 Persei, NSV 1261, BD+42°815, FK5 134, GC 4474, HD 23230, HIP 17529, HR 1135, SAO 39078, CCDM J03452+4235A, WDS J03452+4235A[12]
Database references
SIMBADdata
Close

This object is a highly luminous bright giant star with a stellar classification of F5II.[3] It has five[7] times the mass of the Sun but has expanded to around 21[8] times the Sun's radius. The star has a relatively high rotation rate, spinning with a projected rotational velocity of 48.9 km/s.[10] It is radiating 604[8] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 6,300 K.[8]

Several visual companions beside the primary have been recorded. B, with magnitude 12.1 and separation 31.6", has its own companion, E, with magnitude 14.3 and separation 7.7". Additionally, C has magnitude 13.2 and separation 55.7", and D has magnitude 13.8 and separation 22.8".[14]

References

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