HD 4628

HD 4628 (96 G. Piscium) is a main sequence star in the equatorial constellation of Pisces. It has a spectral classification of K2.5 V and an effective temperature of 5,055 K, giving it an orange-red hue with a slightly smaller mass and girth than the Sun. HD 4628 lies at a distance of approximately 24.3 light years from the Sun based on parallax. The apparent magnitude of 5.7 is just sufficient for this star to be viewed with the unaided eye. The star appears to be slightly older than the Sunapproximately 5.4 billion years in age. The surface activity is low and, based upon the detection of UV emission, it may have a relatively cool corona with a temperature of one million K.

HD 4628
Observation data
Epoch J2000      Equinox J2000
Constellation Pisces
Right ascension 00h 48m 22.97634s
Declination +05° 16 50.2096
Apparent magnitude (V) 5.74
Characteristics
Spectral type K2.5 V
U−B color index +0.60
B−V color index +0.89
Astrometry
Radial velocity (Rv)−10.41±0.15 km/s
Proper motion (μ) RA: 755.561 mas/yr
Dec.: −1,141.745 mas/yr
Parallax (π)134.4948 ± 0.0578 mas
Distance24.25 ± 0.01 ly
(7.435 ± 0.003 pc)
Absolute magnitude (MV)6.37
Details
Mass0.70±0.10 M
Radius0.749±0.051 R
Luminosity0.28 L
Surface gravity (log g)4.39±0.16 cgs
Temperature5,055±40 K
Metallicity [Fe/H]–0.22 dex
Rotation38.0 days
Age5.4 Gyr
Other designations
96 G. Piscium, BD+04°123, HD 4628, HIP 3765, HR 222, SAO 109471, LHS 121, LTT 10285, Wolf 25, Lal 1299
Database references
SIMBADdata

The star has a relatively high proper motion of 1.4 per year and is moving in our general direction with a radial velocity of −10.4 km/s. HD 4628 will make its closest approach to the Sun in about 32,000 years, when it comes within 20 ly (7.3 pc). No definitive companion has yet been found in orbit around this star. In 1958 it was thought to have stellar companion that was also a flare star, but this was subsequently disproved.

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