HD 4313

HD 4313 is a star with an orbiting exoplanetary companion in the constellation of Pisces. It has an apparent visual magnitude of 7.83, which is too faint to be reading visible to the unaided eye. The systam is located at a distance of 446 light years based on parallax, and is drifting further away with a radial velocity of 14.5 km/s. This is a single star, which means it has no binary partners, at least in range of projected separations from 6.85 to 191.78 AU. It hosts an extrasolar planet.

HD 4313
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 00h 45m 40.3578s
Declination +07° 50 42.075
Apparent magnitude (V) 7.83
Characteristics
Evolutionary stage Subgiant
Spectral type K2 IV
B−V color index 0.963±0.017
Astrometry
Radial velocity (Rv)14.48±0.23 km/s
Proper motion (μ) RA: −6.281 mas/yr
Dec.: 6.566 mas/yr
Parallax (π)7.3090 ± 0.0879 mas
Distance446 ± 5 ly
(137 ± 2 pc)
Absolute magnitude (MV)2.17
Details
Mass1.61+0.13
0.12
 M
Radius5.15+0.18
0.17
 R
Luminosity15.81 L
Surface gravity (log g)3.24 cgs
Temperature4,966±40 K
Metallicity [Fe/H]0.05±0.10 dex
Rotational velocity (v sin i)1.91±0.25 km/s
Age2.03+0.64
0.45
 Gyr
Other designations
BD+07°104, Gaia DR2 2557541493057378048, HD 4313, HIP 3574, 2MASS J00454035+0750421
Database references
SIMBADdata

This is an aging K-type star with a mass of nearly twice the Sun, although different methods give mass estimates which differ as much as 0.5 M. It is a swollen star with 5.14 times the radius of the Sun, and has a cool effective temperature of 4,966±40 k. The "IV" in the spectral class means it's a K-type subgiant star which has exhausted the hydrogen at its core, and cooling and expanding to become a red giant. It is around two billion years in age and is spinning with a projected rotational velocity of 1.9 km/s.

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