HD 204313

HD 204313 is a star with two and possibly three exoplanetary companions in the southern constellation of Capricornus. With an apparent magnitude of 7.99, it is an eighth magnitude star that is too faint to be readily visible to the naked eye. The star is located at a distance of 157 light years from the Sun based on parallax measurements, but it is drifting closer with a radial velocity of −10 km/s.

HD 204313
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Capricornus
Right ascension 21h 28m 12.20609s
Declination −21° 43 34.5182
Apparent magnitude (V) 7.99
Characteristics
Spectral type G5V
Apparent magnitude (B) 8.687
Apparent magnitude (J) 6.812±0.024
Apparent magnitude (H) 6.539±0.040
Apparent magnitude (K) 6.459±0.018
B−V color index 0.697±0.022
Astrometry
Radial velocity (Rv)−9.79±0.12 km/s
Proper motion (μ) RA: 42.751 mas/yr
Dec.: −270.443 mas/yr
Parallax (π)20.7705 ± 0.0343 mas
Distance157.0 ± 0.3 ly
(48.15 ± 0.08 pc)
Absolute magnitude (MV)4.61
Details
Mass1.06±0.03 M
Radius1.08±0.03 R
Luminosity1.18±0.03 L
Surface gravity (log g)4.39±0.04 cgs
Temperature5,783±48 K
Metallicity [Fe/H]0.18 dex
Rotational velocity (v sin i)0.846 km/s
Age4.3±1.8 Gyr
Other designations
CD–22°5691, GC 30045, HD 204313, HIP 106006, SAO 190362, PPM 272526, LTT 8525
Database references
SIMBADdata
Exoplanet Archivedata

This is an ordinary G-type main-sequence star with a stellar classification of G5V, which indicates it is generating energy through hydrogen fusion at its core. It is an estimated four billion years old, chromospherically extremely quiet, and is spinning with a projected rotational velocity of just 0.8 km/s. The star has a slightly larger mass and radius compared to the Sun. It is radiating 118% of the luminosity of the Sun from its photosphere at an effective temperature of 5,783 K.

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