HD 204313

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HD 204313
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Capricornus
Right ascension 21h 28m 12.20609s[1]
Declination −21° 43′ 34.5182″[1]
Apparent magnitude (V) 7.99[2]
Characteristics
Spectral type G5V[3]
Apparent magnitude (B) 8.687[2]
Apparent magnitude (J) 6.812±0.024[2]
Apparent magnitude (H) 6.539±0.040[2]
Apparent magnitude (K) 6.459±0.018[2]
B−V color index 0.697±0.022[2]
Distance
157.0 ± 0.3 ly
(48.15 ± 0.08 pc)
Absolute magnitude (MV)4.61[2]
Details
Gyr
LTT 8525[6]
Database references
Exoplanet Archive
data

HD 204313 is a

light years from the Sun based on parallax measurements, but it is drifting closer with a radial velocity of −10 km/s.[1]

This is an ordinary

projected rotational velocity of just 0.8 km/s.[5] 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.[4]

Planetary system

This star was in observation by the

mean motion resonance, which may be stabilizing their periods.[11]

A 2015 study independently confirmed the first two discoveries, but did not detect any significant signal at the claimed period of planet d.[12] Another study in 2022 agreed with these results, in addition to finding a new planet or brown dwarf, designated HD 204313 e to differentiate it from the dubious candidate. The inclination and true mass of planets b & e were measured via astrometry.[13]

The HD 204313 planetary system[12][13]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
c ≥17.6±1.7 M🜨 0.2099±0.0071 34.905±0.012 0.059+0.051
−0.041
b 4.615+1.290
−0.306
 MJ
3.185+0.130
−0.143
2041.1+1.7
−1.9
0.100±0.003 72.917+31.372
−21.476
°
e 15.317+4.890
−5.183
 MJ
7.457+0.399
−0.427
7325.6+399.9
−369.1
0.253+0.071
−0.065
176.092+0.963
−2.122
°

See also

References