Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Reticulum[1] |
Right ascension | 04h 20m 47.046s[2] |
Declination | −59° 24′ 39.02″[2] |
Apparent magnitude (V) | 9.36[1] |
Characteristics | |
Spectral type | K2 V[3] |
U−B color index | +0.90[4] |
B−V color index | +1.003±0.002[1] |
Astrometry | |
Radial velocity (Rv) | 82.785±0.0008[5] km/s |
Proper motion (μ) | RA: 182.473±0.012 mas/yr[2] Dec.: 270.012±0.017 mas/yr[2] |
Parallax (π) | 22.8888 ± 0.0121 mas[2] |
Distance | 142.50 ± 0.08 ly (43.69 ± 0.02 pc) |
Absolute magnitude (MV) | 6.225[6] |
Details | |
Mass | 0.83±0.03[7] M☉ |
Radius | 0.79±0.02[7] R☉ |
Luminosity | 0.33±0.01[7] L☉ |
Surface gravity (log g) | 4.56±0.03[7] cgs |
Temperature | 4,923±32[7] K |
Metallicity [Fe/H] | +0.30±0.07[6] dex |
Rotation | 44 days[6] |
Rotational velocity (v sin i) | ≤ 1.5[6] km/s |
Age | 7.7±2.3[8] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 27894 is a single star with a system of orbiting exoplanets, located in the southern constellation of Reticulum. It is too faint to be seen with the naked eye at an apparent visual magnitude of 9.36.[1] This system lies at a distance of 142.5 light years from the Sun, as determined via parallax measurements, and is drifting further away with a radial velocity of 83 km/s.[5]
The spectrum of HD 27894 presents as a K-type main-sequence star, an orange dwarf,[6] with a stellar classification of K2 V.[3] This is a quiescent solar-type star that displays no significant magnetic activity in its chromosphere[9] and is spinning slowly with a rotation period of roughly 44 days.[6] The abundance of iron in the star is much higher than in the Sun, an indicator that it is metal-rich.[6] It has 83% of the mass of the Sun and 79% of the Sun's radius. The star is radiating 33% of the luminosity of the Sun from its photosphere at an effective temperature of 4,923 K.[7]
Anderson_Francis_2012
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