Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
Right ascension | 09h 51m 07.05180s[1] |
Declination | −43° 30′ 10.0237″[1] |
Apparent magnitude (V) | 7.66 |
Characteristics | |
Spectral type | K6V[2] |
U−B color index | 1.12 |
B−V color index | 1.18 |
V−R color index | 0.71 |
Astrometry | |
Radial velocity (Rv) | −9.78±0.12[1] km/s |
Proper motion (μ) | RA: 461.603 mas/yr[1] Dec.: −471.880 mas/yr[1] |
Parallax (π) | 88.6737 ± 0.0173 mas[1] |
Distance | 36.782 ± 0.007 ly (11.277 ± 0.002 pc) |
Absolute magnitude (MV) | 7.39[3] |
Details[2][4] | |
Mass | 0.69 M☉ |
Radius | 0.533 ± 0.04[note 1] R☉ |
Luminosity (bolometric) | 0.126 ± 0.008 L☉ |
Surface gravity (log g) | 4.604±0.017 cgs |
Temperature | 4404±10 K |
Metallicity | ([Si/H] dex) -0.02 |
Metallicity [Fe/H] | -0.28 dex |
Rotation | 47.13 ± 6.98 |
Rotational velocity (v sin i) | 2.194±0.118 km/s |
Age | 5.61 ± 0.61 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 85512 is a solitary K-type main-sequence star 36.8 light-years (11.3 parsecs) away in the constellation Vela. It is about 1 billion years older than the Sun. It is extremely chromospherically inactive, only slightly more active than Tau Ceti. It exhibits a long-term variability[2] and was thought to host one low-mass planet, although this is now doubtful.[6]
Gaia DR3
was invoked but never defined (see the help page).Holmberg2009
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Laliotis2023
was invoked but never defined (see the help page).
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