HD 89307

HD 89307
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Leo
Right ascension 10h 18m 21.28771s
Declination +12° 37 15.9909
Apparent magnitude (V) 7.02
Characteristics
Spectral type G0V
B−V color index 0.594±0.003
Astrometry
Radial velocity (Rv)+23.27±0.13 km/s
Proper motion (μ) RA: −272.659 mas/yr
Dec.: −39.333 mas/yr
Parallax (π)31.4134±0.0226 mas
Distance103.83 ± 0.07 ly
(31.83 ± 0.02 pc)
Absolute magnitude (MV)4.57
Details
Mass1.028±0.04 M
Radius1.08+0.01
−0.02
 R
Luminosity1.354±0.003 L
Surface gravity (log g)4.414±0.10 cgs
Temperature5,950±44 K
Metallicity [Fe/H]−0.15±0.02 dex
Rotation23.7 d
Rotational velocity (v sin i)3.21±0.50 km/s
Age5.3+2.7
−2.9
 Gyr

6.76 Gyr
Other designations
BD+13 2237, GC 14140, HD 1835, HIP 50473, SAO 99049, PPM 127289
Database references
SIMBADdata

HD 89307 is a star in the equatorial constellation of Leo. It is too faint to be viewed with the naked eye except under ideal conditions, having an apparent visual magnitude of 7.02. The star is located at a distance of 104 light-years (32 parsecs) from the Sun based on parallax, and is drifting further away with a radial velocity of +23 km/s.

This is an ordinary G-type main-sequence star with a stellar classification of G0V. It is chromospherically inactive and appears older than the Sun with a rotation period of 23.7 days. The star has about the same mass as the Sun and is 8% larger. It is radiating 1.35 times the Sun's luminosity from its photosphere at an effective temperature of 5,950 K.