HD 104067

HD 104067
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Corvus
Right ascension 11h 59m 10.00884s
Declination −20° 21 13.6121
Apparent magnitude (V) 7.92
Characteristics
Spectral type K3V
Apparent magnitude (B) 8.894
Apparent magnitude (J) 6.212±0.019
Apparent magnitude (H) 5.754±0.023
Apparent magnitude (K) 5.614±0.024
B−V color index 0.974±0.010
Astrometry
Radial velocity (Rv)+14.89±0.12 km/s
Proper motion (μ) RA: 141.706 mas/yr
Dec.: −423.780 mas/yr
Parallax (π)49.1470±0.0235 mas
Distance66.36 ± 0.03 ly
(20.347 ± 0.010 pc)
Absolute magnitude (MV)6.30
Details
Mass0.818+0.024
−0.025
 M
Radius0.771+0.007
−0.006
 R
Luminosity0.307 L
Surface gravity (log g)4.56±0.10 cgs
Temperature4,942±14 K
Metallicity [Fe/H]0.11±0.06 dex
Rotation18.3±4.9 d
Rotational velocity (v sin i)2.47±0.96 km/s
Age4.8+3.3
−3.0
 Gyr
Other designations
BD−19°3382, GJ 1153, HD 104067, HIP 58451, SAO 180353, PPM 259710, LTT 4461, NLTT 29176
Database references
SIMBADdata
Exoplanet Archivedata

HD 104067 is a star with a planetary system in the southern constellation of Corvus. It has an apparent visual magnitude of 7.92 which is too faint to be visible with the naked eye. The distance to this star is 66.4 light-years (20.4 parsecs) based on parallax. It is drifting further away with a radial velocity of +15 km/s.

This is an ordinary K-type main-sequence star with a stellar classification of K3V. It is a moderately active star with an age of roughly five billion years. HD 104067 is spinning with a projected rotational velocity of 2.5 km/s, giving it a rotation period of approximately a month. The star has 82% of the mass and 77% of the radius of the Sun. It is radiating 31% of the Sun's luminosity from its photosphere at an effective temperature of 4,942 K. The metal content of this star is close to that in the Sun.