HD 104067
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Corvus |
Right ascension | 11h 59m 10.010s[1] |
Declination | −20° 21′ 13.61″[1] |
Apparent magnitude (V) | 7.93 |
Characteristics | |
Spectral type | K2V |
Apparent magnitude (B) | 8.92 |
Apparent magnitude (J) | 6.212 |
Apparent magnitude (H) | 5.754 |
Apparent magnitude (K) | 5.614 |
B−V color index | 0.99 |
Astrometry | |
Proper motion (μ) | RA: 143.31±0.80[1] mas/yr Dec.: −423.67±0.48[1] mas/yr |
Parallax (π) | 47.47 ± 0.90[1] mas |
Distance | 69 ± 1 ly (21.1 ± 0.4 pc) |
Absolute magnitude (MV) | 6.34 |
Details | |
Mass | 0.73 M☉ |
Radius | 0.79±0.06 R☉ |
Luminosity | 0.317±0.017 L☉ |
Surface gravity (log g) | 4.34 cgs |
Temperature | 4880±100 K |
Metallicity | -0.06 |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Extrasolar Planets Encyclopaedia |
data |
HD 104067 is an 8th magnitude K-type main sequence star located approximately 69 light years away[1] in the constellation Corvus. This star is smaller, cooler, dimmer, and less massive than our Sun. Also its metal content is seven-eighths as much as the Sun. In 2009, a gas giant planet was found in orbit around the star.
Planetary system
HD 104067 b is an extrasolar planet which orbits the star. This planet has at least 0.16 times the mass of Jupiter and takes 55.8 days to orbit the star at a semimajor axis of 0.26 AU.[2]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥ 0.16 MJ | 0.2643±0.0045 | 55.806±0.049 | 0 | — | — |
See also
References
Coordinates: 11h 59m 10.0100s, −20° 21′ 13.609″
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