HD 104067
| 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 | K3V[2] |
| 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 |
| Rotation | 29.8±3.1 d[2] |
| 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 80% as 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.[3]
| 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
- 1 2 3 4 5 6 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752
. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.Vizier catalog entry - 1 2 Suárez Mascareño, A.; et al. (September 2015), "Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators", Monthly Notices of the Royal Astronomical Society, 452 (3): 2745−2756, arXiv:1506.08039, Bibcode:2015MNRAS.452.2745S, doi:10.1093/mnras/stv1441.
- 1 2 Ségransan, D.; et al. (2011). "The HARPS search for southern extra-solar planets. XXIX. Four new planets in orbit around the moderately active dwarfs HD 63765, HD 104067, HD 125595, and HIP 70849". Astronomy and Astrophysics. 535. A54. arXiv:1107.0339. Bibcode:2011A&A...535A..54S. doi:10.1051/0004-6361/200913580.
Coordinates: 
11h 59m 10.0100s, −20° 21′ 13.609″
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