HD 104067

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.

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
Distance69 ± 1 ly
(21.1 ± 0.4 pc)
Absolute magnitude (MV)6.34
Details
Mass0.73 M☉
Radius0.79±0.06 R☉
Luminosity0.317±0.017 L☉
Surface gravity (log g)4.34 cgs
Temperature4880±100 K
Metallicity−0.06
Rotation29.8±3.1 d[2]
Other designations
BD−19°3382, GJ 1153, HIP 58451, LTT 4461, NLTT 29176, PPM 259710, SAO 180353
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia		data

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]

The HD 104067 planetary system[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
  • List of extrasolar planets

References
  1. 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. S2CID 18759600.Vizier catalog entry
  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, S2CID 119181646.
  3. 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. S2CID 119197766.


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