HD 96167

HD 96167 is a binary star located approximately 280 light years away in the constellation of Crater.

HD 96167
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Crater
Right ascension 11h 05m 15.0688s[1]
Declination –10° 17 28.6947[1]
Apparent magnitude (V) 8.09
Characteristics
Spectral type G5IV
B−V color index 0.68
Variable type none
Astrometry
Proper motion (μ) RA: −50.494±0.081[1] mas/yr
Dec.: −9.496±0.072[1] mas/yr
Parallax (π)11.6947 ± 0.0565[1] mas
Distance279 ± 1 ly
(85.5 ± 0.4 pc)
Absolute magnitude (MV)3.47
Orbit
PrimaryHD 96167 A
CompanionHD 96167 BC
Semi-major axis (a)5.285"
(506 AU[2])
Details
Mass1.31 ± 0.09 M
Radius1.86 ± 0.07 R
Luminosity3.44 L
Surface gravity (log g)4.11 cgs
Temperature5770 ± 70 K
Metallicity0.34 ± 0.06
Age3.8 ± 1 years
Other designations
BD–09° 3201, Gaia DR2 3758718711877270784, HIP 54195, SAO 156444, 2MASS J11051506-1017286[3]
Database references
SIMBADdata
Exoplanet Archivedata

Primary HD 96167 A is an 8th magnitude G-type subgiant star It is larger, brighter and more massive than our Sun. The star is metal rich and around 3.8 ± 1 Gyr old.

The faint stellar companion was detected in 2014 at the projected separation 506 AU, and existence of additional stellar companions was ruled out at projected distances from 51 to 740 astronomical units.[2]

Planetary system

In 2009 it was found that primary star HD 96167 A is orbited by a planet.[4]

The HD 96167 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥0.71±0.18 MJ 1.332±0.092 498.1±0.81 0.681±0.033

See also

  • List of extrasolar planets

References

  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. Mugrauer, M.; Ginski, C. (12 May 2015). "High-contrast imaging search for stellar and substellar companions of exoplanet host stars". Monthly Notices of the Royal Astronomical Society. 450 (3): 3127–3136. doi:10.1093/mnras/stv771. Retrieved 19 June 2020.
  3. "HD 96167". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-09-21.
  4. Peek, John Asher; et al. (2009). "Old, rich, and eccentric: two jovian planets orbiting evolved metal-rich stars". Publications of the Astronomical Society of the Pacific. 121 (880): 613–620. arXiv:0904.2786. Bibcode:2009PASP..121..613P. doi:10.1086/599862.
  5. Ment, Kristo; et al. (2018). "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810". The Astronomical Journal. 156 (5). 213. arXiv:1809.01228. Bibcode:2018AJ....156..213M. doi:10.3847/1538-3881/aae1f5. S2CID 119243619.

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