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HD 96167 Observation data Epoch J2000.0      Equinox J2000.0 Constellation Crater Right ascension 11h 05m 15.0681s Declination –10° 17′ 28.681″ Apparent magnitude (V) 8.09 Characteristics Spectral type G5D B−V color index 0.68 Variable type none Astrometry Proper motion (μ) RA: –51.79 mas/yr Dec.: –7.06 mas/yr Parallax (π) 11.90 ± 1.29 mas Distance approx. 270 ly (approx. 84 pc) Absolute magnitude (MV) 3.47 Details Mass 1.31 ± 0.09 M☉ Radius 1.86 ± 0.07 R☉ Surface gravity (log g) 4.11 Luminosity 3.44 L☉ Temperature 5770 ± 70 K Metallicity 0.34 ± 0.06 Age 3.8 ± 1 years Other designations BD–09° 3201, HIP 54195, PPM 223905, SAO 156444 Database references SIMBAD data NStED data Extrasolar Planets Encyclopaedia data HD 96167 is an 8th magnitude G-type subgiant star located approximately 274 light years away in the constellation of Crater. It is larger, brighter and more massive than our Sun. The star is metal rich and around 3.8 ± 1 Gyr old. In 2009 it was found that this star has a planet.[1] The HD 96167 system[1] Companion (in order from star) Mass Semimajor axis (AU) Orbital period (days) Eccentricity b ≥0.68 ± 0.18 MJ 1.30 ± 0.07 498.9 ± 1.0 0.71 ± 0.04 See also List of extrasolar planets References ^ a b Peek et al. (2009). "Old, rich, and eccentric: two jovian planets orbiting evolved metal-rich stars" (abstract). Publications of the Astronomical Society of the Pacific 121 (880): 613–620. doi:10.1086/599862. http://www.journals.uchicago.edu/doi/abs/10.1086/599862.  (web Preprint) Coordinates: 11h 05m 15.0681s, −10° 17′ 28.681″ This subgiant star-related article is a stub. You can help Wikipedia by expanding it. v • d • e This extrasolar planet related article is a stub. You can help Wikipedia by expanding it. v • d • e