HD 175167

The HD 175167 is orbited by one known planet, discovered in 2010 by team of Magellan Planet Search Program, lead by Pamela Arriagada.

The HD 175167 planetary system[3]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b ≥7.8 ± 3.5 MJ 2.40 ± 0.05 1290 ± 22 0.54 ± 0.09 — —
HD 175167
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pavo
Right ascension 19h 00m 00.836s[1]
Declination –69° 56′ 39.27″[1]
Apparent magnitude (V) 8.000
Characteristics
Spectral type G5IV/V
Apparent magnitude (B) 8.779
Apparent magnitude (J) 7.89
Apparent magnitude (J) 8.86
Apparent magnitude (J) 6.713
Apparent magnitude (H) 6.381
Apparent magnitude (K) 6.288
B−V color index 0.779
Variable type none
Astrometry
Radial velocity (Rv)4.81±0.13[2] km/s
Proper motion (μ) RA: -7.044 ± 0.041[2] mas/yr
Dec.: -191.511 ± 0.049[2] mas/yr
Parallax (π)14.0386 ± 0.0332[2] mas
Distance232.3 ± 0.5 ly
(71.2 ± 0.2 pc)
Absolute magnitude (MV)3.869
Details
Mass1.102 M☉
Metallicity0.19
Other designations
CD–70°1658, HIP 93281, LTT 7516, NLTT 47212, PPM 363703
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia		data

See also

References
  1. Van Leeuwen, Floor (2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
  2. HD 175167, entry, SIMBAD. Accessed online February 13, 2020.
  3. Arriagada, Pamela; et al. (2010). "Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program". The Astrophysical Journal. 711 (2): 1229–35. arXiv:1001.4093. Bibcode:2010ApJ...711.1229A. doi:10.1088/0004-637X/711/2/1229. S2CID 118682009.

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