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HD 175167 b
Extrasolar planet List of extrasolar planets
Parent star
Star HD 175167
Constellation Pavo
Right ascension (α) 19h 00m 00.84s
Declination (δ) –69° 56′ 39.3″
Apparent magnitude (mV) 8.000
Distance218.6 ± 13.3 ly
(67.02 ± 4.09 pc)
Spectral type K2V
Mass (m) 1.102 M
Metallicity [Fe/H] 0.19
Orbital elements
Semimajor axis(a) 2.40 ± 0.05 AU
(359 Gm)
    35.8 mas
Periastron (q) 1.10 AU
(164 Gm)
Apastron (Q) 3.70 AU
(554 Gm)
Eccentricity (e) 0.54 ± 0.09
Orbital period(P) 1290 ± 22 d
(3.53 y)
Orbital speed (υ) 20.3 km/s
Argument of
periastron
(ω) 342 ± 9°
Time of periastron (T0) 24553598 ± 48 JD
Semi-amplitude (K) 161 ± 55 m/s
Physical characteristics
Minimum mass(m sin i)7.8 ± 3.5 MJ
Discovery information
Discovery date January 26, 2010
Discoverer(s) Arriagada et al.
Discovery method Doppler spectroscopy
Discovery site Las Campanas Observatory
Discovery status Published
Other designations
CD–70°1658 b, HIP 93281 b
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBADdata

HD 175167 b is an extra-solar planet orbiting HD 175167, which is a G type star within the Pavo constellation around 219 light years away from the Earth. The planet was discovered by the Magellan Planet Search Program as the astronomical object fit the Keplerian orbital model. During the observations 13 doppler velocity tests were conducted, which showed this object’s size was at least 7.8 Jovian-masses and its orbit has a high eccentricity. The exoplanet takes 3.53 years to complete a full stellar orbit.[1][2][3]

See also[]

References[]

  1. 175167 b HD 175167. Exoplanets. Retrieved 2010-02-12.
  2. Template:Cite arxiv
  3. Planet : HD 175167 b. Exo Planets. Retrieved 2010-02-12.
  • Arriagada et al. (2010). Five Long-period Extrasolar Planets in Eccentric orbits from the Magellan Planet Search Program. Astrophysical Journal.

Coordinates: Sky map 19h 00m 00.84s, −69° 56′ 39.3″

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