HD 175167 b

HD 175167 b
Exoplanet List of exoplanets
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 G5
Mass (m) 1.102 M
Metallicity [Fe/H] 0.19
Orbital elements
Semi-major 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
Exoplanet Archivedata
Open Exoplanet Cataloguedata

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 dead link] "HD 175167" Check |url= value (help). Exoplanets. Retrieved 2010-02-12.
  2. Pamela Arriagada; Paul Butler; Dante Minniti; Mercedes Lopez-Morales; Shectman; Adams; Boss; Chambers (2010). "Section HD 175167". arXiv:1001.4093 [astro-ph.EP].
  3. "Planet : HD 175167 b". Exo Planets. Retrieved 2010-02-12.

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

This article is issued from Wikipedia - version of the Sunday, November 15, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.