HD 188015 b

HD 188015 b
Exoplanet List of exoplanets
Parent star
Star HD 188015
Constellation Vulpecula
Right ascension (α) 19h 52m 04.5435s
Declination (δ) +28° 06 01.356
Distance171.66 ly
(52.63 pc)
Spectral type G5IV
Orbital elements
Semi-major axis(a) 1.203 ± 0.070 AU
Periastron (q) 1.038 AU
Apastron (Q) 1.368 AU
Eccentricity (e) 0.137 ± 0.026
Orbital period(P) 461.2 ± 1.7 d
(1.263 y)
Orbital speed (υ) 28.47 km/s
Argument of
periastron
(ω) 222° ± 10°
Time of periastron (T0) 2,451,787 ± 17 JD
Semi-amplitude (K) 37.6 ± 1.2 m/s
Physical characteristics
Mass(m)>1.50 ± 0.13 MJ
Discovery information
Discovery date January 25, 2005
Discoverer(s) Marcy et al.[1]
Discovery method Doppler spectroscopy
Discovery site  United States
Discovery status Published[1]
Other designations
HIP 97769 b

HD 188015 b is an extrasolar planet announced by the California and Carnegie Planet Search team in 2005.[1] Like majority of known planets, it was discovered using the radial velocity method.

The planet has a minimum mass about quarter greater than Jupiter. It orbits the star in a slightly eccentric orbit in a mean distance 20% further than Earth orbits the Sun.

Stability analysis reveals that the orbits of Earth-sized planets in the Trojan points of HD 188015 b would be stable for long periods of time.[2]

References

  1. 1 2 3 Marcy, Geoffrey W.; et al. (2005). "Five New Extrasolar Planets". The Astrophysical Journal 619 (1): 570–584. Bibcode:2005ApJ...619..570M. doi:10.1086/426384.
  2. R. Schwarz, R. Dvorak, Á. Süli, and B. Érdi (November 2007). "Survey of the stability region of hypothetical habitable Trojan planets". Astronomy & Astrophysics 474 (3): 1023–1029. Bibcode:2007A&A...474.1023S. doi:10.1051/0004-6361:20077994.: HD 93083, HD 17051, HD 28185, HD 27442, HD 188015, HD 99109, HD 221287

External links


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