Extrasolar planet in the constellation Vulpecula
HD 188015 b Discovery Discovered by Marcy et al. Discovery site United States Discovery date January 25, 2005 Detection method Doppler spectroscopy Orbital characteristics Apastron 1.368 AU (204,600,000 km) Periastron 1.038 AU (155,300,000 km) Semi-major axis 1.203 ± 0.070 AU (180,000,000 ± 10,500,000 km) Eccentricity 0.137 ± 0.026 Orbital period (sidereal) 461.2 ± 1.7 d 1.263 y Average orbital speed 28.47 Time of periastron 2,451,787 ± 17 Argument of periastron 222° ± 10 Semi-amplitude 37.6 ± 1.2 Star HD 188015 Physical characteristics Mass >1.50 ± 0.13 M J
HD 188015 b is an extrasolar planet announced by the California and Carnegie Planet Search team in 2005. Like majority of known planets, it was discovered using the radial velocity method.
The planet has a minimum mass of about 1.25 Jupiter masses . It orbits HD 188015 in a slightly eccentric orbit with a semi-major axis about 20% further than Earth 's.
Stability analysis reveals that if Earth-sized planets existed at the Trojan points of HD 188015 b, their orbits would be stable for long periods of time.
References
^ Marcy, Geoffrey W.; et al. (2005). "Five New Extrasolar Planets" . The Astrophysical Journal . 619 (1): 570–584. Bibcode :2005ApJ...619..570M . CiteSeerX 10.1.1.516.6667 . doi :10.1086/426384 .
R. Schwarz; R. Dvorak; Á. Süli; 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
Bibliography
External links
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