HD 188015 b

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 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.: HD 93083, HD 17051, HD 28185, HD 27442, HD 188015, HD 99109, HD 221287
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Category:Exoplanets
Category:Gas giants
Category:Gas giants in the habitable zone
Category:Vulpecula (constellation)
Category:Exoplanets detected by radial velocity
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