HD 188015 b

HD 188015 b

Discovery
Discovered by	Marcy et al.[1]
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 MJ

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 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.^[2]

• Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701. S2CID 119067572.
• Raghavan; Henry, Todd J.; Mason, Brian D.; Subasavage, John P.; Jao, Wei‐Chun; Beaulieu, Thom D.; Hambly, Nigel C. (2006). "Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems". The Astrophysical Journal. 646 (1): 523–542. arXiv:astro-ph/0603836. Bibcode:2006ApJ...646..523R. doi:10.1086/504823. S2CID 5669768.

• "Notes for planet HD 188015 b". Extrasolar Planets Encyclopaedia.
• "HD 188015". Exoplanets. Archived from the original on 2009-11-25. Retrieved 2008-09-08.

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