HD 114762 - Planetary System

Planetary System

In 1989, a possible brown dwarf or planet was found orbiting HD 114762A by David Latham using Doppler spectroscopy. This object wasn’t fully confirmed until 1996 by Geoffrey Marcy. If it is a planet it is one of the most massive found to date, at the very least 11 Jupiter masses. However, the mass will be known more accurately when the inclination is finally determined. This object is very likely to be a brown dwarf or less likely a red dwarf with upper-mass limit 145 Jupiter masses. It orbits at about the same mean distance and has about the same time of revolution around the central star as Mercury, although HD 114762 b's orbit is eccentric.

The HD 114762 system
Companion
Mass Semimajor axis
Orbital period
Eccentricity Radius
b ≥11.069 ± 0.063 MJ 0.353 ± 0.001 83.9151 ± 0.0030 0.3354 ± 0.0048

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