HD 114762 is a triple star system [3] [4] approximately 125 light-years (38.2 pc) away in the constellation Coma Berenices. It consists of a yellow-white F-type main-sequence star (HD 114762 A) and two red dwarf companions (HD 114762 Ab & HD 114762 B) approximately 0.36 & …

HD 114762 b is a small red dwarf star, in the HD 114762 system, [3] formerly thought to be a massive gaseous [6] [7] extrasolar planet, [8] approximately 126 light-years (38.6 pc) away in the constellation of Coma Berenices.

HD 114762 is a blue to white main sequence star in the constellation of Coma Berenices. It is too faint to be seen in the northern hemisphere night sky without a telescope. HD 114762 distance from Earth is 126.08 light years away.

HD 114762. The planetary system HD 114762 hosts at least one planet. Note that the system is a multiple star system. It hosts at least 2 stellar components.

HD 114762 is a binary star system located approximately 126 light years 938.6 parsecs) away from Earth in the constellation Coma Berenices. The system composes of a yellow-white F-type main-sequence star (HD 114762 A), and either a red or brown dwarf companion, HD 114762 B.

The companion HD 114762 b has been reported to be a planetary candidate with a mass of at least 11 M J, but we showed here that its true mass is significantly higher and does not lie in the planetary domain.

Feb 5, 2019 · HD 114762 is an extrasolar system located 126 ligh-years away in the constellation of Coma Berenices. It is made of two stars and a substellar companion discovered 30 years ago this month. In this animation are represented the primary star (at the center) and the substellar companion (in orbit).

HD 114762 is a Sun-like star in the constellation Coma Berenices, which has an unseen companion first reported in 1989 and described by its discoverers as "probably a brown dwarf, maybe even a giant planet". 1 The existence of this companion has since been confirmed, though its nature remains controversial.

Oct 17, 2019 · The first planetary candidate discovered by Latham et al. (1989) with radial velocities around a solar-like star other than the Sun, HD 114762 b, was detected with a minimum mass of 11 Mjup.

hd 114762 (star system thought to host the first detected exoplanet) The HD 114762 multiple star system includes an object once considered an extra-solar planet -candidate which would have been the first exoplanet discovered, but which has since been classified as a star.