description HD 114762 Overview
HD 114762 is a solar-type star about 132 light-years from Earth whose substellar companion, announced in 1989 by Latham et al., was one of the earliest candidate brown dwarfs or massive exoplanets.
insights Why this score
HD 114762 ranks #141 of 217 in the Star ranking, behind Hamal, ahead of Delta Pavonis.
Early substellar companion candidate, historically important though classification has been debated.
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