HD 114762 b is a fascinating exoplanet orbiting the star HD 114762, discovered back in 1989 using the clever radial velocity technique at Oak Ridge Observatory. This pioneering find was made possible by the trusty CfA Digital Speedometer, a ground-based instrument that helped astronomers detect the tiny stellar wobbles caused by the planet’s gravity. While it doesn't have a catchy nickname yet, HD 114762 b remains an intriguing world, offering a glimpse into the diverse family of planets existing beyond our solar system. Its pioneering discovery marks an early chapter in exoplanet exploration, reminding us of how far our quest to understand distant worlds has come—and how many new adventures await just beyond the stars!
