HD 113337 b is a fascinating exoplanet orbiting the star HD 113337, discovered back in 2013 using the clever radial velocity technique at the Haute-Provence Observatory in France. Thanks to the SOPHIE Spectrograph, astronomers detected its subtle gravitational tug on its host star, revealing its presence without ever seeing it directly. While we don’t have an official nickname for this world yet, it’s certainly a captivating member of the cosmic neighborhood. Imagine a planet dancing closely around its star, completed with a chilly ambiance possibly shaped by its distance and stellar warmth. HD 113337 b showcases how ground-based observatories can unveil distant secrets, proving we don’t always need giant space telescopes to discover new worlds orbiting stars far beyond our Sun.
