HD 102329 c is an intriguing exoplanet orbiting the star HD 102329, spotted back in 2018 using the cunning radial velocity method. This clever technique, aided by the HIRES Spectrometer at the W. M. Keck Observatory, detects the planet's tug on its star, revealing its presence from afar. While HD 102329 c doesn't have a catchy nickname yet, it holds its own in the cosmic dance, showcasing the subtle gravitational pulls that hint at hidden worlds beyond our solar system. Although we can’t pinpoint its exact size or distance here, this planet marks another fascinating chapter in our quest to understand the variety of planets out there, spinning silently in the starry depths.
