HD 33142 c is an intriguing exoplanet orbiting the star HD 33142, discovered in 2018 using the radial velocity method. This nifty technique, a bit like the cosmic version of feeling a star’s gentle tug from orbiting planets, was carried out by the sharp-eyed HIRES Spectrometer at the Western Mauna Kea summit’s Keck Observatory. Though we don’t have a flashy proper name for HD 33142 c yet, this world’s discovery adds a valuable chapter to our ever-growing story of planetary exploration. While it remains a bit of a distant mystery with its precise traits still under wraps, HD 33142 c invites us to imagine what alien skies and landscapes might look like in the vast cosmic neighborhood.
