Meet HAT-P-17 c, a distant world orbiting the star HAT-P-17, discovered back in 2010 using the keen eyes of the HIRES Spectrometer at the W. M. Keck Observatory. This planet was found through the clever radial velocity method, which detects the subtle wobble of its star caused by the planet’s gravitational tug. Though we don’t have a nickname for this exoplanet yet, it’s an intriguing member of its star system, dancing its slow cosmic dance far from its sun compared to its neighbor, HAT-P-17 b. Imagine a giant planet quietly circling far out in space, helping astronomers piece together the mysteries of planetary systems beyond our own. It’s a reminder of how much there is still to explore in our galaxy!
