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HD 60532 c image

HD 60532 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2008
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HD 60532 c orbits the star HD 60532, a celestial dance partner discovered in 2008 through the clever detective work of the HARPS Spectrograph at the La Silla Observatory, perched high in the Chilean Andes. This giant exoplanet was detected using the radial velocity method, which listens closely to the subtle wobble of its host star caused by the planet’s gravitational tug. Though light-years away, HD 60532 c sparks curiosity as part of a dynamic planetary system, orbiting in a place where space and gravity choreograph a cosmic ballet. It's a reminder of the many worlds waiting to be explored beyond the twinkle of stars in our night sky.