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HD 20794 c image

HD 20794 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2011
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HD 20794 c is an intriguing exoplanet orbiting the star HD 20794, discovered back in 2011 by a clever team using the HARPS Spectrograph at the La Silla Observatory in Chile. This planet was found using the radial velocity method, which means scientists spotted its subtle gravitational tug on its cozy host star. While we don’t have an official nickname for this world, it sparks curiosity as part of the HD 20794 system, located relatively nearby in cosmic terms. Picture it as a distant neighbor quietly circling its star, offering a glimpse into the diverse family of planets beyond our own solar system. It’s a fantastic example of how ground-based instruments continue to uncover new worlds in our galactic backyard!