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TOI-1117 c image

TOI-1117 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2025
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TOI-1117 c is a fascinating exoplanet orbiting the star TOI-1117, discovered in 2025 thanks to the sharp eyes of the HARPS Spectrograph at the renowned La Silla Observatory. This distant world was found using the clever radial velocity method, where tiny stellar wobbles reveal hidden planets. Although it keeps its secrets well, TOI-1117 c invites curiosity as a distant cousin in our galaxy's grand family. Imagine a planet discovered from the ground, hundreds of light-years away, patiently orbiting its star while astronomers on Earth peer through telescopes to unravel its mysteries. Not quite ready for tourists, but a cosmic wonder that shows how we keep reaching for the stars, one wobble at a time!