← Back to Cryptoplanets

HD 25171 b image

HD 25171 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2010
FOR_SALE
HD 25171 b is an intriguing exoplanet orbiting the star HD 25171, discovered in 2010 using the radial velocity method with the HARPS Spectrograph at the La Silla Observatory. This ground-based detection showcases the power of precision instruments in unveiling distant worlds. While the planet itself remains a bit of a cosmic mystery with no formal name yet, it orbits its host star with a subtle gravitational dance that teased out its presence from afar. Imagine a world circling a star many light-years away, quietly making its rounds in the vastness of space. HD 25171 b reminds us how our technology peeks into the universe’s depths, finding new planets beyond our solar system and expanding our sense of cosmic neighborhood.