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HD 240210 b image

HD 240210 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
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HD 240210 b is a fascinating exoplanet orbiting the star HD 240210, discovered back in 2009 using the clever technique of radial velocity at the McDonald Observatory. Thanks to the sharp eyes of the High Resolution Spectrograph, astronomers picked up the subtle wobble this planet causes in its star’s light. While details about its exact size and orbit might remain a bit mysterious, HD 240210 b provides a tantalizing glimpse into the diverse worlds beyond our solar system. It's a reminder of how much there is to explore out there, all detected from a ground-based telescope right here on Earth! If you love celestial hide-and-seek, this distant world is a planet worth celebrating.