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HD 26965 b image

HD 26965 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2018
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HD 26965 b orbits a star known as HD 26965, nestled fairly close in cosmic terms to our solar system. Discovered in 2018 using the radial velocity method with the clever TOU instrument at several observatories, this planet is part of the ever-growing family of exoplanets we get to explore from afar. While we don’t have a charming nickname for HD 26965 b, its intriguing dance around its star makes it a fascinating target for understanding worlds beyond our own. Thanks to ground-based telescopes, we've peeked into this distant system, reminding us how much there is to discover in the vastness of space. It's a cosmic neighbor worth watching as we continue mapping the stars and their companions.