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HD 10180 g image

HD 10180 g

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2010
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HD 10180 g is a fascinating world orbiting the sun-like star HD 10180, discovered back in 2010 using the clever radial velocity method at the La Silla Observatory in Chile. This planet is part of a bustling planetary system known for its remarkable number of worlds, making it a cosmic neighborhood that’s buzzing with activity. Thanks to the precise HARPS spectrograph, scientists could detect this distant planet’s subtle gravitational pull on its star. While we don’t know all the details about its surface or atmosphere yet, HD 10180 g sparks the imagination as a distant world dancing around its star many light-years away. It offers a thrilling glimpse into the diversity of planets beyond our solar system!