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HD 104985 b image

HD 104985 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2003
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Meet Meztli, officially known as HD 104985 b, a fascinating exoplanet orbiting the star HD 104985. Discovered in 2003 using the radial velocity method at the Okayama Astrophysical Observatory in Japan, Meztli was detected with the help of the HIDES Echelle Spectrograph. This giant world is a bit of a cosmic character, circling its star at a comfortable distance that keeps it in a steady dance through space. Though it’s far from Earth and a bit mysterious, Meztli invites us to imagine the exotic skies from its vantage point, where the glow of its sun might paint strange, beautiful patterns. It’s a reminder of the incredible variety and wonder waiting to be found beyond our solar system.