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HD 4208 b image

HD 4208 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2001
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Welcome to Xolotlan, also known as HD 4208 b, a fascinating giant planet orbiting the star HD 4208 far beyond our solar system. Discovered back in 2001 using the clever radial velocity technique at the W. M. Keck Observatory with the HIRES Spectrometer, Xolotlan showcases the power of ground-based astronomy. This distant world offers a cosmic playground for exoplanet enthusiasts, orbiting steadily around its sun-like star. While it's not a place for casual strolls, its discovery marks a giant leap in our quest to understand the universe’s planetary diversity. So, buckle up and imagine drifting through the space around Xolotlan, a proudly named member of the ever-growing family of exoplanets!