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HD 209458 b image

HD 209458 b

World type: gas_giant
Discovery method: Radial Velocity
Discovery year: 1999
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HD 209458 b is a trailblazing exoplanet that orbits the star HD 209458. Discovered back in 1999 using the radial velocity method, this hot Jupiter was one of the first distant worlds to reveal its secrets through ground-based observations at the W. M. Keck Observatory with the HIRES Spectrometer. Imagine a giant gas planet sizzling close to its star, much hotter and puffier than our own Jupiter, with a dramatic atmosphere that has been closely studied by astronomers eager to understand its exotic weather. It's a fascinating world that helped open the door to the age of exoplanet exploration, sitting some hundreds of light-years away, reminding us just how vast and varied the universe truly is.