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HD 168443 b image

HD 168443 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 1998
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Meet HD 168443 b, a fascinating giant planet orbiting the star HD 168443. Discovered back in 1998 using the clever radial velocity method, this space heavyweight was found by tracking the subtle wobble of its host star with the HIRES Spectrometer at the W. M. Keck Observatory. While it’s a bit of a mystery planet without a flashy proper name, HD 168443 b stands out as a testament to the ingenuity of ground-based telescopes. This massive world likely boasts a wild orbit around its star, making it an intriguing subject for astronomers hunting the secrets of distant planetary systems. It’s a stellar example of how we can detect worlds far, far away, without ever leaving the surface of Earth!