NFT token detail for exoplanet HD 96167 b. Only at exoplanetary.systems
HD 96167 b is a sub_neptune exoplanet discovered in 2009
using the Radial Velocity method at W. M. Keck Observatory. The 10 m Keck I Telescope
was employed with the instruments of the HIRES Spectrometer.
HD 96167 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope
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HD 96167 b is a fascinating exoplanet orbiting the star HD 96167, discovered back in 2009 using the clever radial velocity method with the help of the HIRES Spectrometer at the W. M. Keck Observatory. This planet is like a cosmic dance partner, tugging slightly on its star and revealing its presence through these subtle stellar wobbles. While it doesn't have a fancy nickname yet, HD 96167 b certainly captures the imagination with its distant orbit around a star far beyond our solar system. A product of ground-based ingenuity, this exoplanet reminds us how much we can learn about the universe just by watching stars carefully and listening to their gravitational whispers.
