NFT token detail for exoplanet HD 50499 b. Only at exoplanetary.systems
HD 50499 b is a sub_neptune exoplanet discovered in 2005
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 50499 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2005
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope
More Sub Neptune worlds you might consider for your collection.
HD 50499 b orbits the sunlike star HD 50499, discovered back in 2005 using the clever radial velocity method at the W. M. Keck Observatory with the HIRES Spectrometer. This giant exoplanet is a fascinating world swirling far from its host star, likely a gas giant with a mysterious atmosphere waiting to be explored. Though we don’t have a catchy nickname for it, HD 50499 b stands as a stellar example of how astronomers use subtle star wobbles to uncover hidden worlds light-years away. A cosmic giant playing hide-and-seek in the vastness of space, it invites curious stargazers to dream about the diverse planetary families scattered across our galaxy.
