NFT token detail for exoplanet HD 218566 b. Only at exoplanetary.systems
HD 218566 b is a sub_neptune exoplanet discovered in 2010
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 218566 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2010
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 218566 b, charmingly named Ugarit, orbits its host star HD 218566 with quiet elegance in a sun-like system far from Earth. Discovered in 2010 using the clever radial velocity technique with the HIRES Spectrometer at the famed W. M. Keck Observatory, this exoplanet invites us to imagine a world beyond our solar neighborhood. Though it's not the closest neighbor, Ugarit’s story sparks curiosity about its environment and the nature of planets around stars like HD 218566. Picture a distant dance partner to its star, sensed by subtle gravitational tugs, reminding us how astronomy turns tiny wobbles into tales of alien worlds waiting to be explored. Ugarit stands as a testament to our ever-expanding horizons in the cosmic expanse.
