NFT token detail for exoplanet HD 222582 b. Only at exoplanetary.systems
HD 222582 b is a sub_neptune exoplanet discovered in 1999
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 222582 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 1999
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 222582 b is a fascinating giant exoplanet orbiting the star HD 222582, discovered back in 1999 using the clever radial velocity technique. This cosmic heavyweight was spotted from the ground at the renowned W. M. Keck Observatory, employing the sharp-eyed HIRES Spectrometer. Though it doesn’t have a catchy proper name yet, HD 222582 b stands out as a gas giant potentially bigger than Jupiter, making it a true giant in its system. Imagine a world dominated by swirling clouds of gas, possibly with fierce storms raging through its thick atmosphere. While it’s far too distant for a quick visit, this planetary giant invites us to dream about the diversity of worlds beyond our solar neighborhood.
