NFT token detail for exoplanet HD 98219 b. Only at exoplanetary.systems
HD 98219 b is a sub_neptune exoplanet discovered in 2011
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 98219 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2011
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope
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Meet Ixbalanqué, officially known as HD 98219 b, a captivating exoplanet orbiting the star HD 98219. Discovered in 2011 using the radial velocity method, Ixbalanqué was spotted from the ground at the renowned W. M. Keck Observatory with the HIRES Spectrometer, a powerful tool that helps astronomers tease out subtle wobbles in distant stars caused by orbiting planets. Though Ixbalanqué keeps its exact distance from Earth a bit of a cosmic secret, its discovery adds to the growing family of intriguing worlds beyond our solar system. Orbiting a star that shines steadily from afar, Ixbalanqué invites us to ponder the diversity of planets out there, each with its own story written in the stars.
