NFT token detail for exoplanet HD 49674 b. Only at exoplanetary.systems
HD 49674 b is a sub_neptune exoplanet discovered in 2002
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 49674 b
FOR SALE
Price
Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2002
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 49674 b, also known by its charming proper name Eburonia, orbits the star HD 49674, detected way back in 2002 using the clever radial velocity method at the W. M. Keck Observatory with the trusty HIRES Spectrometer. This exoplanet is a delightful reminder of the talent involved in peeking into distant solar systems from our own little blue planet. While it may not be the biggest or flashiest planet out there, Eburonia orbits close enough to its star to keep things interesting, making it a fascinating world for astronomers and space enthusiasts alike. Its discovery marked another step in our ever-growing journey to map the diverse family of planets beyond our solar neighborhood.
