NFT token detail for exoplanet HD 24040 b. Only at exoplanetary.systems
HD 24040 b is a sub_neptune exoplanet discovered in 2006
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 24040 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2006
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope
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HD 24040 b is a fascinating giant exoplanet orbiting the star HD 24040, discovered back in 2006 using the radial velocity method with the keen eyes of the HIRES Spectrometer at the W. M. Keck Observatory. This distant world is a gas giant, a planet with a hefty atmosphere of thick gases rather than a solid surface, making it a true heavyweight in its cosmic neighborhood. Though it doesn’t have a catchy nickname yet, HD 24040 b’s discovery adds a valuable piece to the puzzle of understanding planetary systems beyond our own. Imagine a colossal planet, quietly circling its star far from Earth, a silent giant revealed by subtle stellar wobbles far across the galaxy.
