NFT token detail for exoplanet HD 96127 b. Only at exoplanetary.systems
HD 96127 b is a sub_neptune exoplanet discovered in 2011
using the Radial Velocity method at McDonald Observatory. The 9.2 m Hobby-Eberly Telescope
was employed with the instruments of the High Resolution Spectrograph.
HD 96127 b
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Discovery Details
World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2011
Facility: McDonald Observatory
Instrument: High Resolution Spectrograph
Telescope: 9.2 m Hobby-Eberly Telescope
More Sub Neptune worlds you might consider for your collection.
Meet HD 96127 b, a giant world orbiting the star HD 96127 far beyond our solar neighborhood. Discovered in 2011 using the radial velocity method at the McDonald Observatory with a high-resolution spectrograph, this gas giant reveals itself by gently tugging on its host star. While details about its size and climate remain a mystery, you can imagine a realm swirling with thick, alien skies and possibly fierce storms far from Earth’s tender touch. Touring HD 96127 b would be a cosmic adventure, drifting in the darkness around a distant star, where astronomers on Earth patiently await its next subtle wobble to learn more about this intriguing celestial giant.
