NFT token detail for exoplanet HD 86081 b. Only at exoplanetary.systems
HD 86081 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 86081 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
More Sub Neptune worlds you might consider for your collection.
Meet Santamasa, officially known as HD 86081 b, a fascinating exoplanet that orbits the star HD 86081. Discovered back in 2006 using the radial velocity method with the keen eyes of the HIRES Spectrometer at the W. M. Keck Observatory, Santamasa is a world that invites curiosity and wonder. Although we don’t have exact distances in this description, this ground-based discovery showcases the power of Earth’s telescopes in exploring distant planetary systems. Santamasa isn’t just a name; it’s a gateway to imagining what alien skies might look like as this planet circles its host star. A remarkable find that reminds us how much there is to discover beyond our solar system!
