NFT token detail for exoplanet HD 10647 b. Only at exoplanetary.systems
HD 10647 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 10647 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 10647 b is an intriguing exoplanet orbiting the star HD 10647, discovered back in 2006 using the radial velocity method at the W. M. Keck Observatory with the HIRES Spectrometer. This distant world is a gas giant companion that stirs curiosity about its swirling atmosphere and distant sun. While it doesn’t have a catchy nickname yet, HD 10647 b makes up for it with its story of discovery and the clever techniques that let us spot such cosmic neighbors from light-years away. Imagining this giant planet quietly circling its star adds a touch of mystery and wonder to the vast, sparkling tapestry of our galaxy. For stargazers and space enthusiasts alike, HD 10647 b is a lovely reminder that the universe is full of surprises just waiting to be explored.
