NFT token detail for exoplanet HD 126614 b. Only at exoplanetary.systems

HD 126614 b is a gas_giant exoplanet discovered in 2009 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 126614 b image

HD 126614 b

FOR SALE
Price

Discovery Details

World type: gas_giant
Discovery method: Radial Velocity
Discovery year: 2009
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope

More Gas Giant worlds you might consider for your collection.

BD-14 3065 b thumbnail BD-14 3065 b Kepler-820 b thumbnail Kepler-820 b TOI-3856 b thumbnail TOI-3856 b HR 5183 b thumbnail HR 5183 b TOI-4930 b thumbnail TOI-4930 b HD 136118 b thumbnail HD 136118 b WASP-85 A b thumbnail WASP-85 A b Kepler-1964 b thumbnail Kepler-1964 b WASP-195 b thumbnail WASP-195 b Kepler-1326 b thumbnail Kepler-1326 b TOI-4961 b thumbnail TOI-4961 b Kepler-1654 b thumbnail Kepler-1654 b Kepler-1750 b thumbnail Kepler-1750 b HAT-P-4 b thumbnail HAT-P-4 b TOI-1820 b thumbnail TOI-1820 b GQ Lup b thumbnail GQ Lup b
HD 126614 b orbits the star HD 126614, discovered back in 2009 by the clever eyes of astronomers using the trusty HIRES Spectrometer at the W. M. Keck Observatory. This exoplanet was unveiled through the radial velocity method, which is a fancy way of saying scientists spotted the subtle dance tugging on its star. While we might not have its exact size or distance from Earth on hand, HD 126614 b invites you to imagine a world circling a distant sun, hidden among the stars. It’s a great example of how patience and precision from ground-based telescopes can reveal the secrets of faraway planetary neighbors. Who knows what adventures an explorer might dream up here?