NFT token detail for exoplanet HAT-P-44 c. Only at exoplanetary.systems

HAT-P-44 c is a sub_neptune exoplanet discovered in 2014 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.

HAT-P-44 c image

HAT-P-44 c

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Discovery Details

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2014
Facility: W. M. Keck Observatory
Instrument: HIRES Spectrometer
Telescope: 10 m Keck I Telescope

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More planets in the HAT-P-44 system

HAT-P-44 b thumbnail HAT-P-44 b
HAT-P-44 c is a fascinating exoplanet orbiting the star HAT-P-44, discovered back in 2014 using the radial velocity method. This distant world was detected from the ground using the powerful HIRES Spectrometer at the W. M. Keck Observatory, showcasing the marvels of modern astronomy. While we don’t have a snappy nickname for HAT-P-44 c, it holds its own as part of a star system that continues to intrigue space enthusiasts. Its presence helps us understand the diversity of planetary systems out there, highlighting the clever techniques astronomers use to peek beyond our solar neighborhood. HAT-P-44 c invites us to dream of exotic worlds orbiting stars many light-years away, reminding us how vast and varied our galaxy truly is.