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HAT-P-13 c image

HAT-P-13 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
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Meet HAT-P-13 c, a fascinating exoplanet orbiting the star HAT-P-13, discovered back in 2009 using the clever radial velocity method. This distant world was spotted from the ground at the famed W. M. Keck Observatory in Hawaii, utilizing the precise HIRES Spectrometer to catch its subtle stellar wobbles. While its exact distance from Earth isn't headline news, HAT-P-13 c is part of an intriguing planetary system that has captured astronomers' imaginations. If planets were characters in a cosmic play, HAT-P-13 c would be the mysterious supporting actor, influencing its star and neighboring planets in ways that help scientists learn more about planetary dynamics far beyond our solar neighborhood. It’s a silent but vital participant in the cosmic dance!