← Back to Cryptoplanets

HD 166724 b image

HD 166724 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2012
FOR_SALE
HD 166724 b is a fascinating exoplanet orbiting the star HD 166724, discovered back in 2012 using the clever radial velocity method at the La Silla Observatory in Chile. Thanks to the CORALIE Spectrograph, astronomers caught subtle wobbles in the star’s motion, revealing this distant world’s presence. While it doesn’t have a flashy proper name, HD 166724 b still sparks curiosity as a mysterious member of its stellar family. Imagine standing on its surface, somewhere tens or hundreds of light-years away, gazing at a star much like our sun but with its unique cosmic dance partners. This planet reminds us of the exciting frontier beyond our solar system, where each discovery is a new chapter in the grand story of the universe.