← Back to Cryptoplanets

HD 110014 b image

HD 110014 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
FOR_SALE
Orbiting the star HD 110014, this intriguing exoplanet, known simply as HD 110014 b, was discovered back in 2009 using the clever radial velocity method. Scientists spotted its subtle gravitational tug by analyzing starlight with the FEROS Spectrograph at the famed La Silla Observatory nestled in the Chilean Andes. While HD 110014 b’s exact details remain a bit mysterious, it’s known to be a giant world, likely several times the mass of Jupiter, dancing closely around its host star. Imagine the thrill of exploring a giant planet that was uncovered through the patient art of stellar wobble detection — a cosmic game of hide-and-seek played light-years away!