Velocity Variations Caused by Two Transiting Exoplanets
Radial velocity variations of two stars over one planetary revolution, as observed with the FLAMES facility at the 8.2-m VLT Kueyen telescope. The sinusoidal shape reflects the gravitational pull of the planet on the star.
About the Image
|Release date:||7 May 2004|
|Size:||977 x 629 px|