熱木星
In 1995 with Michel Mayor announced a giant planet orbiting the star 51 Pegasi; the planet was identified as 51 Pegasi b and determined to be of a Hot Jupiter. The planet was detected by the measurement of small periodic changes in stellar radial velocity produced by the orbiting planet. Detecting this small variability by the Doppler effect had been possible thanks to the development of a new type of spectrograph, ELODIE, installed at the Haute-Provence Observatory, combined creative approach to measuring precise stellar radial velocity.