51 Pegasi b 2026-11-05
51 Pegasi b is the giant exoplanet whose 1995 discovery established a planet around a Sun-like star. It is a hot Jupiter: its roughly 4.23-day orbital period and about 0.05 astronomical unit separation differ markedly from Jupiter's distant orbit. Earlier confirmed exoplanets had already been found around a pulsar; the host category is part of this discovery's significance.[ref]
Michel Mayor and Didier Queloz used the ELODIE spectrograph to measure periodic Doppler shifts in the host star's spectrum. The star's motion around the shared centre of mass produces alternating approaching and receding velocities even though the planet is unresolved. For a nearly circular orbit and a planet much less massive than its host,
The measured velocity amplitude and period therefore constrain , originally about half Jupiter's mass, rather than independently determining inclination and true mass. Checking spectral-line changes also helps distinguish orbital motion from changing stellar line profiles.[ref]
André Baranne Created 2026-10-18 Updated 2026-11-05
André Baranne designed precision astronomical spectrographs, including the ELODIE spectrograph, which was used for Michel Mayor and Didier Queloz's discovery of the planetary companion to 51 Pegasi. The instrument combined broad spectral coverage with precise radial velocity measurements.
The scientific goal was to distinguish tiny stellar Doppler shifts from instrumental changes. Its design and calibration supported long-term velocity stability sufficient for detecting giant planetary companions. The original instrument paper reports the construction, data treatment and measured performance, making the observing hardware part of the explanation of the discovery.[ref]
Didier Queloz Created 2026-10-18 Updated 2026-11-05
Didier Queloz and Michel Mayor detected a planetary companion to the solar-type star 51 Pegasi through periodic changes in its radial velocity. Their 1995 observations used the ELODIE spectrograph to measure the stellar Doppler shift.
The signal repeated in about four days, implying a close companion rather than a distant analogue of Jupiter. The inferred minimum companion mass was planetary. Because radial velocity measures only the line-of-sight component of the reflex motion, the orbital inclination remains part of the mass inference.[ref]