Earth, planets and orbits
1995
A planet around another sun
Michel Mayor and Didier Queloz
How do you spot a planet you cannot see?
The star 51 Pegasi wobbles back and forth every 4.2 days. Mayor and Queloz realised a giant planet was tugging it, orbiting closer to its star than Mercury is to the Sun. Thousands of planets have been found since.
- Fastest ÷ slowest speed
- 4.00×
- Closest ÷ furthest distance
- 0.25
Each shaded wedge takes the same time to sweep, so all wedges have equal area: the planet races near the Sun and dawdles far away. The chart uses measured years and distances of the eight planets.
How they figured it out
Planet hunters expected planets like Jupiter, taking years to orbit. Michel Mayor and Didier Queloz, using a new spectrograph in southern France, found the star 51 Pegasi wobbling every 4.2 days. A giant planet was orbiting closer to its star than Mercury is to the Sun.
Theory said such “hot Jupiters” should not exist, and many were sceptical. But they were confirmed within weeks, and they changed how we think planets form: planets can migrate. Mayor and Queloz shared the 2019 Nobel Prize in Physics.
The equation
Kepler’s third law, with Newton’s constant: measure the year, and you know the orbit’s size.
See it in real life
The hammer thrower
A hammer thrower spinning a heavy ball leans back and circles too, around a point between them. Stars do the same with their planets. The star’s tiny wobble shifts its light slightly blue, then red, then blue again.
Where engineers use it
Doppler sensing
The star’s wobble is measured by tiny colour shifts, the same physics as Doppler ultrasound.
Where it came from
- Kepler’s laws of planets 1609–1619
Built on
51 Pegasi b obeys Kepler’s laws; its year and its star’s wobble give its orbit and mass.