science & techOur World in Data
The transit method has driven the discovery of thousands of exoplanets
Exoplanets, planets orbiting other stars, were first confirmed in 1992 when Aleksander Wolszczan and Dale Frail found two orbiting a pulsar 2,300 light-years away. The transit method works by watching a star's brightness: when a planet passes in front of it, the light dims by a tiny, regular amount. Measuring those dips reveals the planet's size and orbit, and the method has found far more worlds than any other technique.
Transit surveys like NASA's Kepler mission showed that small planets are common in the galaxy, and they are the main reason the count of known exoplanets has climbed into the thousands.
The first confirmed exoplanets were found orbiting a pulsar, a dead neutron star, rather than a Sun-like star.
background
An exoplanet or extrasolar planet is a planet outside the Solar System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star was in 1995. A different planet, first detected in 1988, was confirmed in 2003. In 2016, it was recognized that the first possible evidence of an exoplanet had been noted in 1917, a precovery. As of 5 November 2026, there are 6,464 confirmed exoplanets in 4,849 planetary systems, with 1,074 systems having more than one planet.
There are many methods of detecting exoplanets. Transit photometry and Doppler spectroscopy have found the most, but these methods suffer from a clear observational bias favoring the detection of large planets close to the star. About 1 in 5 Sun-like stars are estimated to have an "Earth-sized" planet in the habitable zone. Assuming there are 200 billion stars in the Milky Way, it can be hypothesized that there are 11 billion potentially habitable Earth-sized planets in the Milky Way, rising to 40 billion if planets orbiting the numerous red dwarfs are included.
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