List of multiplanetary systems

From the total of stars known to have exoplanets (as of ), there are a total of known multiplanetary systems, or stars with at least three confirmed planets, beyond the Solar System. The stars with the most confirmed planets are our Sun and Kepler-90 with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets. The star with the most candidate planets is HD 10180, with a maximum of 9 planets — 6 confirmed and 3 candidates.
The multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to our Solar System, has two planets (b and c) and a third unconfirmed sub-Earth. The nearest system with three or more confirmed planets is Luyten's Star, with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 ly away.
The table below contains information about the coordinates, spectral and physical properties, and number of confirmed planets. The two most important stellar properties are mass and metallicity because they determine how these planetary systems form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close in planets, orbiting at less than 1 AU.
Stars orbited by both planets and brown dwarfs.
Stars orbited by objects on both sides of the 13 Jupiter mass dividing line.
See also.
For links to specific lists of exoplanets see:
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