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Kepler$97390$ - Übersetzung nach Englisch
![microlensing]]}}
{{col-end}}](https://commons.wikimedia.org/wiki/Special:FilePath/Confirmed exoplanets by methods EPE.svg?width=200 "microlensing]]}}
{{col-end}}")
![Kepler crater]] as photographed by [[Apollo 12]] in 1969](https://commons.wikimedia.org/wiki/Special:FilePath/AS12-52-7745.jpg?width=200 "Kepler crater]] as photographed by [[Apollo 12]] in 1969")
![Monument to Tycho Brahe and Kepler in [[Prague]], Czech Republic](https://commons.wikimedia.org/wiki/Special:FilePath/Brahe kepler.jpg?width=200 "Monument to Tycho Brahe and Kepler in [[Prague]], Czech Republic")
![Karlova street in Old Town, [[Prague]] – house where Kepler lived. Now a museum [https://web.archive.org/web/20090910212442/http://www.keplervpraze.cz/en/]](https://commons.wikimedia.org/wiki/Special:FilePath/Karlova str No4, Prague Old Town.jpg?width=200 "Karlova street in Old Town, [[Prague]] – house where Kepler lived. Now a museum [https://web.archive.org/web/20090910212442/http://www.keplervpraze.cz/en/]")
![Geometrical harmonies from ''[[Harmonice Mundi]]'' (1619)](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler-1619-pl-3.jpg?width=200 "Geometrical harmonies from ''[[Harmonice Mundi]]'' (1619)")
![General Wallenstein]]](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler-Wallenstein-Horoskop.jpg?width=200 "General Wallenstein]]")
![Kepler's [[Platonic solid]] model of the [[Solar System]], from ''[[Mysterium Cosmographicum]]'' (1596)](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler-solar-system-1.png?width=200 "Kepler's [[Platonic solid]] model of the [[Solar System]], from ''[[Mysterium Cosmographicum]]'' (1596)")
![Diagram of the [[geocentric]] trajectory of Mars through several periods of [[apparent retrograde motion]] in ''Astronomia Nova'' (1609)](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler Mars retrograde.jpg?width=200 "Diagram of the [[geocentric]] trajectory of Mars through several periods of [[apparent retrograde motion]] in ''Astronomia Nova'' (1609)")
![A plate from ''Astronomiae Pars Optica'', illustrating the structure of [[eye]]s of various species](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler Optica.jpg?width=200 "A plate from ''Astronomiae Pars Optica'', illustrating the structure of [[eye]]s of various species")
![A statue of Kepler in [[Linz]]](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler Statue Linz.jpg?width=200 "A statue of Kepler in [[Linz]]")
![A diagram illustrating the [[Kepler conjecture]] from ''Strena Seu de Nive Sexangula'' (1611)](https://commons.wikimedia.org/wiki/Special:FilePath/Kepler conjecture 1.jpg?width=200 "A diagram illustrating the [[Kepler conjecture]] from ''Strena Seu de Nive Sexangula'' (1611)")
![Remnant of Kepler's Supernova [[SN 1604]]](https://commons.wikimedia.org/wiki/Special:FilePath/Keplers supernova.jpg?width=200 "Remnant of Kepler's Supernova [[SN 1604]]")
![GDR]] stamp featuring Kepler](https://commons.wikimedia.org/wiki/Special:FilePath/Stamps of Germany (DDR) 1971, MiNr 1649.jpg?width=200 "GDR]] stamp featuring Kepler")
![[[Tycho Brahe]]](https://commons.wikimedia.org/wiki/Special:FilePath/Tycho Brahe.JPG?width=200 "[[Tycho Brahe]]")
![As a child, Kepler witnessed the [[Great Comet of 1577]], which attracted the attention of astronomers across Europe.](https://commons.wikimedia.org/wiki/Special:FilePath/Von einem Schrecklichen vnd Wunderbarlichen Cometen so sich den Dienstag nach Martini dieses lauffenden M. D. Lxxvij. Jahrs am Himmel erzeiget hat (grayscale).png?width=200 "As a child, Kepler witnessed the [[Great Comet of 1577]], which attracted the attention of astronomers across Europe.")
Definition
Wikipedia
From the total of 3,943 stars known to have exoplanets (as of April 1, 2023), there are a total of 855 known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are Sol (the Solar System's star, also referred to as the Sun) and Kepler-90 with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets.
The 855 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d). The nearest system with four or more confirmed planets is Tau Ceti, 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 the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. 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.
