
Kepler-896 - System
Simulates Kepler-896, a Sun-like G-type star of 0.84 solar masses, and Kepler-896 c, a planet with 3.1 Earth radii, with an orbital period of 29.5 days, at 0.179 AU from its star, and an equilibrium temperature near 515.
Exoplanets
Two-planet systems where mutual perturbations can pump eccentricities, lock mean-motion resonances, or destabilize close pairs. Compare compact Kepler pairs with widely spaced radial-velocity giants.

Simulates Kepler-896, a Sun-like G-type star of 0.84 solar masses, and Kepler-896 c, a planet with 3.1 Earth radii, with an orbital period of 29.5 days, at 0.179 AU from its star, and an equilibrium temperature near 515.

Simulates Kepler-903, a Sun-like G-type star of 0.98 solar masses, and Kepler-903 b, a planet with 2.0 Earth radii, with an orbital period of 10.4 days.

Simulates Kepler-913, a Sun-like F-type star of 1.29 solar masses, and Kepler-913 c, a planet with 3.9 Earth radii, with an orbital period of 5.9 days.

Simulates Kepler-920, a Sun-like G-type star of 0.89 solar masses, and Kepler-920 b, a planet with 2.4 Earth radii, with an orbital period of 6.5 days.

Simulates Kepler-937, a Sun-like F-type star of 1.15 solar masses, and Kepler-937 b, a planet with 3.7 Earth radii, with an orbital period of 67.7 days.

Simulates Kepler-94, an orange K-type dwarf of 0.81 solar masses, and Kepler-94 b, a 10.8-Earth-mass planet, with an orbital period of 2.5 days.

Simulates Kepler-949, a Sun-like G-type star of 0.82 solar masses, and Kepler-949 c, a planet with 3.0 Earth radii, with an orbital period of 21.0 days, at 0.139 AU from its star, and an equilibrium temperature near 582.

Simulates Kepler-953, a Sun-like G-type star of 0.95 solar masses, and Kepler-953 c, a planet with 1.2 Earth radii, with an orbital period of 9.1 days.

Simulates Kepler-967, an orange K-type dwarf of 0.84 solar masses, and Kepler-967 b, a planet with 2.4 Earth radii, with an orbital period of 13.2 days.

Simulates Kepler-969, a Sun-like G-type star of 0.92 solar masses, and Kepler-969 c, a planet with 1.0 Earth radii, with an orbital period of 1.7 days.

Simulates Kepler-974, a cool M-dwarf of 0.52 solar masses, and KOI-1843.03, a 8.0-Earth-mass planet, with an orbital period of 4.2 hours.

Simulates Kepler-975, an orange K-type dwarf of 0.95 solar masses, and Kepler-975 c, a planet with 10.7 Earth radii, with an orbital period of 5.1 days, at 0.057 AU from its star, and an equilibrium temperature near.

Simulates Kepler-990, a Sun-like G-type star of 1.05 solar masses, and Kepler-990 c, a planet with 1.5 Earth radii, with an orbital period of 12.9 hours.

Simulates LHS 1140, a nearby red dwarf with a rocky habitable-zone super-Earth. LHS 1140 b is a leading target for atmospheric study with JWST. An inner planet, LHS 1140 c, transits the star as well.

Simulates LP 890-9, also SPECULOOS-2, an ultracool dwarf with two Earth-sized planets. The outer one transits in the habitable zone. The host is one of the coolest stars known to have planets.

Simulates LTT 1445 A, a cool M-dwarf of 0.26 solar masses, and LTT 1445 A c, a 1.5-Earth-mass planet, with an orbital period of 3.1 days, at 0.027 AU from its star, and an equilibrium temperature near 508 K.

Simulates LTT 3780, a cool M-dwarf of 0.38 solar masses, and LTT 3780 b, a 2.5-Earth-mass planet, with an orbital period of 18.4 hours, at 0.012 AU from its star, and an equilibrium temperature near 903 K.

Simulates LkCa 15, an orange K-type dwarf of 1.00 solar masses, and LkCa 15 b, a confirmed exoplanet, at 14.7 AU from its star.