Kepler-187 - System
Simulates Kepler-187, a Sun-like F-type star of 1.08 solar masses, and Kepler-187 b, a planet with 1.4 Earth radii, with an orbital period of 4.9 days, at 0.059 AU from its star.
Exoplanets
2-Planet System
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.
Kepler-188 - System
Simulates Kepler-188, a Sun-like F-type star of 1.02 solar masses, and Kepler-188 b, a planet with 1.7 Earth radii, with an orbital period of 2.1 days, at 0.032 AU from its star.
Kepler-189 - System
Simulates Kepler-189, a Sun-like G-type star of 0.80 solar masses, and Kepler-189 b, a planet with 1.2 Earth radii, with an orbital period of 10.4 days, at 0.088 AU from its star.
Kepler-1894 - System
Simulates Kepler-1894, a Sun-like G-type star of 1.00 solar masses, and Kepler-1894 c, a planet with 1.2 Earth radii, with an orbital period of 5.1 days, at 0.058 AU from its star, and an equilibrium temperature near.
Kepler-19 - System
Simulates Kepler-19, whose unseen outer planet was the first world discovered purely from transit timing. Kepler-19 c never crosses the star itself. Only the inner planet, Kepler-19 b, is seen to transit.
Kepler-190 - System
Simulates Kepler-190, an orange K-type dwarf of 0.83 solar masses, and Kepler-190 b, a planet with 1.6 Earth radii, with an orbital period of 2.0 days, at 0.030 AU from its star.
Kepler-1907 - System
Simulates Kepler-1907, an orange K-type dwarf of 0.75 solar masses, and Kepler-1907 b, a planet with 0.9 Earth radii, with an orbital period of 5.7 days.
Kepler-1921 - System
Simulates Kepler-1921, a Sun-like F-type star of 1.25 solar masses, and Kepler-1921 c, a planet with 1.4 Earth radii, with an orbital period of 3.2 days, at 0.045 AU from its star, and an equilibrium temperature near.
Kepler-193 - System
Simulates Kepler-193, a Sun-like F-type star of 1.05 solar masses, and Kepler-193 b, a planet with 2.4 Earth radii, with an orbital period of 11.4 days, at 0.106 AU from its star.
Kepler-195 - System
Simulates Kepler-195, a Sun-like G-type star of 0.87 solar masses, and Kepler-195 b, a planet with 2.0 Earth radii, with an orbital period of 8.3 days, at 0.077 AU from its star.
Kepler-1972 - System
Simulates Kepler-1972, a Sun-like G-type star of 1.12 solar masses, and Kepler-1972 b, a 2.0-Earth-mass planet, with an orbital period of 7.5 days, on an eccentric orbit (e ≈ 0.07).
Kepler-199 - System
Simulates Kepler-199, a Sun-like G-type star of 0.96 solar masses, and Kepler-199 b, a planet with 3.1 Earth radii, with an orbital period of 23.6 days, at 0.158 AU from its star.
Kepler-1990 - System
Simulates Kepler-1990, a Sun-like G-type star of 1.03 solar masses, and Kepler-1990 b, a planet with 3.3 Earth radii, with an orbital period of 1.7 days, at 0.029 AU from its star, and an equilibrium temperature near.
Kepler-1991 - System
Simulates Kepler-1991, a Sun-like G-type star of 0.91 solar masses, and Kepler-1991 b, a planet with 1.5 Earth radii, with an orbital period of 13.3 days, at 0.106 AU from its star, and an equilibrium temperature near.
Kepler-1996 - System
Simulates Kepler-1996, an orange K-type dwarf of 0.75 solar masses, and Kepler-1996 b, a planet with 2.3 Earth radii, with an orbital period of 32.4 days, at 0.179 AU from its star, and an equilibrium temperature near.
Kepler-200 - System
Simulates Kepler-200, a Sun-like G-type star of 0.97 solar masses, and Kepler-200 b, a planet with 2.1 Earth radii, with an orbital period of 8.6 days, at 0.080 AU from its star.
Kepler-2000 - System
Simulates Kepler-2000, an orange K-type dwarf of 0.58 solar masses, and Kepler-2000 b, a planet with 2.7 Earth radii, with an orbital period of 6.4 days, at 0.056 AU from its star, and an equilibrium temperature near.
Kepler-2001 - System
Simulates Kepler-2001, an orange K-type dwarf of 0.86 solar masses, and Kepler-2001 b, a planet with 1.0 Earth radii, with an orbital period of 1.1 days, at 0.020 AU from its star, and an equilibrium temperature near.