
Kepler-1518 - System
Simulates Kepler-1518, a Sun-like F-type star of 1.54 solar masses, and Kepler-1518 c, a planet with 2.9 Earth radii, with an orbital period of 9.6 days, at 0.090 AU from its star, and an equilibrium temperature near.
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-1518, a Sun-like F-type star of 1.54 solar masses, and Kepler-1518 c, a planet with 2.9 Earth radii, with an orbital period of 9.6 days, at 0.090 AU from its star, and an equilibrium temperature near.

Simulates Kepler-152, an orange K-type dwarf of 0.78 solar masses, and Kepler-152 b, a planet with 2.8 Earth radii, with an orbital period of 18.2 days, at 0.124 AU from its star.

Simulates Kepler-153, a Sun-like G-type star of 0.76 solar masses, and Kepler-153 b, a planet with 2.9 Earth radii, with an orbital period of 18.9 days, at 0.129 AU from its star.

Simulates Kepler-155, an orange K-type dwarf of 0.64 solar masses, and Kepler-155 b, a planet with 2.1 Earth radii, with an orbital period of 5.9 days, at 0.056 AU from its star.

Simulates Kepler-156, an orange K-type dwarf of 0.86 solar masses, and Kepler-156 b, a planet with 2.3 Earth radii, with an orbital period of 5.0 days, at 0.054 AU from its star.

Simulates Kepler-158, an orange K-type dwarf of 0.66 solar masses, and Kepler-158 b, a planet with 2.1 Earth radii, with an orbital period of 16.7 days, at 0.111 AU from its star.

Simulates Kepler-159, an orange K-type dwarf of 0.63 solar masses, and Kepler-159 b, a planet with 2.4 Earth radii, with an orbital period of 10.1 days, at 0.082 AU from its star.

Simulates Kepler-1600, a Sun-like G-type star of 0.86 solar masses, and Kepler-1600 c, a planet with 1.9 Earth radii, with an orbital period of 7.3 days.

Simulates Kepler-161, an orange K-type dwarf of 0.85 solar masses, and Kepler-161 b, a planet with 2.1 Earth radii, with an orbital period of 4.9 days, at 0.054 AU from its star.

Simulates Kepler-1610, a Sun-like G-type star of 0.82 solar masses, and Kepler-1610 c, a planet with 2.1 Earth radii, with an orbital period of 45.0 days, at 0.232 AU from its star, and an equilibrium temperature near.

Simulates Kepler-162, a Sun-like G-type star of 1.05 solar masses, and Kepler-162 b, a planet with 1.3 Earth radii, with an orbital period of 6.9 days, at 0.069 AU from its star.

Simulates Kepler-163, a Sun-like G-type star of 0.88 solar masses, and Kepler-163 b, a planet with 1.1 Earth radii, with an orbital period of 7.8 days, at 0.078 AU from its star.

Simulates Kepler-1641, a Sun-like F-type star of 1.12 solar masses, and Kepler-1641 b, a planet with 3.1 Earth radii, with an orbital period of 19.7 days.

Simulates Kepler-1642, a Sun-like G-type star of 0.88 solar masses, and Kepler-1642 c, a planet with 2.7 Earth radii, with an orbital period of 6.7 days.

Simulates Kepler-1649 c, an Earth-sized habitable-zone planet missed by the pipeline and recovered by citizen scientists rechecking Kepler false positives.

Simulates Kepler-165, a Sun-like G-type star of 0.75 solar masses, and Kepler-165 b, a planet with 2.3 Earth radii, with an orbital period of 8.2 days, at 0.072 AU from its star.

Simulates Kepler-1656, a Sun-like G-type star of 1.03 solar masses, and Kepler-1656 b, a 0.15-Jupiter-mass companion, with an orbital period of 31.6 days, at 0.197 AU from its star, on an eccentric orbit (e ≈ 0.84).

Simulates Kepler-1666, a Sun-like F-type star of 1.23 solar masses, and Kepler-1666 b, a planet with 2.9 Earth radii, with an orbital period of 25.8 days.