
K2-75 - System
Simulates K2-75, a Sun-like G-type star of 1.16 solar masses, and K2-75 b, a planet with 2.7 Earth radii, with an orbital period of 7.8 days, at 0.081 AU from its star.
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 K2-75, a Sun-like G-type star of 1.16 solar masses, and K2-75 b, a planet with 2.7 Earth radii, with an orbital period of 7.8 days, at 0.081 AU from its star.

Simulates K2-8, an orange K-type dwarf of 0.78 solar masses, and K2-8 c, a planet with 2.4 Earth radii, with an orbital period of 5.1 days, at 0.053 AU from its star, and an equilibrium temperature near 801 K.

Simulates K2-80, a Sun-like G-type star of 0.90 solar masses, and K2-80 c, a planet with 1.5 Earth radii, with an orbital period of 5.6 days, at 0.060 AU from its star.

Simulates K2-83, an orange K-type dwarf of 0.48 solar masses, and K2-83 b, a planet with 1.2 Earth radii, with an orbital period of 2.7 days, at 0.030 AU from its star.

Simulates K2-84, a Sun-like G-type star of 0.95 solar masses, and K2-84 b, a planet with 2.4 Earth radii, with an orbital period of 6.4 days, at 0.067 AU from its star.

Simulates K2-90, an orange K-type dwarf of 0.63 solar masses, and K2-90 c, a planet with 1.3 Earth radii, with an orbital period of 2.9 days, at 0.035 AU from its star, on an eccentric orbit (e ≈ 0.19).

Simulates K2-99, a Sun-like F-type star of 1.44 solar masses, and K2-99 b, a 0.87-Jupiter-mass companion, with an orbital period of 18.2 days, at 0.153 AU from its star, and an equilibrium temperature near 1,184 K.

Simulates KELT-6, a Sun-like F-type star of 1.13 solar masses, and KELT-6 c, a 3.71-Jupiter-mass companion, with an orbital period of 3.49 years, at 2.390 AU from its star, on an eccentric orbit (e ≈ 0.21).

Simulates KIC 5437945, a Sun-like F-type star of 1.07 solar masses, and Kepler-460 c, a planet with 5.5 Earth radii, with an orbital period of 220 days.

Simulates KIC 9663113, a Sun-like F-type star of 1.15 solar masses, and Kepler-458 c, a planet with 4.2 Earth radii, with an orbital period of 20.7 days.

Simulates KMT-2020-BLG-0414L, a Sun-like G-type star of 0.49 solar masses, and KMT-2020-BLG-0414L b, a 1.9-Earth-mass planet, at 2.070 AU from its star.

Simulates KMT-2021-BLG-1077L, a cool M-dwarf of 0.14 solar masses, and KMT-2021-BLG-1077L c, a 0.25-Jupiter-mass companion, at 0.930 AU from its star.

Simulates KMT-2022-BLG-1818L, a Sun-like G-type star of 0.79 solar masses, and KMT-2022-BLG-1818L b, a 4.00-Jupiter-mass companion, at 2.600 AU from its star.

Simulates KOBE-1, an orange K-type dwarf of 0.63 solar masses, and KOBE-1 b, a 8.8-Earth-mass planet, with an orbital period of 8.5 days, at 0.070 AU from its star, and an equilibrium temperature near 594 K.

Simulates KOI-12, a Sun-like F-type star of 1.50 solar masses, and KOI-12 b, a 1.10-Jupiter-mass companion, with an orbital period of 17.9 days, at 0.154 AU from its star, on an eccentric orbit (e ≈ 0.34).

Simulates KOI-134, a Sun-like F-type star of 1.41 solar masses, and KOI-134 c, a 0.22-Jupiter-mass companion, with an orbital period of 34.0 days, at 0.231 AU from its star, on an eccentric orbit (e ≈ 0.24).

Simulates KOI-1599, a Sun-like G-type star of 1.02 solar masses, and KOI-1599.02, a 9.0-Earth-mass planet, with an orbital period of 13.6 days, at 0.112 AU from its star.

Simulates KOI-1783, a Sun-like G-type star of 1.08 solar masses, and KOI-1783.01, a 0.22-Jupiter-mass companion, with an orbital period of 134 days.