
WASP-18 - System
Simulates WASP-18 b, a massive hot Jupiter ten times Jupiter's mass. It is a key target for measuring whether tides are pulling it into the star. It is one of the most massive hot Jupiters known.
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 WASP-18 b, a massive hot Jupiter ten times Jupiter's mass. It is a key target for measuring whether tides are pulling it into the star. It is one of the most massive hot Jupiters known.

Simulates WASP-41, a Sun-like G-type star of 0.81 solar masses, and WASP-41 c, a 3.18-Jupiter-mass companion, with an orbital period of 1.15 years, at 1.070 AU from its star, and an equilibrium temperature near 241 K.

Simulates WASP-53, an orange K-type dwarf of 0.84 solar masses, and WASP-53 b, a 2.13-Jupiter-mass companion, with an orbital period of 3.3 days, at 0.041 AU from its star, and an equilibrium temperature near 1,053 K.

Simulates WASP-8, a Sun-like G-type star of 1.34 solar masses, and WASP-8 c, a 9.45-Jupiter-mass companion, with an orbital period of 11.8 years, at 5.280 AU from its star.

Simulates WASP-84, an orange K-type dwarf of 0.85 solar masses, and WASP-84 c, a 15.2-Earth-mass planet, with an orbital period of 1.4 days, at 0.024 AU from its star, and an equilibrium temperature near 1,329 K.

Simulates WISPIT 1, an orange K-type dwarf of 0.72 solar masses, and WISPIT 1 b, a 10.4-Jupiter-mass companion, at 338 AU from its star.

Simulates WISPIT 2, an orange K-type dwarf of 1.08 solar masses, and WISPIT 2 c, a 10.0-Jupiter-mass companion, at 14.0 AU from its star, and an equilibrium temperature near 2,050 K.

Simulates Beta Pictoris, a young star with a famous debris disk and two imaged giant planets. Beta Pic b was the first exoplanet whose spin was measured.

Simulates gam Lib, an orange K-type dwarf of 1.78 solar masses with 2 confirmed companions (gam Lib b, gam Lib c) on NASA archive orbits.

Simulates iot Dra, an orange K-type dwarf of 1.54 solar masses with 2 confirmed companions (iot Dra b, iot Dra c) on NASA archive orbits.

Simulates nu Oph, an orange K-type dwarf of 2.61 solar masses with 2 confirmed companions (nu Oph b, nu Oph c) on NASA archive orbits.