BEBOP-4 A - System
Simulates BEBOP-4 A, a Sun-like G-type star of 1.51 solar masses, and BEBOP-4 AB b, a 26.3-Jupiter-mass companion, with an orbital period of 4.99 years, at 3.634 AU from its star, on an eccentric orbit (e ≈ 0.43).
All Scenarios
Browse every interactive 3D gravity simulation — from NASA exoplanet systems and JPL Horizons Solar System models to n-body choreographies, spacecraft trajectories, and hypothetical what-if experiments. All run on Newtonian n-body physics.
Barnard's star - System
Simulates Barnard's Star, the nearest single star to the Sun. Its low-mass planets are among the closest known worlds beyond the Solar System. The star is famous for its rapid motion across the sky.
Beta Centauri
Simulates Hadar as a hierarchical triple: B-type Aa and Ab (12.0 and 10.6 solar masses) on a 357-day eccentric orbit, with B on a 181-year outer path.
CD Cet - System
Simulates CD Cet, a cool M-dwarf of 0.16 solar masses, and CD Cet b, a 4.0-Earth-mass planet, with an orbital period of 2.3 days, at 0.018 AU from its star, and an equilibrium temperature near 464 K.
CD-35 2722 - System
Simulates CD-35 2722, a cool M-dwarf of 0.40 solar masses, and CD-35 2722 b, a 29.5-Jupiter-mass companion, at 67.0 AU from its star.
CFBDSIR J145829+101343 - System
Simulates CFBDSIR J145829+101343, a cool M-dwarf of 0.02 solar masses, and CFBDSIR J145829+101343 b, a 10.5-Jupiter-mass companion, with an orbital period of 27.5 years, at 2.600 AU from its star, and an equilibrium.
CFHTWIR-Oph 98 A - System
Simulates CFHTWIR-Oph 98 A, a cool M-dwarf of 0.01 solar masses, and CFHTWIR-Oph 98 b, a 7.80-Jupiter-mass companion, with an orbital period of 22,012 years, at 200 AU from its star, and an equilibrium temperature near.
CHXR 73 - System
Simulates CHXR 73, a cool M-dwarf of 0.35 solar masses, and CHXR 73 b, a 12.6-Jupiter-mass companion, at 210 AU from its star.
CI Tau - System
Simulates CI Tauri c, a giant planet on a 25-day eccentric orbit. The host is only about 2 million years old and still surrounded by a protoplanetary disk.
COCONUTS-2 A - System
Simulates COCONUTS-2 A, a cool M-dwarf of 0.40 solar masses, and COCONUTS-2 b, a 7.50-Jupiter-mass companion, and an equilibrium temperature near 493 K.
CT Cha - System
Simulates CT Cha, an orange K-type dwarf of 1.00 solar masses, and CT Cha b, a 17.0-Jupiter-mass companion, at 440 AU from its star, and an equilibrium temperature near 2,600 K.
CWISEP J193518.59-154620.3 - System
Simulates CWISEP J193518.59-154620.3, a Sun-like G-type star of 0.02 solar masses, and CWISEP J193518.59-154620.3 b, a 15.5-Jupiter-mass companion, at 2.480 AU from its star, and an equilibrium temperature near 390 K.
CoRoT-1 - System
Simulates CoRoT-1 b, the first exoplanet whose changing phases were seen in visible light. The orbiting hot Jupiter brightens and fades like a moon. The signal is the planet's own changing brightness.
CoRoT-10 - System
Simulates CoRoT-10, an orange K-type dwarf of 0.89 solar masses, and CoRoT-10 b, a 2.75-Jupiter-mass companion, with an orbital period of 13.2 days, at 0.105 AU from its star, and an equilibrium temperature near 600 K.
CoRoT-11 - System
Simulates CoRoT-11, a Sun-like F-type star of 1.27 solar masses, and CoRoT-11 b, a 2.33-Jupiter-mass companion, with an orbital period of 3.0 days, at 0.044 AU from its star, and an equilibrium temperature near 1,657 K.
CoRoT-12 - System
Simulates CoRoT-12, a Sun-like G-type star of 1.08 solar masses, and CoRoT-12 b, a 0.92-Jupiter-mass companion, with an orbital period of 2.8 days, at 0.040 AU from its star, and an equilibrium temperature near 1,442 K.
CoRoT-13 - System
Simulates CoRoT-13, a Sun-like G-type star of 1.09 solar masses, and CoRoT-13 b, a 1.31-Jupiter-mass companion, with an orbital period of 4.0 days, at 0.051 AU from its star, and an equilibrium temperature near 1,700 K.
CoRoT-14 - System
Simulates CoRoT-14, a Sun-like F-type star of 1.13 solar masses, and CoRoT-14 b, a 7.60-Jupiter-mass companion, with an orbital period of 1.5 days, at 0.027 AU from its star, and an equilibrium temperature near 1,952 K.