OGLE-TR-10 - System
Simulates OGLE-TR-10, a Sun-like G-type star of 1.14 solar masses, and OGLE-TR-10 b, a 0.62-Jupiter-mass companion, with an orbital period of 3.1 days, at 0.043 AU from its star.
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.
OGLE-TR-111 - System
Simulates OGLE-TR-111, an orange K-type dwarf of 0.82 solar masses, and OGLE-TR-111 b, a planet with 11.4 Earth radii, with an orbital period of 4.0 days, at 0.047 AU from its star.
OGLE-TR-113 - System
Simulates OGLE-TR-113, an orange K-type dwarf of 0.78 solar masses, and OGLE-TR-113 b, a 1.26-Jupiter-mass companion, with an orbital period of 1.4 days, at 0.023 AU from its star.
OGLE-TR-132 - System
Simulates OGLE-TR-132, a Sun-like F-type star of 1.30 solar masses, and OGLE-TR-132 b, a 1.18-Jupiter-mass companion, with an orbital period of 1.7 days, at 0.030 AU from its star, and an equilibrium temperature near.
OGLE-TR-182 - System
Simulates OGLE-TR-182, a Sun-like G-type star of 1.14 solar masses, and OGLE-TR-182 b, a 1.01-Jupiter-mass companion, with an orbital period of 4.0 days, at 0.051 AU from its star.
OGLE-TR-211 - System
Simulates OGLE-TR-211, a Sun-like F-type star of 1.33 solar masses, and OGLE-TR-211 b, a 1.03-Jupiter-mass companion, with an orbital period of 3.7 days, at 0.051 AU from its star.
OGLE-TR-56 - System
Simulates OGLE-TR-56 b, the first planet discovered by the transit method itself. Earlier transiting worlds had already been found by radial velocity.
OGLE2-TR-L9 - System
Simulates OGLE2-TR-L9, a Sun-like F-type star of 1.52 solar masses, and OGLE2-TR-L9 b, a 4.50-Jupiter-mass companion, with an orbital period of 2.5 days, at 0.031 AU from its star.
Oph 11 - System
Simulates Oph 11, a cool M-dwarf of 0.02 solar masses, and Oph 11 b, a 14.0-Jupiter-mass companion, with an orbital period of 19,986 years, at 243 AU from its star, and an equilibrium temperature near 2,175 K.
PDS 70 - System
Simulates PDS 70, the first system where planets were seen still forming. Two giants sit inside a gap they have cleared in the protoplanetary disk. Both PDS 70 b and c are still accreting gas.
PH1 - System
Simulates PH1, or Kepler-64 b, a planet in a quadruple star system. It orbits one stellar pair while a second binary shines in the distance. Volunteers in Planet Hunters spotted it in Kepler data.
PH2 - System
Simulates PH2, a Sun-like G-type star of 0.97 solar masses, and PH2 b, a 0.27-Jupiter-mass companion, with an orbital period of 283 days, at 0.833 AU from its star, and an equilibrium temperature near 295 K.
POTS-1 - System
Simulates POTS-1, an orange K-type dwarf of 0.69 solar masses, and POTS-1 b, a 2.31-Jupiter-mass companion, with an orbital period of 3.2 days, at 0.037 AU from its star.
PSR B0329+54 - System
Simulates PSR B0329+54, a Sun-like G-type star of 1.44 solar masses, and PSR B0329+54 b, a 2.0-Earth-mass planet, with an orbital period of 27.8 years, at 10.3 AU from its star, on an eccentric orbit (e ≈ 0.24).
PSR B1257+12 - System
Simulates PSR B1257+12, the first confirmed exoplanets. In 1992 pulsar timing revealed three worlds, including a Moon-mass body, around a dead star. The host is a millisecond pulsar, not a living star.
PSR B1620-26 - System
Simulates the Methuselah planet PSR B1620-26 b, about 12.7 billion years old. It circles a pulsar and white dwarf in the globular cluster Messier 4. Its orbit around the pair takes roughly a century.
PSR J1719-1438 - System
Simulates PSR J1719-1438 b, the so-called diamond planet. This ultra-dense remnant orbits a millisecond pulsar every 2.2 hours and may be crystallized carbon.
PSR J2322-2650 - System
Simulates PSR J2322-2650, a Sun-like G-type star of 1.40 solar masses, and PSR J2322-2650 b, a 0.79-Jupiter-mass companion, with an orbital period of 7.8 hours, at 0.010 AU from its star.