HIP 4845 - System
Simulates HIP 4845, an orange K-type dwarf of 0.62 solar masses, and HIP 4845 b, a 14.4-Earth-mass planet, with an orbital period of 34.1 days, at 0.176 AU from its star, on an eccentric orbit (e ≈ 0.25).
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.
HIP 48714 - System
Simulates HIP 48714, a cool M-dwarf of 0.58 solar masses, and HIP 48714 b, a 0.07-Jupiter-mass companion, with an orbital period of 17.8 days, at 0.112 AU from its star, on an eccentric orbit (e ≈ 0.50).
HIP 5158 - System
Simulates HIP 5158, an orange K-type dwarf of 0.78 solar masses, and HIP 5158 b, a 1.42-Jupiter-mass companion, with an orbital period of 346 days, at 0.890 AU from its star, on an eccentric orbit (e ≈ 0.52).
HIP 54373 - System
Simulates HIP 54373, an orange K-type dwarf of 0.57 solar masses, and HIP 54373 b, a 8.6-Earth-mass planet, with an orbital period of 7.8 days, at 0.063 AU from its star, on an eccentric orbit (e ≈ 0.20).
HIP 54515 - System
Simulates HIP 54515, and HIP 54515 b, a 17.7-Jupiter-mass companion, with an orbital period of 90.3 years, at 24.8 AU from its star, on an eccentric orbit (e ≈ 0.42).
HIP 54597 - System
Simulates HIP 54597, an orange K-type dwarf of 0.80 solar masses, and HIP 54597 b, a 2.40-Jupiter-mass companion, with an orbital period of 8.96 years, at 4.000 AU from its star.
HIP 55507 - System
Simulates HIP 55507, an orange K-type dwarf of 0.65 solar masses, and HIP 55507 b, a 8.13-Jupiter-mass companion, with an orbital period of 14.1 years, at 5.062 AU from its star, on an eccentric orbit (e ≈ 0.36).
HIP 56640 - System
Simulates HIP 56640, an orange K-type dwarf of 1.75 solar masses, and HIP 56640 b, a 6.77-Jupiter-mass companion, with an orbital period of 7.33 years, at 4.550 AU from its star, on an eccentric orbit (e ≈ 0.12).
HIP 56998 - System
Simulates HIP 56998, an orange K-type dwarf of 0.65 solar masses, and HD 101581 b, a planet with 1.0 Earth radii, with an orbital period of 4.5 days, at 0.046 AU from its star, and an equilibrium temperature near 834 K.
HIP 57274 - System
Simulates HIP 57274, an orange K-type dwarf of 0.73 solar masses, and HIP 57274 b, a 6.4-Earth-mass planet, with an orbital period of 8.1 days, at 0.070 AU from its star, on an eccentric orbit (e ≈ 0.19).
HIP 5763 - System
Simulates HIP 5763, an orange K-type dwarf of 0.72 solar masses, and HIP 5763 b, a 0.51-Jupiter-mass companion, with an orbital period of 30.0 days, at 0.170 AU from its star, on an eccentric orbit (e ≈ 0.05).
HIP 63242 - System
Simulates HIP 63242, a Sun-like G-type star of 1.54 solar masses, and HIP 63242 b, a 9.18-Jupiter-mass companion, with an orbital period of 125 days, at 0.565 AU from its star, on an eccentric orbit (e ≈ 0.23).
HIP 65 A - System
Simulates HIP 65 A, an orange K-type dwarf of 0.78 solar masses, and HIP 65 A b, a 3.21-Jupiter-mass companion, with an orbital period of 23.5 hours, at 0.018 AU from its star, and an equilibrium temperature near 1,411 K.
HIP 65407 - System
Simulates HIP 65407, an orange K-type dwarf of 0.93 solar masses, and HIP 65407 b, a 0.43-Jupiter-mass companion, with an orbital period of 28.1 days, at 0.177 AU from its star, on an eccentric orbit (e ≈ 0.14).
HIP 65426 - System
Simulates HIP 65426 b, the first exoplanet JWST imaged directly. This wide, young giant was a commissioning target for the telescope's coronagraphs. The planet orbits far outside any region we can transit.
HIP 65891 - System
Simulates HIP 65891, an orange K-type dwarf of 2.50 solar masses, and HIP 65891 b, a 6.10-Jupiter-mass companion, with an orbital period of 2.98 years, at 2.820 AU from its star, on an eccentric orbit (e ≈ 0.09).
HIP 66074 - System
Simulates HIP 66074, an orange K-type dwarf of 0.70 solar masses, and HIP 66074 b, a 5.00-Jupiter-mass companion, with an orbital period of 311 days, at 0.799 AU from its star, on an eccentric orbit (e ≈ 0.95).
HIP 67522 - System
Simulates HIP 67522 b, a Jupiter-sized planet around a 17-million-year-old Sun-like star. Stellar flares and the young planet interact. The planet's radius is still inflated by youth.