
USco1556 A - System
Simulates USco1556 A, a cool M-dwarf of 0.33 solar masses, and USco1556 b, a 15.0-Jupiter-mass companion, at 3,500 AU from its star, and an equilibrium temperature near 2,240 K.
Scenarios
Confirmed exoplanet systems from the NASA Exoplanet Archive, built from published orbital elements. Browse from single-planet hosts to compact multi-planet systems such as TRAPPIST-1, and watch how real architectures hold together under Newtonian gravity.

Simulates USco1556 A, a cool M-dwarf of 0.33 solar masses, and USco1556 b, a 15.0-Jupiter-mass companion, at 3,500 AU from its star, and an equilibrium temperature near 2,240 K.

Simulates USco1621 A, a cool M-dwarf of 0.36 solar masses, and USco1621 b, a 16.0-Jupiter-mass companion, at 2,880 AU from its star, and an equilibrium temperature near 2,270 K.

Simulates UZ For, a Sun-like G-type star of 0.70 solar masses, and UZ For c, a 7.70-Jupiter-mass companion, with an orbital period of 5.25 years, at 2.800 AU from its star.

Simulates V0391 Peg, and V0391 Peg b, a 3.20-Jupiter-mass companion, with an orbital period of 3.20 years, at 1.700 AU from its star.

Simulates V1298 Tau, a 20-million-year-old star with four transiting planets. They are still contracting and look far puffier than mature planets. The star is a young K dwarf in Taurus.

Simulates V2376 Ori, a cool M-dwarf of 0.45 solar masses, and V2376 Ori b, a 20.0-Jupiter-mass companion, at 71.0 AU from its star, and an equilibrium temperature near 2,100 K.

Simulates V830 Tau, an orange K-type dwarf of 1.00 solar masses, and V830 Tau b, a 0.70-Jupiter-mass companion, with an orbital period of 4.9 days, at 0.057 AU from its star.

Simulates VHS J125601.92-125723.9, a cool M-dwarf of 0.07 solar masses, and VHS J125601.92-125723.9 b, a 16.0-Jupiter-mass companion, with an orbital period of 15,880 years, at 350 AU from its star, and an equilibrium.

Simulates WASP-1, a Sun-like F-type star of 1.24 solar masses, and WASP-1 b, a 0.85-Jupiter-mass companion, with an orbital period of 2.5 days, at 0.039 AU from its star.

Simulates WASP-10, an orange K-type dwarf of 0.75 solar masses, and WASP-10 b, a 3.15-Jupiter-mass companion, with an orbital period of 3.1 days, at 0.038 AU from its star, and an equilibrium temperature near 1,370 K.

Simulates WASP-100, a Sun-like F-type star of 0.77 solar masses, and WASP-100 b, a 1.26-Jupiter-mass companion, with an orbital period of 2.8 days.

Simulates WASP-101, a Sun-like F-type star of 1.41 solar masses, and WASP-101 b, a 0.51-Jupiter-mass companion, with an orbital period of 3.6 days.

Simulates WASP-102, a Sun-like G-type star of 1.08 solar masses, and WASP-102 b, a 0.62-Jupiter-mass companion, with an orbital period of 2.7 days, at 0.041 AU from its star, and an equilibrium temperature near 1,671 K.

Simulates WASP-103 b, the first planet whose tidal bulge was measured. CHEOPS detected the deformation as this hot Jupiter is stretched by its star. The planet is one of the closest, hottest Jupiters known.

Simulates WASP-104, a Sun-like G-type star of 1.08 solar masses, and WASP-104 b, a 1.27-Jupiter-mass companion, with an orbital period of 1.8 days, at 0.029 AU from its star, and an equilibrium temperature near 1,516 K.

Simulates WASP-105, an orange K-type dwarf of 0.89 solar masses, and WASP-105 b, a 1.80-Jupiter-mass companion, with an orbital period of 7.9 days, at 0.075 AU from its star, and an equilibrium temperature near 900 K.

Simulates WASP-106, a Sun-like F-type star of 1.18 solar masses, and WASP-106 b, a 1.93-Jupiter-mass companion, with an orbital period of 9.3 days, at 0.090 AU from its star.

Simulates WASP-107 b, a super-puff Neptune with a helium tail. It is almost Jupiter-sized but only about 30 Earth masses, and its atmosphere is leaking.