
V2376 Ori - System
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.
Exoplanets
Systems with a single confirmed planet. Most are hot Jupiters or super-Earths on short-period orbits; others are distant giants found by radial velocity. A clean two-body laboratory for Keplerian motion around a real star.

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.

Simulates WASP-11, an orange K-type dwarf of 1.42 solar masses, and WASP-11 b, a 0.79-Jupiter-mass companion, with an orbital period of 3.7 days.

Simulates WASP-113, a Sun-like G-type star of 1.32 solar masses, and WASP-113 b, a 0.47-Jupiter-mass companion, with an orbital period of 4.5 days, at 0.059 AU from its star, and an equilibrium temperature near 1,496 K.

Simulates WASP-114, a Sun-like G-type star of 1.29 solar masses, and WASP-114 b, a 1.77-Jupiter-mass companion, with an orbital period of 1.5 days, at 0.029 AU from its star, and an equilibrium temperature near 2,043 K.

Simulates WASP-116, a Sun-like F-type star of 1.25 solar masses, and WASP-116 b, a 0.64-Jupiter-mass companion, with an orbital period of 6.6 days, at 0.065 AU from its star, and an equilibrium temperature near 1,414 K.

Simulates WASP-117, a Sun-like F-type star of 1.29 solar masses, and WASP-117 b, a 0.30-Jupiter-mass companion, with an orbital period of 10.0 days, on an eccentric orbit (e ≈ 0.30).