
ISO-Oph 96 - System
Simulates ISO-Oph 96, an orange K-type dwarf of 0.41 solar masses, and KOINTREAU-3 b, a 3.40-Jupiter-mass companion, at 342 AU from its star.
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 ISO-Oph 96, an orange K-type dwarf of 0.41 solar masses, and KOINTREAU-3 b, a 3.40-Jupiter-mass companion, at 342 AU from its star.

Simulates ITG 15 A, a Sun-like G-type star of 1.00 solar masses, and ITG 15 b, a 21.0-Jupiter-mass companion, at 435 AU from its star, and an equilibrium temperature near 2,601 K.

Simulates K2-10, a Sun-like G-type star of 0.88 solar masses, and K2-10 b, a 0.08-Jupiter-mass companion, with an orbital period of 19.3 days, and an equilibrium temperature near 649 K.

Simulates K2-100, a Sun-like G-type star of 1.15 solar masses, and K2-100 b, a 0.07-Jupiter-mass companion, with an orbital period of 1.7 days, at 0.030 AU from its star, and an equilibrium temperature near 1,841 K.

Simulates K2-101, an orange K-type dwarf of 0.82 solar masses, and K2-101 b, a planet with 2.0 Earth radii, with an orbital period of 14.7 days, at 0.112 AU from its star, and an equilibrium temperature near 618 K.

Simulates K2-104, an orange K-type dwarf of 0.51 solar masses, and K2-104 b, a planet with 1.8 Earth radii, with an orbital period of 2.0 days, at 0.024 AU from its star, and an equilibrium temperature near 798 K.

Simulates K2-105, a Sun-like G-type star of 0.94 solar masses, and K2-105 b, a 15.4-Earth-mass planet, with an orbital period of 8.3 days, and an equilibrium temperature near 805 K.

Simulates K2-107, a Sun-like F-type star of 1.30 solar masses, and K2-107 b, a planet with 16.0 Earth radii, with an orbital period of 3.3 days, at 0.048 AU from its star, and an equilibrium temperature near 1,649 K.

Simulates K2-108, a Sun-like G-type star of 1.17 solar masses, and K2-108 b, a planet with 5.3 Earth radii, with an orbital period of 4.7 days, at 0.058 AU from its star, and an equilibrium temperature near 1,360 K.

Simulates K2-11, a Sun-like G-type star of 1.35 solar masses, and K2-11 b, a planet with 7.5 Earth radii, with an orbital period of 39.9 days, at 0.226 AU from its star, and an equilibrium temperature near 734 K.

Simulates K2-110, an orange K-type dwarf of 0.74 solar masses, and K2-110 b, a 0.05-Jupiter-mass companion, with an orbital period of 13.9 days, at 0.102 AU from its star, and an equilibrium temperature near 638 K.

Simulates K2-111, a Sun-like G-type star of 0.84 solar masses, and K2-111 b, a 5.3-Earth-mass planet, with an orbital period of 5.4 days, at 0.057 AU from its star, and an equilibrium temperature near 1,293 K.

Simulates K2-113, a Sun-like G-type star of 1.04 solar masses, and K2-113 b, a planet with 12.1 Earth radii, with an orbital period of 5.8 days, at 0.064 AU from its star, and an equilibrium temperature near 1,098 K.

Simulates K2-114, an orange K-type dwarf of 0.86 solar masses, and K2-114 b, a 2.01-Jupiter-mass companion, with an orbital period of 11.4 days, at 0.094 AU from its star, and an equilibrium temperature near 701 K.

Simulates K2-115, a Sun-like G-type star of 0.92 solar masses, and K2-115 b, a 1.01-Jupiter-mass companion, with an orbital period of 20.3 days, at 0.141 AU from its star, and an equilibrium temperature near 696 K.

Simulates K2-116, an orange K-type dwarf of 0.69 solar masses, and K2-116 b, a planet with 0.7 Earth radii, with an orbital period of 4.7 days, at 0.048 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates K2-117, an orange K-type dwarf of 0.54 solar masses, and K2-117 b, a planet with 2.0 Earth radii, with an orbital period of 1.3 days, at 0.019 AU from its star, and an equilibrium temperature near 868 K.

Simulates K2-118, an orange K-type dwarf of 0.76 solar masses, and K2-118 b, a planet with 2.5 Earth radii, with an orbital period of 50.9 days, at 0.245 AU from its star, on an eccentric orbit (e ≈ 0.20).