
HD 43197 - System
Simulates HD 43197, a Sun-like G-type star of 0.96 solar masses, and HD 43197 b, a 0.55-Jupiter-mass companion, with an orbital period of 309 days, at 0.882 AU from its star, on an eccentric orbit (e ≈ 0.74).
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 HD 43197, a Sun-like G-type star of 0.96 solar masses, and HD 43197 b, a 0.55-Jupiter-mass companion, with an orbital period of 309 days, at 0.882 AU from its star, on an eccentric orbit (e ≈ 0.74).

Simulates HD 43691, a Sun-like G-type star of 1.32 solar masses, and HD 43691 b, a 2.55-Jupiter-mass companion, with an orbital period of 37.0 days, at 0.238 AU from its star, on an eccentric orbit (e ≈ 0.08).

Simulates HD 44219, a Sun-like G-type star of 1.20 solar masses, and HD 44219 b, a 0.58-Jupiter-mass companion, with an orbital period of 1.29 years, at 1.260 AU from its star, on an eccentric orbit (e ≈ 0.41).

Simulates HD 45184, a Sun-like G-type star of 1.03 solar masses, and HD 45184 b, a 12.2-Earth-mass planet, with an orbital period of 5.9 days, at 0.064 AU from its star, on an eccentric orbit (e ≈ 0.07).

Simulates HD 45350, a Sun-like G-type star of 0.98 solar masses, and HD 45350 b, a 1.79-Jupiter-mass companion, with an orbital period of 2.64 years, at 1.920 AU from its star, on an eccentric orbit (e ≈ 0.78).

Simulates HD 45364, two giant planets locked in a 3:2 mean-motion resonance. They were likely captured into that rhythm while migrating through the disk.

Simulates HD 45652, a Sun-like G-type star of 0.92 solar masses, and HD 45652 b, a 0.43-Jupiter-mass companion, with an orbital period of 44.1 days, at 0.237 AU from its star, on an eccentric orbit (e ≈ 0.61).

Simulates HD 457, a Sun-like F-type star of 1.15 solar masses, and HD 457 b, a 26.6-Jupiter-mass companion, with an orbital period of 55.6 years, at 15.4 AU from its star, on an eccentric orbit (e ≈ 0.56).

Simulates HD 46375, a Sun-like G-type star of 0.92 solar masses, and HD 46375 b, a 0.23-Jupiter-mass companion, with an orbital period of 3.0 days, at 0.040 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates HD 47186, a Sun-like G-type star of 0.96 solar masses, and HD 47186 b, a 0.07-Jupiter-mass companion, with an orbital period of 4.1 days, at 0.050 AU from its star.

Simulates HD 4732, an orange K-type dwarf of 1.39 solar masses, and HD 4732 b, a 1.99-Jupiter-mass companion, with an orbital period of 1.02 years, at 1.129 AU from its star, on an eccentric orbit (e ≈ 0.27).

Simulates HD 47366, an orange K-type dwarf of 1.81 solar masses, and HD 47366 b, a 2.08-Jupiter-mass companion, with an orbital period of 360 days, at 1.207 AU from its star, on an eccentric orbit (e ≈ 0.07).

Simulates HD 47536, an orange K-type dwarf of 2.10 solar masses, and HD 47536 b, a 7.32-Jupiter-mass companion, with an orbital period of 1.95 years, at 1.930 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 4760, an orange K-type dwarf of 1.05 solar masses, and HD 4760 b, a 13.9-Jupiter-mass companion, with an orbital period of 1.19 years, at 1.140 AU from its star, on an eccentric orbit (e ≈ 0.23).

Simulates HD 48265, a Sun-like G-type star of 1.38 solar masses, and HD 48265 b, a 1.52-Jupiter-mass companion, with an orbital period of 2.13 years, at 1.814 AU from its star, on an eccentric orbit (e ≈ 0.21).

Simulates HD 48948, an orange K-type dwarf of 0.69 solar masses, and HD 48948 b, a 4.9-Earth-mass planet, with an orbital period of 7.3 days, at 0.065 AU from its star, and an equilibrium temperature near 957 K.

Simulates HD 4917, an orange K-type dwarf of 1.32 solar masses, and HD 4917 b, a 1.61-Jupiter-mass companion, with an orbital period of 1.10 years, at 1.167 AU from its star, on an eccentric orbit (e ≈ 0.07).

Simulates HD 49674, a Sun-like G-type star of 1.03 solar masses, and HD 49674 b, a 0.10-Jupiter-mass companion, with an orbital period of 4.9 days, at 0.060 AU from its star, on an eccentric orbit (e ≈ 0.09).