
HD 224538 - System
Simulates HD 224538, a Sun-like F-type star of 1.23 solar masses, and HD 224538 b, a 6.53-Jupiter-mass companion, with an orbital period of 3.29 years, at 2.375 AU from its star, on an eccentric orbit (e ≈ 0.48).
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 224538, a Sun-like F-type star of 1.23 solar masses, and HD 224538 b, a 6.53-Jupiter-mass companion, with an orbital period of 3.29 years, at 2.375 AU from its star, on an eccentric orbit (e ≈ 0.48).

Simulates HD 224693, a Sun-like G-type star of 1.31 solar masses, and HD 224693 b, a 0.70-Jupiter-mass companion, with an orbital period of 26.7 days, at 0.191 AU from its star, on an eccentric orbit (e ≈ 0.10).

Simulates HD 22496, an orange K-type dwarf of 0.68 solar masses, and HD 22496 b, a 5.6-Earth-mass planet, with an orbital period of 5.1 days, at 0.051 AU from its star, and an equilibrium temperature near 573 K.

Simulates HD 22532, a Sun-like G-type star of 1.57 solar masses, and HD 22532 b, a 2.12-Jupiter-mass companion, with an orbital period of 2.39 years, at 1.900 AU from its star.

Simulates HD 22781, an orange K-type dwarf of 0.75 solar masses, and HD 22781 b, a 13.7-Jupiter-mass companion, with an orbital period of 1.45 years, at 1.167 AU from its star, on an eccentric orbit (e ≈ 0.82).

Simulates HD 22946, a Sun-like F-type star of 1.10 solar masses, and TOI-411 b, a 13.7-Earth-mass planet, with an orbital period of 4.0 days, at 0.057 AU from its star, and an equilibrium temperature near 1,241 K.

Simulates HD 23079, a Sun-like F-type star of 1.16 solar masses, and HD 23079 b, a 2.66-Jupiter-mass companion, with an orbital period of 2.01 years, on an eccentric orbit (e ≈ 0.07).

Simulates HD 23127, a Sun-like G-type star of 1.21 solar masses, and HD 23127 b, a 1.53-Jupiter-mass companion, with an orbital period of 3.32 years, at 2.370 AU from its star, on an eccentric orbit (e ≈ 0.41).

Simulates HD 231701, a Sun-like F-type star of 1.21 solar masses, and HD 231701 b, a 1.13-Jupiter-mass companion, with an orbital period of 142 days, at 0.567 AU from its star, on an eccentric orbit (e ≈ 0.13).

Simulates HD 233604, an orange K-type dwarf of 1.50 solar masses, and HD 233604 b, a 6.58-Jupiter-mass companion, with an orbital period of 192 days, at 0.747 AU from its star.

Simulates HD 233832, an orange K-type dwarf of 0.71 solar masses, and HD 233832 b, a 1.78-Jupiter-mass companion, with an orbital period of 5.63 years, at 2.827 AU from its star, on an eccentric orbit (e ≈ 0.36).

Simulates HD 23472, an orange K-type dwarf of 0.67 solar masses, with its 5 planets on orbits from 4.0 days to 29.8 days.

Simulates HD 235088, an orange K-type dwarf of 0.85 solar masses, and HD 235088 b, a 4.2-Earth-mass planet, with an orbital period of 7.4 days, at 0.071 AU from its star.

Simulates HD 23596, a Sun-like F-type star of 1.10 solar masses, and HD 23596 b, a 11.9-Jupiter-mass companion, with an orbital period of 4.20 years, at 2.694 AU from its star, on an eccentric orbit (e ≈ 0.28).

Simulates HD 238090, a cool M-dwarf of 0.58 solar masses, and HD 238090 b, a 6.9-Earth-mass planet, with an orbital period of 13.7 days, at 0.093 AU from its star, and an equilibrium temperature near 470 K.

Simulates HD 238914, an orange K-type dwarf of 1.47 solar masses, and HD 238914 b, a 6.00-Jupiter-mass companion, with an orbital period of 11.2 years, at 5.700 AU from its star, on an eccentric orbit (e ≈ 0.56).

Simulates HD 240210, an orange K-type dwarf of 0.82 solar masses, and HD 240210 b, a 5.21-Jupiter-mass companion, with an orbital period of 1.37 years, at 1.160 AU from its star, on an eccentric orbit (e ≈ 0.15).

Simulates HD 240237, an orange K-type dwarf of 8.76 solar masses, and HD 240237 b, a 15.9-Jupiter-mass companion, with an orbital period of 2.04 years, at 1.920 AU from its star, on an eccentric orbit (e ≈ 0.40).