
HD 1397 - System
Simulates HD 1397, a Sun-like G-type star of 1.32 solar masses, and HD 1397 b, a 0.41-Jupiter-mass companion, with an orbital period of 11.5 days, at 0.110 AU from its star, and an equilibrium temperature near 1,228 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 HD 1397, a Sun-like G-type star of 1.32 solar masses, and HD 1397 b, a 0.41-Jupiter-mass companion, with an orbital period of 11.5 days, at 0.110 AU from its star, and an equilibrium temperature near 1,228 K.

Simulates HD 14067, a Sun-like G-type star of 2.40 solar masses, and HD 14067 b, a 15.3-Jupiter-mass companion, with an orbital period of 7.51 years, at 5.150 AU from its star, on an eccentric orbit (e ≈ 0.65).

Simulates HD 140901, a Sun-like G-type star of 1.06 solar masses, and HD 140901 b, a 15.6-Earth-mass planet, with an orbital period of 9.0 days, at 0.085 AU from its star, on an eccentric orbit (e ≈ 0.47).

Simulates HD 141004, a Sun-like G-type star of 1.05 solar masses, and HD 141004 b, a 13.6-Earth-mass planet, with an orbital period of 15.5 days, at 0.124 AU from its star, on an eccentric orbit (e ≈ 0.16).

Simulates HD 141399, an orange K-type dwarf of 1.07 solar masses, and HD 141399 b, a 0.45-Jupiter-mass companion, with an orbital period of 94.4 days, at 0.415 AU from its star.

Simulates HD 141937, a Sun-like G-type star of 1.09 solar masses, and HD 141937 b, a 11.3-Jupiter-mass companion, with an orbital period of 1.81 years, at 1.540 AU from its star, on an eccentric orbit (e ≈ 0.46).

Simulates HD 142, a Sun-like F-type star of 1.21 solar masses, and HD 142 A d, a 0.26-Jupiter-mass companion, with an orbital period of 108 days, at 0.474 AU from its star, on an eccentric orbit (e ≈ 0.13).

Simulates HD 142022 A, a Sun-like G-type star of 0.90 solar masses, and HD 142022 A b, a 4.44-Jupiter-mass companion, with an orbital period of 5.28 years, at 2.930 AU from its star, on an eccentric orbit (e ≈ 0.53).

Simulates HD 142245, an orange K-type dwarf of 3.50 solar masses, and HD 142245 b, a 3.07-Jupiter-mass companion, with an orbital period of 3.56 years, at 2.780 AU from its star.

Simulates HD 142415, a Sun-like G-type star of 1.07 solar masses, and HD 142415 b, a 1.67-Jupiter-mass companion, with an orbital period of 1.06 years, at 1.060 AU from its star, on an eccentric orbit (e ≈ 0.50).

Simulates HD 143105, a Sun-like F-type star of 1.51 solar masses, and HD 143105 b, a 1.21-Jupiter-mass companion, with an orbital period of 2.2 days, at 0.038 AU from its star, on an eccentric orbit (e ≈ 0.07).

Simulates HD 143361, a Sun-like G-type star of 0.97 solar masses, and HD 143361 b, a 3.53-Jupiter-mass companion, with an orbital period of 2.85 years, at 1.988 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 143811 A, a Sun-like F-type star of 1.32 solar masses, and HD 143811 AB b, a 6.10-Jupiter-mass companion, with an orbital period of 320 years, at 63.0 AU from its star, on an eccentric orbit (e ≈ 0.19).

Simulates HD 144899, a Sun-like F-type star of 1.16 solar masses, and HD 144899 b, a 0.06-Jupiter-mass companion, with an orbital period of 40.4 days, at 0.242 AU from its star, on an eccentric orbit (e ≈ 0.82).

Simulates HD 145377, a Sun-like F-type star of 1.20 solar masses, and HD 145377 b, a 6.02-Jupiter-mass companion, with an orbital period of 104 days, at 0.450 AU from its star, on an eccentric orbit (e ≈ 0.31).

Simulates HD 145457, an orange K-type dwarf of 1.90 solar masses, and HD 145457 b, a 2.79-Jupiter-mass companion, with an orbital period of 176 days, at 0.762 AU from its star, on an eccentric orbit (e ≈ 0.11).

Simulates HD 145934, an orange K-type dwarf of 2.06 solar masses, and HD 145934 b, a 2.07-Jupiter-mass companion, with an orbital period of 7.53 years, at 4.890 AU from its star, on an eccentric orbit (e ≈ 0.08).

Simulates HD 1461, a Sun-like G-type star of 1.02 solar masses, and HD 1461 b, a 6.4-Earth-mass planet, with an orbital period of 5.8 days, at 0.063 AU from its star, on an eccentric orbit (e ≈ 0.17).