
HATS-71 - System
Simulates HATS-71, a cool M-dwarf of 0.49 solar masses, and HATS-71 b, a 0.37-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.037 AU from its star, and an equilibrium temperature near 587 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 HATS-71, a cool M-dwarf of 0.49 solar masses, and HATS-71 b, a 0.37-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.037 AU from its star, and an equilibrium temperature near 587 K.

Simulates HATS-72, an orange K-type dwarf of 0.73 solar masses, and HATS-72 b, a 0.13-Jupiter-mass companion, with an orbital period of 7.3 days, at 0.067 AU from its star, and an equilibrium temperature near 739 K.

Simulates HATS-74 A, an orange K-type dwarf of 0.60 solar masses, and HATS-74 A b, a 1.46-Jupiter-mass companion, with an orbital period of 1.7 days, at 0.024 AU from its star, and an equilibrium temperature near 895 K.

Simulates HATS-75, an orange K-type dwarf of 0.60 solar masses, and HATS-75 b, a 0.49-Jupiter-mass companion, with an orbital period of 2.8 days, at 0.033 AU from its star, and an equilibrium temperature near 772 K.

Simulates HATS-76, an orange K-type dwarf of 0.66 solar masses, and HATS-76 b, a 2.63-Jupiter-mass companion, with an orbital period of 1.9 days, at 0.027 AU from its star, and an equilibrium temperature near 940 K.

Simulates HATS-77, an orange K-type dwarf of 0.66 solar masses, and HATS-77 b, a 1.37-Jupiter-mass companion, with an orbital period of 3.1 days, at 0.036 AU from its star, and an equilibrium temperature near 828 K.

Simulates HATS-8, a Sun-like G-type star of 1.06 solar masses, and HATS-8 b, a 0.14-Jupiter-mass companion, with an orbital period of 3.6 days, at 0.047 AU from its star, and an equilibrium temperature near 1,324 K.

Simulates HATS-9, a Sun-like G-type star of 1.10 solar masses, and HATS-9 b, a planet with 13.8 Earth radii, with an orbital period of 1.9 days, at 0.031 AU from its star, and an equilibrium temperature near 1,746 K.

Simulates HD 100508, an orange K-type dwarf of 0.94 solar masses, and HD 100508 b, a 1.20-Jupiter-mass companion, with an orbital period of 15.6 years, at 6.110 AU from its star, on an eccentric orbit (e ≈ 0.42).

Simulates HD 100546, a hot B-type star of 2.40 solar masses, and HD 100546 b, a 8.50-Jupiter-mass companion, at 53.0 AU from its star.

Simulates HD 100655, an orange K-type dwarf of 2.28 solar masses, and HD 100655 b, a 1.61-Jupiter-mass companion, with an orbital period of 158 days, at 0.680 AU from its star, on an eccentric orbit (e ≈ 0.09).

Simulates HD 100777, a Sun-like G-type star of 1.08 solar masses, and HD 100777 b, a 1.23-Jupiter-mass companion, with an orbital period of 1.05 years, at 1.060 AU from its star, on an eccentric orbit (e ≈ 0.38).

Simulates HD 10180, one of the richest radial-velocity systems. At least six planets, mostly packed inside Earth's orbit, orbit this quiet Sun-like star.

Simulates HD 101930, an orange K-type dwarf of 0.57 solar masses, and HD 101930 b, a 0.25-Jupiter-mass companion, with an orbital period of 70.5 days, at 0.300 AU from its star, on an eccentric orbit (e ≈ 0.11).

Simulates HD 102117, a Sun-like G-type star of 1.06 solar masses, and HD 102117 b, a 0.17-Jupiter-mass companion, with an orbital period of 20.8 days, at 0.150 AU from its star, on an eccentric orbit (e ≈ 0.12).

Simulates HD 102195, a Sun-like G-type star of 0.76 solar masses, and HD 102195 b, a 0.41-Jupiter-mass companion, with an orbital period of 4.1 days, at 0.050 AU from its star.

Simulates HD 102272, an orange K-type dwarf of 1.45 solar masses, and HD 102272 b, a 4.94-Jupiter-mass companion, with an orbital period of 128 days, at 0.510 AU from its star.

Simulates HD 102329, an orange K-type dwarf of 3.21 solar masses, and HD 102329 b, a 8.16-Jupiter-mass companion, with an orbital period of 2.13 years, at 1.810 AU from its star, on an eccentric orbit (e ≈ 0.21).