
HD 35759 - System
Simulates HD 35759, a Sun-like G-type star of 1.15 solar masses, and HD 35759 b, a 3.76-Jupiter-mass companion, with an orbital period of 82.5 days, at 0.389 AU from its star, on an eccentric orbit (e ≈ 0.39).
Exoplanets
Systems with a single confirmed planet. Most are hot Jupiters or super-Earths on short-period orbits; others are distant giants found by radial velocity. A clean two-body laboratory for Keplerian motion around a real star.

Simulates HD 35759, a Sun-like G-type star of 1.15 solar masses, and HD 35759 b, a 3.76-Jupiter-mass companion, with an orbital period of 82.5 days, at 0.389 AU from its star, on an eccentric orbit (e ≈ 0.39).

Simulates HD 360, a Sun-like G-type star of 1.69 solar masses, and HD 360 b, a 0.75-Jupiter-mass companion, with an orbital period of 273 days, at 0.980 AU from its star, on an eccentric orbit (e ≈ 0.14).

Simulates HD 36384, a cool M-dwarf of 1.14 solar masses, and HD 36384 b, a 6.60-Jupiter-mass companion, with an orbital period of 1.34 years, at 1.300 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 3651, a Sun-like G-type star of 0.80 solar masses, and HD 3651 b, a 0.23-Jupiter-mass companion, with an orbital period of 62.3 days, at 0.295 AU from its star, on an eccentric orbit (e ≈ 0.65).

Simulates HD 3765, an orange K-type dwarf of 0.85 solar masses, and HD 3765 b, a 0.17-Jupiter-mass companion, with an orbital period of 3.32 years, at 2.108 AU from its star, on an eccentric orbit (e ≈ 0.30).

Simulates HD 38283, a Sun-like G-type star of 1.37 solar masses, and HD 38283 b, a 0.40-Jupiter-mass companion, with an orbital period of 363 days, at 1.020 AU from its star, on an eccentric orbit (e ≈ 0.41).

Simulates HD 38801, a Sun-like G-type star of 1.21 solar masses, and HD 38801 b, a 9.70-Jupiter-mass companion, with an orbital period of 1.88 years, at 1.623 AU from its star.

Simulates HD 39855, a Sun-like G-type star of 0.87 solar masses, and HD 39855 b, a 8.5-Earth-mass planet, with an orbital period of 3.2 days, at 0.041 AU from its star, on an eccentric orbit (e ≈ 0.14).

Simulates HD 40956, an orange K-type dwarf of 2.00 solar masses, and HD 40956 b, a 2.70-Jupiter-mass companion, with an orbital period of 1.58 years, at 1.400 AU from its star, on an eccentric orbit (e ≈ 0.24).

Simulates HD 40979, a Sun-like F-type star of 1.45 solar masses, and HD 40979 b, a 4.67-Jupiter-mass companion, with an orbital period of 264 days, at 0.850 AU from its star, on an eccentric orbit (e ≈ 0.25).

Simulates HD 4113, a Sun-like G-type star of 1.01 solar masses, and HD 4113 b, a 1.70-Jupiter-mass companion, with an orbital period of 1.44 years, at 1.280 AU from its star, on an eccentric orbit (e ≈ 0.90).

Simulates HD 42012, an orange K-type dwarf of 0.83 solar masses, and HD 42012 b, a 1.60-Jupiter-mass companion, with an orbital period of 2.35 years, at 1.670 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 4208, a Sun-like G-type star of 0.88 solar masses, and HD 4208 b, a 0.81-Jupiter-mass companion, with an orbital period of 2.28 years, at 1.662 AU from its star.

Simulates HD 42618, a Sun-like G-type star of 1.01 solar masses, and HD 42618 b, a 14.4-Earth-mass planet, with an orbital period of 150 days, at 0.554 AU from its star, and an equilibrium temperature near 337 K.

Simulates HD 4308, a Sun-like G-type star of 0.93 solar masses, and HD 4308 b, a 0.05-Jupiter-mass companion, with an orbital period of 15.6 days, at 0.120 AU from its star.

Simulates HD 4313, an orange K-type dwarf of 1.63 solar masses, and HD 4313 b, a 1.93-Jupiter-mass companion, with an orbital period of 356 days, at 1.157 AU from its star, on an eccentric orbit (e ≈ 0.15).

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).