
HD 168009 - System
Simulates HD 168009, a Sun-like G-type star of 0.99 solar masses, and HD 168009 b, a 9.5-Earth-mass planet, with an orbital period of 15.1 days, at 0.119 AU from its star, on an eccentric orbit (e ≈ 0.12).
Browse every interactive 3D gravity simulation — from NASA exoplanet systems and JPL Horizons Solar System models to n-body choreographies, spacecraft trajectories, and hypothetical what-if experiments. All run on Newtonian n-body physics.

Simulates HD 168009, a Sun-like G-type star of 0.99 solar masses, and HD 168009 b, a 9.5-Earth-mass planet, with an orbital period of 15.1 days, at 0.119 AU from its star, on an eccentric orbit (e ≈ 0.12).

Simulates HD 168443, a Sun-like G-type star of 0.98 solar masses, and HD 168443 b, a 7.63-Jupiter-mass companion, with an orbital period of 58.1 days, at 0.292 AU from its star, on an eccentric orbit (e ≈ 0.53).

Simulates HD 168746, a Sun-like G-type star of 1.07 solar masses, and HD 168746 b, a 0.27-Jupiter-mass companion, with an orbital period of 6.4 days, at 0.070 AU from its star, on an eccentric orbit (e ≈ 0.11).

Simulates HD 168863, an orange K-type dwarf of 0.80 solar masses, and HD 168863 b, a 6.78-Jupiter-mass companion, with an orbital period of 40.4 years, at 11.0 AU from its star, on an eccentric orbit (e ≈ 0.19).

Simulates HD 1690, an orange K-type dwarf of 1.86 solar masses, and HD 1690 b, a 8.79-Jupiter-mass companion, with an orbital period of 1.46 years, at 1.360 AU from its star, on an eccentric orbit (e ≈ 0.64).

Simulates HD 16905, an orange K-type dwarf of 0.85 solar masses, and HD 16905 b, a 11.3-Jupiter-mass companion, with an orbital period of 28.1 years, at 8.800 AU from its star, on an eccentric orbit (e ≈ 0.68).

Simulates HD 169142, a Sun-like F-type star of 1.85 solar masses, and HD 169142 b, a 3.00-Jupiter-mass companion, at 37.2 AU from its star.

Simulates HD 169830, a Sun-like F-type star of 1.17 solar masses, and HD 169830 b, a 2.53-Jupiter-mass companion, with an orbital period of 226 days, at 0.765 AU from its star, on an eccentric orbit (e ≈ 0.29).

Simulates HD 170469, a Sun-like G-type star of 1.10 solar masses, and HD 170469 b, a 0.66-Jupiter-mass companion, with an orbital period of 3.13 years, at 2.240 AU from its star, on an eccentric orbit (e ≈ 0.11).

Simulates HD 17092, an orange K-type dwarf of 6.73 solar masses, and HD 17092 b, a 10.1-Jupiter-mass companion, with an orbital period of 360 days, at 1.310 AU from its star, on an eccentric orbit (e ≈ 0.17).

Simulates HD 171028, a Sun-like G-type star of 1.53 solar masses, and HD 171028 b, a 2.62-Jupiter-mass companion, with an orbital period of 1.51 years, at 1.320 AU from its star, on an eccentric orbit (e ≈ 0.59).

Simulates HD 171238, a Sun-like G-type star of 0.92 solar masses, and HD 171238 b, a 8.80-Jupiter-mass companion, with an orbital period of 4.15 years, at 2.518 AU from its star, on an eccentric orbit (e ≈ 0.36).

Simulates HD 17156 b, an early discovery of an eccentric transiting giant. It spends most of its year far out, then dives in for a brief, hot transit.

Simulates HD 173416, a Sun-like G-type star of 2.00 solar masses, and HD 173416 b, a 1.84-Jupiter-mass companion, with an orbital period of 322 days, at 1.158 AU from its star, on an eccentric orbit (e ≈ 0.21).

Simulates HD 174205, an orange K-type dwarf of 1.80 solar masses, and HD 174205 b, a 4.20-Jupiter-mass companion, with an orbital period of 1.59 years, at 1.700 AU from its star, on an eccentric orbit (e ≈ 0.40).

Simulates HD 175167, a Sun-like G-type star of 1.09 solar masses, and HD 175167 b, a 14.8-Jupiter-mass companion, with an orbital period of 3.22 years, on an eccentric orbit (e ≈ 0.51).

Simulates HD 175541, an orange K-type dwarf of 1.39 solar masses, and HD 175541 b, a 0.60-Jupiter-mass companion, with an orbital period of 298 days, at 0.975 AU from its star, on an eccentric orbit (e ≈ 0.11).

Simulates HD 17674, a Sun-like G-type star of 0.98 solar masses, and HD 17674 b, a 0.87-Jupiter-mass companion, with an orbital period of 1.71 years, at 1.420 AU from its star, on an eccentric orbit (e ≈ 0.13).