
HD 203030 - System
Simulates HD 203030, a Sun-like G-type star of 0.94 solar masses, and HD 203030 b, a 11.0-Jupiter-mass companion, and an equilibrium temperature near 1,040 K.
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 203030, a Sun-like G-type star of 0.94 solar masses, and HD 203030 b, a 11.0-Jupiter-mass companion, and an equilibrium temperature near 1,040 K.

Simulates HD 20329, a Sun-like G-type star of 0.90 solar masses, and HD 20329 b, a 7.4-Earth-mass planet, with an orbital period of 22.2 hours, at 0.018 AU from its star, and an equilibrium temperature near 2,141 K.

Simulates HD 203387, an orange K-type dwarf of 2.82 solar masses, and HD 203387 b, a 3.48-Jupiter-mass companion, with an orbital period of 1.40 years, at 1.771 AU from its star, on an eccentric orbit (e ≈ 0.73).

Simulates HD 2039, a Sun-like G-type star of 1.23 solar masses, and HD 2039 b, a 6.29-Jupiter-mass companion, with an orbital period of 3.07 years, at 2.200 AU from its star, on an eccentric orbit (e ≈ 0.71).

Simulates HD 204313, a Sun-like G-type star of 1.03 solar masses, and HD 204313 c, a 0.05-Jupiter-mass companion, with an orbital period of 35.0 days, at 0.211 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates HD 204941, an orange K-type dwarf of 0.58 solar masses, and HD 204941 b, a 0.23-Jupiter-mass companion, with an orbital period of 4.74 years, at 2.550 AU from its star, on an eccentric orbit (e ≈ 0.37).

Simulates HD 205158, a Sun-like F-type star of 1.16 solar masses, and HD 205158 b, a 0.39-Jupiter-mass companion, with an orbital period of 25.3 days, at 0.177 AU from its star, on an eccentric orbit (e ≈ 0.14).

Simulates HD 205739, a Sun-like F-type star of 1.22 solar masses, and HD 205739 b, a 1.37-Jupiter-mass companion, with an orbital period of 280 days, at 0.896 AU from its star, on an eccentric orbit (e ≈ 0.27).

Simulates HD 206255, a Sun-like G-type star of 1.42 solar masses, and HD 206255 b, a 0.11-Jupiter-mass companion, with an orbital period of 96.0 days, at 0.461 AU from its star, on an eccentric orbit (e ≈ 0.23).

Simulates HD 206610, an orange K-type dwarf of 1.55 solar masses, and HD 206610 b, a 2.04-Jupiter-mass companion, with an orbital period of 1.84 years, at 1.740 AU from its star, on an eccentric orbit (e ≈ 0.10).

Simulates HD 206893, a Sun-like F-type star of 1.31 solar masses, and HD 206893 c, a 11.1-Jupiter-mass companion, with an orbital period of 6.27 years, at 3.740 AU from its star, on an eccentric orbit (e ≈ 0.28).

Simulates HD 207496, an orange K-type dwarf of 0.80 solar masses, and HD 207496 b, a 6.1-Earth-mass planet, with an orbital period of 6.4 days, at 0.063 AU from its star, and an equilibrium temperature near 743 K.

Simulates HD 20781, an orange K-type dwarf of 0.70 solar masses, and HD 20781 b, a 1.9-Earth-mass planet, with an orbital period of 5.3 days, at 0.053 AU from its star, on an eccentric orbit (e ≈ 0.10).

Simulates HD 20782 b, a giant whose eccentricity is about 0.95 — among the most elongated planetary orbits known. It nearly skims the star, then retreats.

Simulates HD 207832, a Sun-like G-type star of 1.05 solar masses, and HD 207832 b, a 0.56-Jupiter-mass companion, with an orbital period of 160 days, at 0.586 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 207897, an orange K-type dwarf of 0.82 solar masses, and HD 207897 b, a 14.8-Earth-mass planet, with an orbital period of 16.2 days, at 0.117 AU from its star, and an equilibrium temperature near 582 K.

Simulates HD 20794, a Sun-like G-type star of 0.79 solar masses, and HD 20794 b, a 2.1-Earth-mass planet, with an orbital period of 18.3 days, at 0.126 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates HD 208487, a Sun-like G-type star of 1.15 solar masses, and HD 208487 b, a 0.46-Jupiter-mass companion, with an orbital period of 129 days, at 0.530 AU from its star, on an eccentric orbit (e ≈ 0.37).