
HD 190647 - System
Simulates HD 190647, a Sun-like G-type star of 1.07 solar masses, and HD 190647 b, a 1.99-Jupiter-mass companion, with an orbital period of 3.22 years, at 2.231 AU from its star, on an eccentric orbit (e ≈ 0.22).
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 190647, a Sun-like G-type star of 1.07 solar masses, and HD 190647 b, a 1.99-Jupiter-mass companion, with an orbital period of 3.22 years, at 2.231 AU from its star, on an eccentric orbit (e ≈ 0.22).

Simulates HD 190984, a Sun-like F-type star of 0.91 solar masses, and HD 190984 b, a 3.10-Jupiter-mass companion, with an orbital period of 13.4 years, at 5.500 AU from its star, on an eccentric orbit (e ≈ 0.57).

Simulates HD 191806, a Sun-like F-type star of 1.07 solar masses, and HD 191806 b, a 9.33-Jupiter-mass companion, with an orbital period of 4.39 years, at 2.749 AU from its star, on an eccentric orbit (e ≈ 0.21).

Simulates HD 191939, a Sun-like G-type star of 0.81 solar masses, with its 6 planets on orbits from 8.9 days to 7.93 years.

Simulates HD 192263, an orange K-type dwarf of 0.66 solar masses, and HD 192263 b, a 0.56-Jupiter-mass companion, with an orbital period of 24.4 days, at 0.150 AU from its star.

Simulates HD 192310, an orange K-type dwarf of 0.80 solar masses, and HD 192310 b, a 0.05-Jupiter-mass companion, with an orbital period of 74.7 days, at 0.320 AU from its star, and an equilibrium temperature near 355.

Simulates HD 192699, an orange K-type dwarf of 1.38 solar masses, and HD 192699 b, a 2.10-Jupiter-mass companion, with an orbital period of 341 days, at 1.063 AU from its star, on an eccentric orbit (e ≈ 0.08).

Simulates HD 194490, a Sun-like G-type star of 1.06 solar masses, and HD 194490 b, a 11.2-Jupiter-mass companion, with an orbital period of 35.8 years, at 11.1 AU from its star, on an eccentric orbit (e ≈ 0.25).

Simulates HD 195019, a Sun-like G-type star of 1.21 solar masses, and HD 195019 b, a 3.98-Jupiter-mass companion, with an orbital period of 18.2 days, at 0.140 AU from its star.

Simulates HD 196050, a Sun-like G-type star of 1.27 solar masses, and HD 196050 b, a 4.70-Jupiter-mass companion, with an orbital period of 3.81 years, at 2.650 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 196067, a Sun-like G-type star of 1.16 solar masses, and HD 196067 b, a 11.4-Jupiter-mass companion, with an orbital period of 9.35 years, at 4.710 AU from its star, on an eccentric orbit (e ≈ 0.56).

Simulates HD 19615, an orange K-type dwarf of 1.10 solar masses, and HD 19615 b, a 8.50-Jupiter-mass companion, with an orbital period of 1.10 years, at 1.100 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 196885 A, a Sun-like F-type star of 1.28 solar masses, and HD 196885 A b, a 2.58-Jupiter-mass companion, with an orbital period of 3.65 years, at 2.370 AU from its star, on an eccentric orbit (e ≈ 0.48).

Simulates HD 197037, a Sun-like F-type star of 1.11 solar masses, and HD 197037 b, a 0.79-Jupiter-mass companion, with an orbital period of 2.84 years, at 2.070 AU from its star, on an eccentric orbit (e ≈ 0.22).

Simulates HD 199509, a Sun-like G-type star of 1.04 solar masses, and HD 199509 b, a 0.14-Jupiter-mass companion, with an orbital period of 99.6 days, at 0.426 AU from its star, on an eccentric orbit (e ≈ 0.37).

Simulates HD 19994, a Sun-like F-type star of 1.36 solar masses, and HD 19994 b, a 1.37-Jupiter-mass companion, with an orbital period of 1.28 years, at 1.305 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates HD 20003, a Sun-like G-type star of 0.88 solar masses, and HD 20003 b, a 11.7-Earth-mass planet, with an orbital period of 11.8 days, at 0.097 AU from its star, on an eccentric orbit (e ≈ 0.36).

Simulates HD 200964, an orange K-type dwarf of 1.39 solar masses, and HD 200964 b, a 1.60-Jupiter-mass companion, with an orbital period of 1.66 years, at 1.565 AU from its star, on an eccentric orbit (e ≈ 0.09).