
HIP 65891 - System
Simulates HIP 65891, an orange K-type dwarf of 2.50 solar masses, and HIP 65891 b, a 6.10-Jupiter-mass companion, with an orbital period of 2.98 years, at 2.820 AU from its star, on an eccentric orbit (e ≈ 0.09).
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 HIP 65891, an orange K-type dwarf of 2.50 solar masses, and HIP 65891 b, a 6.10-Jupiter-mass companion, with an orbital period of 2.98 years, at 2.820 AU from its star, on an eccentric orbit (e ≈ 0.09).

Simulates HIP 66074, an orange K-type dwarf of 0.70 solar masses, and HIP 66074 b, a 5.00-Jupiter-mass companion, with an orbital period of 311 days, at 0.799 AU from its star, on an eccentric orbit (e ≈ 0.95).

Simulates HIP 67522 b, a Jupiter-sized planet around a 17-million-year-old Sun-like star. Stellar flares and the young planet interact. The planet's radius is still inflated by youth.

Simulates HIP 67537, an orange K-type dwarf of 2.32 solar masses, and HIP 67537 b, a 13.6-Jupiter-mass companion, with an orbital period of 6.91 years, at 4.807 AU from its star, on an eccentric orbit (e ≈ 0.59).

Simulates HIP 67851, an orange K-type dwarf of 1.28 solar masses, and HIP 67851 b, a 1.15-Jupiter-mass companion, with an orbital period of 89.2 days, at 0.420 AU from its star, on an eccentric orbit (e ≈ 0.13).

Simulates HIP 70849, an orange K-type dwarf of 0.65 solar masses, and HIP 70849 b, a 4.50-Jupiter-mass companion, with an orbital period of 9.99 years, at 3.990 AU from its star, on an eccentric orbit (e ≈ 0.65).

Simulates HIP 71135, a cool M-dwarf of 0.66 solar masses, and HIP 71135 b, a 0.06-Jupiter-mass companion, with an orbital period of 87.2 days, at 0.335 AU from its star, on an eccentric orbit (e ≈ 0.21).

Simulates HIP 74890, an orange K-type dwarf of 1.74 solar masses, and HIP 74890 b, a 2.40-Jupiter-mass companion, with an orbital period of 2.25 years, at 2.100 AU from its star, on an eccentric orbit (e ≈ 0.07).

Simulates HIP 75092, an orange K-type dwarf of 1.28 solar masses, and HIP 75092 b, a 1.79-Jupiter-mass companion, with an orbital period of 2.54 years, at 2.020 AU from its star, on an eccentric orbit (e ≈ 0.42).

Simulates HIP 77900, and HIP 77900 b, a 21.0-Jupiter-mass companion, at 3,319 AU from its star, and an equilibrium temperature near 2,507 K.

Simulates HIP 78530, a hot B-type star of 2.50 solar masses, and HIP 78530 b, a 23.0-Jupiter-mass companion, at 740 AU from its star, and an equilibrium temperature near 2,700 K.

Simulates HIP 79098 AB, and HIP 79098 AB b, a 20.5-Jupiter-mass companion, at 345 AU from its star, and an equilibrium temperature near 2,450 K.

Simulates HIP 79431, a cool M-dwarf of 0.49 solar masses, and HIP 79431 b, a 2.10-Jupiter-mass companion, with an orbital period of 112 days, at 0.360 AU from its star, on an eccentric orbit (e ≈ 0.29).

Simulates HIP 81208 C, a cool M-dwarf of 0.14 solar masses, and HIP 81208 C b, a 14.8-Jupiter-mass companion, with an orbital period of 285 years, at 23.0 AU from its star, and an equilibrium temperature near 2,050 K.

Simulates HIP 8152, a Sun-like G-type star of 0.94 solar masses, and HIP 8152 b, a 8.9-Earth-mass planet, with an orbital period of 10.8 days, at 0.093 AU from its star, and an equilibrium temperature near 795 K.

Simulates HIP 8541, an orange K-type dwarf of 2.01 solar masses, and HD 11343 c, a 0.80-Jupiter-mass companion, with an orbital period of 229 days, at 0.923 AU from its star, on an eccentric orbit (e ≈ 0.17).

Simulates HIP 86221, an orange K-type dwarf of 0.79 solar masses, and HIP 86221 b, a 0.71-Jupiter-mass companion, with an orbital period of 2.2 days, at 0.031 AU from its star, on an eccentric orbit (e ≈ 0.09).

Simulates HIP 90988, an orange K-type dwarf of 1.61 solar masses, and HIP 90988 b, a 2.10-Jupiter-mass companion, with an orbital period of 1.25 years, at 1.360 AU from its star, on an eccentric orbit (e ≈ 0.08).