
HD 106906 - System
Simulates HD 106906 b, a giant planet imaged at hundreds of AU. It orbits far above a debris disk, a clue to scattering or a stellar flyby. The planet's separation is hundreds of astronomical units.
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 106906 b, a giant planet imaged at hundreds of AU. It orbits far above a debris disk, a clue to scattering or a stellar flyby. The planet's separation is hundreds of astronomical units.

Simulates HD 10697, a Sun-like G-type star of 0.99 solar masses, and HD 10697 b, a 5.74-Jupiter-mass companion, with an orbital period of 2.94 years, at 2.051 AU from its star, on an eccentric orbit (e ≈ 0.10).

Simulates HD 107148, a Sun-like G-type star of 1.11 solar masses, and HD 107148 c, a 0.06-Jupiter-mass companion, with an orbital period of 18.3 days, at 0.141 AU from its star, on an eccentric orbit (e ≈ 0.34).

Simulates HD 108147, a Sun-like F-type star of 1.22 solar masses, and HD 108147 b, a 0.26-Jupiter-mass companion, with an orbital period of 10.9 days, at 0.102 AU from its star, on an eccentric orbit (e ≈ 0.53).

Simulates HD 108202, an orange K-type dwarf of 0.74 solar masses, and HD 108202 b, a 3.00-Jupiter-mass companion, with an orbital period of 8.19 years, at 3.700 AU from its star, on an eccentric orbit (e ≈ 0.52).

Simulates HD 108236, a Sun-like G-type star of 0.87 solar masses, with its 5 planets on orbits from 3.8 days to 29.5 days.

Simulates HD 108341, an orange K-type dwarf of 0.84 solar masses, and HD 108341 b, a 3.50-Jupiter-mass companion, with an orbital period of 3.09 years, at 2.000 AU from its star, on an eccentric orbit (e ≈ 0.85).

Simulates HD 108863, an orange K-type dwarf of 1.59 solar masses, and HD 108863 b, a 2.41-Jupiter-mass companion, with an orbital period of 1.20 years, at 1.320 AU from its star.

Simulates HD 108874, a Sun-like G-type star of 0.95 solar masses, and HD 108874 b, a 1.42-Jupiter-mass companion, with an orbital period of 1.08 years, at 1.040 AU from its star, on an eccentric orbit (e ≈ 0.13).

Simulates HD 109246, a Sun-like G-type star of 1.20 solar masses, and HD 109246 b, a 0.86-Jupiter-mass companion, with an orbital period of 68.3 days, at 0.330 AU from its star, on an eccentric orbit (e ≈ 0.12).

Simulates HD 109271, a Sun-like G-type star of 1.05 solar masses, and HD 109271 b, a 0.05-Jupiter-mass companion, with an orbital period of 7.9 days, at 0.079 AU from its star, on an eccentric orbit (e ≈ 0.25).

Simulates HD 109286, a Sun-like G-type star of 0.98 solar masses, and HD 109286 b, a 2.99-Jupiter-mass companion, with an orbital period of 1.42 years, at 1.259 AU from its star, and an equilibrium temperature near 259.

Simulates HD 109749, a Sun-like G-type star of 1.13 solar masses, and HD 109749 b, a 0.27-Jupiter-mass companion, with an orbital period of 5.2 days, at 0.061 AU from its star.

Simulates HD 10975, an orange K-type dwarf of 1.41 solar masses, and HD 10975 b, a 0.45-Jupiter-mass companion, with an orbital period of 284 days, at 0.950 AU from its star, on an eccentric orbit (e ≈ 0.44).

Simulates HD 109988, an orange K-type dwarf of 0.88 solar masses, and HD 109988 b, a 21.8-Jupiter-mass companion, with an orbital period of 46.9 years, at 12.5 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates HD 110014, an orange K-type dwarf of 2.17 solar masses, and HD 110014 b, a 11.1-Jupiter-mass companion, with an orbital period of 2.29 years, at 2.140 AU from its star, on an eccentric orbit (e ≈ 0.46).

Simulates HD 110067, six sub-Neptunes in a resonant chain about 105 light-years away. Their periods follow a neat near-integer pattern around a bright K dwarf.

Simulates HD 110082, a Sun-like F-type star of 1.21 solar masses, and HD 110082 b, a planet with 3.2 Earth radii, with an orbital period of 10.2 days, at 0.113 AU from its star, on an eccentric orbit (e ≈ 0.20).