
XO-1 - System
Simulates XO-1, a Sun-like G-type star of 0.88 solar masses, and XO-1 b, a 0.83-Jupiter-mass companion, with an orbital period of 3.9 days.
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 XO-1, a Sun-like G-type star of 0.88 solar masses, and XO-1 b, a 0.83-Jupiter-mass companion, with an orbital period of 3.9 days.

Simulates XO-2 N, a Sun-like G-type star of 0.96 solar masses, and XO-2 N b, a 0.59-Jupiter-mass companion, with an orbital period of 2.6 days, at 0.037 AU from its star.

Simulates XO-2 S, a Sun-like G-type star of 0.98 solar masses, and XO-2 S b, a 0.26-Jupiter-mass companion, with an orbital period of 18.2 days, at 0.135 AU from its star, on an eccentric orbit (e ≈ 0.15).

Simulates XO-3 b, a massive hot Jupiter on a tilted, eccentric orbit. Its spin-orbit misalignment is evidence that the planet was scattered inward. The planet is roughly twelve times Jupiter's mass.

Simulates XO-4, a Sun-like F-type star of 1.10 solar masses, and XO-4 b, a 1.42-Jupiter-mass companion, with an orbital period of 4.1 days.

Simulates XO-5, a Sun-like G-type star of 1.04 solar masses, and XO-5 b, a 1.19-Jupiter-mass companion, with an orbital period of 4.2 days, at 0.051 AU from its star, and an equilibrium temperature near 1,230 K.

Simulates XO-6, a Sun-like F-type star of 1.47 solar masses, and XO-6 b, a 4.40-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.082 AU from its star, and an equilibrium temperature near 1,577 K.

Simulates XO-7, a Sun-like G-type star of 1.41 solar masses, and XO-7 b, a 0.71-Jupiter-mass companion, with an orbital period of 2.9 days, at 0.044 AU from its star, and an equilibrium temperature near 1,743 K.

Simulates YZ Cet, a cool M-dwarf of 0.14 solar masses, and YZ Cet b, a 0.7-Earth-mass planet, with an orbital period of 2.0 days, at 0.016 AU from its star, and an equilibrium temperature near 471 K, on an eccentric.

Simulates alf Ari, an orange K-type dwarf of 1.50 solar masses with 1 confirmed companion (alf Ari b) on NASA archive orbits.

Simulates alf Tau, an orange K-type dwarf of 1.13 solar masses with 1 confirmed companion (alf Tau b) on NASA archive orbits.

Simulates b Cen A, a hot B-type star of 5.50 solar masses with 1 confirmed companion (b Cen AB b) on NASA archive orbits.

Simulates bet Cnc, an orange K-type dwarf of 1.70 solar masses with 1 confirmed companion (bet Cnc b) on NASA archive orbits.

Simulates Beta Pictoris, a young star with a famous debris disk and two imaged giant planets. Beta Pic b was the first exoplanet whose spin was measured.

Simulates bet UMi, an orange K-type dwarf of 1.40 solar masses with 1 confirmed companion (bet UMi b) on NASA archive orbits.

Simulates eps CrB, an orange K-type dwarf of 1.70 solar masses with 1 confirmed companion (eps CrB b) on NASA archive orbits.

Simulates Epsilon Eridani, one of the nearest young Sun-like stars. It has a debris disk and a giant planet, a snapshot of an early planetary system. The star itself is only about 10 light-years from the Sun.

Simulates eps Ind A, an orange K-type dwarf of 0.80 solar masses with 1 confirmed companion (eps Ind A b) on NASA archive orbits.