
PH2 - System
Simulates PH2, a Sun-like G-type star of 0.97 solar masses, and PH2 b, a 0.27-Jupiter-mass companion, with an orbital period of 283 days, at 0.833 AU from its star, and an equilibrium temperature near 295 K.
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 PH2, a Sun-like G-type star of 0.97 solar masses, and PH2 b, a 0.27-Jupiter-mass companion, with an orbital period of 283 days, at 0.833 AU from its star, and an equilibrium temperature near 295 K.

Simulates POTS-1, an orange K-type dwarf of 0.69 solar masses, and POTS-1 b, a 2.31-Jupiter-mass companion, with an orbital period of 3.2 days, at 0.037 AU from its star.

Simulates PSR B0329+54, a Sun-like G-type star of 1.44 solar masses, and PSR B0329+54 b, a 2.0-Earth-mass planet, with an orbital period of 27.8 years, at 10.3 AU from its star, on an eccentric orbit (e ≈ 0.24).

Simulates PSR B1257+12, the first confirmed exoplanets. In 1992 pulsar timing revealed three worlds, including a Moon-mass body, around a dead star. The host is a millisecond pulsar, not a living star.

Simulates the Methuselah planet PSR B1620-26 b, about 12.7 billion years old. It circles a pulsar and white dwarf in the globular cluster Messier 4. Its orbit around the pair takes roughly a century.

Simulates PSR J1719-1438 b, the so-called diamond planet. This ultra-dense remnant orbits a millisecond pulsar every 2.2 hours and may be crystallized carbon.

Simulates PSR J2322-2650, a Sun-like G-type star of 1.40 solar masses, and PSR J2322-2650 b, a 0.79-Jupiter-mass companion, with an orbital period of 7.8 hours, at 0.010 AU from its star.

Simulates PZ Tel, a Sun-like G-type star of 1.36 solar masses, and PZ Tel b, a 27.0-Jupiter-mass companion, with an orbital period of 120 years, at 27.0 AU from its star, on an eccentric orbit (e ≈ 0.52).

Simulates Pr0201, a Sun-like F-type star of 1.24 solar masses, and Pr0201 b, a 0.54-Jupiter-mass companion, with an orbital period of 4.4 days, at 0.060 AU from its star.

Simulates Pr0211, a Sun-like G-type star of 0.94 solar masses, and Pr0211 b, a 1.88-Jupiter-mass companion, with an orbital period of 2.1 days, at 0.032 AU from its star.

Simulates Proxima Centauri, the nearest star to the Sun. Proxima b is an Earth-mass world in the habitable zone, only 4.2 light-years away. The host is a flare-active red dwarf in Alpha Centauri.

Simulates Qatar-1, an orange K-type dwarf of 0.84 solar masses, and Qatar-1 b, a 1.29-Jupiter-mass companion, with an orbital period of 1.4 days, at 0.023 AU from its star, and an equilibrium temperature near 1,418 K.

Simulates Qatar-10, a Sun-like F-type star of 1.16 solar masses, and Qatar-10 b, a 0.74-Jupiter-mass companion, with an orbital period of 1.6 days, at 0.029 AU from its star, and an equilibrium temperature near 1,955 K.

Simulates Qatar-2, an orange K-type dwarf of 0.74 solar masses, and Qatar-2 b, a 2.49-Jupiter-mass companion, with an orbital period of 1.3 days, at 0.022 AU from its star, and an equilibrium temperature near 1,344 K.

Simulates Qatar-3, a Sun-like G-type star of 1.15 solar masses, and Qatar-3 b, a 4.31-Jupiter-mass companion, with an orbital period of 2.5 days, at 0.038 AU from its star, and an equilibrium temperature near 1,681 K.

Simulates Qatar-4, an orange K-type dwarf of 0.90 solar masses, and Qatar-4 b, a 6.10-Jupiter-mass companion, with an orbital period of 1.8 days, at 0.028 AU from its star, and an equilibrium temperature near 1,385 K.

Simulates Qatar-5, a Sun-like G-type star of 1.13 solar masses, and Qatar-5 b, a 4.32-Jupiter-mass companion, with an orbital period of 2.9 days, at 0.041 AU from its star, and an equilibrium temperature near 1,415 K.

Simulates Qatar-6, an orange K-type dwarf of 0.82 solar masses, and Qatar-6 b, a 0.67-Jupiter-mass companion, with an orbital period of 3.5 days, at 0.042 AU from its star, and an equilibrium temperature near 1,006 K.