
TOI-5322 - System
Simulates TOI-5322, a Sun-like G-type star of 1.00 solar masses, and TOI-5322 b, a 0.58-Jupiter-mass companion, with an orbital period of 5.4 days, at 0.060 AU from its star, and an equilibrium temperature near 1,350 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 TOI-5322, a Sun-like G-type star of 1.00 solar masses, and TOI-5322 b, a 0.58-Jupiter-mass companion, with an orbital period of 5.4 days, at 0.060 AU from its star, and an equilibrium temperature near 1,350 K.

Simulates TOI-5340, a Sun-like G-type star of 1.35 solar masses, and TOI-5340 b, a 0.85-Jupiter-mass companion, with an orbital period of 4.9 days, at 0.063 AU from its star, and an equilibrium temperature near 1,566 K.

Simulates TOI-5344, an orange K-type dwarf of 0.61 solar masses, and TOI-5344 b, a 0.41-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.040 AU from its star, and an equilibrium temperature near 689 K.

Simulates TOI-5349, a cool M-dwarf of 0.61 solar masses, and TOI-5349 b, a 0.40-Jupiter-mass companion, with an orbital period of 3.3 days, at 0.037 AU from its star, and an equilibrium temperature near 719 K.

Simulates TOI-5350, a Sun-like F-type star of 1.17 solar masses, and TOI-5350 b, a 6.59-Jupiter-mass companion, with an orbital period of 7.6 days, at 0.080 AU from its star, and an equilibrium temperature near 1,195 K.

Simulates TOI-5386 A, a Sun-like F-type star of 1.17 solar masses, and TOI-5386 A b, a 0.49-Jupiter-mass companion, with an orbital period of 3.6 days, at 0.049 AU from its star, and an equilibrium temperature near.

Simulates TOI-5388, a cool M-dwarf of 0.29 solar masses, and TOI-5388.01, a 2.2-Earth-mass planet, with an orbital period of 2.6 days, and an equilibrium temperature near 488 K.

Simulates TOI-5398, a Sun-like G-type star of 1.15 solar masses, and TOI-5398 c, a 11.8-Earth-mass planet, with an orbital period of 4.8 days, at 0.057 AU from its star, and an equilibrium temperature near 1,242 K.

Simulates TOI-540, a cool M-dwarf of 0.16 solar masses, and TOI-540 b, a planet with 0.9 Earth radii, with an orbital period of 1.2 days, at 0.012 AU from its star, and an equilibrium temperature near 611 K.

Simulates TOI-5422, a Sun-like G-type star of 1.07 solar masses, and TOI-5422 b, a 28.0-Jupiter-mass companion, with an orbital period of 5.4 days, at 0.062 AU from its star, and an equilibrium temperature near 1,369 K.

Simulates TOI-544, an orange K-type dwarf of 0.63 solar masses, and TOI-544 b, a 2.9-Earth-mass planet, with an orbital period of 1.5 days, at 0.022 AU from its star, and an equilibrium temperature near 999 K.

Simulates TOI-5542, a Sun-like G-type star of 0.89 solar masses, and TOI-5542 b, a 1.32-Jupiter-mass companion, with an orbital period of 75.1 days, at 0.332 AU from its star, and an equilibrium temperature near 441 K.

Simulates TOI-5573, an orange K-type dwarf of 0.62 solar masses, and TOI-5573 b, a 0.35-Jupiter-mass companion, with an orbital period of 8.8 days, at 0.071 AU from its star, and an equilibrium temperature near 528 K.

Simulates TOI-558, a Sun-like F-type star of 1.35 solar masses, and TOI-558 b, a 3.61-Jupiter-mass companion, with an orbital period of 14.6 days, at 0.129 AU from its star, and an equilibrium temperature near 1,061 K.

Simulates TOI-559, a Sun-like G-type star of 1.03 solar masses, and TOI-559 b, a 6.01-Jupiter-mass companion, with an orbital period of 7.0 days, at 0.072 AU from its star, and an equilibrium temperature near 1,180 K.

Simulates TOI-5592, a Sun-like F-type star of 1.19 solar masses, and TOI-5592 b, a 0.90-Jupiter-mass companion, with an orbital period of 2.6 days, at 0.039 AU from its star, and an equilibrium temperature near 1,789 K.

Simulates TOI-561, an ancient thick-disk star about 10 billion years old. Its ultra-short-period rocky planet formed when the Milky Way was young. The inner planet's year lasts only about 10.5 hours.

Simulates TOI-5616, an orange K-type dwarf of 0.67 solar masses, and TOI-5616 b, a 1.96-Jupiter-mass companion, with an orbital period of 2.0 days, at 0.027 AU from its star, and an equilibrium temperature near 939 K.