
CD Cet - System
Simulates CD Cet, a cool M-dwarf of 0.16 solar masses, and CD Cet b, a 4.0-Earth-mass planet, with an orbital period of 2.3 days, at 0.018 AU from its star, and an equilibrium temperature near 464 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 CD Cet, a cool M-dwarf of 0.16 solar masses, and CD Cet b, a 4.0-Earth-mass planet, with an orbital period of 2.3 days, at 0.018 AU from its star, and an equilibrium temperature near 464 K.

Simulates CD-35 2722, a cool M-dwarf of 0.40 solar masses, and CD-35 2722 b, a 29.5-Jupiter-mass companion, at 67.0 AU from its star.

Simulates CFBDSIR J145829+101343, a cool M-dwarf of 0.02 solar masses, and CFBDSIR J145829+101343 b, a 10.5-Jupiter-mass companion, with an orbital period of 27.5 years, at 2.600 AU from its star, and an equilibrium.

Simulates CFHTWIR-Oph 98 A, a cool M-dwarf of 0.01 solar masses, and CFHTWIR-Oph 98 b, a 7.80-Jupiter-mass companion, with an orbital period of 22,012 years, at 200 AU from its star, and an equilibrium temperature near.

Simulates CHXR 73, a cool M-dwarf of 0.35 solar masses, and CHXR 73 b, a 12.6-Jupiter-mass companion, at 210 AU from its star.

Simulates CI Tauri c, a giant planet on a 25-day eccentric orbit. The host is only about 2 million years old and still surrounded by a protoplanetary disk.

Simulates COCONUTS-2 A, a cool M-dwarf of 0.40 solar masses, and COCONUTS-2 b, a 7.50-Jupiter-mass companion, and an equilibrium temperature near 493 K.

Simulates CT Cha, an orange K-type dwarf of 1.00 solar masses, and CT Cha b, a 17.0-Jupiter-mass companion, at 440 AU from its star, and an equilibrium temperature near 2,600 K.

Simulates CWISEP J193518.59-154620.3, a Sun-like G-type star of 0.02 solar masses, and CWISEP J193518.59-154620.3 b, a 15.5-Jupiter-mass companion, at 2.480 AU from its star, and an equilibrium temperature near 390 K.

Simulates CoRoT-1 b, the first exoplanet whose changing phases were seen in visible light. The orbiting hot Jupiter brightens and fades like a moon. The signal is the planet's own changing brightness.

Simulates CoRoT-10, an orange K-type dwarf of 0.89 solar masses, and CoRoT-10 b, a 2.75-Jupiter-mass companion, with an orbital period of 13.2 days, at 0.105 AU from its star, and an equilibrium temperature near 600 K.

Simulates CoRoT-11, a Sun-like F-type star of 1.27 solar masses, and CoRoT-11 b, a 2.33-Jupiter-mass companion, with an orbital period of 3.0 days, at 0.044 AU from its star, and an equilibrium temperature near 1,657 K.

Simulates CoRoT-12, a Sun-like G-type star of 1.08 solar masses, and CoRoT-12 b, a 0.92-Jupiter-mass companion, with an orbital period of 2.8 days, at 0.040 AU from its star, and an equilibrium temperature near 1,442 K.

Simulates CoRoT-13, a Sun-like G-type star of 1.09 solar masses, and CoRoT-13 b, a 1.31-Jupiter-mass companion, with an orbital period of 4.0 days, at 0.051 AU from its star, and an equilibrium temperature near 1,700 K.

Simulates CoRoT-14, a Sun-like F-type star of 1.13 solar masses, and CoRoT-14 b, a 7.60-Jupiter-mass companion, with an orbital period of 1.5 days, at 0.027 AU from its star, and an equilibrium temperature near 1,952 K.

Simulates CoRoT-16, a Sun-like G-type star of 1.10 solar masses, and CoRoT-16 b, a 0.54-Jupiter-mass companion, with an orbital period of 5.4 days, at 0.062 AU from its star, on an eccentric orbit (e ≈ 0.33).

Simulates CoRoT-17, a Sun-like G-type star of 1.04 solar masses, and CoRoT-17 b, a 2.43-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.046 AU from its star, and an equilibrium temperature near 1,626 K.

Simulates CoRoT-18, a Sun-like G-type star of 0.95 solar masses, and CoRoT-18 b, a 3.47-Jupiter-mass companion, with an orbital period of 1.9 days, at 0.029 AU from its star, and an equilibrium temperature near 1,550 K.