
Kepler-215 - System
Simulates Kepler-215, a Sun-like G-type star of 0.79 solar masses, and Kepler-215 b, a planet with 1.6 Earth radii, with an orbital period of 9.4 days, at 0.084 AU from its star.
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 Kepler-215, a Sun-like G-type star of 0.79 solar masses, and Kepler-215 b, a planet with 1.6 Earth radii, with an orbital period of 9.4 days, at 0.084 AU from its star.

Simulates Kepler-216, a Sun-like F-type star of 1.13 solar masses, and Kepler-216 b, a planet with 2.4 Earth radii, with an orbital period of 7.7 days, at 0.079 AU from its star.

Simulates Kepler-217, a Sun-like F-type star of 1.37 solar masses, and Kepler-217 b, a planet with 2.2 Earth radii, with an orbital period of 5.4 days, at 0.065 AU from its star.

Simulates Kepler-218, a Sun-like G-type star of 1.01 solar masses, and Kepler-218 b, a planet with 1.5 Earth radii, with an orbital period of 3.6 days, at 0.046 AU from its star.

Simulates Kepler-219, a Sun-like G-type star of 1.16 solar masses, and Kepler-219 b, a planet with 3.0 Earth radii, with an orbital period of 4.6 days, at 0.057 AU from its star.

Simulates Kepler-22 b, the first planet Kepler found in a habitable zone. This super-Earth-sized world circles a Sun-like star every 290 days. The planet is roughly 2.4 times Earth's radius.

Simulates Kepler-220, an orange K-type dwarf of 0.73 solar masses, and Kepler-220 b, a planet with 0.8 Earth radii, with an orbital period of 4.2 days, at 0.046 AU from its star.

Simulates Kepler-221, a Sun-like G-type star of 0.85 solar masses, and Kepler-221 b, a planet with 1.7 Earth radii, with an orbital period of 2.8 days, at 0.037 AU from its star.

Simulates Kepler-222, a Sun-like G-type star of 0.93 solar masses, and Kepler-222 b, a planet with 3.2 Earth radii, with an orbital period of 3.9 days, at 0.048 AU from its star.

Simulates Kepler-223, four planets locked in a chain of mean-motion resonances. Their orbits repeat like a gravitational clockwork. Neighboring pairs sit in 4:3, 3:2, and 4:3 resonances.

Simulates Kepler-224, an orange K-type dwarf of 0.78 solar masses, and Kepler-224 b, a planet with 1.4 Earth radii, with an orbital period of 3.1 days, at 0.038 AU from its star.

Simulates Kepler-225, a cool M-dwarf of 0.59 solar masses, and Kepler-225 b, a planet with 1.2 Earth radii, with an orbital period of 6.7 days, at 0.056 AU from its star.

Simulates Kepler-226, a Sun-like G-type star of 0.90 solar masses, and Kepler-226 b, a planet with 1.6 Earth radii, with an orbital period of 3.9 days, at 0.047 AU from its star.

Simulates Kepler-227, a Sun-like G-type star of 0.95 solar masses, and Kepler-227 b, a planet with 3.1 Earth radii, with an orbital period of 9.5 days, at 0.090 AU from its star.

Simulates Kepler-228, a Sun-like F-type star of 1.01 solar masses, and Kepler-228 b, a planet with 1.5 Earth radii, with an orbital period of 2.6 days, at 0.038 AU from its star.

Simulates Kepler-229, an orange K-type dwarf of 0.81 solar masses, and Kepler-229 b, a planet with 2.2 Earth radii, with an orbital period of 6.3 days, at 0.062 AU from its star.

Simulates Kepler-23, a Sun-like G-type star of 1.08 solar masses, and Kepler-23 b, a 2.6-Earth-mass planet, with an orbital period of 7.1 days.

Simulates Kepler-230, a Sun-like G-type star of 0.78 solar masses, and Kepler-230 b, a planet with 4.3 Earth radii, with an orbital period of 32.6 days, at 0.191 AU from its star.