
Kepler-1625 - System
Simulates Kepler-1625 b, host of the strongest exomoon candidate yet claimed. A Neptune-sized moon has been proposed from Hubble transit residuals, still unconfirmed.
Browse every interactive 3D gravity simulation — from NASA exoplanet systems and JPL Horizons Solar System models to n-body choreographies, spacecraft trajectories, and hypothetical what-if experiments. All run on Newtonian n-body physics.

Simulates Kepler-1625 b, host of the strongest exomoon candidate yet claimed. A Neptune-sized moon has been proposed from Hubble transit residuals, still unconfirmed.

Simulates Kepler-1626, a Sun-like F-type star of 1.51 solar masses, and Kepler-1626 b, a planet with 2.0 Earth radii, with an orbital period of 4.1 days.

Simulates Kepler-1627, a Sun-like G-type star of 0.87 solar masses, and Kepler-1627 b, a planet with 3.7 Earth radii, with an orbital period of 7.2 days.

Simulates Kepler-1628, an orange K-type dwarf of 0.55 solar masses, and Kepler-1628 b, a planet with 6.4 Earth radii, with an orbital period of 76.4 days.

Simulates Kepler-1629, a Sun-like G-type star of 1.01 solar masses, and Kepler-1629 b, a planet with 0.8 Earth radii, with an orbital period of 3.9 days.

Simulates Kepler-163, a Sun-like G-type star of 0.88 solar masses, and Kepler-163 b, a planet with 1.1 Earth radii, with an orbital period of 7.8 days, at 0.078 AU from its star.

Simulates Kepler-1630, an orange K-type dwarf of 0.66 solar masses, and Kepler-1630 b, a planet with 2.2 Earth radii, with an orbital period of 1.40 years.

Simulates Kepler-1631, a Sun-like G-type star of 0.97 solar masses, and Kepler-1631 b, a planet with 1.4 Earth radii, with an orbital period of 4.1 days.

Simulates Kepler-1632, a Sun-like F-type star of 1.12 solar masses, and Kepler-1632 b, a planet with 2.5 Earth radii, with an orbital period of 1.23 years.

Simulates Kepler-1633, a Sun-like F-type star of 1.20 solar masses, and Kepler-1633 b, a planet with 1.6 Earth radii, with an orbital period of 186 days.

Simulates Kepler-1634, a Sun-like G-type star of 0.92 solar masses, and Kepler-1634 b, a planet with 3.2 Earth radii, with an orbital period of 1.03 years.

Simulates Kepler-1635, a Sun-like G-type star of 0.89 solar masses, and Kepler-1635 b, a planet with 3.6 Earth radii, with an orbital period of 1.29 years.

Simulates Kepler-1636, a Sun-like G-type star of 1.01 solar masses, and Kepler-1636 b, a planet with 3.2 Earth radii, with an orbital period of 1.16 years.

Simulates Kepler-1637, a Sun-like G-type star of 1.02 solar masses, and Kepler-1637 b, a planet with 0.9 Earth radii, with an orbital period of 6.1 days.

Simulates Kepler-1638, a Sun-like G-type star of 0.97 solar masses, and Kepler-1638 b, a planet with 1.9 Earth radii, with an orbital period of 259 days.

Simulates Kepler-1639, a Sun-like F-type star of 1.12 solar masses, and Kepler-1639 b, a planet with 2.6 Earth radii, with an orbital period of 9.9 days.

Simulates Kepler-164, a Sun-like G-type star of 0.97 solar masses, and Kepler-164 b, a planet with 1.4 Earth radii, with an orbital period of 5.0 days, at 0.058 AU from its star.

Simulates Kepler-1640, a Sun-like F-type star of 1.27 solar masses, and Kepler-1640 b, a planet with 4.8 Earth radii, with an orbital period of 7.6 days.