
Kepler-1635 - System
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.
Exoplanets
Systems with a single confirmed planet. Most are hot Jupiters or super-Earths on short-period orbits; others are distant giants found by radial velocity. A clean two-body laboratory for Keplerian motion around a real star.

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-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.

Simulates Kepler-1643, an orange K-type dwarf of 0.84 solar masses, and Kepler-1643 b, a planet with 2.3 Earth radii, with an orbital period of 5.3 days.

Simulates Kepler-1644, a Sun-like G-type star of 0.89 solar masses, and Kepler-1644 b, a planet with 1.9 Earth radii, with an orbital period of 21.1 days.

Simulates Kepler-1645, a Sun-like G-type star of 1.02 solar masses, and Kepler-1645 b, a planet with 1.8 Earth radii, with an orbital period of 16.2 days.

Simulates Kepler-1646, a cool M-dwarf of 0.24 solar masses, and Kepler-1646 b, a planet with 1.2 Earth radii, with an orbital period of 4.5 days.

Simulates Kepler-1647 b, a gas giant on the longest circumbinary orbit Kepler found. It circles two stars near their shared habitable zone. Its year around the stellar pair lasts about three years.

Simulates Kepler-1650, a cool M-dwarf of 0.33 solar masses, and Kepler-1650 b, a planet with 1.0 Earth radii, with an orbital period of 1.5 days.

Simulates Kepler-1651, an orange K-type dwarf of 0.52 solar masses, and Kepler-1651 b, a planet with 1.8 Earth radii, with an orbital period of 9.9 days, on an eccentric orbit (e ≈ 0.13).

Simulates Kepler-1652, a cool M-dwarf of 0.40 solar masses, and Kepler-1652 b, a planet with 1.6 Earth radii, with an orbital period of 38.1 days, at 0.165 AU from its star, and an equilibrium temperature near 268 K.

Simulates Kepler-1653, an orange K-type dwarf of 0.72 solar masses, and Kepler-1653 b, a planet with 2.2 Earth radii, with an orbital period of 140 days, at 0.471 AU from its star, and an equilibrium temperature near.

Simulates Kepler-1654, a Sun-like G-type star of 1.01 solar masses, and Kepler-1654 b, a 0.50-Jupiter-mass companion, with an orbital period of 2.87 years, at 2.026 AU from its star, and an equilibrium temperature near.

Simulates Kepler-1655, a Sun-like F-type star of 1.03 solar masses, and Kepler-1655 b, a 5.4-Earth-mass planet, with an orbital period of 11.9 days, at 0.103 AU from its star, and an equilibrium temperature near 938 K.

Simulates Kepler-1660 A, a Sun-like F-type star of 1.14 solar masses, and Kepler-1660 AB b, a 4.99-Jupiter-mass companion, with an orbital period of 240 days, on an eccentric orbit (e ≈ 0.06).