
Kepler-1911 - System
Simulates Kepler-1911, a Sun-like G-type star of 0.95 solar masses, and Kepler-1911 b, a planet with 1.0 Earth radii, with an orbital period of 6.0 days.
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-1911, a Sun-like G-type star of 0.95 solar masses, and Kepler-1911 b, a planet with 1.0 Earth radii, with an orbital period of 6.0 days.

Simulates Kepler-1912, a Sun-like G-type star of 0.98 solar masses, and Kepler-1912 b, a planet with 1.4 Earth radii, with an orbital period of 6.1 days.

Simulates Kepler-1913, a Sun-like F-type star of 1.17 solar masses, and Kepler-1913 b, a planet with 1.5 Earth radii, with an orbital period of 14.2 days.

Simulates Kepler-1914, a Sun-like G-type star of 1.05 solar masses, and Kepler-1914 b, a planet with 2.9 Earth radii, with an orbital period of 30.8 days.

Simulates Kepler-1915, a Sun-like F-type star of 1.03 solar masses, and Kepler-1915 b, a planet with 3.2 Earth radii, with an orbital period of 13.8 days.

Simulates Kepler-1916, a Sun-like F-type star of 1.18 solar masses, and Kepler-1916 b, a planet with 2.6 Earth radii, with an orbital period of 31.3 days.

Simulates Kepler-1917, a Sun-like G-type star of 0.88 solar masses, and Kepler-1917 b, a planet with 1.9 Earth radii, with an orbital period of 12.9 days.

Simulates Kepler-1918, a Sun-like G-type star of 0.97 solar masses, and Kepler-1918 b, a planet with 2.3 Earth radii, with an orbital period of 47.1 days.

Simulates Kepler-1919, a Sun-like G-type star of 0.87 solar masses, and Kepler-1919 b, a planet with 2.6 Earth radii, with an orbital period of 37.9 days.

Simulates Kepler-1920, a Sun-like F-type star of 1.24 solar masses, and Kepler-1920 b, a planet with 3.0 Earth radii, with an orbital period of 30.3 days.

Simulates Kepler-1922, a Sun-like G-type star of 0.95 solar masses, and Kepler-1922 b, a planet with 2.3 Earth radii, with an orbital period of 13.2 days.

Simulates Kepler-1923, a Sun-like G-type star of 1.11 solar masses, and Kepler-1923 b, a planet with 2.0 Earth radii, with an orbital period of 52.6 days.

Simulates Kepler-1924, a Sun-like G-type star of 1.02 solar masses, and Kepler-1924 b, a planet with 2.7 Earth radii, with an orbital period of 15.3 days.

Simulates Kepler-1925, a Sun-like G-type star of 1.06 solar masses, and Kepler-1925 b, a planet with 3.0 Earth radii, with an orbital period of 46.7 days.

Simulates Kepler-1926, a Sun-like G-type star of 0.77 solar masses, and Kepler-1926 b, a planet with 2.3 Earth radii, with an orbital period of 42.9 days.

Simulates Kepler-1927, a Sun-like F-type star of 1.41 solar masses, and Kepler-1927 b, a planet with 3.4 Earth radii, with an orbital period of 73.8 days.

Simulates Kepler-1928, a Sun-like G-type star of 1.01 solar masses, and Kepler-1928 b, a planet with 2.0 Earth radii, with an orbital period of 19.6 days, at 0.194 AU from its star, on an eccentric orbit (e ≈ 0.43).

Simulates Kepler-1929, a Sun-like G-type star of 1.01 solar masses, and Kepler-1929 b, a planet with 3.1 Earth radii, with an orbital period of 59.4 days.