
Wendelstein-2 - System
Simulates Wendelstein-2, an orange K-type dwarf of 0.73 solar masses, and Wendelstein-2 b, a 0.73-Jupiter-mass companion, with an orbital period of 1.8 days, at 0.023 AU from its star, and an equilibrium temperature.
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Simulates Wendelstein-2, an orange K-type dwarf of 0.73 solar masses, and Wendelstein-2 b, a 0.73-Jupiter-mass companion, with an orbital period of 1.8 days, at 0.023 AU from its star, and an equilibrium temperature.

Simulates Wolf 1061, a red dwarf 14 light-years away. Planet c orbits in the habitable zone of one of the nearest known planetary systems. Three planets orbit this nearby M dwarf.

Simulates Wolf 1069, a cool M-dwarf of 0.17 solar masses, and Wolf 1069 b, a 1.3-Earth-mass planet, with an orbital period of 15.6 days, at 0.067 AU from its star, and an equilibrium temperature near 250 K.

Simulates Wolf 327, a cool M-dwarf of 0.41 solar masses, and Wolf 327 b, a 2.5-Earth-mass planet, with an orbital period of 13.8 hours, at 0.010 AU from its star, and an equilibrium temperature near 996 K.

Simulates Wolf 503, an orange K-type dwarf of 0.69 solar masses, and Wolf 503 b, a 6.3-Earth-mass planet, with an orbital period of 6.0 days, at 0.057 AU from its star, and an equilibrium temperature near 790 K.

Simulates three equal masses whose paths cross at the center to draw an X inside a circle. Each body passes through the same central region at different times of the periodic cycle.

Simulates XEST 17-036, a cool M-dwarf of 0.26 solar masses, and KOINTREAU-1 b, a 10.6-Jupiter-mass companion, at 690 AU from its star.

Simulates XO-1, a Sun-like G-type star of 0.88 solar masses, and XO-1 b, a 0.83-Jupiter-mass companion, with an orbital period of 3.9 days.

Simulates XO-2 N, a Sun-like G-type star of 0.96 solar masses, and XO-2 N b, a 0.59-Jupiter-mass companion, with an orbital period of 2.6 days, at 0.037 AU from its star.

Simulates XO-2 S, a Sun-like G-type star of 0.98 solar masses, and XO-2 S b, a 0.26-Jupiter-mass companion, with an orbital period of 18.2 days, at 0.135 AU from its star, on an eccentric orbit (e ≈ 0.15).

Simulates XO-3 b, a massive hot Jupiter on a tilted, eccentric orbit. Its spin-orbit misalignment is evidence that the planet was scattered inward. The planet is roughly twelve times Jupiter's mass.

Simulates XO-4, a Sun-like F-type star of 1.10 solar masses, and XO-4 b, a 1.42-Jupiter-mass companion, with an orbital period of 4.1 days.

Simulates XO-5, a Sun-like G-type star of 1.04 solar masses, and XO-5 b, a 1.19-Jupiter-mass companion, with an orbital period of 4.2 days, at 0.051 AU from its star, and an equilibrium temperature near 1,230 K.

Simulates XO-6, a Sun-like F-type star of 1.47 solar masses, and XO-6 b, a 4.40-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.082 AU from its star, and an equilibrium temperature near 1,577 K.

Simulates XO-7, a Sun-like G-type star of 1.41 solar masses, and XO-7 b, a 0.71-Jupiter-mass companion, with an orbital period of 2.9 days, at 0.044 AU from its star, and an equilibrium temperature near 1,743 K.

Simulates YZ Cet, a cool M-dwarf of 0.14 solar masses, and YZ Cet b, a 0.7-Earth-mass planet, with an orbital period of 2.0 days, at 0.016 AU from its star, and an equilibrium temperature near 471 K, on an eccentric.

Simulates alf Ari, an orange K-type dwarf of 1.50 solar masses with 1 confirmed companion (alf Ari b) on NASA archive orbits.

Simulates alf Tau, an orange K-type dwarf of 1.13 solar masses with 1 confirmed companion (alf Tau b) on NASA archive orbits.