
HATS-36 - System
Simulates HATS-36, a Sun-like G-type star of 1.10 solar masses, and HATS-36 b, a planet with 12.9 Earth radii, with an orbital period of 4.2 days, at 0.052 AU from its star, and an equilibrium temperature near 1,203 K.
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 HATS-36, a Sun-like G-type star of 1.10 solar masses, and HATS-36 b, a planet with 12.9 Earth radii, with an orbital period of 4.2 days, at 0.052 AU from its star, and an equilibrium temperature near 1,203 K.

Simulates HATS-37 A, a Sun-like G-type star of 0.84 solar masses, and HATS-37 A b, a 0.10-Jupiter-mass companion, with an orbital period of 4.3 days, at 0.049 AU from its star, and an equilibrium temperature near 1,085 K.

Simulates HATS-38, a Sun-like G-type star of 0.89 solar masses, and HATS-38 b, a 0.07-Jupiter-mass companion, with an orbital period of 4.4 days, at 0.050 AU from its star, and an equilibrium temperature near 1,294 K.

Simulates HATS-39, a Sun-like F-type star of 1.38 solar masses, and HATS-39 b, a 0.63-Jupiter-mass companion, with an orbital period of 4.6 days, at 0.060 AU from its star, and an equilibrium temperature near 1,645 K.

Simulates HATS-4, a Sun-like G-type star of 1.00 solar masses, and HATS-4 b, a 1.32-Jupiter-mass companion, with an orbital period of 2.5 days, at 0.036 AU from its star, and an equilibrium temperature near 1,315 K.

Simulates HATS-40, a Sun-like F-type star of 1.56 solar masses, and HATS-40 b, a 1.59-Jupiter-mass companion, with an orbital period of 3.3 days, at 0.050 AU from its star, and an equilibrium temperature near 2,101 K.

Simulates HATS-41, a Sun-like F-type star of 1.50 solar masses, and HATS-41 b, a 9.70-Jupiter-mass companion, with an orbital period of 4.2 days, at 0.058 AU from its star, and an equilibrium temperature near 1,710 K.

Simulates HATS-42, a Sun-like F-type star of 1.27 solar masses, and HATS-42 b, a 1.88-Jupiter-mass companion, with an orbital period of 2.3 days, at 0.037 AU from its star, and an equilibrium temperature near 1,856 K.

Simulates HATS-43, an orange K-type dwarf of 0.84 solar masses, and HATS-43 b, a 0.26-Jupiter-mass companion, with an orbital period of 4.4 days, at 0.049 AU from its star, and an equilibrium temperature near 1,003 K.

Simulates HATS-44, an orange K-type dwarf of 0.86 solar masses, and HATS-44 b, a 0.56-Jupiter-mass companion, with an orbital period of 2.7 days, at 0.036 AU from its star, and an equilibrium temperature near 1,161 K.

Simulates HATS-45, a Sun-like F-type star of 1.27 solar masses, and HATS-45 b, a 0.70-Jupiter-mass companion, with an orbital period of 4.2 days, at 0.055 AU from its star, and an equilibrium temperature near 1,518 K.

Simulates HATS-46, a Sun-like G-type star of 0.92 solar masses, and HATS-46 b, a 0.17-Jupiter-mass companion, with an orbital period of 4.7 days, at 0.054 AU from its star, and an equilibrium temperature near 1,054 K.

Simulates HATS-47, an orange K-type dwarf of 0.67 solar masses, and HATS-47 b, a 0.37-Jupiter-mass companion, with an orbital period of 3.9 days, at 0.043 AU from its star, and an equilibrium temperature near 853 K.

Simulates HATS-48 A, an orange K-type dwarf of 0.73 solar masses, and HATS-48 A b, a 0.24-Jupiter-mass companion, with an orbital period of 3.1 days, at 0.038 AU from its star, and an equilibrium temperature near 955 K.

Simulates HATS-49, an orange K-type dwarf of 0.71 solar masses, and HATS-49 b, a 0.35-Jupiter-mass companion, with an orbital period of 4.1 days, at 0.045 AU from its star, and an equilibrium temperature near 835 K.

Simulates HATS-5, a Sun-like G-type star of 0.94 solar masses, and HATS-5 b, a 0.24-Jupiter-mass companion, with an orbital period of 4.8 days, at 0.054 AU from its star, and an equilibrium temperature near 1,025 K.

Simulates HATS-50, a Sun-like G-type star of 1.17 solar masses, and HATS-50 b, a 0.39-Jupiter-mass companion, with an orbital period of 3.8 days, at 0.050 AU from its star, on an eccentric orbit (e ≈ 0.52).

Simulates HATS-51, a Sun-like G-type star of 1.19 solar masses, and HATS-51 b, a 0.77-Jupiter-mass companion, with an orbital period of 3.3 days, at 0.046 AU from its star, and an equilibrium temperature near 1,553 K.