
TOI-5108 - System
Simulates TOI-5108, a Sun-like G-type star of 1.10 solar masses, and TOI-5108 b, a 0.10-Jupiter-mass companion, with an orbital period of 6.8 days, at 0.073 AU from its star, and an equilibrium temperature near 1,180 K.
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Simulates TOI-5108, a Sun-like G-type star of 1.10 solar masses, and TOI-5108 b, a 0.10-Jupiter-mass companion, with an orbital period of 6.8 days, at 0.073 AU from its star, and an equilibrium temperature near 1,180 K.

Simulates TOI-5110, a Sun-like F-type star of 1.47 solar masses, and TOI-5110 b, a 2.90-Jupiter-mass companion, with an orbital period of 30.2 days, at 0.216 AU from its star, and an equilibrium temperature near 976 K.

Simulates TOI-5126, a Sun-like F-type star of 1.24 solar masses, and TOI-5126 b, a planet with 4.7 Earth radii, with an orbital period of 5.5 days, at 0.065 AU from its star, and an equilibrium temperature near 1,442 K.

Simulates TOI-5143, an orange K-type dwarf of 0.86 solar masses, and TOI-5143 c, a planet with 16.3 Earth radii, with an orbital period of 5.2 days, at 0.056 AU from its star.

Simulates TOI-5153, a Sun-like F-type star of 1.24 solar masses, and TOI-5153 b, a 3.26-Jupiter-mass companion, with an orbital period of 20.3 days, at 0.158 AU from its star, and an equilibrium temperature near 906 K.

Simulates TOI-5181 A, a Sun-like F-type star of 1.25 solar masses, and TOI-5181 A b, a 1.04-Jupiter-mass companion, with an orbital period of 3.9 days, at 0.052 AU from its star, and an equilibrium temperature near.

Simulates TOI-519, a cool M-dwarf of 0.34 solar masses, and TOI-519 b, a 0.46-Jupiter-mass companion, with an orbital period of 1.3 days, at 0.016 AU from its star, and an equilibrium temperature near 687 K.

Simulates TOI-5205, a cool M-dwarf of 0.39 solar masses, and TOI-5205 b, a 1.08-Jupiter-mass companion, with an orbital period of 1.6 days, at 0.020 AU from its star, and an equilibrium temperature near 737 K.

Simulates TOI-521, a cool M-dwarf of 0.42 solar masses, and TOI-521 b, a 5.3-Earth-mass planet, with an orbital period of 1.5 days, at 0.019 AU from its star, and an equilibrium temperature near 794 K.

Simulates TOI-5210, a Sun-like G-type star of 1.10 solar masses, and TOI-5210 b, a 0.26-Jupiter-mass companion, with an orbital period of 4.6 days, at 0.056 AU from its star, and an equilibrium temperature near 1,286 K.

Simulates TOI-5218, an orange K-type dwarf of 0.74 solar masses, and TOI-5218 b, a 2.07-Jupiter-mass companion, with an orbital period of 4.3 days, at 0.047 AU from its star, and an equilibrium temperature near 783 K.

Simulates TOI-5232, a Sun-like F-type star of 1.39 solar masses, and TOI-5232 b, a 2.34-Jupiter-mass companion, with an orbital period of 4.1 days, at 0.056 AU from its star, and an equilibrium temperature near 1,772 K.

Simulates TOI-5261, a Sun-like G-type star of 1.04 solar masses, and TOI-5261 b, a 11.5-Jupiter-mass companion, with an orbital period of 4.2 days, at 0.051 AU from its star, and an equilibrium temperature near 1,244 K.

Simulates TOI-5292 A, a cool M-dwarf of 0.60 solar masses, and TOI-5292 A b, a 1.30-Jupiter-mass companion, with an orbital period of 2.0 days, at 0.028 AU from its star, and an equilibrium temperature near 809 K.

Simulates TOI-5293 A, a cool M-dwarf of 0.54 solar masses, and TOI-5293 A b, a 0.54-Jupiter-mass companion, with an orbital period of 2.9 days, at 0.034 AU from its star, and an equilibrium temperature near 675 K.

Simulates TOI-530, a cool M-dwarf of 0.53 solar masses, and TOI-530 b, a 0.40-Jupiter-mass companion, with an orbital period of 6.4 days, at 0.052 AU from its star, and an equilibrium temperature near 565 K.

Simulates TOI-5300, an orange K-type dwarf of 0.67 solar masses, and TOI-5300 b, a 0.60-Jupiter-mass companion, with an orbital period of 2.3 days, at 0.029 AU from its star, and an equilibrium temperature near 1,043 K.

Simulates TOI-5301, a Sun-like F-type star of 1.48 solar masses, and TOI-5301 b, a 3.72-Jupiter-mass companion, with an orbital period of 5.9 days, at 0.073 AU from its star, and an equilibrium temperature near 1,648 K.