
TOI-2010 - System
Simulates TOI-2010, a Sun-like F-type star of 1.11 solar masses, and TOI-2010 b, a 1.29-Jupiter-mass companion, with an orbital period of 142 days, at 0.552 AU from its star, and an equilibrium temperature near 400 K.
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Simulates TOI-2010, a Sun-like F-type star of 1.11 solar masses, and TOI-2010 b, a 1.29-Jupiter-mass companion, with an orbital period of 142 days, at 0.552 AU from its star, and an equilibrium temperature near 400 K.

Simulates TOI-2015, a cool M-dwarf of 0.30 solar masses, and TOI-2015 b, a 9.2-Earth-mass planet, with an orbital period of 3.3 days, at 0.029 AU from its star, and an equilibrium temperature near 531 K, on an eccentric.

Simulates TOI-2019, a Sun-like G-type star of 1.18 solar masses, and TOI-2019 b, a 0.11-Jupiter-mass companion, with an orbital period of 15.3 days, at 0.128 AU from its star, and an equilibrium temperature near 917 K.

Simulates TOI-2025, a Sun-like G-type star of 1.20 solar masses, and TOI-2025 b, a 3.60-Jupiter-mass companion, with an orbital period of 8.9 days, at 0.089 AU from its star, and an equilibrium temperature near 1,166 K.

Simulates TOI-2031 A, a Sun-like F-type star of 1.17 solar masses, and TOI-2031 A b, a 0.80-Jupiter-mass companion, with an orbital period of 5.7 days, at 0.066 AU from its star, and an equilibrium temperature near.

Simulates TOI-206, a cool M-dwarf of 0.35 solar masses, and TOI-206 b, a planet with 1.3 Earth radii, with an orbital period of 17.7 hours, at 0.011 AU from its star, and an equilibrium temperature near 910 K.

Simulates TOI-2068, an orange K-type dwarf of 0.56 solar masses, and TOI-2068 b, a planet with 1.8 Earth radii, with an orbital period of 7.8 days, at 0.063 AU from its star, and an equilibrium temperature near 521 K.

Simulates TOI-2076, an orange K-type dwarf of 0.85 solar masses, and TOI-2076 e, a 4.7-Earth-mass planet, with an orbital period of 3.0 days, at 0.039 AU from its star, and an equilibrium temperature near 1,110 K.

Simulates TOI-2081, a cool M-dwarf of 0.54 solar masses, and TOI-2081 b, a planet with 2.0 Earth radii, with an orbital period of 10.5 days, at 0.075 AU from its star, and an equilibrium temperature near 488 K.

Simulates TOI-2084, a cool M-dwarf of 0.45 solar masses, and TOI-2084 b, a planet with 2.5 Earth radii, with an orbital period of 6.1 days, at 0.050 AU from its star, and an equilibrium temperature near 527 K.

Simulates TOI-2088, an orange K-type dwarf of 0.90 solar masses, and TOI-2088 b, a 0.12-Jupiter-mass companion, with an orbital period of 125 days, at 0.472 AU from its star, and an equilibrium temperature near 300 K.

Simulates TOI-2093, an orange K-type dwarf of 0.74 solar masses, and TOI-2093 b, a 10.6-Earth-mass planet, with an orbital period of 12.8 days, at 0.097 AU from its star, and an equilibrium temperature near 535 K.

Simulates TOI-2094, a cool M-dwarf of 0.42 solar masses, and TOI-2094 b, a planet with 1.9 Earth radii, with an orbital period of 18.8 days, at 0.136 AU from its star, and an equilibrium temperature near 276 K.

Simulates TOI-2095, a cool M-dwarf of 0.44 solar masses, and TOI-2095 b, a 4.1-Earth-mass planet, with an orbital period of 17.7 days, at 0.101 AU from its star, and an equilibrium temperature near 347 K.

Simulates TOI-2096, a cool M-dwarf of 0.23 solar masses, and TOI-2096 b, a planet with 1.2 Earth radii, with an orbital period of 3.1 days, at 0.025 AU from its star, and an equilibrium temperature near 445 K.

Simulates TOI-2107, a Sun-like G-type star of 0.96 solar masses, and TOI-2107 b, a 0.83-Jupiter-mass companion, with an orbital period of 2.5 days, at 0.035 AU from its star, and an equilibrium temperature near 1,397 K.

Simulates TOI-2109 b, one of the shortest-period giant planets known. An orbit of about 16 hours makes it an ultra-hot Jupiter near tidal breakup. The dayside is hot enough to vaporize most metals.

Simulates TOI-2120, a cool M-dwarf of 0.21 solar masses, and TOI-2120 b, a 6.8-Earth-mass planet, with an orbital period of 5.8 days, at 0.038 AU from its star, and an equilibrium temperature near 384 K, on an eccentric.