
GQ Lup - System
Simulates GQ Lup, an orange K-type dwarf of 0.70 solar masses, and GQ Lup b, a 20.0-Jupiter-mass companion, at 100 AU from its star, and an equilibrium temperature near 2,650 K.
Scenarios
Confirmed exoplanet systems from the NASA Exoplanet Archive, built from published orbital elements. Browse from single-planet hosts to compact multi-planet systems such as TRAPPIST-1, and watch how real architectures hold together under Newtonian gravity.

Simulates GQ Lup, an orange K-type dwarf of 0.70 solar masses, and GQ Lup b, a 20.0-Jupiter-mass companion, at 100 AU from its star, and an equilibrium temperature near 2,650 K.

Simulates GSC 06214-00210, an orange K-type dwarf of 0.90 solar masses, and GSC 06214-00210 b, a 16.0-Jupiter-mass companion, at 320 AU from its star, and an equilibrium temperature near 2,300 K.

Simulates GU Psc, a cool M-dwarf of 0.33 solar masses, and GU Psc b, a 11.3-Jupiter-mass companion, at 2,000 AU from its star, and an equilibrium temperature near 1,050 K.

Simulates Gaia-1, a Sun-like G-type star of 0.95 solar masses, and Gaia-1 b, a 1.68-Jupiter-mass companion, with an orbital period of 3.1 days, at 0.040 AU from its star.

Simulates Gaia-2, a Sun-like G-type star of 1.00 solar masses, and Gaia-2 b, a 0.82-Jupiter-mass companion, with an orbital period of 3.7 days, at 0.047 AU from its star.

Simulates Gaia22dkvL, a Sun-like G-type star of 1.15 solar masses, and Gaia22dkvL b, a 0.59-Jupiter-mass companion, at 1.400 AU from its star.

Simulates Gl 378, a cool M-dwarf of 0.56 solar masses, and Gl 378 b, a 13.0-Earth-mass planet, with an orbital period of 3.8 days, at 0.039 AU from its star, and an equilibrium temperature near 830 K, on an eccentric.

Simulates Gl 410, an orange K-type dwarf of 0.55 solar masses, and Gl 410 b, a 8.4-Earth-mass planet, with an orbital period of 6.0 days, at 0.053 AU from its star.

Simulates Gl 49, a cool M-dwarf of 0.52 solar masses, and Gl 49 b, a 5.6-Earth-mass planet, with an orbital period of 13.9 days, at 0.090 AU from its star, on an eccentric orbit (e ≈ 0.36).

Simulates Gl 686, a cool M-dwarf of 0.43 solar masses, and Gl 686 b, a 6.6-Earth-mass planet, with an orbital period of 15.5 days, at 0.091 AU from its star.

Simulates Gl 725 A, a cool M-dwarf of 0.33 solar masses, and Gl 725 A b, a 2.8-Earth-mass planet, with an orbital period of 11.2 days, at 0.068 AU from its star.

Simulates Gliese 12, a cool M-dwarf of 0.26 solar masses, and Gliese 12 b, a 0.9-Earth-mass planet, with an orbital period of 12.8 days, on an eccentric orbit (e ≈ 0.24).

Simulates HAT-P-1, a Sun-like G-type star of 1.15 solar masses, and HAT-P-1 b, a 0.53-Jupiter-mass companion, with an orbital period of 4.5 days, at 0.056 AU from its star, and an equilibrium temperature near 1,322 K.

Simulates HAT-P-11 b, an eccentric warm Neptune with water vapor in its atmosphere. It is one of the smallest planets with a measured transmission spectrum.

Simulates HAT-P-12, an orange K-type dwarf of 0.73 solar masses, and HAT-P-12 b, a 0.21-Jupiter-mass companion, with an orbital period of 3.2 days, at 0.038 AU from its star, and an equilibrium temperature near 963 K.

Simulates HAT-P-13, a Sun-like G-type star of 1.32 solar masses, and HAT-P-13 b, a 0.85-Jupiter-mass companion, with an orbital period of 2.9 days.

Simulates HAT-P-14, a Sun-like F-type star of 2.65 solar masses, and HAT-P-14 b, a 3.44-Jupiter-mass companion, with an orbital period of 4.6 days, on an eccentric orbit (e ≈ 0.11).

Simulates HAT-P-15, a Sun-like G-type star of 1.00 solar masses, and HAT-P-15 b, a 1.94-Jupiter-mass companion, with an orbital period of 10.9 days, on an eccentric orbit (e ≈ 0.19).