
MOA-2015-BLG-337L - System
Simulates MOA-2015-BLG-337L, a Sun-like G-type star of 0.01 solar masses, and MOA-2015-BLG-337L b, a 0.11-Jupiter-mass companion, at 0.240 AU from its star.
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 MOA-2015-BLG-337L, a Sun-like G-type star of 0.01 solar masses, and MOA-2015-BLG-337L b, a 0.11-Jupiter-mass companion, at 0.240 AU from its star.

Simulates MOA-2016-BLG-227L, a Sun-like G-type star of 0.29 solar masses, and MOA-2016-BLG-227L b, a 2.80-Jupiter-mass companion, at 1.390 AU from its star.

Simulates MOA-2016-BLG-319L, a Sun-like G-type star of 0.15 solar masses, and MOA-2016-BLG-319L b, a 0.62-Jupiter-mass companion, at 0.950 AU from its star.

Simulates MOA-2016-BLG-526L, a Sun-like G-type star of 0.37 solar masses, and MOA-2016-BLG-526L b, a 14.9-Earth-mass planet, at 2.070 AU from its star.

Simulates MOA-2020-BLG-135L, a Sun-like G-type star of 0.23 solar masses, and MOA-2020-BLG-135L b, a 11.3-Earth-mass planet, at 1.110 AU from its star.

Simulates MOA-2020-BLG-208L, a Sun-like G-type star of 0.43 solar masses, and MOA-2020-BLG-208L b, a 0.14-Jupiter-mass companion, at 2.740 AU from its star.

Simulates MOA-2022-BLG-033L, a Sun-like F-type star of 0.51 solar masses, and MOA-2022-BLG-033L b, a 12.2-Earth-mass planet, at 2.150 AU from its star.

Simulates MOA-2022-BLG-091L, a Sun-like G-type star of 0.75 solar masses, and MOA-2022-BLG-091L b, a 3.59-Jupiter-mass companion, at 3.440 AU from its star.

Simulates MOA-2022-BLG-249L, a Sun-like G-type star of 0.18 solar masses, and MOA-2022-BLG-249L b, a 4.8-Earth-mass planet, at 1.630 AU from its star.

Simulates MOA-2022-BLG-563L, a Sun-like G-type star of 0.48 solar masses, and MOA-2022-BLG-563L b, a 0.40-Jupiter-mass companion, at 2.150 AU from its star.

Simulates MOA-bin-1L, a Sun-like G-type star of 0.75 solar masses, and MOA-bin-1L b, a 3.70-Jupiter-mass companion, at 8.300 AU from its star.

Simulates MOA-bin-29, a Sun-like G-type star of 0.03 solar masses, and MOA-bin-29 b, a 0.60-Jupiter-mass companion, at 0.480 AU from its star.

Simulates MWC 758, and MWC 758 c, a confirmed exoplanet, at 100 AU from its star, and an equilibrium temperature near 500 K.

Simulates MXB 1658-298, a Sun-like G-type star of 1.98 solar masses, and MXB 1658-298 b, a 23.7-Jupiter-mass companion, with an orbital period of 2.08 years, at 1.613 AU from its star.

Simulates NGC 2682 Sand 1429, a Sun-like F-type star of 1.26 solar masses, and NGC 2682 Sand 1429 b, a 1.80-Jupiter-mass companion, with an orbital period of 77.5 days, at 0.384 AU from its star, and an equilibrium.

Simulates NGTS-1, a cool M-dwarf of 0.62 solar masses, and NGTS-1 b, a 0.81-Jupiter-mass companion, with an orbital period of 2.6 days, at 0.033 AU from its star, and an equilibrium temperature near 790 K.

Simulates NGTS-10 b, an ultra-short-period hot Jupiter orbiting in about 18 hours. Tides are expected to drag this already-close planet inward. It was found by the Next-Generation Transit Survey.

Simulates NGTS-11, an orange K-type dwarf of 0.86 solar masses, and NGTS-11 b, a 0.34-Jupiter-mass companion, with an orbital period of 35.5 days, at 0.201 AU from its star, and an equilibrium temperature near 435 K.