
HD 37605 - System
Simulates HD 37605, an orange K-type dwarf of 0.94 solar masses, and HD 37605 b, a 2.69-Jupiter-mass companion, with an orbital period of 55.0 days, at 0.277 AU from its star, on an eccentric orbit (e ≈ 0.67).
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 HD 37605, an orange K-type dwarf of 0.94 solar masses, and HD 37605 b, a 2.69-Jupiter-mass companion, with an orbital period of 55.0 days, at 0.277 AU from its star, on an eccentric orbit (e ≈ 0.67).

Simulates HD 3765, an orange K-type dwarf of 0.85 solar masses, and HD 3765 b, a 0.17-Jupiter-mass companion, with an orbital period of 3.32 years, at 2.108 AU from its star, on an eccentric orbit (e ≈ 0.30).

Simulates HD 38283, a Sun-like G-type star of 1.37 solar masses, and HD 38283 b, a 0.40-Jupiter-mass companion, with an orbital period of 363 days, at 1.020 AU from its star, on an eccentric orbit (e ≈ 0.41).

Simulates HD 38529, a Sun-like G-type star of 0.98 solar masses, and HD 38529 b, a 0.65-Jupiter-mass companion, with an orbital period of 14.3 days, at 0.115 AU from its star, on an eccentric orbit (e ≈ 0.26).

Simulates HD 38801, a Sun-like G-type star of 1.21 solar masses, and HD 38801 b, a 9.70-Jupiter-mass companion, with an orbital period of 1.88 years, at 1.623 AU from its star.

Simulates Pi Mensae, also HD 39091. An eccentric giant was already known; TESS then found an inner transiting super-Earth, its first planet. The super-Earth was TESS's first confirmed planet.

Simulates HD 39194, a Sun-like G-type star of 0.86 solar masses, and HD 39194 b, a 4.6-Earth-mass planet, with an orbital period of 5.6 days, at 0.059 AU from its star, on an eccentric orbit (e ≈ 0.10).

Simulates HD 39855, a Sun-like G-type star of 0.87 solar masses, and HD 39855 b, a 8.5-Earth-mass planet, with an orbital period of 3.2 days, at 0.041 AU from its star, on an eccentric orbit (e ≈ 0.14).

Simulates HD 40307, a nearby packed system of super-Earths. Several worlds orbit inside a few tenths of an AU around a quiet K dwarf. The star is a quiet K dwarf about 42 light-years away.

Simulates HD 40956, an orange K-type dwarf of 2.00 solar masses, and HD 40956 b, a 2.70-Jupiter-mass companion, with an orbital period of 1.58 years, at 1.400 AU from its star, on an eccentric orbit (e ≈ 0.24).

Simulates HD 40979, a Sun-like F-type star of 1.45 solar masses, and HD 40979 b, a 4.67-Jupiter-mass companion, with an orbital period of 264 days, at 0.850 AU from its star, on an eccentric orbit (e ≈ 0.25).

Simulates HD 4113, a Sun-like G-type star of 1.01 solar masses, and HD 4113 b, a 1.70-Jupiter-mass companion, with an orbital period of 1.44 years, at 1.280 AU from its star, on an eccentric orbit (e ≈ 0.90).

Simulates HD 42012, an orange K-type dwarf of 0.83 solar masses, and HD 42012 b, a 1.60-Jupiter-mass companion, with an orbital period of 2.35 years, at 1.670 AU from its star, on an eccentric orbit (e ≈ 0.20).

Simulates HD 4203, a Sun-like G-type star of 1.25 solar masses, and HD 4203 b, a 2.23-Jupiter-mass companion, with an orbital period of 1.18 years, at 1.170 AU from its star, on an eccentric orbit (e ≈ 0.52).

Simulates HD 4208, a Sun-like G-type star of 0.88 solar masses, and HD 4208 b, a 0.81-Jupiter-mass companion, with an orbital period of 2.28 years, at 1.662 AU from its star.

Simulates HD 42618, a Sun-like G-type star of 1.01 solar masses, and HD 42618 b, a 14.4-Earth-mass planet, with an orbital period of 150 days, at 0.554 AU from its star, and an equilibrium temperature near 337 K.

Simulates HD 4308, a Sun-like G-type star of 0.93 solar masses, and HD 4308 b, a 0.05-Jupiter-mass companion, with an orbital period of 15.6 days, at 0.120 AU from its star.

Simulates HD 4313, an orange K-type dwarf of 1.63 solar masses, and HD 4313 b, a 1.93-Jupiter-mass companion, with an orbital period of 356 days, at 1.157 AU from its star, on an eccentric orbit (e ≈ 0.15).