
2MASS J16262785-2625152 - System
Simulates 2MASS J16262785-2625152, a cool M-dwarf of 1.00 solar masses, and KOINTREAU-4 b, a 15.3-Jupiter-mass companion, at 182 AU from its star.
Exoplanets
Systems with a single confirmed planet. Most are hot Jupiters or super-Earths on short-period orbits; others are distant giants found by radial velocity. A clean two-body laboratory for Keplerian motion around a real star.

Simulates 2MASS J16262785-2625152, a cool M-dwarf of 1.00 solar masses, and KOINTREAU-4 b, a 15.3-Jupiter-mass companion, at 182 AU from its star.

Simulates 2MASS J19383260+4603591, and 2MASS J19383260+4603591 b, a 1.86-Jupiter-mass companion, with an orbital period of 1.11 years, on an eccentric orbit (e ≈ 0.33).

Simulates 2MASS J21252752-8138278, a cool M-dwarf of 0.64 solar masses, and 2MASS J21252752-8138278 b, a 12.0-Jupiter-mass companion, at 7,493 AU from its star, and an equilibrium temperature near 1,616 K.

Simulates 2MASS J22362452+4751425, an orange K-type dwarf of 0.60 solar masses, and 2MASS J22362452+4751425 b, a 12.5-Jupiter-mass companion, at 230 AU from its star.

Simulates 2MASS J22501512+2325342, a cool M-dwarf of 0.43 solar masses, and 2MASS J22501512+2325342 b, a 30.0-Jupiter-mass companion, at 518 AU from its star, and an equilibrium temperature near 1,600 K.

Simulates 4 UMa, an orange K-type dwarf of 1.23 solar masses, and 4 UMa b, a 7.90-Jupiter-mass companion, with an orbital period of 270 days, at 0.877 AU from its star, on an eccentric orbit (e ≈ 0.45).

Simulates 51 Eridani b, a young Jupiter analog imaged in a debris disk. Its methane-rich atmosphere looks more like Jupiter's than most imaged giants.

Simulates 51 Pegasi b, the first planet found around a Sun-like star. This 1995 hot Jupiter won Michel Mayor and Didier Queloz the 2019 Nobel Prize in Physics.

Simulates 6 Lyn, an orange K-type dwarf of 1.32 solar masses, and 6 Lyn b, a 1.88-Jupiter-mass companion, with an orbital period of 2.52 years, at 2.028 AU from its star.

Simulates 70 Virginis b, a massive eccentric giant announced in 1996. It was one of the first exoplanets and briefly a candidate for a habitable moon host.

Simulates 8 UMi, an orange K-type dwarf of 1.51 solar masses, and 8 UMi b, a 1.65-Jupiter-mass companion, with an orbital period of 93.3 days, at 0.462 AU from its star, on an eccentric orbit (e ≈ 0.06).

Simulates 81 Cet, a Sun-like G-type star of 1.23 solar masses, and 81 Cet b, a 3.31-Jupiter-mass companion, with an orbital period of 2.75 years, at 2.104 AU from its star.

Simulates 91 Aqr, an orange K-type dwarf of 1.40 solar masses, and 91 Aqr b, a 3.20-Jupiter-mass companion, with an orbital period of 181 days, at 0.700 AU from its star.

Simulates AB Aur, and AB Aur b, a 9.00-Jupiter-mass companion, at 93.9 AU from its star, on an eccentric orbit (e ≈ 0.40).

Simulates AB Pic, an orange K-type dwarf of 0.90 solar masses, and AB Pic b, a 13.5-Jupiter-mass companion, at 260 AU from its star.

Simulates AF Lep, a Sun-like F-type star of 1.22 solar masses, and AF Lep b, a 3.61-Jupiter-mass companion, with an orbital period of 24.4 years, at 8.996 AU from its star.

Simulates AT2021ueyL, a cool M-dwarf of 0.49 solar masses, and AT2021ueyL b, a 1.34-Jupiter-mass companion, with an orbital period of 11.4 years, at 4.010 AU from its star.

Simulates BD+03 2562, an orange K-type dwarf of 1.14 solar masses, and BD+03 2562 b, a 6.40-Jupiter-mass companion, with an orbital period of 1.32 years, at 1.300 AU from its star, on an eccentric orbit (e ≈ 0.20).