
Kepler-48 - System
Simulates Kepler-48, an orange K-type dwarf of 0.88 solar masses, with its 5 planets on orbits from 4.8 days to 2.69 years.
Exoplanets
Five-planet systems sit near the edge of known multiplicity. Packed inner chains leave little dynamical room; small changes in mass or spacing can decide whether the system survives.

Simulates Kepler-48, an orange K-type dwarf of 0.88 solar masses, with its 5 planets on orbits from 4.8 days to 2.69 years.

Simulates Kepler-55, an orange K-type dwarf of 0.62 solar masses, with its 5 planets on orbits from 2.2 days to 42.2 days.

Simulates Kepler-62, a five-planet system with two worlds in the habitable zone. Kepler-62 f was an early favorite in the search for temperate rocky planets.

Simulates Kepler-80, a compact resonant chain of five planets. Neighboring orbits are so close that transit timing reveals their masses. Transit timing of the chain yields several of the masses.

Simulates Kepler-82, a Sun-like G-type star of 0.95 solar masses, with its 5 planets on orbits from 2.4 days to 75.7 days.

Simulates Kepler-84, a Sun-like F-type star of 1.06 solar masses, with its 5 planets on orbits from 4.2 days to 12.9 days.

Simulates L 98-59, a nearby compact system around a bright red dwarf. The inner planet may be volcanic, and outer worlds sit near the habitable zone. The host is bright enough for detailed JWST spectra.

Simulates TOI-5624, a Sun-like G-type star of 0.86 solar masses, with its 5 planets on orbits from 3.4 days to 45.4 days.