AST-228intermediate

Io, Europa, Ganymede & Callisto: Physical Mechanisms

The four Galilean moons form a natural experiment in how distance from Jupiter, composition, tidal heating, and orbital history produce very different worlds. The Galilean moons demonstrate tidal heating, ocean-world physics, orbital resonance, differentiation, and how habitability can exist far outside a star's classical surface-liquid-water zone when internal energy sources are available.

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Io, Europa, Ganymede & Callisto: Physical Mechanisms

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AST-227Io, Europa, Ganymede & Callisto: Structures & Vocabulary→

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AST-229Io, Europa, Ganymede & Callisto: Observation, Measurement & Evidence→

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The four Galilean moons form a natural experiment in how distance from Jupiter, composition, tidal heating, and orbital history produce very different worlds.

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The Laplace resonance links the orbital periods of Io, Europa, and Ganymede, maintaining small orbital eccentricities that allow Jupiter's gravity to flex their interiors repeatedly.

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