Tidal heating
Definition: Conversion of mechanical energy into internal heat as changing tidal stresses deform a body and dissipate energy.
Why it matters and connects: It can maintain volcanism or subsurface oceans in moons too small to retain much primordial heat.
Boundary or common confusion: Tides require both forcing and dissipation; a perfectly circular, rigid, synchronous moon would generate little heat.
Orbital resonance
Definition: A repeated orbital configuration produced by a near ratio of small whole-number periods.
Why it matters and connects: Moon resonances can maintain eccentricity, focus gravitational forcing, and power long-lived tidal activity.
Boundary or common confusion: A period ratio near an integer is insufficient by itself; the resonant geometry must remain bounded.
\(P_2/P_1\approx p/q\)
Subsurface ocean
Definition: A persistent layer of liquid, usually water-rich, beneath an ice shell or crust.
Why it matters and connects: Magnetic induction, gravity, libration, geology, and plume chemistry can provide independent tests of an ocean.
Boundary or common confusion: Surface fractures or young terrain alone do not prove a global liquid layer.
Induced magnetic field
Definition: A secondary magnetic response produced when a changing external field drives electric currents in a conductor.
Why it matters and connects: At moons such as Europa, induction is evidence for a globally connected conductive layer consistent with salty liquid water.
Boundary or common confusion: Conductivity and depth are partly degenerate, and plasma effects must be modeled.
Ring particle
Definition: An individual ice, rock, or dust fragment orbiting within a planetary ring system.
Why it matters and connects: Collective collisions, resonances, and shepherding create gaps, waves, sharp edges, and changing structures.
Boundary or common confusion: Rings are not solid disks, and images usually do not resolve typical particles individually.
Roche limit
Definition: The approximate distance within which tides from a primary can prevent a self-gravitating fluid satellite from remaining intact.
Why it matters and connects: It helps explain why dense rings occupy regions where loose material may not accrete into a large moon.
Boundary or common confusion: The limit depends on density, material strength, shape, and orbit; rigid bodies can survive inside the fluid estimate.
\(d_R\approx2.44R_p(\rho_p/\rho_s)^{1/3}\)