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The 101 pages that link to Angular momentum, each with the reason it gives.

• Orbital mechanicsRelated: Its conservation explains why orbital speed increases near periapsis.

• Atmospheric circulationRelated: Air moving poleward or equatorward changes speed as it redistributes angular momentum.

• MomentumRelated: It is the rotational counterpart to linear momentum.

• Earth’s rotationRelated: Earth’s spin carries angular momentum that exchanges with the Moon and atmosphere.

• Orbital eccentricityRelated: In a two-body orbit, angular momentum helps determine the conic’s eccentricity.

• PulsarRelated: Conservation of angular momentum makes a collapsing stellar core spin faster as it shrinks.

• Steam turbineRelated: Steam produces torque by changing its angular momentum across rotor blades.

• Magnetic momentRelated: Intrinsic particle moments are linked to spin, while orbital motion also produces magnetic moments.

• Cross productRelated: For a particle, angular momentum is position crossed with momentum.

• Tidal lockingRelated: Tidal evolution redistributes angular momentum between spin and orbit rather than destroying it.

• Gravitational collapseRelated: Rotation can impede direct infall and redistribute collapsing matter into a disk.

• Giant-impact hypothesisRelated: Impact simulations must account for the Earth–Moon system’s unusually high angular momentum.

• Moment of inertiaRelated: It connects the axis-dependent inertia to the body's rotational motion.

• Ekman transportRelated: Earth's rotation provides the dynamical setting for Coriolis deflection.

• Three-body problemRelated: Its conservation provides another invariant that can reduce the equations' effective complexity.

• Axial precessionRelated: Earth's large spin angular momentum makes its axis respond gradually to torque.

• Coriolis forceRelated: It provides a broader framework for understanding motion in rotating systems.

• ProtostarRelated: Conservation of angular momentum helps make infalling protostellar gas form a disk.

• Solar System formationRelated: Conservation of angular momentum helped flatten the collapsing cloud into a disk.

• Galactic diskRelated: A galaxy’s retained angular momentum helps spread collapsing matter into a rotating disk.

• Planet formationRelated: Conservation of angular momentum helps explain why young stars are surrounded by disks.

• X-ray binaryRelated: Gas must shed angular momentum to spiral inward and accrete.

• Yarkovsky effectRelated: The direction of rotation helps determine whether thermal recoil raises or lowers orbital energy.

• Foucault pendulumRelated: Its conservation helps keep the pendulum’s swing direction nearly fixed in inertial space.

• Solar nebulaRelated: Conservation of angular momentum helped the collapsing cloud spin faster and flatten.

• TurbineRelated: Fluid angular-momentum change produces torque on the turbine rotor.

• Figure skating spinRelated: Pulling the limbs inward reduces rotational inertia and increases spin speed while angular momentum is conserved.

• Rigid body dynamicsRelated: Torque changes angular momentum, which need not point along angular velocity.

• Balance beamRelated: Flips and turns use angular momentum to control rotation in the air.

• FlywheelRelated: The flywheel’s angular momentum makes its rotation resist disturbances.

• Francis turbineRelated: Water’s change in angular momentum is the basis of torque on the runner.

• Golf swingRelated: Changing body and arm rotation helps transfer motion through the swing.

• OrbitRelated: Its conservation helps explain why orbital motion stays in a plane and sweeps equal areas.

• Rotational motionRelated: Its conservation explains why rotation can persist when external torque is absent.

• Tidal accelerationRelated: Tidal torques redistribute it between rotation and orbital motion.

• Nebular hypothesisRelated: Conservation of rotation helps explain why infalling cloud material formed a disk.

• Poynting–Robertson effectRelated: The drag removes orbital angular momentum, allowing the particle to move inward.

• Circular orbitRelated: In a central gravitational field, conserved angular momentum helps constrain orbital motion.

• Dust devilRelated: Converging air can spin faster as its distance from the rotation axis decreases.

• Larmor precessionRelated: Many magnetic moments are proportional to angular momentum, linking field torque to motion.

• Scattering theoryRelated: Its conserved channels organize scattering in rotationally symmetric systems.

• Axel jumpRelated: Skaters create and conserve rotation in the air by controlling body position and takeoff.

• PrecessionRelated: A spinning body's angular momentum sets the direction that torque changes during precession.

• True anomalyRelated: In a Keplerian orbit, conservation of angular momentum governs the rate of change of true anomaly.

• Central forceRelated: A central force exerts no torque about its center, so angular momentum remains constant.

• Discus throwRelated: The thrower manages rotational motion to accelerate the discus while maintaining balance.

• Gyromagnetic ratioRelated: It is the denominator that relates rotation to magnetic moment.

• Rotation groupRelated: Rotational invariance connects the group's symmetry to conserved angular momentum.

• Molecular physicsRelated: Electronic, vibrational, and rotational states are classified by angular momentum.

• Fire whirlRelated: Inward-moving air can spin faster as its distance from the vortex axis decreases.