Linked from

The 21 pages that link to Differential rotation, each with the reason it gives.

• Milky WayRelated: The Milky Way’s inner regions orbit faster than distant regions, continually reshaping its spiral pattern.

• Accretion diskRelated: Different orbital speeds at different radii shear disk material and help drive instabilities.

• JupiterRelated: Jupiter’s cloud-level atmosphere rotates differently by latitude, sustaining strong jet streams.

• Spiral galaxyRelated: A galaxy’s faster inner orbits would wind material into tight spirals without other mechanisms.

• Solar cycleRelated: The Sun’s latitude-dependent rotation stretches magnetic fields as a cycle begins.

• Galactic diskRelated: Stars and gas at different disk radii orbit the galactic center at different rates.

• Solar magnetic fieldRelated: The Sun’s latitude-dependent rotation stretches and shears magnetic fields.

• Solar dynamoRelated: The Sun’s latitude-dependent rotation shears magnetic fields, converting poloidal field into toroidal field.

• Density wave theoryNarrower topic: Different orbital speeds explain why material arms would wind up without a wave pattern.

• Stellar rotationBroader topic: Many stars rotate faster near the equator than near the poles.

• Gas giantRelated: Cloud bands can rotate at different rates, revealing complex atmospheric and interior flows.

• Spiral armRelated: A galaxy’s inner disk rotates faster than its outer disk, shaping how spiral patterns wind.

• Grand-design spiral galaxyRelated: A galaxy's faster inner rotation would wind up material arms without a mechanism that sustains their pattern.

• Stellar magnetic fieldRelated: Shearing between stellar layers can wind magnetic fields into stronger components.

• Tolman–Oppenheimer–Volkoff limitCompared with: Strong differential rotation can temporarily support merger remnants beyond the nonrotating limit.

• Flocculent spiral galaxyRelated: It shears gas clouds and young stellar structures into short, irregular arm segments.

• Orion ArmRelated: The Milky Way’s varying rotation rates affect the shape and winding of its arms.

• Pinwheel GalaxyRelated: The galaxy’s inner regions orbit faster than its outer disk, shaping its spiral pattern.

• Scutum–Centaurus ArmRelated: The Milky Way’s varying orbital speeds shape and wind its spiral pattern.

• Unbarred spiral galaxyRelated: It shapes disk structure and winds material around galactic centers.

• Von Zeipel theoremCompared with: It violates uniform rotation, a condition underlying the theorem.