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RETURN::Planetary Science

Magnetospheres

Magnetic Fields, Solar Wind & Auroras

Magnetic Field vs Solar Wind

Solar wind streams in from the left. The bow shock decelerates it, the magnetopause deflects it, the magnetotail stretches downwind. Particles that leak through the polar cusps spiral down field lines and excite the auroral ovals.

The Dynamo

A planet generates a global magnetic field when its interior hosts a convecting electrically conductive fluid — Earth's liquid Fe-Ni outer core, Jupiter's metallic hydrogen mantle, or the icy ionic fluid in Uranus and Neptune.

The fluid's motion plus the planet's rotation stretches and twists existing field lines into a self-sustaining dipole. Stop the convection (Mars) or stop the rotation (Venus) and the dynamo dies.

What It Protects
AtmosphereDeflected solar wind cannot strip light gases — Mars lost its air after the dynamo died
Surface lifeCosmic rays + UV blocked — biosphere shielded
Ozone layerMagnetic + atmospheric protection chain together
EquipmentCharged particles harmlessly redirected to poles

Without a magnetosphere, atmospheric retention drops by 100–1000×.

Auroras

Solar-wind particles that breach the polar cusps spiral down magnetic field lines and slam into the upper atmosphere near the magnetic poles, exciting atmospheric atoms into glowing rings — the auroral ovals.

Colour comes from atomic species: O at high altitude → red, O at lower altitude → green, N₂ → pink/violet. The ED engine renders aurora-like effects on certain bodies in scenic systems.

Jupiter's auroras are 100× brighter than Earth's and continuously powered by Io's volcanic plume — not just the solar wind.

Magnetospheres in the Solar System
BodyStrengthSourceRetentionNote
Mercury1% of EarthLiquid Fe core (weak dynamo)Lost most volatilesCompressed magnetosphere — no atmosphere shield
VenusNegligibleInduced by solar wind onlyCO₂ retained by massNo internal dynamo — high atmospheric loss
Earth1.0× (reference)Liquid Fe outer coreStrong protectionAurora borealis/australis from cusp particles
MarsCrustal patches onlyLost dynamo ~4 Gyr agoAtmosphere strippedMagnetic anomalies in southern crust
Jupiter20,000× EarthLiquid metallic-H mantleMassive — extends past SaturnMost powerful in the system; deadly radiation
Saturn600× EarthMetallic H, smaller coreStrongAurora visible at radio + UV wavelengths
Uranus50× EarthIonic water mantle (offset)StrongMagnetic axis tilted 60° from rotation axis
Neptune30× EarthIonic water mantle (offset)StrongMagnetic axis offset from planet centre
Ganymede1% of EarthInternal dynamo (only moon!)Embedded inside Jupiter's magnetosphere