MODULE:KNOWLEDGE-BASE
SIMULATION: ACTIVE
RETURN::Planetary Science

Planetary Interiors

Differentiation, Cores & Tidal Heating

Half-Sphere Cross-Sections

Right half: surface as you'd see from orbit. Left half: cut-away interior. Hot layers (cores, oceans, metallic-H) pulse subtly. Body sizes are scaled relative to each other.

Differentiation

When a young world is hot enough to melt, denser materials sink to the centre and lighter ones float up — forming distinct core, mantle, and crust layers.

Iron and nickel concentrate in the core. Silicates (rock) dominate the mantle. The crust is what cooled and solidified first — often enriched in lighter elements like Si, Al, K.

Whether a planet keeps an active dynamo depends on the core staying partially liquid and convecting — Earth does, Mars used to but cooled out, Venus has a liquid core but no convection.

Heat Sources
PrimordialHeat from accretion + differentiation; slowly leaks out
Radioactive decayU, Th, K isotopes — primary heat source for rocky planets
Tidal flexingGravitational squeezing in eccentric orbits — Io, Europa
PressureCompression at depth maintains liquid metallic phases

Smaller bodies cool faster — surface area scales as r², heat content as r³.

ED: Geological Signals

In Elite Dangerous, the surface scanner highlights geological signal sources — fumaroles, ice geysers, and lava spouts. They form on bodies with active or recently-active interiors.

Tidally-heated moons around gas giants — analogues of Io and Europa — are prime candidates for biological signals (bacteria), while volcanic hot rocky bodies host raw-material harvest sites.

The Vista Genomics organic samples cluster on bodies with appropriate interior heat — too cold and there's nothing; too hot and the surface is hostile.

Interior Reference — Sol System
BodyRadiusCoreMantleCrustNote
Mercury2,440 km~83% (Fe-rich)Thin silicateThinAnomalously large iron core; partial dynamo
Venus6,052 km~50%Stagnant lidSingle plateHot mantle, no plate tectonics, no dynamo
Earth6,371 km~55% (Fe-Ni)ConvectingPlate tectonicsSolid inner + liquid outer core → strong dynamo
Mars3,389 km~50% (liquid)Thick silicateStagnant lidCooled core; lost dynamo; thin atmosphere stripped
Moon1,737 km~20% (small)Cold/rigidAnorthositeTiny core; differentiation from giant impact
Io1,822 km~20% (Fe-S)Partial meltActive volcanismTidal heating from Jupiter — most volcanic body
Europa1,561 km~20% (Fe)RockyIce + oceanSubsurface H₂O ocean; potential biosphere
Titan2,575 kmRocky/ice mixIce/waterIce + hydrocarbonsPossible internal ocean; hydrocarbon surface lakes
Jupiter69,911 km~10% (rock/ice)Metallic HH₂/He envelopeDiluted core; metallic-H mantle drives dynamo
Saturn58,232 km~10%Metallic HH₂/He envelopeLower density than water; banded ring system