Linked from

The 34 pages that link to Planetary differentiation, each with the reason it gives.

• MeteoriteRelated: Meteorite compositions reveal whether their parent bodies melted and separated into layers.

• Planetary scienceRelated: It links interior composition to planetary history and magnetic properties.

• Tidal heatingRelated: Early tidal heating can melt interiors and promote the formation of distinct layers.

• Earth's mantleRelated: Early differentiation concentrated metal in the core and left silicate material in the mantle.

• Gravitational binding energyRelated: Gravitational energy released as dense material sinks can heat a young planet.

• CeresRelated: Ceres’s rocky interior and ice-rich outer layers point to partial differentiation.

• Earth's coreNarrower topic: Dense metal sank inward during this process to form Earth's core.

• Planetary geologyRelated: Layering explains how interior composition controls later tectonic and volcanic activity.

• HadeanRelated: Iron sank toward Earth’s center while lighter materials formed the mantle and early crust.

• MercuryRelated: Mercury’s core and silicate exterior provide evidence about this process in rocky planets.

• Lunar magma oceanNarrower topic: The magma ocean is a proposed early stage in the Moon’s separation into crust and mantle.

• Early EarthRelated: Differentiation built Earth’s metallic core and silicate mantle from its initially mixed materials.

• Terrestrial planetRelated: Differentiation helps produce the metallic cores and rocky mantles typical of these planets.

• Earth's outer coreRelated: Differentiation concentrated iron-rich metal at Earth's center, forming the core.

• High-pressure mineral physicsRelated: Mineral properties at extreme conditions help explain how planetary layers form and persist.

• Iron meteoriteNarrower topic: Iron-nickel metal sank during differentiation, concentrating in asteroid interiors.

• Earth's inner coreRelated: Dense iron sank inward, creating the metallic core from which the inner core later formed.

• OutgassingRelated: Differentiation redistributes volatile-bearing materials and helps set the sources available for later release.

• Planetary coreRelated: Dense metals sank toward planetary centers, forming cores during early differentiation.

• Carbon planetRelated: Differentiation would sort dense carbides and metals from any graphite- or diamond-rich mantle.

• FayaliteRelated: Fayalite’s iron content helps track silicate–metal partitioning in planetary materials.

• Giant planetRelated: Differentiation helps produce the layered interiors inferred for giant planets.

• Goldschmidt classificationRelated: Differentiation sorts elements according to their affinities for coexisting phases.

• 2 PallasCompared with: Pallas appears less thoroughly differentiated than Vesta despite its substantial size.

• Chthonian planetRelated: A differentiated interior affects the density and composition expected for an exposed core.

• Geological history of EarthRelated: It produced Earth’s core, mantle, and crust from an initially mixed body.

• Meteoric ironRelated: Iron meteorites often come from metallic cores of differentiated asteroids.

• TroiliteRelated: Troilite abundance and distribution can inform models of sulfur and iron partitioning in planetary bodies.

• Composition of astronomical objectsRelated: Bulk chemistry helps reconstruct how a body separated into core, mantle, and crust.

• Geological history of MarsRelated: Differentiation established Mars’s internal layers and shaped its early thermal evolution.

• Geology of MercuryRelated: Mercury’s unusually large metallic core is a major outcome its geological history must explain.

• Geology of VenusRelated: Venus’s core, mantle, and crust reflect the planet’s early internal separation.

• Iron planetRelated: Differentiation concentrates dense iron at the center, helping produce an iron-dominated interior.

• Magnesium sulfideRelated: Sulfur-bearing phases such as MgS inform models of chemical separation inside planets.