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An inverse-square force models attraction between point masses.
ModelEarth & cosmosRock cycle and geological transformationRock materials can change through multiple geological pathways.
ModelEarth & cosmosPlate tectonicsMoving lithospheric plates organize many large-scale geological processes.
ModelEarth & cosmosEarth's water cycleWater moves among reservoirs above, on and below Earth's surface.
ModelEarth & cosmos · Biology · ChemistryEarth's carbon cycleCarbon moves through biological, oceanic, atmospheric and geological reservoirs.
ModelEarth & cosmosPlanetary radiative energy balanceEarth's energy storage changes when incoming and outgoing energy differ.
ModelEarth & cosmosAtmospheric greenhouse effectInfrared absorption and emission affect how Earth loses heat to space.
ModelEarth & cosmosWeather, climate and their time scalesWeather describes short-term conditions; climate describes their longer-term patterns.
DefinitionEarth & cosmosOrbits as gravitational motionAn orbiting body can remain in continuous gravitational free fall.
ModelEarth & cosmosStellar fusion and evolutionMain-sequence stars release energy by fusing hydrogen into helium.
ModelEarth & cosmosHot Big Bang and the cosmic microwave backgroundExpansion and relic radiation support an earlier hot, dense Universe.
ModelPhysics · Earth & cosmosFriedmann cosmological evolutionHomogeneity and isotropy reduce gravitational expansion to two balances.
ModelPhysics · Earth & cosmosNuclear binding energyA bound nucleus has less rest mass than its separated nucleons.
ModelPhysics · Earth & cosmosExponential radioactive decayA fixed decay probability per time gives a population timescale.
ModelPhysics · Earth & cosmosFission, fusion and reaction energyNuclear rearrangement can release or require energy.
ModelEarth & cosmosMinerals, structure and diagnostic propertiesMineral identification combines structural and physical evidence.
MethodEarth & cosmosRadiometric ages and sample historyIsotopic measurements estimate an age only with a suitable geological model.
MethodEarth & cosmosSeismic constraints on Earth's interiorWave travel, refraction and transmission constrain an interior model.
MethodEarth & cosmosThe geodynamo modelFluid motion in the outer core maintains much of Earth's magnetic field.
ModelEarth & cosmosWater budgets and storage changeA defined area's water storage changes with total inflow and outflow.
ModelEarth & cosmosDarcy flux and hydraulic conductivityGroundwater flow is often approximately linear in hydraulic-head gradient.
ApproximationEarth & cosmosOcean circulation and overturningWind, buoyancy changes and mixing contribute to ocean transport.
ModelEarth & cosmosGlobal atmospheric circulationUnequal heating and rotation organize broad circulation patterns.
ModelEarth & cosmosClimate forcing and energy-budget perturbationsExternal changes can disturb climate's radiation budget.
DefinitionEarth & cosmosClimate feedback mechanismsClimate responses can amplify or damp a change.
ModelEarth & cosmosClimate detection and attribution methodsAttribution compares observed changes with plausible drivers and variability.
MethodEarth & cosmosStellar evolution and fuel stagesStellar structure changes as core fuel and conditions change.
ModelEarth & cosmosWhite dwarfs, neutron stars and stellar black holesDifferent evolutionary outcomes leave different compact remnants.
ModelEarth & cosmosAnnual stellar parallax and distanceChanging observing position permits geometric distance inference.
MethodEarth & cosmosCosmological redshift and distance inferenceSpectral stretching carries expansion information but is not one universal distance ruler.
Method