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For a spherical quasistatic Newtonian star, enclosed mass increases with shell volume and density, while the pressure gradient balances gravity due to enclosed mass.
ModelEarth & cosmosRadiative diffusion inside an opaque starIn an optically thick stellar region close to local thermodynamic equilibrium, radiative diffusion relates luminosity to the temperature gradient through density and an appropriate mean opacity.
ModelEarth & cosmosStellar energy conservation during evolutionA stellar shell's luminosity divergence accounts for local energy production, change in specific internal energy and compression or expansion work.
ModelEarth & cosmosStellar convection and the Schwarzschild criterionA displaced parcel that adjusts pressure rapidly but exchanges little heat can continue rising when it becomes less dense than its environment.
ModelEarth & cosmosHydrogen and helium fusion pathways in starsThe proton–proton chains and CNO cycles convert hydrogen into helium through different reaction sequences; CNO nuclei participate in a catalytic cycle.
ModelEarth & cosmosHertzsprung–Russell diagram and stellar interpretationAn HR diagram compares luminosity with effective temperature or a related spectral classification.
MethodEarth & cosmosBinary stars as stellar-mass measurementsA resolved relative orbit and period can constrain a binary's total mass through Newtonian two-body dynamics.
MethodEarth & cosmosGravitational cloud collapse and protostarsCold dense regions of molecular clouds can contract gravitationally when support is insufficient.
ModelEarth & cosmosPlanetary material classes and interior inferenceTerrestrial planets are dominated by rock and metal; giant planets contain larger proportions of light gases and volatile-rich material.
ModelEarth & cosmosComparative planetary atmospheres and energy balanceAtmospheric mass, composition and opacity affect a planet's surface conditions.
ModelEarth & cosmosAsteroid and comet material evidenceAsteroids include bodies with differing rocky, carbon-rich and metallic material signatures; meteorites and spacecraft observations test interpretations of their histories.
ModelEarth & cosmosGas phases of the interstellar mediumThe interstellar medium contains ionized, atomic and molecular gas alongside dust.
DefinitionEarth & cosmosGalactic components and stellar populationsThe Milky Way contains disk, bulge and halo components with differing distributions, motions and stellar populations.
ModelEarth & cosmosGalaxy morphology and physical populationsSpiral galaxies commonly contain a disk, bulge and spiral patterns with gas and ongoing star formation.
DefinitionEarth & cosmosGravitational lens geometry and image multiplicityA thin gravitational lens relates a source's unlensed angular position to observed image positions through a mass-dependent deflection.
ModelEarth & cosmosCosmological redshift and expansionIn an FLRW expansion model, light emitted and observed by comoving observers is stretched by the ratio of their scale factors.
ModelEarth & cosmosEarly-universe nuclei and photon decouplingThe hot expanding universe passed through changing particle and radiation conditions.
ModelEarth & cosmosCosmic structure growth and dark-matter modellingIn the standard cosmological model, small density variations grow gravitationally and dark-matter structures help concentrate baryonic matter after photon coupling becomes less effective.
ModelBiology · Chemistry · Earth & cosmosCalvin–Benson carbon fixation cycleThe Calvin–Benson cycle carboxylates ribulose-1,5-bisphosphate through RuBisCO, reduces the resulting carbon compounds using ATP and NADPH, and regenerates the acceptor.
ModelBiology · Earth & cosmos · ChemistryBiological nitrogen and phosphorus transformationsNitrogen fixation converts N₂ toward biologically usable reduced nitrogen; ammonification, nitrification and denitrification transform nitrogen among distinct chemical pools.
ModelEarth & cosmosGeological stress, strain and deformationStress describes force per area on a specified plane; strain describes deformation.
ModelEarth & cosmosFolds, faults and relative displacementFold geometry includes limbs, hinge/axis and axial surface; antiform/synform describe shape while anticline/syncline also depend on stratigraphic order.
DefinitionEarth & cosmosStrike, dip and geological map constraintsStrike is the bearing of a horizontal line in a plane; dip is the maximum inclination from horizontal, perpendicular to strike, with direction specified.
MethodEarth & cosmosRelative dating and unconformitiesSuperposition constrains age order in an undisturbed depositional sequence; inclusions predate their host, and cross-cutting features postdate what they cut.
MethodEarth & cosmos · BiologyFossils, correlation and palaeoenvironmentFossil assemblages can constrain relative age and depositional environment through observed succession and known ecological context.
MethodEarth & cosmosSedimentary facies and basin interpretationGrain size, sorting, sedimentary structures, composition and fossils together constrain depositional processes and environments.
ModelEarth & cosmosIsostasy and load responseIsostasy describes buoyancy-related balance of lithospheric columns over a deformable mantle in an appropriate model.
ModelEarth & cosmos · ChemistrySilicate structures and substitutionSilicate structures organize silicon–oxygen tetrahedra as isolated units, chains, sheets or frameworks.
DefinitionEarth & cosmosPartial melting and magma formationRock can begin melting without every component entering the liquid.
ModelEarth & cosmosCrystallization and igneous differentiationCrystallizing minerals remove selected chemical components from a melt.
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