OAE Earth and Space Science study materials
OAE Earth and Space Science study resources

OAE Earth and Space Science cheat sheet

OAE Earth and Space Science · Keep the key ideas within reach.

Quick reference

Nature of Science

  • Scientific inquiry cycle: observation → question → hypothesis → prediction → test → analysis → revision; hypotheses must be falsifiable and testable.

  • Independent variable is manipulated; dependent variable is measured; controlled variables are held constant to isolate cause and effect.

  • A theory is a well-tested explanatory framework supported by multiple lines of evidence (e.g., plate tectonics, evolution); a law describes a consistent relationship (e.g., Newton's law of gravitation). Neither is a guess.

  • Reliability increases with repeated trials and larger samples; validity means the design actually measures the intended quantity.

  • Correlation does not establish causation; a controlled experiment or a natural experiment with a plausible mechanism strengthens causal claims.

  • Earth and space science relies on indirect evidence: seismic waves, isotope ratios, spectra, and remote sensing because direct sampling is limited.

  • Deep time and large spatial scales require uniformitarianism plus catastrophism: present processes plus rare high-energy events explain the rock record.

  • Peer review, replication, and open data are the social mechanisms that filter error; scientific claims are provisional and revised with new evidence.

  • Measurement precision is limited by instrument resolution; report uncertainty and significant figures consistent with that precision.

Quick reference

Earth's Structure and Internal Processes

  • Earth's layers by composition: crust (oceanic ~5-10 km, continental ~30-70 km), mantle (to ~2900 km), core (iron-nickel, to ~6371 km).

  • By physical properties: lithosphere (rigid, crust plus uppermost mantle), asthenosphere (ductile, ~100-350 km), mesosphere, outer core (liquid, generates the geodynamo), inner core (solid).

  • P-wave velocity drops and S-waves disappear at the core-mantle boundary, proving the outer core is liquid; the Moho marks the crust-mantle boundary.

  • Isostasy: buoyant lithosphere floats on the asthenosphere; thicker or less dense crust rides higher, explaining mountain roots and post-glacial rebound.

  • Plate tectonics: divergent boundaries create new crust (mid-ocean ridges), convergent boundaries destroy or thicken crust (subduction, collision), transform boundaries slide past.

  • Seafloor magnetic striping symmetric about ridges records geomagnetic reversals and supports seafloor spreading; ages increase away from ridges.

  • Mantle convection and slab pull drive plates; ridge push and basal drag are secondary forces.

  • Earthquake focus depth and first-motion data locate faults; shallow quakes at ridges, deep quakes in subducting slabs.

  • Radioactive decay (U-238, K-40, Rb-87) supplies internal heat, driving convection and the geodynamo.

Quick reference

Earth's Surface Processes and Landforms

  • Weathering breaks rock in place (physical: frost wedging, exfoliation; chemical: hydrolysis, oxidation, dissolution); erosion transports the products.

  • Stream power depends on discharge and gradient; competence is the largest clast moved, capacity is the total load; deposition occurs when velocity falls.

  • V-shaped valleys form by fluvial incision; U-shaped valleys and moraines indicate glacial erosion and deposition.

  • Karst landscapes form where soluble limestone dissolves, producing caves, sinkholes, and disappearing streams.

  • Mass wasting is classified by material and motion (creep, slump, debris flow, rockfall) and triggered by water, slope steepening, or earthquakes.

  • Wind erodes by deflation and abrasion, producing ventifacts, yardangs, and dunes; dune type (barchan, transverse, longitudinal) reflects wind and sand supply.

  • Wave refraction concentrates energy on headlands and erodes them; longshore drift moves sediment along coasts, building spits and barrier islands.

  • Soils form from parent material, climate, organisms, topography, and time (CLORPT); horizons O, A, E, B, C, R develop with leaching.

  • Drainage patterns reflect bedrock: dendritic in uniform rock, trellis in folded strata, radial around domes, rectangular along joint sets.

Quick reference

Earth's Atmosphere, Weather, and Climate

  • Atmospheric composition: ~78% N2, ~21% O2, ~0.93% Ar, ~0.04% CO2; water vapor varies 0-4% and drives latent heat transfer.

  • Layers by temperature profile: troposphere (lapse rate ~6.5 °C/km), stratosphere (ozone heating), mesosphere, thermosphere, exosphere.

  • Pressure decreases exponentially with altitude; the Coriolis effect deflects moving air right in the Northern Hemisphere and left in the Southern, strongest at poles.

  • Cloud formation requires condensation nuclei, cooling to the dew point, and saturation; adiabatic cooling with ascent produces clouds and precipitation.

  • Mid-latitude cyclones form along the polar front with warm and cold fronts; cold fronts produce narrow, intense bands, warm fronts broad, gentle precipitation.

  • Thunderstorms require instability, moisture, and lift; tornadoes form in rotating supercells, and hurricanes need sea surface temperatures ≥26.5 °C and low wind shear.

  • Climate vs. weather: climate is long-term statistics; Milankovitch cycles, solar output, albedo, and greenhouse gases control climate over different timescales.

  • Greenhouse gases absorb and re-emit infrared radiation; CO2, CH4, N2O, and water vapor are the principal absorbers.

  • El Niño (warm eastern Pacific, weakened trade winds) and La Niña (cool eastern Pacific) shift global precipitation and storm tracks.

Quick reference

Earth's Hydrosphere and Cryosphere

  • Water distribution: ~97.5% saline ocean, ~2.5% freshwater; of freshwater, ~69% glaciers and ice caps, ~30% groundwater, <1% surface water.

  • The hydrologic cycle transfers water by evaporation, transpiration, condensation, precipitation, infiltration, runoff, and groundwater flow.

  • Porosity is the fraction of void space; permeability is the ability to transmit fluid; a confining layer (aquitard) restricts flow.

  • An aquifer is unconfined when bounded by a water table, confined when bounded by aquitards; artesian wells flow where the potentiometric surface exceeds land elevation.

  • Groundwater flows from high hydraulic head to low; Darcy's law: Q = K·A·(Δh/ΔL).

  • Ocean circulation includes wind-driven surface gyres and thermohaline deep circulation driven by temperature and salinity; upwelling brings nutrient-rich water to the surface.

  • Glaciers form where accumulation exceeds ablation; they flow by internal deformation and basal sliding, and retreat when mass balance is negative.

  • Sea level rises from thermal expansion, glacier and ice-sheet melt, and land subsidence; ice cores and tree rings provide paleoclimate proxies.

  • Watersheds (drainage basins) collect precipitation and route it to a common outlet; land use and impervious surfaces alter hydrographs.

Quick reference

Astronomy: Earth, Moon, Sun, and Solar System

  • Earth's rotation (23 h 56 m sidereal) causes day and night; revolution (365.25 days) and 23.5° axial tilt cause seasons.

  • Moon phases result from the changing angle between Earth, Moon, and Sun; a synodic month (29.5 days) exceeds the sidereal month (27.3 days).

  • Solar and lunar eclipses occur only near syzygy when the Moon's orbital plane (inclined ~5°) crosses the ecliptic at nodes.

  • Kepler's laws: elliptical orbits with the Sun at one focus; equal areas in equal times; P² ∝ a³ (P in years, a in AU).

  • Newton's law of gravitation: F = G·m1·m2/r²; it explains orbits, tides, and the barycenter of the Earth-Moon system.

  • Solar structure: core (fusion), radiative zone, convective zone, photosphere, chromosphere, corona; sunspots follow an ~11-year cycle.

  • Solar system formation from a rotating nebula: inner rocky planets, outer gas and ice giants, plus asteroid belt, Kuiper belt, and Oort cloud.

  • Tides result from differential gravitational pull; spring tides at new and full moon, neap tides at quarter moons.

  • Terrestrial planets have high density and thin or no atmospheres; Jovian planets have low density, thick hydrogen-helium atmospheres, and many moons.

Quick reference

Stars, Galaxies, and the Universe

  • Hertzsprung-Russell diagram plots luminosity vs. temperature; main sequence runs from hot, luminous O stars to cool, dim M stars.

  • Stellar fusion: proton-proton chain in Sun-like stars; CNO cycle in hotter stars; heavier elements form through fusion up to iron, then via supernovae.

  • Stellar evolution depends on mass: low-mass stars become white dwarfs, intermediate become neutron stars, high-mass become black holes.

  • Stellar parallax measures distance to nearby stars; standard candles (Cepheids, Type Ia supernovae) extend the distance ladder.

  • Spectral classification OBAFGKM by temperature; absorption lines indicate composition and ionization state.

  • Galaxies: spiral, elliptical, irregular; the Milky Way is a barred spiral with a supermassive black hole at its center.

  • Hubble's law: v = H0·d, with H0 ≈ 70 km/s/Mpc; recession velocity increases with distance, evidence for cosmic expansion.

  • Big Bang evidence: cosmic microwave background, primordial element abundances, and redshift of distant galaxies.

  • Dark matter and dark energy dominate the mass-energy budget; dark energy drives accelerating expansion.

Quick reference

Earth and Space Science Instruction and Assessment

  • Three-dimensional learning aligns disciplinary core ideas, science and engineering practices, and crosscutting concepts (e.g., patterns, cause and effect, systems).

  • Inquiry-based instruction uses phenomena to drive questions; students construct explanations from evidence rather than memorize facts.

  • Formative assessment informs instruction in real time (exit tickets, questioning, concept maps); summative assessment evaluates learning at the end of a unit.

  • Rubrics should describe observable performance levels aligned to learning objectives; inter-rater reliability improves with shared scoring practice.

  • Misconceptions (e.g., seasons caused by distance from the Sun, Moon phases caused by Earth's shadow) require targeted conceptual-change instruction.

  • Modeling (physical, conceptual, mathematical) and data analysis build representational competence; students should evaluate model limitations.

  • Safety and ethics: lab safety plans, appropriate handling of samples and equipment, and ethical use of data and sources.

  • Differentiation and universal design support diverse learners through multiple representations, scaffolded tasks, and accessible materials.

  • Assessment items should be aligned to standards, free of bias, and include distractor analysis to reveal misconceptions.