BSSE General Science 1430 study materials
BSSE General Science 1430 study resources

BSSE General Science 1430 cheat sheet

BSSE General Science 1430 · Keep the key ideas within reach.

Quick reference

Scientific Inquiry, Measurement, and the Nature of Science

  • Scientific method: observation, question, hypothesis, experiment, data analysis, conclusion, communication; hypotheses must be testable and falsifiable.

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

  • Accuracy is closeness to true value; precision is closeness of repeated measurements to each other; random errors affect precision, systematic errors affect accuracy.

  • SI base units: length meter (m), mass kilogram (kg), time second (s), temperature kelvin (K), amount mole (mol), electric current ampere (A), luminous intensity candela (cd).

  • Metric prefixes: kilo (10^3), centi (10^-2), milli (10^-3), micro (10^-6), nano (10^-9); convert by moving decimal or multiplying by power of ten.

  • Significant figures: all nonzero digits count; zeros between nonzero digits count; leading zeros do not count; trailing zeros after a decimal point count; multiplication/division result keeps least number of sig figs, addition/subtraction keeps least decimal places.

  • Density = mass/volume; percent error = |experimental - accepted| / accepted × 100%; scientific notation expresses numbers as a × 10^n where 1 ≤ a < 10.

  • A scientific theory is a well-tested explanation supported by evidence; a law describes a consistent relationship; both are subject to revision with new evidence.

  • Correlation does not imply causation; controlled experiments with randomization and blinding reduce bias; peer review and replication strengthen claims.

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Matter, Atomic Structure, and Chemical Reactions

  • Matter is anything with mass and volume; pure substances (elements, compounds) have fixed composition; mixtures (homogeneous, heterogeneous) do not.

  • Atomic number Z = protons; mass number A = protons + neutrons; isotopes have same Z but different A; ions form by gaining or losing electrons.

  • Electron configuration follows Aufbau principle, Pauli exclusion principle, and Hund's rule; valence electrons determine chemical properties and group number for main-group elements.

  • Periodic trends: atomic radius decreases left to right and increases top to bottom; ionization energy and electronegativity increase left to right and decrease top to bottom.

  • Chemical reactions conserve mass and atoms; balance equations by adjusting coefficients, never subscripts; types include synthesis, decomposition, single replacement, double replacement, combustion.

  • Mole concept: 1 mol = 6.022 × 10^23 particles; molar mass in g/mol; moles = mass/molar mass; stoichiometry uses mole ratios from balanced equations.

  • Acids donate H+ (proton) and bases accept H+; pH = -log[H+]; pH < 7 acidic, pH = 7 neutral, pH > 7 basic; strong acids/bases dissociate completely.

  • Bonding: ionic bonds transfer electrons between metals and nonmetals; covalent bonds share electrons between nonmetals; metallic bonds involve delocalized electrons.

  • Conservation of energy in reactions: exothermic releases heat (ΔH < 0), endothermic absorbs heat (ΔH > 0); activation energy is the minimum energy for reaction.

Quick reference

Forces, Motion, Energy, and Waves

  • Newton's laws: (1) inertia-objects resist changes in motion; (2) F_net = ma; (3) every action has an equal and opposite reaction.

  • Kinematics: v = v0 + at; Δx = v0t + ½at²; v² = v0² + 2aΔx; average speed = distance/time; velocity includes direction.

  • Weight = mg (g ≈ 9.8 m/s² on Earth); friction opposes motion and depends on normal force and surfaces; net force determines acceleration.

  • Work = Fd cosθ; kinetic energy KE = ½mv²; gravitational potential energy PE = mgh; power = work/time; conservation of mechanical energy when only conservative forces act.

  • Momentum p = mv; impulse = FΔt = Δp; in isolated systems total momentum is conserved in collisions (elastic: KE conserved; inelastic: KE not conserved).

  • Wave properties: wavelength λ, frequency f, period T = 1/f, amplitude, speed v = fλ; transverse waves oscillate perpendicular to travel, longitudinal waves parallel.

  • Sound requires a medium; speed depends on medium (fastest in solids); pitch relates to frequency, loudness to amplitude; Doppler effect is frequency shift due to relative motion.

  • Light behaves as wave and particle; reflection angle equals incidence angle; refraction bends light when speed changes (Snell's law); electromagnetic spectrum ordered by wavelength/frequency.

Quick reference

Electricity, Magnetism, and Modern Physics

  • Electric charge is quantized (e = 1.6 × 10^-19 C); like charges repel, opposite attract; Coulomb's law F = kq1q2/r².

  • Ohm's law V = IR; electric power P = IV = I²R = V²/R; series circuits share current and sum resistance; parallel circuits share voltage and sum currents as 1/R_total = Σ1/R_i.

  • Electric current is flow of charge (I = Q/t); voltage is potential difference driving current; conductors allow charge flow, insulators resist it.

  • Magnetic fields arise from moving charges and permanent magnets; field lines run from north to south outside a magnet; like poles repel, opposite poles attract.

  • Electromagnetic induction: changing magnetic flux through a conductor induces voltage (Faraday's law); generators convert mechanical energy to electrical energy.

  • Wave-particle duality: light exhibits interference and diffraction (wave) and photoelectric effect (particle); photoelectric effect depends on frequency, not intensity.

  • Atomic spectra: emission lines occur when electrons drop to lower energy levels; absorption lines occur when electrons absorb specific photon energies.

  • Radioactive decay types: alpha (helium nucleus), beta (electron or positron), gamma (high-energy photon); half-life is time for half of a sample to decay.

  • Nuclear fission splits heavy nuclei releasing energy; fusion combines light nuclei; E = mc² relates mass defect to released energy.

Quick reference

Earth's Structure, Plate Tectonics, and Geological Processes

  • Earth's layers: crust (thin, rocky), mantle (silicate rock, convection), outer core (liquid iron-nickel, generates magnetic field), inner core (solid iron-nickel).

  • Plate tectonics: lithospheric plates move on asthenosphere; divergent boundaries create new crust (mid-ocean ridges, rift valleys); convergent boundaries cause subduction, mountains, volcanoes; transform boundaries cause earthquakes.

  • Rock types: igneous forms from cooling magma/lava; sedimentary forms from compaction and cementation of sediments; metamorphic forms from heat and pressure altering existing rock.

  • Rock cycle links igneous, sedimentary, and metamorphic rocks through melting, weathering, erosion, deposition, and metamorphism.

  • Earthquakes occur at faults where stress releases energy; focus is underground origin, epicenter is surface point above; seismographs record P waves (fast, longitudinal) and S waves (slower, transverse).

  • Volcanoes form at subduction zones, mid-ocean ridges, and hotspots; magma composition affects eruption style (high silica = explosive, low silica = fluid).

  • Weathering breaks rock (mechanical, chemical); erosion transports sediment; deposition lays it down; these processes shape landforms over time.

  • Relative dating uses superposition (older layers below), cross-cutting relationships, and index fossils; absolute dating uses radioactive isotopes such as carbon-14 and potassium-argon.

Quick reference

Weather, Climate, and the Atmosphere

  • Atmosphere layers: troposphere (weather, temperature decreases with altitude), stratosphere (ozone layer, temperature increases), mesosphere, thermosphere, exosphere.

  • Air pressure decreases with altitude; wind flows from high pressure to low pressure; Coriolis effect deflects moving air right in Northern Hemisphere and left in Southern Hemisphere.

  • Temperature, pressure, humidity, and wind determine weather; relative humidity is amount of water vapor relative to saturation; dew point is temperature at which air saturates.

  • Clouds form when rising moist air cools and water vapor condenses on condensation nuclei; types include cumulus, stratus, cirrus, and nimbus (precipitation).

  • Air masses classified by source region (continental/maritime, polar/tropical); fronts form where air masses meet: cold front (steep, short storms), warm front (gentle, long precipitation), stationary, occluded.

  • Greenhouse effect: atmospheric gases (CO2, H2O, CH4) absorb and re-emit infrared radiation, warming Earth's surface; enhanced greenhouse effect drives climate change.

  • Climate vs weather: climate is long-term average conditions; factors include latitude, altitude, ocean currents, proximity to water, and prevailing winds.

  • Severe weather: thunderstorms require instability and moisture; tornadoes form in severe thunderstorms; hurricanes form over warm ocean water and lose strength over land.

Quick reference

Astronomy and the Solar System

  • Solar system order from Sun: Mercury, Venus, Earth, Mars (terrestrial), Jupiter, Saturn, Uranus, Neptune (gas/ice giants); asteroid belt between Mars and Jupiter.

  • Kepler's laws: orbits are ellipses with Sun at one focus; planets sweep equal areas in equal times; orbital period squared is proportional to semi-major axis cubed (T² ∝ a³).

  • Gravity governs orbits; Newton's law of universal gravitation F = Gm1m2/r²; escape velocity depends on mass and radius of body.

  • Earth's rotation causes day/night; revolution and axial tilt (23.5°) cause seasons; Moon phases result from changing Sun-Earth-Moon angles; eclipses occur at new (solar) and full (lunar) moon when aligned.

  • Sun is a main-sequence star powered by nuclear fusion of hydrogen to helium; energy travels by radiation and convection; sunspots and solar flares are magnetic activity.

  • Stars are classified by spectral type OBAFGKM (hot to cool) and luminosity; Hertzsprung-Russell diagram plots luminosity vs temperature; main sequence stars fuse hydrogen.

  • Stellar evolution: nebula → protostar → main sequence → red giant/supergiant → white dwarf (low mass) or supernova/neutron star/black hole (high mass).

  • Galaxies: spiral, elliptical, irregular; Milky Way is a spiral galaxy; universe expansion evidenced by redshift and cosmic microwave background; Big Bang theory describes origin ~13.8 billion years ago.

  • Light-year is distance light travels in one year (~9.46 × 10^12 km); astronomical unit (AU) is average Earth-Sun distance (~1.5 × 10^8 km).

Quick reference

Cell Biology, Genetics, and Evolution

  • Cell theory: all living things made of cells; cells are basic unit of life; cells arise from existing cells. Prokaryotes lack nucleus; eukaryotes have membrane-bound organelles.

  • Organelles: nucleus (DNA control), ribosomes (protein synthesis), mitochondria (ATP production), chloroplasts (photosynthesis), endoplasmic reticulum (transport), Golgi apparatus (packaging), lysosomes (digestion), cell membrane (selective barrier).

  • Photosynthesis: 6CO2 + 6H2O + light → C6H12O6 + 6O2 in chloroplasts; cellular respiration: C6H12O6 + 6O2 → 6CO2 + 6H2O + ATP in mitochondria.

  • Cell division: mitosis produces identical diploid cells for growth and repair; meiosis produces haploid gametes with genetic variation through crossing over and independent assortment.

  • DNA structure: double helix with sugar-phosphate backbone and complementary base pairs A-T, C-G; DNA replicates semiconservatively; genes code for proteins via transcription and translation.

  • Mendelian genetics: dominant and recessive alleles; genotype vs phenotype; Punnett squares predict offspring ratios; law of segregation and law of independent assortment.

  • Mutations are changes in DNA sequence; can be harmful, beneficial, or neutral; sources include replication errors and mutagens; variation is raw material for evolution.

  • Evolution by natural selection: variation exists, more offspring produced than survive, individuals with advantageous traits reproduce more, traits become more common over generations.

  • Evidence for evolution: fossil record, comparative anatomy (homologous structures), embryology, molecular biology (DNA similarities), and observed adaptation.

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Human Anatomy, Physiology, and Health

  • Levels of organization: cells → tissues → organs → organ systems → organism; four tissue types: epithelial, connective, muscle, nervous.

  • Circulatory system: heart pumps blood through arteries, veins, capillaries; blood carries oxygen, nutrients, hormones, wastes; red blood cells contain hemoglobin for O2 transport.

  • Respiratory system: nose, trachea, bronchi, lungs, alveoli; gas exchange occurs in alveoli by diffusion; diaphragm contracts during inhalation.

  • Digestive system: mechanical and chemical breakdown; enzymes (amylase, protease, lipase) catalyze hydrolysis; nutrients absorbed in small intestine; water reabsorbed in large intestine.

  • Nervous system: neurons transmit electrical impulses; central nervous system (brain, spinal cord) and peripheral nervous system; reflex arcs bypass brain for quick response.

  • Endocrine system: glands secrete hormones into blood; insulin lowers blood glucose, glucagon raises it; negative feedback maintains homeostasis.

  • Immune system: innate defenses (skin, mucus, inflammation) and adaptive immunity (B cells produce antibodies, T cells destroy infected cells); vaccines stimulate immunity.

  • Skeletal and muscular systems: bones support and protect, muscles contract to move bones; antagonistic muscle pairs (biceps/triceps) produce movement.

  • Health: balanced diet, exercise, sleep, hygiene, and avoiding harmful substances support homeostasis; pathogens cause infectious disease; noninfectious diseases include genetic and lifestyle conditions.

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Ecology, Environment, and Natural Resources

  • Levels of ecology: organism, population, community, ecosystem, biome, biosphere; habitat is where an organism lives, niche is its role.

  • Energy flow: sunlight → producers (photosynthesis) → consumers (herbivores, carnivores, omnivores) → decomposers; only about 10% of energy transfers between trophic levels; food webs show interconnected chains.

  • Biogeochemical cycles: carbon (photosynthesis, respiration, combustion, decomposition), nitrogen (fixation, nitrification, denitrification), water (evaporation, condensation, precipitation, runoff), phosphorus (rock weathering, uptake, decomposition).

  • Population growth: exponential when resources unlimited; logistic when carrying capacity limits growth; limiting factors include food, water, space, disease, predation.

  • Symbiosis: mutualism (both benefit), commensalism (one benefits, other unaffected), parasitism (one benefits, other harmed); competition occurs when organisms need same resources.

  • Biodiversity includes genetic, species, and ecosystem diversity; threats include habitat loss, invasive species, pollution, overharvesting, climate change.

  • Natural resources: renewable (solar, wind, water, biomass) replenish naturally; nonrenewable (fossil fuels, minerals) are finite; conservation and efficiency reduce depletion.

  • Human impact: pollution, deforestation, greenhouse gas emissions, and urbanization alter ecosystems; sustainability meets present needs without compromising future generations.

  • Succession: primary succession starts on bare rock (lichens, mosses); secondary succession follows disturbance where soil remains; climax community is stable end stage.