Science

Physics, chemistry, biology, Earth science and astronomy — the formulas, constants, and “who discovered what” facts that come up again and again. Science tossups mix computation (plug into the formula fast, watch the units) with name recognition (the law, unit, or experiment named after someone). Kansas connections are flagged with (Kansas).

Motion & Kinematics

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Distance vs. displacement, speed vs. velocity

Speed is not velocity. A car going around a curve at a steady 60 mph has constant speed but changing velocity — so it is accelerating. Likewise, a ball at the top of its flight has zero velocity but still has acceleration g (downward). learn more

Constant-acceleration (“SUVAT”) equations

For constant acceleration a, initial velocity v₀, final velocity v, displacement d (or Δx), time t. Each equation leaves out one variable — pick the one missing the quantity you don't know and don't need. learn more

EquationMissing variableMore
v = v₀ + atdlearn more
d = v₀t + ½at²vlearn more
v² = v₀² + 2adtlearn more
d = ½(v₀ + v)talearn more

(Textbooks using the SUVAT letters write s = displacement, u = initial velocity, v = final velocity, a, t: v = u + at, s = ut + ½at², v² = u² + 2as, s = ½(u + v)t.)

Free fall

Near Earth's surface, ignoring air resistance, every object falls with the same acceleration g ≈ 9.8 m/s² (≈ 32 ft/s²; standard value 9.80665 m/s²) regardless of its mass — Galileo's insight. On the Moon g is about 1.6 m/s², roughly ⅙ of Earth's. learn more · standard gravity

Dropped from rest: v = gt and d = ½gt²
Example: a rock falls 3 s → v = 9.8 × 3 = 29.4 m/s; d = ½ × 9.8 × 3² = 44.1 m.
Thrown straight up at 19.6 m/s → reaches the top in t = v₀/g = 2 s, max height v₀²/2g = 19.6 m, lands after 4 s.

With air resistance, a falling object eventually stops accelerating at its terminal velocity (about 55 m/s ≈ 120 mph for a skydiver belly-down). Apollo 15 astronaut David Scott dropped a hammer and a feather on the airless Moon in 1971 — they landed together. terminal velocity · hammer & feather

Projectile motion

One-liners to do in your head: a car going from 0 to 30 m/s in 6 s has a = 5 m/s². A car at 20 m/s for 15 s goes 300 m. 60 mph = 88 ft/s ≈ 27 m/s; 1 m/s ≈ 2.24 mph. learn more

Forces & Newton's Laws

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Newton's three laws of motion

Published in the Philosophiæ Naturalis Principia Mathematica (“the Principia”), 1687. Force is measured in newtons: 1 N = 1 kg·m/s² (about the weight of a small apple). learn more · Principia

LawStatementExample / clueMore
1st — inertiaAn object stays at rest or in uniform straight-line motion unless acted on by a net external force.Passengers lurch forward when a bus brakes; tablecloth trick. Inertia depends on mass. Galileo stated an early form.learn more
2nd — F = maNet force equals mass × acceleration (more precisely, rate of change of momentum, F = Δp/Δt).10 N on a 2 kg cart → a = 5 m/s².learn more
3rd — action–reactionFor every action there is an equal and opposite reaction; forces come in pairs acting on different objects.Rocket pushes exhaust back, exhaust pushes rocket forward; recoil of a gun.learn more

Weight, normal force & friction

Mass vs. weight: mass (kg) is the amount of matter and is the same everywhere; weight (N, or pounds) is a force and changes with gravity. On the Moon your mass is unchanged but your weight is about ⅙. The pound is a unit of force; the kilogram is a unit of mass. (The rarely used English mass unit is the slug.) learn more

Momentum & impulse

Hooke's law (springs)

F = −kx: the restoring force of a spring is proportional to its stretch or compression x (k = spring constant, N/m; the minus sign means it opposes the displacement). Robert Hooke published it in 1678 as the Latin anagram “ceiiinosssttuv” = ut tensio, sic vis (“as the extension, so the force”). A mass on a spring has period T = 2π√(m/k); a simple pendulum T = 2π√(L/g) — independent of mass and (for small swings) amplitude. learn more · pendulum

Universal gravitation

F = G m₁m₂ / r² G = 6.674 × 10⁻¹¹ N·m²/kg²

Newton's law of universal gravitation is an inverse-square law: double the distance → ¼ the force; triple → ⅑. G was first measured by Henry Cavendish (1797–98) with a torsion balance — the experiment called “weighing the Earth.” Acceleration due to gravity at a planet's surface is g = GM/r². learn more · G

Big G (6.674 × 10⁻¹¹, the universal constant) is not little g (9.8 m/s², Earth's surface gravity). Astronauts on the ISS are not “weightless” because gravity is gone — gravity there is still about 90% of surface strength; they are in continuous free fall. learn more

Circular motion

An object moving in a circle at constant speed accelerates toward the center: centripetal acceleration ac = v²/r, requiring a centripetal force Fc = mv²/r (supplied by tension, friction, gravity…). “Centrifugal force” is the apparent outward push felt in a rotating frame — not a real force in an inertial frame. learn more · centrifugal

Torque & rotation

Torque is a twisting force: τ = rF sin θ (lever arm × force), unit N·m. That's why door handles are far from the hinges and long wrenches loosen tight bolts. Rotational analog of F = ma is τ = Iα (I = moment of inertia). Angular momentum L = Iω is conserved — a spinning figure skater pulls in her arms and spins faster. learn more · angular momentum

Pressure, density & fluids

“Eureka,” “crown,” “displaced water” → Archimedes / buoyancy. “Hydraulic press” → Pascal. “Airplane wing lift,” “fast fluid = low pressure” → Bernoulli. learn more

Work, Energy & Power

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Work

W = Fd cos θ, where θ is the angle between force and displacement. Unit: the joule (1 J = 1 N·m). No displacement → no work (pushing a wall, holding a heavy box still). A force perpendicular to motion does no work (θ = 90°, cos 90° = 0) — e.g. gravity on a satellite in circular orbit. learn more

Lifting a 10 kg box 2 m: W = mgh = 10 × 9.8 × 2 = 196 J. Work–energy theorem: net work = change in kinetic energy. learn more

Kinetic & potential energy

TypeFormulaNotesMore
Kinetic (motion)KE = ½mv²Double the speed → 4× the KE (why highway crashes are so much worse). 2 kg at 3 m/s → 9 J.learn more
Gravitational potentialPE = mghDepends on height above a chosen reference level.learn more
Elastic potentialPE = ½kx²Stored in a stretched/compressed spring (Hooke's law).learn more
Mass–energyE = mc²Einstein, 1905. 1 gram of mass ≈ 9 × 10¹³ J (about a 21-kiloton bomb). Explains the energy of fission, fusion, and the Sun.learn more

Conservation of energy & efficiency

Energy cannot be created or destroyed, only transformed (first law of thermodynamics). A pendulum or roller coaster trades PE for KE: a frictionless object dropped from height h reaches v = √(2gh) (from 5 m: v = √98 ≈ 9.9 m/s). learn more

Efficiency = useful energy (or work) out ÷ energy in × 100%. No real machine is 100% efficient — some energy always goes to heat via friction. Incandescent bulbs are only a few % efficient at making light; large electric motors exceed 90%. learn more

A “perpetual motion machine” is impossible — it would violate the first (or second) law of thermodynamics. learn more

Power

P = W/t (also P = Fv). Unit: the watt (1 W = 1 J/s), named for James Watt. 1 horsepower ≈ 746 W — a unit Watt himself coined to market steam engines. Climbing 5 m of stairs (60 kg) in 6 s: P = (60 × 9.8 × 5)/6 ≈ 490 W. learn more · horsepower

Energy units

UnitValueUsed forMore
joule (J)1 N·m = 1 kg·m²/s²SI unit of energy/work/heat (James Prescott Joule)learn more
calorie (cal)4.184 JHeat to raise 1 g of water by 1 °Clearn more
food Calorie (Cal, kcal)1000 cal = 4184 JNutrition labels (capital C)learn more
kilowatt-hour (kWh)3.6 × 10⁶ JElectric bills (power × time — an energy unit, not power)learn more
electronvolt (eV)1.602 × 10⁻¹⁹ JAtomic & particle physics (energy gained by one electron through 1 V)learn more
British thermal unit (BTU)≈ 1055 JHeat to raise 1 lb of water by 1 °F; furnaces & air conditionerslearn more
erg10⁻⁷ JOld CGS unit (dyne·cm)learn more

The kilowatt-hour measures energy; the kilowatt measures power (energy per time). A 100 W bulb left on for 10 hours uses 1 kWh. learn more

Simple machines & mechanical advantage

The six classical simple machines (Renaissance list): lever, wheel and axle, pulley, inclined plane, wedge, screw. (The wedge and screw are variations of the inclined plane.) Machines trade force for distance — they never multiply work. learn more

Lever classIn the middleExamplesMore
1st classFulcrumSeesaw, crowbar, scissors, plierslearn more
2nd classLoad (resistance)Wheelbarrow, nutcracker, bottle openerlearn more
3rd classEffortTweezers, broom, fishing rod, baseball bat, human forearm (biceps)learn more

Mnemonic “F-L-E, 1-2-3”: what's in the middle — Fulcrum, Load, Effort — gives the class. “Archimedes' screw” raises water; the screw is “an inclined plane wrapped around a cylinder.” Archimedes' screw

Waves, Sound & Light

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Wave basics

v = fλ (wave speed = frequency × wavelength) T = 1/f (period = 1 / frequency)

Sound

Doppler effect

The observed frequency rises when source and observer approach and falls when they separate — the falling pitch of a passing siren or train horn. Described by Austrian physicist Christian Doppler (1842). In light: approaching objects are blueshifted, receding ones redshifted — Hubble used galaxy redshifts to show the universe is expanding. Also used in radar guns and Doppler weather radar. learn more · redshift

Electromagnetic spectrum

All EM waves travel in vacuum at c = 299,792,458 m/s ≈ 3.00 × 10⁸ m/s (≈ 186,000 mi/s) — exact by definition since 1983. Listed from longest wavelength / lowest frequency / lowest energy to shortest/highest. Boundaries are approximate. learn more · speed of light

BandWavelength (approx.)Uses / factsMore
Radio> 1 m (up to km)AM/FM, TV; predicted by Maxwell, produced by Hertz (1887); Marconi's wirelesslearn more
Microwave1 mm – 1 mMicrowave ovens (2.45 GHz), radar, Wi-Fi, cell phones, cosmic microwave backgroundlearn more
Infrared~700 nm – 1 mmHeat radiation, remote controls, night vision, JWST; discovered by William Herschel (1800)learn more
Visible~400 – 700 nmROYGBIV — red ~700 nm to violet ~400 nmlearn more
Ultraviolet~10 – 400 nmSunburn, vitamin D, black lights, sterilization; blocked mostly by ozone; discovered by Johann Ritter (1801)learn more
X-ray~0.01 – 10 nmMedical imaging, crystallography; discovered by Wilhelm Röntgen (1895)learn more
Gamma ray< ~0.01 nmNuclear decay, cancer therapy, food irradiation; discovered by Paul Villard (1900)learn more

Order mnemonic (long → short): “Rabbits Mate In Very Unusual eXpensive Gardens” — Radio, Microwave, Infrared, Visible, Ultraviolet, X-ray, Gamma. learn more

Higher frequency = shorter wavelength = more energy per photon. Radio waves are light too (EM radiation), not sound. learn more

Visible light & color

Reflection, refraction & Snell's law

Lenses & mirrors

1/f = 1/do + 1/di m = −di/do = hi/ho (mirror: f = R/2)

Thin-lens / mirror equation. f = focal length, do = object distance, di = image distance (positive = real image, negative = virtual). Example: object 30 cm from a lens with f = 10 cm → 1/di = 1/10 − 1/30 = 2/30 → di = 15 cm, m = −0.5 (real, inverted, half size). Lens power in diopters = 1/f (in meters). learn more · curved mirrors

ConvergingDivergingMore
LensesConvex (thicker in middle) — magnifying glass, camera, eye, corrects farsightedness (hyperopia)Concave (thinner in middle) — corrects nearsightedness (myopia)learn more
MirrorsConcave — makeup/shaving mirror, flashlight reflector, reflecting telescopeConvex — car side mirror (“objects are closer than they appear”), store security mirrorlearn more

Convex lens converges, but convex mirror diverges — the shapes swap roles. Plane mirrors form virtual, upright, same-size, left-right reversed images. plane mirror

Light as particles: photons

E = hf = hc/λ, with Planck's constant h = 6.626 × 10⁻³⁴ J·s. Planck proposed energy quanta in 1900; Einstein applied them to light in 1905 (photoelectric effect). Light shows wave–particle duality. learn more · Planck constant · duality

Newton favored a corpuscular (particle) theory of light; Huygens a wave theory; Young's double slit (c. 1801) backed waves; Einstein's photons brought particles back. A laser (“light amplification by stimulated emission of radiation”) — first built by Theodore Maiman, 1960. corpuscular theory · laser

Electricity & Magnetism

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Charge & Coulomb's law

Circuits: Ohm's law & electric power

V = IR P = IV = I²R = V²/R Q = It
SeriesParallelMore
ResistorsR = R₁ + R₂ + …1/R = 1/R₁ + 1/R₂ + … (two resistors: R₁R₂/(R₁+R₂))learn more
CurrentSame through every componentSplits among branchesKirchhoff's laws
VoltageSplits among componentsSame across every branchlearn more
ExampleTwo 6 Ω in series = 12 Ω. Old holiday lights: one bulb out → all out.Two 6 Ω in parallel = 3 Ω. House wiring is parallel.learn more

Capacitors combine the opposite way from resistors: capacitors in parallel add directly; in series they add as reciprocals. Kirchhoff's laws: currents into a junction = currents out; voltages around a loop sum to zero. capacitors

Electrical & magnetic units

UnitMeasuresNamed forMore
volt (V)Potential difference / EMF (J/C)Alessandro Volta (Italy)learn more
ampere (A)Current (C/s) — SI base unitAndré-Marie Ampère (France)learn more
ohm (Ω)Resistance (V/A)Georg Ohm (Germany)learn more
coulomb (C)Charge (A·s)Charles-Augustin de Coulomb (France)learn more
farad (F)Capacitance (C/V)Michael Faraday (England)learn more
tesla (T)Magnetic field strength (flux density)Nikola Tesla (Serbian-American)learn more
henry (H)InductanceJoseph Henry (USA; first Secretary of the Smithsonian)learn more
weber (Wb)Magnetic flux (T·m²)Wilhelm Weber (Germany)learn more
siemens (S)Conductance (1/Ω; old name “mho”)Werner von Siemens (Germany)learn more
gauss (G)Magnetic field, CGS (1 T = 10,000 G)Carl Friedrich Gauss (Germany)learn more

Magnetism & electromagnetism

Transformers

Vs/Vp = Ns/Np (secondary/primary voltage = ratio of coil turns). A step-up transformer has more secondary turns (raises voltage, lowers current); step-down the reverse. Ideal transformer: VpIp = VsIs. Power lines use very high voltage to reduce I²R losses. Transformers work only with AC. Example: 120 V primary with 100 turns, 500 secondary turns → 600 V. learn more

AC vs. DC — the “War of the Currents”

Batteries were invented by Volta (voltaic pile, 1800), not Franklin or Galvani. Galvani's frog-leg experiments (1780s, “animal electricity”) inspired Volta — and gave us the word “galvanize.” voltaic pile · Galvani

Heat & Thermodynamics

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Temperature scales

°F = (9/5)°C + 32 °C = (5/9)(°F − 32) K = °C + 273.15
Reference point°F°CKMore
Absolute zero−459.67−273.150learn more
F and C are equal−40−40233.15learn more
Water freezes320273.15learn more
Room temperature (approx.)68–7220–22≈ 293–295learn more
Normal body temperature98.637310.15learn more
Water boils (1 atm)212100373.15learn more

Quick checks: 25 °C = 77 °F; 30 °C = 86 °F; 100 °F ≈ 37.8 °C; −40 is the same on both scales. Absolute zero can be approached but never reached. learn more

Heat, specific heat & latent heat

Q = mcΔT (temperature change) Q = mL (phase change, no temperature change)

Heat vs. temperature: temperature measures the average kinetic energy of particles; heat is energy transferred because of a temperature difference (in joules). A bathtub of warm water holds more thermal energy than a cup of boiling water, but has a lower temperature. learn more

Heat transfer

ModeHowExamplesMore
ConductionDirect contact; particle collisions (best in metals)Hot pan handle; cold tile floor feels colder than carpetlearn more
ConvectionBulk movement of a fluid (hot fluid rises)Boiling water, sea breezes, mantle convection, radiatorslearn more
RadiationElectromagnetic waves (mostly infrared); needs no mediumSunlight reaching Earth through space; campfire warmthlearn more

A thermos (Dewar flask, James Dewar, 1892) blocks all three: vacuum stops conduction and convection, silvered walls reflect radiation. Radiated power rises as T⁴ (Stefan–Boltzmann law). learn more · Stefan–Boltzmann

Laws of thermodynamics

LawStatementCluesMore
ZerothIf A and B are each in thermal equilibrium with C, they are in equilibrium with each other.Justifies thermometers; added and named last (by Ralph Fowler, 1930s) but more basic, hence “zeroth.”learn more
FirstEnergy is conserved: ΔU = Q − W (change in internal energy = heat added − work done by the system).No perpetual motion machines of the first kind; Joule, Mayer, Helmholtz.learn more
SecondThe total entropy of an isolated system never decreases; heat flows spontaneously from hot to cold; no heat engine is 100% efficient.Clausius and Kelvin statements; Carnot efficiency 1 − Tcold/Thot (kelvins); “arrow of time.”learn more · Carnot
ThirdAs temperature approaches absolute zero, entropy approaches a minimum (zero for a perfect crystal); absolute zero cannot be reached in a finite number of steps.Walther Nernst (Nernst heat theorem, 1906; Nobel 1920).learn more

Joke version: (1) You can't win. (2) You can't break even. (3) You can't get out of the game. Entropy (S, units J/K) measures disorder / the number of microstates; the word was coined by Rudolf Clausius (1865). Ludwig Boltzmann's S = k log W is engraved on his tombstone in Vienna. learn more

Atomic, Nuclear & Modern Physics

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Atomic models, in order

YearScientistModel / nicknameKey evidence or ideaMore
c. 400s BCDemocritus (& Leucippus)atomos (“uncuttable”)Philosophical idea that matter is made of indivisible particles.learn more
1803–1808John DaltonSolid sphere / “billiard ball”Atomic theory: elements are made of identical atoms that combine in whole-number ratios; law of multiple proportions.learn more
1897 / 1904J. J. ThomsonPlum puddingDiscovered the electron with cathode-ray tubes (1897); electrons embedded in a positive “pudding.”learn more
1909–1911Ernest RutherfordNuclear (planetary) modelGold foil experiment (done by Geiger & Marsden): a few alpha particles bounced back → tiny, dense, positive nucleus; atom mostly empty space.learn more
1913Niels BohrBohr modelElectrons in fixed energy levels (orbits); emit/absorb photons when jumping — explains hydrogen's spectral lines.learn more
1926 →Schrödinger, Heisenberg, et al.Quantum mechanical / electron cloudElectrons described by wave functions; orbitals (s, p, d, f) give probability, not paths.learn more
1932James Chadwick(adds the neutron)Discovered the neutral neutron in the nucleus.learn more

J. J. Thomson (electron, plum pudding, Nobel 1906 — showed the electron is a particle) is the father of G. P. Thomson (Nobel 1937 — electron diffraction showed the electron is a wave). Neither is spelled “Thompson.” Kelvin was William Thomson — no relation. G. P. Thomson

Quantum ideas

Radioactivity & decay

Discovered by Henri Becquerel (1896, uranium salts fogging photographic plates); the word “radioactivity” was coined by Marie Curie, who with Pierre discovered polonium and radium (1898). Rutherford named alpha and beta rays (1899); Paul Villard found gamma rays (1900). learn more

DecayParticleChange to nucleusStopped byMore
Alpha (α)Helium-4 nucleus (2p + 2n), charge +2Mass number −4, atomic number −2.
²³⁸U → ²³⁴Th + ⁴He
Sheet of paper / skin (least penetrating, most ionizing)learn more
Beta-minus (β⁻)Electron (+ antineutrino); a neutron becomes a protonMass number same, atomic number +1.
¹⁴C → ¹⁴N + e⁻
Thin aluminum, plasticlearn more
Beta-plus (β⁺)Positron (antielectron); a proton becomes a neutronAtomic number −1 (used in PET scans)Thin metallearn more
Gamma (γ)High-energy photonNo change in A or Z (nucleus drops to lower energy)Thick lead or concrete (most penetrating)learn more

Half-life

N = N₀ (½)t / t½ after n half-lives, (½)n remains: 1 → ½ → ¼ → ⅛ → 1/16 …

Example: 80 g of a substance with a 5-day half-life → after 15 days (3 half-lives) 10 g remain. Rutherford introduced the half-life concept (1907). learn more

IsotopeHalf-lifeUse / noteMore
Carbon-14≈ 5,730 yearsRadiocarbon dating of once-living things (up to ~50,000 yr); Willard Libby, Nobel 1960learn more
Uranium-238≈ 4.5 billion yearsAbout the age of the Earth; dating rockslearn more
Uranium-235≈ 704 million yearsFissile fuel for reactors and the Hiroshima bomblearn more
Potassium-40≈ 1.25 billion yearsPotassium–argon dating of volcanic rock; makes bananas slightly radioactivelearn more
Plutonium-239≈ 24,100 yearsNagasaki bomb, Trinity testlearn more
Iodine-131≈ 8 daysThyroid treatment; fallout (Chernobyl)learn more
Radon-222≈ 3.8 daysRadioactive gas seeping into basements (a lung-cancer risk in parts of Kansas)learn more
Cobalt-60≈ 5.3 yearsRadiation therapy, sterilizationlearn more

Fission vs. fusion

FissionFusion
WhatA heavy nucleus (U-235, Pu-239) splits when hit by a neutron, releasing more neutrons → chain reactionLight nuclei (hydrogen isotopes) join to form helium
WhereNuclear power plants, atomic (A-) bombsStars (the Sun), hydrogen (H-) bombs, experimental reactors (tokamaks, ITER)
HistoryDiscovered by Otto Hahn & Fritz Strassmann (Dec 1938); explained and named by Lise Meitner & Otto Frisch (1939). First self-sustaining reactor: Enrico Fermi's Chicago Pile-1, Dec 2, 1942.Hans Bethe explained stellar fusion (1939; Nobel 1967). First H-bomb: “Ivy Mike,” 1952. U.S. National Ignition Facility reached fusion ignition (more energy out than laser energy in) in Dec 2022.
Mass–energyIn both, products have slightly less mass than reactants; the “missing” mass becomes energy via E = mc².
Morelearn morelearn more

Critical mass, control rods (absorb neutrons — boron, cadmium), moderator (slows neutrons — water, graphite) → fission reactor. Major accidents: Three Mile Island (1979, PA), Chernobyl (1986, Ukrainian SSR), Fukushima (2011, Japan). learn more

The four fundamental forces

ForceRelative strengthRangeCarrier (boson)Does whatMore
Strong nuclear1 (strongest)~10⁻¹⁵ m (nucleus)GluonHolds quarks together in protons/neutrons; binds the nucleuslearn more
Electromagnetic~1/137InfinitePhotonElectricity, magnetism, light, chemistrylearn more
Weak nuclear~10⁻⁶~10⁻¹⁸ mW⁺, W⁻, Z⁰Beta decay; powers the Sun's first fusion steplearn more
Gravity~10⁻³⁸ (weakest)InfiniteGraviton (hypothetical)Planets, stars, galaxieslearn more

Electromagnetic and weak forces are unified as the electroweak force (Glashow, Salam, Weinberg; Nobel 1979). learn more

The Standard Model

Relativity

“Annus mirabilis,” “1905,” “Brownian motion,” “photoelectric,” “E = mc²” → Einstein. Einstein's Nobel (1921) was for the photoelectric effect. learn more

Units, Prefixes & Constants

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The seven SI base units

The International System of Units (SI, from French Système international, 1960). Since the 2019 redefinition, all seven are defined by fixed constants — the kilogram via Planck's constant, retiring the platinum–iridium cylinder “Le Grand K” kept near Paris. learn more · 2019 revision

QuantityUnitSymbolDefined byMore
TimesecondsCesium-133 atomic clock frequencylearn more
Lengthmeter (metre)mSpeed of light (distance light travels in 1/299,792,458 s)learn more
MasskilogramkgPlanck constant h (the only base unit with a prefix)learn more
Electric currentampereAElementary charge elearn more
TemperaturekelvinKBoltzmann constant klearn more
Amount of substancemolemolAvogadro constant NAlearn more
Luminous intensitycandelacdLuminous efficacy of 540 THz lightlearn more

Mnemonic for the 7 base units: “Some Mean Kids Always Kick My Cat” — second, meter, kilogram, ampere, kelvin, mole, candela. Everything else (newton, joule, watt, volt…) is a derived unit. Only three countries haven't fully adopted metric: the U.S., Liberia, and Myanmar. learn more · U.S. metrication

Metric prefixes

PrefixSymbolFactorExampleMore
tera-T10¹²terabytelearn more
giga-G10⁹gigawatt, gigahertzlearn more
mega-M10⁶megaton, megapixellearn more
kilo-k10³kilometer, kilogramlearn more
hecto-h10²hectare, hectopascallearn more
deca- (deka-)da10¹decameterlearn more
(base)—10⁰ = 1meter, gram, literlearn more
deci-d10⁻¹deciliterlearn more
centi-c10⁻²centimeterlearn more
milli-m10⁻³milliliter, millisecondlearn more
micro-μ (Greek mu)10⁻⁶micrometer (micron), microgramlearn more
nano-n10⁻⁹nanometer (light wavelengths), nanosecondlearn more
pico-p10⁻¹²picometer (atomic radii)learn more

Beyond: peta- (10¹⁵), exa- (10¹⁸), zetta-, yotta-, and (added 2022) ronna- (10²⁷) and quetta- (10³⁰); femto- (10⁻¹⁵), atto- (10⁻¹⁸), zepto-, yocto-, ronto- (10⁻²⁷), quecto- (10⁻³⁰). Mnemonic (kilo → milli): “King Henry Died By Drinking Chocolate Milk” (kilo, hecto, deca, base, deci, centi, milli). learn more

Capital M = mega (10⁶) but lowercase m = milli (10⁻³). 1 mL = 1 cm³ = 1 cc. 1 L of water has a mass of about 1 kg. learn more

Key physical constants

ConstantSymbolValueMore
Speed of light in vacuumc2.998 × 10⁸ m/s (exactly 299,792,458 m/s)learn more
Acceleration of gravity (Earth's surface)g9.8 m/s² = 32 ft/s²learn more
Universal gravitational constantG6.674 × 10⁻¹¹ N·m²/kg²learn more
Planck's constanth6.626 × 10⁻³⁴ J·slearn more
Boltzmann constantkB1.381 × 10⁻²³ J/Klearn more
Avogadro's numberNA6.022 × 10²³ per molelearn more
Elementary chargee1.602 × 10⁻¹⁹ Clearn more
Electron massme9.109 × 10⁻³¹ kglearn more
Proton massmp1.673 × 10⁻²⁷ kg (≈ 1836 me)learn more
Ideal gas constantR8.314 J/(mol·K) = 0.0821 L·atm/(mol·K)learn more
Coulomb constantk8.99 × 10⁹ N·m²/C²learn more
Standard atmosphereatm101.325 kPa = 760 mmHg = 14.7 psilearn more
Speed of sound (air, 20 °C)vs≈ 343 m/slearn more
Molar volume of ideal gas at STP (0 °C, 1 atm)Vm22.4 L/mollearn more
Astronomical unitAU≈ 1.496 × 10⁸ km ≈ 93 million mileslearn more
Light-yearly≈ 9.46 × 10¹² km ≈ 5.88 trillion mileslearn more

Units named after scientists

SI rule: the unit name is lowercase (newton), but the symbol is capitalized (N). learn more

UnitMeasuresPersonMore
newton (N)ForceIsaac Newtonlearn more
joule (J)Energy, work, heatJames Prescott Joulelearn more
watt (W)PowerJames Wattlearn more
pascal (Pa)PressureBlaise Pascallearn more
hertz (Hz)FrequencyHeinrich Hertzlearn more
kelvin (K)TemperatureWilliam Thomson, Lord Kelvinlearn more
volt, ampere, ohm, coulomb, farad, tesla, henry, weber, siemensElectrical (see table above)Volta, Ampère, Ohm, Coulomb, Faraday, Tesla, Henry, Weber, Siemenslearn more
becquerel (Bq)Radioactivity (1 decay/s)Henri Becquerellearn more
curie (Ci)Radioactivity, older unit (3.7 × 10¹⁰ decays/s ≈ 1 g of radium)Pierre & Marie Curielearn more
gray (Gy)Absorbed radiation dose (J/kg)Louis Harold Graylearn more
sievert (Sv)Biological dose equivalentRolf Sievertlearn more
ångström (Å)Length, 10⁻¹⁰ m (atomic scale)Anders Jonas Ångströmlearn more
degree Celsius / FahrenheitTemperatureAnders Celsius / Daniel Gabriel FahrenheitCelsius · Fahrenheit
torrPressure (1 mmHg)Evangelista Torricellilearn more
bel / decibel (dB)Sound level (log ratio)Alexander Graham Belllearn more
dalton (Da)Atomic mass unitJohn Daltonlearn more
röntgen (R)X/gamma exposure (old)Wilhelm Röntgenlearn more

Curie units: the curie (Ci) is a large, older unit of radioactivity; the SI unit is the becquerel (Bq, one decay per second), so 1 Ci = 3.7 × 10¹⁰ Bq. Don't confuse either with the Curie temperature (Pierre Curie — where a magnet loses its ferromagnetism) or the element curium (Cm, element 96). The roentgen, gray, and sievert measure dose, not activity. Curie temperature · curium

Atoms & the Periodic Table

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Atomic structure

ParticleChargeMassLocationDiscoveredMore
Proton (p⁺)+1≈ 1 u (1.007 u)NucleusRutherford, c. 1917–1919 (named 1920)learn more
Neutron (n⁰)0≈ 1 u (1.009 u, slightly heavier)NucleusJames Chadwick, 1932learn more
Electron (e⁻)−1≈ 1/1836 uOrbitals / electron cloudJ. J. Thomson, 1897learn more

Mass number (count of nucleons, always an integer) ≠ atomic mass (weighted average, usually a decimal). Changing protons changes the element; changing neutrons gives an isotope; changing electrons gives an ion. learn more

Organization of the periodic table

Dmitri Mendeleev (Russia, 1869) arranged elements by atomic mass and properties, leaving gaps and predicting undiscovered elements — eka-aluminium (gallium, 1875), eka-boron (scandium, 1879), eka-silicon (germanium, 1886). Today: 118 elements, 7 periods (rows) and 18 groups (columns). Elements in a group share valence electrons and similar chemistry. learn more · Mendeleev's predictions

GroupNameMembersCluesMore
1Alkali metalsLi, Na, K, Rb, Cs, Fr1 valence e⁻; soft, very reactive (explode in water), stored in oil; +1 ions. Hydrogen sits atop group 1 but is not an alkali metal.learn more
2Alkaline earth metalsBe, Mg, Ca, Sr, Ba, Ra2 valence e⁻; +2 ions; strontium gives red fireworks, barium green.learn more
3–12Transition metalsFe, Cu, Ag, Au, Zn, Ni, Hg, …d-block; colored compounds; multiple oxidation states; catalysts.learn more
13Boron groupB, Al, Ga, In, Tl, NhAluminum = most abundant metal in Earth's crust. Gallium melts in your hand (29.8 °C).learn more
14Carbon group (tetrels)C, Si, Ge, Sn, Pb, Fl4 valence e⁻; carbon (life), silicon (chips, sand).learn more
15Pnictogens (nitrogen group)N, P, As, Sb, Bi, McNitrogen is ~78% of air.learn more
16Chalcogens (oxygen group)O, S, Se, Te, Po, LvOxygen = most abundant element in Earth's crust (~46% by mass).learn more
17Halogens (“salt-formers”)F, Cl, Br, I, At, Ts7 valence e⁻; −1 ions; diatomic. Bromine is one of only two elements liquid at room temperature (with mercury).learn more
18Noble gases (inert gases)He, Ne, Ar, Kr, Xe, Rn, OgFull outer shell; very unreactive (Neil Bartlett made the first noble-gas compound, with xenon, 1962). Argon ≈ 0.93% of air. Most found by William Ramsay.learn more
f-blockLanthanides (57–71) & actinides (89–103)La…Lu; Ac…LrThe two rows below the table; lanthanides ≈ “rare earths” (neodymium magnets); actinides all radioactive (U, Pu). Glenn Seaborg proposed the actinide series (1944).lanthanides · actinides

Metals (left, ~¾ of elements: shiny, malleable, ductile, conductive) vs. nonmetals (upper right) separated by a staircase of metalloids (B, Si, Ge, As, Sb, Te — semiconductors). Most abundant element in the universe: hydrogen (then helium); in Earth's crust: oxygen (then silicon); in the human body by mass: oxygen; in air: nitrogen. metalloids · abundance

PropertyAcross a period (→)Down a group (↓)ExtremesMore
Atomic radiusDecreases (more protons pull e⁻ closer)Increases (more shells)Largest: cesium/francium; smallest: heliumlearn more
Ionization energyIncreasesDecreasesHighest: helium; low: cesiumlearn more
ElectronegativityIncreasesDecreasesHighest: fluorine (3.98 on Pauling scale); lowest: cesium/francium (~0.7–0.8)learn more
Metallic characterDecreasesIncreasesMost metallic: lower leftlearn more

Electronegativity, ionization energy and nonmetal reactivity all rise toward the upper right (fluorine corner; noble gases usually excluded from electronegativity). Atomic radius and metallic character rise toward the lower left. learn more

Symbols that don't match English names

SymbolElementZFromMore
NaSodium11Latin natrium (from natron)learn more
KPotassium19New Latin kalium (from Arabic qali, alkali)learn more
FeIron26Latin ferrumlearn more
CuCopper29Latin cuprum (from Cyprus)learn more
AgSilver47Latin argentum (Argentina is named for silver)learn more
SnTin50Latin stannumlearn more
SbAntimony51Latin stibiumlearn more
WTungsten74German Wolfram (not Latin); “tungsten” is Swedish for “heavy stone.” Highest melting point of any metal (3,422 °C).learn more
AuGold79Latin aurum (“shining dawn”)learn more
HgMercury80Greek-Latin hydrargyrum (“water-silver,” quicksilver)learn more
PbLead82Latin plumbum (source of “plumbing”)learn more

Chemical symbols of one or two letters were introduced by Jöns Jacob Berzelius (1810s). learn more

The first 20 elements

ZSymbolNameAtomic massQuiz clueMore
1HHydrogen1.008Lightest, most abundant in universe; Cavendish isolated it (1766, “inflammable air”); Lavoisier named it (“water-former”); Hindenburg 1937.learn more
2HeHelium4.003Found in the Sun's spectrum (1868, Janssen & Lockyer) before Earth (Ramsay, 1895); named for Greek helios; lowest boiling point.learn more
3LiLithium6.94Lightest metal; batteries; mood-stabilizing drug.learn more
4BeBeryllium9.012From the gem beryl (emerald); JWST mirrors; toxic dust.learn more
5BBoron10.81Borax, Pyrex (borosilicate glass); metalloid.learn more
6CCarbon12.011Basis of organic chemistry; allotropes diamond, graphite, fullerenes (buckyballs), graphene.learn more · allotropes
7NNitrogen14.007~78% of air; discovered by Daniel Rutherford (1772); Haber process → fertilizer.learn more
8OOxygen15.999Discovered by Scheele (c. 1771) and Priestley (1774); named by Lavoisier (“acid-former”); ozone is O₃.learn more
9FFluorine18.998Most electronegative and reactive element; isolated by Henri Moissan (1886; Nobel 1906); toothpaste fluoride.learn more
10NeNeon20.180Red-orange signs; Ramsay & Travers 1898 (Greek “new”).learn more
11NaSodium22.990Isolated by Humphry Davy via electrolysis (1807); table salt NaCl; yellow streetlights.learn more
12MgMagnesium24.305Burns with brilliant white light (flares); center of chlorophyll; Epsom salts.learn more
13AlAluminum26.982Most abundant metal in crust; once more precious than gold (Washington Monument cap, 1884); Hall–Héroult process (1886).learn more
14SiSilicon28.0852nd most abundant in crust; semiconductors; isolated by Berzelius (1823).learn more
15PPhosphorus30.974Discovered by Hennig Brand (1669) from urine — first element discovered by a known person; glows in the dark; matches; DNA backbone.learn more
16SSulfur32.06“Brimstone”; rotten-egg smell is H₂S; vulcanizes rubber; sulfuric acid.learn more
17ClChlorine35.45Scheele (1774); named by Davy (Greek “pale green”); WWI poison gas; pool disinfectant.learn more
18ArArgon39.95First noble gas isolated (Rayleigh & Ramsay, 1894); Greek “lazy”; ~0.93% of air; fills light bulbs.learn more
19KPotassium39.098First metal isolated by electrolysis (Davy, 1807); bananas; nerve impulses.learn more
20CaCalcium40.078Bones, teeth, limestone, chalk; most abundant metal in the human body; Davy (1808).learn more

Note argon (39.95) is heavier than potassium (39.10) even though it comes first — one of the “pair reversals” that convinced chemists to order by atomic number, not mass. Mnemonic for 1–20: “Happy Henry Likes Beer But Could Not Obtain Food. Next Nancy Might Also Sit Peacefully Sipping Claret Around Kansas Capitals.” atomic number order

Elements named after people & places

Named forElementsMore
ScientistsCurium (Cm, the Curies), einsteinium (Es), fermium (Fm), mendelevium (Md), nobelium (No), lawrencium (Lr, Ernest Lawrence — cyclotron), rutherfordium (Rf), seaborgium (Sg — named while Glenn Seaborg was alive), bohrium (Bh), meitnerium (Mt, Lise Meitner), roentgenium (Rg), copernicium (Cn), flerovium (Fl), oganesson (Og — Yuri Oganessian, also living when named), gadolinium (Gd, Johan Gadolin)learn more
PlacesAmericium, berkelium, californium, tennessine (Tennessee), livermorium (Livermore lab), dubnium (Dubna, Russia), moscovium, nihonium (Japan), darmstadtium, hassium (Hesse), germanium, gallium (Gaul/France), francium, polonium (Poland — Marie Curie's homeland), europium, scandium, ruthenium (Russia), copper (Cyprus), magnesium & manganese (Magnesia, Greece), strontium (Strontian, Scotland), lutetium (Paris), hafnium (Copenhagen), holmium (Stockholm), thulium (Thule), rhenium (Rhine)learn more
One Swedish villageYtterby gave four: yttrium, ytterbium, terbium, erbiumlearn more
Mythology & spaceHelium (Sun), selenium (Moon), tellurium (Earth), uranium, neptunium, plutonium (planets), cerium (Ceres), palladium (Pallas), titanium (Titans), thorium (Thor), promethium (Prometheus), niobium (Niobe), tantalum (Tantalus), vanadium (Vanadís/Freyja)learn more

States of matter & phase changes

Solid (fixed shape & volume), liquid (fixed volume), gas (neither), and plasma (ionized gas — stars, lightning, neon signs; the most common state of visible matter in the universe). A Bose–Einstein condensate (predicted 1924–25; first made by Eric Cornell & Carl Wieman, 1995) forms near absolute zero. learn more · BEC

ChangeFrom → toExampleMore
Melting (fusion)solid → liquidIce meltinglearn more
Freezing (solidification)liquid → solidWater to icelearn more
Vaporization (boiling, evaporation)liquid → gasPuddle dryinglearn more
Condensationgas → liquidDew, fog on a cold glasslearn more
Sublimationsolid → gasDry ice (solid CO₂), mothballs, freezer burnlearn more
Depositiongas → solidFrost, snowflakes forminglearn more
Ionization / recombinationgas ↔ plasmaLightninglearn more

A phase diagram shows the triple point (all three phases coexist; water: 0.01 °C) and the critical point (beyond which liquid and gas are indistinguishable — a supercritical fluid). Water's solid–liquid line slopes backward, so pressure can melt ice. learn more · triple point

Physical change (shape, state — no new substance) vs. chemical change (new substance: gas produced, color change, precipitate, light/heat, odor). Exothermic releases heat (combustion, freezing, condensing); endothermic absorbs it (melting, evaporating, cold packs, photosynthesis). learn more

Balancing Equations & Reaction Types

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Conservation of mass

In a chemical reaction, mass is neither created nor destroyed — the same atoms rearrange. Established by Antoine Lavoisier through careful weighing in sealed vessels (summarized in his Elementary Treatise of Chemistry, 1789); he is called the “father of modern chemistry.” A balanced equation has the same number of each kind of atom on both sides. learn more · Lavoisier

Step-by-step method

  1. Write correct formulas for every reactant and product (never change these afterward).
  2. Count atoms of each element on each side.
  3. Balance one element at a time by changing coefficients — start with the element in the most complex molecule; save H and O for near the end, and lone elements (like O₂ or Fe) for last.
  4. Treat unchanged polyatomic ions (SO₄²⁻, NO₃⁻) as single units.
  5. Recount; reduce coefficients to the smallest whole numbers. (If you get a fraction like 7/2 O₂, multiply everything by 2.)

learn more

Worked examples

UnbalancedBalancedCheckMore
H₂ + O₂ → H₂O2H₂ + O₂ → 2H₂OH: 4 = 4; O: 2 = 2. (Formation of water — synthesis.)learn more
CH₄ + O₂ → CO₂ + H₂OCH₄ + 2O₂ → CO₂ + 2H₂OC: 1 = 1; H: 4 = 4; O: 4 = 2 + 2. (Burning natural gas — combustion.)learn more
C₃H₈ + O₂ → CO₂ + H₂OC₃H₈ + 5O₂ → 3CO₂ + 4H₂OC: 3; H: 8; O: 10 = 6 + 4. (Propane grill.) Balance C first, then H, then O last.learn more
Fe + O₂ → Fe₂O₃4Fe + 3O₂ → 2Fe₂O₃Fe: 4 = 4; O: 6 = 6. (Rusting — synthesis/redox.)learn more
Al + HCl → AlCl₃ + H₂2Al + 6HCl → 2AlCl₃ + 3H₂Al: 2; H: 6 = 6; Cl: 6 = 6. (Single replacement.)learn more
N₂ + H₂ → NH₃N₂ + 3H₂ → 2NH₃N: 2; H: 6. (The Haber process — makes fertilizer.)learn more
C₆H₁₂O₆ + O₂ → CO₂ + H₂OC₆H₁₂O₆ + 6O₂ → 6CO₂ + 6H₂OC: 6; H: 12; O: 18 = 12 + 6. (Cellular respiration.)learn more

Coefficients vs. subscripts: balance only by changing the big numbers in front (coefficients). Changing a subscript changes the substance itself — H₂O is water, H₂O₂ is hydrogen peroxide. Coefficients multiply the whole formula: 3H₂O contains 6 H and 3 O. learn more

Reaction types

TypePatternExampleMore
Synthesis (combination)A + B → AB2Na + Cl₂ → 2NaCllearn more
DecompositionAB → A + B2H₂O₂ → 2H₂O + O₂; electrolysis of water; CaCO₃ → CaO + CO₂learn more
Single replacement (displacement)A + BC → AC + BZn + 2HCl → ZnCl₂ + H₂; a more active metal replaces a less active one (activity series)learn more
Double replacement (metathesis)AB + CD → AD + CBAgNO₃ + NaCl → AgCl↓ + NaNO₃ (forms a precipitate)learn more
CombustionFuel + O₂ → CO₂ + H₂O (for hydrocarbons)CH₄ + 2O₂ → CO₂ + 2H₂O; incomplete combustion makes COlearn more
Acid–base (neutralization)Acid + base → salt + waterHCl + NaOH → NaCl + H₂Olearn more
Redox (oxidation–reduction)Electrons transferRusting, batteries, combustion, photosynthesislearn more

OIL RIG: Oxidation Is Loss, Reduction Is Gain (of electrons). Or LEO the lion says GER: Lose Electrons = Oxidation, Gain Electrons = Reduction. The reducing agent is itself oxidized; the oxidizing agent is reduced. In a cell, oxidation happens at the anode, reduction at the cathode (“An Ox, Red Cat”). learn more · anode

Reaction rates increase with temperature, concentration, surface area, and catalysts (which lower activation energy and aren't consumed; enzymes are biological catalysts). Le Chatelier's principle: a system at equilibrium shifts to counteract a stress (added reactant, pressure, heat). rates · Le Chatelier

Moles, Stoichiometry & Gas Laws

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The mole

Stoichiometry

Use the balanced equation's coefficients as mole ratios: grams A → moles A → (ratio) → moles B → grams B. Example: in 2H₂ + O₂ → 2H₂O, 4 g H₂ (2 mol) makes 2 mol = 36 g of water. The limiting reactant runs out first and sets the amount of product; the other is in excess. Percent yield = actual ÷ theoretical × 100. learn more · limiting reagent

Concentration

Gas laws

Always use kelvins for temperature in gas laws. learn more

LawFormulaHeld constantRelationship / exampleMore
Boyle's (Robert Boyle, 1662)P₁V₁ = P₂V₂T, nPressure and volume inversely proportional. 6 L at 2 atm → 4 L at 3 atm. Syringes, bubbles growing as they rise.learn more
Charles's (Jacques Charles, c. 1787)V₁/T₁ = V₂/T₂P, nVolume directly proportional to temperature. 2 L at 300 K → 4 L at 600 K. Hot-air balloons; balloon shrinks in a freezer.learn more
Gay-Lussac's (also Amontons's law)P₁/T₁ = P₂/T₂V, nPressure directly proportional to temperature. Aerosol cans warn not to heat; tire pressure rises on hot days.learn more
Avogadro's (1811)V₁/n₁ = V₂/n₂P, TEqual volumes of gases at the same T and P contain equal numbers of molecules.learn more
CombinedP₁V₁/T₁ = P₂V₂/T₂nBoyle + Charles + Gay-Lussac together.learn more
Ideal gas law (Émile Clapeyron, 1834)PV = nRT—R = 0.0821 L·atm/(mol·K) = 8.314 J/(mol·K). 1 mol at 273 K and 1 atm → V = 22.4 L.learn more
Dalton's law of partial pressures (1801)Ptotal = P₁ + P₂ + …—Each gas in a mixture exerts pressure independently. Air at 1 atm: P(N₂) ≈ 0.78 atm, P(O₂) ≈ 0.21 atm.learn more
Graham's law (Thomas Graham, 1848)rate₁/rate₂ = √(M₂/M₁)—Lighter gases effuse/diffuse faster. H₂ (2 g/mol) escapes 4× faster than O₂ (32 g/mol) since √16 = 4.learn more

Charles vs. Boyle: Boyle = pressure–volume (inverse, “Boyle's PV”); Charles = volume–temperature (direct, “Charles is Cool with Temperature”); Gay-Lussac = pressure–temperature. Jacques Charles also flew the first hydrogen balloon (1783). Doubling Celsius temperature does not double volume — convert to kelvins. learn more

STP & the kinetic molecular theory

Acids, Bases, Solutions & Bonding

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The pH scale

pH = −log[H⁺] pOH = −log[OH⁻] pH + pOH = 14 (at 25 °C)

Scale runs roughly 0–14: below 7 acidic, 7 neutral, above 7 basic (alkaline). It's logarithmic — each step is a factor of 10, so pH 3 is 100× more acidic than pH 5. [H⁺] = 10⁻⁴ M → pH 4. Introduced by Danish chemist Søren Sørensen at the Carlsberg Laboratory (1909). learn more

Approx. pHSubstanceMore
0–1Battery acid (sulfuric acid)learn more
1.5–3.5Stomach acid (HCl)learn more
~2Lemon juice (citric acid)learn more
~2.5Cola (phosphoric & carbonic acid); vinegar ~2.5–3 (acetic acid)learn more
~5Black coffee; normal rain ~5.6 (acid rain is below that)learn more
7Pure water (neutral)learn more
7.35–7.45Human blood (slightly basic)learn more
~8.1Seawater (slowly acidifying from absorbed CO₂)learn more
~8.3Baking soda solution (NaHCO₃)learn more
~10.5Milk of magnesia (Mg(OH)₂)learn more
~11–12Household ammonia (NH₃)learn more
~12.5–13Bleach (sodium hypochlorite)learn more
~14Lye / drain cleaner (NaOH)learn more

Common acids & bases

FormulaNameWhere / clueMore
HClHydrochloric (muriatic) acidStomach acid; strong acidlearn more
H₂SO₄Sulfuric acid (oil of vitriol)Car batteries; most-produced industrial chemical; stronglearn more
HNO₃Nitric acidFertilizers, explosives; turns skin yellow; stronglearn more
CH₃COOHAcetic acidVinegar (~5%); weaklearn more
H₂CO₃Carbonic acidCarbonated drinks (CO₂ + H₂O); weaklearn more
H₃PO₄Phosphoric acidColas, rust removerslearn more
HCOOHFormic acidAnt stings (Latin formica = ant)learn more
C₆H₈O₇ / C₃H₆O₃Citric / lactic acidCitrus fruit / sour milk & muscle fatiguecitric · lactic
NaOH / KOHSodium / potassium hydroxide (lye, caustic soda/potash)Soap making, drain cleaner; strong baseslearn more
NH₃AmmoniaCleaners, fertilizer; weak baselearn more
Ca(OH)₂Calcium hydroxide (slaked lime)Mortar, soil treatmentlearn more

The common strong acids (ionize completely): HCl, HBr, HI, HNO₃, H₂SO₄, HClO₄ (perchloric). Strong bases: group 1 hydroxides plus Ca, Sr, Ba hydroxides. learn more

“Strong” ≠ “concentrated.” Strength is how completely an acid ionizes; concentration is how much is dissolved. Hydrofluoric acid (HF) is a weak acid yet extremely dangerous. HF

Three definitions of acids & bases

DefinitionAcidBaseMore
Arrhenius (Svante Arrhenius, 1884–87; Nobel 1903)Produces H⁺ (H₃O⁺, hydronium) in waterProduces OH⁻ in waterlearn more
Brønsted–Lowry (Johannes Brønsted & Thomas Lowry, 1923)Proton (H⁺) donorProton acceptor; acids and bases form conjugate pairslearn more
Lewis (Gilbert N. Lewis, 1923)Electron-pair acceptorElectron-pair donor (broadest definition)learn more

Water is amphoteric (amphiprotic) — it can act as acid or base. A buffer (weak acid + its conjugate base, like the carbonic acid/bicarbonate system in blood) resists pH change. learn more

Indicators & neutralization

IndicatorIn acidIn baseMore
Litmus (from lichens)RedBluelearn more
PhenolphthaleinColorlessPink/magenta (above ~pH 8.2)learn more
Bromothymol blueYellowBluelearn more
Methyl orangeRedYellow (changes ~pH 3.1–4.4)learn more
Red cabbage juice (anthocyanins)Red/pinkGreen/yellowlearn more

Neutralization: acid + base → salt + water (HCl + NaOH → NaCl + H₂O). A titration adds a solution of known concentration until the equivalence point, shown by an indicator's color change. Antacids neutralize stomach acid. learn more

Litmus mnemonic: “Base turns red litmus Blue.” Acids taste sour and react with metals to make H₂; bases taste bitter and feel slippery. learn more · base

Chemical bonds & intermolecular forces

BondHowTypical betweenProperties / examplesMore
IonicElectron transfer; + and − ions attractMetal + nonmetal (electronegativity difference > ~1.7)NaCl; crystal lattices, high melting points, conduct when melted or dissolvedlearn more
Covalent — polarUnequal sharing of electronsNonmetals with different electronegativity (~0.4–1.7)H₂O, HCl, NH₃ — partial charges (δ+ / δ−)learn more
Covalent — nonpolarEqual sharingIdentical or similar atomsH₂, O₂, N₂, Cl₂, CH₄; single, double, triple bondslearn more
Metallic“Sea” of delocalized electronsMetal atomsConductivity, luster, malleabilitylearn more
Hydrogen bond (intermolecular)H bonded to N, O, or F attracted to a lone pair on another N/O/FBetween molecules (or parts of one)Water's high boiling point & surface tension; ice floats; holds DNA strands together; protein shapelearn more
Van der Waals / London dispersionTemporary dipolesAll molecules (only force in nonpolar ones)Why geckos stick to walls; weakestlearn more

Lewis dot structures (G. N. Lewis, 1916) show valence electrons. “Like dissolves like”: polar solvents (water — the “universal solvent”) dissolve polar and ionic solutes; nonpolar solvents dissolve nonpolar solutes (oil and water don't mix). Soap and detergents have a polar head and nonpolar tail, forming micelles. Lewis structures · solubility · soap

Solution vocabulary: solute dissolves in solvent; saturated holds the max; supersaturated holds more (unstable — rock candy, hand warmers); suspension settles out; colloid (milk, fog, gelatin) shows the Tyndall effect (scatters a light beam). Gas solubility decreases with temperature (warm soda goes flat). solutions · Tyndall

VSEPR molecular shapes

Valence Shell Electron Pair Repulsion (Gillespie & Nyholm, 1957): electron domains around a central atom spread as far apart as possible; lone pairs repel more and squeeze bond angles. learn more

DomainsLone pairsShapeBond angleExampleMore
20Linear180°CO₂, BeCl₂learn more
30Trigonal planar120°BF₃, SO₃learn more
31Bent< 120° (~119°)SO₂learn more
40Tetrahedral109.5°CH₄, CCl₄learn more
41Trigonal pyramidal~107°NH₃learn more
42Bent~104.5°H₂Olearn more
50Trigonal bipyramidal90°, 120°PCl₅learn more
51Seesaw< 90°, < 120°SF₄learn more
52T-shaped< 90°ClF₃learn more
60Octahedral90°SF₆learn more
62Square planar90°XeF₄learn more

CO₂ has polar bonds but is a nonpolar molecule (linear, dipoles cancel); H₂O is polar because it is bent. Molecular polarity depends on both bond polarity and shape. learn more

Organic Chemistry & Biomolecules

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Organic chemistry is the chemistry of carbon compounds. Carbon forms 4 bonds and makes chains and rings. In 1828 Friedrich Wöhler synthesized urea (an organic compound) from inorganic ammonium cyanate, undermining vitalism (the idea that organic compounds need a “life force”). learn more · Wöhler synthesis

Hydrocarbons & naming prefixes

CarbonsPrefixAlkaneFormulaClueMore
1meth-MethaneCH₄Natural gas; potent greenhouse gas; cow burpslearn more
2eth-EthaneC₂H₆Natural gas componentlearn more
3prop-PropaneC₃H₈Grills, rural home heatinglearn more
4but-ButaneC₄H₁₀Lighterslearn more
5pent-PentaneC₅H₁₂First liquid alkane at room templearn more
6hex-HexaneC₆H₁₄Solventlearn more
7hept-HeptaneC₇H₁₆0 on the octane rating scalelearn more
8oct-OctaneC₈H₁₈Gasoline; isooctane = 100 on the octane scalelearn more
9non-NonaneC₉H₂₀Kerosene componentlearn more
10dec-DecaneC₁₀H₂₂Fuel componentlearn more

Mnemonic for meth/eth/prop/but: “Monkeys Eat Peeled Bananas.” From pent- on, the prefixes are Greek numbers. numeric prefixes

Functional groups

GroupStructureName endingExampleMore
Alcohol (hydroxyl)R–OH-olEthanol (drinking alcohol), methanol (wood alcohol, toxic), isopropanol (rubbing alcohol)learn more
AldehydeR–CHO-alFormaldehyde (methanal; preservative), vanillinlearn more
KetoneR–CO–R′-oneAcetone (propanone; nail-polish remover)learn more
Carboxylic acidR–COOH-oic acidAcetic acid (ethanoic acid; vinegar)learn more
EsterR–COO–R′-oateFruity smells (isoamyl acetate = banana); fats; aspirin; made from acid + alcohollearn more
EtherR–O–R′etherDiethyl ether (early anesthetic, 1840s)learn more
AmineR–NH₂-amineMethylamine; fishy odors; amino acidslearn more
AmideR–CO–NH₂-amidePeptide bonds in proteins; nylon; acetaminophenlearn more
HaloalkaneR–X (F, Cl, Br, I)halo- prefixChloroform; CFCs (Freon) that deplete ozonelearn more

Polymers

Polymers are long chains of repeating monomers (the term “polymer” was coined by Berzelius). Made by addition or condensation (releases water) polymerization. learn more

PolymerClueMore
Vulcanized rubberCharles Goodyear heated rubber with sulfur (1839)learn more
BakeliteLeo Baekeland (1907) — first fully synthetic plasticlearn more
NylonWallace Carothers at DuPont (1935); stockings, toothbrush bristleslearn more
Teflon (PTFE)Roy Plunkett at DuPont, accidental discovery (1938); nonstick panslearn more
KevlarStephanie Kwolek at DuPont (1965); bulletproof vestslearn more
Polyethylene, PVC, polystyrene, PETBags (most common plastic), pipes, Styrofoam, soda bottleslearn more
Natural polymersCellulose, starch, proteins, DNA, chitin, natural rubberlearn more

The four classes of biomolecules

ClassMonomer / building blockExamplesFunctionMore
Carbohydrates (C, H, O ≈ 1:2:1)Monosaccharides (glucose, fructose, galactose)Disaccharides: sucrose (table sugar), lactose (milk), maltose. Polysaccharides: starch (plants store), glycogen (animals store, in liver & muscle), cellulose (plant cell walls), chitin (insect shells)Quick energy, structurelearn more
LipidsGlycerol + 3 fatty acids (triglyceride)Fats, oils, waxes, phospholipids (cell membranes), steroids (cholesterol, testosterone, estrogen). Saturated (no C=C, solid, animal fats) vs. unsaturated (C=C kinks, liquid oils)Long-term energy storage, insulation, membranes, hormoneslearn more
ProteinsAmino acids (20 standard) joined by peptide bondsEnzymes (lactase, amylase), hemoglobin, keratin, collagen, insulin, antibodies. Four levels of structure (primary → quaternary)Catalysis, structure, transport, defense, signalslearn more
Nucleic acidsNucleotides (5-carbon sugar + phosphate + nitrogenous base)DNA, RNA; ATP is a nucleotide (energy currency)Store and transmit genetic informationlearn more

Enzymes end in -ase, sugars in -ose. Enzymes work by the “lock and key” (Emil Fischer, 1894) or “induced fit” models and can be denatured by heat or pH. CHNOPS = the six most common elements of life (carbon, hydrogen, nitrogen, oxygen, phosphorus, sulfur). learn more

Biology

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Cell theory

(1) All living things are made of cells; (2) the cell is the basic unit of life; (3) all cells come from pre-existing cells. Robert Hooke coined “cell” looking at cork in Micrographia (1665); Antonie van Leeuwenhoek first saw living microbes (“animalcules”) in the 1670s; Matthias Schleiden (plants, 1838) and Theodor Schwann (animals, 1839) proposed cell theory; Rudolf Virchow added omnis cellula e cellula (“every cell from a cell,” 1855). learn more

Cell parts & functions

OrganelleFunction / clueFound inMore
Nucleus“Control center”; holds DNA (chromatin); surrounded by nuclear envelope with poresEukaryoteslearn more
NucleolusInside the nucleus; makes ribosomes (rRNA)Eukaryoteslearn more
Mitochondrion“Powerhouse of the cell” — cellular respiration makes ATP; has its own DNA (inherited from the mother); folds called cristaeNearly all eukaryoteslearn more
ChloroplastPhotosynthesis; contains green chlorophyll; stacks of thylakoids called grana; fluid = stroma; own DNAPlants, algaelearn more
RibosomeMakes proteins (translation); not membrane-boundAll cells (prokaryotes too)learn more
Rough EREndoplasmic reticulum studded with ribosomes; makes and transports proteinsEukaryoteslearn more
Smooth ERMakes lipids; detoxifies drugs (abundant in liver)Eukaryoteslearn more
Golgi apparatusModifies, packages, and ships proteins (“post office”); named for Camillo GolgiEukaryoteslearn more
LysosomeDigestive enzymes; breaks down waste (“suicide sac”)Mainly animal cellslearn more
VacuoleStorage of water, food, waste; plants have one large central vacuole providing turgor pressurePlants (large), animals (small)learn more
Cell membranePhospholipid bilayer; selectively permeable; fluid mosaic model (Singer & Nicolson, 1972)All cellslearn more
Cell wallRigid support outside the membrane: cellulose (plants), chitin (fungi), peptidoglycan (bacteria)Plants, fungi, bacterialearn more
Cytoplasm / cytoskeletonGel-like interior / protein fibers (microtubules, microfilaments) giving shape and movementAll cells / eukaryoteslearn more
CentriolesOrganize spindle fibers during cell divisionAnimal cellslearn more
Flagella / ciliaWhip-like tail / short hairs for movementVariouslearn more

Endosymbiotic theory (championed by Lynn Margulis, 1967): mitochondria and chloroplasts descend from free-living bacteria engulfed by ancestral cells — evidence: their own circular DNA, double membranes, and bacteria-like ribosomes. learn more

Transport: diffusion (high → low concentration), osmosis (diffusion of water across a membrane), facilitated diffusion (via proteins) — all passive; active transport uses ATP to go against the gradient (sodium–potassium pump). A cell in a hypotonic solution swells; in a hypertonic solution it shrinks. osmosis · active transport

Prokaryotes vs. eukaryotes; plant vs. animal cells

ProkaryoteEukaryote
NucleusNone — DNA in a nucleoid region (plus plasmids)True membrane-bound nucleus (Greek eu = true, karyon = kernel)
OrganellesNo membrane-bound organelles; has ribosomesMitochondria, ER, Golgi, etc.
SizeSmall (~1–10 μm)Larger (~10–100 μm)
ExamplesBacteria, archaeaAnimals, plants, fungi, protists
Morelearn morelearn more

Plant cells have a cell wall, chloroplasts, and a large central vacuole, and are usually boxy; animal cells lack these but have centrioles and more lysosomes. Viruses are not cells — they need a host to reproduce. plant cell · virus

Mitosis vs. meiosis

The cell cycle: interphase (G₁ growth, S = DNA synthesis/replication, G₂) → mitosis → cytokinesis. Mitosis phases: PMAT — learn more

  1. Prophase — chromosomes condense, nuclear envelope breaks down, spindle forms.
  2. Metaphase — chromosomes line up at the middle (metaphase plate).
  3. Anaphase — sister chromatids pulled apart to opposite poles.
  4. Telophase — two new nuclei form; then cytokinesis splits the cytoplasm (cleavage furrow in animals, cell plate in plants).
MitosisMeiosis
PurposeGrowth, repair, asexual reproductionMaking gametes (sperm, egg) for sexual reproduction
Divisions12 (meiosis I and II)
Daughter cells2, diploid (2n), genetically identical4, haploid (n), genetically different
Humans46 → 46 chromosomes46 → 23 chromosomes
VariationNone (clones)Crossing over (prophase I) and independent assortment; homologous pairs separate in anaphase I
Morelearn morelearn more

Mitosis vs. meiosis: miTosis = Two identical cells; mEiosis = sEx cells, four different haploid cells. Humans have 23 pairs (46 total) — 22 pairs of autosomes + 1 pair of sex chromosomes (XX or XY). Cancer is uncontrolled mitosis. learn more

Photosynthesis & cellular respiration

Photosynthesis (chloroplasts): 6CO₂ + 6H₂O + light energy → C₆H₁₂O₆ + 6O₂
Cellular respiration (cytoplasm + mitochondria): C₆H₁₂O₆ + 6O₂ → 6CO₂ + 6H₂O + energy (ATP)

The two equations are reverses of each other. ATP (adenosine triphosphate) is the cell's energy currency. Plants do both photosynthesis and respiration. ATP

DNA, RNA & the genetic code

DNARNA
SugarDeoxyriboseRibose
BasesAdenine, Thymine, Guanine, CytosineA, Uracil (replaces T), G, C
StrandsDouble helix (antiparallel)Usually single
Types / roleStores genetic information (in nucleus)mRNA (messenger), tRNA (transfer — carries amino acids), rRNA (ribosomal)
Morelearn morelearn more

“Transforming principle” → Griffith (1928) / Avery–MacLeod–McCarty (1944) showed DNA is the genetic material; Hershey–Chase (1952) confirmed it with radioactively labeled viruses. Friedrich Miescher first isolated DNA (“nuclein”) in 1869. learn more

Mendelian genetics & Punnett squares

Gregor Mendel, an Augustinian friar in Brno (now Czech Republic), bred pea plants (c. 1856–1863) and published in 1866; his work was ignored until rediscovered in 1900 by Hugo de Vries, Carl Correns, and Erich von Tschermak. He studied seven traits (seed shape, seed color, flower color, pod shape, pod color, flower position, stem height). learn more · Mendelian inheritance

Bb × BbBb
BBBBb
bBbbb

→ ¼ BB, ½ Bb, ¼ bb; ¾ show the dominant trait. learn more

Taxonomy & classification

Carl Linnaeus (Sweden) introduced binomial nomenclature — Genus species, italicized, genus capitalized (Homo sapiens, “wise man,” a name he coined) — in Systema Naturae (1st ed. 1735; 10th ed. 1758 is the starting point for animal names) and Species Plantarum (1753). learn more · ranks

RankHumanGray wolf / dogMnemonicMore
DomainEukaryaEukaryaDearlearn more
KingdomAnimaliaAnimaliaKinglearn more
PhylumChordataChordataPhiliplearn more
ClassMammaliaMammaliaCamelearn more
OrderPrimatesCarnivoraOverlearn more
FamilyHominidaeCanidaeForlearn more
GenusHomoCanisGoodlearn more
SpeciessapienslupusSouplearn more

“Dear King Philip Came Over For Good Soup.” learn more

Evolution

Darwin did not say humans descended from modern apes — humans and apes share a common ancestor. And Lamarck, not Darwin, proposed inheriting traits acquired during life. learn more

Ecology

BiomeFeaturesMore
TundraColdest; permafrost; mosses, lichens, caribou; treelesslearn more
Taiga (boreal forest)Conifers; largest land biome; Canada, Siberialearn more
Temperate deciduous forestTrees drop leaves in fall; four seasons; eastern U.S.learn more
Tropical rainforestGreatest biodiversity; canopy layers; Amazon, Congolearn more
Temperate grassland (prairie, steppe, pampas)Rich soils, fire & grazing; (Kansas) the Flint Hills hold the largest remaining stretch of tallgrass prairie in North America (Tallgrass Prairie National Preserve; Konza Prairie near Manhattan); big bluestem, bisontallgrass prairie · Flint Hills
SavannaTropical grassland with scattered trees; African megafaunalearn more
Desert< 25 cm (10 in) rain/yr; can be hot or cold (Antarctica is the largest desert)learn more
Chaparral (Mediterranean)Hot dry summers, mild wet winters; shrubs; fire-adaptedlearn more

Human body systems

SystemMain organsQuiz cluesMore
Circulatory (cardiovascular)Heart, arteries, veins, capillaries, blood4-chambered heart (2 atria, 2 ventricles); arteries carry blood away from the heart; aorta = largest artery; William Harvey described circulation (1628)learn more
RespiratoryLungs, trachea, bronchi, alveoli, diaphragmGas exchange in alveoli; diaphragm drives breathinglearn more
DigestiveMouth, esophagus, stomach, small & large intestine, liver, pancreas, gallbladderMost absorption in the small intestine (villi); liver = largest internal organ, makes bile; peristalsislearn more
NervousBrain, spinal cord, nervesNeuron parts: dendrite, cell body, axon, myelin; cerebrum (thinking), cerebellum (balance), medulla (breathing, heartbeat)learn more
SkeletalBones, cartilage, ligamentsAdults: 206 bones; femur longest, stapes (in the ear) smallest; marrow makes blood cellslearn more
MuscularSkeletal, smooth, cardiac muscleTendons connect muscle to bone (ligaments bone to bone); gluteus maximus largest musclelearn more
IntegumentarySkin, hair, nailsSkin is the largest organ; epidermis, dermis; makes vitamin Dlearn more
EndocrinePituitary, thyroid, adrenal glands, pancreas, gonadsHormones; pituitary = “master gland”; insulin (pancreas) lowers blood sugar; adrenaline = fight or flightlearn more
Immune / lymphaticWhite blood cells, lymph nodes, spleen, thymusAntibodies, B and T cells; vaccines train itlearn more
Excretory / urinaryKidneys, ureters, bladder, urethraKidneys filter blood via nephronslearn more
ReproductiveOvaries, testes, uterusProduces gametes by meiosislearn more

Blood & blood types

TypeAntigens on red cellsAntibodies in plasmaCan receive red cells fromMore
AAanti-BA, Olearn more
BBanti-AB, Olearn more
ABA and BneitherA, B, AB, O — universal recipient (AB+)learn more
Oneitheranti-A and anti-BO only — O− is the universal donor of red cellslearn more

O+ is the most common type in the U.S.; AB− the rarest. For plasma the roles flip: AB is the universal plasma donor. Charles Drew pioneered large-scale blood plasma banking (1940s). distribution · Drew

Vitamins & deficiency diseases

Casimir Funk coined “vitamine” (1912). (Kansas) Elmer McCollum, born near Fort Scott and a University of Kansas graduate, co-discovered vitamin A (1913) and named vitamin D (1922), starting the letter-naming system. Fat-soluble vitamins: A, D, E, K (stored in fat; can build up); the rest (B's, C) are water-soluble. learn more · McCollum

Vitamin / nutrientDeficiency diseaseClueMore
A (retinol)Night blindnessCarrots (beta-carotene)learn more
B₁ (thiamine)BeriberiPolished white rice diets; Christiaan Eijkmanlearn more
B₃ (niacin)Pellagra (“4 D's”: dermatitis, diarrhea, dementia, death)Corn-heavy diets in the American South; Joseph Goldbergerlearn more
B₉ (folate / folic acid)Anemia; neural-tube birth defectsLeafy greens; prenatal vitaminslearn more
B₁₂ (cobalamin)Pernicious anemiaContains cobalt; Dorothy Hodgkin found its structurelearn more
C (ascorbic acid)Scurvy (bleeding gums)Sailors; James Lind's citrus trial (1747) → British “limeys”learn more
D (calciferol)Rickets (soft, bowed bones)“Sunshine vitamin” — made in skin by UV lightlearn more
KBleeding (poor clotting)From German Koagulation; made by gut bacterialearn more
Iodine (mineral)Goiter (enlarged thyroid)Iodized salt (U.S., 1924)learn more
Iron (mineral)Iron-deficiency anemiaNeeded for hemoglobinlearn more

Earth Science & Weather

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Earth's layers

LayerState / compositionFactsMore
CrustSolid rock: continental (granite, ~30–70 km thick, less dense) and oceanic (basalt, ~5–10 km, denser)Thinnest layer; most abundant elements O, Si, Al, Felearn more
MantleHot, solid rock that flows slowly (peridotite); upper part includes the plastic asthenosphereThickest layer (~2,900 km), ~84% of Earth's volume; convection drives plates. Crust + rigid uppermost mantle = lithospherelearn more
Outer coreLiquid iron–nickelIts flow generates Earth's magnetic field (geodynamo)learn more
Inner coreSolid iron–nickel (solid due to immense pressure)~5,200 °C — roughly as hot as the Sun's surface; discovered by Inge Lehmann (1936)learn more

Plate tectonics

BoundaryMotionFeatures & examplesMore
DivergentPlates move apartMid-ocean ridges (Mid-Atlantic Ridge, Iceland), rift valleys (East African Rift); new crust formslearn more
ConvergentPlates collideOceanic–continental subduction: volcanic mountains (Andes, Cascades — Mt. St. Helens 1980). Oceanic–oceanic: trenches and island arcs (Mariana Trench, deepest point, Challenger Deep ≈ 11 km; Japan). Continent–continent: Himalayas (India hitting Asia; Everest)learn more
TransformPlates slide past each otherEarthquakes; San Andreas Fault (California)learn more

The Ring of Fire rings the Pacific with ~75% of the world's volcanoes. Hot spots (mantle plumes) form volcano chains away from boundaries: Hawaii, Yellowstone. Volcano types: shield (Mauna Loa — gentle basalt flows), stratovolcano/composite (Fuji, St. Helens — explosive), cinder cone. Ring of Fire · hot spots · volcanoes

Rock types & the rock cycle

TypeForms byExamplesMore
Igneous (“fire”)Cooling of magma/lava. Intrusive (plutonic, slow-cooled underground, large crystals) vs. extrusive (volcanic, fast-cooled at surface, small or no crystals)Granite (intrusive); basalt, obsidian (volcanic glass), pumice (floats on water)learn more
SedimentaryWeathering, erosion, deposition, compaction and cementation of sediments; layers (strata); contain fossilsSandstone, shale, limestone, conglomerate, chalk, coal, rock saltlearn more
Metamorphic (“change form”)Heat and pressure transform existing rock without melting; often foliated (banded)Limestone → marble; shale → slate; sandstone → quartzite; granite → gneiss; schistlearn more

The rock cycle links all three: any rock can become any other. James Hutton (“father of modern geology”) proposed deep time and uniformitarianism — “the present is the key to the past” (Hutton's 1788 paper; phrase popularized later); Charles Lyell's Principles of Geology (1830–33) spread it. Nicolas Steno (1669): law of superposition — lower layers are older. rock cycle · uniformitarianism · superposition

(Kansas) Western Kansas was covered by the Western Interior Seaway in the Cretaceous: its Niobrara Chalk forms Monument Rocks and Castle Rock and yields famous fossils — Pteranodon (Kansas state flying fossil), the mosasaur Tylosaurus (state marine fossil), and the “fish-within-a-fish” Xiphactinus at the Sternberg Museum in Hays. The Flint Hills are Permian limestone with chert (flint) — too rocky to plow, which preserved the prairie. Hutchinson sits on thick Permian rock salt beds (Strataca underground salt museum). Niobrara · Monument Rocks · Western Interior Seaway

Mohs hardness scale

Devised by German mineralogist Friedrich Mohs (1812): a harder mineral scratches a softer one. It is ordinal, not linear — diamond (10) is far more than twice as hard as apatite (5). learn more

HardnessMineralNoteMore
1TalcSoftest; talcum powderlearn more
2GypsumDrywall, plaster of Paris; fingernail ≈ 2.5learn more
3CalciteLimestone, marble; fizzes in acid; copper coin ≈ 3learn more
4FluoriteGlows under UV (gave us “fluorescence”)learn more
5ApatiteSame mineral family as tooth enamel; glass/knife ≈ 5.5learn more
6Orthoclase feldsparMost common mineral group in the crustlearn more
7QuartzSiO₂; scratches glass; amethystlearn more
8TopazGemstonelearn more
9CorundumAl₂O₃ — ruby (red) and sapphirelearn more
10DiamondHardest natural mineral; pure carbonlearn more

Mnemonic: “Tall Giraffes Can Fight Anyone Other Than Carnivorous Dinosaurs.” Other mineral ID tests: streak (powder color), luster, cleavage vs. fracture, specific gravity. Hematite has a red-brown streak; pyrite (“fool's gold”) a greenish-black one. learn more

Earthquakes & their scales

Magnitude (Richter/moment) measures the energy released at the source — one number per quake. Intensity (Mercalli) varies by place. A magnitude 7 releases about 1,000× (32²) the energy of a magnitude 5. learn more

Geologic time scale

Eons: Hadean → Archean → Proterozoic (together often called “Precambrian,” ~88% of Earth history) → Phanerozoic (“visible life,” the last ~539 million years). Phanerozoic eras: Paleozoic (“ancient life”), Mesozoic (“middle life,” age of reptiles/dinosaurs), Cenozoic (“recent life,” age of mammals). Ma = millions of years ago (approximate, ICS chart). learn more

EraPeriodBegan (Ma)HighlightsMore
PaleozoicCambrian539“Cambrian explosion” of animal life; trilobites; Burgess Shale. Named for Cambria (Wales)learn more
Ordovician485Marine invertebrates; first land plants; ends in mass extinctionlearn more
Silurian444Jawed fish; vascular plantslearn more
Devonian419“Age of Fishes”; first tetrapods, forestslearn more
Carboniferous359Coal swamps; giant insects; first reptiles. In the U.S. split into the Mississippian and Pennsylvanian (much of eastern Kansas's bedrock is Pennsylvanian)learn more
Permian299Pangaea assembled; ends with the Great Dying (~252 Ma), the largest mass extinction (~80–90%+ of marine species). Named for Perm, Russialearn more
MesozoicTriassic252First dinosaurs and mammalslearn more
Jurassic201Giant sauropods; Archaeopteryx; named for the Jura Mountainslearn more
Cretaceous145Flowering plants; T. rex; Kansas under the seaway. Ends 66 Ma with the K–Pg extinction — asteroid impact at Chicxulub (Yucatán), proposed by Luis & Walter Alvarez (1980) from an iridium layerlearn more
CenozoicPaleogene66Mammals diversifylearn more
Neogene23Grasslands spread; early homininslearn more
Quaternary2.6Ice ages; Homo sapiens; Pleistocene and Holocene (current epoch, since ~11,700 years ago). A proposed “Anthropocene” epoch was rejected in 2024.learn more

Period mnemonic: “Camels Often Sit Down Carefully; Perhaps Their Joints Creak — Possibly Next Quarter.” The “Big Five” mass extinctions: end-Ordovician, Late Devonian, end-Permian, end-Triassic, end-Cretaceous. learn more

Atmosphere

Composition of dry air: nitrogen ~78%, oxygen ~21%, argon ~0.93%, carbon dioxide ~0.04% (over 420 ppm and rising; measured at Mauna Loa since 1958 — the Keeling Curve). learn more · Keeling Curve

Layer (bottom → top)Altitude (approx.)Temperature trendFeaturesMore
Troposphere0 – ~12 km (8 km at poles, ~17 km at equator)Cools with heightAll weather; ~75% of the atmosphere's mass; top = tropopauselearn more
Stratosphere~12 – 50 kmWarms with heightOzone layer absorbs UV; jets cruise near its base; weather balloonslearn more
Mesosphere~50 – 85 kmCools with height (coldest layer, ~−90 °C)Meteors burn up herelearn more
Thermosphere~85 – 600 kmWarms sharply (can exceed 1,500 °C, though it wouldn't feel hot)Auroras; the ISS orbits here (~400 km); contains most of the ionospherelearn more
Exosphere~600 km – 10,000 km—Fades into space; many satelliteslearn more

Mnemonic: “The Strong Man's Triceps Explode.” The Kármán line (100 km) is the conventional edge of space. The 1987 Montreal Protocol phased out ozone-destroying CFCs (Molina, Rowland & Crutzen, Nobel 1995). Kármán line · Montreal Protocol

Clouds

Latin cloud names were proposed by English pharmacist Luke Howard (1802–03). learn more

Name / rootMeaningLook & weatherMore
Cirrus“curl of hair”High, thin, wispy ice crystals (“mares' tails”); fair weather but may signal an approaching warm frontlearn more
Cumulus“heap”Puffy, flat-bottomed, cotton-ball; fair weatherlearn more
Stratus“layer”Flat, gray sheets; drizzle; fog is stratus at ground levellearn more
Nimbus / nimbo-“rain cloud”Precipitation-producing: nimbostratus (steady rain/snow)learn more
Cumulonimbus“heap + rain”Towering thunderstorm cloud with an anvil top; lightning, hail, tornadoeslearn more
Alto- / cirro-middle / highAltocumulus, altostratus (mid-level); cirrocumulus, cirrostratus (high; halos around Sun/Moon)learn more

Weather & severe storms

Tornadoes — the (Enhanced) Fujita scale

Created by Tetsuya “Ted” Fujita (University of Chicago, “Mr. Tornado”) in 1971; replaced in the U.S. by the Enhanced Fujita (EF) scale on Feb 1, 2007. Ratings are assigned after the storm from damage surveys (28 damage indicators), giving estimated 3-second gust speeds. EF scale · original F scale

RatingEst. wind (mph)Typical damageMore
EF065–85Light: shingles, brancheslearn more
EF186–110Moderate: mobile homes overturned, roofs strippedlearn more
EF2111–135Considerable: roofs torn off frame houses, large trees snappedlearn more
EF3136–165Severe: entire stories of houses destroyedlearn more
EF4166–200Devastating: well-built houses leveledlearn more
EF5> 200Incredible: houses swept off foundationsEF5 list

(Kansas) Kansas sits in Tornado Alley. Notable Kansas tornadoes: Udall, May 25, 1955 (F5; deadliest in state history, 80 killed); Topeka, June 8, 1966 (F5; tore through downtown and Washburn University, then the costliest U.S. tornado); Greensburg, May 4, 2007 (the first EF5 under the new scale; ~1.7 miles wide; destroyed about 95% of the town, which rebuilt as a model “green” town). A tornado watch means conditions are favorable; a warning means one is occurring or detected — take shelter. Udall · Topeka · Greensburg · Tornado Alley

The Fujita scales rate tornadoes by damage (winds are estimated from it); the Saffir–Simpson scale rates hurricanes by measured sustained wind. Don't swap them. learn more

Hurricanes — the Saffir–Simpson scale

Developed by engineer Herbert Saffir and National Hurricane Center director Robert Simpson (early 1970s); based on 1-minute sustained winds. A tropical storm (39–73 mph) gets a name; at 74 mph it becomes a hurricane (called a typhoon in the western Pacific, a cyclone in the Indian Ocean). The calm center is the eye. learn more · tropical cyclones

CategorySustained wind (mph)More
174–95learn more
296–110learn more
3 (“major”)111–129learn more
4130–156learn more
5157 or higherCat 5 list

The water cycle

Processes: evaporation (mostly from oceans), transpiration (water vapor released by plants; together “evapotranspiration”), condensation (clouds), precipitation, infiltration (soaking into ground → groundwater/aquifers), runoff, collection; also sublimation from snow and ice. The Sun powers it. About 97% of Earth's water is salty ocean; of the ~3% fresh water, about two-thirds is locked in ice caps and glaciers. learn more · water distribution

(Kansas) Western Kansas farms irrigate from the Ogallala (High Plains) Aquifer, one of the world's largest — but it is being pumped far faster than rain recharges it. learn more

Astronomy & Space

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The planets

Order from the Sun: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune — “My Very Educated Mother Just Served Us Nachos.” The four inner terrestrial (rocky) planets are separated from the outer gas giants (Jupiter, Saturn) and ice giants (Uranus, Neptune) by the asteroid belt. Moon counts below are as of mid-2026 and keep rising as small moons are found. learn more · Solar System

PlanetMoonsLargest / notable moonDay (rotation)YearNotable features (quiz clues)More
Mercury0—58.6 Earth days (a solar day lasts 176)88 daysSmallest planet; closest to Sun; huge temperature swings; Caloris Basin; MESSENGER orbiter; named for the swift messenger godlearn more
Venus0—243 days, retrograde (longer than its year)225 daysHottest planet (~465 °C) from runaway greenhouse effect; thick CO₂ air, sulfuric-acid clouds; “Earth's twin” in size; brightest planet — “morning/evening star”; Soviet Venera 7 made the first landing on another planet (1970); Magellan mapped it by radarlearn more
Earth1The Moon23 h 56 min (sidereal)365.25 daysDensest planet (5.5 g/cm³); only known life; liquid surface waterlearn more
Mars2Phobos and Deimos (“fear” and “dread”; found by Asaph Hall, 1877)24 h 37 min687 days“Red Planet” (iron oxide); Olympus Mons — tallest volcano in the solar system; Valles Marineris canyon; rovers Sojourner, Spirit, Opportunity, Curiosity, Perseverance (with the Ingenuity helicopter)learn more
Jupiter115Ganymede — largest moon in the solar system (bigger than Mercury)~9 h 56 min (shortest day)11.9 yearsLargest planet; Great Red Spot storm; four Galilean moons — Io (volcanoes), Europa (subsurface ocean), Ganymede, Callisto — found by Galileo in 1610; faint rings; Juno orbiter; Europa Clipper (launched 2024)learn more · moons
Saturn~290 (most of any planet)Titan — thick nitrogen atmosphere, methane lakes; Huygens probe landed 2005~10 h 33 min29.4 yearsSpectacular rings (ice; Cassini Division); least dense planet — would float in water; hexagon storm at north pole; Enceladus' ice geysers; Cassini–Huygens missionlearn more · moons
Uranus29Titania; moons named for characters of Shakespeare and Alexander Pope (Miranda, Oberon, Ariel, Umbriel)~17 h 14 min, retrograde84 yearsTilted ~98° — rotates on its side; first planet discovered by telescope (William Herschel, 1781; he called it “Georgium Sidus” for George III); blue-green from methane; visited only by Voyager 2 (1986)learn more
Neptune16Triton — orbits backward (retrograde), nitrogen geysers; likely a captured Kuiper belt object~16 h165 yearsFound by mathematical prediction (Urbain Le Verrier; also John Couch Adams) and spotted by Johann Galle, 1846; strongest winds in the solar system; Great Dark Spot; visited only by Voyager 2 (1989)learn more

Venus, not Mercury, is the hottest planet. Venus and Uranus spin “backward.” Saturn has the most known moons (the lead has flipped with Jupiter as discoveries are announced — check the date of any “how many moons” clue). Titan is the only moon with a thick atmosphere. retrograde rotation

Earth's Moon

About ¼ Earth's diameter, ~384,000 km away; tidally locked (we always see the same side). Phases: new → waxing crescent → first quarter → waxing gibbous → full → waning gibbous → third quarter → waning crescent (~29.5-day synodic month). Likely formed by the giant-impact hypothesis (a Mars-sized body, “Theia,” hit early Earth). Tides are caused mainly by the Moon's gravity (spring tides at new/full moon, neap tides at quarters). A solar eclipse happens at new moon; a lunar eclipse at full moon. learn more · phases · giant impact

Dwarf planets & small bodies

(Kansas) Clyde Tombaugh (1906–1997) was born in Illinois but grew up on a farm near Burdett, Kansas, where he built telescopes from farm-machinery parts and sent his drawings of Jupiter and Mars to Lowell Observatory, which hired him. After discovering Pluto he earned his degrees at the University of Kansas. Some of his ashes flew past Pluto aboard New Horizons. Kansas is also rich in meteorites — the Brenham pallasite field in Kiowa County is famous. Tombaugh · Brenham meteorite

The Sun

Stars

Stellar life cycle

Star massPathMore
Low / Sun-likeNebula → protostar → main sequence → red giant → planetary nebula (outer layers shed) → white dwarf (Earth-sized, cooling) → (theoretical) black dwarflearn more · white dwarf
High mass (≳ 8 Suns)Nebula → main sequence (blue) → red supergiant → supernova (core collapse; forges heavy elements) → neutron star (city-sized; a spinning one is a pulsar, first found by Jocelyn Bell Burnell, 1967) or, for the most massive, a black holesupernova · neutron star · black hole

Kepler's laws of planetary motion

Derived by Johannes Kepler from Tycho Brahe's precise naked-eye observations of Mars; later explained by Newton's gravity. learn more

LawStatementPublishedMore
1st — law of ellipsesPlanets orbit in ellipses with the Sun at one focus.Astronomia nova, 1609learn more
2nd — law of equal areasA line from Sun to planet sweeps out equal areas in equal times — planets move fastest at perihelion (closest), slowest at aphelion.Astronomia nova, 1609learn more
3rd — harmonic lawT² ∝ a³; with T in years and a in AU, T² = a³. A planet at 4 AU takes √64 = 8 years.Harmonices Mundi, 1619learn more

Distances

A light-year is a unit of distance, not time. learn more

Galaxies

The Big Bang & cosmology

Space exploration milestones

DateMission / eventCluesMore
Oct 4, 1957Sputnik 1 (USSR)First artificial satellite; started the Space Race. Sputnik 2 carried the dog Laika.learn more
Jan 31, 1958Explorer 1 (USA)First U.S. satellite; discovered the Van Allen radiation belts. NASA founded later in 1958.learn more
Apr 12, 1961Vostok 1Yuri Gagarin, first human in space and in orbit.learn more
May 5, 1961Freedom 7 (Mercury)Alan Shepard, first American in space (suborbital).learn more
Feb 20, 1962Friendship 7 (Mercury)John Glenn, first American to orbit Earth.learn more
June 16, 1963Vostok 6Valentina Tereshkova, first woman in space.learn more
July 20, 1969Apollo 11Neil Armstrong and Buzz Aldrin land the lunar module Eagle in the Sea of Tranquility; Michael Collins orbits in Columbia. “That's one small step for [a] man, one giant leap for mankind.”learn more
April 1970Apollo 13Oxygen tank explosion; “Houston, we've had a problem”; crew returned safely. (Kansas) Its command module Odyssey is displayed at the Cosmosphere in Hutchinson.learn more
Dec 1972Apollo 17Last crewed Moon landing (Gene Cernan, Harrison Schmitt). (Kansas) Command module pilot Ronald Evans was born in St. Francis, Kansas, and attended KU.learn more · Evans
1977Voyager 1 & 2Grand Tour of the outer planets; carry the Golden Record (Carl Sagan's committee). Voyager 1 crossed into interstellar space in 2012 and is the most distant human-made object; its “Pale Blue Dot” photo (1990). Voyager 2 is the only craft to visit Uranus and Neptune.learn more · Golden Record
1981–2011Space ShuttleFirst reusable spacecraft; disasters: Challenger (Jan 28, 1986) and Columbia (Feb 1, 2003). (Kansas) Joe Engle of Chapman, KS commanded STS-2 (1981); KU's Steven Hawley deployed the Hubble telescope (1990).learn more · Engle · Hawley
Apr 24, 1990Hubble Space TelescopeLaunched on Shuttle Discovery; flawed mirror fixed by astronauts in 1993; Hubble Deep Field.learn more
1997–2017Cassini–HuygensNASA/ESA/Italy mission to Saturn (arrived 2004); Huygens probe landed on Titan (2005); ended with a deliberate plunge into Saturn (“Grand Finale,” Sept 15, 2017).learn more
Nov 2000 →International Space StationContinuously crewed since Nov 2, 2000; orbits ~400 km up about every 90 minutes.learn more
2006 / 2015New HorizonsLaunched Jan 2006; first flyby of Pluto (July 14, 2015); then Kuiper belt object Arrokoth (Jan 1, 2019).learn more
Dec 25, 2021James Webb Space TelescopeInfrared telescope with a 6.5 m gold-coated beryllium mirror of 18 hexagonal segments; orbits the Sun–Earth L2 point, 1.5 million km away; first images July 2022.learn more
2022 / 2026Artemis programArtemis I (uncrewed, Nov 2022); Artemis II (April 2026) flew four astronauts around the Moon — the first crewed lunar flight since Apollo 17.learn more

(Kansas) The Cosmosphere in Hutchinson (a Smithsonian affiliate) holds one of the world's largest space-artifact collections: the Apollo 13 command module Odyssey, Gus Grissom's recovered Mercury capsule Liberty Bell 7, an SR-71 Blackbird, and the largest collection of Soviet space hardware outside Russia. learn more

Scientists

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About 25 of the most-asked names in each field, with the facts that show up as clues: laws, units, equations, discoveries, and inventions named after them. Women scientists from every field are collected in their own table. learn more

Physicists

NameDatesNationalityKnown for (quiz clues)More
Archimedesc. 287 – c. 212 BCGreek (Syracuse, Sicily)Buoyancy principle and “Eureka!”; law of the lever; Archimedes' screw; war machines and “death ray” mirrors (legendary) defending Syracuse; killed by a Roman soldier (“Do not disturb my circles”).learn more
Galileo Galilei1564–1642ItalianInclined-plane experiments; falling bodies; pendulum timing; improved the telescope (1609) — saw Jupiter's four big moons, phases of Venus, sunspots, lunar mountains (Sidereus Nuncius, 1610); Dialogue Concerning the Two Chief World Systems (1632) led to his trial and house arrest (1633).learn more
Christiaan Huygens1629–1695DutchWave theory of light (Huygens' principle); invented the pendulum clock (1656); discovered Titan and explained Saturn's rings (1655–59).learn more
Robert Hooke1635–1703EnglishHooke's law of springs; Micrographia (1665) — coined “cell” from cork; Royal Society curator of experiments; feuded with Newton.learn more
Isaac Newton1643–1727EnglishPrincipia (1687): three laws of motion and universal gravitation; co-invented calculus (rivalry with Leibniz); Opticks — white light split by a prism; reflecting telescope; Lucasian Professor at Cambridge; Master of the Royal Mint; the falling-apple story. Unit: newton.learn more
Benjamin Franklin1706–1790AmericanKite experiment (1752) showing lightning is electricity; lightning rod; named positive/negative charge and “battery”; bifocals; Franklin stove; mapped the Gulf Stream.learn more
Alessandro Volta1745–1827ItalianVoltaic pile (1800), the first electric battery (stacked zinc and copper disks); disputed Galvani's “animal electricity”; discovered methane. Unit: volt.learn more
Georg Ohm1789–1854GermanOhm's law V = IR (1827). Unit: ohm (Ω).learn more
Michael Faraday1791–1867EnglishElectromagnetic induction (1831); first electric motor and dynamo; Faraday cage; laws of electrolysis; discovered benzene; Humphry Davy's lab assistant with little formal schooling; started the Royal Institution Christmas Lectures. Unit: farad.learn more
William Thomson, Lord Kelvin1824–1907British (born Belfast)Absolute temperature scale; second law of thermodynamics; transatlantic telegraph cable; badly underestimated Earth's age. Unit: kelvin.learn more
James Clerk Maxwell1831–1879ScottishMaxwell's equations unifying electricity, magnetism and light; first color photograph (1861, tartan ribbon); Maxwell–Boltzmann distribution; “Maxwell's demon”; showed Saturn's rings are particles.learn more
Heinrich Hertz1857–1894GermanFirst to produce and detect radio waves (1887), confirming Maxwell; observed the photoelectric effect. Unit: hertz.learn more
Wilhelm Röntgen1845–1923GermanDiscovered X-rays (Nov 1895); famous X-ray of his wife's hand with her ring; won the first Nobel Prize in Physics (1901). Element: roentgenium.learn more
Henri Becquerel1852–1908FrenchDiscovered radioactivity (1896) when uranium salts fogged photographic plates in a drawer; shared 1903 Nobel with the Curies. Unit: becquerel.learn more
J. J. Thomson1856–1940EnglishDiscovered the electron (1897) with cathode-ray tubes; “plum pudding” model; measured charge-to-mass ratio; Nobel 1906; Cavendish Laboratory director. Son G. P. Thomson also won a Nobel.learn more
Ernest Rutherford1871–1937New Zealander (worked in Canada & Britain)“Father of nuclear physics”; gold foil experiment → nucleus (1911); discovered the proton; named alpha and beta rays; first artificial transmutation; Nobel Prize in Chemistry (1908). Element: rutherfordium.learn more
Max Planck1858–1947GermanFounder of quantum theory (1900): energy quanta, E = hf, Planck's constant; blackbody radiation; Nobel 1918; the Max Planck Society is named for him.learn more
Albert Einstein1879–1955German-born (Swiss, later American)1905 “miracle year”: photoelectric effect, Brownian motion, special relativity, E = mc²; general relativity (1915); Nobel 1921 for the photoelectric effect; worked in the Swiss patent office; 1939 letter to FDR urging atomic research; declined Israel's presidency (1952); “God does not play dice.” Element: einsteinium.learn more
Niels Bohr1885–1962DanishBohr model of the atom (1913); complementarity and the Copenhagen interpretation; debates with Einstein; Nobel 1922 (son Aage won in 1975); escaped occupied Denmark in 1943. Element: bohrium.learn more
Erwin Schrödinger1887–1961AustrianWave equation of quantum mechanics (1926); “Schrödinger's cat” thought experiment (1935); Nobel 1933 (with Dirac); book What Is Life? (1944) inspired DNA researchers.learn more
Werner Heisenberg1901–1976GermanUncertainty principle (1927); matrix mechanics (1925); Nobel 1932; led Nazi Germany's nuclear program; subject of the play Copenhagen.learn more
Enrico Fermi1901–1954Italian-AmericanBuilt the first nuclear reactor, Chicago Pile-1 (1942); Nobel 1938 (neutron-induced radioactivity); named the neutrino; Fermi paradox (“Where is everybody?”); Fermi estimation problems. Fermilab, fermions, and fermium are named for him.learn more
J. Robert Oppenheimer1904–1967AmericanScientific director of the Manhattan Project at Los Alamos — “father of the atomic bomb”; quoted the Bhagavad Gita, “Now I am become Death, the destroyer of worlds”; security clearance revoked in 1954 (decision vacated 2022); subject of the 2023 film Oppenheimer.learn more
Richard Feynman1918–1988AmericanQuantum electrodynamics (QED) and Feynman diagrams; Nobel 1965; Manhattan Project; showed the Challenger O-ring failure with a glass of ice water (1986); bongo drums and safecracking; Surely You're Joking, Mr. Feynman!; The Feynman Lectures on Physics.learn more
Stephen Hawking1942–2018EnglishHawking radiation (black holes emit radiation, 1974); A Brief History of Time (1988); had ALS (motor neuron disease) and spoke through a speech synthesizer; Lucasian Professor at Cambridge; died on Pi Day, Einstein's birthday.learn more

Chemists

NameDatesNationalityKnown for (quiz clues)More
Robert Boyle1627–1691Anglo-IrishBoyle's law (PV constant, 1662); The Sceptical Chymist (1661) separated chemistry from alchemy; air pump experiments; founding member of the Royal Society.learn more
Henry Cavendish1731–1810EnglishDiscovered hydrogen (“inflammable air,” 1766) and showed water is H + O; measured Earth's density and G with a torsion balance (1798); extremely shy. Cambridge's Cavendish Laboratory is named for his family.learn more
Joseph Priestley1733–1804English (emigrated to Pennsylvania 1794)Discovered oxygen (1774, “dephlogisticated air”) by heating mercuric oxide; invented carbonated (soda) water; mint-and-mouse experiment; named the rubber eraser; dissenting minister whose house was burned by a mob.learn more
Carl Wilhelm Scheele1742–1786Swedish (German-born)Found oxygen (“fire air”) independently and probably first (c. 1771), but published later (1777); discovered chlorine and several acids; Scheele's green pigment; tasted his chemicals.learn more
Antoine Lavoisier1743–1794French“Father of modern chemistry”; law of conservation of mass; named oxygen and hydrogen; disproved phlogiston theory; Elementary Treatise of Chemistry (1789); helped create the metric system; guillotined in the Terror as a tax collector. Wife Marie-Anne assisted him.learn more
Jacques Charles1746–1823FrenchCharles's law (V ∝ T); built and flew the first hydrogen balloon (1783).learn more
John Dalton1766–1844EnglishModern atomic theory (1803–08); law of partial pressures; law of multiple proportions; studied his own color blindness (“Daltonism”). Unit: dalton.learn more
Amedeo Avogadro1776–1856ItalianAvogadro's hypothesis (1811): equal gas volumes at the same T and P hold equal numbers of molecules; distinguished atoms from molecules. Avogadro's number, 6.022 × 10²³, is named for him.learn more
Joseph Louis Gay-Lussac1778–1850FrenchPressure–temperature gas law; law of combining volumes (1808); record-setting hot-air/hydrogen balloon ascent (1804); co-discovered boron.learn more
Humphry Davy1778–1829EnglishUsed electrolysis to isolate sodium and potassium (1807), then calcium, magnesium, barium, strontium, boron; studied laughing gas (N₂O); invented the miners' safety lamp (1815); mentor of Faraday.learn more
Jöns Jacob Berzelius1779–1848SwedishInvented modern letter symbols for elements; discovered silicon, selenium, cerium, thorium; coined “protein,” “polymer,” “catalysis,” “isomer.”learn more
Friedrich Wöhler1800–1882GermanSynthesized urea from ammonium cyanate (1828), undermining vitalism and launching organic chemistry; isolated aluminum and beryllium.learn more
Robert Bunsen1811–1899GermanPopularized the Bunsen burner (1855); with Kirchhoff founded spectroscopy and discovered cesium (1860) and rubidium (1861).learn more
August Kekulé1829–1896GermanCarbon's four bonds (tetravalence); ring structure of benzene (1865) — said to come from a daydream of a snake biting its tail.learn more
Dmitri Mendeleev1834–1907RussianPeriodic table (1869), arranged by atomic weight with gaps for undiscovered elements — correctly predicted gallium, scandium, germanium; legend says he saw it in a dream. Element: mendelevium.learn more
William Ramsay1852–1916ScottishDiscovered the noble gases — argon (with Lord Rayleigh, 1894), helium on Earth (1895), neon, krypton, xenon (1898, with Morris Travers); Nobel 1904.learn more
Svante Arrhenius1859–1927SwedishArrhenius acid–base definition; electrolytic dissociation (Nobel 1903); Arrhenius equation for reaction rates/activation energy; first calculated CO₂'s greenhouse warming (1896).learn more
Fritz Haber1868–1934GermanHaber process (N₂ + 3H₂ → 2NH₃) for ammonia fertilizer, scaled up by Carl Bosch — “bread from air”; Nobel 1918; also directed chlorine gas attacks in WWI (“father of chemical warfare”).learn more
Gilbert N. Lewis1875–1946AmericanLewis dot structures; the covalent bond as a shared electron pair (1916); Lewis acids and bases; named the “photon”; nominated dozens of times but never won a Nobel.learn more
Otto Hahn1879–1968GermanDiscovered nuclear fission of uranium (Dec 1938, with Fritz Strassmann); sole winner of the 1944 Chemistry Nobel — his longtime partner Lise Meitner was left out.learn more
Henry Moseley1887–1915EnglishUsed X-ray spectra to show atomic number (proton count) orders the periodic table (1913); killed by a sniper at Gallipoli at age 27.learn more
Percy Julian1899–1975AmericanSynthesized physostigmine (glaucoma drug, 1935); made cortisone and sex hormones cheaply from soybeans; fire-fighting foam; first Black chemist elected to the National Academy of Sciences.learn more
Linus Pauling1901–1994AmericanThe Nature of the Chemical Bond; electronegativity scale; alpha helix of proteins; Nobel Chemistry 1954 and Nobel Peace 1962 (anti–nuclear testing) — only person with two unshared Nobels; promoted vitamin C megadoses.learn more
Glenn Seaborg1912–1999AmericanCo-discovered plutonium and nine other transuranium elements; reorganized the table with the actinide series; Nobel 1951; seaborgium was named while he was alive.learn more
Frederick Sanger1918–2013EnglishSequenced insulin, the first protein sequence (Nobel 1958); invented Sanger DNA sequencing (Nobel 1980) — one of only two people with two Chemistry Nobels.learn more

Biologists & medicine

NameDatesNationalityKnown for (quiz clues)More
Hippocratesc. 460 – c. 370 BCGreek (Kos)“Father of medicine”; Hippocratic Oath; disease has natural causes; theory of four humors.learn more
Andreas Vesalius1514–1564FlemishDe humani corporis fabrica (1543), founding modern anatomy from human dissection — corrected Galen's errors; published the same year as Copernicus's book.learn more
William Harvey1578–1657EnglishDiscovered the circulation of blood pumped by the heart (De Motu Cordis, 1628); physician to James I and Charles I.learn more
Antonie van Leeuwenhoek1632–1723Dutch“Father of microbiology”; a Delft cloth merchant who ground tiny single-lens microscopes and first saw bacteria, protists, sperm and blood cells (“animalcules,” 1670s).learn more
Carl Linnaeus1707–1778Swedish“Father of taxonomy”; binomial nomenclature; Systema Naturae (1735); named Homo sapiens; classified plants by their reproductive parts.learn more
Jean-Baptiste Lamarck1744–1829FrenchEarly evolution theory — inheritance of acquired characteristics (giraffe necks; Philosophie zoologique, 1809); helped coin “biology”; classified invertebrates.learn more
Edward Jenner1749–1823EnglishFirst vaccine (1796): inoculated James Phipps with cowpox from milkmaid Sarah Nelmes to protect against smallpox; “vaccine” comes from Latin vacca, cow. Smallpox was declared eradicated in 1980.learn more
Charles Darwin1809–1882EnglishEvolution by natural selection; HMS Beagle voyage; Galápagos finches; On the Origin of Species (1859), The Descent of Man (1871); also studied barnacles, orchids, earthworms; buried in Westminster Abbey.learn more
Ignaz Semmelweis1818–1865Hungarian“Savior of mothers”: in Vienna (1847) showed doctors' hand-washing with chlorinated lime slashed deaths from childbed (puerperal) fever; ridiculed, he died in an asylum. The “Semmelweis reflex” = rejecting new evidence.learn more
Gregor Mendel1822–1884Austrian (Moravia; now Czech Republic)“Father of genetics”; Augustinian friar (later abbot) in Brno; pea-plant experiments; laws of segregation and independent assortment (1866); rediscovered in 1900.learn more
Louis Pasteur1822–1895FrenchGerm theory; pasteurization (originally for wine and beer); swan-neck flask disproved spontaneous generation; vaccines for anthrax, chicken cholera and rabies (Joseph Meister, 1885); discovered molecular chirality; Pasteur Institute.learn more
Alfred Russel Wallace1823–1913British (Welsh-born)Co-discoverer of natural selection (1858 letter from the Malay Archipelago prompted Darwin to publish); father of biogeography — the Wallace Line between Asian and Australian fauna.learn more
Joseph Lister1827–1912EnglishAntiseptic surgery using carbolic acid (phenol), 1867, inspired by Pasteur; Listerine mouthwash is named after him.learn more
Robert Koch1843–1910GermanKoch's postulates linking a microbe to a disease; identified the bacteria causing anthrax, tuberculosis (1882) and cholera; Nobel 1905; his lab gave us agar plates and the Petri dish.learn more
Ivan Pavlov1849–1936RussianClassical conditioning — dogs salivating at a signal (bell, metronome); his Nobel (1904) was actually for research on digestion.learn more
George Washington Carverc. 1864–1943AmericanAgricultural scientist at Tuskegee Institute; crop rotation to restore Southern soils; hundreds of uses for peanuts and sweet potatoes. (Kansas) Finished high school in Minneapolis, Kansas, and homesteaded in Ness County; a Kansas college (Highland) rejected him because of his race.learn more
Thomas Hunt Morgan1866–1945AmericanFruit-fly (Drosophila) genetics in Columbia's “fly room”; proved genes are carried on chromosomes; sex-linked traits (white eyes); Nobel 1933. The centimorgan is named for him.learn more
Karl Landsteiner1868–1943Austrian-AmericanDiscovered the ABO blood groups (1901) — made safe transfusions possible; co-discovered the Rh factor and the polio virus; Nobel 1930.learn more
Elmer McCollum1879–1967American(Kansas) Born near Fort Scott, KU graduate; co-discovered vitamin A, named vitamin D, began the letter system for vitamins; started the first U.S. rat colony for nutrition research; nicknamed “Dr. Vitamin.”learn more
Alexander Fleming1881–1955ScottishDiscovered penicillin (1928) when Penicillium mold killed bacteria on a forgotten culture plate; also discovered lysozyme; Nobel 1945 with Howard Florey and Ernst Chain, who mass-produced it.learn more
Frederick Banting1891–1941CanadianCo-discovered insulin (1921, Toronto) with Charles Best, transforming diabetes treatment; Nobel 1923 at age 32 (shared with J. J. R. Macleod).learn more
Charles Drew1904–1950AmericanDeveloped methods to process and store blood plasma; ran the “Blood for Britain” program and the first American Red Cross blood bank (1941); resigned over the policy of segregating blood by race.learn more
Jonas Salk1914–1995AmericanFirst effective polio vaccine (injected, killed virus; declared safe in 1955); refused to patent it — “Could you patent the sun?” (Albert Sabin later made the oral, live-virus vaccine.)learn more
Francis Crick1916–2004EnglishCo-discovered the DNA double helix (1953) with Watson; stated the “central dogma” (1958); helped crack the triplet genetic code; Nobel 1962.learn more
James Watson1928–2025AmericanCo-discovered the DNA double helix with Crick (1953), using Rosalind Franklin's data; Nobel 1962; wrote The Double Helix (1968); first director of the Human Genome Project.learn more

Earth & space scientists

NameDatesNationalityKnown for (quiz clues)More
Aristarchus of Samosc. 310 – c. 230 BCGreekFirst known heliocentric (Sun-centered) model; estimated relative sizes and distances of the Sun and Moon.learn more
Eratosthenesc. 276 – c. 194 BCGreek (Cyrene; librarian at Alexandria)Measured Earth's circumference using shadow angles at Syene and Alexandria; sieve for primes; coined “geography.”learn more
Claudius Ptolemyc. 100 – c. 170 ADGreco-Egyptian (Alexandria)Almagest: Earth-centered (geocentric) universe with epicycles, accepted for ~1,400 years; also Geography.learn more
Nicolaus Copernicus1473–1543PolishHeliocentric model in De revolutionibus orbium coelestium (1543, published as he died) — the “Copernican Revolution”; also a church canon and economist. Element: copernicium.learn more
Tycho Brahe1546–1601DanishMost precise naked-eye observations ever, from his Uraniborg observatory on the island of Hven; saw the 1572 supernova; lost part of his nose in a duel and wore a metal prosthetic; hybrid Tychonic model; hired Kepler.learn more
Johannes Kepler1571–1630GermanThree laws of planetary motion (elliptical orbits, equal areas, T² ∝ a³) from Tycho's Mars data; Astronomia nova (1609), Harmonices Mundi (1619); Rudolphine Tables; defended his mother in a witchcraft trial. NASA's Kepler telescope found thousands of exoplanets.learn more
Edmond Halley1656–1742EnglishPredicted the return of the comet now named for him (it came back in 1758, after his death); paid to publish Newton's Principia; Astronomer Royal.learn more
James Hutton1726–1797Scottish“Father of modern geology”; uniformitarianism and deep time — “no vestige of a beginning, no prospect of an end”; the unconformity at Siccar Point.learn more
Charles Messier1730–1817FrenchComet hunter who cataloged 110 fuzzy non-comet objects (M1 = Crab Nebula, M31 = Andromeda, M42 = Orion Nebula, M45 = Pleiades).learn more
William Herschel1738–1822German-born BritishDiscovered Uranus (1781) and infrared radiation (1800); built the largest telescopes of his day; also a composer and oboist. Worked with his sister Caroline.learn more
Charles Lyell1797–1875ScottishPrinciples of Geology (1830–33) popularized uniformitarianism; strongly influenced Darwin, who read it on the Beagle.learn more
Louis Agassiz1807–1873Swiss-AmericanProposed past ice ages (glacial theory, 1837–40); studied fossil fish; founded Harvard's Museum of Comparative Zoology; opposed Darwin.learn more
Urbain Le Verrier1811–1877FrenchPredicted Neptune's position from irregularities in Uranus's orbit; Johann Galle found it within 1° (1846). (John Couch Adams made a similar prediction in England.)learn more
Alfred Wegener1880–1930GermanContinental drift and Pangaea (1912/1915); meteorologist and polar explorer; died on the Greenland ice cap; vindicated by plate tectonics in the 1960s.learn more
Edwin Hubble1889–1953AmericanShowed “spiral nebulae” like Andromeda are separate galaxies (1924, using Cepheids); Hubble's law — the universe is expanding (1929); tuning-fork galaxy classification; former lawyer and Rhodes Scholar. The Hubble Space Telescope is named for him.learn more
Georges Lemaître1894–1966BelgianCatholic priest who proposed the expanding universe (1927) and the “primeval atom” — the Big Bang theory.learn more
Charles Richter1900–1985AmericanRichter magnitude scale (1935, Caltech, with Beno Gutenberg).learn more
Harry Hess1906–1969AmericanSeafloor spreading (1962) using sonar data gathered as a U.S. Navy officer in WWII — key to plate tectonics; Princeton geologist.learn more
Clyde Tombaugh1906–1997American(Kansas) Discovered Pluto (Feb 18, 1930) at Lowell Observatory; raised on a farm near Burdett, Kansas; self-taught telescope maker; later studied at the University of Kansas; taught at New Mexico State.learn more
Subrahmanyan Chandrasekhar1910–1995Indian-AmericanChandrasekhar limit (~1.4 solar masses) for white dwarfs, worked out on a voyage to England at age 19; Nobel 1983; NASA's Chandra X-ray Observatory is named for him.learn more
Luis Alvarez (& son Walter)1911–1988 (Walter b. 1940)AmericanFather (physicist, Nobel 1968 for the bubble chamber) and son (geologist) proposed in 1980 that an asteroid impact killed the dinosaurs, based on an iridium-rich clay layer at the K–Pg boundary.learn more
Fred Hoyle1915–2001EnglishCoined “Big Bang” (1949) while defending the rival steady-state theory; explained how stars forge heavy elements (stellar nucleosynthesis); science-fiction author.learn more
Tetsuya “Ted” Fujita1920–1998Japanese-American“Mr. Tornado”: created the Fujita tornado scale (1971) at the University of Chicago; discovered microbursts/downbursts that endanger aircraft; had surveyed bomb damage at Nagasaki and Hiroshima.learn more
Arno Penzias & Robert Wilson1933–2024 / b. 1936American (Penzias born in Germany)Discovered the cosmic microwave background (1964–65) with a horn antenna at Bell Labs in New Jersey — strong evidence for the Big Bang; Nobel 1978.Penzias · Wilson
Carl Sagan1934–1996AmericanTV series Cosmos (1980); “Pale Blue Dot”; Voyager Golden Record and Pioneer plaques; novel Contact; Pulitzer for The Dragons of Eden; nuclear winter research.learn more

Inventors & engineers

NameDatesNationalityKnown for (quiz clues)More
Johannes Gutenbergc. 1400–1468German (Mainz)Movable-type printing press (c. 1440s–1450); Gutenberg Bible (c. 1455).learn more
James Watt1736–1819ScottishSeparate condenser made steam engines far more efficient (patent 1769), powering the Industrial Revolution; partnered with Matthew Boulton; coined “horsepower.” Unit: watt.learn more
Eli Whitney1765–1825AmericanCotton gin (1793) — which expanded slavery in the South; promoted interchangeable parts for muskets.learn more
Robert Fulton1765–1815AmericanFirst commercially successful steamboat, the Clermont (Hudson River, 1807); earlier built the submarine Nautilus.learn more
George Stephenson1781–1848English“Father of Railways”; Locomotion No. 1 on the Stockton and Darlington Railway (1825); the Rocket (built with son Robert) won the 1829 Rainhill Trials; standard gauge.learn more
Charles Babbage1791–1871English“Father of the computer”: Difference Engine and the programmable Analytical Engine (never completed); Ada Lovelace wrote its first program.learn more
Samuel Morse1791–1872AmericanElectric telegraph and Morse code; first long-distance message “What hath God wrought” (Washington to Baltimore, May 24, 1844); earlier a portrait painter.learn more
Cyrus McCormick1809–1884AmericanMechanical reaper (1831) that transformed grain harvesting on the Great Plains; company later part of International Harvester.learn more
Alfred Nobel1833–1896SwedishInvented dynamite (1867) by stabilizing nitroglycerin in diatomaceous earth; a premature obituary calling him the “merchant of death” reportedly led him to endow the Nobel Prizes. Element: nobelium.learn more
Karl Benz1844–1929GermanBenz Patent-Motorwagen (patented 1886), the first practical gasoline automobile; wife Bertha Benz made the first long-distance drive (1888).learn more
George Westinghouse1846–1914AmericanRailway air brake (1869); backed Tesla's alternating current and won the War of the Currents; lit the 1893 Chicago World's Fair.learn more
Alexander Graham Bell1847–1922Scottish-born (American, Canadian)Telephone patent (March 7, 1876) — filed the same day as Elisha Gray's caveat; “Mr. Watson, come here, I want to see you”; teacher of the deaf; photophone; early president of the National Geographic Society. Unit: bel/decibel.learn more
Thomas Edison1847–1931American“Wizard of Menlo Park”; phonograph (1877); practical incandescent light bulb (1879); Pearl Street power station (1882, DC); motion-picture kinetoscope; first industrial research lab; 1,093 U.S. patents; “Genius is one percent inspiration, ninety-nine percent perspiration.”learn more
Nikola Tesla1856–1943Serbian-American (born in modern Croatia)AC induction motor and polyphase AC power (with Westinghouse); Tesla coil; worked briefly for Edison, then became his rival; Wardenclyffe Tower for wireless power; died nearly broke in a New York hotel. Unit: tesla.learn more
Henry Ford1863–1947AmericanModel T (1908); moving assembly line (1913); $5 workday (1914) — made cars affordable for the middle class.learn more
Wilbur & Orville Wright1867–1912 / 1871–1948American (Dayton, Ohio)Bicycle makers who made the first controlled, sustained, powered airplane flights at Kill Devil Hills near Kitty Hawk, NC, on Dec 17, 1903 (first flight: Orville, 12 seconds, 120 ft); wing warping for control.learn more
Guglielmo Marconi1874–1937ItalianWireless telegraphy (radio); first transatlantic radio signal (1901, Cornwall to Newfoundland — the letter “S”); Nobel Physics 1909 with Karl Ferdinand Braun.learn more
Walter Chrysler1875–1940American(Kansas) Born in Wamego and raised in Ellis, Kansas, where he began as a Union Pacific railroad machinist; founded the Chrysler Corporation (1925); the Chrysler Building (1930) bears his name.learn more
Clyde Cessna1879–1954American(Kansas) Kingman County farmer and self-taught aviator who built his own monoplanes from 1911; founded Cessna Aircraft in Wichita (1927). With Beech, Stearman and later Learjet, Wichita became the “Air Capital of the World.”learn more · Wichita
Robert Goddard1882–1945AmericanLaunched the first liquid-fueled rocket (March 16, 1926, Auburn, Massachusetts); mocked by the New York Times, which printed a correction in 1969 during Apollo 11. NASA's Goddard Space Flight Center is named for him.learn more
Philo Farnsworth1906–1971AmericanInvented all-electronic television (first transmission 1927), an idea he said came to him as a teenager plowing furrows on an Idaho farm.learn more
Wernher von Braun1912–1977German-AmericanDesigned Nazi Germany's V-2 rocket; brought to the U.S. in Operation Paperclip; launched Explorer 1 (1958); chief architect of the Saturn V that carried Apollo to the Moon; directed NASA's Marshall Space Flight Center.learn more
Alan Turing1912–1954EnglishTuring machine (1936) — foundation of computer science; broke the German Enigma code at Bletchley Park; the Turing test for machine intelligence (1950); prosecuted for homosexuality, posthumously pardoned (2013); on the £50 note. The Turing Award is computing's top prize.learn more
Jack Kilby1923–2005American(Kansas) Grew up in Great Bend, Kansas; built the first integrated circuit (microchip) at Texas Instruments in 1958 (Robert Noyce independently made a silicon version); co-invented the handheld calculator; Nobel Physics 2000.learn more
Tim Berners-Leeb. 1955EnglishInvented the World Wide Web (proposal 1989, at CERN) — HTML, HTTP, URLs, the first web browser and server; knighted; Turing Award 2016. (The Internet's TCP/IP protocols were by Vint Cerf and Bob Kahn.)learn more

Women in science

NameDatesNationalityKnown for (quiz clues)More
Mary Anning1799–1847EnglishFossil hunter of Lyme Regis's “Jurassic Coast”; found the first correctly identified ichthyosaur skeleton (with her brother) and early plesiosaurs; said to inspire “She sells seashells by the seashore.”learn more
Ada Lovelace1815–1852EnglishWrote the first published computer algorithm (1843, for Babbage's Analytical Engine, computing Bernoulli numbers); daughter of poet Lord Byron; the Ada programming language is named for her.learn more
Maria Mitchell1818–1889AmericanDiscovered “Miss Mitchell's Comet” (1847) from Nantucket; first American woman professional astronomer; professor at Vassar.learn more
Florence Nightingale1820–1910EnglishFounder of modern nursing — “Lady with the Lamp” in the Crimean War; pioneering statistician whose polar-area (“coxcomb”) diagrams showed most soldiers died of preventable disease.learn more
Elizabeth Blackwell1821–1910English-AmericanFirst woman to earn a medical degree in the U.S. (Geneva Medical College, 1849).learn more
Annie Jump Cannon1863–1941AmericanHarvard “computer” who created the OBAFGKM stellar classification and classified ~350,000 stars; largely deaf.learn more
Marie Curie1867–1934Polish-French (born Maria Skłodowska, Warsaw)Coined “radioactivity”; discovered polonium (named for Poland) and radium with Pierre (1898); first woman Nobel laureate (Physics 1903) and only person to win in two sciences (Chemistry 1911); mobile X-ray units in WWI; died of aplastic anemia from radiation. Element: curium.learn more
Henrietta Swan Leavitt1868–1921AmericanHarvard computer who found the period–luminosity relation of Cepheid variable stars (1908–12) in the Magellanic Clouds — the “standard candle” Hubble used to measure galaxy distances.learn more
Lise Meitner1878–1968Austrian-SwedishWith nephew Otto Frisch, explained and named nuclear fission (1939) after fleeing Nazi Germany; excluded from Otto Hahn's 1944 Nobel; refused to work on the bomb. Element: meitnerium.learn more
Emmy Noether1882–1935GermanNoether's theorem: every symmetry of physics gives a conservation law (e.g., time symmetry → conservation of energy); founder of abstract algebra; Einstein praised her genius; fled to Bryn Mawr College in 1933.learn more
Amelia Earhart1897–1937American(Kansas) Aviation pioneer (not a scientist, but quizzable alongside aviation clues) born in Atchison, Kansas; first woman to fly solo across the Atlantic (1932); vanished near Howland Island in the Pacific (July 2, 1937) attempting to fly around the world.learn more
Cecilia Payne-Gaposchkin1900–1979English-American1925 Harvard Ph.D. thesis showed stars are made mostly of hydrogen and helium — called the most brilliant astronomy thesis ever; first woman to chair a Harvard department.learn more
Barbara McClintock1902–1992AmericanDiscovered transposons (“jumping genes”) in maize; unshared Nobel in Physiology or Medicine (1983).learn more
Grace Hopper1906–1992AmericanNavy rear admiral (“Amazing Grace”); wrote the first compiler (A-0, 1952); her work led to COBOL; popularized “bug” after a moth was found in the Harvard Mark II (1947).learn more
Rachel Carson1907–1964AmericanMarine biologist; Silent Spring (1962) on DDT's harm launched the environmental movement and led to the EPA (1970) and the U.S. DDT ban (1972).learn more
Dorothy Crowfoot Hodgkin1910–1994EnglishX-ray crystallography of penicillin, vitamin B₁₂ and insulin; Nobel Chemistry 1964.learn more
Chien-Shiung Wu1912–1997Chinese-American“First Lady of Physics”: the Wu experiment (1956, cobalt-60) showed the weak force violates parity — but the 1957 Nobel went only to theorists Lee and Yang; worked on the Manhattan Project.learn more
Katherine Johnson1918–2020AmericanNASA “human computer” who calculated trajectories for Alan Shepard's flight and checked the computer's numbers for John Glenn's orbit (1962) and Apollo 11; featured in Hidden Figures with Dorothy Vaughan and Mary Jackson; Presidential Medal of Freedom (2015).learn more
Rosalind Franklin1920–1958EnglishX-ray diffraction images of DNA, including Photo 51, crucial to the double-helix model; also studied virus and coal structure; died of ovarian cancer at 37, before the 1962 Nobel.learn more
Marie Tharp1920–2006AmericanMapped the ocean floor with Bruce Heezen and found the rift valley along the Mid-Atlantic Ridge (early 1950s) — evidence for continental drift.learn more
Vera Rubin1928–2016AmericanGalaxy rotation curves (with Kent Ford, 1970s) — strong evidence for dark matter; the Vera C. Rubin Observatory in Chile is named for her.learn more
Jane Goodall1934–2025EnglishSix decades studying wild chimpanzees at Gombe Stream, Tanzania (from 1960); discovered tool use (termite fishing) and meat eating; protégée of Louis Leakey.learn more
Jocelyn Bell Burnellb. 1943Northern IrishDiscovered the first pulsars (1967) as a graduate student (signal nicknamed “LGM-1,” Little Green Men); the 1974 Nobel went to her supervisor Antony Hewish.learn more
Sally Ride1951–2012AmericanPhysicist and first American woman in space (STS-7, June 1983); served on the Challenger and Columbia accident boards.learn more
Jennifer Doudna & Emmanuelle Charpentierb. 1964 / b. 1968American / FrenchDeveloped CRISPR-Cas9 gene editing (2012); Nobel Chemistry 2020 — the first science Nobel shared only by women.Doudna · Charpentier

Many “overlooked women” clues end with the man who got the credit: Franklin → Watson & Crick; Meitner → Hahn; Wu → Lee & Yang; Bell Burnell → Hewish; Leavitt → Hubble. If a clue stresses a missed Nobel, think of these pairs. Matilda effect

Famous Experiments

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Listed roughly in chronological order. Tossups often describe the apparatus (“oil droplets between charged plates,” “a flask with a curved neck”) and ask for the scientist or the result. learn more

ExperimentWho / whenWhat was doneWhat it showedMore
Measuring the EarthEratosthenes, c. 240 BCAt noon on the summer solstice the Sun was overhead at Syene (a well's bottom was lit) but cast a ~7.2° shadow at Alexandria — 1/50 of a circle.Earth's circumference ≈ 50 × the Syene–Alexandria distance (~250,000 stadia) — remarkably close.learn more
Inclined planes & the Leaning TowerGalileo, c. 1590s–1630sRolled balls down ramps, timing them (with water clocks); the story of dropping balls from the Leaning Tower of Pisa comes from his pupil Viviani and is probably legend.Falling objects accelerate uniformly; distance ∝ time²; heavy and light objects fall together (contradicting Aristotle). Apollo 15's hammer and feather confirmed it on the Moon (1971).learn more
Torricelli's barometerEvangelista Torricelli, 1643Filled a glass tube with mercury and inverted it in a dish; the column fell to ~76 cm, leaving a vacuum on top.Air has pressure (1 atm = 760 mmHg) and a vacuum can exist; invented the barometer. Unit: torr.learn more
Magdeburg hemispheresOtto von Guericke, 1654Pumped the air out of two joined copper hemispheres; teams of horses could not pull them apart.The enormous force of atmospheric pressure; demonstrated his vacuum pump.learn more
Prism experimentsIsaac Newton, 1666 (published 1672)Split sunlight with a prism, then used a second prism to show a single color could not be split further (the experimentum crucis).White light is a mixture of colors; color is a property of light.learn more
Redi's fliesFrancesco Redi, 1668Meat in open jars got maggots; meat in jars covered with gauze did not.First experimental challenge to spontaneous generation of larger organisms.learn more
Kite experimentBenjamin Franklin, 1752 (Philadelphia)Flew a kite in a thunderstorm with a key on the string; sparks jumped from the key (he was not struck by lightning).Lightning is electricity → the lightning rod.learn more
Smallpox vaccinationEdward Jenner, 1796Infected 8-year-old James Phipps with cowpox, then exposed him to smallpox.Cowpox gives immunity to smallpox — the first vaccine.learn more
Cavendish experimentHenry Cavendish, 1797–98Torsion balance: large lead balls slightly twisted a rod holding small balls.Measured the gravitational force between masses → G and Earth's density (~5.4× water) — “weighing the Earth.”learn more
Double-slit experimentThomas Young, c. 1801–1803Light through two narrow slits produced alternating bright and dark bands (interference fringes).Light is a wave. Repeated with single electrons in the 20th century, it shows quantum wave–particle duality.learn more
Ørsted's compassHans Christian Ørsted, 1820A wire carrying current deflected a nearby compass needle.Electric currents create magnetic fields — birth of electromagnetism.learn more
Joule's paddle wheelJames Prescott Joule, 1840sA falling weight turned paddles in insulated water; he measured the tiny temperature rise.The mechanical equivalent of heat — work and heat are interchangeable forms of energy (first law of thermodynamics).learn more
Foucault pendulumLéon Foucault, 1851 (Panthéon, Paris)A heavy bob on a 67 m wire swung while its plane of swing slowly rotated.Direct visible proof that Earth rotates.learn more
Mendel's peasGregor Mendel, 1856–1863Crossed thousands of pea plants for seven traits and counted offspring (3 : 1 ratios).Heredity comes in discrete units (genes); laws of segregation and independent assortment.learn more
Swan-neck flaskLouis Pasteur, 1859–1862Boiled broth in flasks with long S-curved necks that let in air but trapped dust; broth stayed sterile until the neck was broken.Disproved spontaneous generation; supported germ theory.learn more
Michelson–Morley experimentAlbert Michelson & Edward Morley, 1887 (Cleveland)An interferometer compared light speed in perpendicular directions as Earth moved.No difference — no “luminiferous aether”; paved the way for special relativity. The most famous “failed” experiment.learn more
Pavlov's dogsIvan Pavlov, 1890s–1900sPaired a neutral stimulus (e.g., a metronome or bell) with food; dogs began salivating to the stimulus alone.Classical conditioning.learn more
Cathode-ray tubeJ. J. Thomson, 1897Deflected cathode rays with electric and magnetic fields and measured their charge-to-mass ratio.Discovered the electron, the first subatomic particle.learn more
Oil-drop experimentRobert Millikan (with Harvey Fletcher), 1909Balanced tiny charged oil droplets between charged plates by adjusting the voltage.Charge is quantized; measured the electron's charge (e ≈ 1.6 × 10⁻¹⁹ C). Nobel 1923.learn more
Gold foil experimentHans Geiger & Ernest Marsden under Ernest Rutherford, 1909 (interpreted 1911)Fired alpha particles at thin gold foil; most passed through, but a few bounced back — “as if you fired a 15-inch shell at a piece of tissue paper and it came back and hit you.”Atoms have a tiny, dense, positive nucleus; mostly empty space. Overturned the plum-pudding model.learn more
Eddington's eclipse expeditionArthur Eddington and others, 1919 (Príncipe and Sobral, Brazil)Photographed stars near the Sun during a total solar eclipse.Starlight bends around the Sun by the amount general relativity predicts — made Einstein world-famous.learn more
Griffith's experimentFrederick Griffith, 1928Heat-killed virulent pneumonia bacteria mixed with live harmless bacteria made mice die.A “transforming principle” passes genetic information (later shown to be DNA by Avery, 1944).learn more
Chicago Pile-1Enrico Fermi and team, Dec 2, 1942 (University of Chicago, under the stands of Stagg Field)Stacked graphite blocks and uranium; pulled out cadmium control rods.First human-made self-sustaining nuclear chain reaction. Coded message: “The Italian navigator has landed in the new world.”learn more
Trinity testManhattan Project (Oppenheimer), July 16, 1945Detonated “the Gadget,” a plutonium implosion bomb, in the New Mexico desert (Jornada del Muerto, near Alamogordo).First nuclear explosion (~20+ kilotons); ushered in the Atomic Age.learn more
Hershey–Chase experimentAlfred Hershey & Martha Chase, 1952Labeled bacteriophage protein with ³⁵S and DNA with ³²P, let them infect bacteria, then separated them in a kitchen blender.Only the DNA entered the bacteria — DNA is the genetic material.learn more
Miller–Urey experimentStanley Miller & Harold Urey, 1952 (published 1953)Ran electric sparks (“lightning”) through methane, ammonia, hydrogen and water vapor (“primordial soup”).Produced amino acids — life's building blocks can form from simple chemicals.learn more
Wu experimentChien-Shiung Wu, 1956Measured the direction of electrons emitted by cobalt-60 nuclei aligned in a magnetic field near absolute zero.The weak force does not conserve parity (mirror symmetry).learn more
Meselson–Stahl experimentMatthew Meselson & Franklin Stahl, 1958Grew E. coli on heavy nitrogen (¹⁵N), switched to ¹⁴N, and separated DNA by density in a centrifuge.DNA replication is semiconservative. Called “the most beautiful experiment in biology.”learn more
LIGO detectionLIGO team, Sept 14, 2015 (announced 2016)Laser interferometers in Louisiana and Washington measured a stretch of space smaller than a proton.First direct detection of gravitational waves, from two merging black holes; Nobel 2017.learn more

Rutherford directed the gold foil experiment but Geiger and Marsden performed it. Millikan measured the electron's charge; Thomson measured its charge-to-mass ratio. Pasteur (swan-neck flask, 1859) and Redi (meat and flies, 1668) both attacked spontaneous generation — Redi for maggots, Pasteur for microbes. spontaneous generation

Nobel Prizes & Named Laws

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The Nobel Prizes

Multiple / notable winnersPrizesMore
Marie CuriePhysics 1903 (with Pierre Curie & Henri Becquerel, radioactivity) and Chemistry 1911 (alone, discovering polonium and radium) — first woman laureate; only person to win in two different sciences.learn more
Linus PaulingChemistry 1954 (chemical bond) and Peace 1962 (campaign against nuclear testing) — only person with two unshared Nobels.learn more
John BardeenPhysics 1956 (the transistor, with Shockley and Brattain at Bell Labs) and Physics 1972 (BCS theory of superconductivity) — only person with two Physics prizes.learn more
Frederick SangerChemistry 1958 (structure of insulin) and Chemistry 1980 (DNA sequencing). (K. Barry Sharpless later also won Chemistry twice, 2001 and 2022.)learn more
International Committee of the Red CrossPeace 1917, 1944, 1963 — the most Peace prizes.learn more
Curie familyMarie and Pierre; daughter Irène Joliot-Curie and her husband Frédéric Joliot (Chemistry 1935, artificial radioactivity) — five Nobel Prizes among four family members.learn more
Father–son pairsThe Braggs (shared Physics 1915; Lawrence Bragg was 25); Niels (1922) & Aage Bohr (1975); J. J. (1906) & G. P. Thomson (1937).learn more
Albert EinsteinPhysics 1921 (awarded in 1922) — for the photoelectric effect, not relativity.learn more
(Kansas) Kansas-connected laureatesJack Kilby (Physics 2000, integrated circuit; grew up in Great Bend); Earl W. Sutherland Jr. (Physiology or Medicine 1971, how hormones act through cyclic AMP; born in Burlingame, Kansas, Washburn graduate); Vernon L. Smith (Economics 2002, experimental economics; born in Wichita).Kilby · Sutherland · Smith

Rutherford's Nobel was in Chemistry, Pavlov's was for digestion, and Einstein's was for the photoelectric effect — three favorite trick clues. Rutherford · Pavlov

Laws & principles named after people

Law / principleFieldIn a nutshellMore
Archimedes' principleFluidsBuoyant force = weight of displaced fluidlearn more
Pascal's principleFluidsPressure on an enclosed fluid is transmitted equally everywhere (hydraulics)learn more
Bernoulli's principleFluidsFaster-moving fluid has lower pressurelearn more
Hooke's lawMechanicsF = −kx for springslearn more
Newton's lawsMechanicsInertia; F = ma; action–reaction; universal gravitationlearn more
Kepler's lawsAstronomyElliptical orbits; equal areas; T² ∝ a³learn more
Hubble's lawCosmologyv = H₀d — galaxies recede in proportion to distancelearn more
Snell's lawOpticsn₁ sin θ₁ = n₂ sin θ₂learn more
Doppler effectWavesFrequency shifts with relative motion of source and observerlearn more
Ohm's lawElectricityV = IRlearn more
Coulomb's lawElectricityF = kq₁q₂/r²learn more
Kirchhoff's circuit lawsElectricityCurrent into a junction = current out; loop voltages sum to zerolearn more
Faraday's lawMagnetismA changing magnetic flux induces a voltagelearn more
Lenz's lawMagnetismInduced current opposes the change that caused itlearn more
Boyle's lawGasesP₁V₁ = P₂V₂ (constant T)learn more
Charles's lawGasesV₁/T₁ = V₂/T₂ (constant P)learn more
Gay-Lussac's lawGasesP₁/T₁ = P₂/T₂ (constant V)learn more
Avogadro's lawGasesEqual volumes of gas (same T, P) contain equal numbers of moleculeslearn more
Dalton's lawGasesTotal pressure = sum of partial pressureslearn more
Graham's lawGasesEffusion rate ∝ 1/√(molar mass)learn more
Henry's lawSolutionsGas solubility ∝ its partial pressure (why soda fizzes when opened; “the bends”)learn more
Le Chatelier's principleEquilibriumA system at equilibrium shifts to relieve an applied stresslearn more
Hess's lawThermochemistryTotal enthalpy change is the same regardless of the reaction path (Germain Hess, 1840)learn more
Hund's ruleElectron configurationElectrons fill equal-energy orbitals singly before pairinglearn more
Pauli exclusion principleQuantumNo two electrons share all four quantum numberslearn more
Heisenberg uncertainty principleQuantumCan't know position and momentum exactly at once: Δx·Δp ≥ ħ/2learn more
Mendel's lawsGeneticsSegregation, independent assortment, dominancelearn more
Hardy–Weinberg principleGeneticsAllele frequencies stay constant without evolutionary forces: p² + 2pq + q² = 1learn more
Steno's law of superpositionGeologyIn undisturbed strata, lower layers are olderlearn more
Moore's lawTechnologyTransistors on a chip double about every two years (Gordon Moore, Intel, 1965/1975)learn more

If a clue says “this man's law” and mentions a gas, think Boyle (P–V), Charles (V–T), Gay-Lussac (P–T), Avogadro (V–n), Dalton (partial pressures), Graham (effusion), or Henry (solubility). If it mentions electrons in orbitals, think Aufbau, Hund, or Pauli. Aufbau