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
↑ topDistance vs. displacement, speed vs. velocity
- Scalar = magnitude only (distance, speed, mass, time, energy). Vector = magnitude and direction (displacement, velocity, acceleration, force, momentum). learn more
- Distance is the total path length; displacement is the straight-line change in position (start to finish, with direction). Run one lap of a 400 m track: distance 400 m, displacement 0. learn more
- Average speed = distance / time; average velocity v = Δx / Δt (displacement / time). Often written simply v = d/t. SI unit: m/s. speed · velocity
- Acceleration is the rate of change of velocity: a = Δv / t = (v − v₀)/t, unit m/s². Speeding up, slowing down (“deceleration”), or changing direction are all accelerations. learn more
- Graphs: the slope of a position–time graph is velocity; the slope of a velocity–time graph is acceleration; the area under a velocity–time graph is displacement. learn more
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
| Equation | Missing variable | More |
|---|---|---|
| v = v₀ + at | d | learn more |
| d = v₀t + ½at² | v | learn more |
| v² = v₀² + 2ad | t | learn more |
| d = ½(v₀ + v)t | a | learn 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
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
- Horizontal and vertical motion are independent: horizontal velocity stays constant (no air resistance); vertical motion is free fall. The path is a parabola. learn more
- A bullet fired horizontally and a bullet dropped from the same height hit level ground at the same time. learn more
- Launched at speed v₀ and angle θ over level ground: components vₓ = v₀ cos θ, vy = v₀ sin θ; time of flight 2v₀ sin θ / g; range R = v₀² sin 2θ / g. Maximum range at 45°; complementary angles (30° and 60°) give equal ranges. learn more
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
↑ topNewton'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
| Law | Statement | Example / clue | More |
|---|---|---|---|
| 1st — inertia | An 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 = ma | Net 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–reaction | For 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
- Weight is the gravitational force on a mass: W = mg. A 50 kg student weighs 50 × 9.8 = 490 N (≈ 110 lb). learn more
- The normal force is the perpendicular push of a surface (equals mg on level ground). learn more
- Friction: f = μN (μ = coefficient of friction, unitless). Static friction (not yet sliding) is usually greater than kinetic (sliding) friction — that's why it's harder to start a box moving than to keep it moving. Rolling friction is smaller still. learn more
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
- Momentum p = mv (kg·m/s), a vector. learn more
- Impulse J = FΔt = Δp. Spreading a stop over more time lowers the force — air bags, crumple zones, bending your knees when you land, “following through” in sports. learn more
- Conservation of momentum: in a closed system with no external force, total momentum before = total momentum after. learn more
- Elastic collisions conserve momentum and kinetic energy (billiard balls, approximately); inelastic collisions conserve only momentum; perfectly inelastic = objects stick together. Example: 2 kg cart at 3 m/s hits a stationary 1 kg cart and they stick → v = 6/3 = 2 m/s. learn more · elastic
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
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
- Pressure P = F/A; SI unit the pascal (1 Pa = 1 N/m²). Snowshoes spread force over a large area; a knife edge concentrates it. Atmospheric pressure at sea level: 1 atm = 101,325 Pa = 101.3 kPa = 760 mmHg (torr) = 14.7 psi ≈ 1.013 bar. learn more · atm
- Fluid pressure increases with depth: P = ρgh. About every 10 m of seawater adds 1 atm. learn more
- Density ρ = m/V. Water ≈ 1 g/cm³ = 1 g/mL = 1000 kg/m³ (max density at about 4 °C — ice floats because it is ~9% less dense than liquid water). Densest element: osmium (≈ 22.6 g/cm³, with iridium a near tie); least dense: hydrogen. Densest planet: Earth; least dense: Saturn. learn more · osmium
- Archimedes' principle: the buoyant force on a submerged object equals the weight of the fluid it displaces. An object floats if it is less dense than the fluid. Legend: Archimedes shouted “Eureka!” (“I have found it!”) in his bath when he realized how to test King Hiero II's gold crown. learn more · Eureka
- Pascal's principle: pressure applied to an enclosed fluid is transmitted undiminished throughout it — the basis of hydraulic lifts and brakes (F₁/A₁ = F₂/A₂). learn more
- Bernoulli's principle (1738): where a fluid flows faster, its pressure is lower. Used to explain lift on wings, curveballs, atomizers, and shower curtains blowing inward. learn more
“Eureka,” “crown,” “displaced water” → Archimedes / buoyancy. “Hydraulic press” → Pascal. “Airplane wing lift,” “fast fluid = low pressure” → Bernoulli. learn more
Work, Energy & Power
↑ topWork
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
| Type | Formula | Notes | More |
|---|---|---|---|
| Kinetic (motion) | KE = ½mv² | Double the speed → 4× the KE (why highway crashes are so much worse). 2 kg at 3 m/s → 9 J. | learn more |
| Gravitational potential | PE = mgh | Depends on height above a chosen reference level. | learn more |
| Elastic potential | PE = ½kx² | Stored in a stretched/compressed spring (Hooke's law). | learn more |
| Mass–energy | E = mc² | Einstein, 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
| Unit | Value | Used for | More |
|---|---|---|---|
| joule (J) | 1 N·m = 1 kg·m²/s² | SI unit of energy/work/heat (James Prescott Joule) | learn more |
| calorie (cal) | 4.184 J | Heat to raise 1 g of water by 1 °C | learn more |
| food Calorie (Cal, kcal) | 1000 cal = 4184 J | Nutrition labels (capital C) | learn more |
| kilowatt-hour (kWh) | 3.6 × 10⁶ J | Electric bills (power × time — an energy unit, not power) | learn more |
| electronvolt (eV) | 1.602 × 10⁻¹⁹ J | Atomic & particle physics (energy gained by one electron through 1 V) | learn more |
| British thermal unit (BTU) | ≈ 1055 J | Heat to raise 1 lb of water by 1 °F; furnaces & air conditioners | learn more |
| erg | 10⁻⁷ J | Old 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
- Mechanical advantage MA = output force / input force. Ideal MA = input distance / output distance. Inclined plane: IMA = length / height. Pulley system: IMA ≈ number of supporting rope segments. Wheel and axle: IMA = wheel radius / axle radius. learn more
- Archimedes on the lever: “Give me a place to stand, and I shall move the Earth.” learn more
| Lever class | In the middle | Examples | More |
|---|---|---|---|
| 1st class | Fulcrum | Seesaw, crowbar, scissors, pliers | learn more |
| 2nd class | Load (resistance) | Wheelbarrow, nutcracker, bottle opener | learn more |
| 3rd class | Effort | Tweezers, 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
↑ topWave basics
- Frequency is measured in hertz (Hz = cycles per second), named for Heinrich Hertz. Example: a 340 Hz sound in air (343 m/s) has λ ≈ 1 m. learn more · frequency
- Transverse waves vibrate perpendicular to travel (light, waves on a string, S-waves). Longitudinal (compression) waves vibrate parallel to travel (sound, P-waves) — made of compressions and rarefactions. transverse · longitudinal
- Parts: crest, trough, amplitude (height — relates to energy/loudness/brightness), wavelength (crest to crest). learn more
- Wave behaviors: reflection (bounce), refraction (bend on changing speed), diffraction (spread around obstacles/through openings), interference (constructive/destructive), standing waves (nodes & antinodes), resonance (Tacoma Narrows Bridge collapse, 1940, is the classic — though imperfect — example). interference · diffraction · resonance
Sound
- Sound is a mechanical, longitudinal wave — it needs a medium and cannot travel through a vacuum. learn more
- Speed of sound: about 343 m/s in dry air at 20 °C (≈ 767 mph, ≈ 1125 ft/s), faster in warmer air; about 1,480 m/s in water and about 5,000–6,000 m/s in steel. Generally solids > liquids > gases. learn more
- Lightning rule of thumb: count seconds from flash to thunder; ÷ 3 ≈ km, ÷ 5 ≈ miles. learn more
- Pitch ↔ frequency; loudness ↔ amplitude, measured in decibels (dB, a log scale named for Alexander Graham Bell: +10 dB = 10× intensity). Human hearing: about 20 Hz to 20,000 Hz; below = infrasound (elephants, whales), above = ultrasound (bats, dolphins, medical imaging). decibel · hearing range
- Mach number = speed ÷ speed of sound (Ernst Mach). Chuck Yeager first broke the sound barrier in level flight in the Bell X-1 on Oct 14, 1947; a sonic boom is the shock wave. Mach · Bell X-1
- Echolocation/sonar; the musical note A above middle C = 440 Hz (concert pitch); doubling frequency raises pitch one octave. A440
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
| Band | Wavelength (approx.) | Uses / facts | More |
|---|---|---|---|
| Radio | > 1 m (up to km) | AM/FM, TV; predicted by Maxwell, produced by Hertz (1887); Marconi's wireless | learn more |
| Microwave | 1 mm – 1 m | Microwave ovens (2.45 GHz), radar, Wi-Fi, cell phones, cosmic microwave background | learn more |
| Infrared | ~700 nm – 1 mm | Heat radiation, remote controls, night vision, JWST; discovered by William Herschel (1800) | learn more |
| Visible | ~400 – 700 nm | ROYGBIV — red ~700 nm to violet ~400 nm | learn more |
| Ultraviolet | ~10 – 400 nm | Sunburn, vitamin D, black lights, sterilization; blocked mostly by ozone; discovered by Johann Ritter (1801) | learn more |
| X-ray | ~0.01 – 10 nm | Medical imaging, crystallography; discovered by Wilhelm Röntgen (1895) | learn more |
| Gamma ray | < ~0.01 nm | Nuclear 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
- ROYGBIV: Red, Orange, Yellow, Green, Blue, Indigo, Violet. Red has the longest wavelength and lowest energy; violet the shortest and highest. “Roy G. Biv.” Newton split sunlight with a prism and named seven colors (adding indigo to match the seven notes of the scale). learn more
- Additive primaries (light, screens): red, green, blue → together make white. Subtractive primaries (ink, pigment): cyan, magenta, yellow (+ black = CMYK). additive · subtractive
- The sky is blue because of Rayleigh scattering (short wavelengths scatter more, ∝ 1/λ⁴); sunsets are red for the same reason. learn more
- Rainbows: refraction + dispersion + internal reflection in raindrops; red on the outside of the primary bow; seen with the Sun behind you at ~42°. learn more
- Polarization (light vibrating in one plane) proves light is a transverse wave; used in sunglasses and LCD screens. learn more
Reflection, refraction & Snell's law
- Law of reflection: angle of incidence = angle of reflection (measured from the normal). learn more
- Index of refraction n = c/v: vacuum 1 (air ≈ 1.0003), water 1.33, glass ~1.5, diamond 2.42 (why diamonds sparkle). learn more
- Snell's law: n₁ sin θ₁ = n₂ sin θ₂. Light bends toward the normal entering a slower (higher-n) medium. Named for Dutch astronomer Willebrord Snellius (1621); first described by Ibn Sahl (984). learn more
- Total internal reflection occurs when light going from high n to low n exceeds the critical angle (sin θc = n₂/n₁; about 49° for water→air) — fiber optics, diamond brilliance, mirages are related. learn more
- Dispersion: n depends on wavelength, so a prism spreads white light into colors (violet bends most). learn more
Lenses & mirrors
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
| Converging | Diverging | More | |
|---|---|---|---|
| Lenses | Convex (thicker in middle) — magnifying glass, camera, eye, corrects farsightedness (hyperopia) | Concave (thinner in middle) — corrects nearsightedness (myopia) | learn more |
| Mirrors | Concave — makeup/shaving mirror, flashlight reflector, reflecting telescope | Convex — car side mirror (“objects are closer than they appear”), store security mirror | learn 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
↑ topCharge & Coulomb's law
- Like charges repel, opposite charges attract. Charge is conserved and quantized in units of the elementary charge e = 1.602 × 10⁻¹⁹ C (electron −e, proton +e). Measured by Millikan's oil-drop experiment (1909). learn more · elementary charge
- Benjamin Franklin named the charges positive and negative; because of his choice, electrons are negative and conventional current flows opposite to electron flow. learn more
- Coulomb's law (1785): F = k q₁q₂ / r², k ≈ 8.99 × 10⁹ N·m²/C² — another inverse-square law, measured with a torsion balance. learn more
- Electron mass ≈ 9.109 × 10⁻³¹ kg; a proton is about 1836× heavier. learn more
- Conductors (metals — silver is the best, copper common) vs. insulators (rubber, glass, plastic) vs. semiconductors (silicon, germanium). Superconductors have zero resistance below a critical temperature (discovered by Heike Kamerlingh Onnes in mercury, 1911). A Faraday cage shields its interior from external electric fields. conductors · superconductivity · Faraday cage
Circuits: Ohm's law & electric power
- Ohm's law (Georg Ohm, 1827): voltage = current × resistance. Example: a 12 V battery across 4 Ω → I = 3 A, P = 36 W. learn more
- Electric power P = IV. A 1200 W hair dryer on 120 V draws 10 A. learn more
- Resistance of a wire R = ρL/A: longer and thinner wires resist more; resistance usually rises with temperature in metals. learn more
| Series | Parallel | More | |
|---|---|---|---|
| Resistors | R = R₁ + R₂ + … | 1/R = 1/R₁ + 1/R₂ + … (two resistors: R₁R₂/(R₁+R₂)) | learn more |
| Current | Same through every component | Splits among branches | Kirchhoff's laws |
| Voltage | Splits among components | Same across every branch | learn more |
| Example | Two 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
| Unit | Measures | Named for | More |
|---|---|---|---|
| volt (V) | Potential difference / EMF (J/C) | Alessandro Volta (Italy) | learn more |
| ampere (A) | Current (C/s) — SI base unit | André-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) | Inductance | Joseph 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
- Magnets have north and south poles; like poles repel. Cutting a magnet makes two smaller magnets — no isolated magnetic monopole has been found. Ferromagnetic metals: iron, nickel, cobalt (and some rare earths like neodymium, gadolinium). Earth's geographic North Pole is near a magnetic south pole (that's why a compass's north end points there). William Gilbert, De Magnete (1600): Earth is a giant magnet. learn more · Earth's field
- Hans Christian Ørsted (1820) noticed an electric current deflects a compass needle — the first link between electricity and magnetism. learn more
- Right-hand rule: point your right thumb along conventional current, and your fingers curl in the direction of the magnetic field around the wire. For force on a moving positive charge (F = qvB sin θ, the Lorentz force), fingers along v, curl toward B, thumb gives F (reverse for electrons). learn more · Lorentz force
- Faraday's law of induction (Michael Faraday, 1831; Joseph Henry independently): a changing magnetic flux induces a voltage (EMF), ε = −N ΔΦ/Δt. Basis of generators, transformers, induction stoves. learn more
- Lenz's law (Heinrich Lenz, 1834): the induced current opposes the change that produced it (the minus sign in Faraday's law). learn more
- Motors turn electrical energy into motion; generators (dynamos) turn motion into electricity. Faraday built the first electric motor (1821) and the first dynamo (Faraday disk, 1831). motor · generator
- Maxwell's equations (James Clerk Maxwell, 1860s) unify electricity, magnetism, and light: light is an electromagnetic wave. learn more
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”
- DC (direct current) flows one way — batteries, electronics, solar cells. Thomas Edison championed DC (Pearl Street Station, New York, 1882). DC · Pearl Street
- AC (alternating current) reverses direction — 60 Hz, ~120 V in U.S. homes (50 Hz, 230 V in much of the world). Nikola Tesla's polyphase AC system and induction motor were backed by George Westinghouse. AC · mains electricity
- The War of the Currents (late 1880s–1890s): Edison's camp publicized AC's dangers (including electrocuting animals, and AC was used in the first electric chair, 1890). AC won — Westinghouse lit the 1893 Chicago World's Columbian Exposition and built the Niagara Falls hydroelectric plant (1895–96). learn more
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
↑ topTemperature scales
| Reference point | °F | °C | K | More |
|---|---|---|---|---|
| Absolute zero | −459.67 | −273.15 | 0 | learn more |
| F and C are equal | −40 | −40 | 233.15 | learn more |
| Water freezes | 32 | 0 | 273.15 | learn more |
| Room temperature (approx.) | 68–72 | 20–22 | ≈ 293–295 | learn more |
| Normal body temperature | 98.6 | 37 | 310.15 | learn more |
| Water boils (1 atm) | 212 | 100 | 373.15 | learn more |
- Fahrenheit — Daniel Gabriel Fahrenheit (1724), also invented the mercury thermometer (1714). Celsius — Anders Celsius (1742); his original scale was inverted (100 = freezing). Kelvin — William Thomson, Lord Kelvin (1848); the absolute scale uses no degree sign (“300 kelvins,” not “300 °K”). Rankine = absolute Fahrenheit. Celsius · kelvin · Rankine
- A change of 1 °C = a change of 1 K = a change of 1.8 °F. learn 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
- Specific heat c = heat needed to raise 1 g by 1 °C. Water: 4.184 J/(g·°C) = 1 cal/(g·°C) — unusually high, which is why oceans moderate climate and coastal cities have milder weather. Metals are low (iron ≈ 0.45 J/g·°C). Example: heating 200 g of water from 20 °C to 70 °C takes 200 × 4.184 × 50 ≈ 41,800 J. learn more
- Latent heat is absorbed or released during a phase change at constant temperature. Water: heat of fusion 334 J/g (80 cal/g); heat of vaporization 2,260 J/g (540 cal/g). Steam burns are worse than boiling-water burns because condensing steam releases this latent heat. Joseph Black discovered latent heat (c. 1760s). learn more
- A calorimeter measures heat flow; heat lost by the hot object = heat gained by the cold one. learn more
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
| Mode | How | Examples | More |
|---|---|---|---|
| Conduction | Direct contact; particle collisions (best in metals) | Hot pan handle; cold tile floor feels colder than carpet | learn more |
| Convection | Bulk movement of a fluid (hot fluid rises) | Boiling water, sea breezes, mantle convection, radiators | learn more |
| Radiation | Electromagnetic waves (mostly infrared); needs no medium | Sunlight reaching Earth through space; campfire warmth | learn 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
| Law | Statement | Clues | More |
|---|---|---|---|
| Zeroth | If 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 |
| First | Energy 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 |
| Second | The 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 |
| Third | As 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
↑ topAtomic models, in order
| Year | Scientist | Model / nickname | Key evidence or idea | More |
|---|---|---|---|---|
| c. 400s BC | Democritus (& Leucippus) | atomos (“uncuttable”) | Philosophical idea that matter is made of indivisible particles. | learn more |
| 1803–1808 | John Dalton | Solid sphere / “billiard ball” | Atomic theory: elements are made of identical atoms that combine in whole-number ratios; law of multiple proportions. | learn more |
| 1897 / 1904 | J. J. Thomson | Plum pudding | Discovered the electron with cathode-ray tubes (1897); electrons embedded in a positive “pudding.” | learn more |
| 1909–1911 | Ernest Rutherford | Nuclear (planetary) model | Gold foil experiment (done by Geiger & Marsden): a few alpha particles bounced back → tiny, dense, positive nucleus; atom mostly empty space. | learn more |
| 1913 | Niels Bohr | Bohr model | Electrons 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 cloud | Electrons described by wave functions; orbitals (s, p, d, f) give probability, not paths. | learn more |
| 1932 | James 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
- Planck (1900): energy comes in quanta E = hf — solved the blackbody “ultraviolet catastrophe.” Considered the birth of quantum theory. learn more
- Photoelectric effect: light above a threshold frequency ejects electrons from metal; brighter light gives more electrons, higher frequency gives faster ones. KEmax = hf − φ (φ = work function). Explained by Einstein (1905) using photons — the work cited for his 1921 Nobel Prize, not relativity. learn more
- de Broglie (1924): matter has waves too, λ = h/p = h/mv. Confirmed by electron diffraction (Davisson–Germer, 1927). learn more
- Heisenberg uncertainty principle (1927): position and momentum can't both be known exactly, Δx·Δp ≥ ħ/2 (ħ = h/2π). learn more
- Schrödinger equation (1926) governs wave functions; Schrödinger's cat (1935) thought experiment mocks superposition. learn more
- Pauli exclusion principle (1925): no two electrons in an atom share all four quantum numbers (n, l, ml, ms) → at most 2 electrons per orbital, with opposite spins. learn more
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
| Decay | Particle | Change to nucleus | Stopped by | More |
|---|---|---|---|---|
| Alpha (α) | Helium-4 nucleus (2p + 2n), charge +2 | Mass 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 proton | Mass number same, atomic number +1. ¹⁴C → ¹⁴N + e⁻ | Thin aluminum, plastic | learn more |
| Beta-plus (β⁺) | Positron (antielectron); a proton becomes a neutron | Atomic number −1 (used in PET scans) | Thin metal | learn more |
| Gamma (γ) | High-energy photon | No change in A or Z (nucleus drops to lower energy) | Thick lead or concrete (most penetrating) | learn more |
Half-life
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
| Isotope | Half-life | Use / note | More |
|---|---|---|---|
| Carbon-14 | ≈ 5,730 years | Radiocarbon dating of once-living things (up to ~50,000 yr); Willard Libby, Nobel 1960 | learn more |
| Uranium-238 | ≈ 4.5 billion years | About the age of the Earth; dating rocks | learn more |
| Uranium-235 | ≈ 704 million years | Fissile fuel for reactors and the Hiroshima bomb | learn more |
| Potassium-40 | ≈ 1.25 billion years | Potassium–argon dating of volcanic rock; makes bananas slightly radioactive | learn more |
| Plutonium-239 | ≈ 24,100 years | Nagasaki bomb, Trinity test | learn more |
| Iodine-131 | ≈ 8 days | Thyroid treatment; fallout (Chernobyl) | learn more |
| Radon-222 | ≈ 3.8 days | Radioactive gas seeping into basements (a lung-cancer risk in parts of Kansas) | learn more |
| Cobalt-60 | ≈ 5.3 years | Radiation therapy, sterilization | learn more |
Fission vs. fusion
| Fission | Fusion | |
|---|---|---|
| What | A heavy nucleus (U-235, Pu-239) splits when hit by a neutron, releasing more neutrons → chain reaction | Light nuclei (hydrogen isotopes) join to form helium |
| Where | Nuclear power plants, atomic (A-) bombs | Stars (the Sun), hydrogen (H-) bombs, experimental reactors (tokamaks, ITER) |
| History | Discovered 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–energy | In both, products have slightly less mass than reactants; the “missing” mass becomes energy via E = mc². | |
| More | learn more | learn 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
| Force | Relative strength | Range | Carrier (boson) | Does what | More |
|---|---|---|---|---|---|
| Strong nuclear | 1 (strongest) | ~10⁻¹⁵ m (nucleus) | Gluon | Holds quarks together in protons/neutrons; binds the nucleus | learn more |
| Electromagnetic | ~1/137 | Infinite | Photon | Electricity, magnetism, light, chemistry | learn more |
| Weak nuclear | ~10⁻⁶ | ~10⁻¹⁸ m | W⁺, W⁻, Z⁰ | Beta decay; powers the Sun's first fusion step | learn more |
| Gravity | ~10⁻³⁸ (weakest) | Infinite | Graviton (hypothetical) | Planets, stars, galaxies | learn more |
Electromagnetic and weak forces are unified as the electroweak force (Glashow, Salam, Weinberg; Nobel 1979). learn more
The Standard Model
- 6 quarks: up, down, charm, strange, top, bottom. Proton = uud (charge +1), neutron = udd (charge 0). Up = +⅔, down = −⅓. Named by Murray Gell-Mann (1964) from James Joyce's Finnegans Wake (“Three quarks for Muster Mark!”). Top quark (heaviest) found at Fermilab, 1995. learn more
- 6 leptons: electron, muon, tau, and their three neutrinos. Pauli predicted the neutrino (1930); Fermi named it (“little neutral one”). learn more · neutrino
- Gauge bosons (force carriers): photon, gluon, W and Z. Higgs boson gives particles mass — predicted 1964, discovered at CERN's Large Hadron Collider in 2012 (Nobel 2013 to Peter Higgs & François Englert); nicknamed the “God particle.” Higgs · Standard Model
- Fermions (half-integer spin; obey Pauli exclusion; named for Fermi) vs. bosons (integer spin; named for Satyendra Nath Bose). Hadrons are made of quarks: baryons (3 quarks) and mesons (quark + antiquark). fermion · hadron
- Antimatter: Paul Dirac predicted it (1928); Carl Anderson found the positron (1932). Matter + antimatter annihilate into energy. learn more
Relativity
- Special relativity (Einstein, 1905 — his “miracle year,” annus mirabilis). Postulates: (1) the laws of physics are the same in all inertial frames; (2) the speed of light in vacuum is the same for all observers. Consequences: time dilation (moving clocks run slow), length contraction, relativity of simultaneity, E = mc², nothing with mass reaches c. Lorentz factor γ = 1/√(1 − v²/c²). Twin paradox. learn more · 1905 papers
- General relativity (1915): gravity is the curvature of spacetime by mass and energy. Equivalence principle (gravity ≡ acceleration). Evidence: precession of Mercury's perihelion; starlight bending observed by Arthur Eddington in the 1919 solar eclipse; gravitational redshift; GPS satellite clock corrections; black holes; gravitational waves detected by LIGO on Sept 14, 2015 (Nobel 2017). learn more · LIGO
- The 1887 Michelson–Morley experiment found no “luminiferous aether,” setting the stage for special relativity. learn more
“Annus mirabilis,” “1905,” “Brownian motion,” “photoelectric,” “E = mc²” → Einstein. Einstein's Nobel (1921) was for the photoelectric effect. learn more
Units, Prefixes & Constants
↑ topThe 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
| Quantity | Unit | Symbol | Defined by | More |
|---|---|---|---|---|
| Time | second | s | Cesium-133 atomic clock frequency | learn more |
| Length | meter (metre) | m | Speed of light (distance light travels in 1/299,792,458 s) | learn more |
| Mass | kilogram | kg | Planck constant h (the only base unit with a prefix) | learn more |
| Electric current | ampere | A | Elementary charge e | learn more |
| Temperature | kelvin | K | Boltzmann constant k | learn more |
| Amount of substance | mole | mol | Avogadro constant NA | learn more |
| Luminous intensity | candela | cd | Luminous efficacy of 540 THz light | learn 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
| Prefix | Symbol | Factor | Example | More |
|---|---|---|---|---|
| tera- | T | 10¹² | terabyte | learn more |
| giga- | G | 10⁹ | gigawatt, gigahertz | learn more |
| mega- | M | 10⁶ | megaton, megapixel | learn more |
| kilo- | k | 10³ | kilometer, kilogram | learn more |
| hecto- | h | 10² | hectare, hectopascal | learn more |
| deca- (deka-) | da | 10¹ | decameter | learn more |
| (base) | — | 10⁰ = 1 | meter, gram, liter | learn more |
| deci- | d | 10⁻¹ | deciliter | learn more |
| centi- | c | 10⁻² | centimeter | learn more |
| milli- | m | 10⁻³ | milliliter, millisecond | learn more |
| micro- | μ (Greek mu) | 10⁻⁶ | micrometer (micron), microgram | learn more |
| nano- | n | 10⁻⁹ | nanometer (light wavelengths), nanosecond | learn more |
| pico- | p | 10⁻¹² | picometer (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
| Constant | Symbol | Value | More |
|---|---|---|---|
| Speed of light in vacuum | c | 2.998 × 10⁸ m/s (exactly 299,792,458 m/s) | learn more |
| Acceleration of gravity (Earth's surface) | g | 9.8 m/s² = 32 ft/s² | learn more |
| Universal gravitational constant | G | 6.674 × 10⁻¹¹ N·m²/kg² | learn more |
| Planck's constant | h | 6.626 × 10⁻³⁴ J·s | learn more |
| Boltzmann constant | kB | 1.381 × 10⁻²³ J/K | learn more |
| Avogadro's number | NA | 6.022 × 10²³ per mole | learn more |
| Elementary charge | e | 1.602 × 10⁻¹⁹ C | learn more |
| Electron mass | me | 9.109 × 10⁻³¹ kg | learn more |
| Proton mass | mp | 1.673 × 10⁻²⁷ kg (≈ 1836 me) | learn more |
| Ideal gas constant | R | 8.314 J/(mol·K) = 0.0821 L·atm/(mol·K) | learn more |
| Coulomb constant | k | 8.99 × 10⁹ N·m²/C² | learn more |
| Standard atmosphere | atm | 101.325 kPa = 760 mmHg = 14.7 psi | learn more |
| Speed of sound (air, 20 °C) | vs | ≈ 343 m/s | learn more |
| Molar volume of ideal gas at STP (0 °C, 1 atm) | Vm | 22.4 L/mol | learn more |
| Astronomical unit | AU | ≈ 1.496 × 10⁸ km ≈ 93 million miles | learn more |
| Light-year | ly | ≈ 9.46 × 10¹² km ≈ 5.88 trillion miles | learn more |
Units named after scientists
SI rule: the unit name is lowercase (newton), but the symbol is capitalized (N). learn more
| Unit | Measures | Person | More |
|---|---|---|---|
| newton (N) | Force | Isaac Newton | learn more |
| joule (J) | Energy, work, heat | James Prescott Joule | learn more |
| watt (W) | Power | James Watt | learn more |
| pascal (Pa) | Pressure | Blaise Pascal | learn more |
| hertz (Hz) | Frequency | Heinrich Hertz | learn more |
| kelvin (K) | Temperature | William Thomson, Lord Kelvin | learn more |
| volt, ampere, ohm, coulomb, farad, tesla, henry, weber, siemens | Electrical (see table above) | Volta, Ampère, Ohm, Coulomb, Faraday, Tesla, Henry, Weber, Siemens | learn more |
| becquerel (Bq) | Radioactivity (1 decay/s) | Henri Becquerel | learn more |
| curie (Ci) | Radioactivity, older unit (3.7 × 10¹⁰ decays/s ≈ 1 g of radium) | Pierre & Marie Curie | learn more |
| gray (Gy) | Absorbed radiation dose (J/kg) | Louis Harold Gray | learn more |
| sievert (Sv) | Biological dose equivalent | Rolf Sievert | learn more |
| ångström (Å) | Length, 10⁻¹⁰ m (atomic scale) | Anders Jonas Ångström | learn more |
| degree Celsius / Fahrenheit | Temperature | Anders Celsius / Daniel Gabriel Fahrenheit | Celsius · Fahrenheit |
| torr | Pressure (1 mmHg) | Evangelista Torricelli | learn more |
| bel / decibel (dB) | Sound level (log ratio) | Alexander Graham Bell | learn more |
| dalton (Da) | Atomic mass unit | John Dalton | learn more |
| röntgen (R) | X/gamma exposure (old) | Wilhelm Röntgen | learn 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
↑ topAtomic structure
| Particle | Charge | Mass | Location | Discovered | More |
|---|---|---|---|---|---|
| Proton (p⁺) | +1 | ≈ 1 u (1.007 u) | Nucleus | Rutherford, c. 1917–1919 (named 1920) | learn more |
| Neutron (n⁰) | 0 | ≈ 1 u (1.009 u, slightly heavier) | Nucleus | James Chadwick, 1932 | learn more |
| Electron (e⁻) | −1 | ≈ 1/1836 u | Orbitals / electron cloud | J. J. Thomson, 1897 | learn more |
- Atomic number (Z) = number of protons — it defines the element. Henry Moseley (1913) showed X-ray spectra track Z, and the table was reordered by it. learn more
- Mass number (A) = protons + neutrons (a whole number). Neutrons = A − Z. Notation: AZX, e.g. 146C has 6 p, 8 n. learn more
- Isotopes: same element (same Z), different numbers of neutrons. Hydrogen's three: protium (¹H), deuterium (²H, “heavy hydrogen,” found by Harold Urey 1931), tritium (³H, radioactive). Term coined by Frederick Soddy (1913). learn more · hydrogen isotopes
- Atomic mass on the periodic table is a weighted average of isotopes (why chlorine is 35.45, not a whole number: ~76% Cl-35, ~24% Cl-37). learn more
- Ions: atoms that gained (anion, −) or lost (cation, +) electrons. Valence electrons (outer shell) control bonding; the octet rule says atoms tend toward 8. ion · octet rule
- Electron configuration fills by the Aufbau principle (lowest energy first: 1s 2s 2p 3s 3p 4s 3d 4p…), Hund's rule (spread out in equal-energy orbitals before pairing), and the Pauli exclusion principle. Orbital capacities: s = 2, p = 6, d = 10, f = 14. Example: oxygen = 1s² 2s² 2p⁴. learn 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
| Group | Name | Members | Clues | More |
|---|---|---|---|---|
| 1 | Alkali metals | Li, Na, K, Rb, Cs, Fr | 1 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 |
| 2 | Alkaline earth metals | Be, Mg, Ca, Sr, Ba, Ra | 2 valence e⁻; +2 ions; strontium gives red fireworks, barium green. | learn more |
| 3–12 | Transition metals | Fe, Cu, Ag, Au, Zn, Ni, Hg, … | d-block; colored compounds; multiple oxidation states; catalysts. | learn more |
| 13 | Boron group | B, Al, Ga, In, Tl, Nh | Aluminum = most abundant metal in Earth's crust. Gallium melts in your hand (29.8 °C). | learn more |
| 14 | Carbon group (tetrels) | C, Si, Ge, Sn, Pb, Fl | 4 valence e⁻; carbon (life), silicon (chips, sand). | learn more |
| 15 | Pnictogens (nitrogen group) | N, P, As, Sb, Bi, Mc | Nitrogen is ~78% of air. | learn more |
| 16 | Chalcogens (oxygen group) | O, S, Se, Te, Po, Lv | Oxygen = most abundant element in Earth's crust (~46% by mass). | learn more |
| 17 | Halogens (“salt-formers”) | F, Cl, Br, I, At, Ts | 7 valence e⁻; −1 ions; diatomic. Bromine is one of only two elements liquid at room temperature (with mercury). | learn more |
| 18 | Noble gases (inert gases) | He, Ne, Ar, Kr, Xe, Rn, Og | Full 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-block | Lanthanides (57–71) & actinides (89–103) | La…Lu; Ac…Lr | The 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
Periodic trends
| Property | Across a period (→) | Down a group (↓) | Extremes | More |
|---|---|---|---|---|
| Atomic radius | Decreases (more protons pull e⁻ closer) | Increases (more shells) | Largest: cesium/francium; smallest: helium | learn more |
| Ionization energy | Increases | Decreases | Highest: helium; low: cesium | learn more |
| Electronegativity | Increases | Decreases | Highest: fluorine (3.98 on Pauling scale); lowest: cesium/francium (~0.7–0.8) | learn more |
| Metallic character | Decreases | Increases | Most metallic: lower left | learn 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
| Symbol | Element | Z | From | More |
|---|---|---|---|---|
| Na | Sodium | 11 | Latin natrium (from natron) | learn more |
| K | Potassium | 19 | New Latin kalium (from Arabic qali, alkali) | learn more |
| Fe | Iron | 26 | Latin ferrum | learn more |
| Cu | Copper | 29 | Latin cuprum (from Cyprus) | learn more |
| Ag | Silver | 47 | Latin argentum (Argentina is named for silver) | learn more |
| Sn | Tin | 50 | Latin stannum | learn more |
| Sb | Antimony | 51 | Latin stibium | learn more |
| W | Tungsten | 74 | German Wolfram (not Latin); “tungsten” is Swedish for “heavy stone.” Highest melting point of any metal (3,422 °C). | learn more |
| Au | Gold | 79 | Latin aurum (“shining dawn”) | learn more |
| Hg | Mercury | 80 | Greek-Latin hydrargyrum (“water-silver,” quicksilver) | learn more |
| Pb | Lead | 82 | Latin 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
| Z | Symbol | Name | Atomic mass | Quiz clue | More |
|---|---|---|---|---|---|
| 1 | H | Hydrogen | 1.008 | Lightest, most abundant in universe; Cavendish isolated it (1766, “inflammable air”); Lavoisier named it (“water-former”); Hindenburg 1937. | learn more |
| 2 | He | Helium | 4.003 | Found in the Sun's spectrum (1868, Janssen & Lockyer) before Earth (Ramsay, 1895); named for Greek helios; lowest boiling point. | learn more |
| 3 | Li | Lithium | 6.94 | Lightest metal; batteries; mood-stabilizing drug. | learn more |
| 4 | Be | Beryllium | 9.012 | From the gem beryl (emerald); JWST mirrors; toxic dust. | learn more |
| 5 | B | Boron | 10.81 | Borax, Pyrex (borosilicate glass); metalloid. | learn more |
| 6 | C | Carbon | 12.011 | Basis of organic chemistry; allotropes diamond, graphite, fullerenes (buckyballs), graphene. | learn more · allotropes |
| 7 | N | Nitrogen | 14.007 | ~78% of air; discovered by Daniel Rutherford (1772); Haber process → fertilizer. | learn more |
| 8 | O | Oxygen | 15.999 | Discovered by Scheele (c. 1771) and Priestley (1774); named by Lavoisier (“acid-former”); ozone is O₃. | learn more |
| 9 | F | Fluorine | 18.998 | Most electronegative and reactive element; isolated by Henri Moissan (1886; Nobel 1906); toothpaste fluoride. | learn more |
| 10 | Ne | Neon | 20.180 | Red-orange signs; Ramsay & Travers 1898 (Greek “new”). | learn more |
| 11 | Na | Sodium | 22.990 | Isolated by Humphry Davy via electrolysis (1807); table salt NaCl; yellow streetlights. | learn more |
| 12 | Mg | Magnesium | 24.305 | Burns with brilliant white light (flares); center of chlorophyll; Epsom salts. | learn more |
| 13 | Al | Aluminum | 26.982 | Most abundant metal in crust; once more precious than gold (Washington Monument cap, 1884); Hall–Héroult process (1886). | learn more |
| 14 | Si | Silicon | 28.085 | 2nd most abundant in crust; semiconductors; isolated by Berzelius (1823). | learn more |
| 15 | P | Phosphorus | 30.974 | Discovered by Hennig Brand (1669) from urine — first element discovered by a known person; glows in the dark; matches; DNA backbone. | learn more |
| 16 | S | Sulfur | 32.06 | “Brimstone”; rotten-egg smell is H₂S; vulcanizes rubber; sulfuric acid. | learn more |
| 17 | Cl | Chlorine | 35.45 | Scheele (1774); named by Davy (Greek “pale green”); WWI poison gas; pool disinfectant. | learn more |
| 18 | Ar | Argon | 39.95 | First noble gas isolated (Rayleigh & Ramsay, 1894); Greek “lazy”; ~0.93% of air; fills light bulbs. | learn more |
| 19 | K | Potassium | 39.098 | First metal isolated by electrolysis (Davy, 1807); bananas; nerve impulses. | learn more |
| 20 | Ca | Calcium | 40.078 | Bones, 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 for | Elements | More |
|---|---|---|
| Scientists | Curium (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 |
| Places | Americium, 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 village | Ytterby gave four: yttrium, ytterbium, terbium, erbium | learn more |
| Mythology & space | Helium (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
| Change | From → to | Example | More |
|---|---|---|---|
| Melting (fusion) | solid → liquid | Ice melting | learn more |
| Freezing (solidification) | liquid → solid | Water to ice | learn more |
| Vaporization (boiling, evaporation) | liquid → gas | Puddle drying | learn more |
| Condensation | gas → liquid | Dew, fog on a cold glass | learn more |
| Sublimation | solid → gas | Dry ice (solid CO₂), mothballs, freezer burn | learn more |
| Deposition | gas → solid | Frost, snowflakes forming | learn more |
| Ionization / recombination | gas ↔ plasma | Lightning | learn 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
↑ topConservation 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
- Write correct formulas for every reactant and product (never change these afterward).
- Count atoms of each element on each side.
- 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.
- Treat unchanged polyatomic ions (SO₄²⁻, NO₃⁻) as single units.
- Recount; reduce coefficients to the smallest whole numbers. (If you get a fraction like 7/2 O₂, multiply everything by 2.)
Worked examples
| Unbalanced | Balanced | Check | More |
|---|---|---|---|
| H₂ + O₂ → H₂O | 2H₂ + O₂ → 2H₂O | H: 4 = 4; O: 2 = 2. (Formation of water — synthesis.) | learn more |
| CH₄ + O₂ → CO₂ + H₂O | CH₄ + 2O₂ → CO₂ + 2H₂O | C: 1 = 1; H: 4 = 4; O: 4 = 2 + 2. (Burning natural gas — combustion.) | learn more |
| C₃H₈ + O₂ → CO₂ + H₂O | C₃H₈ + 5O₂ → 3CO₂ + 4H₂O | C: 3; H: 8; O: 10 = 6 + 4. (Propane grill.) Balance C first, then H, then O last. | learn more |
| Fe + O₂ → Fe₂O₃ | 4Fe + 3O₂ → 2Fe₂O₃ | Fe: 4 = 4; O: 6 = 6. (Rusting — synthesis/redox.) | learn more |
| Al + HCl → AlCl₃ + H₂ | 2Al + 6HCl → 2AlCl₃ + 3H₂ | Al: 2; H: 6 = 6; Cl: 6 = 6. (Single replacement.) | learn more |
| N₂ + H₂ → NH₃ | N₂ + 3H₂ → 2NH₃ | N: 2; H: 6. (The Haber process — makes fertilizer.) | learn more |
| C₆H₁₂O₆ + O₂ → CO₂ + H₂O | C₆H₁₂O₆ + 6O₂ → 6CO₂ + 6H₂O | C: 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
| Type | Pattern | Example | More |
|---|---|---|---|
| Synthesis (combination) | A + B → AB | 2Na + Cl₂ → 2NaCl | learn more |
| Decomposition | AB → A + B | 2H₂O₂ → 2H₂O + O₂; electrolysis of water; CaCO₃ → CaO + CO₂ | learn more |
| Single replacement (displacement) | A + BC → AC + B | Zn + 2HCl → ZnCl₂ + H₂; a more active metal replaces a less active one (activity series) | learn more |
| Double replacement (metathesis) | AB + CD → AD + CB | AgNO₃ + NaCl → AgCl↓ + NaNO₃ (forms a precipitate) | learn more |
| Combustion | Fuel + O₂ → CO₂ + H₂O (for hydrocarbons) | CH₄ + 2O₂ → CO₂ + 2H₂O; incomplete combustion makes CO | learn more |
| Acid–base (neutralization) | Acid + base → salt + water | HCl + NaOH → NaCl + H₂O | learn more |
| Redox (oxidation–reduction) | Electrons transfer | Rusting, batteries, combustion, photosynthesis | learn 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
↑ topThe mole
- One mole = 6.022 × 10²³ particles (Avogadro's number) — the chemist's “dozen.” Named for Amedeo Avogadro (the number itself was named and estimated later, notably by Jean Perrin, Nobel 1926). Mole Day is October 23, from 6:02 a.m. to 6:02 p.m. learn more · Mole Day
- Molar mass (g/mol) = sum of atomic masses in the formula. H₂O = 2(1.008) + 16.00 = 18.02 g/mol; CO₂ = 44.01; NaCl = 58.44; glucose C₆H₁₂O₆ = 180.16. learn more
- Conversions: moles = grams ÷ molar mass; particles = moles × 6.022 × 10²³. Example: 36 g of water = 2 mol = 1.2 × 10²⁴ molecules. learn more
- Percent composition = (mass of element in formula ÷ molar mass) × 100. Water: H = 2.016/18.02 ≈ 11.2%, O ≈ 88.8%. Glucose is 40.0% carbon. Empirical formula = simplest ratio (glucose C₆H₁₂O₆ → CH₂O); molecular formula = actual count. learn more · empirical formula
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
- Molarity M = moles of solute / liters of solution. 0.5 mol NaCl in 250 mL → 2 M. 58.44 g NaCl in 1 L of solution → 1 M. learn more
- Dilution: M₁V₁ = M₂V₂. 100 mL of 6 M acid diluted to 600 mL → 1 M. learn more
- Molality (m) = moles solute per kg of solvent. Colligative properties (depend on number of particles, not identity): boiling-point elevation, freezing-point depression (salting icy roads; antifreeze), osmotic pressure. learn more
Gas laws
Always use kelvins for temperature in gas laws. learn more
| Law | Formula | Held constant | Relationship / example | More |
|---|---|---|---|---|
| Boyle's (Robert Boyle, 1662) | P₁V₁ = P₂V₂ | T, n | Pressure 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/T₂ | P, n | Volume 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/T₂ | V, n | Pressure directly proportional to temperature. Aerosol cans warn not to heat; tire pressure rises on hot days. | learn more |
| Avogadro's (1811) | V₁/n₁ = V₂/n₂ | P, T | Equal volumes of gases at the same T and P contain equal numbers of molecules. | learn more |
| Combined | P₁V₁/T₁ = P₂V₂/T₂ | n | Boyle + 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
- STP (standard temperature and pressure), classic textbook definition: 0 °C (273.15 K) and 1 atm — one mole of any ideal gas occupies 22.4 L. (IUPAC since 1982 uses 100 kPa, giving 22.7 L; some tests still use 22.4.) learn more
- Kinetic molecular theory: gas particles are tiny, in constant random motion, have elastic collisions, and no attractions; average KE ∝ kelvin temperature. Real gases deviate at high pressure and low temperature (van der Waals equation). learn more · van der Waals
Acids, Bases, Solutions & Bonding
↑ topThe pH scale
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. pH | Substance | More |
|---|---|---|
| 0–1 | Battery acid (sulfuric acid) | learn more |
| 1.5–3.5 | Stomach acid (HCl) | learn more |
| ~2 | Lemon juice (citric acid) | learn more |
| ~2.5 | Cola (phosphoric & carbonic acid); vinegar ~2.5–3 (acetic acid) | learn more |
| ~5 | Black coffee; normal rain ~5.6 (acid rain is below that) | learn more |
| 7 | Pure water (neutral) | learn more |
| 7.35–7.45 | Human blood (slightly basic) | learn more |
| ~8.1 | Seawater (slowly acidifying from absorbed CO₂) | learn more |
| ~8.3 | Baking soda solution (NaHCO₃) | learn more |
| ~10.5 | Milk of magnesia (Mg(OH)₂) | learn more |
| ~11–12 | Household ammonia (NH₃) | learn more |
| ~12.5–13 | Bleach (sodium hypochlorite) | learn more |
| ~14 | Lye / drain cleaner (NaOH) | learn more |
Common acids & bases
| Formula | Name | Where / clue | More |
|---|---|---|---|
| HCl | Hydrochloric (muriatic) acid | Stomach acid; strong acid | learn more |
| H₂SO₄ | Sulfuric acid (oil of vitriol) | Car batteries; most-produced industrial chemical; strong | learn more |
| HNO₃ | Nitric acid | Fertilizers, explosives; turns skin yellow; strong | learn more |
| CH₃COOH | Acetic acid | Vinegar (~5%); weak | learn more |
| H₂CO₃ | Carbonic acid | Carbonated drinks (CO₂ + H₂O); weak | learn more |
| H₃PO₄ | Phosphoric acid | Colas, rust removers | learn more |
| HCOOH | Formic acid | Ant stings (Latin formica = ant) | learn more |
| C₆H₈O₇ / C₃H₆O₃ | Citric / lactic acid | Citrus fruit / sour milk & muscle fatigue | citric · lactic |
| NaOH / KOH | Sodium / potassium hydroxide (lye, caustic soda/potash) | Soap making, drain cleaner; strong bases | learn more |
| NH₃ | Ammonia | Cleaners, fertilizer; weak base | learn more |
| Ca(OH)₂ | Calcium hydroxide (slaked lime) | Mortar, soil treatment | learn 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
| Definition | Acid | Base | More |
|---|---|---|---|
| Arrhenius (Svante Arrhenius, 1884–87; Nobel 1903) | Produces H⁺ (H₃O⁺, hydronium) in water | Produces OH⁻ in water | learn more |
| Brønsted–Lowry (Johannes Brønsted & Thomas Lowry, 1923) | Proton (H⁺) donor | Proton acceptor; acids and bases form conjugate pairs | learn more |
| Lewis (Gilbert N. Lewis, 1923) | Electron-pair acceptor | Electron-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
| Indicator | In acid | In base | More |
|---|---|---|---|
| Litmus (from lichens) | Red | Blue | learn more |
| Phenolphthalein | Colorless | Pink/magenta (above ~pH 8.2) | learn more |
| Bromothymol blue | Yellow | Blue | learn more |
| Methyl orange | Red | Yellow (changes ~pH 3.1–4.4) | learn more |
| Red cabbage juice (anthocyanins) | Red/pink | Green/yellow | learn 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
| Bond | How | Typical between | Properties / examples | More |
|---|---|---|---|---|
| Ionic | Electron transfer; + and − ions attract | Metal + nonmetal (electronegativity difference > ~1.7) | NaCl; crystal lattices, high melting points, conduct when melted or dissolved | learn more |
| Covalent — polar | Unequal sharing of electrons | Nonmetals with different electronegativity (~0.4–1.7) | H₂O, HCl, NH₃ — partial charges (δ+ / δ−) | learn more |
| Covalent — nonpolar | Equal sharing | Identical or similar atoms | H₂, O₂, N₂, Cl₂, CH₄; single, double, triple bonds | learn more |
| Metallic | “Sea” of delocalized electrons | Metal atoms | Conductivity, luster, malleability | learn more |
| Hydrogen bond (intermolecular) | H bonded to N, O, or F attracted to a lone pair on another N/O/F | Between molecules (or parts of one) | Water's high boiling point & surface tension; ice floats; holds DNA strands together; protein shape | learn more |
| Van der Waals / London dispersion | Temporary dipoles | All molecules (only force in nonpolar ones) | Why geckos stick to walls; weakest | learn 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
| Domains | Lone pairs | Shape | Bond angle | Example | More |
|---|---|---|---|---|---|
| 2 | 0 | Linear | 180° | CO₂, BeCl₂ | learn more |
| 3 | 0 | Trigonal planar | 120° | BF₃, SO₃ | learn more |
| 3 | 1 | Bent | < 120° (~119°) | SO₂ | learn more |
| 4 | 0 | Tetrahedral | 109.5° | CH₄, CCl₄ | learn more |
| 4 | 1 | Trigonal pyramidal | ~107° | NH₃ | learn more |
| 4 | 2 | Bent | ~104.5° | H₂O | learn more |
| 5 | 0 | Trigonal bipyramidal | 90°, 120° | PCl₅ | learn more |
| 5 | 1 | Seesaw | < 90°, < 120° | SF₄ | learn more |
| 5 | 2 | T-shaped | < 90° | ClF₃ | learn more |
| 6 | 0 | Octahedral | 90° | SF₆ | learn more |
| 6 | 2 | Square planar | 90° | XeF₄ | learn 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
↑ topOrganic 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
| Carbons | Prefix | Alkane | Formula | Clue | More |
|---|---|---|---|---|---|
| 1 | meth- | Methane | CH₄ | Natural gas; potent greenhouse gas; cow burps | learn more |
| 2 | eth- | Ethane | C₂H₆ | Natural gas component | learn more |
| 3 | prop- | Propane | C₃H₈ | Grills, rural home heating | learn more |
| 4 | but- | Butane | C₄H₁₀ | Lighters | learn more |
| 5 | pent- | Pentane | C₅H₁₂ | First liquid alkane at room temp | learn more |
| 6 | hex- | Hexane | C₆H₁₄ | Solvent | learn more |
| 7 | hept- | Heptane | C₇H₁₆ | 0 on the octane rating scale | learn more |
| 8 | oct- | Octane | C₈H₁₈ | Gasoline; isooctane = 100 on the octane scale | learn more |
| 9 | non- | Nonane | C₉H₂₀ | Kerosene component | learn more |
| 10 | dec- | Decane | C₁₀H₂₂ | Fuel component | learn more |
Mnemonic for meth/eth/prop/but: “Monkeys Eat Peeled Bananas.” From pent- on, the prefixes are Greek numbers. numeric prefixes
- Alkanes (single bonds, saturated): CnH2n+2, suffix -ane. Alkenes (one C=C double bond): CnH2n, -ene (ethene = ethylene, ripens fruit). Alkynes (C≡C triple bond): CnH2n−2, -yne (ethyne = acetylene, welding torches). alkanes · alkenes · alkynes
- Aromatic compounds contain a benzene ring (C₆H₆). August Kekulé said the ring structure came to him (1865) in a dream of a snake biting its own tail (the ouroboros). Benzene was first isolated by Michael Faraday (1825). learn more
- Isomers: same formula, different structure (butane vs. isobutane). Mirror-image isomers are enantiomers (chirality — discovered by Pasteur in tartaric acid crystals, 1848). learn more · chirality
- Crude oil is separated by fractional distillation; fossil fuels are coal, oil, natural gas. learn more
Functional groups
| Group | Structure | Name ending | Example | More |
|---|---|---|---|---|
| Alcohol (hydroxyl) | R–OH | -ol | Ethanol (drinking alcohol), methanol (wood alcohol, toxic), isopropanol (rubbing alcohol) | learn more |
| Aldehyde | R–CHO | -al | Formaldehyde (methanal; preservative), vanillin | learn more |
| Ketone | R–CO–R′ | -one | Acetone (propanone; nail-polish remover) | learn more |
| Carboxylic acid | R–COOH | -oic acid | Acetic acid (ethanoic acid; vinegar) | learn more |
| Ester | R–COO–R′ | -oate | Fruity smells (isoamyl acetate = banana); fats; aspirin; made from acid + alcohol | learn more |
| Ether | R–O–R′ | ether | Diethyl ether (early anesthetic, 1840s) | learn more |
| Amine | R–NH₂ | -amine | Methylamine; fishy odors; amino acids | learn more |
| Amide | R–CO–NH₂ | -amide | Peptide bonds in proteins; nylon; acetaminophen | learn more |
| Haloalkane | R–X (F, Cl, Br, I) | halo- prefix | Chloroform; CFCs (Freon) that deplete ozone | learn 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
| Polymer | Clue | More |
|---|---|---|
| Vulcanized rubber | Charles Goodyear heated rubber with sulfur (1839) | learn more |
| Bakelite | Leo Baekeland (1907) — first fully synthetic plastic | learn more |
| Nylon | Wallace Carothers at DuPont (1935); stockings, toothbrush bristles | learn more |
| Teflon (PTFE) | Roy Plunkett at DuPont, accidental discovery (1938); nonstick pans | learn more |
| Kevlar | Stephanie Kwolek at DuPont (1965); bulletproof vests | learn more |
| Polyethylene, PVC, polystyrene, PET | Bags (most common plastic), pipes, Styrofoam, soda bottles | learn more |
| Natural polymers | Cellulose, starch, proteins, DNA, chitin, natural rubber | learn more |
The four classes of biomolecules
| Class | Monomer / building block | Examples | Function | More |
|---|---|---|---|---|
| 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, structure | learn more |
| Lipids | Glycerol + 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, hormones | learn more |
| Proteins | Amino acids (20 standard) joined by peptide bonds | Enzymes (lactase, amylase), hemoglobin, keratin, collagen, insulin, antibodies. Four levels of structure (primary → quaternary) | Catalysis, structure, transport, defense, signals | learn more |
| Nucleic acids | Nucleotides (5-carbon sugar + phosphate + nitrogenous base) | DNA, RNA; ATP is a nucleotide (energy currency) | Store and transmit genetic information | learn 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
↑ topCell 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
| Organelle | Function / clue | Found in | More |
|---|---|---|---|
| Nucleus | “Control center”; holds DNA (chromatin); surrounded by nuclear envelope with pores | Eukaryotes | learn more |
| Nucleolus | Inside the nucleus; makes ribosomes (rRNA) | Eukaryotes | learn more |
| Mitochondrion | “Powerhouse of the cell” — cellular respiration makes ATP; has its own DNA (inherited from the mother); folds called cristae | Nearly all eukaryotes | learn more |
| Chloroplast | Photosynthesis; contains green chlorophyll; stacks of thylakoids called grana; fluid = stroma; own DNA | Plants, algae | learn more |
| Ribosome | Makes proteins (translation); not membrane-bound | All cells (prokaryotes too) | learn more |
| Rough ER | Endoplasmic reticulum studded with ribosomes; makes and transports proteins | Eukaryotes | learn more |
| Smooth ER | Makes lipids; detoxifies drugs (abundant in liver) | Eukaryotes | learn more |
| Golgi apparatus | Modifies, packages, and ships proteins (“post office”); named for Camillo Golgi | Eukaryotes | learn more |
| Lysosome | Digestive enzymes; breaks down waste (“suicide sac”) | Mainly animal cells | learn more |
| Vacuole | Storage of water, food, waste; plants have one large central vacuole providing turgor pressure | Plants (large), animals (small) | learn more |
| Cell membrane | Phospholipid bilayer; selectively permeable; fluid mosaic model (Singer & Nicolson, 1972) | All cells | learn more |
| Cell wall | Rigid support outside the membrane: cellulose (plants), chitin (fungi), peptidoglycan (bacteria) | Plants, fungi, bacteria | learn more |
| Cytoplasm / cytoskeleton | Gel-like interior / protein fibers (microtubules, microfilaments) giving shape and movement | All cells / eukaryotes | learn more |
| Centrioles | Organize spindle fibers during cell division | Animal cells | learn more |
| Flagella / cilia | Whip-like tail / short hairs for movement | Various | learn 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
| Prokaryote | Eukaryote | |
|---|---|---|
| Nucleus | None — DNA in a nucleoid region (plus plasmids) | True membrane-bound nucleus (Greek eu = true, karyon = kernel) |
| Organelles | No membrane-bound organelles; has ribosomes | Mitochondria, ER, Golgi, etc. |
| Size | Small (~1–10 μm) | Larger (~10–100 μm) |
| Examples | Bacteria, archaea | Animals, plants, fungi, protists |
| More | learn more | learn 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
- Prophase — chromosomes condense, nuclear envelope breaks down, spindle forms.
- Metaphase — chromosomes line up at the middle (metaphase plate).
- Anaphase — sister chromatids pulled apart to opposite poles.
- Telophase — two new nuclei form; then cytokinesis splits the cytoplasm (cleavage furrow in animals, cell plate in plants).
| Mitosis | Meiosis | |
|---|---|---|
| Purpose | Growth, repair, asexual reproduction | Making gametes (sperm, egg) for sexual reproduction |
| Divisions | 1 | 2 (meiosis I and II) |
| Daughter cells | 2, diploid (2n), genetically identical | 4, haploid (n), genetically different |
| Humans | 46 → 46 chromosomes | 46 → 23 chromosomes |
| Variation | None (clones) | Crossing over (prophase I) and independent assortment; homologous pairs separate in anaphase I |
| More | learn more | learn 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
Cellular respiration (cytoplasm + mitochondria): C₆H₁₂O₆ + 6O₂ → 6CO₂ + 6H₂O + energy (ATP)
- Photosynthesis has light-dependent reactions (thylakoid membranes; split water and release O₂; make ATP and NADPH) and the Calvin cycle (light-independent, in the stroma; fixes CO₂ into sugar using the enzyme RuBisCO — likely the most abundant protein on Earth). Melvin Calvin, Nobel 1961. The O₂ we breathe comes from the water, not the CO₂. learn more · Calvin cycle
- Respiration stages: glycolysis (cytoplasm; glucose → 2 pyruvate; net 2 ATP; anaerobic) → Krebs (citric acid) cycle (mitochondrial matrix; Hans Krebs, 1937) → electron transport chain (inner mitochondrial membrane; most ATP; O₂ is the final electron acceptor). Total ≈ 30–38 ATP per glucose (textbooks often say 36–38). learn more · Krebs cycle
- Without oxygen: fermentation — lactic acid (muscle cramps, yogurt) or alcoholic (yeast → ethanol + CO₂: bread, beer). Only 2 ATP. learn more
- History: Jan Ingenhousz (1779) showed plants need light to “restore” air; Joseph Priestley's mint-and-mouse experiment (1771). learn more
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
| DNA | RNA | |
|---|---|---|
| Sugar | Deoxyribose | Ribose |
| Bases | Adenine, Thymine, Guanine, Cytosine | A, Uracil (replaces T), G, C |
| Strands | Double helix (antiparallel) | Usually single |
| Types / role | Stores genetic information (in nucleus) | mRNA (messenger), tRNA (transfer — carries amino acids), rRNA (ribosomal) |
| More | learn more | learn more |
- Base pairing: A–T (2 hydrogen bonds), G–C (3 hydrogen bonds); in RNA, A–U. Purines (A, G — two rings) pair with pyrimidines (C, T, U — one ring). Chargaff's rules (Erwin Chargaff, ~1950): %A = %T and %G = %C. learn more · Chargaff
- Double helix (1953): James Watson and Francis Crick (Cambridge) built the model, using X-ray diffraction data from Rosalind Franklin — notably “Photo 51,” taken by her student Raymond Gosling in 1952 and shown to Watson by Maurice Wilkins (King's College London) without her knowledge. Watson, Crick and Wilkins shared the 1962 Nobel in Physiology or Medicine; Franklin had died in 1958, and Nobels are not awarded posthumously. Watson's memoir: The Double Helix (1968). 1953 paper · Photo 51
- Replication is semiconservative (each new helix keeps one old strand — Meselson–Stahl, 1958), using DNA polymerase, helicase (unzips), and ligase. learn more
- Central dogma (Crick, 1958): DNA → RNA → protein. Transcription (DNA → mRNA, in the nucleus, by RNA polymerase); translation (mRNA → protein, at ribosomes; tRNA anticodons match mRNA codons). Exception: retroviruses like HIV use reverse transcriptase (RNA → DNA). learn more
- Codons are 3 bases long; 4³ = 64 codons code for 20 amino acids (the code is redundant). Start codon AUG (methionine); stop codons UAA, UAG, UGA. First cracked by Marshall Nirenberg & Heinrich Matthaei (1961: UUU = phenylalanine). learn more
- Mutations: point (substitution — sickle-cell anemia is a single base change), insertions/deletions (frameshift). learn more
- Human Genome Project completed 2003: ~3 billion base pairs, ~20,000 protein-coding genes. PCR (Kary Mullis, 1983) copies DNA; CRISPR-Cas9 (Doudna & Charpentier, 2012) edits it. HGP · CRISPR
“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
- Law of segregation: each parent passes one of its two alleles per gene to each gamete. Law of independent assortment: genes for different traits sort independently (true for unlinked genes). Law of dominance. learn more
- Vocabulary: allele (gene version), genotype (Bb) vs. phenotype (brown eyes), homozygous (BB, bb) vs. heterozygous (Bb), dominant (capital) vs. recessive (lowercase). learn more
- Punnett square — named for Reginald Punnett. Monohybrid cross Bb × Bb → genotypes 1 BB : 2 Bb : 1 bb, phenotypes 3 dominant : 1 recessive. Dihybrid cross (AaBb × AaBb) → phenotypes 9 : 3 : 3 : 1. A test cross with a homozygous recessive reveals an unknown genotype. learn more
| Bb × Bb | B | b |
|---|---|---|
| B | BB | Bb |
| b | Bb | bb |
→ ¼ BB, ½ Bb, ¼ bb; ¾ show the dominant trait. learn more
- Incomplete dominance: blended phenotype (red × white snapdragons → pink). Codominance: both show (AB blood type, roan cattle). Polygenic traits (height, skin color) vary continuously. learn more
- Sex-linked (X-linked) traits — red-green color blindness, hemophilia (Queen Victoria's descendants) — show up more in males (XY). Thomas Hunt Morgan's fruit flies (Drosophila, white eyes) proved genes ride on chromosomes (Nobel 1933). learn more
- Hardy–Weinberg equilibrium: p² + 2pq + q² = 1, p + q = 1. 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
| Rank | Human | Gray wolf / dog | Mnemonic | More |
|---|---|---|---|---|
| Domain | Eukarya | Eukarya | Dear | learn more |
| Kingdom | Animalia | Animalia | King | learn more |
| Phylum | Chordata | Chordata | Philip | learn more |
| Class | Mammalia | Mammalia | Came | learn more |
| Order | Primates | Carnivora | Over | learn more |
| Family | Hominidae | Canidae | For | learn more |
| Genus | Homo | Canis | Good | learn more |
| Species | sapiens | lupus | Soup | learn more |
“Dear King Philip Came Over For Good Soup.” learn more
- Three domains (Carl Woese, 1977/1990, from ribosomal RNA): Bacteria, Archaea (extremophiles — hot springs, salt lakes), Eukarya. learn more
- Six kingdoms (common U.S. textbook system): Animalia, Plantae, Fungi, Protista, Archaebacteria, Eubacteria. Robert Whittaker's earlier five-kingdom system (1969) lumped bacteria as Monera. Fungi are more closely related to animals than to plants. learn more
Evolution
- Charles Darwin: voyage of HMS Beagle (1831–1836), including the Galápagos Islands (finches, tortoises, mockingbirds); On the Origin of Species (Nov 24, 1859); The Descent of Man (1871). Influenced by Thomas Malthus (population) and Charles Lyell (geology). learn more · Beagle voyage
- Alfred Russel Wallace independently conceived natural selection in the Malay Archipelago; their joint papers were read at the Linnean Society in 1858. learn more
- Natural selection: variation + inheritance + overproduction + competition → individuals with favorable traits survive and reproduce more. “Survival of the fittest” was coined by Herbert Spencer (1864). learn more
- Jean-Baptiste Lamarck (1809): inheritance of acquired characteristics — the giraffe stretching its neck — now rejected. learn more
- Evidence: fossils, homologous structures (same origin — human arm, bat wing, whale flipper), analogous structures (same function, different origin — bird vs. insect wings), vestigial structures (appendix, whale hip bones), embryology, DNA comparisons. Other ideas: genetic drift, gene flow, punctuated equilibrium (Eldredge & Gould, 1972), convergent evolution, the peppered moth in industrial England. learn more
- The Scopes “Monkey” Trial (Dayton, Tennessee, 1925) tested a ban on teaching evolution. learn more
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
- Organism → population → community → ecosystem → biome → biosphere. “Ecology” was coined by Ernst Haeckel (1866). learn more
- Trophic levels: producers (autotrophs — plants, algae) → primary consumers (herbivores) → secondary consumers → tertiary consumers / apex predators; decomposers (fungi, bacteria) recycle nutrients. Food chain vs. food web. learn more
- 10% rule: only about 10% of energy passes to the next trophic level (the rest is lost mostly as heat) — why energy pyramids are narrow at the top (Raymond Lindeman, 1942). 10,000 kcal of grass → ~1,000 in grasshoppers → ~100 in frogs → ~10 in snakes. learn more
- Symbiosis: mutualism (+/+, bees & flowers, lichens), commensalism (+/0, barnacles on whales), parasitism (+/−, ticks). learn more
- Succession: primary (bare rock; pioneer species like lichens) vs. secondary (after fire/plowing; soil remains). Keystone species (sea otters, wolves in Yellowstone, prairie dogs on the plains). succession · keystone
- Biogeochemical cycles: carbon, nitrogen (nitrogen-fixing bacteria on legume roots), water, phosphorus. nitrogen cycle
- Rachel Carson's Silent Spring (1962) exposed DDT's harm (eggshell thinning in birds), spurring the modern environmental movement; DDT was banned in the U.S. in 1972. learn more
| Biome | Features | More |
|---|---|---|
| Tundra | Coldest; permafrost; mosses, lichens, caribou; treeless | learn more |
| Taiga (boreal forest) | Conifers; largest land biome; Canada, Siberia | learn more |
| Temperate deciduous forest | Trees drop leaves in fall; four seasons; eastern U.S. | learn more |
| Tropical rainforest | Greatest biodiversity; canopy layers; Amazon, Congo | learn 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, bison | tallgrass prairie · Flint Hills |
| Savanna | Tropical grassland with scattered trees; African megafauna | learn 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-adapted | learn more |
Human body systems
| System | Main organs | Quiz clues | More |
|---|---|---|---|
| Circulatory (cardiovascular) | Heart, arteries, veins, capillaries, blood | 4-chambered heart (2 atria, 2 ventricles); arteries carry blood away from the heart; aorta = largest artery; William Harvey described circulation (1628) | learn more |
| Respiratory | Lungs, trachea, bronchi, alveoli, diaphragm | Gas exchange in alveoli; diaphragm drives breathing | learn more |
| Digestive | Mouth, esophagus, stomach, small & large intestine, liver, pancreas, gallbladder | Most absorption in the small intestine (villi); liver = largest internal organ, makes bile; peristalsis | learn more |
| Nervous | Brain, spinal cord, nerves | Neuron parts: dendrite, cell body, axon, myelin; cerebrum (thinking), cerebellum (balance), medulla (breathing, heartbeat) | learn more |
| Skeletal | Bones, cartilage, ligaments | Adults: 206 bones; femur longest, stapes (in the ear) smallest; marrow makes blood cells | learn more |
| Muscular | Skeletal, smooth, cardiac muscle | Tendons connect muscle to bone (ligaments bone to bone); gluteus maximus largest muscle | learn more |
| Integumentary | Skin, hair, nails | Skin is the largest organ; epidermis, dermis; makes vitamin D | learn more |
| Endocrine | Pituitary, thyroid, adrenal glands, pancreas, gonads | Hormones; pituitary = “master gland”; insulin (pancreas) lowers blood sugar; adrenaline = fight or flight | learn more |
| Immune / lymphatic | White blood cells, lymph nodes, spleen, thymus | Antibodies, B and T cells; vaccines train it | learn more |
| Excretory / urinary | Kidneys, ureters, bladder, urethra | Kidneys filter blood via nephrons | learn more |
| Reproductive | Ovaries, testes, uterus | Produces gametes by meiosis | learn more |
Blood & blood types
- Blood components: red blood cells (erythrocytes — hemoglobin carries O₂; no nucleus; live ~120 days), white blood cells (leukocytes — fight infection), platelets (thrombocytes — clotting), plasma (~55%, mostly water). learn more
- ABO system discovered by Karl Landsteiner (1901; Nobel 1930); he and Alexander Wiener later found the Rh factor (1937–40, named for rhesus monkeys). learn more · Rh
| Type | Antigens on red cells | Antibodies in plasma | Can receive red cells from | More |
|---|---|---|---|---|
| A | A | anti-B | A, O | learn more |
| B | B | anti-A | B, O | learn more |
| AB | A and B | neither | A, B, AB, O — universal recipient (AB+) | learn more |
| O | neither | anti-A and anti-B | O only — O− is the universal donor of red cells | learn 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 / nutrient | Deficiency disease | Clue | More |
|---|---|---|---|
| A (retinol) | Night blindness | Carrots (beta-carotene) | learn more |
| B₁ (thiamine) | Beriberi | Polished white rice diets; Christiaan Eijkman | learn more |
| B₃ (niacin) | Pellagra (“4 D's”: dermatitis, diarrhea, dementia, death) | Corn-heavy diets in the American South; Joseph Goldberger | learn more |
| B₉ (folate / folic acid) | Anemia; neural-tube birth defects | Leafy greens; prenatal vitamins | learn more |
| B₁₂ (cobalamin) | Pernicious anemia | Contains cobalt; Dorothy Hodgkin found its structure | learn 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 light | learn more |
| K | Bleeding (poor clotting) | From German Koagulation; made by gut bacteria | learn more |
| Iodine (mineral) | Goiter (enlarged thyroid) | Iodized salt (U.S., 1924) | learn more |
| Iron (mineral) | Iron-deficiency anemia | Needed for hemoglobin | learn more |
Earth Science & Weather
↑ topEarth's layers
| Layer | State / composition | Facts | More |
|---|---|---|---|
| Crust | Solid rock: continental (granite, ~30–70 km thick, less dense) and oceanic (basalt, ~5–10 km, denser) | Thinnest layer; most abundant elements O, Si, Al, Fe | learn more |
| Mantle | Hot, solid rock that flows slowly (peridotite); upper part includes the plastic asthenosphere | Thickest layer (~2,900 km), ~84% of Earth's volume; convection drives plates. Crust + rigid uppermost mantle = lithosphere | learn more |
| Outer core | Liquid iron–nickel | Its flow generates Earth's magnetic field (geodynamo) | learn more |
| Inner core | Solid 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 |
- Boundaries: Mohorovičić discontinuity (“Moho,” crust–mantle; Andrija Mohorovičić, 1909); Gutenberg discontinuity (mantle–core; Beno Gutenberg, 1913); Lehmann discontinuity. Moho · core–mantle boundary
- Seismic waves reveal the interior: P-waves (primary, compressional, fastest, travel through solids and liquids) and S-waves (secondary, shear, slower, cannot pass through liquid — the S-wave “shadow zone” proved the outer core is liquid). Surface waves (Love and Rayleigh) cause the most damage. learn more
- Earth is about 4.54 billion years old (radiometric dating of meteorites — Clair Patterson, 1956). learn more
Plate tectonics
- Alfred Wegener (German meteorologist) proposed continental drift (1912; book The Origin of Continents and Oceans, 1915): all continents were once one supercontinent, Pangaea (“all lands”), surrounded by the ocean Panthalassa; it later split into Laurasia (north) and Gondwana (south). Evidence: jigsaw fit of South America and Africa, matching fossils (Mesosaurus, Glossopteris), rock formations, glacial scratches. He couldn't explain the mechanism and was largely rejected; he died on a Greenland expedition in 1930. continental drift · Pangaea
- Seafloor spreading (Harry Hess, early 1960s), magnetic striping on the seafloor (Vine–Matthews–Morley, 1963), and Marie Tharp's maps of the Mid-Atlantic Ridge led to the theory of plate tectonics by the late 1960s. plate tectonics · seafloor spreading
| Boundary | Motion | Features & examples | More |
|---|---|---|---|
| Divergent | Plates move apart | Mid-ocean ridges (Mid-Atlantic Ridge, Iceland), rift valleys (East African Rift); new crust forms | learn more |
| Convergent | Plates collide | Oceanic–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 |
| Transform | Plates slide past each other | Earthquakes; 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
| Type | Forms by | Examples | More |
|---|---|---|---|
| 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 |
| Sedimentary | Weathering, erosion, deposition, compaction and cementation of sediments; layers (strata); contain fossils | Sandstone, shale, limestone, conglomerate, chalk, coal, rock salt | learn more |
| Metamorphic (“change form”) | Heat and pressure transform existing rock without melting; often foliated (banded) | Limestone → marble; shale → slate; sandstone → quartzite; granite → gneiss; schist | learn 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
| Hardness | Mineral | Note | More |
|---|---|---|---|
| 1 | Talc | Softest; talcum powder | learn more |
| 2 | Gypsum | Drywall, plaster of Paris; fingernail ≈ 2.5 | learn more |
| 3 | Calcite | Limestone, marble; fizzes in acid; copper coin ≈ 3 | learn more |
| 4 | Fluorite | Glows under UV (gave us “fluorescence”) | learn more |
| 5 | Apatite | Same mineral family as tooth enamel; glass/knife ≈ 5.5 | learn more |
| 6 | Orthoclase feldspar | Most common mineral group in the crust | learn more |
| 7 | Quartz | SiO₂; scratches glass; amethyst | learn more |
| 8 | Topaz | Gemstone | learn more |
| 9 | Corundum | Al₂O₃ — ruby (red) and sapphire | learn more |
| 10 | Diamond | Hardest natural mineral; pure carbon | learn 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
- The focus (hypocenter) is where rupture starts underground; the epicenter is the point on the surface directly above. Locate the epicenter by triangulation from three seismograph stations using the P–S arrival gap. learn more
- Richter scale (Charles Richter with Beno Gutenberg, Caltech, 1935): logarithmic — each whole number = 10× the wave amplitude and about 32× the energy. learn more
- Moment magnitude scale (Mw; Hanks & Kanamori, 1979) has replaced Richter for large quakes and is what the USGS reports. learn more
- Modified Mercalli intensity scale (Roman numerals I–XII) rates shaking and damage at a location, not energy. learn more
- Largest recorded: 1960 Valdivia, Chile (Mw ≈ 9.5). Others: 1964 Alaska (9.2, largest in U.S.), 2004 Indian Ocean (≈ 9.1–9.3, tsunami), 2011 Tōhoku, Japan (≈ 9.0–9.1, Fukushima), 1906 San Francisco (≈ 7.9). learn more · lists
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
| Era | Period | Began (Ma) | Highlights | More |
|---|---|---|---|---|
| Paleozoic | Cambrian | 539 | “Cambrian explosion” of animal life; trilobites; Burgess Shale. Named for Cambria (Wales) | learn more |
| Ordovician | 485 | Marine invertebrates; first land plants; ends in mass extinction | learn more | |
| Silurian | 444 | Jawed fish; vascular plants | learn more | |
| Devonian | 419 | “Age of Fishes”; first tetrapods, forests | learn more | |
| Carboniferous | 359 | Coal 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 | |
| Permian | 299 | Pangaea assembled; ends with the Great Dying (~252 Ma), the largest mass extinction (~80–90%+ of marine species). Named for Perm, Russia | learn more | |
| Mesozoic | Triassic | 252 | First dinosaurs and mammals | learn more |
| Jurassic | 201 | Giant sauropods; Archaeopteryx; named for the Jura Mountains | learn more | |
| Cretaceous | 145 | Flowering 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 layer | learn more | |
| Cenozoic | Paleogene | 66 | Mammals diversify | learn more |
| Neogene | 23 | Grasslands spread; early hominins | learn more | |
| Quaternary | 2.6 | Ice 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 trend | Features | More |
|---|---|---|---|---|
| Troposphere | 0 – ~12 km (8 km at poles, ~17 km at equator) | Cools with height | All weather; ~75% of the atmosphere's mass; top = tropopause | learn more |
| Stratosphere | ~12 – 50 km | Warms with height | Ozone layer absorbs UV; jets cruise near its base; weather balloons | learn more |
| Mesosphere | ~50 – 85 km | Cools with height (coldest layer, ~−90 °C) | Meteors burn up here | learn more |
| Thermosphere | ~85 – 600 km | Warms sharply (can exceed 1,500 °C, though it wouldn't feel hot) | Auroras; the ISS orbits here (~400 km); contains most of the ionosphere | learn more |
| Exosphere | ~600 km – 10,000 km | — | Fades into space; many satellites | learn 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 / root | Meaning | Look & weather | More |
|---|---|---|---|
| Cirrus | “curl of hair” | High, thin, wispy ice crystals (“mares' tails”); fair weather but may signal an approaching warm front | learn more |
| Cumulus | “heap” | Puffy, flat-bottomed, cotton-ball; fair weather | learn more |
| Stratus | “layer” | Flat, gray sheets; drizzle; fog is stratus at ground level | learn 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, tornadoes | learn more |
| Alto- / cirro- | middle / high | Altocumulus, altostratus (mid-level); cirrocumulus, cirrostratus (high; halos around Sun/Moon) | learn more |
Weather & severe storms
- Fronts: cold front (blue line with triangles — cold air pushes under warm, fast; thunderstorms, then cooler), warm front (red line with semicircles — slow, long steady rain), stationary, occluded (purple). High pressure → generally fair; low pressure → storms. learn more
- Coriolis effect (Gaspard-Gustave de Coriolis): Earth's rotation deflects winds right in the Northern Hemisphere — hurricanes spin counterclockwise there (clockwise in the Southern). learn more
- Instruments: barometer (pressure — Torricelli, 1643), anemometer (wind speed), wind vane, hygrometer/psychrometer (humidity), rain gauge, thermometer, Doppler radar. Dew point = temperature at which air becomes saturated. barometer · anemometer
- Climate classification: Köppen system (Wladimir Köppen, 1884/1900). learn more
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
| Rating | Est. wind (mph) | Typical damage | More |
|---|---|---|---|
| EF0 | 65–85 | Light: shingles, branches | learn more |
| EF1 | 86–110 | Moderate: mobile homes overturned, roofs stripped | learn more |
| EF2 | 111–135 | Considerable: roofs torn off frame houses, large trees snapped | learn more |
| EF3 | 136–165 | Severe: entire stories of houses destroyed | learn more |
| EF4 | 166–200 | Devastating: well-built houses leveled | learn more |
| EF5 | > 200 | Incredible: houses swept off foundations | EF5 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
| Category | Sustained wind (mph) | More |
|---|---|---|
| 1 | 74–95 | learn more |
| 2 | 96–110 | learn more |
| 3 (“major”) | 111–129 | learn more |
| 4 | 130–156 | learn more |
| 5 | 157 or higher | Cat 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
↑ topThe 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
| Planet | Moons | Largest / notable moon | Day (rotation) | Year | Notable features (quiz clues) | More |
|---|---|---|---|---|---|---|
| Mercury | 0 | — | 58.6 Earth days (a solar day lasts 176) | 88 days | Smallest planet; closest to Sun; huge temperature swings; Caloris Basin; MESSENGER orbiter; named for the swift messenger god | learn more |
| Venus | 0 | — | 243 days, retrograde (longer than its year) | 225 days | Hottest 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 radar | learn more |
| Earth | 1 | The Moon | 23 h 56 min (sidereal) | 365.25 days | Densest planet (5.5 g/cm³); only known life; liquid surface water | learn more |
| Mars | 2 | Phobos and Deimos (“fear” and “dread”; found by Asaph Hall, 1877) | 24 h 37 min | 687 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 |
| Jupiter | 115 | Ganymede — largest moon in the solar system (bigger than Mercury) | ~9 h 56 min (shortest day) | 11.9 years | Largest 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 min | 29.4 years | Spectacular rings (ice; Cassini Division); least dense planet — would float in water; hexagon storm at north pole; Enceladus' ice geysers; Cassini–Huygens mission | learn more · moons |
| Uranus | 29 | Titania; moons named for characters of Shakespeare and Alexander Pope (Miranda, Oberon, Ariel, Umbriel) | ~17 h 14 min, retrograde | 84 years | Tilted ~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 |
| Neptune | 16 | Triton — orbits backward (retrograde), nitrogen geysers; likely a captured Kuiper belt object | ~16 h | 165 years | Found 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
- The IAU (meeting in Prague, Aug 24, 2006) defined a planet as a body that (1) orbits the Sun, (2) is round (hydrostatic equilibrium), and (3) has cleared its orbital neighborhood. Pluto fails #3 and was reclassified as a dwarf planet. The 2005 discovery of Eris (Mike Brown's team — “How I Killed Pluto”) — slightly smaller than Pluto but more massive — forced the decision. learn more
- The five recognized dwarf planets: Ceres (largest asteroid-belt object; first found, by Giuseppe Piazzi, Jan 1, 1801; Dawn mission), Pluto, Haumea (football-shaped, fast spin), Makemake, Eris (moon Dysnomia). learn more
- Pluto: discovered Feb 18, 1930 by Clyde Tombaugh at Lowell Observatory (Flagstaff, AZ) using a blink comparator; named by 11-year-old Venetia Burney of Oxford, England. Five moons: Charon (half Pluto's size, found 1978), Nix, Hydra, Kerberos, Styx. New Horizons flew by on July 14, 2015, revealing the heart-shaped Tombaugh Regio. learn more · Tombaugh Regio
- Asteroid belt (between Mars and Jupiter); Kuiper belt (beyond Neptune; Pluto, Arrokoth); Oort cloud (distant shell, source of long-period comets). Comets: icy “dirty snowballs” with tails pointing away from the Sun; Halley's Comet returns every ~76 years (last 1986, next 2061). Meteoroid (in space) → meteor (streak in sky) → meteorite (hits the ground). Kuiper belt · Halley's Comet · meteoroid
(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
- A G2V main-sequence star (“yellow dwarf”), ~4.6 billion years old, about halfway through its main-sequence life. Holds ~99.86% of the solar system's mass; diameter ~109 Earths; mass ~333,000 Earths. learn more
- Powered by nuclear fusion of hydrogen into helium (proton–proton chain) in the core (~15 million °C). Visible surface (photosphere) ~5,500 °C (5,772 K); the corona is over 1 million °C (the “coronal heating problem”). p–p chain
- Sunlight takes about 8 minutes 20 seconds to reach Earth. Sunspots (cooler, magnetic regions) follow an ~11-year cycle; solar flares and the solar wind cause auroras. sunspots · solar cycle
- NASA's Parker Solar Probe (launched 2018) made the closest-ever approach to the Sun on Dec 24, 2024, becoming the fastest human-made object. learn more
Stars
- Hertzsprung–Russell (H–R) diagram (Ejnar Hertzsprung & Henry Norris Russell, c. 1910–13) plots luminosity vs. temperature (hot on the left). Most stars lie on the diagonal main sequence; giants and supergiants at upper right; white dwarfs lower left. learn more
- Spectral classes: O B A F G K M, hottest (blue) to coolest (red) — “Oh Be A Fine Girl/Guy, Kiss Me.” Scheme finalized by Annie Jump Cannon at Harvard. The Sun is G2. learn more
- Magnitude: smaller (even negative) numbers are brighter (from Hipparchus). Apparent magnitude = how bright it looks; absolute magnitude = brightness at 10 parsecs. learn more
- Notable stars: Sirius (brightest in the night sky, “Dog Star,” Canis Major); Proxima Centauri (nearest star after the Sun, ~4.24 ly; part of the Alpha Centauri system); Polaris (North Star, end of the Little Dipper's handle — not especially bright); Betelgeuse (red supergiant in Orion's shoulder); Rigel (blue supergiant, Orion's foot); Vega. Sirius · Proxima · Polaris · Betelgeuse
Stellar life cycle
| Star mass | Path | More |
|---|---|---|
| Low / Sun-like | Nebula → protostar → main sequence → red giant → planetary nebula (outer layers shed) → white dwarf (Earth-sized, cooling) → (theoretical) black dwarf | learn 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 hole | supernova · neutron star · black hole |
- Chandrasekhar limit ≈ 1.4 solar masses — the maximum mass of a white dwarf. learn more
- A black hole's boundary of no return is the event horizon (radius = Schwarzschild radius). The Event Horizon Telescope released the first image of one (M87*) in April 2019, then Sagittarius A* (2022). John Wheeler popularized the term “black hole” (1967). learn more
- The Crab Nebula (M1) is the remnant of a supernova recorded by Chinese astronomers in 1054. learn more
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
| Law | Statement | Published | More |
|---|---|---|---|
| 1st — law of ellipses | Planets orbit in ellipses with the Sun at one focus. | Astronomia nova, 1609 | learn more |
| 2nd — law of equal areas | A line from Sun to planet sweeps out equal areas in equal times — planets move fastest at perihelion (closest), slowest at aphelion. | Astronomia nova, 1609 | learn more |
| 3rd — harmonic law | T² ∝ a³; with T in years and a in AU, T² = a³. A planet at 4 AU takes √64 = 8 years. | Harmonices Mundi, 1619 | learn more |
Distances
- Astronomical unit (AU): mean Earth–Sun distance ≈ 150 million km (93 million miles). learn more
- Light-year: the distance light travels in a year ≈ 9.46 × 10¹² km ≈ 5.88 trillion miles ≈ 63,000 AU. learn more
- Parsec: distance at which a star shows a parallax of one arcsecond ≈ 3.26 light-years. learn more
- “Standard candles” for measuring distance: Cepheid variable stars (Henrietta Leavitt's period–luminosity relation, 1912) and Type Ia supernovae. learn more
A light-year is a unit of distance, not time. learn more
Galaxies
- The Milky Way is a barred spiral galaxy ~100,000 light-years across with roughly 100–400 billion stars; the Sun is ~26,000 ly from the center, in the Orion Arm. At its center is the supermassive black hole Sagittarius A* (~4 million solar masses; Nobel 2020 to Reinhard Genzel and Andrea Ghez). learn more · Sgr A*
- Andromeda Galaxy (M31): nearest large spiral galaxy, ~2.5 million ly away; the most distant object easily visible to the naked eye; approaching the Milky Way and may merge with it in several billion years. Edwin Hubble proved it lies outside our galaxy (1920s), ending the “Great Debate” (Shapley vs. Curtis, 1920). learn more
- The Milky Way, Andromeda, Triangulum and dozens of dwarf galaxies (including the Large and Small Magellanic Clouds) form the Local Group. Hubble's tuning fork classifies galaxies as elliptical, spiral, barred spiral, (lenticular) and irregular. Local Group · Hubble sequence
The Big Bang & cosmology
- The universe began ~13.8 billion years ago. Belgian priest-physicist Georges Lemaître proposed the expanding universe and the “primeval atom” (1927–31). The name “Big Bang” was coined by rival Fred Hoyle (a steady-state supporter) on BBC radio in 1949. learn more
- Hubble's law (1929; now Hubble–Lemaître law): galaxies recede at speeds proportional to their distance, v = H₀d, H₀ ≈ 70 km/s per megaparsec (the exact value is disputed — the “Hubble tension”). learn more
- Cosmic microwave background (CMB): afterglow of the Big Bang at ~2.7 K, discovered accidentally by Arno Penzias and Robert Wilson at Bell Labs (1964–65; Nobel 1978) — they first suspected pigeon droppings in their antenna. Mapped by COBE, WMAP, Planck. learn more
- The universe is roughly 5% ordinary matter, 27% dark matter, 68% dark energy. Dark matter: Fritz Zwicky (1933), Vera Rubin's galaxy rotation curves (1970s). Dark energy: the expansion is accelerating (1998; Nobel 2011 to Perlmutter, Schmidt, Riess). dark matter · dark energy
Space exploration milestones
| Date | Mission / event | Clues | More |
|---|---|---|---|
| Oct 4, 1957 | Sputnik 1 (USSR) | First artificial satellite; started the Space Race. Sputnik 2 carried the dog Laika. | learn more |
| Jan 31, 1958 | Explorer 1 (USA) | First U.S. satellite; discovered the Van Allen radiation belts. NASA founded later in 1958. | learn more |
| Apr 12, 1961 | Vostok 1 | Yuri Gagarin, first human in space and in orbit. | learn more |
| May 5, 1961 | Freedom 7 (Mercury) | Alan Shepard, first American in space (suborbital). | learn more |
| Feb 20, 1962 | Friendship 7 (Mercury) | John Glenn, first American to orbit Earth. | learn more |
| June 16, 1963 | Vostok 6 | Valentina Tereshkova, first woman in space. | learn more |
| July 20, 1969 | Apollo 11 | Neil 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 1970 | Apollo 13 | Oxygen 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 1972 | Apollo 17 | Last 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 |
| 1977 | Voyager 1 & 2 | Grand 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 |
| 1981–2011 | Space Shuttle | First 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, 1990 | Hubble Space Telescope | Launched on Shuttle Discovery; flawed mirror fixed by astronauts in 1993; Hubble Deep Field. | learn more |
| 1997–2017 | Cassini–Huygens | NASA/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 Station | Continuously crewed since Nov 2, 2000; orbits ~400 km up about every 90 minutes. | learn more |
| 2006 / 2015 | New Horizons | Launched Jan 2006; first flyby of Pluto (July 14, 2015); then Kuiper belt object Arrokoth (Jan 1, 2019). | learn more |
| Dec 25, 2021 | James Webb Space Telescope | Infrared 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 / 2026 | Artemis program | Artemis 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
↑ topAbout 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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Archimedes | c. 287 – c. 212 BC | Greek (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 Galilei | 1564–1642 | Italian | Inclined-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 Huygens | 1629–1695 | Dutch | Wave theory of light (Huygens' principle); invented the pendulum clock (1656); discovered Titan and explained Saturn's rings (1655–59). | learn more |
| Robert Hooke | 1635–1703 | English | Hooke's law of springs; Micrographia (1665) — coined “cell” from cork; Royal Society curator of experiments; feuded with Newton. | learn more |
| Isaac Newton | 1643–1727 | English | Principia (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 Franklin | 1706–1790 | American | Kite experiment (1752) showing lightning is electricity; lightning rod; named positive/negative charge and “battery”; bifocals; Franklin stove; mapped the Gulf Stream. | learn more |
| Alessandro Volta | 1745–1827 | Italian | Voltaic pile (1800), the first electric battery (stacked zinc and copper disks); disputed Galvani's “animal electricity”; discovered methane. Unit: volt. | learn more |
| Georg Ohm | 1789–1854 | German | Ohm's law V = IR (1827). Unit: ohm (Ω). | learn more |
| Michael Faraday | 1791–1867 | English | Electromagnetic 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 Kelvin | 1824–1907 | British (born Belfast) | Absolute temperature scale; second law of thermodynamics; transatlantic telegraph cable; badly underestimated Earth's age. Unit: kelvin. | learn more |
| James Clerk Maxwell | 1831–1879 | Scottish | Maxwell'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 Hertz | 1857–1894 | German | First to produce and detect radio waves (1887), confirming Maxwell; observed the photoelectric effect. Unit: hertz. | learn more |
| Wilhelm Röntgen | 1845–1923 | German | Discovered 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 Becquerel | 1852–1908 | French | Discovered radioactivity (1896) when uranium salts fogged photographic plates in a drawer; shared 1903 Nobel with the Curies. Unit: becquerel. | learn more |
| J. J. Thomson | 1856–1940 | English | Discovered 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 Rutherford | 1871–1937 | New 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 Planck | 1858–1947 | German | Founder 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 Einstein | 1879–1955 | German-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 Bohr | 1885–1962 | Danish | Bohr 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 Schrödinger | 1887–1961 | Austrian | Wave 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 Heisenberg | 1901–1976 | German | Uncertainty principle (1927); matrix mechanics (1925); Nobel 1932; led Nazi Germany's nuclear program; subject of the play Copenhagen. | learn more |
| Enrico Fermi | 1901–1954 | Italian-American | Built 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 Oppenheimer | 1904–1967 | American | Scientific 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 Feynman | 1918–1988 | American | Quantum 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 Hawking | 1942–2018 | English | Hawking 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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Robert Boyle | 1627–1691 | Anglo-Irish | Boyle'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 Cavendish | 1731–1810 | English | Discovered 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 Priestley | 1733–1804 | English (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 Scheele | 1742–1786 | Swedish (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 Lavoisier | 1743–1794 | French | “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 Charles | 1746–1823 | French | Charles's law (V ∝ T); built and flew the first hydrogen balloon (1783). | learn more |
| John Dalton | 1766–1844 | English | Modern atomic theory (1803–08); law of partial pressures; law of multiple proportions; studied his own color blindness (“Daltonism”). Unit: dalton. | learn more |
| Amedeo Avogadro | 1776–1856 | Italian | Avogadro'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-Lussac | 1778–1850 | French | Pressure–temperature gas law; law of combining volumes (1808); record-setting hot-air/hydrogen balloon ascent (1804); co-discovered boron. | learn more |
| Humphry Davy | 1778–1829 | English | Used 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 Berzelius | 1779–1848 | Swedish | Invented modern letter symbols for elements; discovered silicon, selenium, cerium, thorium; coined “protein,” “polymer,” “catalysis,” “isomer.” | learn more |
| Friedrich Wöhler | 1800–1882 | German | Synthesized urea from ammonium cyanate (1828), undermining vitalism and launching organic chemistry; isolated aluminum and beryllium. | learn more |
| Robert Bunsen | 1811–1899 | German | Popularized the Bunsen burner (1855); with Kirchhoff founded spectroscopy and discovered cesium (1860) and rubidium (1861). | learn more |
| August Kekulé | 1829–1896 | German | Carbon's four bonds (tetravalence); ring structure of benzene (1865) — said to come from a daydream of a snake biting its tail. | learn more |
| Dmitri Mendeleev | 1834–1907 | Russian | Periodic 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 Ramsay | 1852–1916 | Scottish | Discovered the noble gases — argon (with Lord Rayleigh, 1894), helium on Earth (1895), neon, krypton, xenon (1898, with Morris Travers); Nobel 1904. | learn more |
| Svante Arrhenius | 1859–1927 | Swedish | Arrhenius acid–base definition; electrolytic dissociation (Nobel 1903); Arrhenius equation for reaction rates/activation energy; first calculated CO₂'s greenhouse warming (1896). | learn more |
| Fritz Haber | 1868–1934 | German | Haber 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. Lewis | 1875–1946 | American | Lewis 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 Hahn | 1879–1968 | German | Discovered 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 Moseley | 1887–1915 | English | Used 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 Julian | 1899–1975 | American | Synthesized 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 Pauling | 1901–1994 | American | The 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 Seaborg | 1912–1999 | American | Co-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 Sanger | 1918–2013 | English | Sequenced 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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Hippocrates | c. 460 – c. 370 BC | Greek (Kos) | “Father of medicine”; Hippocratic Oath; disease has natural causes; theory of four humors. | learn more |
| Andreas Vesalius | 1514–1564 | Flemish | De 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 Harvey | 1578–1657 | English | Discovered the circulation of blood pumped by the heart (De Motu Cordis, 1628); physician to James I and Charles I. | learn more |
| Antonie van Leeuwenhoek | 1632–1723 | Dutch | “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 Linnaeus | 1707–1778 | Swedish | “Father of taxonomy”; binomial nomenclature; Systema Naturae (1735); named Homo sapiens; classified plants by their reproductive parts. | learn more |
| Jean-Baptiste Lamarck | 1744–1829 | French | Early evolution theory — inheritance of acquired characteristics (giraffe necks; Philosophie zoologique, 1809); helped coin “biology”; classified invertebrates. | learn more |
| Edward Jenner | 1749–1823 | English | First 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 Darwin | 1809–1882 | English | Evolution 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 Semmelweis | 1818–1865 | Hungarian | “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 Mendel | 1822–1884 | Austrian (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 Pasteur | 1822–1895 | French | Germ 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 Wallace | 1823–1913 | British (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 Lister | 1827–1912 | English | Antiseptic surgery using carbolic acid (phenol), 1867, inspired by Pasteur; Listerine mouthwash is named after him. | learn more |
| Robert Koch | 1843–1910 | German | Koch'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 Pavlov | 1849–1936 | Russian | Classical conditioning — dogs salivating at a signal (bell, metronome); his Nobel (1904) was actually for research on digestion. | learn more |
| George Washington Carver | c. 1864–1943 | American | Agricultural 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 Morgan | 1866–1945 | American | Fruit-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 Landsteiner | 1868–1943 | Austrian-American | Discovered the ABO blood groups (1901) — made safe transfusions possible; co-discovered the Rh factor and the polio virus; Nobel 1930. | learn more |
| Elmer McCollum | 1879–1967 | American | (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 Fleming | 1881–1955 | Scottish | Discovered 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 Banting | 1891–1941 | Canadian | Co-discovered insulin (1921, Toronto) with Charles Best, transforming diabetes treatment; Nobel 1923 at age 32 (shared with J. J. R. Macleod). | learn more |
| Charles Drew | 1904–1950 | American | Developed 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 Salk | 1914–1995 | American | First 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 Crick | 1916–2004 | English | Co-discovered the DNA double helix (1953) with Watson; stated the “central dogma” (1958); helped crack the triplet genetic code; Nobel 1962. | learn more |
| James Watson | 1928–2025 | American | Co-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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Aristarchus of Samos | c. 310 – c. 230 BC | Greek | First known heliocentric (Sun-centered) model; estimated relative sizes and distances of the Sun and Moon. | learn more |
| Eratosthenes | c. 276 – c. 194 BC | Greek (Cyrene; librarian at Alexandria) | Measured Earth's circumference using shadow angles at Syene and Alexandria; sieve for primes; coined “geography.” | learn more |
| Claudius Ptolemy | c. 100 – c. 170 AD | Greco-Egyptian (Alexandria) | Almagest: Earth-centered (geocentric) universe with epicycles, accepted for ~1,400 years; also Geography. | learn more |
| Nicolaus Copernicus | 1473–1543 | Polish | Heliocentric 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 Brahe | 1546–1601 | Danish | Most 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 Kepler | 1571–1630 | German | Three 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 Halley | 1656–1742 | English | Predicted 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 Hutton | 1726–1797 | Scottish | “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 Messier | 1730–1817 | French | Comet hunter who cataloged 110 fuzzy non-comet objects (M1 = Crab Nebula, M31 = Andromeda, M42 = Orion Nebula, M45 = Pleiades). | learn more |
| William Herschel | 1738–1822 | German-born British | Discovered 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 Lyell | 1797–1875 | Scottish | Principles of Geology (1830–33) popularized uniformitarianism; strongly influenced Darwin, who read it on the Beagle. | learn more |
| Louis Agassiz | 1807–1873 | Swiss-American | Proposed past ice ages (glacial theory, 1837–40); studied fossil fish; founded Harvard's Museum of Comparative Zoology; opposed Darwin. | learn more |
| Urbain Le Verrier | 1811–1877 | French | Predicted 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 Wegener | 1880–1930 | German | Continental 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 Hubble | 1889–1953 | American | Showed “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 Lemaître | 1894–1966 | Belgian | Catholic priest who proposed the expanding universe (1927) and the “primeval atom” — the Big Bang theory. | learn more |
| Charles Richter | 1900–1985 | American | Richter magnitude scale (1935, Caltech, with Beno Gutenberg). | learn more |
| Harry Hess | 1906–1969 | American | Seafloor spreading (1962) using sonar data gathered as a U.S. Navy officer in WWII — key to plate tectonics; Princeton geologist. | learn more |
| Clyde Tombaugh | 1906–1997 | American | (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 Chandrasekhar | 1910–1995 | Indian-American | Chandrasekhar 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) | American | Father (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 Hoyle | 1915–2001 | English | Coined “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” Fujita | 1920–1998 | Japanese-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 Wilson | 1933–2024 / b. 1936 | American (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 Sagan | 1934–1996 | American | TV 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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Johannes Gutenberg | c. 1400–1468 | German (Mainz) | Movable-type printing press (c. 1440s–1450); Gutenberg Bible (c. 1455). | learn more |
| James Watt | 1736–1819 | Scottish | Separate condenser made steam engines far more efficient (patent 1769), powering the Industrial Revolution; partnered with Matthew Boulton; coined “horsepower.” Unit: watt. | learn more |
| Eli Whitney | 1765–1825 | American | Cotton gin (1793) — which expanded slavery in the South; promoted interchangeable parts for muskets. | learn more |
| Robert Fulton | 1765–1815 | American | First commercially successful steamboat, the Clermont (Hudson River, 1807); earlier built the submarine Nautilus. | learn more |
| George Stephenson | 1781–1848 | English | “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 Babbage | 1791–1871 | English | “Father of the computer”: Difference Engine and the programmable Analytical Engine (never completed); Ada Lovelace wrote its first program. | learn more |
| Samuel Morse | 1791–1872 | American | Electric 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 McCormick | 1809–1884 | American | Mechanical reaper (1831) that transformed grain harvesting on the Great Plains; company later part of International Harvester. | learn more |
| Alfred Nobel | 1833–1896 | Swedish | Invented 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 Benz | 1844–1929 | German | Benz Patent-Motorwagen (patented 1886), the first practical gasoline automobile; wife Bertha Benz made the first long-distance drive (1888). | learn more |
| George Westinghouse | 1846–1914 | American | Railway 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 Bell | 1847–1922 | Scottish-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 Edison | 1847–1931 | American | “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 Tesla | 1856–1943 | Serbian-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 Ford | 1863–1947 | American | Model T (1908); moving assembly line (1913); $5 workday (1914) — made cars affordable for the middle class. | learn more |
| Wilbur & Orville Wright | 1867–1912 / 1871–1948 | American (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 Marconi | 1874–1937 | Italian | Wireless telegraphy (radio); first transatlantic radio signal (1901, Cornwall to Newfoundland — the letter “S”); Nobel Physics 1909 with Karl Ferdinand Braun. | learn more |
| Walter Chrysler | 1875–1940 | American | (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 Cessna | 1879–1954 | American | (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 Goddard | 1882–1945 | American | Launched 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 Farnsworth | 1906–1971 | American | Invented 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 Braun | 1912–1977 | German-American | Designed 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 Turing | 1912–1954 | English | Turing 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 Kilby | 1923–2005 | American | (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-Lee | b. 1955 | English | Invented 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
| Name | Dates | Nationality | Known for (quiz clues) | More |
|---|---|---|---|---|
| Mary Anning | 1799–1847 | English | Fossil 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 Lovelace | 1815–1852 | English | Wrote 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 Mitchell | 1818–1889 | American | Discovered “Miss Mitchell's Comet” (1847) from Nantucket; first American woman professional astronomer; professor at Vassar. | learn more |
| Florence Nightingale | 1820–1910 | English | Founder 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 Blackwell | 1821–1910 | English-American | First woman to earn a medical degree in the U.S. (Geneva Medical College, 1849). | learn more |
| Annie Jump Cannon | 1863–1941 | American | Harvard “computer” who created the OBAFGKM stellar classification and classified ~350,000 stars; largely deaf. | learn more |
| Marie Curie | 1867–1934 | Polish-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 Leavitt | 1868–1921 | American | Harvard 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 Meitner | 1878–1968 | Austrian-Swedish | With 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 Noether | 1882–1935 | German | Noether'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 Earhart | 1897–1937 | American | (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-Gaposchkin | 1900–1979 | English-American | 1925 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 McClintock | 1902–1992 | American | Discovered transposons (“jumping genes”) in maize; unshared Nobel in Physiology or Medicine (1983). | learn more |
| Grace Hopper | 1906–1992 | American | Navy 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 Carson | 1907–1964 | American | Marine 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 Hodgkin | 1910–1994 | English | X-ray crystallography of penicillin, vitamin B₁₂ and insulin; Nobel Chemistry 1964. | learn more |
| Chien-Shiung Wu | 1912–1997 | Chinese-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 Johnson | 1918–2020 | American | NASA “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 Franklin | 1920–1958 | English | X-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 Tharp | 1920–2006 | American | Mapped 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 Rubin | 1928–2016 | American | Galaxy 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 Goodall | 1934–2025 | English | Six 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 Burnell | b. 1943 | Northern Irish | Discovered 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 Ride | 1951–2012 | American | Physicist and first American woman in space (STS-7, June 1983); served on the Challenger and Columbia accident boards. | learn more |
| Jennifer Doudna & Emmanuelle Charpentier | b. 1964 / b. 1968 | American / French | Developed 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
↑ topListed 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
| Experiment | Who / when | What was done | What it showed | More |
|---|---|---|---|---|
| Measuring the Earth | Eratosthenes, c. 240 BC | At 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 Tower | Galileo, c. 1590s–1630s | Rolled 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 barometer | Evangelista Torricelli, 1643 | Filled 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 hemispheres | Otto von Guericke, 1654 | Pumped 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 experiments | Isaac 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 flies | Francesco Redi, 1668 | Meat 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 experiment | Benjamin 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 vaccination | Edward Jenner, 1796 | Infected 8-year-old James Phipps with cowpox, then exposed him to smallpox. | Cowpox gives immunity to smallpox — the first vaccine. | learn more |
| Cavendish experiment | Henry Cavendish, 1797–98 | Torsion 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 experiment | Thomas Young, c. 1801–1803 | Light 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 compass | Hans Christian Ørsted, 1820 | A wire carrying current deflected a nearby compass needle. | Electric currents create magnetic fields — birth of electromagnetism. | learn more |
| Joule's paddle wheel | James Prescott Joule, 1840s | A 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 pendulum | Léon 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 peas | Gregor Mendel, 1856–1863 | Crossed 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 flask | Louis Pasteur, 1859–1862 | Boiled 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 experiment | Albert 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 dogs | Ivan Pavlov, 1890s–1900s | Paired a neutral stimulus (e.g., a metronome or bell) with food; dogs began salivating to the stimulus alone. | Classical conditioning. | learn more |
| Cathode-ray tube | J. J. Thomson, 1897 | Deflected 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 experiment | Robert Millikan (with Harvey Fletcher), 1909 | Balanced 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 experiment | Hans 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 expedition | Arthur 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 experiment | Frederick Griffith, 1928 | Heat-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-1 | Enrico 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 test | Manhattan Project (Oppenheimer), July 16, 1945 | Detonated “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 experiment | Alfred Hershey & Martha Chase, 1952 | Labeled 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 experiment | Stanley 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 experiment | Chien-Shiung Wu, 1956 | Measured 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 experiment | Matthew Meselson & Franklin Stahl, 1958 | Grew 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 detection | LIGO 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
↑ topThe Nobel Prizes
- Founded by the will (1895) of Alfred Nobel (1833–1896), the Swedish chemist who invented dynamite. First awarded in 1901; presented each year on December 10, the anniversary of his death. learn more
- Five original categories: Physics, Chemistry, Physiology or Medicine, Literature, and Peace. The Peace Prize is awarded in Oslo, Norway; the rest in Stockholm, Sweden. The Economics prize (Sveriges Riksbank Prize in Economic Sciences in Memory of Alfred Nobel) was created in 1968 and first given in 1969 — technically not a “Nobel Prize.” There is no Nobel for mathematics (see the Fields Medal). economics
- Firsts (1901): Physics — Wilhelm Röntgen (X-rays); Chemistry — Jacobus van 't Hoff; Medicine — Emil von Behring (diphtheria antitoxin); Peace — Henry Dunant (Red Cross founder) and Frédéric Passy. Prizes are not awarded posthumously (since 1974) and at most three people may share one. list of laureates
| Multiple / notable winners | Prizes | More |
|---|---|---|
| Marie Curie | Physics 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 Pauling | Chemistry 1954 (chemical bond) and Peace 1962 (campaign against nuclear testing) — only person with two unshared Nobels. | learn more |
| John Bardeen | Physics 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 Sanger | Chemistry 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 Cross | Peace 1917, 1944, 1963 — the most Peace prizes. | learn more |
| Curie family | Marie 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 pairs | The Braggs (shared Physics 1915; Lawrence Bragg was 25); Niels (1922) & Aage Bohr (1975); J. J. (1906) & G. P. Thomson (1937). | learn more |
| Albert Einstein | Physics 1921 (awarded in 1922) — for the photoelectric effect, not relativity. | learn more |
| (Kansas) Kansas-connected laureates | Jack 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 / principle | Field | In a nutshell | More |
|---|---|---|---|
| Archimedes' principle | Fluids | Buoyant force = weight of displaced fluid | learn more |
| Pascal's principle | Fluids | Pressure on an enclosed fluid is transmitted equally everywhere (hydraulics) | learn more |
| Bernoulli's principle | Fluids | Faster-moving fluid has lower pressure | learn more |
| Hooke's law | Mechanics | F = −kx for springs | learn more |
| Newton's laws | Mechanics | Inertia; F = ma; action–reaction; universal gravitation | learn more |
| Kepler's laws | Astronomy | Elliptical orbits; equal areas; T² ∝ a³ | learn more |
| Hubble's law | Cosmology | v = H₀d — galaxies recede in proportion to distance | learn more |
| Snell's law | Optics | n₁ sin θ₁ = n₂ sin θ₂ | learn more |
| Doppler effect | Waves | Frequency shifts with relative motion of source and observer | learn more |
| Ohm's law | Electricity | V = IR | learn more |
| Coulomb's law | Electricity | F = kq₁q₂/r² | learn more |
| Kirchhoff's circuit laws | Electricity | Current into a junction = current out; loop voltages sum to zero | learn more |
| Faraday's law | Magnetism | A changing magnetic flux induces a voltage | learn more |
| Lenz's law | Magnetism | Induced current opposes the change that caused it | learn more |
| Boyle's law | Gases | P₁V₁ = P₂V₂ (constant T) | learn more |
| Charles's law | Gases | V₁/T₁ = V₂/T₂ (constant P) | learn more |
| Gay-Lussac's law | Gases | P₁/T₁ = P₂/T₂ (constant V) | learn more |
| Avogadro's law | Gases | Equal volumes of gas (same T, P) contain equal numbers of molecules | learn more |
| Dalton's law | Gases | Total pressure = sum of partial pressures | learn more |
| Graham's law | Gases | Effusion rate ∝ 1/√(molar mass) | learn more |
| Henry's law | Solutions | Gas solubility ∝ its partial pressure (why soda fizzes when opened; “the bends”) | learn more |
| Le Chatelier's principle | Equilibrium | A system at equilibrium shifts to relieve an applied stress | learn more |
| Hess's law | Thermochemistry | Total enthalpy change is the same regardless of the reaction path (Germain Hess, 1840) | learn more |
| Hund's rule | Electron configuration | Electrons fill equal-energy orbitals singly before pairing | learn more |
| Pauli exclusion principle | Quantum | No two electrons share all four quantum numbers | learn more |
| Heisenberg uncertainty principle | Quantum | Can't know position and momentum exactly at once: Δx·Δp ≥ ħ/2 | learn more |
| Mendel's laws | Genetics | Segregation, independent assortment, dominance | learn more |
| Hardy–Weinberg principle | Genetics | Allele frequencies stay constant without evolutionary forces: p² + 2pq + q² = 1 | learn more |
| Steno's law of superposition | Geology | In undisturbed strata, lower layers are older | learn more |
| Moore's law | Technology | Transistors 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