Famous laws of science

22 items · Ages 12+

22 laws. Many were found by more than one person; the item notes say who else, and the matching accepts the other names. Years are when the law was first stated or published.

A scientific law is a short statement of something nature always does, tested again and again. These are the ones that turn up in every physics and chemistry class, and knowing who found them, and when, ties science to history.

How to learn it

Encode the meaning before the name: for each law, picture the everyday scene in the hook and say the law in your own words (narration). Then hang it on a timeline, chunked by century, so the people line up in order: Archimedes alone in the ancient world, then Kepler, Boyle, Hooke and Newton in the 1600s, and so on. Retrieve it by explaining one law a day to someone else.

Encode make it vivid → Space bring it back on day 1, 3, 7, 21 → Retrieve pull it from your head. From the infographic Remember It on Purpose.

Famous laws of science

LawWhoYearWhat it says
Archimedes' principleArchimedesc. 250 BCAnything in water or another fluid is pushed up by a force equal to the weight of the fluid it pushes aside.
Kepler's first lawJohannes Kepler1609Each planet travels around the Sun in an ellipse (a stretched circle), with the Sun at one focus, a little off center.
Kepler's second lawJohannes Kepler1609A line from the Sun to a planet sweeps out equal areas in equal times, so a planet moves faster when it is nearer the Sun.
Kepler's third lawJohannes Kepler1619The farther a planet is from the Sun, the longer its year: the square of its year is proportional to the cube of its average distance.
Snell's law (refraction)Willebrord Snellius1621When light passes from one clear material into another, it bends by an amount set by how much each material slows it.
Note: Ibn Sahl described the same rule in about AD 984. Snellius did not publish it; René Descartes published it in 1637.
Boyle's lawRobert Boyle1662At a steady temperature, squeeze a gas into half the space and its pressure doubles: pressure times volume stays the same.
Note: Richard Towneley and Henry Power found the same relation about a year earlier, and Edme Mariotte independently in 1676.
Hooke's lawRobert Hooke1678A spring stretches in proportion to the force pulling it, as long as it is not stretched too far.
Newton's first law of motionIsaac Newton1687An object stays still, or keeps moving in a straight line at the same speed, unless a force acts on it.
Newton's second law of motionIsaac Newton1687Force equals mass times acceleration (F = ma): the same push speeds up a light object more than a heavy one.
Newton's third law of motionIsaac Newton1687When one object pushes on another, the second pushes back just as hard in the opposite direction.
Newton's law of universal gravitationIsaac Newton1687Every mass pulls on every other mass, more strongly for bigger masses and more weakly with distance (one over the distance squared).
Bernoulli's principleDaniel Bernoulli1738Where a moving fluid speeds up, its pressure drops.
Note: Published in his book Hydrodynamica.
Coulomb's lawCharles-Augustin de Coulomb1785Electric charges push apart if alike and pull together if opposite, with a force that weakens with the square of the distance.
Charles's lawJacques Charles1787At a steady pressure, a gas expands as it warms: its volume is proportional to its absolute temperature.
Note: Charles did the work around 1787 but did not publish it; Joseph Louis Gay-Lussac published the law in 1802 and credited him.
Law of conservation of massAntoine Lavoisier1789In a chemical reaction, matter is not created or destroyed: the total mass stays the same.
Note: Mikhail Lomonosov showed the same idea decades earlier, but his work was less known. Lavoisier stated it in his 1789 textbook.
Avogadro's lawAmedeo Avogadro1811Equal volumes of gases, at the same temperature and pressure, hold the same number of molecules.
Note: André-Marie Ampère reached nearly the same idea in 1814.
Ohm's lawGeorg Simon Ohm1827The current through a wire equals the voltage across it divided by its resistance (I = V / R).
Faraday's law of inductionMichael Faraday1831A changing magnetic field through a loop of wire makes an electric current flow in the wire.
Law of conservation of energy (first law of thermodynamics)Hermann von Helmholtz1847Energy is never created or destroyed; it only changes from one form to another.
Note: Built on work by Julius Robert von Mayer (1842) and James Prescott Joule (1840s); Rudolf Clausius wrote it as the first law of thermodynamics in 1850.
Second law of thermodynamicsRudolf Clausius1850Heat flows on its own from hot to cold, never from cold to hot; some energy always spreads out as unusable heat.
Note: Lord Kelvin gave another form of it in 1851, building on Sadi Carnot (1824).
Mendel's laws of inheritanceGregor Mendel1865Each parent passes on one of its two copies of each gene, by chance; genes for different traits are often passed on independently.
Note: Presented in 1865 and published in 1866; mostly overlooked until 1900.
Hubble-Lemaître lawEdwin Hubble1929Distant galaxies are moving away from us, and the farther away a galaxy is, the faster it is moving away.
Note: Georges Lemaître proposed it in 1927; Hubble published the observations in 1929. The International Astronomical Union recommended the name Hubble-Lemaître law in 2018.

Encode the meaning before the name: for each law, picture the everyday scene in the hook and say the law in your own words (narration). Then hang it on a timeline, chunked by century, so the people line up in order: Archimedes alone in the ancient world, then Kepler, Boyle, Hooke and Newton in the 1600s, and so on. Retrieve it by explaining one law a day to someone else. · teddyrookbook.com/memory/challenges/scientific-laws/

Sources

Checked October 30, 2026. Progress is kept on this device only (per learner). More lists: all memory challenges · memory games.

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