Atlas/Timeline

History of Physics

Twenty-six centuries of matter, motion, and light on one screen — the experiments, laws, and revolutions that revealed how the universe works.

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Ancient Physics600 BCE500 CE
Medieval & Islamic Physics500 CE1400 CE
The Scientific Revolution1400 CE1700 CE
Classical Mechanics1700 CE1800 CE
Fields & Thermodynamics1800 CE1900 CE
Relativity & Quantum1900 CE1950 CE
Particles & Cosmology1950 CE2000 CE
Contemporary Physics2000 CE2025 CE
500 BCE
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250 CE
500 CE
750 CE
1000 CE
1250 CE
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2000 CE

Each star is a thinker or work; solid lines draw the constellation of a school, dashed threads the passage of ideas between eras.

Select any point on the timeline to read about it.

All entries by era

Ancient Physics 600 BCE500 CE

Greek natural philosophers seek the principles behind motion, matter, and the heavens; Archimedes turns statics and buoyancy into exact law.

  • 624 BCE – 546 BCE

    He noticed that rubbed amber attracts light bodies and that lodestone draws iron — the first recorded observations of electricity and magnetism.

  • 384 BCE – 322 BCE

    His Physics framed motion, cause, place, and the elements for two thousand years — a system so complete it had to be overthrown to move forward.

  • 287 BCE – 212 BCE

    He founded statics and hydrostatics, stating the law of the lever and the buoyancy principle that still bears his name.

  • 100 CE – 170 CE

    His Almagest gave a mathematical model of the heavens, and his Optics tabulated the refraction of light — quantitative physics of vision.

Medieval & Islamic Physics 500 CE1400 CE

Scholars from Cairo to Paris rebuild optics on experiment and question Aristotle's account of falling bodies and projectile motion.

  • 965 CE – 1040 CE

    His Book of Optics showed that vision works by light entering the eye and pioneered controlled experiment — a founder of the scientific method.

  • 1301 CE – 1358 CE

    His theory of 'impetus' held that a thrown body keeps an impressed force — a medieval step toward the modern concept of inertia and momentum.

The Scientific Revolution 1400 CE1700 CE

Copernicus, Galileo, Kepler, and Newton replace the closed cosmos with a mathematical universe governed by universal laws of motion.

  • 1473 CE – 1543 CE

    He placed the Sun, not the Earth, at the centre of the planetary system, setting off the revolution that remade physics and cosmology.

  • 1543 CE

    Published in the year of his death, this book moved the Earth into motion and gave astronomy a Sun-centred mathematical framework.

  • 1564 CE – 1642 CE

    By measuring falling and rolling bodies and turning the telescope on the sky, he made experiment and mathematics the language of physics.

  • 1571 CE – 1630 CE

    From Tycho Brahe's data he derived three laws of planetary motion, showing that orbits are ellipses obeying exact mathematical rules.

  • 1629 CE – 1695 CE

    He built the pendulum clock, worked out centripetal force, and proposed that light travels as a wave — a rival to Newton's corpuscles.

  • 1643 CE – 1727 CE

    His three laws of motion and universal gravitation unified the heavens and the Earth under one mathematics, founding classical physics.

  • 1687 CE

    Perhaps the most important book in the history of science: it stated the laws of motion and gravity and derived Kepler's laws from them.

Classical Mechanics 1700 CE1800 CE

Newtonian mechanics is recast in the powerful language of analysis, while the first laws of gases and electrostatics take shape.

  • 1627 CE – 1691 CE

    His experiments with the air-pump gave the first gas law relating pressure and volume, bridging physics and the new chemistry.

  • 1736 CE – 1813 CE

    His Analytical Mechanics recast Newton's laws as elegant equations derived from energy, a form still used across modern physics.

  • 1736 CE – 1806 CE

    With a torsion balance he measured the force between electric charges, giving electrostatics its precise inverse-square law.

Fields & Thermodynamics 1800 CE1900 CE

Heat, energy, electricity, and magnetism are unified into fields and conservation laws — Maxwell's equations crown classical physics.

  • 1791 CE – 1867 CE

    He discovered electromagnetic induction and introduced the idea of the field — invisible lines of force filling space around charges and magnets.

  • 1796 CE – 1832 CE

    His analysis of the ideal heat engine founded thermodynamics and revealed the deep limit on how much heat can become work.

  • 1818 CE – 1889 CE

    His precise experiments measured the mechanical equivalent of heat, establishing that energy is conserved as it changes form.

  • 1831 CE – 1879 CE

    He unified electricity, magnetism, and light in four equations, predicting electromagnetic waves and crowning classical physics.

  • 1844 CE – 1906 CE

    He explained heat and entropy as the statistics of countless moving atoms, founding statistical mechanics against fierce opposition.

  • 1873 CE

    Maxwell's masterwork laid out the complete field theory of electromagnetism, the foundation of all later electrical technology.

  • 1897 CE

    J. J. Thomson showed cathode rays are streams of tiny negatively charged particles — the first subatomic particle, opening the atomic age.

Relativity & Quantum 1900 CE1950 CE

Relativity remakes space and time; quantum theory remakes matter and light. The two deepest revolutions in the history of physics.

  • 1858 CE – 1947 CE

    To explain the glow of hot bodies he proposed that energy comes in discrete quanta — the reluctant birth of quantum theory in 1900.

  • 1871 CE – 1937 CE

    His gold-foil experiment revealed the tiny dense atomic nucleus, and he later achieved the first artificial transmutation of an element.

  • 1879 CE – 1955 CE

    In one 'miracle year' he explained the photoelectric effect, Brownian motion, and special relativity, then remade gravity as curved spacetime.

  • 1885 CE – 1962 CE

    His model of the atom with quantized electron orbits explained the spectral lines and shaped the philosophy of quantum mechanics.

  • 1902 CE – 1984 CE

    His relativistic equation for the electron predicted antimatter, uniting quantum mechanics with special relativity and founding quantum field theory.

  • 1905 CE

    Einstein's 1905 paper made the speed of light absolute and space and time relative, giving the famous relation between mass and energy.

  • 1915 CE

    Einstein's field equations recast gravity as the curvature of spacetime by mass and energy, predicting bending light and an evolving cosmos.

  • 1925 CE – 1926 CE

    Heisenberg's matrix mechanics and Schrödinger's wave equation gave quantum theory its full mathematics; uncertainty replaced classical certainty.

Particles & Cosmology 1950 CE2000 CE

The Standard Model orders the particle zoo while the Big Bang, the cosmic microwave background, and black holes map the universe at large.

  • 1889 CE – 1953 CE

    He proved that galaxies lie far beyond the Milky Way and are rushing apart, giving the first evidence of an expanding universe.

  • 1918 CE – 1988 CE

    His diagrams and formulation of quantum electrodynamics made the interaction of light and matter calculable to astonishing precision.

  • 1942 CE – 2018 CE

    He showed that black holes are not wholly black but slowly radiate, forging a deep link between gravity, quantum theory, and thermodynamics.

  • 1964 CE

    Penzias and Wilson detected the faint afterglow of the Big Bang, turning cosmology from speculation into an observational science.

  • 1973 CE

    A single quantum field theory brought quarks, leptons, and three forces into one framework — the most tested theory in all of physics.

Contemporary Physics 2000 CE2025 CE

Giant detectors confirm the Higgs boson and catch gravitational waves, opening a new era of precision and multi-messenger astronomy.

  • 2012 CE

    The Large Hadron Collider found the particle that gives mass to matter, completing the Standard Model nearly fifty years after its prediction.

  • 2015 CE

    LIGO caught ripples in spacetime from two merging black holes, confirming Einstein's century-old prediction and opening a new astronomy.

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