History · Depth 2 · Introductory · 3 min read
Scientific Revolution
The 16th–17th century shift to an orderly, rational universe: Copernicus, Galileo, Kepler and Newton, and the scholars across cultures they built on.
On this page
What was the Scientific Revolution?
In the 16th and 17th centuries, a series of discoveries established a new view of the universe: that it was orderly and rational, and could be understood through observation and reason.[1] Those ideas went on to shape the Enlightenment of the 18th century.[1]
From an Earth-centred to a Sun-centred universe
Nicolaus Copernicus (1473–1543) concluded that Earth is a planet and that all the planets circle the Sun. His book On the Revolutions of the Celestial Orbs was published in 1543, the year he died.[2]
Galileo’s telescope
Galileo Galilei (1564–1642) turned a telescope to the sky and found strong evidence for the new picture:[2]
- Four moons orbiting Jupiter, taking from just under 2 days to about 17 days to go around.
- Phases of Venus, like the Moon’s, showing that Venus must orbit the Sun.
- A rugged Moon, with craters, mountain ranges, valleys and flat, dark areas.
Galileo also studied motion, and realised that a force is needed not just to start something moving, but also to slow it down, stop it, speed it up or change its direction.[2] His ideas brought him into conflict with the Church. He was condemned to house arrest, and only in 1992 did the Catholic Church publicly admit that it had erred.[2]
Kepler’s laws
Tycho Brahe recorded the positions of the Sun, Moon and planets for almost 20 years.[3] His assistant, Johannes Kepler (1571–1630), spent more than 20 years analysing that data, and published his first two laws of planetary motion in 1609 in The New Astronomy.[3] His first law states that each planet moves around the Sun in an ellipse, with the Sun at one focus.[3] See Kepler’s Laws on the map.
Newton’s synthesis
Isaac Newton (1643–1727) brought it all together. His Principia, published in 1687 at Edmond Halley’s expense, set out three laws of motion meant to govern the motions of all objects.[4]
New ways of knowing
The revolution was also about method. Francis Bacon championed inductive reasoning, reaching conclusions only after collecting evidence. René Descartes combined deductive reasoning with empiricism, helping establish the foundations of the scientific method.[1]
A global inheritance
The Scientific Revolution did not come from nowhere. Medieval Persian mathematicians such as Muhammad ibn Musa al-Khwarizmi and Omar Khayyam provided intellectual tools, the Indian philosopher Aryabhata played a pivotal role in trigonometry, and the decimal number system from classical India and fractions in the Arabic numeral systems of North Africa made advanced calculation possible.[1] The Enlightenment that followed was the result of cross-cultural networks of scholarship.[1]
Real-life examples
Venus has phases
Through his telescope, Galileo saw Venus go through phases like the Moon, showing it must orbit the Sun.[2]
Moons around another world
Galileo discovered four moons circling Jupiter, taking from just under 2 days to about 17 days per orbit: clearly not everything circles Earth.[2]
An apology 350 years late
Galileo was condemned to house arrest. Not until 1992 did the Catholic Church publicly admit it had erred.[2]
A book paid for by a friend
Newton's Principia, which laid out his laws of motion, was published in 1687 at Edmond Halley's expense.[4]
Go deeper
2 of 3 topics below this one are written so far. The rest are uncharted: on the map, but not yet written. The Atlas is growing.
- Johannes KeplerJohannes Kepler (1571–1630) used Tycho Brahe's observations to discover that planets move in ellipses, and wrote the three laws of planetary motion.
- Isaac NewtonIsaac Newton (1643–1727) set out the laws of motion and the law of universal gravitation in his Principia, published in 1687.
- Galileo Galilei
Connected across the map
- Scientific Method
- Solar SystemThe Sun and everything bound to it: eight planets, five dwarf planets, hundreds of moons, and more than a million asteroids and comets.4 branches
- Kepler's LawsThree rules for how planets move: in ellipses, sweeping equal areas in equal times, with bigger orbits taking predictably longer (P² = a³).
Learn more
Short descriptions are our own summaries. The resources belong to, and are run by, their publishers.
- World History Volume 2: from 1400 (free textbook) ↗
by OpenStax
A free, peer-reviewed world history textbook covering 1400 to the present, including the Scientific Revolution.
- Astronomy 2e (free textbook) ↗
by OpenStax
A free, peer-reviewed introductory astronomy textbook, from the night sky to galaxies.
Evidence & sources
Supported by academic sources such as university textbooks and peer-reviewed research.
Why this level? This page summarises mainstream history from peer-reviewed university textbooks. History also involves interpretation, which is why we don't class it as Established.
This is a Knowledge Atlas editorial classification of the sources we could find, not a certificate of truth. How we evaluate knowledge
Sources
Based on 4 sources from 1 institution: OpenStax.
Show all 4 sourcesHide the list
- ScholarlyOpenStax (Rice University)· Academic publisherWorld History Volume 2, 7.1 The EnlightenmentOpened and checked against this page on 28 Sept 2026 · License: CC BY-NC-SA 4.0
- ScholarlyOpenStax (Rice University)· Academic publisherAstronomy 2e, 2.4 The Birth of Modern AstronomyOpened and checked against this page on 28 Sept 2026 · License: CC BY-NC-SA 4.0
- ScholarlyOpenStax (Rice University)· Academic publisherAstronomy 2e, 3.1 The Laws of Planetary MotionOpened and checked against this page on 28 Sept 2026 · License: CC BY-NC-SA 4.0
- ScholarlyOpenStax (Rice University)· Academic publisherAstronomy 2e, 3.2 Newton’s Great SynthesisOpened and checked against this page on 28 Sept 2026 · License: CC BY-NC-SA 4.0