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B. The World, 1450–1650 · The World, 1450–1650

Beginnings of the Scientific Revolution

B3 B1 A1 A1.7About 70 minutes
Learning goals
  • I can explain the geocentric model and why it was accepted.
  • I can describe the contributions of Copernicus, Vesalius, Tycho, Kepler, Galileo, Bacon, Harvey and Descartes.
  • I can describe astronomical work outside Europe in this period.
  • I can evaluate the label "Scientific Revolution" and the Galileo affair using historical perspective.

Words to know

geocentric
Earth-centred model of the universe.
heliocentric
Sun-centred model of the solar system.
humours
In Galen's medicine, four body fluids whose balance was thought to determine health.
induction
Reasoning from many observations to a general conclusion.
deduction
Reasoning from general principles to specific conclusions.
recant
To publicly withdraw a belief or statement.
Inquisition
Catholic Church courts that investigated and punished heresy.

Moons that should not exist

In January 1610, the Italian mathematician Galileo Galilei pointed a telescope he had built at Jupiter. Night after night he saw four small "stars" beside it that changed position. He concluded they were moons orbiting Jupiter. That was a problem for the accepted picture of the universe, in which everything circled the Earth.

His little book Sidereus Nuncius (The Starry Messenger, 1610) sold out quickly. Within twenty-five years he would be on trial in Rome. This lesson explores how new ways of studying nature began between 1450 and 1650. (The story continues with Newton and the Enlightenment in the sibling unit The World, 1650–1789.)

The old picture

Most educated Europeans, Muslims and Jews in 1500 relied on the ancient Greek thinkers Aristotle and Ptolemy, as developed by medieval Islamic and Christian scholars:

  • Geocentric universe: the Earth sits still at the centre; the Moon, Sun, planets and stars move around it in perfect circles.
  • Heavens versus Earth: the heavens were perfect and unchanging; the Earth was the place of change and decay.
  • Medicine: the Roman physician Galen taught that health depended on balancing four humours (blood, phlegm, yellow bile, black bile).
  • Method: knowledge came mainly from authoritative texts and logical reasoning from them.

This system was not foolish: it explained everyday observations (the Sun does seem to move) and made workable predictions.

Two models of the cosmos (orbits not to scale)Geocentric (Ptolemy)Centre: Earth1. Moon2. Mercury3. Venus4. Sun5. Mars6. Jupiter7. SaturnHeliocentric (Copernicus)Centre: Sun1. Mercury2. Venus3. Earth + Moon4. Mars5. Jupiter6. Saturn
In the geocentric model the Earth is at the centre, circled in order by the Moon, Mercury, Venus, the Sun, Mars, Jupiter and Saturn. In the heliocentric model the Sun is at the centre and the Earth is a planet, with the Moon orbiting it.

Astronomy beyond Europe

Astronomy was a global science:

  • In Samarkand, the Timurid ruler Ulugh Beg built a great observatory in the 1420s and produced a star catalogue of high accuracy.
  • Astronomers of the Maragha observatory in Iran (1200s), such as Nasir al-Din al-Tusi, devised mathematical models to fix problems in Ptolemy's system. Very similar devices appear in Copernicus's work; historians still debate whether he learned of them from earlier Islamic work (and if so, how) or reached them independently.
  • In Istanbul, Taqi al-Din built an observatory in 1577; it was demolished in 1580 after religious and political opposition.
  • In Ming China, the Jesuit Matteo Ricci and the scholar-official Xu Guangqi translated the first books of Euclid's geometry into Chinese (1607), and the court later used Jesuits to reform the calendar.
  • Earlier Mesoamerican peoples, including the Maya, had tracked Venus and eclipses with great precision.

Key steps, 1543 to 1637

  • 1543: Nicolaus Copernicus, a Polish cleric, published On the Revolutions of the Heavenly Spheres, arguing that the Sun, not the Earth, is near the centre and the Earth orbits it. He still used perfect circles. Few people accepted it at first.
  • 1543: Andreas Vesalius published On the Fabric of the Human Body, based on his own dissections, with superb printed illustrations. He showed that Galen, who had dissected mainly animals, made errors about human anatomy.
  • 1572 to 1601: Tycho Brahe made the most accurate naked-eye observations ever; a new star (a supernova) in 1572 suggested the heavens could change.
  • 1609 and 1619: Johannes Kepler, using Tycho's data, showed that planets move in ellipses, not circles, and found mathematical laws for their motion.
  • 1610: Galileo reported mountains on the Moon and moons around Jupiter; soon after, he observed the phases of Venus, which fit a Sun-centred system but not Ptolemy's.
  • 1620: Francis Bacon argued in Novum Organum that knowledge should be built by careful observation and experiment, reasoning upward from many facts (induction).
  • 1628: William Harvey showed that the heart pumps blood in a circuit around the body.
  • 1637: René Descartes, in Discourse on the Method, argued for doubting everything not certain and reasoning step by step from clear first principles (deduction), using mathematics.
A new method for knowledge (Bacon's ideal, simplified)ObservecarefullyForm ahypothesisTest byexperimentAnalyseresultsRevise orshare
Bacon's approach stressed evidence over authority. Real scientists rarely follow such neat steps, but the ideal of testing ideas against nature spread.

Galileo and the Church

Galileo argued openly for Copernicus. In 1616 the Catholic Church declared the idea that the Earth moves to be contrary to Scripture and warned Galileo not to hold or defend it. In 1632 he published the Dialogue Concerning the Two Chief World Systems, which seemed to mock the geocentric view. In 1633 he was tried by the Inquisition, forced to recant (publicly reject) the idea, and kept under house arrest until his death in 1642.

Historical perspective: it is easy to tell this as "science versus religion". Historians show it was more complicated: many churchmen were astronomers and some supported him; Galileo's proofs were not yet conclusive; the trial happened during the Thirty Years' War and Counter-Reformation fears about authority, and Galileo had offended a former ally, Pope Urban VIII. The Catholic Church formally acknowledged its errors in the case in 1992.

Why "revolution"? A debated label

The term Scientific Revolution suggests a sudden, complete break. Some historians reject it: change took 150 years or more; leading figures also practised astrology and alchemy (Kepler cast horoscopes; Newton later studied alchemy); and many ideas built on Islamic and medieval scholarship. Others keep the term because the period truly changed how knowledge was made: by observation, experiment, mathematics and printed sharing of results. Either way, by 1650 the old certainty that ancient authorities were right had been broken.

Worked example

Modelled example: Continuity and change in knowledge

How much did European ideas about the universe change between 1500 and 1650?

  1. Changes: heliocentrism had strong supporters (Kepler, Galileo); ellipses replaced perfect circles; the heavens were shown to change (Tycho's new star); the telescope revealed new objects; experiment and mathematics gained authority.
  2. Continuities: most people, including most university teachers, still held the geocentric view in 1650; the Church banned heliocentric books; astrology remained popular; the reasons planets moved were still unexplained (Newton came in 1687).
  3. Who changed? A small network of scholars, connected by printing and letters.
  4. Judgement: big change among experts; limited change in general belief.

Sample thesis: "Between 1500 and 1650 a small group of scholars overturned the ancient picture of the universe, but most Europeans' beliefs changed little until the late 1600s; the revolution was in method more than in popular opinion."

Just for fun

Galileo named Jupiter's four largest moons the Medicean Stars to honour the Medici family, who then gave him a job. Later astronomers renamed them Io, Europa, Ganymede and Callisto. Flattering your boss works, but the name may not last.

Hands-on activity

Observe like Galileo

You need: a clear evening, binoculars if you have them (any pair works), a notebook, warm clothes in winter; 15 minutes on three or four nights. Never look at the Sun, with or without binoculars.

  1. Check a free sky app or website to see whether Jupiter is visible this month. Ask a grown-up to go out with you.
  2. Steady the binoculars against a fence or a car roof. Look for tiny dots in a line beside Jupiter: those are its moons.
  3. Sketch Jupiter and the dots each night, with the date and time.
  4. Compare your sketches: do the dots move? (If Jupiter is not visible, sketch the Moon's phases over a week instead.)

Look for: careful, dated records, the essence of the new method. Ask: what would someone who believed everything orbits the Earth make of moving moons around Jupiter?

Your turn

1

What is the geocentric model?

2

What did Copernicus argue in 1543?

3

What did Vesalius show about Galen?

4

What did Kepler discover about planetary orbits?

5

What did Galileo observe in 1610?

6

What happened to Galileo in 1633?

7

Give one example of astronomy outside Europe in this period.

More practice: warm-up

1

Which Roman physician's ideas dominated medicine in 1500?

2

Who made the most accurate naked-eye observations of the period?

3

Who described the circulation of blood in 1628?

4

Who argued for knowledge built by observation and experiment in 1620?

5

What does "recant" mean?

More practice: on your own

1

Explain why the geocentric model was reasonable for its time.

2

Why was the phase cycle of Venus important evidence?

3

Compare Bacon's and Descartes's methods.

4

Why is "science versus religion" too simple for the Galileo affair?

5

How did printing help the new science? Give an example.

Challenge

1

Evaluate whether "Scientific Revolution" is a good label for 1543 to 1650.

2

Use historical perspective to explain why many educated people rejected Copernicus in the 1500s.

3

Assess the significance of non-European contributions to the beginnings of the Scientific Revolution.

Check your understanding

Quiz

1.

Which model placed the Sun near the centre with the Earth orbiting it?

2.

What did Kepler show about planetary orbits?

3.

Which discovery by Galileo challenged the idea that everything orbits the Earth?

4.

What was Vesalius's main contribution?

5.

Francis Bacon promoted knowledge built mainly from:

6.

Which statement about the Galileo trial reflects historians' current view?

For parents and teachers

Big idea: This lesson covers the beginnings of the Scientific Revolution for B3 (new ideas and key individuals) and B1 (intellectual developments), and practises evaluating the label "revolution" and continuity and change (A1, A1.7). The story continues in the sibling unit The World, 1650–1789.

How to help: Go outside on a clear night together. Ask: How would you prove the Earth moves, using only what you see?

Safety: never look at the Sun with or without binoculars; an adult should supervise night-time observing.

Common difficulties: assuming people before 1543 were simply ignorant; telling the Galileo story as pure science-versus-religion.