Chapter 16 Toward a New Heaven and a New Earth: The Scientific Revolution and the Emergence of Modern Science.

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Chapter 16 Toward a New Heaven and a New Earth:
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Chapter 16 Toward a New Heaven and a New Earth: The Scientific Revolution and the Emergence of Modern Science

A nineteenth-century painting of Galileo before the Holy Office in the Vatican in 1633

Background to the Scientific Revolution Ancient Authors and Renaissance Artists Limitations in the perspectives of medieval scientists The Renaissance and ancient knowledge Contradictions of medieval authorities Close observation of nature Perspective and anatomical proportions Technological Innovations and Mathematics Creating a framework for innovation Renaissance Magic Hermetic magic and alchemical thought

Toward a New Heaven: a Revolution in Astronomy Medieval Cosmological Views Based on Aristotle, Ptolemy, and Christian theology Geocentric conception Concentric spheres with fixed earth at center Nicolaus Copernicus (1473 – 1543) On The Revolution of the Heavenly Spheres Observation and heliocentric conception The conservatism of Copernicus Creates doubt about the Ptolemaic system

Medieval Conception of the Universe Medieval Conception of the Universe. As this sixteenth-century illustration shows, the medieval cosmological view placed the earth at the center of the universe, surrounded by a series of concentric spheres. The earth was imperfect and constantly changing, whereas the heavenly bodies that surrounded it were perfect and incorruptible. Beyond the tenth and final sphere was heaven, where God and all the saved souls were located. (The circles read, from the center outward: 1. Moon, 2. Mercury, 3. Venus, 4. Sun, 5. Mars, 6. Jupiter, 7. Saturn, 8. Firmament (of the Stars), 9. Crystalline Sphere, 10. Prime Mover; and around the outside, Empyrean Heaven—Home of God and All the Elect, that is, saved souls.) p478

The Copernican System The Copernican System. The Copernican system was presented in On the Revolutions of the Heavenly Spheres, published shortly before Copernicus’s death. As shown in this illustration from the first edition of the book, Copernicus maintained that the sun was the center of the universe and that the planets, including the earth, revolved around it. Moreover, the earth rotated daily on its axis. (The circles read, from the inside out: 1. Sun; 2. Mercury, orbit of 80 days; 3. Venus; 4. Earth, with the moon, orbit of one year; 5. Mars, orbit of 2 years; 6. Jupiter, orbit of 12 years; 7. Saturn, orbit of 30 years; 8. Immobile Sphere of the Fixed Stars.) p479

Toward a New Heaven: a Revolution in Astronomy Tycho Brahe (1546 – 1601) Johannes Kepler (1571 – 1630) Hermetic thought and mathematical magic Laws of planetary motion Discrediting the Aristotelian-Ptolemaic system Eliminating the idea of uniform circular motion Galileo Galilei (1564 – 1642) The telescope and The Starry Messenger Galileo and the Inquisition Galileo and the problem of motion The principle of inertia

Johannes Kepler Johannes Kepler. Abandoning theology in favor of mathematics and astronomy, Kepler became a key figure in the rise of the new astronomy. Using Tycho Brahe’s vast store of astronomical data, Kepler discovered the three laws of planetary motion that both confirmed and modified the Copernican theory. They also eliminated the Aristotelian- Ptolemaic ideas of uniform circular motion and crystalline spheres moving in circular orbits. This portrait was done by an unknown painter three years before Kepler’s death. p481

The Telescope The Telescope. The invention of the telescope enabled Europeans to inaugurate a new age in astronomy. Shown here is Johannes Hevelius (huh-VAY-lee-uss), an eminent German-Polish astrologer (1611–1697), making an observation with his telescope. Hevelius’s observations were highly regarded. He located his telescope on the roof of his own house, and by the 1660s, his celestial observatory was considered one of the best in Europe. The photograph above shows Galileo’s original telescope, built in 1609. p483

The Telescope The Telescope. The invention of the telescope enabled Europeans to inaugurate a new age in astronomy. Shown here is Johannes Hevelius (huh-VAY-lee-uss), an eminent German-Polish astrologer (1611–1697), making an observation with his telescope. Hevelius’s observations were highly regarded. He located his telescope on the roof of his own house, and by the 1660s, his celestial observatory was considered one of the best in Europe. The photograph above shows Galileo’s original telescope, built in 1609. p483

Isaac Newton (1642 – 1727) Early Achievements Newton and the Occult Invention of calculus Mathematical Principles of Natural Philosophy, or Principia (1684 – 1686) Newton and the Occult Universal Law of Gravitation A new cosmology Three laws of motion Consequences: world seen in mechanistic terms God and Newton’s world-machine

Isaac Newton Isaac Newton. With a single law, that of universal gravitation, Isaac Newton was able to explain all motion in the universe. His great synthesis of the work of his predecessors created a new picture of the universe, one in which the universe was viewed as a great machine operating according to natural laws. Enoch Seeman painted this portrait of Newton one year before his death. p487

Advances in Medicine and Chemistry Paracelsus (1493 – 1541) Rejection of Aristotle and Galen The macrocosmic-microcosmic principle Andreas Vesalius (1514 – 1564) On the Fabric of the Human Body (1543) Based on dissection of a human body William Harvey (1578 – 1657) On the Motion of the Heart and Blood (1628) Chemistry Robert Boyle (1627 – 1691) Antoine Lavoisier (1743 – 1794)

Women in the Origins of Modern Science Margaret Cavendish (1623 – 1673) Observations upon Experimental Philosophy Grounds of Natural Philosophy Attacks on rationalist and empiricist approaches to scientific knowledge Maria Sibylla Merian (1647 – 1717) Entomology and the craft tradition Maria Winkelmann (1670 – 1720) Achievements in astronomy Difficulties with the Berlin Academy

CHRONOLOGY Important Works of the Scientific Revolution

Debates on the Nature of Women The Querelles des Femmes Tradition: women as inherently base, prone to vice, easily swayed, and “sexually insatiable” Challenges to tradition Women joined debate in the 17th century, rejecting this view The impact of science The new anatomy Women’s loss of traditional spheres of influence Reaffirmation of traditional ideas about the nature of women

Maria Merian and the Insects of Surinam Maria Merian and the Insects of Surinam. Shown in the engraving is a portrait of Maria Merian, the German naturalist and illustrator, whose study and detailed paintings of plants and insects, especially the transformation of caterpillars into butterflies, attracted scientific attention. The illustration from Merian’s Metamorphosis of the Insects of Surinam (Plate 55), depicting a bell pepper plant, caterpillar, and butterfly, shows her meticulous attention to detail. p492

Maria Merian and the Insects of Surinam Maria Merian and the Insects of Surinam. Shown in the engraving is a portrait of Maria Merian, the German naturalist and illustrator, whose study and detailed paintings of plants and insects, especially the transformation of caterpillars into butterflies, attracted scientific attention. The illustration from Merian’s Metamorphosis of the Insects of Surinam (Plate 55), depicting a bell pepper plant, caterpillar, and butterfly, shows her meticulous attention to detail. p492

Toward a New Earth: Descartes, Rationalism, and a New View of Humankind Rene Descartes (1596 – 1650) Reflections on doubt and uncertainty Discourse on Method (1637) “I think, therefore I am.” Separation of mind and matter Cartesian Dualism Consequences: the birth of modern rationalism

Descartes Descartes. Rene´ Descartes was one of the primary figures in the Scientific Revolution. Claiming to use reason as his sole guide to truth, Descartes posited a sharp distinction between mind and matter. He is shown here in a portrait done around 1649 by Frans Hals, one of the painters of the Dutch golden age who was famous for his portraits, especially that of Descartes. p493

The Scientific Method and the Spread of Scientific Knowledge Francis Bacon (1561 – 1626) Rejection of Copernicus and Kepler; Misunderstanding of Galileo The Great Instauration and correct scientific method Built on inductive principles, proceeding from the particular to the general Experimentation and domination of nature Descartes Deduction and mathematical logic Newton’s unification of Bacon’s empiricism and Descartes rationalism

Louis XIV and Colbert Visit the Academy of Sciences Louis XIV and Colbert Visit the Academy of Sciences. In the seventeenth century, individual scientists received royal and princely patronage, and a number of learned societies were established. In France, Louis XIV, urged on by his controller general, Jean- Baptiste Colbert, gave formal recognition to the French Academy in 1666. In this painting by Henri Testelin, Louis XIV is shown seated, surrounded by Colbert and members of the French Royal Academy of Sciences. p495

The Royal Observatory at Greenwich The Royal Observatory at Greenwich. To facilitate their astronomical investigations, both the English and the French constructed observatories such as the one pictured here, which was built at Greenwich, England, in 1675. Here the royal astronomer works at the table while his two assistants make observations. p496

The Scientific Method and the Spread of Scientific Knowledge The Scientific Societies English Royal Society Informal meetings at London and Oxford Received formal charter in 1662 from Charles II French Royal Academy Informal meetings in Paris Formally recognized by Louis XIV (1666) Contributions Recognition of the practical value of scientific research Focus on theoretical work in mechanics and astronomy

The Scientific Method and the Spread of Scientific Knowledge Science and Society People recognized science’s rational superiority Economic implications Science offered new ways to exploit resources for profit Science as a part of elite culture Political implications Linking the scientific conception of the natural world to social stability Patronage to bolster military applications

Science and Religion Tensions between Science and Religion Benedict de Spinoza (1632 – 1677) Philosophy of pantheism (monism) Reason creates happiness and freedom Blaise Pascal (1623 – 1662) Sought unity of science and religion Pensées (Thoughts) Sought to convert rationalists to Christianity Christianity not contrary to reason Reason had limits

CHRONOLOGY Consequences of the Scientific Revolution: Important Works

Blaise Pascal Blaise Pascal. Blaise Pascal was a brilliant scientist and mathematician who hoped to keep science and Christianity united. In his Pense´es, he made a passionate argument on behalf of the Christian religion. He is pictured here in a portrait by Philippe de Champaigne, a well-known French portrait painter of the Baroque period. p498

Chapter Timeline p500

Discussion Questions How did the Middle Ages and the Renaissance contribute to the Scientific Revolution? Why were advances in mathematics so important during the Scientific Revolution? Why did religious leaders react so negatively to the new advances in Science, especially in astronomy? Why is Newton’s Principia called the “hinge point of modern scientific thought”? How did women come to play such an important role in the Scientific Revolution? Why did scientific societies refuse to recognize women involved in the sciences?