The Scientific Revolution (1550-1700) (SparkNotes History Note)
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SparkNotes History Guides help students strengthen their grasp of history by focusing on individual eras or episodes in U.S. or world history. Breaking history up into digestible lessons, the History Guides make it easier for students to see how events, figures, movements, and trends interrelate. SparkNotes History Guides are perfect for high school and college history classes, for students studying for History AP Test or SAT Subject Tests, and simply as general reference tools. Each note contains a general overview of historical context, a concise summary of events, lists of key people and terms, in-depth summary and analysis with timelines, study questions and suggested essay topics, and a 50-question review quiz.
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The Scientific Revolution (1550-1700) (SparkNotes History Note) - SparkNotes
General Summary
For the long centuries of the Middle Ages (500-1350 AD) the canon of scientific knowledge had experienced little change, and the Catholic Church had preserved acceptance of a system of beliefs based on the teachings of the ancient Greeks and Romans which it had incorporated into religious doctrine. During this period there was little scientific inquiry and experimentation. Rather, students of the sciences simply read the works of the alleged authorities and accepted their word as truth. However, during the Renaissance this doctrinal passivity began to change. The quest to understand the natural world led to the revival of botany and anatomy by thinkers such as Andreas Vesalius during the later sixteenth century.
These scientific observers were surprised to find that their conclusions did not always match up with the accepted truths, and this finding inspired others to delve further into the study of the world around them. Scientific study quickly extended from the earth to the heavens, and Nicolas Copernicus, upon examining the records of the motions of heavenly bodies, soon discarded the old geocentric theory that placed the Earth at the center of the solar system and replaced it with a heliocentric theory in which the Earth was simply one of a number of planets orbiting the sun. Though this scheme seemed to comply better with the astronomical records of the time, Copernicus had little direct evidence to support his claims. Not ready to abandon traditional beliefs, the forces of tradition, in the form of the Church and the mass of Europeans, kept the heliocentric theory from achieving full acceptance. The theory awaited the advancement of mathematics and physics to support its claims.
The wait was not very long. During the early seventeenth century, mathematics experienced a great deal of progress in the form of the development of algebra, trigonometry, the advance of geometry, and the linkage of form and motion with quantifiable numeric values undertaken by Rene Descartes. Armed with these tools, the science of physics began to advance rapidly. During the late sixteenth century Galileo Galilei demonstrated that gravity accelerated all objects toward the Earth at the same rate, and further explored the laws of motion. Other physicists explored the nature of matter, with the greatest advances coming in the understanding of the properties of gases, leading to the invention of the barometer, thermometer, and air pump. Physicists even strove (largely unsuccessfully) to discover the structure of matter on the atomic scale.
One of the first applications of the knowledge gained from the advance of physics was in the realm of biology. The physiology of the human body could now be understood in terms of its mechanical properties, and during the seventeenth century many of the mysteries of the human body disappeared. However, the most notable application of the laws of physics was in the field of astronomy. Johannes Kepler proved the orbits of the planets were elliptical, but was unable to come up with an effective model of the solar system. That was left to Galileo, who in 1630 published his Dialogue on the Two Chief Systems of the World, in which he supported the Copernican, or heliocentric theory of the universe, and denounced the Aristotelian system, which maintained the geocentric theory. Galileo supported his claims with elaborate evidence derived from the study of physics.
Sir Isaac Newton's work was the capstone of this evolving chain of science. He integrated Kepler's laws of planetary motion and Galileo's forays into the laws of gravity into a comprehensive understanding of the organization of the universe according to the law of universal gravitation. Newton's Principia, in which he lays out this comprehensive system of organization and develops the mathematical field of calculus, is seen as the key which unlocked the mysteries of the universe, the climax of the strivings of all of the Scientists of the Scientific Revolution.
Context
The Middle Ages were long centuries of stability in the intellectual world. All scientific and philosophical expression was monitored extensively by, and most often produced from within, the Church. During the Middle Ages, the Church ruled conclusively on a number of truths about the natural world, which it claimed were undeniable. These alleged truths were produced by Biblical study and the widely accepted Aristotelian system, which became official Church doctrine. The Aristotelian system defined the laws of physics erroneously in many cases. It claimed that the rate of fall of an object was determined by its weight, held that matter was constructed out of four possible elements, with different matter containing different combinations of these four, and described the universe as the Greek astronomer Ptolemy had described it, as a static and finite thing in which the Earth occupied the central position, with the sun and planets in revolution and the distant stars inhabiting its farthest edges. The physicians of the period considered that the human body contained four different kinds of liquid and that illness was caused by the imbalance of these 'humors.' These truths went generally unquestioned for years, backed up by the teachings of the Church and the common teaching of the educational institutions of the era.
With the rise of the Renaissance, new interest sparked in reference to the physical world. In part boosted by the spirit of geographical exploration, which dominated Europe and provided many new specimens for study and experimentation, the artists