John Dee 1527 A.D. – 1608 A.D. English mathematician and astronomer, Dee drew on traditional magic and Hermetic philosophy, he believed the universe was governed by mathematical principles. William Gilbert 1544 A.D. – 1603 A.D. English physician and natural philosopher who supported Copernicus and was highly critical of Aristotelian physics. He realized that electricity and magnetism were related but separate phenomena, summarizing his discoveries in de Magnete. Tycho Brahe 1546 A.D. – 1601 A.D. Danish nobleman who built the best observatory of its time at Hveen. His instruments provided far better measurements of planetary positions and provided Kepler with the detailed data leading to his three laws of planetary motion. Giordano Bruno 1548 A.D. – 1600 A.D. Italian philosopher and astronomer who supported the Copernican theory but also believed that the sun was only one of many similar stars, and not at the center of the universe. He was convicted of heresy and burned at the stake for his religious views, not primarily for his support of heliocentricity. Galileo Galilei 1564 A.D. – 1642 A.D. Italian physicist and astronomy who promoted the Copernican heliocentric theory and criticized Aristotelian mechanics, fighting the opposition of Italian physicists who thought Galileo was also criticizing the Church’s interpretation of Scripture. Nicolaus Copernicus Johannes Kepler 1473 A.D. – 1543 A.D. 1571 A.D. – 1630 A.D. Polish scientist who proposed a heliocentric model of the universe to replace the geocentric model popularized by Ptolemy. While it was not possible to prove Copernicus’ theory by direct observational evidence for several centuries, the theory became the most popular explanation of planetary motion. German mathematician and astronomer who realized that planets move in ellipses with speed that varies with distance from the sun, and that distance and periodicity are related by a specific relationship. Isaac Newton 1643 A.D. – 1727 A.D. English physicist, mathematician, and astronomer whose Principia Mathematic demonstrated the consistency between his own theory of gravity and Kepler’s laws of planetary motion. He also developed the mathematical calculus, a method of rate analysis Scientific Revolution in Astronomy 1475 A.D. 1480 A.D. 1485 A.D. 1490 A.D. 1495 A.D. 1500 A.D. 1505 A.D. 1510 A.D. 1515 A.D. 1520 A.D. 1525 A.D. 1530 A.D. 1535 A.D. 1540 A.D. 1545 A.D. 1550 A.D. 1555 A.D. 1560 A.D. 1565 A.D. 1570 A.D. 1575 A.D. 1580 A.D. 1585 A.D. 1590 A.D. 1595 A.D. 1600 A.D. 1605 A.D. 1610 A.D. 1615 A.D. 1620 A.D. 1625 A.D. 1630 A.D. 1635 A.D. 1640 A.D. 1645 A.D. 1650 A.D. 1655 A.D. 1660 A.D. 1665 A.D. 1670 A.D. 1675 A.D. 1680 A.D. 1685 A.D. 1690 A.D. 1695 A.D. 1700 A.D. 1705 A.D. 1710 A.D. 1715 A.D.
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