Nicolaus Copernicus
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Among the great [[polymath]]s of the [[Renaissance]], Copernicus was a [[mathematician]], [[astronomer]], [[physician]], [[classical scholar]], [[translator]], [[Roman Catholic Church|Catholic cleric]], [[jurist]], [[governor]], [[military|military leader]], [[diplomacy|diplomat]] and [[economist]]. Amid his extensive responsibilities, astronomy figured as little more than an avocation — yet it was in that field that he made his mark upon the world. | Among the great [[polymath]]s of the [[Renaissance]], Copernicus was a [[mathematician]], [[astronomer]], [[physician]], [[classical scholar]], [[translator]], [[Roman Catholic Church|Catholic cleric]], [[jurist]], [[governor]], [[military|military leader]], [[diplomacy|diplomat]] and [[economist]]. Amid his extensive responsibilities, astronomy figured as little more than an avocation — yet it was in that field that he made his mark upon the world. | ||
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+ | Despite the near universal acceptance today of the basic heliocentric idea (though not the epicycles or the circular orbits), Copernicus' theory was originally slow to catch on. Scholars hold that sixty years after the publication of ''The Revolutions'' there were only around 15 astronomers espousing Copernicanism in all of Europe: "[[Thomas Digges]] and [[Thomas Harriot]] in England; [[Giordano Bruno]] and [[Galileo Galilei]] in Italy; [[Diego de Zúñiga|Diego Zuniga]] in Spain; [[Simon Stevin]] in the Low Countries; and in Germany, the largest group – [[Georg Joachim Rheticus]], [[Michael Maestlin]], [[Christoph Rothmann]] (who may have later recanted), and [[Johannes Kepler]]." Additional possibilities are Englishman [[William Gilbert (astronomer)|William Gilbert]], along with [[Achilles Gasser]], Georg Vogelin, [[Valentin Otto]], and [[Tiedemann Giese]]. | ||
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Nicolaus Copernicus (February 19, 1473 – May 24, 1543) was the first astronomer to formulate a scientifically based heliocentric cosmology that displaced the Earth from the center of the universe. His epochal book, De revolutionibus orbium coelestium (On the Revolutions of the Celestial Spheres), is often regarded as the starting point of modern astronomy and the defining epiphany that began the Scientific Revolution.
Although Greek, Indian and Muslim savants had published heliocentric hypotheses centuries before Copernicus, his publication of a scientific theory of heliocentrism, demonstrating that the motions of celestial objects can be explained without putting the Earth at rest in the center of the universe, stimulated further scientific investigations, and became a landmark in the history of modern science that is known as the Copernican Revolution.
Among the great polymaths of the Renaissance, Copernicus was a mathematician, astronomer, physician, classical scholar, translator, Catholic cleric, jurist, governor, military leader, diplomat and economist. Amid his extensive responsibilities, astronomy figured as little more than an avocation — yet it was in that field that he made his mark upon the world.
Despite the near universal acceptance today of the basic heliocentric idea (though not the epicycles or the circular orbits), Copernicus' theory was originally slow to catch on. Scholars hold that sixty years after the publication of The Revolutions there were only around 15 astronomers espousing Copernicanism in all of Europe: "Thomas Digges and Thomas Harriot in England; Giordano Bruno and Galileo Galilei in Italy; Diego Zuniga in Spain; Simon Stevin in the Low Countries; and in Germany, the largest group – Georg Joachim Rheticus, Michael Maestlin, Christoph Rothmann (who may have later recanted), and Johannes Kepler." Additional possibilities are Englishman William Gilbert, along with Achilles Gasser, Georg Vogelin, Valentin Otto, and Tiedemann Giese.