In fact the Copernican theory was no more accurate than the Ptolemaic model. It had no compelling physical arguments for its superiority, and it proposed no experiments for testing its novel features. In some respects, it was actually less accurate, as more epicycles had to be added (in place of Ptolemy's [[equant]]). Copernicus' main argument in favor of his theory was that it was aesthetically more pleasing as it allowed the planets to move in uniform circular motion, an idea later proven false by Kepler. Many of the ancient Greek arguments for and against [[heliocentrism]] remained unresolved for some time. <ref>Ancient Greeks objected to Aristarchus's heliocentrim because (1) we don't feel the Earth's motion, (2) unattached objects don't fly off, and (3) no annual stellar parallax. [http://physics.gmu.edu/~jevans/astr103/CourseNotes/history_greekGeocentricHeliocentric.html] Stellar parallax was not measured until 1838, while (1) and (2) were resolved by the work of [[Isaac Newton]].</ref> | In fact the Copernican theory was no more accurate than the Ptolemaic model. It had no compelling physical arguments for its superiority, and it proposed no experiments for testing its novel features. In some respects, it was actually less accurate, as more epicycles had to be added (in place of Ptolemy's [[equant]]). Copernicus' main argument in favor of his theory was that it was aesthetically more pleasing as it allowed the planets to move in uniform circular motion, an idea later proven false by Kepler. Many of the ancient Greek arguments for and against [[heliocentrism]] remained unresolved for some time. <ref>Ancient Greeks objected to Aristarchus's heliocentrim because (1) we don't feel the Earth's motion, (2) unattached objects don't fly off, and (3) no annual stellar parallax. [http://physics.gmu.edu/~jevans/astr103/CourseNotes/history_greekGeocentricHeliocentric.html] Stellar parallax was not measured until 1838, while (1) and (2) were resolved by the work of [[Isaac Newton]].</ref> |