From the epicycles of the Greeks to Kepler's ellipse - The breakdown of the circle paradigm
Dino Boccaletti (University of Rome "La Sapienza")

TL;DR
This paper discusses the historical shift from the circle paradigm in astronomy to Kepler's elliptical orbits, highlighting Kepler's groundbreaking analysis that led to the rejection of circular models in favor of ellipses, foundational for Newtonian physics.
Contribution
It provides a detailed analysis of Kepler's methodological breakthrough in establishing elliptical orbits, marking a fundamental shift in astronomical modeling.
Findings
Kepler established that Mars's orbit is an ellipse.
The shift from circular to elliptical orbits was crucial for Newtonian physics.
Kepler's analysis exemplifies rigorous scientific modeling based on observations.
Abstract
The principle that celestial bodies must move on circular orbits or on paths resulting from the composition of circular orbits has been assumed as a constant guide in the astronomical thougth of the peoples facing the Mediterranean sea as from the second century B.C. until the beginning of the XVII century. The mathematical model based on such an assumption, the theory of epicycles in all its versions and modifications, has been taken as a scheme for all astronomical calculations during at least eighteen centuries, from Hipparcus to Kepler. As it is known, in Astronomia Nova (1609), Kepler succeded to establish the two laws which after him were named the first and the second Kepler's laws. The revolution he performed by giving up the circle paradigm is of fundamental importance and represents the indispensable premise to Newtonian theory. This revolution, the result of what Kepler…
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Taxonomy
TopicsHistorical Astronomy and Related Studies · Historical Geography and Cartography · History and Theory of Mathematics
