Early Modern Europe – 1450 to 1750
The law of ellipses is a fundamental principle in celestial mechanics that states that planets move in elliptical orbits around the sun, with the sun located at one of the foci of the ellipse. This concept was introduced by Johannes Kepler and marked a significant departure from the previously held belief in circular orbits, reshaping the understanding of planetary motion within the heliocentric model proposed by Copernicus.
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