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Callippus was a Greek astronomer who lived around the 4th century BCE. He was a student of Eudoxus of Cnidus and made improvements to his teacher's model of celestial motion. Eudoxus's theory of homocentric spheres, which described celestial bodies as being carried on concentric spheres, was modified by Callippus to better account for planetary movements, particularly for Mercury and Venus. While Eudoxus's model was influential in cosmology, it failed to explain observed brightness changes in planets, suggesting their distances from Earth varied. Callippus's refinements were part of the ongoing effort in ancient Greek astronomy to "save the phenomena" by creating mathematical models that could predict celestial movements using uniform circular motion.12

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