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ASTRONOMY 9: HISTORY OF COSMOLOGY

Handout #12

J. E. Baker
UC Berkeley, Spring 2000

Cosmology in the Middle Ages

1.
Early Middle Ages (approx. 200-1200 AD)
2.
Cosmic Innovation in Arabia (approx. 700-1250 AD)
(a)
Adalusian school (Iberian peninsula)
  • Followers of Aristotle's physics: uniform, geocentric, circular motion is only natural possibility
  • Rejected Ptolemaic equant (non-uniform), epicycles and eccentric (not geocentric) as against physical principles
  • Reverted to Aristotelian model with concentric spheres
  • Predictions for planets off by up to 21$^\circ$!
(b)
Maragha school (Persia)
  • Desired to improve accuracy of Ptolemaic model with new data and mathematical tricks
  • al-Tusi (d. 1274) invented Tusi couple
    • Combination of two circles, one smaller inside the other
    • Can produce variety of motion, even linear!
  • Ptolemy's eccentric and equant replaced with Tusi couples
  • Back to uniform circular motion, with little loss of accuracy
3.
Late Middle Ages and Early Renaissance (approx. 1200-1500)

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next up previous
Up: Astronomy 9 Lecture Notes
jonathan baker
2000-02-23