It is probably not exaggerate to say that after the wonderful successes pioneered by the Greek astronomers, mathematicians, and physicists, the renaissance of sciences in the 16th century came through the study of the movements of the planets on their trajectory around the Sun. Together with Copernicus’ heliocentric conception, the three Kepler laws provided a clear and essential framework for astronomy.

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Two-Body Problems

  • Peter Richmond,
  • Bertrand Roehner

摘要

It is probably not exaggerate to say that after the wonderful successes pioneered by the Greek astronomers, mathematicians, and physicists, the renaissance of sciences in the 16th century came through the study of the movements of the planets on their trajectory around the Sun. Together with Copernicus’ heliocentric conception, the three Kepler laws provided a clear and essential framework for astronomy.