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Abstract

One of the first converts to Kepler’s elliptic astronomy was a young Englishman, Jeremiah Horrocks (or Horrox). He was born in 1619 at Toxteth, then a small village near Liverpool, and was educated at Emmanuel College, Cambridge. Horrocks’s goal was to correct Kepler’s theories of planetary motions in order to bring them into closer agreement with observation.1 Perhaps his most important work was in devising an accurate theory of the motion of the Moon. He also devoted much effort to understanding the motion of Venus. In October 1639, Horrocks was at Hoole, Lancashire, a rather desolate site, bordered by a morass on the east and Marton Mere and the Douglass River on the south. There he repeated the calculations of the times of the planet’s transits. Kepler had predicted no such events until 1761, but Horrocks found that a transit was due to take place on November 24, 1639 (old style; the new style date is December 4, 1639). He and his friend, William Crabtree, a draper and fellow astronomer at Broughton near Manchester, succeeded in observing it—thus becoming sole witnesses of an event not to be repeated for 122 years.

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Notes and References

  1. For information on Horrocks, the following have been consulted: Rev. Arundell Blount Whatton, Memoir of the Life and Labours of the Rev. Jeremiah Horrox (London, 1859),

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© 1997 Richard Baum and William Sheehan

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Baum, R., Sheehan, W. (1997). Le Grand Newton. In: In Search of Planet Vulcan. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-6100-6_3

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  • DOI: https://doi.org/10.1007/978-1-4899-6100-6_3

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