Chapter

Chapter Six

Alan C. Bowen and Robert B. Todd

in Cleomedes' Lectures on Astronomy

Published by University of California Press

Published in print January 2004 | ISBN: 9780520233256
Published online March 2012 | e-ISBN: 9780520928510 | DOI: http://dx.doi.org/10.1525/california/9780520233256.003.0015
Chapter Six

Show Summary Details

Preview

This chapter explains that the lunar eclipses are caused by the Moon falling into the Earth's shadow. The shadow of the Earth moves in direct opposition to the Sun, and is, as it were, “dragged” by it. It is not always the case that the Moon as a whole is darkened by the Earth, but on occasion [the Moon is darkened] just partially. The Moon is eclipsed by falling into the Earth's shadow, and only in that way, can it be seen from the phenomena alone. It affects a total eclipse at a very great height, when very close to the Earth, and at an intermediary distance.

Keywords: lunar eclipses; Moon; Earth; shadow; Sun; total eclipse

Chapter.  3820 words. 

Subjects: Classical Philosophy

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.