Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-27T21:35:38.736Z Has data issue: false hasContentIssue false
  • English
  • Français

Eclipse Calculations: An Elementary Treatment For Schools

Published online by Cambridge University Press:  03 November 2016

T.T. Whitehead
Get access Rights & Permissions [Opens in a new window]

Extract

1. A Solar eclipse occurs whenever the sun, moon and earth have their centres so nearly in line that the moon hides some part, or all, of the sun from an observer on the earth’s surface. In the former case the eclipse is partial, in the latter total. The relative motions of the three bodies are extremely complicated; but as knowledge of the apparent positions of the sun and moon is of importance for safe navigation, these are regularly computed in advance and published by the Admiralty in the Nautical Almanac. Since the Nautical Almanac tables are the data for eclipse calculations, it is essential to understand the method there employed for recording the positions of the heavenly bodies, and the meanings of a few technical terms.

Type
Research Article
Information
The Mathematical Gazette , Volume 13 , Issue 188 , May 1927 , pp. 342 - 348
Copyright
Copyright © Mathematical Association 1927

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

* The altitude of the moon may be assumed, for this purpose, to be equal to that of the sun, and is given by the formula sinα = sinλ sind—cosλ cos d cos t, when α is the altitude, and λ is the geographical latitude of the station : d and t have the same meanings as in § 9.