The calculation of solar eclipses without parallaxes. [electronic resource] : With a specimen of the same in the total eclipse of the sun, May 11. 1724. Now first made Publick. To which is added, A Proposal how, with the Latitude given, the Geographical Longitude of all the Parts of the Earth may be settled by the bare Knowledge of the Duration of Solar Eclipses, and especially of Total Darkness. With An Account of some late Observations made with Dipping Needles, in order to discover the Longitude and Latitude at Sea. By Will. Whiston, M. A. Sometime Professor of the Mathematicks in the University of Cambridge.
1724
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The calculation of solar eclipses without parallaxes. [electronic resource] : With a specimen of the same in the total eclipse of the sun, May 11. 1724. Now first made Publick. To which is added, A Proposal how, with the Latitude given, the Geographical Longitude of all the Parts of the Earth may be settled by the bare Knowledge of the Duration of Solar Eclipses, and especially of Total Darkness. With An Account of some late Observations made with Dipping Needles, in order to discover the Longitude and Latitude at Sea. By Will. Whiston, M. A. Sometime Professor of the Mathematicks in the University of Cambridge.
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Publication Details
London : printed for J. Senex in Fleetstreet; and W. Taylor in Pater-Noster-Row, 1724.
Place of Publication or Printing
Great Britain -- England -- London.
Language
English
Description
[4],94,[2]p.,plate ; 8⁰.
Note
With a half-title and a final errata leaf.
Reproduction of original from British Library.
Reproduction of original from British Library.
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Access limited to authorized users.
Indexed In
English Short Title Catalog, T105408.
Reproduction
Electronic reproduction. Farmington Hills, Mich. : Cengage Gale, 2009. Available via the World Wide Web. Access limited by licensing agreements.
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