Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-30T03:54:23.551Z Has data issue: false hasContentIssue false
  • English
  • Français

On Leonhard Euler’s Contribution to the Theory of Precession and Nutation

Published online by Cambridge University Press:  12 April 2016

Victor K. Abalakin
Victor K. Abalakin*
Affiliation:
Pulkovo Observatory, Saint-Petersburg, Russia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Among the immense heritage of Leonhard Euler’s astronomical, mechanical, and mathematical works there has been particularly strong interest in those that deal with principles describing the Earth’s perturbed rotation around its axis. The outstanding meaning of the works is obvious even today, since they give a deep insight into the essence of the phenomena of precessional and nutational displacements of the fundamental coordinate planes and axes constituting astronomical frames of reference.

Type
Part 1. History of Early Polar Motion Research
Information
International Astronomical Union Colloquium , Volume 178: Polar Motion: Historical and Scientific Problems , 2000 , pp. 25 - 40
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Euler, L., Mémoires de l’académie des sciences de Berlin, 1751, p. 289–325.Google Scholar
Euler, L., 1752, p. 412.Google Scholar
Euler, L., 1765, pp. 194–218.Google Scholar
Euler, L., 1766, pp. 265–309.Google Scholar
Lamb, H., Dynamics, Cambridge University Press, 1929.Google Scholar
Yurkina, M.L., Bondarewa, M.D. Einige Probleme der Erdrotationermittlung. In: Technical Report No. 18, Institute of Geodesy, University of Stuttgart, 1993.Google Scholar