Skip to main content

Abstract

The spheroidal shape of the Earth causes a deviation of the absolute period, i.e. the time required to pass through 360°, from the Kepler period of an Earth satellite.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 29.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 37.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

Copyright information

© 1989 Friedr. Vieweg & Sohn Verlagsgesellschaft mbH, Braunschweig

About this chapter

Cite this chapter

Rimrott, F.P.J. (1989). Orbital Periods. In: Introductory Orbit Dynamics. Fundamentals and Advances in the Engineering Sciences / Grundlagen und Fortschritte der Ingenieurwissenschaften. Vieweg+Teubner Verlag. https://doi.org/10.1007/978-3-322-90338-9_8

Download citation

  • DOI: https://doi.org/10.1007/978-3-322-90338-9_8

  • Publisher Name: Vieweg+Teubner Verlag

  • Print ISBN: 978-3-322-90339-6

  • Online ISBN: 978-3-322-90338-9

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics