[SA1-2-10-2] Perturbed motion

Perturbed motion accounts for deviations from ideal Keplerian orbits due to gravity harmonics, acceleration of third bodies, atmospheric drag, solar radiation pressure, tides, maneuvers, and other environmental forces.

External resources

• Sanz Subirana, J., Juan Zornoza, J.M. and Hernández-Pajares, M. (2013) GNSS Data Processing, Vol. 1: Fundamentals and Algorithms (ESA TM-23/1, May 2013) ESA Communications, Noordwijk, The Netherlands.

Outgoing relations

• [SA1-2-10-2] Perturbed motion is subconcept of [SA1-2-10] Orbital elements

Contributors

• Adria Rovira Garcia
  https://wwwdfen.webs.upc.edu/php_pagina_web/person_id.php?id=adria.rovira
• Adriano Camps
  https://prs.upc.edu/2018/08/17/adriano-camps/