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9 - pK Tidal Effects: Distant 3rd Body

Published online by Cambridge University Press:  28 November 2024

Lorenzo Iorio
Affiliation:
Ministero dell’ Istruzione e del Merito, Bari, Italy
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Summary

The precessions of the Keplerian orbital elements are calculated for several tidal-type accelerations due to the presence of a distant 3rd body: Newtonian, post-Newtonian gravitoelectric, and post-Newtonian gravitomagnetic. The calculation is made, first, in a kinematically and dynamically non-rotating frame. Then, it is repeated in a dynamically non-rotating and kinematically rotating frame accounting for the de Sitter–Fokker and Pugh–Schiff precessions of its axes.

Type
Chapter
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General Post-Newtonian Orbital Effects
From Earth's Satellites to the Galactic Centre
, pp. 155 - 164
Publisher: Cambridge University Press
Print publication year: 2024

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  • pK Tidal Effects: Distant 3rd Body
  • Lorenzo Iorio, Ministero dell’ Istruzione e del Merito, Bari, Italy
  • Book: General Post-Newtonian Orbital Effects
  • Online publication: 28 November 2024
  • Chapter DOI: https://doi.org/10.1017/9781009562911.009
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  • pK Tidal Effects: Distant 3rd Body
  • Lorenzo Iorio, Ministero dell’ Istruzione e del Merito, Bari, Italy
  • Book: General Post-Newtonian Orbital Effects
  • Online publication: 28 November 2024
  • Chapter DOI: https://doi.org/10.1017/9781009562911.009
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • pK Tidal Effects: Distant 3rd Body
  • Lorenzo Iorio, Ministero dell’ Istruzione e del Merito, Bari, Italy
  • Book: General Post-Newtonian Orbital Effects
  • Online publication: 28 November 2024
  • Chapter DOI: https://doi.org/10.1017/9781009562911.009
Available formats
×