The orbital propulsion of spinning tether via angular momentum transfer

  • Yang Yu*
  • , Hexi Baoyin
  • , Yang Chen
  • , Junfeng Li
  • , Shengping Gong
  • , Xiangyuan Zeng
  • *Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

During past decades, the spinning tethered systems were primarily discussed for specific space missions, including on-orbit capture and propellantless orbit transfer etc. such as the famous project Momentum-Exchange/Electrodynamic- Reboost (MXER) by NASA. As an elementary large-scale space structure, the spinning tethered binary system is intriguing for the dynamic behaviors and basic laws of motion control in gravitational field, which is essentially different from that of mass particle. The present work studies the dynamic behaviors of spinning tethered binary system, especially for that with the tether length variable. Considering the characteristics of coupled librational and orbital motions, a typical model is adopted to discuss the orbital motion of mass center. An averaging approach is introduced to deal with the slow-fast system equations of the spinning tethered binary system, thus a definite equivalent model is derived. Thus, the general orbit motion is completely determined with an analytical method employed, including the orbit geometry, periodicity, conversations and moving region etc. Since the possibility of orbit control using tether reaction has been proved by previous studies, the general principles of orbital propulsion are still interesting and worth investigating. In this paper, special attention is paid to the transportation of angular momentum and mechanical energy between the orbit and tether spin, which governs the variation of mass center orbit. A perturbation method is applied to investigate the relationship between the orbit shape variation and the tether length change. The results show that the secular perturbation caused by the tether deploying and retrieving is the major factor that influences the orbit shape, and the orbit angular momentum and mechanical energy can be controlled independently. Numerical investigations under the full model validate the conclusions stated above. The final part of this paper discusses some special applications of this technology in space missions.

Original languageEnglish
Title of host publication62nd International Astronautical Congress 2011, IAC 2011
Pages8149-8160
Number of pages12
StatePublished - 2011
Externally publishedYes
Event62nd International Astronautical Congress 2011, IAC 2011 - Cape Town, South Africa
Duration: 3 Oct 20117 Oct 2011

Publication series

Name62nd International Astronautical Congress 2011, IAC 2011
Volume10

Conference

Conference62nd International Astronautical Congress 2011, IAC 2011
Country/TerritorySouth Africa
CityCape Town
Period3/10/117/10/11

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