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The effect of zonal harmonics on dynamical structures in the circular restricted three-body problem near the secondary body
The circular restricted three-body model is widely used for astrodynamical studies in systems where two major bodies are present. However, this model relies on many simplifications, such as point-mass gravity and planar, circular orbits of the bodies, and limiting its accuracy. In an effort to achie...
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| Publicado no: | Celest Mech Dyn Astron |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Springer Netherlands
2020
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7646744/ https://ncbi.nlm.nih.gov/pubmed/33184532 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1007/s10569-020-09983-3 |
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