A simple model to determine chaotic motions around asteroids
It is well known that the 3-D motion around the asteroid (433) Eros is chaotic for a wide set of inclinations.The main feature of this body is its elongated shape, which originates that the usual procedure of expandingthe potential function in spherical harmonics is useless. This is the reason why w...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2006
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57102504 |
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