Dynamical chaos in the Solar system
Methods and results of a new major part of science on the dynamics of the Solar system bodies, namely, the part devoted to researches of dynamical chaos in the motion of celestial bodies, are described and analyzed. The dynamical chaos (non-determined dynamical behavior in the absence of any random...
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| Formato: | Objeto de conferencia |
| Lenguaje: | Inglés |
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2011
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/167645 |
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I19-R120-10915-167645 |
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I19-R120-10915-1676452024-07-01T20:02:30Z http://sedici.unlp.edu.ar/handle/10915/167645 Dynamical chaos in the Solar system Shevchenko, Ivan I. 2011-07 2012 2024-07-01T16:49:12Z en Ciencias Astronómicas dynamics of the Solar system bodies dynamical chaos Methods and results of a new major part of science on the dynamics of the Solar system bodies, namely, the part devoted to researches of dynamical chaos in the motion of celestial bodies, are described and analyzed. The dynamical chaos (non-determined dynamical behavior in the absence of any random perturbations) in the motion of celestial bodies is caused by interaction of nonlinear resonances, either orbital or spin-orbit. The resonances and chaos in the motion of minor and large bodies of the Solar system, — planetary satellites, asteroids, comets, and planets, are considered. Special attention is given to the problem of observability of the chaotic behavior; in particular, methods of analytical estimating the Lyapunov time, specifying the “predictability horizon” of the motion, are described. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 217-246 |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
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SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas dynamics of the Solar system bodies dynamical chaos |
| spellingShingle |
Ciencias Astronómicas dynamics of the Solar system bodies dynamical chaos Shevchenko, Ivan I. Dynamical chaos in the Solar system |
| topic_facet |
Ciencias Astronómicas dynamics of the Solar system bodies dynamical chaos |
| description |
Methods and results of a new major part of science on the dynamics of the Solar system bodies, namely, the part devoted to researches of dynamical chaos in the motion of celestial bodies, are described and analyzed. The dynamical chaos (non-determined dynamical behavior in the absence of any random perturbations) in the motion of celestial bodies is caused by interaction of nonlinear resonances, either orbital or spin-orbit. The resonances and chaos in the motion of minor and large bodies of the Solar system, — planetary satellites, asteroids, comets, and planets, are considered. Special attention is given to the problem of observability of the chaotic behavior; in particular, methods of analytical estimating the Lyapunov time, specifying the “predictability horizon” of the motion, are described. |
| format |
Objeto de conferencia Objeto de conferencia |
| author |
Shevchenko, Ivan I. |
| author_facet |
Shevchenko, Ivan I. |
| author_sort |
Shevchenko, Ivan I. |
| title |
Dynamical chaos in the Solar system |
| title_short |
Dynamical chaos in the Solar system |
| title_full |
Dynamical chaos in the Solar system |
| title_fullStr |
Dynamical chaos in the Solar system |
| title_full_unstemmed |
Dynamical chaos in the Solar system |
| title_sort |
dynamical chaos in the solar system |
| publishDate |
2011 |
| url |
http://sedici.unlp.edu.ar/handle/10915/167645 |
| work_keys_str_mv |
AT shevchenkoivani dynamicalchaosinthesolarsystem |
| _version_ |
1807223540023296000 |