Orbital Dynamics in the Gravitational Field of Small Bodies

This prizewinning PhD thesis presents a general discussion of the orbital motion close to solar system small bodies (SSSBs), which induce non-central asymmetric gravitational fields in their neighborhoods. It introduces the methods of qualitative theory in nonlinear dynamics to the study of local/gl...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Yu, Yang (Autor)
Autor Corporativo: SpringerLink (Online service)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2016.
Edición:1st ed. 2016.
Colección:Springer Theses, Recognizing Outstanding Ph.D. Research,
Temas:
Astrophysics.
Aerospace engineering.
Astronautics.
Dynamical systems.
Computer simulation.
Nonlinear Optics.
Mechanics.
Aerospace Technology and Astronautics.
Dynamical Systems.
Computer Modelling.
Classical Mechanics.
Acceso en línea:Texto Completo

MARC

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245 1 0 |a Orbital Dynamics in the Gravitational Field of Small Bodies  |h [electronic resource] /  |c by Yang Yu. 
250 |a 1st ed. 2016. 
264 1 |a Berlin, Heidelberg :  |b Springer Berlin Heidelberg :  |b Imprint: Springer,  |c 2016. 
300 |a XVIII, 123 p. 49 illus., 17 illus. in color.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
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490 1 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5061 
505 0 |a Introduction -- SSSB Model and equations of motion -- Stability of equilibrium points and the local behavior of orbits -- Topology and stability of large-scale periodic orbits -- Resonant orbit near the equatorial plane -- Free motion of a particle close to the surface of SSSBs -- Conclusions and future directions. 
520 |a This prizewinning PhD thesis presents a general discussion of the orbital motion close to solar system small bodies (SSSBs), which induce non-central asymmetric gravitational fields in their neighborhoods. It introduces the methods of qualitative theory in nonlinear dynamics to the study of local/global behaviors around SSSBs. Detailed mechanical models are employed throughout this dissertation, and specific numeric techniques are developed to compensate for the difficulties of directly analyzing. Applying this method, several target systems, like asteroid 216 Kleopatra, are explored in great detail, and the results prove to be both revealing and pervasive for a large group of SSSBs. . 
650 0 |a Astrophysics. 
650 0 |a Aerospace engineering. 
650 0 |a Astronautics. 
650 0 |a Dynamical systems. 
650 0 |a Computer simulation. 
650 0 |a Nonlinear Optics. 
650 0 |a Mechanics. 
650 1 4 |a Astrophysics. 
650 2 4 |a Aerospace Technology and Astronautics. 
650 2 4 |a Dynamical Systems. 
650 2 4 |a Computer Modelling. 
650 2 4 |a Nonlinear Optics. 
650 2 4 |a Classical Mechanics. 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer Nature eBook 
776 0 8 |i Printed edition:  |z 9783662526910 
776 0 8 |i Printed edition:  |z 9783662526927 
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830 0 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5061 
856 4 0 |u https://doi.uam.elogim.com/10.1007/978-3-662-52693-4  |z Texto Completo 
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950 |a Physics and Astronomy (SpringerNature-11651) 
950 |a Physics and Astronomy (R0) (SpringerNature-43715) 

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