國立虎尾科技大學 |

Orbital dynamics in the gravitational field of small bodies

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Orbital dynamics in the gravitational field of small bodies/ by Yang Yu.
作者:	Yu, Yang.
出版者:	Berlin, Heidelberg :Springer Berlin Heidelberg : : 2016.,
面頁冊數:	xviii, 123 p. :ill. (some col.), digital ; : 24 cm.;
Contained By:	Springer eBooks
標題:	Orbital mechanics. -
電子資源:	http://dx.doi.org/10.1007/978-3-662-52693-4
ISBN:	9783662526934

Orbital dynamics in the gravitational field of small bodies
Yu, Yang.

Orbital dynamics in the gravitational field of small bodies[electronic resource] /by Yang Yu. - Berlin, Heidelberg :Springer Berlin Heidelberg :2016. - xviii, 123 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

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.

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.

ISBN: 9783662526934

Standard No.: 10.1007/978-3-662-52693-4doiSubjects--Topical Terms:

908547
Orbital mechanics.

LC Class. No.: TL1050

Dewey Class. No.: 521.3

Orbital dynamics in the gravitational field of small bodies
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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.
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