Effect of solar pressure on the motion and stability of the system of two inter-connected satellites in an elliptical orbit
The effect of solar pressure on the motion and stability of a system of two interconnected satellites (such as a manned-space capsule attached to its booster with a flexible and inextensible string near some equilibrium position) is investigated analytically for the case of elliptical orbit. In this...
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Veröffentlicht in: | Astrophysics and space science 1988, Vol.140 (1), p.49-54 |
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creator | SACHINDRA KUMAR SINHA SINGH, R. B |
description | The effect of solar pressure on the motion and stability of a system of two interconnected satellites (such as a manned-space capsule attached to its booster with a flexible and inextensible string near some equilibrium position) is investigated analytically for the case of elliptical orbit. In this model, which is based on the work of Beletsky (1965, 1969), Singh (1973), and Sinha (1987), the equations of motion obtained are nonlinear and nonautomous; the solution of the system was obtained using Bogoliubov et al. (1961) method. The results indicate that the amplitude of the system remains constant up to the order of e-squared (where e denotes eccentricity). If the value of e is very small, the system will always oscillate about the position of equilibrium with tight string-like dumb- bell satellite with changing phase and constant amplitude. (I.S.) |
doi_str_mv | 10.1007/BF00643527 |
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B</creator><creatorcontrib>SACHINDRA KUMAR SINHA ; SINGH, R. B</creatorcontrib><description>The effect of solar pressure on the motion and stability of a system of two interconnected satellites (such as a manned-space capsule attached to its booster with a flexible and inextensible string near some equilibrium position) is investigated analytically for the case of elliptical orbit. In this model, which is based on the work of Beletsky (1965, 1969), Singh (1973), and Sinha (1987), the equations of motion obtained are nonlinear and nonautomous; the solution of the system was obtained using Bogoliubov et al. (1961) method. The results indicate that the amplitude of the system remains constant up to the order of e-squared (where e denotes eccentricity). If the value of e is very small, the system will always oscillate about the position of equilibrium with tight string-like dumb- bell satellite with changing phase and constant amplitude. 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If the value of e is very small, the system will always oscillate about the position of equilibrium with tight string-like dumb- bell satellite with changing phase and constant amplitude. (I.S.)</description><subject>Astronomy</subject><subject>Celestial mechanics (including n-body problems)</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fundamental astronomy</subject><subject>Fundamental astronomy and astrophysics. 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Instrumentation, techniques, and astronomical observations</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>SACHINDRA KUMAR SINHA</creatorcontrib><creatorcontrib>SINGH, R. B</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>SACHINDRA KUMAR SINHA</au><au>SINGH, R. 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(1961) method. The results indicate that the amplitude of the system remains constant up to the order of e-squared (where e denotes eccentricity). If the value of e is very small, the system will always oscillate about the position of equilibrium with tight string-like dumb- bell satellite with changing phase and constant amplitude. (I.S.)</abstract><cop>Dordrecht</cop><pub>Kluwer</pub><doi>10.1007/BF00643527</doi><tpages>6</tpages></addata></record> |
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source | SpringerLink Journals; EZB-FREE-00999 freely available EZB journals |
subjects | Astronomy Celestial mechanics (including n-body problems) Earth, ocean, space Exact sciences and technology Fundamental astronomy Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations |
title | Effect of solar pressure on the motion and stability of the system of two inter-connected satellites in an elliptical orbit |
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