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DC Field | Value | Language |
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dc.contributor.author | Kumar, V | - |
dc.contributor.author | Choudhry, R. K | - |
dc.date.accessioned | 2006-04-10T06:34:00Z | - |
dc.date.available | 2006-04-10T06:34:00Z | - |
dc.date.issued | 1986-06 | - |
dc.identifier.citation | BASI, Vol. 14, No. 2, pp. 79-90 | en |
dc.identifier.uri | http://hdl.handle.net/2248/909 | - |
dc.description.abstract | The motion of an infinitesimal mass under the gravitational field of two radiating bodies of finite mass is investigated analytically, with a focus on the possible existence of libration points, in the framework of the generalized restricted three-body problem. The analysis of Simmons et al. (1985) is extended to the case of an oblate-spheroid (rather than spherical) infinitesimal mass. A general radiation-pressure expression is introduced; the equations of motion are derived; and conditions for the existence of collinear, coplanar, and triangular libration points are obtained. It is shown that in the general case there are seven libration points: three collinear, two coplanar, and two triangular. Nine points are possible for small degrees of infinitesimal-mass oblateness | en |
dc.format.extent | 622965 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of Indian | en |
dc.subject | Celestial mechanics | en |
dc.subject | Libration points | en |
dc.subject | Three body problem | en |
dc.title | Existence of libration points in the generalized photogravitational restricted problem of three bodies | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
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