Stability of triangular points in the generalised photogravitational restricted three body problem

dc.contributor.author	Singh, J
dc.contributor.author	Ishwar, B
dc.date.accessioned	2008-02-08T11:23:26Z
dc.date.available	2008-02-08T11:23:26Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 3, pp. 415 – 424	en
dc.identifier.uri	http://hdl.handle.net/2248/2024
dc.description.abstract	We study the effect of oblateness and radiation pressure forces of the primaries on the location and the stability of the triagular points in the restricted three body problem. We observe that the equations of motion and locations of the triangular points are affected by the radiation pressure forces and oblateness of the primaries. It is further seen that these points are stable for 0≤µ≤µc, and unstable for µc≤µ≤1/2. It is also seen that for these points the range of stability increases or decreases according as p > or < 0 where p depends upon the radiating and oblateness coefficients.	en
dc.format.extent	495462 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999BASI...27..415S	en
dc.subject	Stability	en
dc.subject	Triagnular points	en
dc.subject	Generalised	en
dc.subject	Photo gravitational RTBP	en
dc.title	Stability of triangular points in the generalised photogravitational restricted three body problem	en
dc.type	Article	en