Effect of solar radiation pressure on a planet in the photogravitational restricted three-body problem

dc.contributor.author	Ahmad, A
dc.contributor.author	Islam, N
dc.date.accessioned	2007-10-16T06:00:53Z
dc.date.available	2007-10-16T06:00:53Z
dc.date.issued	1997
dc.identifier.citation	BASI, Vol. 25, No. 1, pp. 83 - 86	en
dc.identifier.uri	http://hdl.handle.net/2248/1886
dc.description.abstract	Here, we have deduced the equations of motion of the photogravitional restricted three-body problem considering the effect of solar radiation pressure on a planet and found that it is stabilizing for the triangular libration points.	en
dc.format.extent	213600 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/1997BASI...25...83A	en
dc.subject	Photogravitional	en
dc.subject	Lagrangian	en
dc.subject	Three-body	en
dc.title	Effect of solar radiation pressure on a planet in the photogravitational restricted three-body problem	en
dc.type	Article	en