Abstract
This paper deals with the libration points in the elliptic restricted three-body problem. The combined effects of the primary bodies’ orbital eccentricity and albedo on the existence and stability of libration points is analyzed. It is found that there exist five libration points, three collinear and two non-collinear. The non-collinear libration points are stable for a critical value of mass parameter μc, the collinear libration points are unstable for all values of μ.
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