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We have discussed the location of collinear equilibrium points in the generalised photogravitational restricted three body problem. The problem is generalised in the sense that both primaries are oblate spheroid. They are source of radiation as well. We have found the solution for the location of collinear point L1. We found that location of collinear point L1 is affected by eccentricity, oblateness and radiation factor terms. The same method may be applied for location of collinear points L2and L3.

Location of collinear equilibrium points in the generalised photogravitational elliptic restricted three body problem