The three-body problem is investigated under the initial assumption that Newton's third law may be neglected (i.e., the bodies are separated by considerable distances); subsequently, the effects of the third law are taken into account in treating the mutual attraction of the two non-central bodies. New triangular Lagrangian solutions, as well as a new linear Eulerian solution, are developed through use of the method of stationary solutions introduced by Levi-Civita.