New Integrals of Motion and the Orbital History of the Moon

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GOUDAS1 has criticized the integrals of motion that I have given2 for the elliptic restricted three body problem. He states: ``Contopoulos has given an integral equivalent to the Jacobi integral for the elliptic restricted problem as well as one additional time-independent integral for the same equations of motion. It seems, however, that the work of Contopoulos is not in harmony with a famous theorem by Poincaré'' because ``if two integrals, time-independent and independent of one another, exist, then there should be two zero characteristic exponents associated with each periodic solution'', which is not the case.

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