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By Neil., . Ashby

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J. Phys. [ 51 Schlegel's expression for this discontinuity contains an error. [6] C. W. Misner, K. S. Thorne, and J. A . Wheeler, Gravitation, W. H. , San Francisco, p . 596 (1973). [7] F. K. Manasse and C. W. Misner, J. Math. Phys. [81 B. Hoffman, Phys. Rev. [ 91 M. Caputo, The Gravity Field of the Earth, Academic Press, New York, p. 32 (1Y67). [lo) G. D. Garland, The Earth's Shape and Gravity, Pergamon Press, New York (1Y65); R. H. Rapp, Geophys. Res. Letters 1, 35 (1Y74). Ll] W. J. Cocke, Phys.

The leading correction term is due to retardation and will be of order 4Gm 2-t c Ir - The velocity of the moon is such that v/c Y -t r'l - c -6 3 x 10 . 84 x 10" m cm , we obtain 4Gm 2-t -t c Ir - r'I E ;10-18 c This retardation term contributes a term of order lasting to hO0 . In a typical flight 10 hours , such a term would contribute no more than about 4 x the elapsed coordinate time and may, therefore, be neglected. sec to Thus, we conclude that retardation corrections to the metric from motion of the moon may be neglected.

Phys. [ 51 Schlegel's expression for this discontinuity contains an error. [6] C. W. Misner, K. S. Thorne, and J. A . Wheeler, Gravitation, W. H. , San Francisco, p . 596 (1973). [7] F. K. Manasse and C. W. Misner, J. Math. Phys. [81 B. Hoffman, Phys. Rev. [ 91 M. Caputo, The Gravity Field of the Earth, Academic Press, New York, p. 32 (1Y67). [lo) G. D. Garland, The Earth's Shape and Gravity, Pergamon Press, New York (1Y65); R. H. Rapp, Geophys. Res. Letters 1, 35 (1Y74). Ll] W. J. Cocke, Phys.

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