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Surveyor V: Television pictures

E.M. Shoemaker·R. M. Batson·H. E. Holt·E. C. Morris·J. J. Rennilson·E. A. Whitaker
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Abstract

Surveyor V landed in a small crater, 8.5 meters wide and 12.5 meters long, which was probably formed by drainage of surficial fragmental debris into a subsurface fissure. The lunar surface debris layer is exposed in the walls of this crater. At depths below about 10 centimeters, the debris appears to be composed mainly of shock-compressed aggregates, ranging from a few millimeters up to 3 centimeters in diameter, set in a matrix of less-coherent finer particles. Rocky chips and fragments larger than a millimeter are dispersed as a subordinate constituent of the debris.

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E.M. Shoemaker, R. M. Batson, H. E. Holt, E. C. Morris, J. J. Rennilson, E. A. Whitaker. 1967. Surveyor V: Television pictures. https://doi.org/10.1126/science.158.3801.642

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