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Observations of the lunar regolith and the Earth from the television camera on Surveyor 7

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

Surveyor 7, the last spacecraft of the Surveyor series, landed about 30 km north of the rim crest of Tycho, one of the most prominent and well-known features in the southern part of the moon. About 21,000 pictures were transmitted during two lunar days of operation. At the Surveyor 7 site, the cumulative size-frequency distribution of craters 13 cm to 3 meters in diameter follows closely the distribution of craters observed at the other Surveyor sites in the lunar maria. This distribution of small craters is believed to be a steady-state distribution.

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Eugene Merle Shoemaker, R. M. Batson, H. E. Holt, E. C. Morris, J. J. Rennilson, E. A. Whitaker. 2012-09-20. Observations of the lunar regolith and the Earth from the television camera on Surveyor 7. https://doi.org/10.1029/jb074i025p06081

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