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Moonquakes and lunar tectonism results from the Apollo passive seismic experiment.The natural seismicity of the moon appears to be very low relative to that of the earth. However, moonquakes do occur. They are detected by the stations of the Apollo seismic network at an average rate of 1800/yr at Station 14 and at lower rates at Stations 12 and 15. All of the moonquakes are small, and in the few cases for which the foci have been located, they occur at great depth (about 800 km). The frequency of occurrence of moonquakes is strongly correlated with lunar tides. The dynamic processes that generate quakes are clearly much less vigorous within the moon than they are within the earth.
Document ID
19730035046
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Latham, G.
Ewing, M.
Dorman, J.
Lammlein, D.
(Lamont-Doherty Geological Observatory Palisades, N.Y., United States)
Press, F.
Toksoz, N.
(MIT Cambridge, Mass., United States)
Sutton, G.
Duennebier, F.
(Hawaii, University Honolulu, Hawaii, United States)
Nakamura, Y.
(General Dynamics Corp. Fort Worth, Tex., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: January 10, 1972
End Date: January 13, 1972
Accession Number
73A19848
Funding Number(s)
CONTRACT_GRANT: NAS9-5957
CONTRACT_GRANT: NAS9-12334
Distribution Limits
Public
Copyright
Other

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