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A Prediction of Mars Seismicity from Surface Faulting
Matthew P. Golombek, W. Bruce Banerdt, Kenneth L. Tanaka and David M. Tralli
New Series, Vol. 258, No. 5084 (Nov. 6, 1992), pp. 979-981
Published by: American Association for the Advancement of Science
Stable URL: http://www.jstor.org/stable/2881674
Page Count: 3
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The shallow seismicity of Mars has been estimated by measurement of the total slip on faults visible on the surface of the planet throughout geologic time. Seismicity was calibrated with estimates based on surface structures on the moon and measured lunar seismicity that includes the entire seismogenic lithosphere. Results indicate that Mars is seismically active today, with a sufficient number of detectable marsquakes to allow seismic investigations of its interior.
Science © 1992 American Association for the Advancement of Science