Martian seismicity

Details Martian seismicity Martian seismicity

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979georl...6..368g&link_type=abstract

Geophysical Research Letters, vol. 6, May 1979, p. 368-370. Research supported by the California Institute of Technology;

Physics

6

Mars (Planet), Seismic Waves, Viking Mars Program, Seismographs, Viking Lander Spacecraft, Mars, Seismicity, Viking, Seismometers, Seismic Waves, Viking 2 Lander, Tharsis

Scientific paper

During the Viking mission to Mars, the seismometer on Lander II collected approximately 0.24 earth years of observational data, excluding periods of time dominated by wind-induced Lander vibration. The 'quiet-time' data set contains no confirmed seismic events. A proper assessment of the significance of this fact requires quantitative estimates of the expected detection rate of the Viking seismometer. The first step is to calculate the minimum magnitude event detectable at a given distance, including the effects of geometric spreading, anelastic attenuation, seismic signal duration, seismometer frequency response, and possible poor ground coupling. Assuming various numerical quantities and a Martian seismic activity comparable to that of intraplate earthquakes, the appropriate integral gives an expected annual detection rate of 10 events, nearly all of which are local. Thus only two to three events would be expected in the observational period presently on hand and the lack of observed events is not in gross contradiction to reasonable expectations. Given the same assumptions, a seismometer 20 times more sensitive than the present instrument would be expected to detect about 120 events annually.

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