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The Viking seismometryEfforts were made to determine the seismicity of Mars as well as define its internal structure by detecting vibrations generated by marsquakes and meteoroid impacts. The lack of marsquakes recognized in the Viking data made it impossible to make any direct inferences about the interior of Mars and only allowed the setting of upper bounds on the seismic activity of the planet. After obtaining more than 2100 hours worth of data during the quite periods at rates of one sample per second or higher, the Viking 2 seismometer was turned off as a consequence of a landing system failure. During the periods when adequate data were obtained, one event of possible seismic or meteoroid impact origin was recognized; however, there is a significant probability that this event was generated by a wind gust.
Document ID
19810013458
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Lazarewicz, A. R.
(NASA Headquarters Washington, DC United States)
Anderson, D. L.
(NASA Headquarters Washington, DC United States)
Anderson, K.
(NASA Headquarters Washington, DC United States)
Daonty, A. M.
(NASA Headquarters Washington, DC United States)
Duennebier, F. K.
(NASA Headquarters Washington, DC United States)
Gains, N. R.
(NASA Headquarters Washington, DC United States)
Knight, T. C. D.
(NASA Headquarters Washington, DC United States)
Kovach, R. L.
(NASA Headquarters Washington, DC United States)
Latham, G. V.
(NASA Headquarters Washington, DC United States)
Miller, W. F.
(NASA Headquarters Washington, DC United States)
Date Acquired
September 4, 2013
Publication Date
April 1, 1981
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
NASA-CR-3408
Accession Number
81N21988
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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