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Lunar seismology - The internal structure of the moonIt is pointed out that seismology has provided the most detailed information concerning the structure and state of the earth's interior. Beginning in 1969, seismometers were landed on the moon by the Apollo missions, providing the first opportunity to attempt similar studies on another planetary body. In September 1977 the operation of these instruments was terminated. A description is presented of the internal structure of the moon, as determined from the obtained lunar seismic data. The analysis of the lunar data is approached in a systematic fashion, using appropriate techniques to minimize the number of necessary assumptions, extract the maximum amount of structural information, and determine its reliability. The completed lunar seismic network consists of four stations located at the landing sites of Apollo missions 12, 14, 15, and 16. Attention is given to crustal structure, the structure of the lunar mantle, the attenuating region, and the core.
Document ID
19810055569
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Goins, N. R.
(Mobil Research and Development Corp. Dallas, TX, United States)
Dainty, A. M.
(Georgia Institute of Technology Atlanta, GA, United States)
Toksoz, M. N.
(MIT Cambridge, MA, United States)
Date Acquired
August 11, 2013
Publication Date
June 10, 1981
Publication Information
Publication: Journal of Geophysical Research
Volume: 86
Subject Category
Lunar And Planetary Exploration
Accession Number
81A39973
Funding Number(s)
CONTRACT_GRANT: NAS9-12334
CONTRACT_GRANT: NSG-7081
Distribution Limits
Public
Copyright
Other

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