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Meteoroid flux from passive seismic experiment dataThe meteoroid flux hitting the moon is recomputed using new information on the decrease of seismic signal amplitude with range. The new data are principally 17 large meteoroid impacts whose locations have been computed from recordings at all four of the operating Passive Seismic Experiment stations. These data suggest a rapid decrease in amplitudes beyond about 2200 km (chord range) which was not suspected earlier. The new estimate predicts the abundance of meteoroids with masses between 500 and 50,000 g. The result is considerably lower than estimates from earth-based observations, and close to our previous estimate from long-period lunar seismic data.
Document ID
19780062831
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Duennebier, F.
(Texas Univ. Galveston, TX, United States)
Dorman, J.
(Texas Univ. Galveston, TX, United States)
Lammlein, D.
(Texas Univ. Galveston, TX, United States)
Latham, G.
(Texas Univ. Galveston, TX, United States)
Nakamura, Y.
(Texas, University Galveston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46740
Funding Number(s)
CONTRACT_GRANT: NAS9-14581
Distribution Limits
Public
Copyright
Other

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