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Lunar Meteoroid Impact Observations and the Flux of Kilogram-sized MeteoroidsLunar impact monitoring provides useful information about the flux of meteoroids in the hundreds of grams to kilograms size range. The large collecting area of the night side of the lunar disk, approximately 3.8 10(exp 6)sq km in our camera field-of-view, provides statistically significant counts of the meteoroids striking the lunar surface. Over 200 lunar impacts have been observed by our program in roughly 4 years. Photometric calibration of the flashes observed in the first 3 years along with the luminous efficiency determined using meteor showers and hypervelocity impact tests (Bellot Rubio et al. 2000; Ortiz et al. 2006; Moser et al. 2010; Swift et al. 2010) provide their impact kinetic energies. The asymmetry in the flux on the evening and morning hemispheres of the Moon is compared with sporadic and shower sources to determine their most likely origin. These measurements are consistent with other observations of large meteoroid fluxes.
Document ID
20110016595
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Suggs, R. M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cooke, W. J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Koehler, H. M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Suggs, R. J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Moser, D. E.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Swift, W. R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 25, 2013
Publication Date
July 1, 2011
Publication Information
Publication: Meteoroids: The Smallest Solar System Bodies
Subject Category
Space Sciences (General)
Distribution Limits
Public
Copyright
Public Use Permitted.
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