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Lunar Meteoroid Impact Observations and the Flux of Kilogram-sized Meteoroids

Authors :
Suggs, R. M
Cooke, W. J
Koehler, H. M
Suggs, R. J
Moser, D. E
Swift, W. R
Source :
Meteoroids: The Smallest Solar System Bodies.
Publication Year :
2011
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2011.

Abstract

Lunar 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.

Subjects

Subjects :
Space Sciences (General)

Details

Language :
English
Database :
NASA Technical Reports
Journal :
Meteoroids: The Smallest Solar System Bodies
Publication Type :
Report
Accession number :
edsnas.20110016595
Document Type :
Report