Mathematics – Logic
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mbns.conf...66w&link_type=abstract
The Moon Beyond 2002: Next Steps in Lunar Science and Exploration, p. 66
Mathematics
Logic
Lunar Surface, Lunar Craters, Regolith, Thickness, Lunar Maria, Lunar Orbiter, Geomorphology, Lunar Maps
Scientific paper
We have utilized very high resolution (60-200 cm/p) Lunar Orbiter frames to investigate regolith thickness, distribution, and processes in both mare and highland areas. Previous studies have proposed that the depth to an interface between the regolith and a coherent substrate controls crater interior morphology (Q&O craters) and block distributions in and around host craters. To test this hypothesis we have mapped the distribution of these key morphologic indicators over mare and highland regions. Our data show that the block populations and Q&O crater populations are generally consistent with this idea. However, we have noted some important deviations, namely that the indicators are irregularly distributed and thus seem to imply a highly variable regolith thickness in a local area. Another important result of our data is the documentation that at small sizes the mare contain greater numbers of craters.
Robinson Mark S.
Thomas Peter C.
Wilcox B. B.
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