Geophysical Research Letters · 2015 · 146 citations · 30 references
GeophysicsAeolian ProcessEarth-moon SystemRegolith StratigraphyLpr ObservationsSurface AgeEngineeringLunar Penetrating RadarPlanetary GeologyGeologyLunar ScienceEarth SciencesE‐3 LunarEarth SciencePlanetary Geomorphology
Abstract The Chang'E‐3 lunar penetrating radar (LPR) observations at 500 MHz reveal four major stratigraphic zones from the surface to a depth of ~20 m along the survey line: a layered reworked zone (<1 m), an ejecta layer (~2–6 m), a paleoregolith layer (~4–11 m), and the underlying mare basalts. The reworked zone has two to five distinct layers and consists of surface regolith. The paleoregolith buried by the ejecta from a 500 m crater is relatively homogenous and contains only a few rocks. Population of buried rocks increases with depth to ~2 m at first, and then decreases with depth, representing a balance between initial deposition of the ejecta and later turnover of the regolith. Combining with the surface age, the LPR observations indicate a mean accumulation rate of about 5–10 m/Gyr for the surface regolith, which is at least 4–8 times larger than previous estimation.
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T. H. Prettyman, J. J. Hagerty, R. C. Elphic et al. · Journal of Geophysical Research Atmospheres · 2006 · 446 citations · Full text
Engineering, Trace Element Geochemistry, Elemental Composition +12
Ages of mare basalts on the lunar nearside
H. Hiesinger, R. Jaumann, G. Neukum et al. · Journal of Geophysical Research Atmospheres · 2000 · 400 citations · Full text
The lunar regolith: Chemistry, mineralogy, and petrology
J. J. Papike, S. B. Simon, J. C. Laul · Reviews of Geophysics · 1982 · 319 citations