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LRO observations of morphology and surface roughness of volcanic cones and lobate lava flows in the Marius Hills
2013
Journal of Geophysical Research - Planets
1] The volcanic domes, cones, sinuous rilles, and pyroclastic deposits of the Marius Hills region of the Moon (~13.4 N, 304.6 E) represent a significant episode of magmatic activity at or near the lunar surface that is still poorly understood. Comparisons between LROC NAC block populations, Mini-RF data, and Diviner-derived rock abundances confirm that blocky lava flows comprise the domes of the Marius Hills. 8 mm features measured by Diviner indicate that the domes are not rich in silica and
doi:10.1002/jgre.20060
fatcat:5yeg5f6tpjegxhw64usqmbd464