Petrography of Apollo 17 soilsAn analysis of soils collected on the valley floor at Taurus-Littrow (dark mantle) reveals that these soils are formed by comminution of mare basalt flows and a clastic deposit consisting of black and orange glass spheres. There is no evidence for the pyroclastic origin of the dark mantle. It is found that the North Massif soils contain a large amount of mare-derived fragments being transported horizontally from the basaltic valley floor. A light mantle deposit of uniform composition including comminuted noritic and anorthositic breccia is observed. It is suggested that the light mantle is an avalanche deposit from regolith developed high on the South Massif.
Document ID
19750055521
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Heiken, G.
Mckay, D. S. (NASA Johnson Space Center Planetary and Earth Sciences Div., Houston, Tex., United States)