Astrogeologic studies - Summary Annual progress report, 1 Jul. 1964 - 1 Jul. 1965
Geologic mapping of lunar surface, crater phenomenology, and petrology of extraterrestrial material
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Geologic mapping of lunar surface, crater phenomenology, and petrology of extraterrestrial material
Previous spectroscopic studies of the lunar crater Bullialdus, located in the Nubium Basin, indicated an unusual stratigraphy of two gabbroic layers overlying a noritic unit. The possible existence of a layered mafic pluton at Bullialdus was suggested. To investigate the geologic context with more detailed spatial information, charge-coupled device (CCD) images of Bullialdus were obtained using eight filters. A linear mixing model was used to investigate the fractional abundances of spectral end-members chosen from within the multispectral image. Since the reflectance properties of lunar materials over this wavelength range are sensitive to variations in composition and soil maturity, fractional abundance images were used to create a new geologic map of the crater. The spatial relationships of the surface materials confirm the previously inferred stratigraphy, and further reveal the central peaks to exhibit two distinct compositional units: noritic anorthosite and anorthositic norite. Three models for the origin of the observed stratigraphy are considered: Bullialdus has excavated stratigraphic units containing (1) early mare basalt overlying anorthositic-noritic crustal material, (2) part of a layered mafic pluton, and/or (3) part of an impact melt sheet formed by the Nubium Basin impact event.
Computer coupled automatic activation and remote lunar analyses - chemical analysis
Thermal properties of simulated lunar material in air and in vacuum
Infrared spectrophotometry for lunar and planetary soil analysis
Nature of lunar surface and major structural features
Discussion of experimental apparatus and results of a dynamic penetration study of crushed rock under atmospheric and vacuum conditions /see accession no. a-63 12763, issue no. 7/
Investigation of the physical properties of the lunar surface layer as simulated by terrestrial and extraterrestrial materials
Speculation on the origin formation of tektites from silicic igneous rocks, specifically rhyolitic tuffs, forming the upper layers of the lunar maria
Lunar chemical composition, hydrostatic equilibrium, thermal history and material evaporation are considered in a study of the internal structure of the moon
Origin of the lunar walled plain ptolemaeus deduced from tectonic relations between diverse features in ptolemaeus and the grid systems in its vicinity
Possible origin of the lunar walled plain ptolemaeus
Theory of tektite origin on moon as impact fragments
Nonuniform expansion and contraction effects on moon, mercury and mars
Lunar and planetary X-ray diffraction program - instrumentation, mineralogy, and petrology
Pressure, temperature, and voidage calculations for lunar ash flow explanation of tektite chemistry