The Kana-a flow, an alkali basalt of the San Francisco volcanic field, Arizona
Geological and petrographical analyses of Kana-a basalt flow in San Francisco Volcanic Field, Arizona
PETROGRAPHY↗
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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.
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Development of technological concepts leading to the beneficial use of lunar magma products Technical progress report, Oct. - Dec. 1966
Gabbro, serpentine, and artificial olivine analyses and petrographic properties of cast and formed geometric shapes
OLIVINE↗
Astrogeologic studies. Part B - Crater investigations Annual progress report, 1 Jul. 1965 - 1 Jul. 1966
Astrogeologic studies - crater investigations
METEORITIC CRATER↗
Impact metamorphism
Diagnostic petrographic criteria for establishing progressive stages of hypervelocity meteorite impact
METEORITIC CRATER↗
Sudbury structure, Ontario - Some petrographic evidence for an origin by meteorite impact
Petrographic evidence of meteorite impact in Canadian rock structure
METEORITIC MICROSTRUCTURE↗
Some aspects of the Manicouagan Lake structure in Quebec, Canada
Geologic structure, petrographic data, and suggested meteoritic impact origin of Canadian Manicouagan-Mushalagan Lakes area
GEOLOGY↗
Investigations of the Orgueil carbonaceous meteorite.
Orgueil carbonaceous meteorite composition and mineral texture including petrogenesis and origin of organic content and mineralized microstructures
PETROGRAPHY↗
Sudbury Structure, Ontario: Some Petrographic Evidence for Origin by Meteorite Impact
Deformation in Sudbury structure, Ontario, suggests petrographic evidence for origin by meteorite impact
METEORITIC CRATER↗
Chromite composition in relation to chemistry and texture of ordinary chondrites.
Chromite composition in chondrites using electron microprobe technique, discussing petrographic origin and vanadium abundance
METEORITIC COMPOSITION↗
Initial Petrographic Analysis of Apollo 17 73002 Continuous Core Thin Sections Using QEMSCAN Mapping Techniques
In 1972, the Apollo 17 mission landed in the Taurus-Littrow Valley located in the southeastern edge of Mare Serenitatis [1].During EVA 2at Station 3,a double drive tube was used to collect a sealed core sample (73001/2)of the upper~70cm of the lunar regolith[2-4].The core was taken from the surface of the light mantle deposit, found at the base of the South Massif [3]. For nearly 50 years, the sealed core samples have remained unopened. This study is part of the Apollo Next Generation Sample Analysis (ANGSA) initiative to analyze the continuous thin sections from the Apollo 17 drive tubes opened in 2019[5-7].
QEMSCAN↗