Tranquillityite - A new silicate mineral from Apollo 11 and Apollo 12 basaltic rocks
Tranquillityite silicate mineral in crystalline basaltic rocks from Apollo 11 and 12 samples
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Tranquillityite silicate mineral in crystalline basaltic rocks from Apollo 11 and 12 samples
Minor element concentrations and population sources of Apollo 11 and 12 olivine and plagioclase, using microprobe analyses
Zirconium liquid-crystal distribution in phase ilmenite of Apollo 11 and 12 lunar rocks
Apollo 11 and 12 unshocked and shocked microbreccias petrology, noting shock compression and shock welding
Apollo 11 and 12 devitrified glass fragments temperature histories indicating broad range of subsolidus crystallization temperatures
Apollo 11 and 12 lunar rock and soil examination, emphasizing Au and Ag excess in soil
Apollo 11 and 12 fines cosmogenic He, Ne and Ar radionuclides composition determination, using electron microprobe analysis
Indigenous gases and hydrolyzable carbon compounds in Apollo 11 and 12 samples through gas chromatographic and mass spectrometric examination, noting meteoritic impact and solar wind implantation as probable origins
Chemical characteristics of carbon compounds in Apollo 11 and 12 lunar fines, using organic solvent extraction, mass spectrometry and gas chromatographic method
Biological activity in Apollo 11 and 12 core samples searched for after placement in Petri dishes containing media
Regular particle morphology and petrostatistics in Apollo 11 and 12 lunar fines and conglomerates, using phase contrast and scanning microscopes
IR vibrational spectroscopic analysis of Apollo 11 and 12 rocks and dust isolated silicate minerals, using LF absorption bands
Apollo 11 and 12 rocks luminescence under proton, electron, UV and X irradiation
Apollo 11 and 12 rocks specific heat and thermal conductivity at 2-5 K, comparing elastic properties
Magnetic properties of glass spherules from Apollo 11 and 12 fines, determining oxidation effect
Electron spin resonance studies of Apollo 11 and 12 lunar soil samples, determining ferromagnetism due to Fe particles
The crew members on the last seven Apollo flights observed light flashes that are tentatively attributed to cosmic ray nuclei (atomic number equal to or greater than 6) penetrating the head and eyes of the observers. Analyses of the event rates for all missions has revealed an anomalously low rate for transearth coast observations with respect to translunar coast observations.
Apollo 11 magnesium-rich opaque oxide armalcolite mineral from Tranquility Base noting relation to pseudobrookite series