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Noonan, A.

Publications and source records attributed to Noonan, A..

5 records
All sourcesNASA NTRSDOE OSTI
NASA NTRS1978

Eleven new meteorites from Antarctica, 1976-1977

Basic petrographic, mineralogic, and chemical descriptions are given for all eleven meteorites recovered by the U.S.-Japan team in Antarctica during the austral summer 1976-1977. The meteorites are: Mt. Baldr a (H6), Mt. Baldr b (H6), Allan Hills 1 (L6), Allan Hills 2 (coarsest octahedrite, chemical group IA), Allan Hills 3 (L6), Allan Hills 4 (LL3), Allan Hills 5 (eucrite), Allan Hills 6 (H6), Allan Hills 7 (L6), Allan Hills 8 (H6), and Allan Hills 9 (L6).

Olsen, E. J.↗
NASA NTRS1973

Meteoritic, lunar and Lonar impact chondrules.

Impact-generated silicate spherules from the Lonar Crater, India and from all Apollo sites are analogous to meteoritic chondrules (and some microtektites). Thus, the impact origin of chondrules, first proposed by Urey (1952) is a mechanism strongly supported by physical evidence from both the moon and the earth. Chondrites appear to be essentially impact breccias similar to lunar and Lonar microbreccias. The implications of this with regard to size and composition of the meteorite parent bodies are reviewed as well as the possible variations of element fractionation by volatilization-condensation.

Fredriksson, K.↗
NASA NTRS1972

Lunar glasses, breccias, and chondrules.

Glasses from Apollo 11, 12, 14, and 15 soil samples have been grouped on the basis of their chemistry and appear to provide an independent tool for identifying the presence of various rock types. The glasses also appear to constitute a record of complex differentiation processes that seem to have taken place within the moon. A green glass, abundant in some samples from Hadley Delta, could have been formed from a previously proposed differentiation model. Four breccias are described briefly and certain similarities between impact features, including chondrules, in lunar samples and meteorites are noted.

Nellen, J.↗
NASA NTRS1971

A summary of phase analysis on Apollo 14 samples

The results of an analysis of lunar samples from Apollo 14 are presented. The large number of breccias returned from the Fra Mauro formation show that impact events are an important rock forming mechanism on the moon. Larger rocks as well as micro breccias bear structural resemblance to brecciated chondrites and terrestrial impactites. Many show evidence of repetitious events of break-up and accumulation welding. The surface of the regolith has become thoroughly mixed by this process. Most components however appear locally derived from basalts rich in feldspar and Kreep components, similar to rocks such as 14310.

Fredriksson, K.↗