Computer Science
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975moon...12..331c&link_type=abstract
The Moon, vol. 12, Mar. 1975, p. 331-360.
Computer Science
3
Lunar Rocks, Meteoritic Composition, Tektites, Volcanology, Ballistic Trajectories, Geomorphology, Lunar Composition, Lunar Maria, Metamorphism (Geology)
Scientific paper
The possibility is considered that tektites are lunar volcanic ejecta, and lunar regions are examined from which tektites could be ejected with the necessary velocities and trajectories to reach the earth. The examined regions include areas around the Lunar Transient Phenomena sites near Censorinus, Messier, Messier A, and Taruntius, the area of Mare Foecunditatis near Secchi X, areas near Cauchy and Capella, and the eastern part of Mare Tranquillitatis. Evidence of acidic volcanic activity in these regions is described in detail, including possible calderas, mudflows, and endogenous domes. It is suggested that the moon is still gently degassing and that more violent eruptions of material may still occur on rare occasions. Remotely-sensed evidence of recent lunar internal activity is noted.
Lowrey Barbara E.
Sawtell Cameron Winifred
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