NDLI: Preliminary discussion on the origin of lei-gong-mo (tektites)

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Preliminary discussion on the origin of lei-gong-mo (tektites)

Content Provider	NASA Technical Reports Server (NTRS)
Author	Baoyin, Y.
Copyright Year	1983
Description	The specimens of lei-gong-mo (tektites) were collected from Hainan Island and Leizhow Peninsula during the period from 1963 to 1975. The distribution, forms, sculpture, abration surface (bald spot), internal structure and chemical composition of lei-gong-mo are discussed. Studies of these materials lead to the following conclusions: (1) the specimens of lei-gong-mo can be morphologically divided into eight types; (2) the sculptures on the surface of lei-gong-mo are probably due to the corrosion effect of volcanic gas, and the abration surface due to the aerodynamic corrosion; (3) the folded structures in the layered lei-gong-mo (Muong Nong-type tektite) seem hardly to be formed by an impact of meteorites, but they might be produced in the magma flow process when the lei-gong-mo was melting within the crater vent; and (4) the comparison of its chemical composition with that of basalt from Hainan Island does not show that lei-gong-mo came from the local volcano. The hypothesis of the lunar volcanic origin of tektites is examined.
File Size	1028828
Page Count	19
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19840009027
Archival Resource Key	ark:/13960/t22c3v97n
Language	English
Publisher Date	1983-04-01
Access Restriction	Open
Subject Keyword	Lunar And Planetary Exploration Origins Tektites Corrosion Lunar Composition Vitreous Materials Meteoritic Composition Surface Roughness Chemical Composition Shapes Evolution Development Lunar Rocks Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Article

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