ON THE LUNAR ORIGIN OF TEKTITES
Lunar origin of tektites - atmospheric entry dynamics
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Lunar origin of tektites - atmospheric entry dynamics
Theory of origin and distribution of tektites based on aerodynamic considerations and from observations of satellite and meteor breakup
Atmospheric entry aerodynamics applied to tektites to give evidence of their lunar origin
Speculation on the origin formation of tektites from silicic igneous rocks, specifically rhyolitic tuffs, forming the upper layers of the lunar maria
Spectroscopic analysis reveals that gases in tektite bubbles are neon, helium and oxygen
Rubidium, strontium, & strontium isotopic composition of tektites
Hypothesis on tektite origin by comet impact with earth
Tektites and silica glasses - history, chemical composition, geometry, nomenclature, distribution, localization, and local geology at discovery sites
Metal spherules synthesized by melting philippine tektites
Comparison of specific gravity of tektites from australia, asia, texas, and czechoslovakia
Theory of tektite origin on moon as impact fragments
Terrestrial and lunar origin of tektites evaluated, emphasizing meteorite impact on the lunar mare
Origin of tektites and impact fragments from the moon
Physical and chemical properties of tektites from various locations
Rubidium, strontium, and strontium isotopic compositions in tektites from various locations
Analyses of major elements in tektite by rapid silicate procedures and X-ray fluorescence techniques