On Earth, natural glasses are typically produced by rapid cooling of melts, and as in the case of minerals and rocks, natural glasses can provide key information on the evolution of the Earth. However, we are aware that natural glasses are products not solely terrestrial and that the formation mechanisms give rise to a variety of natural amorphous materials. On the Earth´s surface, glasses are scarce compared to other terrestrial bodies (i.e. Moon), since the
CONTENTS-QUENCHED GLASSES 1.1 -Volcanic glasses Applications: alteration of natural glasses as analogue of nuclear waste glasses 1.2 -Lunar glasses 2 -IMPACT GLASSES 2.1 -Tektites and microtektites 2.2 -K-Pg (KT) spherules 2.3 -Younger Dryas (YD) event 2.4 -Enigmatic impact glasses 2.4.1 -LDG -Libyan Desert Glass 2.4.2 -Darwin glass 2.5 -Fulgurites 3 -OBSIDIAN 3.1 -Hydrated and altered obsidians 4 -OTHERS 4.1 -Glasses from nuclear explosion 4.2 -Friction melts 4.3 -Bioglasses 5 -Insights into the structure and properties of glasses
-ConclusionsTo date, four main groups of tektites, associated with separate impacts and strewn fields (SF), are known (e.g., [68][69][70][71]): the North American, the Ivory Coast, the central European and the Australasian (Fig. 10). The source craters have been located for three of the four tektite strewn fields, based on geographic location, geochemical evidences, and composition [72][73][74].The oldest strewn field is the North American (NA) field of ~ 35.5 Ma age associated with the ~ 40 km wide Chesapeake Bay impact structure [75] and includes Bediasites, Georgianites, Barbados and Cuba tektites, respectively found in Texas, Georgia, Barbados and Cuba (Fig. 10). The central European (CE) or moldavite strewn field of 14.4 Ma age is associated with the Ries crater of about 24km in diameter (Nördlinger Ries, Bavaria, D).There is another impact crater, the Steinheim crater, ~ 3.8 km in diameter, located about 42 kilometers west-southwest from the centre of Ries. These two craters are believed to have formed nearly simultaneously by the impact of a binary asteroid [76]. The Ivory Coast (IC) tektite strewn field is associated with the 1.07 Ma old Bosumtwi crater (10.5 km diameter, Ghana, Africa). The youngest SF, of about 0.8 Ma, is the Australasian one, for which no source crater has been identified so far. Tektites of the Australasian strewn field (AA) include australites, thailandites, indochinites, philippinites and javanites and spread from the southeastern region of Asia down to Australia (Fig. 10). Recently, glass spherules (microtektites) were discovered on the Victoria Land Transantarctic Mountains (Antarctica) and there is clear evidence [69,77,78] that these microtektites represent a major southeastward extension of the Australasian strewn field.Even if no source crater has been discovered yet, several authors suggest a location for the AA crater in the Indochina region (see [79][80][81][82]).