Structural changes in shocked tektite and their implications to impact-induced glass formationOPEN ACCESS 

Toshimori Sekine, Tsubasa Tobase, Youjun Zhang, Ginga Kitahara, Akira Yoshiasa, Tomoko Sato, Takamichi Kobayashi, and Akihisa Mori

American Mineralogist


“Heavy meteorite impacts on the Earth surface produce melt and vapor which are quenched rapidly and scattered over wide areas as natural glasses with various shapes and characteristic chemistry, that are known as tektites and impact glasses. Their detailed formation conditions have long been debated in many studies using mineralogical and geochemical data and numerical simulations of impact melt formations. These impact processes are also related to the formation and evolution of planets. To unravel the formation conditions of impact-induced glasses, we performed shock recovery experiments on a tektite. Recovered samples were characterized by X-ray diffraction, Raman spectroscopy, and X-ray absorption fine structure spectroscopy on Ti K-edge. Results indicate that the densification by shock compression is subjected to post-shock annealing that alters the density and silicate-framework structures, but that the local structures around octahedrally coordinated Ti ions remain in the quenched glass. The relationship between the average Ti-O distance and Ti K pre-edge centroid energy is found to distinguish the valance state of Ti ions between Ti4+ and Ti3+ in the glass. This relationship is useful in understanding the formation conditions of impact derived natural glasses. The presence of Ti3+ in tektites constrains the formation conditions at extreme high temperatures or reduced environments. However, impact glasses collected near the impact sites do not display such conditions, but rather relatively mild and oxidizing formation conditions. These different formation conditions are consistent with the previous numerical results on the crater size dependence.”