Experimental Simulations of Shock Textures in BCC Iron: Implications for Iron Meteorites
Eiji Ohtani, Toru Sakurabayashi, Kosuke Kurosawa

TL;DR
This study combines laboratory shock experiments and numerical simulations to understand the formation and disappearance of deformation twins in iron meteorites, revealing temperature and pressure conditions critical for their preservation.
Contribution
It provides new insights into the conditions under which Neumann bands form and are erased in iron meteorites through combined experimental and simulation approaches.
Findings
Neumann bands form at shock pressures of 1.5-13 GPa at temperatures up to 670 K.
Neumann bands disappear after annealing above 1070 K.
Meteorites with Neumann bands experienced shock pressures and temperatures below 1070 K.
Abstract
Neumann band in iron meteorites, which is deformation twins in kamacite (Fe-Ni alloy), has been known to be a characteristic texture indicating ancient collisions on parent bodies of meteorites. We conducted a series of shock recovery experiments on bcc iron with the projectile velocity at 1.5 km/sec at various initial temperatures, room temperature, 670 K, and 1100 K, and conducted an annealing experiment on the shocked iron. We also conducted numerical simulations with the iSALE-2D code to investigate peak pressure and temperature distributions in the nontransparent targets. The effects of pressure and temperature on the formation and disappearance of the twins (Neumann band) were explored based on laboratory and numerical experiments. The twin was formed in the run products of the experiments conducted at room temperature and 670 K, whereas it was not observed in the run product…
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