Shock synthesis of quasicrystals with implications for their origin in asteroid collisions

1Paul D. Asimow, 2Chaney Lin, 3,4Luca Bindi, 1Chi Ma, 5,6Oliver Tschauner, 7Lincoln S. Hollister,8Paul J. Steinhardt
Proceedings of the National Academy of Sciences 113 7077–7081 Link to Article [doi: 10.1073/pnas.1600321113]
1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125;
2Department of Physics, Princeton University, Princeton, NJ 08544;
3Dipartimento di Scienze della Terra, Università degli Studi di Firenze, I-50121 Firenze, Italy;
4Consiglio Nazionale delle Ricerche–Istituto di Geoscienze e Georisorse, Sezione di Firenze, I-50121 Firenze, Italy;
5Department of Geoscience, University of Nevada, Las Vegas, NV 89154;
6High Pressure Science and Engineering Center, University of Nevada, Las Vegas, NV 89154;
7Department of Geosciences, Princeton University, Princeton, NJ 08544;
8Princeton Center for Theoretical Science, Princeton University, Princeton, NJ 08544

We designed a plate impact shock recovery experiment to simulate the starting materials and shock conditions associated with the only known natural quasicrystals, in the Khatyrka meteorite. At the boundaries among CuAl5, (Mg0.75Fe2+0.25)2SiO4 olivine, and the stainless steel chamber walls, the recovered specimen contains numerous micron-scale grains of a quasicrystalline phase displaying face-centered icosahedral symmetry and low phason strain. The compositional range of the icosahedral phase is Al68–73Fe11–16Cu10–12Cr1–4Ni1–2 and extends toward higher Al/(Cu+Fe) and Fe/Cu ratios than those reported for natural icosahedrite or for any previously known synthetic quasicrystal in the Al-Cu-Fe system. The shock-induced synthesis demonstrated in this experiment reinforces the evidence that natural quasicrystals formed during a shock event but leaves open the question of whether this synthesis pathway is attributable to the expanded thermodynamic stability range of the quasicrystalline phase at high pressure, to a favorable kinetic pathway that exists under shock conditions, or to both thermodynamic and kinetic factors.

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