Abstract
The mineral apatite, Ca5(PO4)3(F,Cl,OH), is a ubiquitous accessory mineral, with its volatile content and isotopic compositions used to interpret the evolution of H2O on planetary bodies. During hypervelocity impact, extreme pressures shock target rocks resulting in deformation of minerals; however, relatively few microstructural studies of apatite have been undertaken. Given its widespread distribution in the solar system, it is important to understand how apatite responds to progressive shock metamorphism. Here, we present detailed microstructural analyses of shock deformation in ~560 apatite grains throughout ~550 m of shocked granitoid rock from the peak ring of the Chicxulub impact structure, Mexico. A combination of high-resolution backscattered electron (BSE) imaging, electron backscatter diffraction mapping, transmission Kikuchi diffraction mapping, and transmission electron microscopy is used to characterize deformation within apatite grains. Systematic, crystallographically controlled deformation bands are present within apatite, consistent with tilt boundaries that contain the 'c' (axis) and result from slip in ' (Formula presented.) ' (direction) on (Formula presented.) (plane) during shock deformation. Deformation bands contain complex subgrain domains, isolated dislocations, and low-angle boundaries of ~1° to 2°. Planar fractures within apatite form conjugate sets that are oriented within either { (Formula presented.), { (Formula presented.), { (Formula presented.), or (Formula presented.). Complementary electron microprobe analyses (EPMA) of a subset of recrystallized and partially recrystallized apatite grains show that there is an apparent change in MgO content in shock-recrystallized apatite compositions. This study shows that the response of apatite to shock deformation can be highly variable, and that application of a combined microstructural and chemical analysis workflow can reveal complex deformation histories in apatite grains, some of which result in changes to crystal structure and composition, which are important for understanding the genesis of apatite in both terrestrial and extraterrestrial environments.
Original language | English |
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Pages (from-to) | 1715-1733 |
Number of pages | 19 |
Journal | Meteoritics and Planetary Science |
Volume | 55 |
Issue number | 8 |
Early online date | 4 Aug 2020 |
DOIs | |
Publication status | Published - Aug 2020 |
Funding
The IODP-ICDP Expedition 364 Science Party is composed of S. Gulick (US), J. V. Morgan (UK), G. Carter (UK), E. Chenot (France), G. Christeson (US), Ph. Claeys (Belgium), C. Cockell (UK), M. J. L. Coolen (Australia), L. Ferri?re (Austria), C. Gebhardt (Germany), K. Goto (Japan), H. Jones (US), D. A. Kring (US), J. Lofi (France), C. Lowery (US), R. Ocampo-Torres (France), L. Perez-Cruz (Mexico), A. Pickersgill (UK), M. Poelchau (Germany), A. Rae (UK), C. Rasmussen (US), M. Rebolledo-Vieyra (Mexico), U. Riller (Germany), H. Sato (Japan), J. Smit (Netherlands), S. Tikoo (US), N. Tomioka (Japan), M. Whalen (US), A. Wittmann (US), J. Urrutia-Fucugauchi (Mexico), L. Xiao (China), and K. E. Yamaguchi (Japan). Work by MAC, MS, and DAK at the LPI was partially supported by National Science Foundation (NSF) award 1736826. Support was also provided by the LPI Summer Intern Program in Planetary Sciences and the Space Science and Technology Center at Curtin University. LPI Contribution no. 2370. LPI is operated by USRA under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. We thank the editor Christian Koeberl and reviewers A. Cernok and an anonymous reviewer for constructive comments.
Funders | Funder number |
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Space Science and Technology Center at Curtin University | 2370 |
USRA | |
National Science Foundation | |
Directorate for Geosciences | 1736826 |
National Aeronautics and Space Administration |