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Microstructural Characterization of TiO2-II in the Chicxulub Peak RingThe peak ring of the approximately 180 kilometer-diameter Chicxulub impact crater on the Yucatan Peninsula, Mexico, was recently drilled during IODP-ICDP (International Ocean Discovery Program-International Continental Scientific Drilling Program) Expedition 364, producing core M0077A. The new core provides insights into the anatomy, composition, tectonic deformation, shock metamorphism, and post-impact overprint of crater-filling impactites and crystalline basement rocks. The basement rocks were shocked to approximately 12.5-17.5 gigapascals, uplifted, and hydrothermally altered. This study presents a combined Raman spectroscopic and electron backscatter diffraction (EBSD) study of TiO2-II, a high-pressure polymorph of TiO2 with an alpha-PbO2 structure (orthorhombic; space group Pbcn; density 4.34 grams per cubic centimeter, in shocked granitoid rock of the Chicxulub peak ring.
Document ID
20190001742
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Schmieder, Martin
(Lunar and Planetary Institute (LPI) Houston, TX, United States)
Erickson, Timmons M.
(Jacobs Technology, Inc. Houston, TX, United States)
Kring, David A.
(Lunar and Planetary Institute (LPI) Houston, TX, United States)
Date Acquired
March 21, 2019
Publication Date
March 18, 2019
Subject Category
Geophysics
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-E-DAA-TN64829
Report Number: JSC-E-DAA-TN64829
Funding Number(s)
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
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