Journal
EARTH AND PLANETARY SCIENCE LETTERS
Volume 288, Issue 3-4, Pages 619-623Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.epsl.2009.10.030
Keywords
martian meteorite; Chassigny; ringwoodite; high-pressure phase; shock metamorphism
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Funding
- Helmholtz-Alliance
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Shock-induced melt pockets in the martian meteorite Chassigny are completely transformed into a set of high-pressure mineral phases previously unknown from ultramafic rocks, the major constituents of the Earth's mantle. Ferropericlase, amorphous (Mg,Fe)SiO(3)-perovskite, ringwoodite, wadsleyite, high-pressure phosphate gamma-Ca(3)(PO(4))(2), and CaTi(2)O(4)-structurecl chromite were formed by solid state transformation and fractional crystallization upon pressure release from >23 to 10 GPa. During shock pressure release the temperatures in the melt pocket dropped to timescales of 10(-2) to 10(-3) S to allow preservation of the high-pressure phases. Formation and preservation of these phases in Chassigny depend on the duration of shock compression, which increases with the pre-impact burial depth of the meteorite below the martian surface. The estimated burial depth of 25 to 250 m is in agreement with the sampling depth of potential source craters for the Chassigny meteorite. (C) 2009 Elsevier B.V. All rights reserved.
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