The source craters of the martian meteorites: Implications for the igneous evolution of Mars

被引:4
作者
Herd, Christopher D. K. [1 ]
Hamilton, Jarret S. [1 ,17 ]
Walton, Erin L. [2 ]
Tornabene, Livio L. [3 ,4 ]
Lagain, Anthony [5 ,6 ,7 ]
Benedix, Gretchen K. [5 ,8 ,9 ]
Sheen, Alex I. [1 ,10 ,11 ]
Melosh, Harry J. [12 ,13 ]
Johnson, Brandon C. [12 ,13 ]
Wiggins, Sean E. [12 ,14 ]
Sharp, Thomas G. [15 ]
Darling, James R. [16 ]
机构
[1] Univ Alberta, Dept Earth & Atmospher Sci, Edmonton, AB T6G 2E3, Canada
[2] MacEwan Univ, Dept Phys Sci, Edmonton, AB T5J 4S2, Canada
[3] Univ Western Ontario, Inst Earth & Space Explorat, Dept Earth Sci, 1151 Richmond St, London, ON N6A 5B7, Canada
[4] SETI Inst, 339 Bernardo Ave,Suite 200, Mountain View, CA 94043 USA
[5] Curtin Univ, Space Sci & Technol Ctr, Sch Earth & Planetary Sci, Bentley, WA, Australia
[6] Aix Marseille Univ, CNRS, IRD, INRAE,CEREGE, Aix En Provence, France
[7] Aix Marseille Univ, Inst ORIGINES, Marseille, France
[8] Planetary Sci Inst, Tucson, AZ 85719 USA
[9] Western Australian Museum, Dept Earth & Planetary Sci, Perth, WA, Australia
[10] Royal Ontario Museum, 100 Queens Pk, Toronto, ON M5S 2C6, Canada
[11] Univ Toronto, Dept Earth Sci, Toronto, ON M5S 3B1, Canada
[12] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA
[13] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA
[14] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[15] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
[16] Univ Portsmouth, Sch Environm Geog & Geosci, Portsmouth PO1 3QL, England
[17] Environm & Climate Change Canada, 9250 49 St NW, Edmonton, AB T6B 1K5, Canada
基金
加拿大自然科学与工程研究理事会; 澳大利亚研究理事会;
关键词
IMPACT CRATERS; MELT POCKETS; LOS-ANGELES; AGE; HISTORY; PETROLOGY; EJECTION; TISSINT; CONSTRAINTS; CHRONOLOGY;
D O I
10.1126/sciadv.adn2378
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Approximately 200 meteorites come from similar to 10 impact events on the surface of Mars, yet their pre-ejection locations are largely unknown. Here, we combine the results of diverse sets of observations and modeling to constrain the source craters for several groups of martian meteorites. We compute that ejection-paired groups of meteorites are derived from lava flows within the top 26 m of the surface. We link ejection-paired groups to specific source craters and geologic units, providing context for these important samples, reconciling microscopic observations with remote sensing records, and demonstrating the potential to constrain the ages of their source geologic units. Furthermore, we show that there are craters that may have produced martian meteorites not represented in the world's meteorite collections that have yet to be discovered.
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页数:9
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