Contrasting meteoritic signatures within the Clearwater East and Clearwater West impact structures: The view from osmium isotopes

被引:2
|
作者
Daly, R. Terik [1 ]
Schultz, Peter H. [1 ]
Lassiter, John C. [2 ]
Loewy, Staci W. [2 ]
Thompson, Lucy M. [3 ]
Spray, John G. [3 ]
机构
[1] Brown Univ, Dept Earth Environm & Planetary Sci, 324 Brook St,Box 1846, Providence, RI 02912 USA
[2] Univ Texas Austin, Jackson Sch Geosci, Dept Geol Sci, 1 Univ Stn C1100, Austin, TX 78712 USA
[3] Univ New Brunswick, Planetary & Space Sci Ctr, Fredericton, NB E3B 5A3, Canada
基金
美国国家科学基金会;
关键词
Impact crater; West clearwater; East clearwater; Osmium isotopes; Meteoritic signature; Impactor component; Projectile signature; PLATINUM-GROUP ELEMENTS; JURASSIC-CRETACEOUS BOUNDARY; HIGHLY SIDEROPHILE ELEMENTS; SOLAR-SYSTEM; SOUTH-AFRICA; UPPER-MANTLE; MELT ROCKS; CRATER; OS; PROJECTILE;
D O I
10.1016/j.gca.2018.06.002
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Osmium isotopes provide a powerful tool for identifying meteoritic signatures in impactites. We apply the osmium isotope method to impact melt and country rocks from the Clearwater East and Clearwater West craters located in Quebec, Canada. Impact melts from Clearwater East have Os-187/Os-188 ratios of 0.1281-0.1285. These values indicate a significant meteoritic component, which exceeds that in impact melts at all terrestrial craters studied to date, except Morokweng. Such findings align with earlier results from chromium isotopes and platinum-group elements. In contrast, impact melts from Clearwater West have Os-187/Os-188 ratios between 6.604 and 59.12. These highly radiogenic ratios are indistinguishable from the Os-187/Os-188 ratios in country rocks. Hence, osmium isotopes provide no evidence for a meteoritic component in impact melts at Clearwater West. The Clearwater craters formed in almost identical targets. Therefore, target effects cannot readily explain the stark difference between the two Clearwater craters. If melt sheet heterogeneity is similar at the two craters, the probability that melts at Clearwater West host an undetected chondritic component is < 0.2%. Multiple scenarios may explain the non-detection of a meteoritic signature at West; the possibility of a differentiated achondrite impactor could be tested using chromium isotopes. At Clearwater East, a low impact speed (<10 km s(-1)) may best explain the unusually strong meteoritic signature. Although the signature (or its nondetection) at each crater may be related to asymmetric preservation of the impactor component, the results presented here provide further evidence that Clearwater East and Clearwater West were temporally separate impact events. (C) 2018 Elsevier Ltd. All rights reserved.
引用
收藏
页码:262 / 284
页数:23
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