Pressure–temperature–time controls on shock vein formation within the Steen River impact structure

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Randy G. Hopkins, John. G. Spray, Erin L. Walton
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Abstract

Thermodynamic modeling has been applied to determine pressure–temperature–time conditions leading to shock vein formation during the passage of a natural shock wave generated by hypervelocity impact. The approach is novel in considering both shock front and rarefaction pressures, as well as simultaneously forming and cooling the shock veins via two-dimensional steady-state conduction. Model results are tested using shock veins developed in granitic rocks that constitute the central uplift of the Steen River impact structure in Canada. Here, two variants of majoritic garnet were generated in different settings: (1) along the margins of shock veins due to pargasite and biotite breakdown (accompanied by maskelynite formation), and (2) within the originally molten shock vein matrix as newly grown crystals. We determine that during shock vein formation, the shock front pressure and wave width at the reconstructed sample location were 18 GPa and 830 m, respectively, with a dwell time of 160 ms. Intra-vein melting at 2150°C was attained within 1 μs. Melt cooled to the solidus in 150 ms following shock front passage. Majoritic garnet formation was facilitated by the high temperatures realized within the veins as a result of frictional melting that accompanied shock loading. The calculated pressure–temperature–time (PTt) path provides constraints on the formation conditions of majoritic garnet at Steen River. The model results independently support previously determined PT conditions based on mineral stability fields. The vein margin garnets (35–39 mole% majorite) and maskelynite formed first under higher PT conditions for a longer duration (36 ms). The matrix garnets (11–22 mole% majorite) crystallized from melt under lower PT conditions and for a shorter duration (22 ms). Our results indicate that shock pressure alone should not be used as a basis for shock classification. Instead, the interplay between pressure and temperature with time and the duration of shock immersion (dwell) must be considered.

Abstract Image

斯泰恩河冲击结构内冲击脉形成的压力-温度-时间控制因素
应用热力学模型确定了超高速撞击产生的自然冲击波通过时导致冲击脉形成的压力-温度-时间条件。该方法的新颖之处在于同时考虑了冲击前压和稀释压力,以及通过二维稳态传导同时形成和冷却冲击脉。模型结果利用花岗岩中形成的冲击脉进行了检验,花岗岩构成了加拿大斯蒂恩河冲击构造的中央隆起。在这里,两种主要石榴石变体是在不同环境下产生的:(1)沿冲击脉边缘,由于辉石和生物榴石的分解(伴随着蒙脱石的形成),以及(2)在最初熔融的冲击脉基质内,作为新生长的晶体。我们确定,在冲击脉形成过程中,重建样本位置的冲击前沿压力和波宽分别为 18 GPa 和 830 米,停留时间为 160 毫秒。在 1 μs 内达到 2150°C 的脉内熔化。熔体在冲击前沿通过后的 150 毫秒内冷却至凝固点。由于伴随着冲击加载的摩擦熔化,矿脉内的高温促进了主要石榴石的形成。计算出的压力-温度-时间(P-T-t)路径为斯蒂恩河的大橄榄石榴榴石的形成条件提供了约束。模型结果独立地支持了之前根据矿物稳定性场确定的 P-T 条件。脉缘石榴石(35-39 摩尔%的橄榄石)和蒙德拉石首先在较高的 P-T 条件下形成,持续时间较长(36 毫秒)。基质石榴石(11-22 摩尔%的橄榄石)在较低的 P-T 条件下从熔体中结晶,持续时间较短(22 毫秒)。我们的研究结果表明,不应仅以冲击压力作为冲击分类的依据。相反,必须考虑压力和温度与时间以及冲击浸泡(停留)时间之间的相互作用。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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