霍顿撞击结构的撞击生成热液系统建模

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Journal of Geophysical Research: Planets Pub Date : 2024-07-10 DOI:10.1029/2023JE008267
A. J. Trowbridge, Simone Marchi, Gordon R. Osinski, Joshua M. Taron
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引用次数: 0

摘要

超高速撞击可产生热液系统,被认为是早期地球上前生物化学的候选环境。霍顿撞击结构(位于加拿大北极努纳武特地区德文岛的一个直径 23 千米的陨石坑)显示了水岩蚀变的证据,表明宇宙撞击产生了热液系统。为了模拟这个陨石坑的形成和随后的热液蚀变,我们成功地开发了一种新的双代码方法,即利用冲击物理代码和热液代码(HYDROTHERM)。我们可以用直径为 700 米、撞击速度为 14 千米/秒的弹丸最好地再现霍顿陨石坑。通过我们的方法,我们能够与在霍顿撞击结构上观测到的所有主要地质制约因素相匹配。我们的模型显示,霍顿陨石坑内部可以维持嗜热生命和超嗜热生命理想的温度(50-120°C)超过5万年,这表明这些系统可以维持前生物化学和生命的时间比以前估计的要长。
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Modeling of the Impact-Generated Hydrothermal System at the Haughton Impact Structure

Hypervelocity impacts can generate hydrothermal systems, which have been suggested as candidate environments for prebiotic chemistry on the early Earth. The Haughton impact structure (a 23 km diameter crater located on Devon Island, Nunavut, Arctic Canada) displays evidence of water-rock alteration indicative of a hydrothermal system generated from a cosmic impact. To model the formation of this crater and subsequent hydrothermal alteration, we have successfully developed a new two-code methodology that utilizes a shock physics code and a hydrothermal code (HYDROTHERM). We can best reproduce the Haughton crater with a ∼700 m diameter projectile with an impact velocity of 14 km/s. With our approach, we were able to match all the major geological constraints observed at the Haughton impact structure. Our models show that the Haughton crater interior could have sustained temperatures ideal for thermophilic and hyperthermophilic life (50–120°C) for more than 50,000 years, indicating that these systems can sustain prebiotic chemistry and life for longer than previously estimated.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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