来自Lonar陨石坑撞击物(印度)和月球风化层的原生镍铁金属

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2023-08-15 DOI:10.1134/S0038094623040032
T. A. Gornostaeva, P. M. Kartashov, A. V. Mokhov, A. P. Rybchuk, A. T. Basilevsky
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引用次数: 0

摘要

印度的Lonar陨石坑是地球上保存最好、研究最多的陨石坑,它是由玄武岩形成的,可以与月球和太阳系其他行星上的矿物撞击转化进行比较研究。比较研究表明,无论是在地球上还是在月球上,撞击物的物质不仅像以前认为的那样以地球化学的分散形式存在,而且还以单个亚微米颗粒的形式分布在熔融的目标物质中。这些是天然镍、带长石和高镍卡玛石的颗粒,很明显,它们是撞击器的转化物质。高镍亚微米金属夹杂物在洛纳尔陨石坑的撞击物中广泛存在,因为它们在所有研究过的从陨石坑边缘不同地点收集的材料制成的准备物中都有发现。在这项研究中发现的高镍颗粒是支持先前关于球粒陨石类型撞击器的假设的另一个论据。
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Native Nickel–Iron Metals from Lonar Crater Impactites (India) and Regolith of the Moon

Abstract

The Lonar crater (India) is the best preserved and most studied on Earth, formed in basalts, which makes it possible to conduct a comparative study with impact transformations of mineral matter on the Moon and other planets of the Solar System. Comparative studies have shown that impactor material, both on the Earth and on the Moon, is present in impactites not only in a geochemically dispersed form, as previously thought, but also in the form of individual submicron particles distributed in the molten target material. These are particles of native nickel, taenite, and high-nickel kamacite, which, apparently, are the transformed material of the impactor. High-nickel submicron metal inclusions are widespread in the impactites of the Lonar crater, as they were found in all studied preparations made from materials collected from different points along the rim of the crater. The high-nickel particles found in this study are an additional argument in favor of the previously stated assumption about the chondrite type of impactor.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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