印度隆纳尔陨石坑撞击岩和月球岩石中的铜镍系天然合金

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2024-07-12 DOI:10.1134/s0038094624700266
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

摘要 对印度德干玄武岩高原洛纳尔陨石坑的撞击玻璃和苏联自动站(AS)月球-16 号和月球-24 号(丰饶之海和危机之海)提供的月球碎屑岩的撞击玻璃进行了比较研究。在洛纳尔陨石坑的撞击岩和月球碎屑中发现了许多以前在自然界中未知的天然合金(Cu3Ni2、Ni2Cu 和 Ni3Cu)。这类合金的发现扩大了铜镍系统的同构范围。通过对地球和月球的撞击岩进行比较,发现铜镍合金颗粒的成分、大小和形态都很相似,这可能是撞击过程的一个指标。形成镍-铜粒子的可能机制之一是气体等离子体云的冷凝。铜镍合金的可能材料来源是撞击器材料和目标材料。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Natural Alloys of the Cu–Ni System from Impactites of the Lonar Crater (India) and Lunar Regolith

Abstract

A comparative study of impact glasses from the Lonar crater, located on the Deccan basalt plateau, India, and impact glasses from lunar regolith delivered by the Soviet automatic stations (AS) Luna-16 and Luna-24 (Sea of Plenty and Sea of Crises) was carried out. Numerous natural alloys (Cu3Ni2, Ni2Cu and Ni3Cu) that were previously unknown in nature were discovered in the impactites of the Lonar crater and the regolith of the Moon. The discovery of such alloys expands the area of isomorphism in the Cu–Ni system. As a result of a comparison of impactites of the Earth and the Moon, similarities were discovered in the composition, size and morphology of particles of copper–nickel alloys, which may be an indicator of impact processes. One of the possible mechanisms for the formation of Ni–Cu particles was condensation from a gas–plasma cloud. A possible source of material for Cu–Ni alloys was both the impactor material and the target material.

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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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