Experimental Transformation of the Chelyabinsk LL5 Meteorite Matter of Light-colored Lithology into Dark-colored Lithology

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
E. V. Petrova, V. I. Grokhovsky
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Abstract

The effects of temperature, impacts, and irradiation on Chelyabinsk LL5 chondrite light-colored lithology matter were simulated in the laboratory conditions. Various changings of the texture and structure registered by different methods and techniques. As similarity as differences between the experimental results and the natural dark-colored lithology samples of Chelyabinsk LL5 were detected. Irradiation with Ar ions cause darkening, but this effect touches a surface only. While the shock experiment with the spherically-converted shock waves produced all types of lithologies that were found among the Chelyabinsk LL5 chondrite collection. Impact melt zone was formed under maximum pressure at the center of the sample. Next—zone with extensive silicate melting, then zone of dark lithology or black-ring zone, and zone of additionally shock-loaded original light-colored lithology situated in the shocked ball sample. Heating to 1100°C led to the dark-colored lithology structure formation with troilite melting, metal recrystallization, and optical darkening. Heating for a lower temperature produced effects in morphology of the metal and troilite inclusions. While heating for higher temperature induce melting of the host silicates and new crystals grows. It was assumed that dark-colored lithology was formed as a result of heating of the material of light-colored lithology. This assumption was verified by experimental studies of the meteorite substance after thermal, shock and radiation effects in laboratory experiments.

Abstract Image

车里雅宾斯克LL5陨石浅色岩性向深色岩性转化的实验研究
在实验室条件下模拟了温度、撞击和辐照对车里雅宾斯克LL5球粒陨石浅色岩性物质的影响。用不同的方法和技术记录纹理和结构的各种变化。检测了实验结果与车里雅宾斯克LL5天然深色岩性样品的异同。用氩离子照射会使颜色变暗,但这种影响只会触及表面。而用球体转换冲击波进行的冲击实验产生了车里雅宾斯克LL5球粒陨石收集中发现的所有类型的岩性。在最大压力作用下,试样中心形成冲击熔体区。下一个区域是广泛的硅酸盐熔融区,然后是深色岩性区或黑环区,以及位于受冲击球样品中的原始浅色岩性的额外冲击加载区。加热至1100℃,形成深色岩性结构,并伴有三硅石熔融、金属再结晶和光学变暗。在较低温度下加热会对金属和三苯胺包裹体的形貌产生影响。当加热温度升高时,主体硅酸盐熔化,新晶体生长。据推测,深色岩性是浅色岩性材料受热而形成的。在实验室实验中对陨石物质进行了热、冲击和辐射作用后的实验研究,验证了这一假设。
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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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