Features of Degassing of the Murchison (CM2) Carbonaceous Chondrite in the Temperature Interval of 200–800°C

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
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引用次数: 0

Abstract

The degassing of Murchison carbonaceous chondrite (CM2 type) was studied using a setup specially designed for this purpose. The experiments involved stepwise heating (without gas accumulation) and isothermal annealing of meteorite samples with the composition of released gases determined through gas chromatography methods in the temperature range from 200 to 800°C. To account for sorbed water, degassing at 50 and 110°C was additionally analyzed. The IR spectra of the Murchison meteorite were obtained after annealing at different temperatures and used to trace the thermal degradation. The comparison with the degassing of the ordinary chondrite Chelyabinsk (type LL5) revealed a significant increase in the release of carbonaceous gases for the Murchison meteorite.

默奇森(CM2)碳质软玉在 200-800°C 温度区间的脱气特征
摘要 利用专门为此目的设计的装置研究了默奇森碳质软玉(CM2 型)的脱气情况。实验包括陨石样品的逐步加热(无气体积累)和等温退火,在 200 至 800°C 的温度范围内通过气相色谱法测定释放气体的成分。为了考虑吸附水,还对 50 和 110°C 的脱气情况进行了分析。在不同温度下退火后,获得了默奇森陨石的红外光谱,用于追踪热降解情况。通过与普通陨石车里雅宾斯克陨石(LL5 型)的脱气情况进行比较,发现默奇森陨石释放的碳质气体显著增加。
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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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