Features of Degassing of the Carbonaceous Chondrite Dar al Gani 190 (CO3) in the Temperature Range 200–800°C

IF 0.7 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
S. A. Voropaev, N. V. Dushenko, A. P. Krivenko, V. S. Fedulov, K. M. Ryazantsev
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引用次数: 0

Abstract

The degassing of material from the carbonaceous chondrite Dar al Gani (DaG) 190 (type CO3) was studied using a specially designed experimental setup. The results of experimental investigations on heating and isothermal holding (pyrolysis) of meteorite samples are presented, with the composition of released gases determined by gas chromatography. Raman spectra and IR spectra were obtained for both the primary material of DaG 190 (CO3 type) and after annealing at three temperatures: 200, 500, and 800°C. Based on these data, the thermal transformation process of the asteroid material—the parent body of the meteorite—was traced. A comparison was made with the degassing results of another carbonaceous chondrite, Allende (type CV3). Cosmochemical applications to the accretion processes of terrestrial planets are discussed, as well as the role of carbonaceous chondrites as sources of water, gases, and volatile compounds for the Moon and early Earth.

Abstract Image

200 ~ 800℃范围内碳质球粒陨石Dar al Gani 190 (CO3)脱气特征
采用专门设计的实验装置研究了碳质球粒陨石Dar al Gani (DaG) 190 (CO3型)的脱气过程。本文介绍了对陨石样品进行加热和等温保温(热解)的实验研究结果,并用气相色谱法测定了释放气体的组成。获得了DaG 190 (CO3型)的原始材料以及在200、500和800℃三种温度下退火后的拉曼光谱和红外光谱。根据这些数据,对小行星物质(陨石的母体)的热转化过程进行了追踪。并与另一种碳质球粒陨石Allende (CV3型)的脱气结果进行了比较。讨论了宇宙化学在类地行星吸积过程中的应用,以及碳质球粒陨石作为月球和早期地球的水、气体和挥发性化合物来源的作用。
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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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