Abstract

The study of the degassing of primitive cosmic matter (in particular meteorites) allows us to better understand and evaluate the processes that occur during the formation of the primary (lost) and secondary atmospheres of rocky planets. To do this, the author’s technique using a specially designed device was employed. Continuing the ideas of the previous work, where the composition of the volatile LL5 chondrite was analyzed, this article describes the study of Aba Panu L3 chondrite by the same methods: calcination in the temperature range from 200 to 800°C in increments of 100°C. The composition and amount of volatile components extracted is evaluated on a chromatograph.

中文翻译：

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ABA Panu（L3）陨石脱气产物组成的研究

摘要

对原始宇宙物质（特别是陨石）进行脱气的研究使我们能够更好地理解和评估岩石行星一次（失落）和二次大气形成过程中发生的过程。为此，采用了作者使用的特殊设计的技术。继续先前工作的思想，分析了挥发性LL5球粒陨石的成分，本文通过相同的方法描述了Aba Panu L3球粒陨石的研究：在200至800°C的温度范围内以100°为增量进行煅烧C。在色谱仪上评估提取的挥发性成分的组成和量。