Low-temperature thermal and physical properties of lunar meteorites

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
R. J. Macke, C. P. Opeil, D. T. Britt, G. J. Consolmagno, A. Irving
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引用次数: 0

Abstract

Lunar meteorites are the most diverse and readily available specimens for the direct laboratory study of lunar surface materials. In addition to informing us about the composition and heterogeneity of lunar material, measurements of their thermo-physical properties provide data necessary to inform the models of the thermal evolution of the lunar surface and provide data on fundamental physical properties of the surface material for the design of exploration and resource extraction hardware. Low-temperature data are particularly important for the exploration of low-temperature environments of the lunar poles and permanently shadowed regions. We report low-temperature-specific heat capacity, thermal conductivity, and linear thermal expansion for six lunar meteorites: Northwest Africa [NWA] 5000, NWA 6950, NWA 8687, NWA 10678, NWA 11421, and NWA 11474, over the range 5 ≤ T ≤ 300 K. From these, we calculate thermal inertia and thermal diffusivity as functions of temperature. Additionally, heat capacities were measured for 15 other lunar meteorites, from which we calculate their Debye temperature and effective molar mass.

月球陨石的低温热和物理特性
月球陨石是实验室直接研究月球表面物质的最多样化和最容易获得的标本。除了让我们了解月球材料的成分和异质性之外,对其热物理性质的测量还提供了必要的数据,为月球表面的热演变模型提供了信息,并为设计探测和资源提取硬件提供了有关表面材料基本物理性质的数据。低温数据对于探测月球两极和永久阴影区的低温环境尤为重要。我们报告了六块月球陨石的低温特定热容量、热导率和线性热膨胀率:我们报告了六块月球陨石:西北非洲[NWA] 5000、NWA 6950、NWA 8687、NWA 10678、NWA 11421 和 NWA 11474 在 5 ≤ T ≤ 300 K 范围内的低温特定热容量和线性热膨胀率。此外,我们还测量了其他 15 块月球陨石的热容量,并从中计算出它们的德拜温度和有效摩尔质量。
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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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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