A short history of astropedology

Gregory J. Retallack
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Abstract

Astropedology is the study of soils on other planetary bodies and stretches the definition of soil to materials on the surface of a planetary body altered in place by physical, chemical, or biological processes. This new disciplinary name was coined by Roy E. Cameron in 1966 from studies of desert soils and their microbes in Arizona and Antarctica as analogs for Martian soils to be investigated by NASA Viking missions. Astropedology now has documented numerous actual soil profiles exposed in cliff faces, natural cracks, or cores studied by robotic missions to the Moon, Venus, and Mars, with increasingly advanced and precise chemical and other analyses. Specimens are also available for study from Lunar and Martian meteorites, and from sample return from the Moon, also planned from Mars. Life has yet to be found beyond Earth, but Mars has surprisingly Earth-like soils, which can be identified as Gypsids in US taxonomy. Soil formation by micrometeoroid bombardment on the Moon and by melting and glazing on Venus are truly out of this world.

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星象学的简短历史
天体土壤学是一门研究其他行星上土壤的学科,它将土壤的定义扩展到行星表面经过物理、化学或生物过程改变的物质。这个新的学科名称是由罗伊·e·卡梅伦在1966年创造的,他在亚利桑那州和南极洲研究沙漠土壤及其微生物,作为美国宇航局维京号任务研究的火星土壤的类似物。通过对月球、金星和火星的机器人任务,以及越来越先进和精确的化学和其他分析,天体学现在已经记录了大量暴露在悬崖表面、自然裂缝或岩心中的实际土壤剖面。月球和火星陨石的样本也可用于研究,以及从月球返回的样本,也计划从火星返回。在地球以外的地方还没有发现生命,但火星上有令人惊讶的类似地球的土壤,在美国的分类中可以将其识别为吉普赛人。月球上的微流星体撞击形成的土壤,以及金星上的融化和玻璃化形成的土壤,都是真实存在的。
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