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Volatile loss during homogenization of lunar melt inclusions

机译:月球融化夹杂物均质化期间的挥发性损失

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摘要

Volatile abundances in lunar mantle are critical factors to consider for constraining the model of Moon formation. Recently, the earlier understanding of a "dry" Moon has shifted to a fairly "wet" Moon due to the detection of measurable amount of H2O in lunar volcanic glass beads, mineral grains, and olivine-hosted melt inclusions. The ongoing debate on a "dry" or "wet" Moon requires further studies on lunar melt inclusions to obtain a broader understanding of volatile abundances in the lunar mantle. One important uncertainty for lunar melt inclusion studies, however, is whether the homogenization of melt inclusions would cause volatile loss. In this study, a series of homogenization experiments were conducted on olivine-hosted melt inclusions from the sample 74220 to evaluate the possible loss of volatiles during homogenization of lunar melt inclusions. Our results suggest that significant loss of H2O could occur even during minutes of homogenization, while F, Cl and S in the inclusions remain unaffected.
机译:月球地幔中的挥发性丰度是考虑约束月球形成模型的关键因素。最近,由于在月球火山玻璃珠,矿物质颗粒和橄榄石托管熔体夹杂物中检测到莫拉克玻璃珠粒的可测量量,对“干”月亮的早期了解了一个相当“湿”的月亮。关于“干”或“湿”月亮的持续争论需要进一步研究月球融化夹杂物,以便在月球地幔中获得更广泛的挥发性丰富。然而,月球融化研究的一个重要不确定性是熔体夹杂物的均质化是否会导致挥发性损失。在该研究中,在来自样品74220的橄榄石宿主宿主夹杂物上进行一系列均化实验,以评估月球熔体夹杂物均质期间挥发物的可能丧失。我们的研究结果表明,即使在均质化分钟内,也可能发生显着的H2O损失,而夹杂物中的F,Cl和S仍未受到影响。

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