在玄武岩欧克里特的多态的相变的实验证据:对原行星地的热史的影响
Rei Kanemaru1, Naoya Imae2,3, Akira Yamaguchi2,3
1Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Kanagawa, 252-5210, Japan. Kanemaru.rei@jaxa.jp.
Scientific reports
|November 3, 2024
概括
尤克里特体中的单体三胺在重新加热时是稳定的,与石英和玻璃不同. 这挑战了cristobalite始终是eucritic magma中形成的第一个石阶段的假设.
科学领域:
- 行星科学 行星科学
- 矿物学是什么?矿物学是什么?
- 地质化学 地质化学
背景情况:
- 多态提供了洞察行星材料的变形历史.
- 了解玄武岩的状物中的二氧化行为对于解释它们的形成至关重要.
研究的目的:
- 研究在受控加热条件下,在玄武岩中形成和稳定多态的二氧化.
- 为了评估石英,三石和二氧化玻璃在eucrite样本中的变态反应.
主要方法:
- 异热加热实验是在基岩岩石样本中的二氧化多态体上进行的.
- 样品被加热到特定的温度,以观察再结晶和相变.
主要成果:
- 石英在≥1040°C时重新结晶成为克里斯托巴利特.
- 单临床三胺矿在高达1070°C的温度下保持稳定.
- 玻璃转化为石英 (900-1010°C) 或克里斯托巴莱特 (≥1040°C).
- 伪正三度矿在≥1070°C的温度下从化物中结晶.
结论:
- 在eucrites中在固体温度 (~1060°C) 以下的再加热事件中,单临床三聚是稳定的.
- 尤克里特岩中的初始石阶段可能并不总是克里斯托巴利特,因此需要重新评估石矿物形成过程.
- 这些发现挑战了以前关于eucrites中的二氧化阶段演变的假设.
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