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大约20亿年前,月球上的火山活动激增
Heng-Ci Tian1, Chi Zhang2, Wei Yang3
1Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, 100029, Beijing, China. hctian@mail.iggcas.ac.cn.
Nature communications
|June 22, 2023
概括
这是一个变化,一个变化.
科学领域:
- 月球地质学和行星科学.
- 月球样本的地球化学和矿物学.
- 天体的热进化建模.天体的热进化建模.
背景情况:
- 了解月球海火山活动对于破译月球的热历史至关重要.
- 之前对月球年轻火山爆发的研究受到遥感和样本可用性的限制.
- 五号任务提供了访问已知最年轻的月球基岩的机会,提供了新的见解.
研究的目的:
- 分析来自长五基岩的奥利文和烯晶体的矿物学和地化学.
- 为了限制月球火山的火山爆发流和冷却时间表.
- 根据新的火山数据,修订月球热演变模型.
主要方法:
- 矿物学和地质化学研究42个橄烯和火烯晶体.
- 对晶体区分模式的分析,以推断岩充电和同化过程.
- 用热建模来估计五火山的厚度,体积和岩流量.
主要成果:
- 大多数分析的奥利文和烯晶体都表现出正常的区域划分,表明有限的岩充电或浅层同化.
- 橄素颗粒表明,采样的岩的冷却时间短.
- 热建模表明,大约20亿年前,岩流量增强.
结论:
- 晚期的月球火山喷发,虽然可能不频繁,但可以显示出显著的喷发流.
- 五基岩为修订的月球热演变模型提供了证据.
- 在月球的后期进化阶段,偶发性增强的岩活动发生.
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