硼
蒸发岩
地质学
过碱性岩
大陆地壳
地球化学
矿物
天体生物学
结壳
矿物学
化学
沉积岩
物理
火山
有机化学
出处
期刊:Elements
[Mineralogical Society of America]
日期:2017-08-01
卷期号:13 (4): 225-229
被引量:30
标识
DOI:10.2138/gselements.13.4.225
摘要
Boron is rare in the cosmos because its nucleus is “fragile.” So, how does one get from the interstellar medium, where boron was first produced, to Earth's upper continental crust where boron is concentrated in deposits containing remarkably diverse suites of boron minerals? Processes that led to the formation of continental crust also concentrated boron, which is preferentially incorporated into melts and aqueous fluids. Deposits with high boron-mineral diversity include granitic pegmatites, peralkaline intrusions, boron-enriched skarns, and evaporite deposits. Despite the loss of boron minerals from the geologic record due to their ready solubility in water and breakdown at low temperatures, the increase in boron-mineral diversity with time is real, and is accelerated during supercontinent assembly.
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