A review of possible mechanisms for mercury migration in diagenesis: Clay to pyrite

被引:3
|
作者
Xu, Huan [1 ]
Ran, Bo [1 ]
Liu, Shugen [1 ]
Sun, Tong [1 ]
Luo, Chao [2 ]
Li, Yi [2 ]
Zhu, Yiqing [2 ]
机构
[1] Chengdu Univ Technol, State Key Lab Oil & Gas Reservoir Geol & Exploitat, Chengdu, Peoples R China
[2] Petrochina Southwest Oil & Gasfield Co, Chengdu, Peoples R China
基金
中国国家自然科学基金;
关键词
mercury; diagenesis; smectite; illite; framboidal pyrite; ATMOSPHERIC MERCURY; GASEOUS MERCURY; ORGANIC-MATTER; SEDIMENTS; SPECIATION; VOLCANISM; EXTINCTION; EMISSIONS; ISOTOPES; MINERALS;
D O I
10.3389/feart.2022.1011598
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Though sedimentary mercury in marine sediments has been regarded as a geological indicator of volcanic activity based on volcanism activity is the dominant natural source of Hg to the oceans, the influence of diagenesis on mercury cannot be dismissed. Marine mudstone has been selected to explore the migration of mercury from the syn-sedimentary stage to the diagenetic stage in this review. Marine mudstones undergo a series of significant transformation processes, including the illitization of smectite and the formation of framboidal pyrite aggregates during the diagenetic stage. This process makes the adsorption capacity of minerals change significantly that clay minerals are weakened, while pyrites are enhanced. In this reason, it is inferred that the sedimentary mercury may re-migrate from clay minerals to pyrite. This at least means that the indication of volcanic activity by mercury enrichment in marine mudstone need to be re-evaluated.
引用
收藏
页数:6
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