地质学
大陆地壳
结壳
大洋地壳
熔岩
地球化学
地幔(地质学)
稀土元素
原始地幔
Mercury(编程语言)
矿物学
部分熔融
火山
稀土
俯冲
古生物学
程序设计语言
构造学
计算机科学
作者
Frédéric Moynier,Matthew G. Jackson,Ke Zhang,Hongming Cai,Sæmundur A. Halldórsson,Raphaël Pik,James M.D. Day,Jiubin Chen
摘要
Abstract The element mercury (Hg) can develop large mass‐independent fractionation (MIF) (Δ 199 Hg) due to photo‐chemical reactions at Earth's surface. This results in globally negative Δ 199 Hg for terrestrial sub‐aerially‐derived materials and positive Δ 199 Hg for sub‐aqueously‐derived marine sediments. The mantle composition least affected by crustal recycling is estimated from high‐ 3 He/ 4 He lavas from Samoa and Iceland, providing an average of Δ 199 Hg = 0.00 ± 0.10, Δ 201 Hg = −0.02 ± 0.0.09, δ 202 Hg = −1.7 ± 1.2; 2SD, N = 11. By comparison, a HIMU‐type lava from Tubuai exhibits positive Δ 199 Hg, consistent with altered oceanic crust in its mantle source. A Samoan (EM2) lava has negative Δ 199 Hg reflecting incorporation of continental crust materials into its source. Three Pitcairn lavas exhibit positive Δ 199 Hg which correlate with 87 Sr/ 86 Sr, consistent with variable proportions of continental (low Δ 199 Hg and high 87 Sr/ 86 Sr) and oceanic (high Δ 199 Hg and low 87 Sr/ 86 Sr) crustal material in their mantle sources. These observations indicate that MIF signatures offer a powerful tool for examining atmosphere‐deep Earth interactions.
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