Temporal variation in relative zircon abundance throughout Earth history

被引:37
|
作者
Keller, C. B. [1 ,2 ,3 ]
Boehnke, P. [4 ,5 ]
Schoene, B. [3 ]
机构
[1] Berkeley Geochronol Ctr, Berkeley, CA 94709 USA
[2] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
[3] Princeton Univ, Dept Geosci, Guyot Hall, Princeton, NJ 08544 USA
[4] Univ Chicago, Chicago Ctr Cosmochem, Chicago, IL 60637 USA
[5] Univ Chicago, Dept Geophys Sci, Chicago, IL 60637 USA
关键词
CONTINENTAL-CRUST; GROWTH; TEMPERATURE; CONSTRAINTS; EVOLUTION;
D O I
10.7185/geochemlet.1721
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Zircon is the preeminent chronometer of deep time on Earth, informing models of crustal growth and providing our only direct window into the Hadean Eon. However, the quantity of zircon crystallised per unit mass of magma is highly variable, complicating interpretation of the terrestrial zircon record. Here we combine zircon saturation simulations with a dataset of similar to 52,000 igneous whole rock geochemical analyses to quantify secular variation in relative zircon abundance throughout Earth history. We find dramatically increasing zircon abundance per mass of magma through geologic time, suggesting that the zircon record underestimates past crustal volume even if preservation bias is eliminated. Similarly, zircons were even less likely to crystallise from low-silica magmas in early Earth history than they are today, together suggesting that the observed Hadean zircon record may require a larger volume of generally felsic Hadean crust than previously expected.
引用
收藏
页码:179 / 189
页数:6
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