کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
6429344 1634763 2014 10 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
A relatively reduced Hadean continental crust and implications for the early atmosphere and crustal rheology
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
A relatively reduced Hadean continental crust and implications for the early atmosphere and crustal rheology
چکیده انگلیسی


- The continental crust was much more reduced in the Hadean than in post-Hadean.
- A relatively reduced early crust due to late veneer in crustal production.
- Formation of CH4-rich fluids by degassing of reduced granitic melts in the Hadean.
- The atmosphere was probably reduced in the early Hadean.
- The Hadean crust was probably very weak allowing faster crustal growth.

It is widely believed that the Earth was strongly reduced during its early accretion, however, the transition from the reduced state that prevailed during Earth's early period to the modern oxidized crust and mantle has never been captured by geochemical surveys on Earth materials as old as ∼4.0 billion years ago. By combining available trace-elements data of igneous zircons of crustal origin, we show that the Hadean continental crust was significantly more reduced than its modern counterpart and experienced progressive oxidation till ∼3.6 billions years ago. We suggest that the increase in the oxidation state of the Hadean continental crust is related to the progressive decline in the intensity of chondritic addition during the late veneer. Inputs of carbon- and hydrogen-rich chondritic materials during the formation of Hadean granitic crust must have favored strongly reduced magmatism. The conjunction of cold, wet and reduced granitic magmatism during the Hadean implies the production of methane-rich fluids, in addition to the CO- and H2-rich volcanic species produced by degassing of hot reduced basaltic melts as modified by delivered materials during the late veneer. When the late veneer events ended, magma produced by normal decompression melting of the mantle imparted more oxidizing conditions to erupted lavas and the related crust, emitting CO2- and H2O-rich gases. Our model suggests that the Hadean continental crust was possibly much weaker than present-day, facilitating intrusion of underplating magma and thus allowing faster crustal growth in the early Earth.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 393, 1 May 2014, Pages 210-219
نویسندگان
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