Title of article
Stagnant-lid tectonics in early Earth revealed by 142Nd variations in late Archean rocks
Author/Authors
Debaille، نويسنده , , Vinciane and OʹNeill، نويسنده , , Craig and Brandon، نويسنده , , Alan D. and Haenecour، نويسنده , , Pierre and Yin، نويسنده , , Qing-Zhu and Mattielli، نويسنده , , Nadine and Treiman، نويسنده , , Allan H.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2013
Pages
10
From page
83
To page
92
Abstract
A major change in Earthʹs geodynamics occurred ~3 billion years (Ga) ago, likely related to the onset of modern and continuous plate tectonics. However, the question of how Earth functioned prior to this time is poorly constrained. Here, we find a resolvable positive 142Nd anomaly in a 2.7 Ga old tholeiitic lava flow from the Abitibi Greenstone Belt indicating that early-formed mantle heterogeneities persisted at least 1.8 Ga after Earthʹs formation. This result contradicts the expected rapid early (~0.1 Ga), as well as the slower present-day (~1 Ga) mixing rates in the convecting mantle. Using a numerical modeling approach, we show that convective mixing is inefficient in absence of mobile-lid plate tectonics. The preservation of a 142Nd anomaly until 2.7 Ga ago can be explained if throughout the Hadean and Archean, Earth was characterized by a stagnant-lid regime, possibly with sporadic and short subduction episodes. The major change in geodynamics observed around ~3 Ga ago can then reflect the transition from stagnant-lid plate tectonics to modern mobile-lid plate tectonics. Solving the paradox of a convective but poorly-mixed mantle has implications not only for Archean Earth, but also for other planets in the solar system such as Mars.
Keywords
Archean , plate tectonics , stagnant-lid regime , Convective mixing , Mars , 142Nd
Journal title
Earth and Planetary Science Letters
Serial Year
2013
Journal title
Earth and Planetary Science Letters
Record number
2331788
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