Open AccessOrigin of geochemical mantle components: Role of spreading ridges and thermal evolution of mantle
Author(s) -
Kimura JunIchi,
Gill James B.,
van Keken Peter E.,
Kawabata Hiroshi,
Skora Susanne
Publication year - 2017
Publication title -
geochemistry, geophysics, geosystems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.928
H-Index - 136
ISSN - 1525-2027
DOI - 10.1002/2016gc006696
Subject(s) - mantle (geology) , geology , planetary differentiation , mantle convection , transition zone , mantle wedge , earth's internal heat budget , crustal recycling , geochemistry , peridotite , subduction , hotspot (geology) , primitive mantle , adakite , basalt , oceanic crust , continental crust , geophysics , partial melting , paleontology , tectonics
We explore the element redistribution at mid‐ocean ridges (MOR) using a numerical model to evaluate the role of decompression melting of the mantle in Earth's geochemical cycle, with focus on the formation of the depleted mantle component. Our model uses a trace element mass balance based on an internally consistent thermodynamic‐petrologic computation to explain the composition of MOR basalt (MORB) and residual peridotite. Model results for MORB‐like basalts from 3.5 to 0 Ga indicate a high mantle potential temperature ( T p ) of 1650–1500°C during 3.5–1.5 Ga before decreasing gradually to ∼1300°C today. The source mantle composition changed from primitive (PM) to depleted as T p decreased, but this source mantle is variable with an early depleted reservoir (EDR) mantle periodically present. We examine a two‐stage Sr‐Nd‐Hf‐Pb isotopic evolution of mantle residues from melting of PM or EDR at MORs. At high‐ T p (3.5–1.5 Ga), the MOR process formed extremely depleted DMM. This coincided with formation of the majority of the continental crust, the subcontinental lithospheric mantle, and the enriched mantle components formed at subduction zones and now found in OIB. During cooler mantle conditions (1.5–0 Ga), the MOR process formed most of the modern ocean basin DMM. Changes in the mode of mantle convection from vigorous deep mantle recharge before ∼1.5 Ga to less vigorous afterward is suggested to explain the thermochemical mantle evolution.