Cookies

We use cookies to ensure that we give you the best experience on our website. You can change your cookie settings at any time. Otherwise, we'll assume you're OK to continue.

Durham University

Research & business

View Profile

Publication details

Niu, Yaoling & O'Hara, M.J. (2009). MORB mantle hosts the missing Eu (Sr, Nb, Ta and Ti) in the continental crust: New perspectives on crustal growth, crust-mantle differentiation and chemical structure of oceanic upper mantle. Lithos 112(1-2): 1-17.

Author(s) from Durham

Abstract

We have examined the high quality data of 306 mid-ocean ridge basalt (MORB) glass samples from the East
Pacific Rise (EPR), near-EPR seamounts, Pacific Antarctic Ridge (PAR), near-PAR seamounts, Mid-Atlantic Ridge
(MAR), and near-MAR seamounts. The data show a correlated variation between Eu/Eu. and Sr/Sr., and both
decrease with decreasing MgO, pointing to the effect of plagioclase crystallization. The observation that
samples with MgON9.5 wt.% (before plagioclase on the liquidus) show Eu/Eu.N1 and Sr/Sr.N1 and that none
of the major phases (i.e., olivine, orthopyroxene, clinopyroxene, spinel and garnet) in the sub-ridge mantle
melting region can effectively fractionate Eu and Sr from otherwise similarly incompatible elements indicates
that the depleted MORB mantle (DMM) possesses excess Sr and Eu, i.e., [Sr/Sr.]DMMN1 and [Eu/Eu.]DMMN1.
Furthermore, the well-established observation that DNb≈DTh, DTa≈DU and DTi≈DSm during MORB mantle
melting, yet primitive MORB melts all have [Nb/Th]PM
MORBN1, [Ta/U]PM
MORBN1 and [Ti/Sm]PM
MORBN1 (where PM
indicates primitivemantle normalized), also points to the presence of excess Nb, Ta and Ti in the DMM, i.e., [Nb/
Th]PM
DMMN1, [Ta/U]PM
DMMN1 and [Ti/Sm]PM
DMMN1. The excesses of Eu, Sr, Nb, Ta and Ti in the DMM complement the
well-known deficiencies of these elements in the bulk continental crust (BCC). These new observations, which
support the notion that the DMM and BCC are complementary in terms of the overall abundances of
incompatible elements, offer new insights into the crust–mantle differentiation. These observations are best
explained by partial melting of amphibolite of MORB protolith during continental collision, which produces
andesitic melts with a remarkable compositional (major and trace element abundances as well as key
elemental ratios) similarity to the BCC, as revealed by andesites in southern Tibet produced during the India–
Asia continental collision. An average amphibolite of MORB protolith consists of ~66.4% amphibole, ~29.2%
plagioclase and 4.4% ilmenite. In terms of simple modal melting models, the bulk distribution coefficient ratios
D2Eu/(Sm + Gd)=1.21, D2Sr/(Pr + Nd)=1.04, DNb/Th=44, DTa/U=57, DTi/Sm=3.39 and DNb/Ta=1.30 readily explains the
small but significant negative Eu and Sr anomalies, moderate negative Ti anomaly and huge negative Nb and Ta
anomalies as well as the more sub-chondritic Nb/Ta ratio in the syncollisional andesitic melt that is
characteristic of and contributes to the continental crust mass. These results support the hypothesis that
continental collision zones are primary sites of net continental crust growth, whereas the standard “island arc”
model has many more difficulties than certainties. That is, it is the continental collision (vs. "island arc
magmatism" or "episodic super mantle avalanche events") that produces and preserves the juvenile crust, and
hence maintains net continental growth. The data also allow us to establish the robust composition of depleted
and most primitive (or “primary”) MORB melt with 13% MgO. This, together with the estimated positive Eu and
Sr anomalies in the DMM, further permits estimation that theDMMmay occupy the uppermost ~680 km of the
convective mantle following the tradition that the DMM lies in the shallowest mantle. However, the tradition
may be in error. The seismic low velocity zone (LVZ) may be compositionally stratified with small melt fractions
concentrated towards the interface with the growing lithosphere because of buoyancy. Such small melt
fractions, enriched in volatiles and incompatible elements, continue to metasomatize the growing lithosphere
before it reaches the full thickness after ~70 Myrs. Hence, the oceanic mantle lithosphere is a huge enriched
geochemical reservoir. On the other hand, deep portions of the LVZ, which are thus relatively depleted, become
the primary source feeding the ridge because of ridge-suction-driven lateral material supply to form the crust
and much of the lithosphere at and in the vicinity of the ridge.