Geochemical/petrologic constraints on the origin of cratonic mantle

2006 ◽  
pp. 89-114 ◽  
Author(s):  
Cin-Ty Aeolus Lee
Keyword(s):  
Cratonic Mantle

scholarly journals Isopycnicity of cratonic mantle restricted to kimberlite provinces

2019 ◽  
Vol 505 ◽  
pp. 13-19 ◽  
Author(s):  
I.M. Artemieva ◽  
H. Thybo ◽  
Y. Cherepanova
Keyword(s):  
Cratonic Mantle

Formation of Siberian cratonic mantle websterites from high-Mg magmas

Lithos ◽  
2019 ◽  
Vol 326-327 ◽  
pp. 384-396 ◽  
Author(s):  
Dirk Spengler ◽  
Taisia A. Alifirova
Keyword(s):  
Cratonic Mantle

A fresh isotopic look at Greenland kimberlites: Cratonic mantle lithosphere imprint on deep source signal

2011 ◽  
Vol 305 (1-2) ◽  
pp. 235-248 ◽  
Author(s):  
Sebastian Tappe ◽  
D. Graham Pearson ◽  
Geoff Nowell ◽  
Troels Nielsen ◽  
Phil Milstead ◽  
...  
Keyword(s):  
Mantle Lithosphere ◽  
Source Signal ◽  
Cratonic Mantle ◽  
Deep Source

Numerical Insights into the Formation and Stability of Cratons

2021 ◽  
Author(s):  
Charitra Jain ◽  
Antoine Rozel ◽  
Emily Chin ◽  
Jeroen van Hunen
Keyword(s):  
Continental Crust ◽  
Seismic Velocity ◽  
Potential Temperature ◽  
Crustal Material ◽  
Spinel Lherzolite ◽  
Seismic Velocities ◽  
Geophysical Research ◽  
Thermal Buoyancy ◽  
Depleted Mantle ◽  
Cratonic Mantle

<div>Geophysical, geochemical, and geological investigations have attributed the stable behaviour of Earth's continents to the presence of strong and viscous cratons underlying the continental crust. The cratons are underlain by thick and cold mantle keels, which are composed of melt-depleted and low density peridotite residues [1]. Progressive melt extraction increases the magnesium number Mg# in the residual peridotite, thereby making the roots of cratons chemically buoyant [2, 3] and counteracting their negative thermal buoyancy. Recent global models have shown the production of Archean continental crust by two-step mantle differentiation, however this primordial crust gets recycled and no stable continents form [4]. This points to the missing ingredient of cratonic lithosphere in these models, which could act as a stable basement for the crustal material to accumulate on and may also help with the transition of global regime from "vertical tectonics'' to "horizontal tectonics''. Based on the bulk FeO and MgO content of the residual peridotites, it has been proposed that cratonic mantle formed by hot shallow melting with mantle potential temperature, which was higher by 200-300 °C than present-day [5]. We introduce Fe-Mg partitioning between mantle peridotite and melt to track the Mg# variation through melting, and parametrise craton formation using the corresponding P-T formation conditions. Using self-consistent global convection models, we show the dynamic formation of cratons as a result of naturally occurring lateral compression and thickening of the lithosphere, which has been suggested by geochemical and petrological data. To allow for the material to compact and thicken, but prevent it from collapsing under its own weight, a combination of lithospheric strength, plastic yielding, dehydration strengthening, and depletion-induced density reduction of the depleted mantle material is necessary.</div><div> </div><div> [1] Boyd, F. R. High-and low-temperature garnet peridotite xenoliths and their possible relation to the lithosphere- asthenosphere boundary beneath Africa. In Nixon, P. H. (ed.) <em>Mantle Xenolith</em>, 403–412 (John Wiley & Sons Ltd., 1987).</div><div>[2] Jordan, T. H. Mineralogies, densities and seismic velocities of garnet lherzolites and their geophysical implications. In <em>The Mantle Sample: Inclusion in Kimberlites and Other Volcanics</em>, 1–14 (American Geophysical Union, Washington, D. C., 1979).</div><div>[3] Schutt, D. L. & Lesher, C. E. Effects of melt depletion on the density and seismic velocity of garnet and spinel lherzolite. <em>Journal of Geophysical Research </em><strong>111</strong> (2006).</div><div>[4] Jain, C., Rozel, A. B., Tackley, P. J., Sanan, P. & Gerya, T. V. Growing primordial continental crust self-consistently in global mantle convection models. <em>Gondwana Research</em> <strong>73</strong>, 96–122 (2019).</div><div>[5] Lee, C.-T. A. & Chin, E. J. Calculating melting temperatures and pressures of peridotite protoliths: Implications for the origin of cratonic mantle. <em>Earth and Planetary Science Letters</em> <strong>403</strong>, 273–286 (2014)</div>

scholarly journals Redox state of southern Tibetan upper mantle and ultrapotassic magmas

Geology ◽  
2020 ◽  
Vol 48 (7) ◽  
pp. 733-736 ◽  
Author(s):  
Weikai Li ◽  
Zhiming Yang ◽  
Massimo Chiaradia ◽  
Yong Lai ◽  
Chao Yu ◽  
...  
Keyword(s):  
Upper Mantle ◽  
Lithospheric Mantle ◽  
Redox State ◽  
Volcanic Rocks ◽  
Mantle Xenoliths ◽  
Continental Plate ◽  
Cratonic Mantle ◽  
Tectonic Settings ◽  
Mantle Condition ◽  
Typical Range

Abstract The redox state of Earth’s upper mantle in several tectonic settings, such as cratonic mantle, oceanic mantle, and mantle wedges beneath magmatic arcs, has been well documented. In contrast, oxygen fugacity () data of upper mantle under orogens worldwide are rare, and the mechanism responsible for the mantle condition under orogens is not well constrained. In this study, we investigated the of mantle xenoliths derived from the southern Tibetan lithospheric mantle beneath the Himalayan orogen, and that of postcollisional ultrapotassic volcanic rocks hosting the xenoliths. The of mantle xenoliths ranges from ΔFMQ = +0.5 to +1.2 (where ΔFMQ is the deviation of log from the fayalite-magnetite-quartz buffer), indicating that the southern Tibetan lithospheric mantle is more oxidized than cratonic and oceanic mantle, and it falls within the typical range of mantle wedge values. Mineralogical evidence suggests that water-rich fluids and sediment melts liberated from both the subducting Neo-Tethyan oceanic slab and perhaps the Indian continental plate could have oxidized the southern Tibetan lithospheric mantle. The conditions of ultrapotassic magmas show a shift toward more oxidized conditions during ascent (from ΔFMQ = +0.8 to +3.0). Crustal evolution processes (e.g., fractionation) could influence magmatic , and thus the redox state of mantle-derived magma may not simply represent its mantle source.

scholarly journals Highly depleted cratonic mantle in West Greenland extending into diamond stability field in the Proterozoic

Lithos ◽  
2013 ◽  
Vol 168-169 ◽  
pp. 160-172 ◽  
Author(s):  
Stefan Bernstein ◽  
Kristoffer Szilas ◽  
Peter B. Kelemen
Keyword(s):  
Stability Field ◽  
West Greenland ◽  
Cratonic Mantle

scholarly journals Volatile-rich Metasomatism in the Cratonic Mantle beneath SW Greenland: Link to Kimberlites and Mid-lithospheric Discontinuities

2017 ◽  
Vol 58 (12) ◽  
pp. 2311-2338 ◽  
Author(s):  
Sonja Aulbach ◽  
Jing Sun ◽  
Sebastian Tappe ◽  
Heidi E Höfer ◽  
Axel Gerdes
Keyword(s):  
Cratonic Mantle

Thermochemical lithosphere differentiation and the origin of cratonic mantle

Nature ◽  
2020 ◽  
Vol 588 (7836) ◽  
pp. 89-94
Author(s):  
Fabio A. Capitanio ◽  
Oliver Nebel ◽  
Peter A. Cawood
Keyword(s):  
Cratonic Mantle
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