The Formation and Evolution of Cratonic Mantle Lithosphere – Evidence from Mantle Xenoliths

2014 ◽  
pp. 255-292 ◽  
Author(s):  
D.G. Pearson ◽  
N. Wittig
2020 ◽  
Author(s):  
Sergei Lebedev ◽  
Nicolas Luca Celli ◽  
Andrew J. Schaeffer

<p>Waveform inversion was introduced in global seismic imaging in the early days of seismic tomography, in the beginning of the 1980s. Thanks to the continual improvements in the data sampling and methodology since then, waveform tomography has been getting more and more effective in extracting structural information from seismic records and producing detailed 3D models of the Earth’s crust and upper mantle. Today, tomography’s original problems relating to the large-scale Earth structure have been solved: the structure at the scale of thousands of kilometres is remarkably consistent across recent global models. Resolution of the imaging is now at hundreds of kilometres, the scale of tectonic units and major tectonic and magmatic processes. This has opened a new chapter for waveform tomography. It now fuels discoveries on the structure of individual cratons, evolution of cratons in general, origins of intraplate volcanism, plume-lithosphere interactions and other processes.   </p><p>In continents, high-resolution tomography can now map the deep boundaries of different tectonic blocks with useful accuracy.  A global comparison with geological data shows that, as a rule, Archean crust is underlain by thick (180-250 km), cratonic mantle lithosphere. This mantle lithosphere is likely to be of the Archean age as well, as often evidenced by mantle xenoliths. Where Archean crust is unexposed (covered by sediments), its presence can be inferred from the presence of the cratonic mantle lithosphere, imaged by tomography. A growing number of previously unknown cratons in different continents are now being discovered by waveform tomography. The lateral extent of other cratons, hypothesized previously, can now be established.</p><p>The lithosphere of most known cratons has been remarkably stable since its Archean formation, thanks to its compositional buoyancy and mechanical strength. In some instances, however, cratonic lithosphere is known to have been eroded. This is inferred from the existence of the thick lithosphere in the past, as evidenced by diamondiferous kimberlites, and its absence at present, as evidenced by  seismic imaging. Waveform tomography of continents now reveals more and more occurrences of this process and offers new insights into its mechanisms.</p><p>References</p><p>Celli, N.L., S. Lebedev, A.J. Schaeffer, C. Gaina. African cratonic lithosphere carved by mantle plumes. Nature Communications, 11, 92, doi:10.1038/s41467-019-13871-2, 2020.</p><p>Schaeffer, A. J., S. Lebedev. Global heterogeneity of the lithosphere and underlying mantle: A seismological appraisal based on multimode surface-wave dispersion analysis, shear-velocity tomography, and tectonic regionalization. In: "The Earth's Heterogeneous Mantle," A. Khan and F. Deschamps (eds.), pp. 3–46, Springer Geophysics, doi:10.1007/978-3-319-15627-9_1, 2015.</p><p>Steinberger, B., E. Bredow, S. Lebedev, A. Schaeffer, T. H. Torsvik. Widespread volcanism in the Greenland-North Atlantic region explained by the Iceland plume. Nature Geoscience, 12, 61–68, doi:10.1038/s41561-018-0251-0, 2019.</p>


Minerals ◽  
2020 ◽  
Vol 10 (9) ◽  
pp. 831 ◽  
Author(s):  
Munjae Park ◽  
Youngwoo Kil ◽  
Haemyeong Jung

Knowledge of the formation and evolution of cratonic subcontinental lithospheric mantle is critical to our understanding of the processes responsible for continental development. Here, we report the deformation microstructures and lattice preferred orientations (LPOs) of olivine and pyroxenes alongside petrological data from spinel peridotite xenoliths beneath the Baekdusan volcano. We have used these datasets to constrain the evolution of deformation fabrics related to petrogenesis from the Baekdusan peridotites. Based on petrographic features and deformation microstructures, we have identified two textural categories for these peridotites: coarse- and fine-granular harzburgites (CG and FG Hzb). We found that mineral composition, equilibrium temperature, olivine LPO, stress, and extraction depth vary considerably with the texture. We suggest that the A-type olivine LPO in the CG Hzb may be related to the preexisting Archean cratonic mantle fabric (i.e., old frozen LPO) formed under high-temperature, low-stress, and dry conditions. Conversely, we suggest that the D-type olivine LPOs in the FG Hzb samples likely originated from later localized deformation events under low-temperature, high-stress, and dry conditions after a high degree of partial melting. Moreover, we consider the Baekdusan peridotite xenoliths to have been derived from a compositionally and texturally heterogeneous vertical mantle section beneath the Baekdusan volcano.


2021 ◽  
Author(s):  
Sergey Sablukov ◽  
Lyudmila Sablukova ◽  
Yury Stegnitsky

<p>Detail study kimberlites and mantle xenoliths from Nakyn field pipes has revealed their unusual, interesting and important mineralogical features. Absence of Megacrystic picroilmenites of is compensated by presence of large orange-red titanium pyropes of "megacryst" type, underlining the reduced character asthenospheric melts influences on the mantle lithosphere in Nakyn. Picroilmenite in Nakyn kimberlites present only in xenoliths eclogites, garnet peridotites and clinopyroxenites with directive structures attributed to zones of melt fluid interaction. The clinopyroxene composition referred to Cr-omfacite, c (instead of Cr-diopside) suggest the Na-Al oceanic spilitic metasomatism at subduction stage or later interaction of the mantle material with the subducted pelitic sediments which is in accord with the presence of Al-rich eclogites wide distribution of the wehrlitic associations may suggest carbonatitic metasomatism. Cr- diopsides occurred in the peridotites with primary magmatic textures.</p><p>Absence of picroilmenite megacrysts in Nakyn kimberlites is filled with presence of large orange-red titanious-pyropes of "megacryst" associations, underlining the reduced character astenospheric influences on the mantle substratum of area</p><p>Picroilmenites in Nakyn kimberlites are present only in xenoliths of eclogites, and garnet peridotites and clinopyroxenites with, directive structures related to the zones of the metasomatism or melt interaction. The picroilmenite compositions from these rock inclusions sharply differs from composition of picroilmenite typical "megacryst" associations the raised contents of the titanium and the lowest share hematite component. In the same types mantle rocks is unusual also the composition of clinopyroxene: omphacite, chrome-omphacite (but not chrome-diopside) suggesting the high activity of the Na-Al metasomatism probably related to the oceanic spilitic metasomatism. The important participation in their formation of subduction processes allows to assume the specific features of a structure, mineral composition and composition of minerals of these rock inclusions.</p><p>Th ALCREMITE and MARID associations probably refer to the interaction of the lamprophyric Al2O3, H2O rich melts with peridotites or interaction of mica bearing Al, alkali rich sediments with peridotites. . The Botuobinskaya and Mayskaya kimberlite pipes contain essential amount of color a green garnets of different shades and compositions, that are very rare in worldwide kimberlites. It specifies on intensive influence of processes "calcium" (“chrome-calcium” and the “titanium–chrome-calcium”) metasomatism in mantle lithosphere</p><p><img src="https://contentmanager.copernicus.org/fileStorageProxy.php?f=gepj.c78cc1a3fdff57948740161/sdaolpUECMynit/12UGE&app=m&a=0&c=3c81a036683b53d2fa801210cd6674a4&ct=x&pn=gepj.elif&d=1" alt=""></p><p><img src="https://contentmanager.copernicus.org/fileStorageProxy.php?f=gepj.041a7fb3fdff57258740161/sdaolpUECMynit/12UGE&app=m&a=0&c=e223b463964dafd811fdb9bcf1d1cf94&ct=x&pn=gepj.elif&d=1" alt=""></p><p><img src="https://contentmanager.copernicus.org/fileStorageProxy.php?f=gepj.573044e3fdff54658740161/sdaolpUECMynit/12UGE&app=m&a=0&c=15da5e6bc74fe792450dfb38d30b4f5e&ct=x&pn=gepj.elif&d=1" alt=""></p>


2011 ◽  
Vol 305 (1-2) ◽  
pp. 235-248 ◽  
Author(s):  
Sebastian Tappe ◽  
D. Graham Pearson ◽  
Geoff Nowell ◽  
Troels Nielsen ◽  
Phil Milstead ◽  
...  

Geology ◽  
2020 ◽  
Vol 48 (7) ◽  
pp. 733-736 ◽  
Author(s):  
Weikai Li ◽  
Zhiming Yang ◽  
Massimo Chiaradia ◽  
Yong Lai ◽  
Chao Yu ◽  
...  

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.


2011 ◽  
Vol 3 (Special Issue) ◽  
pp. 1-7
Author(s):  
I. V. Ashchepkov ◽  
D. A. Ionov ◽  
T. Ntaflos ◽  
H. Downes ◽  
P. V. Afanasieva

2020 ◽  
Author(s):  
Sonja Aulbach ◽  
A-Bing Lin ◽  
Yaakov Weiss ◽  
Gregory Yaxley

<p>Continental rifting has been linked to the thinning and destruction of cratonic lithospheres and to the release of enough CO<sub>2</sub> to impact the global climate [1]. This fundamental plate tectonic process facilitates the infiltration and/or mobilisation of small-volume carbonated melts, which interact with mantle peridotite to form wehrlite through the reaction: enstatite + CO<sub>3</sub><sup>2- </sup>(melt) = forsterite + diopside + CO<sub>2</sub> (vapour) [2]. An analysis of the literature reveals that wehrlites are common in shallow mantle lithosphere in disrupted craton settings affected by either extension or subduction, and they have been linked to agents ranging from carbonatites to basanites [e.g. 3,4]. Conversely, the low abundance of wehrlitic diamond and garnet in cratonic mantle xenoliths (as opposed to lherzolitic or harzburgitic) indicate that wehrlitisation is not an important process at depths >~120 km. This may be due to the presence of a dominantly reducing lithosphere, which favours diamond precipitation or dissolution during reaction with carbonated silicate melts, depending on carbon saturation. Based on the relationship between wehrlite and small-volume carbonated melts, we suggest that wehrlite-bearing xenoliths can be used to monitor CO<sub>2</sub> mobility through the shallow continental lithosphere. Assuming a depleted protolith, typically harzburgite at shallow lithospheric depth, the amount of newly-added cpx can be estimated and related to CO<sub>2</sub> in the melt volume based on the above reaction. Considering the proportion of wehrlite in the xenolith population, an estimate of the total CO<sub>2</sub> transported out of the shallow lithosphere can be made. For example, peridotite xenoliths from Liaoyuan in the reactivated northeastern North China craton sample the mantle beneath the mid-Cretaceous Tan Lu Fault Belt (TLFB), which is even vaster in size (5000 x 800-1000 km) than the EAR, the latter linked to degassing of 28 to 34 Mt C/yr over 40 Ma [1]. If wehrlitisation affected only a 10 km depth interval over a similar time, 23 Mt C/yr has passed through the TLFB, possibly contributing to the mid-Cretaceous greenhouse climate. Thus, wehrlites reveal the hidden carbon cycle in lithospheric provinces where CO<sub>2</sub>-rich melts are not necessarily observed at the surface.</p><p> </p><p>[1] Foley and Fischer 2017 Nature Geosci 10; [2] Yaxley et al. 1998 J Petrol 39; [3] Aulbach et al. J Petrol 2017 58; [4] Lin et al. subm. J Geophys Res</p>


Sign in / Sign up

Export Citation Format

Share Document