Rare Earth Element Evidence Research Articles

The composition and evolution of the continental crust: rare earth element evidence from sedimentary rocks

The composition of the present-day upper crust, inferred from the uniformity of sedimentary rock r.e.e. (rare earth element) patterns, is close to that of granodiorite. A revised ‘andesite’ model is used to obtain total crustal composition. The lower crust is the composition remaining, assuming that the upper crust, one-third of the total, is derived from intracrustal partial melting. The upper-crustal r.e.e. pattern has pronounced Eu depletion (Eu/Eu* = 0.64), the lower-crustal pattern has Eu enrichment (Eu/Eu* = 1.17) and the total crust has no Eu anomaly relative to chondritic abundances. The Eu depletion in the upper crust is attributed to retention of Eu in plagioclase in the lower crust. Because plagioclase is not stable below 40 km (> 10 kbar), the anomaly is intracrustal in origin. The Archaean upper crust has a different r.e.e. pattern to that of the present-day upper crust, being lower in total r.e.e., and La/Yb ratios, and lacking an Eu anomaly. These data are used to infer the Archaean upper-crustal composition, which resembles that of the present-day total crust, except that Ni and Cr contents are higher. The Archaean crustal composition can be modelled by a mixture of tholeiites and tonalite trondhjemites. The latter have steep light r.e.e.-enriched-heavy r.e.e.-depleted patterns, consistent with equilibration with garnet and hence probable mantle derivation. There is little reason to suppose that the Archaean lower crust was different in composition from the upper crust, except locally where partial melting episodes occurred. The r.e.e. evidence is consistent with isotopic and geological evidence for a low continental growth rate in the early Archaean, a massive increase (to about 70% of the total crust) between about 3000 and 2500 Ma B.P. and a slow increase until the present day. The change from Archaean to post-Archaean r.e.e. patterns in the upper crust is not isochronous, but is reflected in the sedimentary rock r.e.e. patterns at differing times in different continents. On the basis of a model composition for the mantle, 36% of the potassium, 30% of uranium, 15% of lanthanum and 3 % of ytterbium are concentrated in the present continental crust. This enrichment is related to ionic size and valency differences from common mantle cations (e.g. Mg, Fe). Pre-3.9 Ga B.P. crusts were obliterated by meteorite bombardment. No geochemical evidence exists for primordial anorthositic, sialic or mafic crusts.

Rare earth evidence concerning the origin of granites of the Isle of Skye, northwest Scotland

Eleven samples of Skye granites, two samples of Torridonian sandstone and one sample of Lewisian gneiss have been analysed for ten rare earth elements (REE) by neutron activation analysis. The granites are representative of the main granite centres and compositional types. All granites have sub-parallel light-REE-enriched patterns with chondrite-normalised Ce (Ce N) = 78–263,Yb N = 16–60and Ce N/Yb N = 2.9–8.0 . REE patterns for the Lewisian gneiss and Torridonian sandstone are similar to each other, with Ce N = 32–61 , Yb N = 3–5and Ce N/Yb N = 8–18 . These two rock types as well as the Glamaig granite have negligible Eu anomalies (Eu/Eu* > 0.9), and the other granites have Eu/Eu* in the range 0.83-0.34. The REE evidence suggests that Lewisian gneiss or Torridonian sandstone are not suitable materials from which the granites could be derived by partial melting. The Western Red Hills granite intrusions show a systematic relation of REE content with Eu/Eu*. We suggest that the Glamaig granite is the most primitive, and was derived from a source with no Eu anomaly by fractional crystallization of a more basic magma. The later Western Red Hills granites might then have resulted from further fractional crystallization of magma with a composition like that of the Glamaig granite. The Coire Uaigneich and Eastern Red Hills granites may also be products of fractional crystallization, but from different magmas to those parental to the Western Red Hills granites. The basaltic parent magmas of the Skye granites may be “continental” tholeiites derived by interaction of basalt magma with Lewisian gneiss.

Rare earth element evidence for differentiation of McMurdo volcanics, Ross Island, Antarctica

Eighteen samples of the McMurdo volcanics on Ross Island, Antarctica consisting of basanitoid, trachybasalt and phonolite have been analyzed for rare earth elements (REE) in order to determine the details of differentiation using quantitative trace element modeling. The basanitoids have REE patterns similar to those for alkali basalts or nephelinites from ocean islands. Since there is no correlation between REE and silica contents among five basanitoids, some of the variability in the REE contents must be related to the extent of partial melting, variation in the residual mineralogies of the mantle during melting, or to inhomogeneities in the REE composition of the mantle.

Rare earth element geochemistry of potassic lavas from the Birunga and Toro-Ankole regions of Uganda, Africa

Neutron activation determination of La, Ce, Sm, Eu, Tb, Yb, Lu, Ta, Hf, Sc, Co and Th in potassic lavas from the Birunga and Toro-Ankole regions show that the rocks are characterized by high rare earth element (REE) contents (161–754 ppm) and form two groups based upon differing La/Yb ratios. One group is made up of katungite, ugandite and mafurite with La/Yb =146–312, and the other of rocks of the leucitite and phonolitic tephrite series, La/Yb =30–56. The trace element content of the ugandite group is similar to that of kimberlites. The data do not indicate any trends of differentiation or simple relationships between the two groups of rocks, although katungite is unlikely to be parental to rocks of lower La/Yb ratios. It is unlikely that in terms of La/Yb ratios that partial melting of mica-garnet-lherzolite mantle can form katungite because of the very small amounts of partial melting required (0.2%), although the La/Yb ratios of 150–200 (ugandites, mafurites) and 30–60 (leucitites, phonolitic tephrites) can be accounted for by 0.3–1.5% and 1–9% melting respectively, if the REE are then concentrated without further La and Yb fractionation. Partial melting of mantle which has been metasomatized by alkaline earths and REE bearing fluids or mixing of carbonatite and nephelenite are also compatable with the observed geochemistry of the lavas. It is considered that gas transfer processes which selectively enrich the light REE may have obscured REE evidence pertaining to early partial melting and/or differentiation processes and therefore that REE geochemistry is of little use in determining the petrogenetic processes involved in the formation of potassic lavas.