『Abstract
We report new estimates of abundances of rarely analyzed elements
(As, B, Be, Bi, Cd, Ge, In, Mo, Sb, Sn, Te, Tl, W) in the upper
continental crust based on precise ICP-MS analyses of well-characterized
upper crustal samples (shales, pelites, loess, graywackes, granitoids
and their composites) from Australia, China, Europe, New Zealand
and North American. Obtaining a better understanding of the upper
crustal abundance and associated uncertainties of these elements
is important in placing better constraints on bulk crust composition
and, from that, whole Earth models of element cycling and crust
generation. We also present revised abundance estimates of some
more commonly analyzed trace elements (Li, Cr, Ni, and Tm) that
vary by >20% compared to previous estimates. The new estimates
are mainly based on significant (r2>0.6) inter-element
correlations observed in clastic sediments and sedimentary rocks,
which yield upper continental crust elemental ratios that are
used in conjunction with well-determined abundances for certain
key elements to place constraints on the concentrations of the
rarely analyzed elements. Using the well-established upper crustal
abundances of La (31 ppm), Th (10.5 ppm), Al2O3 (15.40%), K2O (2.80%) and
Fe2O3 (5.92%), these
ratios led to revised upper crustal abundances of B=47 ppm, Bi=0.23
ppm, Cr=73 ppm, Li=41 ppm, Ni=34 ppm, Sb=0.075, Te=0.027 ppm,
Tl=0.53 ppm and W=1.4 ppm. No significant correlations exist between
Mo and Cd and other elements in the clastic sediments and sedimentary
rocks, probably due to their enrichment in organic carbon. We
thus calculate abundances of these elements by assuming the upper
continental crust consists of 65% granitoid rocks plus 35% clastic
sedimentary rocks. The validity of this approach is supported
by the similarity of SiO2, Al2O3, La and Th abundances calculated in this way
with their upper crustal abundances given in Rudnick and Gao [Rudnick,
R., Gao, S., 2003. Composition of the continental crust. In: Rudnick,R.L.
(Ed.), The Crust. In: Holland, H.D., Turekian, K.K. (Eds.), Treatise
on Geochemistry, vol. 3, Elsevier-Pergamon, Oxford, pp. 1-64].
The upper crustal abundances thus obtained are Mo=0.6 ppm and
Cd=0.06 ppm. Our data also suggest a 〜20% increase of the Tm,
Yb and Lu abundances reported in Rudnick and Gao [Rudnick, R.,
Gao, S., 2003. Composition of the continental crust. In: Rudnick,
R.L. (Ed.), The Crust. In: Holland, H.D., Turekian, K.K. (Eds.),
Treatise on Geochemistry, vol. 3, Elsevier-Pergamon, Oxford, pp.
1-64.
Keywords: Geochemistry; Composition of the upper continental crust;
Trace elements』
1. Introduction
2. Samples of the upper continental crust
3. Analytical methods
3.1. Instrumentation
3.2. Reagents
3.3. Sample digestion
3.4. Accuracy and precision
4. Discussion
4.1. Nb, Ta, Zr and Hf
4.2. Ga and In
4.3. Sn
4.4. Rb and Cs
4.5. Tl
4.6. Be
4.7. Ge and W
4.8. Bi
4.9. U
4.10 Transition metals Sc, Co, V, Cr, Ni, Cu and Zn
4.11 Li
4.12 B
4.13 Te
4.14 Sb and As
4.15 Mo and Cd
4.16 Heavy rare earth elements Er, Tm, Yb and Lu
5. Conclusions
Acknowledgments
Appendix A. Supplementary data
References
Element | 1 Shaw et al. (1967,1976) | 2 Eade and Fahrig (1973) | 3 Condie (1993) | 4 Gao et al. (1998) | 5 Sims et al. (1990) | 6 Plank and Langmuir (1998) | 7 Taylor and McLennan (1985,1995) | 8 McLennan (2001) | 9 Wedepohl (1995) | 10 Rudbick and Gao (2003) | 11 This study |
Li | 22 | 20 | 20 | (22) | 21 | 41 | |||||
Be | 1.3 | 1.95 | 3 | 3.1 | 2.1 | 1.9 | |||||
B | 9.2 | 28 | 15 | 17 | 17 | 47 | |||||
Sc | 7 | 12 | 13.5 | 15 | 11 | 13.6 | (7) | 14.0 | 14 | ||
V | 53 | 59 | 86 | 98 | 60 | 107 | (53) | 97 | 106 | ||
Cr | 35 | 76 | 112 | 80 | 35 | 85 | (35) | 92 | 73 | ||
Co | 12 | 18 | 17 | 10 | 17 | (12) | 17.3 | 15 | |||
Ni | 19 | 19 | 60 | 38 | 20 | 44 | (19) | 47 | 34 | ||
Cu | 14 | 26 | 32 | 25 | (14) | 28 | 27 | ||||
Zn | 52 | 60 | 70 | 71 | (52) | 67 | 75 | ||||
Ga | 14 | 18 | 17 | (14) | 17.5 | 18.6 | |||||
Ge | 1.34 | 1.6 | 1.4 | 1.4 | 1.3 | ||||||
As | 4.4 | 5.1 | 1.5 | 2 | 4.8 | 5.7 | |||||
Rb | 110 | 85 | 83 | 82 | 112 | 110 | 84 | 94 | |||
Nb | 26 | 9.8 | 12 | 13.7 | 25 | 12 | (26) | 12 | 11.6 | ||
Mo | 0.78 | 1.2 | 1.5 | 1.4 | 1.1 | 0.6 | |||||
Cd | 0.075 | 0.079 | 0.098 | 0.102 | 0.09 | 0.06 | |||||
In | 0.05 | 0.061 | 0.056 | 0.066 | |||||||
Sn | 1.73 | 5.5 | 2.5 | 2.1 | 2.2 | ||||||
Sb | 0.3 | 0.45 | 0.2 | 0.31 | 0.4 | 0.75 | |||||
Te | 0.027 | ||||||||||
Cs | 3.55 | 7.3 | 3.7 | 4.6 | 5.8 | 4.9 | 4.9 | ||||
Er | 2.3 | 2.3 | 2.30 | ||||||||
Tm | 0.33 | 0.30 | 0.37 | ||||||||
Yb | 1.47 | 1.91 | 2.26 | 2.2 | (1.5) | 2.0 | 2.34 | ||||
Lu | 0.233 | 0.32 | 0.35 | 0.32 | (0.27) | 0.31 | 0.36 | ||||
Ta | 5.7 | 0.79 | 0.74 | 0.96 | 2.2 | 1.0 | 1.5 | 0.9 | 0.92 | ||
W | 0.91 | 3.3 | 2 | 1.4 | 1.9 | 1.4 | |||||
Tl | 0.524 | 1.55 | 0.75 | 0.75 | 0.9 | 0.55 | |||||
Bi | 0.035 | 0.23 | 0.13 | 0.123 | 0.16 | 0.23 | |||||
U | 2.45 | 1.5 | 2.2 | 1.55 | 2.8 | (2.5) | 2.7 | 2.6 | |||
Columns 1-4 represent averages of surface exposures. Columns 5-9 are estimates derived from fine-grain clastic sedimentary rocks and loess. Bracketed data in column 9 are values derived from Shaw et al. (1967,1976). |