Skip to main content Accessibility help
×
Hostname: page-component-7bb8b95d7b-dtkg6 Total loading time: 0 Render date: 2024-09-12T19:21:02.216Z Has data issue: false hasContentIssue false

11 - Applications of radiogenic tracers

from Part III - ‘Where’: tracking the course of material through

Published online by Cambridge University Press:  05 June 2016

Bruce F. Schaefer
Affiliation:
Macquarie University, Sydney
Get access

Summary

The earth can be simply divided into several broad geochemical reservoirs. At the first order, the earth is composed of a metallic core, the convecting silicate earth (including the asthenosphere), and the lithosphere. The lithosphere comprises a crust and corresponding lithospheric mantle, which does not convect. Continental crust and subcontinental lithospheric mantle (SCLM) are quite heterogeneous and compositionally distinct compared with the oceanic crust and oceanic lithospheric mantle.

Since each reservoir is chemically distinct, they will evolve to correspondingly distinct isotopic ratios, potentially allowing the tracking of magmas and fluids from and between them. The relevance of this in the minerals industry can be varied, from requiring/desiring magmas sourced from the mantle for exploration models, or needing crustal contamination to drive sulphide saturation, through to monitoring the effects of fluids of differing compositions in a hydrothermal system.

Differentiation within the crust and crustal growth

Nd model ages (TDM) and crustal evolution

Nd isotopes offer an effective way of placing first-order constraints on processes pertaining to the formation and subsequent stabilisation and recycling of continental crustal material. In principle, when new continental crust is formed (e.g. on the modern earth at plate margins), the crustal material will start out with an isotopic signature in equilibrium with the depleted mantle (DMM) from which it was derived (Figure 11.1a). However, because continental crustal material contains relatively low Sm/Nd ratios with respect to the mantle, this new material will only ingrow new (additional) 143Nd relatively slowly. Hence it will evolve to negative εNd values (Figure 11.1a), and if unmodified will preserve a TDM which is the same as its magmatic age. Hence we would be able to measure its Nd isotopic signature today and calculate a TDM which would reflect precisely the age of formation of that portion of the continental crust, and hence constrain the time of that particular episode of crustal addition.

However, more generally, the continental crust undergoes processes of continued internal differentiation. For example, remelting of this crust during orogenesis or granite formation will segregate crustal material into a more differentiated granitic component, with even lower Sm/Nd (∝ 147Sm/144Nd) ratios, and a (relatively) more mafic residue with higher Sm/Nd ratios than the protolith. Over time these two products will evolve to distinctly different measured values today (Figure 11.1b).

Type
Chapter
Information
Radiogenic Isotope Geochemistry
A Guide for Industry Professionals
, pp. 145 - 176
Publisher: Cambridge University Press
Print publication year: 2016

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Armit, R.J., Betts, P.G., Schaefer, B.F., Pankhurst, M.J. and Giles, D. 2014. Provenance of the Early Mesoproterozoic Radium Creek Group in the northern Mount Painter Inlier: correlating isotopic signatures to inform tectonic reconstructions. Precambrian Research 243: 63–87.CrossRefGoogle Scholar
Belousouva, E.A., Reid, A.J., Griffin, W.L. and O‧Reilly, S.Y. 2009. Rejuvenation vs. recycling of Archean crust in the Gawler Craton, South Australia: evidence from U–Pb and Hf isotopes in detrital zircon. Lithos, 113(3–4): 570–582.Google Scholar
Cummin, V.M., Selby, D., Lillis, P.G. and Lewan, M.D. 2014. Re–Os geochronology and Os isotope fingerprinting of petroleum sourced from a Type I lacustrine kerogen: insights from the natural Green River petroleum system in the Uinta Basin and hydrous pyrolysis experiments. Geochimica et Cosmochimica Acta 138: 32–56.Google Scholar
DePaolo, D.J. 1983. The mean life of continents: estimates of continent recycling rates from Nd and Hf isotopic data and implications for mantle structure. Geophysical Research Letters 90: 263–271.Google Scholar
Hart, S.R. 1984. A large-scale isotopic anomaly in the Southern Hemisphere mantle. Nature 309: 753–757.CrossRefGoogle Scholar
Hofmann, A.W. 1997. Mantle geochemistry: the message from oceanic volcanism. Nature 385: 219–229.CrossRefGoogle Scholar
Jackson, S.E., Pearson, N.J., Griffin, W.L. and Belousova, E.A. 2004. The application of laser ablation-inductively coupled plasma-mass spectrometry to in situ U–Pb zircon geochronology. Chemical Geology 211(1): 47–69.CrossRefGoogle Scholar
Ravizza, G. and Turekian, K.K. 1989. Application of the 187Re–187Os system to black shale geochronometry. Geochimica et Cosmochimica Acta 53(12): 3257–3262.CrossRefGoogle Scholar
Selby, D. and Creaser, R.A. 2003. Re–Os geochronology of organic rich sediments: an evaluation of organic matter analysis methods. Chemical Geology 200(3–4): 225–240.CrossRefGoogle Scholar
Selby, D., Creaser, R.A. and Fowler, M.G. 2007. Re–Os elemental and isotopic systematics in crude oils. Geochimica et Cosmochimica Acta 71(2): 378–386.CrossRefGoogle Scholar
Sircombe, K.N. and Hazelton, M.L. 2004. Comparison of detrital age data by kernel functional estimation. Sedimentary Geology 171(1–4): 91–111.CrossRefGoogle Scholar
Stracke, A., Hofmann, A.W. and Hart, S.R. 2005. FOZO, HIMU, and the rest of the mantle zoo. Geochemistry, Geophysics, Geosystems 6(5): 1–20.CrossRefGoogle Scholar
Sun, S.S. and McDonough, W.F. 1989. Chemical and isotopic systematics of oceanic basalts: implications for mantle composition and processes. Geological Society of London, Special Publications 42: 313–345.CrossRefGoogle Scholar
Vermeesch, P. 2004. How many grains are needed for a provenance study?Earth and Planetary Science Letters 224(3–4): 441–451.CrossRefGoogle Scholar
Vermeesch, P. 2012. On the visualisation of detrital age distributions. Chemical Geology 312–313: 190–194.Google Scholar
Woodhead, J., Hergt, J., Shelley, M., Eggins, S. and Kemp, R. 2004. Zircon Hf-isotope analysis with an excimer laser, depth profiling, ablation of complex geometries, and concomitant age estimation. Chemical Geology 209(1–2): 121–135.CrossRefGoogle Scholar
Zindler, A. and Hart, S. 1986. Chemical geodynamics. Annual Reviews in Earth and Planetary Sciences 14: 493–571CrossRefGoogle Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×