Simon Chenery

Dr. Simon Chenery

British Geological Survey (BGS), Keyworth, Nottingham, UK
orcid

Research Focus & Metrics

Academic Career Length

39Years (1988-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 June 1997 in Geostandards Newsletter
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Journal Article
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NPNick Pearce
Nick Pearce
WPWilliam T. Perkins
William T. Perkins
JWJohn A. Westgate
John A. Westgate
MGMichael P. Gorton
Michael P. Gorton
SJSimon E. Jackson
Simon E. Jackson
SCSimon Chenery
Simon Chenery

1 October 2000 in Geochimica et Cosmochimica Acta
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Journal Article
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FPFranck Poitrasson
Franck Poitrasson
SCSimon Chenery
Simon Chenery
TSThomas J Shepherd
Thomas J Shepherd

1 December 1996 in Earth and Planetary Science Letters
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Journal Article
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FPFranck Poitrasson
Franck Poitrasson
SCSimon Chenery
Simon Chenery
DBDavid J. Bland
David J. Bland

1 September 2001 in Journal of Experimental Marine Biology and Ecology
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Journal Article
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DMDavid A Milton
David A Milton
SCSimon Chenery
Simon Chenery

1 August 2016 in Precambrian Research
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Journal Article
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RSRichard Shaw
Richard Shaw
KGKathryn Goodenough
Kathryn Goodenough
Nick RobertsNick Roberts
Nick Roberts
MHM.S.A. Horstwood
M.S.A. Horstwood
SCSimon Chenery
Simon Chenery
AGA.G. Gunn
A.G. Gunn
Many rare metals used today are derived from granitic pegmatites, but debate continues about the origin of these rocks. It is clear that some pegmatites represent the most highly fractionated products of a parental granite body, whilst others have formed by anatexis of local crust. However, the importance of these two processes in the formation of rare-metal pegmatites is not always evident.\ud \ud The Lewisian Gneiss Complex of NW Scotland comprises Archaean meta-igneous gneisses which were highly reworked during accretional and collisional events in the Palaeoproterozoic (Laxfordian orogeny). Crustal thickening and subsequent decompression led to melting and the formation of abundant granitic and pegmatitic sheets in many parts of the Lewisian Gneiss Complex. This paper presents new petrological, geochemical and age data for those pegmatites and shows that, whilst the majority are barren biotite-magnetite granitic pegmatites, a few muscovite-garnet (rare-metal) pegmatites are present. These are mainly intruded into a belt of Palaeoproterozoic metasedimentary and meta-igneous rocks known as the Harris Granulite Belt.\ud \ud The rare-metal pegmatites are distinct in their mineralogy, containing garnet and muscovite, with local tourmaline and a range of accessory minerals including columbite and tantalite. In contrast, the biotite-magnetite pegmatites have biotite and magnetite as their main mafic components. The rare-metal pegmatites are also distinguished by their bulk-rock and mineral chemistry, including a more peraluminous character and enrichments in Rb, Li, Cs, Be, Nb and Ta. New U-Pb ages (c. 1690–1710 Ma) suggest that these rare-metal pegmatites are within the age range of nearby biotite-magnetite pegmatites, indicating that similar genetic processes could have been responsible for their formation.\ud \ud The peraluminous nature of the rare-metal pegmatites strongly points towards a metasedimentary source. Notably, within the Lewisian Gneiss Complex, such pegmatites are only found in areas where a metasedimentary source is available. The evidence thus points towards all the Laxfordian pegmatites being formed by a process of crustal anatexis, with the formation of rare-metal pegmatites being largely controlled by source composition rather than solely by genetic process. This is in keeping with previous studies that have also challenged the widely accepted model that all rare-metal pegmatites are formed by fractionation from a parental granite, and raises questions about the origin of other mineralised pegmatites worldwide.\u

1 November 2004 in Earth and Planetary Science Letters
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Journal Article
Closed access
GFG. Foster
G. Foster
RPR.R. Parrish
R.R. Parrish
MHM.S.A. Horstwood
M.S.A. Horstwood
SCSimon Chenery
Simon Chenery
JPJ. Pyle
J. Pyle
HGH.D. Gibson
H.D. Gibson