Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
Economic Geology Don't get GSW? Talk to your librarian.
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

Economic Geology; May 1995; v. 90; no. 3; p. 648-657
This Article
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Right arrow Order Hardcopy of Full Text via AGI/GeoRef
Citing Articles
Right arrow Citing Articles via HighWire
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Trumbull, R. B.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Tin mineralization in the Archean Sinceni rare element pegmatite field, Kaapvaal Craton, Swaziland

Robert B. Trumbull

Technische Universitaet Mu1.nchen, Lehrstuhl fuer Angewandte Mineralogie und Geochemie, Munich, Federal Republic of Germany

The Sinceni pegmatite field constitutes a large group of 3.0 Ga granitic pegmatites in the exocontact of the Sinceni pluton in south-central Swaziland. Field relations, age dating, and geochemical evidence indicate a genetic relationship between the pegmatites and the Sinceni pluton. The Sinceni pegmatites are moderately fractionated granitic pegmatites belonging to the beryl type of the rare element class. The pegmatite field is compositionally zoned, with the highest fractionation and strongest mineralization in a restricted area referred to as Sinceni West. Only the alluvial and eluvial tin concentrations are of economic interest, and the largest of these is the Sinceni West deposit. Primary tin mineralization at the Sinceni West deposit consists of cassiterite in late-stage pegmatite units of sugary albite, associated with mica-tourmaline metasomatic selvages in the host rock. The albitic units are interpreted as the products of late residual melt, and the metasomatic selvages reflect fluid exsolution from the melt at the latest stage of pegmatite consolidation. Several factors contributed to the development of primary tin mineralization in the Sinceni West area. First, the pegmatites in this area are the most highly fractionated, as shown by Ta, Rb, and Cs concentrations in blocky K feldspar. Second, the richest mineralization occurs in pegmatites that lack tourmaline, whereas tourmaline is abundant in the barren pegmatites. A lack of tourmaline allows the buildup of boron in residual melts, which promotes extended fractionation by increasing water solubility and depressing the solidus temperature. Third, the best tin values occur in pegmatites that exhibit boudinage and other signs of ductile deformation caused by an adjacent shear zone. Microstructures show that at least some cassiterite predates the deformation and that the albitic units and wall-rock alteration are synkinematic. The ductile deformation may have influenced the distribution of residual melt and its interaction with preexisting pegmatite and wall rocks, but it was probably of minor importance for the mineralization itself.

This record provided courtesy of AGI/GeoRef.




This article has been cited by other articles:


Home page
Can MineralHome page
P. Alfonso, J. C. Melgarejo, I. Yusta, and F. Velasco
GEOCHEMISTRY OF FELDSPARS AND MUSCOVITE IN GRANITIC PEGMATITE FROM THE CAP DE CREUS FIELD, CATALONIA, SPAIN
Can Mineral, February 1, 2003; 41(1): 103 - 116.
[Abstract] [Full Text] [PDF]


Home page
Mineral MagHome page
M. Belkasmi, M. Cuney, P. J. Pollard, and A. Bastoul
Chemistry of the Ta-Nb-Sn-W oxide minerals from the Yichun rare metal granite (SE China): genetic implications and comparison with Moroccan and French Hercynian examples
Mineralogical Magazine, June 1, 2000; 64(3): 507 - 523.
[Abstract] [Full Text] [PDF]




JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2008 by Society of Economic Geologists