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

The Canadian Mineralogist; April 2008; v. 46; no. 2; p. 379-393; DOI: 10.3749/canmin.46.2.379
© 2008 Mineralogical Association of Canada
This Article
Right arrow Résumé
Right arrow Figures Only
Right arrow Full Text
Right arrow Full Text (PDF)
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Right arrow Citation Map
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Download to citation manager
Right arrow reprints & permissions
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Galliski, M. A.
Right arrow Articles by Chapman, R.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Articles

THE Ta–Nb–Sn–Ti OXIDE-MINERAL PARAGENESIS FROM LA VIQUITA, A SPODUMENE-BEARING RARE-ELEMENT GRANITIC PEGMATITE, SAN LUIS, ARGENTINA

Miguel Angel Galliski1,§, Maria Florencia Marquez-Zavalía1, Petr Cerny2, Viviana Alejandra Martínez3 and Ron Chapman4

1 IANIGLA, CRICYT (CONICET), Avda. Ruiz Leal s/n, Parque Gral. San Martín; C.C.330 (5.500) Mendoza, Argentina
2 Department of Geological Sciences, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada
3 Departamento de Ciencias Geológicas, Universidad Nacional de La Pampa, Av. Uruguay 151, (6300) Santa Rosa, La Pampa, Argentina
4 Department of Geological Sciences, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada

§ E-mail address: galliski{at}lab.cricyt.edu.ar

The paragenesis and chemical composition of the primary Ta–Nb–Sn–Ti oxide minerals in the La Viquita spodumene-bearing granitic pegmatite, San Luis, Sierras Pampeanas, Argentina, evolved from the border zone inward. Early phases consist of minor columbite-(Fe) in the border and wall zones. In the intermediate zones, formed by a coarse-grained association of Kfs + Qtz + Ms + Ab with inwardly increasing proportions of spodumene, homogeneous or oscillatory-zoned columbite-(Fe) crystals occur in the outer parts. They show a fractionation trend to tantalite-(Fe) with Ta/(Ta + Nb) ranging from 0.35 to 0.56 at an almost constant Mn/(Mn + Fe2+ + Fe3+) of ~0.33, and locally to rare columbite-(Mn). In the middle and inner intermediate zones, the dominant phases are cassiterite, wodginite with elevated Zr contents and ferrowodginite. All members of the wodginite group are structurally ordered and carry some signs of exsolution-induced lamellae of ferrotapiolite. Ferrotapiolite is dominant in small Ms + Ab + Qtz units of the core-margin association, with intergrowths of ferrotitanowodginite, inclusions of hafnian zircon, and late-stage cassiterite. From the wall zone to the core-margin assemblage, the suite of Ta–Nb–Sn–Ti minerals shows a fractionation path with a non-linear increase in Ta/(Ta + Nb), basically in three stages marked by sequential dominance of columbite-group minerals, wodginite-group minerals and ferrotapiolite + cassiterite. The phase changes and compositional variations are attributed mainly to the combined effects of increasing proportion of Sn, Fe and Ti (the latter two possibly introduced from the host rocks), and of increasing f(O2) in the melt.

Keywords: wodginite-group minerals, columbite-group minerals, ferrotapiolite, cassiterite, granitic pegmatite, San Luis, Argentina.







JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS
Copyright © 2008 by Mineralogical Association of Canada