Journal of Petrology Advance Access originally published online on November 24, 2004
Journal of Petrology 2005 46(3):441-472; doi:10.1093/petrology/egh083
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Occurrence and Origin of Andalusite in Peraluminous Felsic Igneous Rocks
1 DEPARTMENT OF EARTH SCIENCES, DALHOUSIE UNIVERSITY, HALIFAX, NS, CANADA B3H 3J5
2 DEPARTMENT OF GEOLOGY, BRIGHAM YOUNG UNIVERSITY, PROVO, UT 84602, USA
3 LABORATOIRE MAGMAS ET VOLCANS, UNIVERSITÉ BLAISE PASCAL, 5 RUE KESSLER, F63038 CLERMONT-FERRAND CEDEX, FRANCE
4 DEPARTMENT OF GEOLOGICAL SCIENCES, UNIVERSITY OF TEXAS, AUSTIN, TX 78712, USA
5 DIPARTIMENTO DI MINERALOGIA E PETROLOGIA, UNIVERSITÁ DI PADOVA, I-35137 PADOVA, ITALY
6 SCHOOL OF GEOSCIENCES, UNIVERSITY OF SYDNEY, SYDNEY, N.S.W. 2006, AUSTRALIA
7 LABORATOIRE D'EXPLORATION ET GESTION DES RESSOURCES NATURELLES, DÉPARTEMENT DES SCIENCES DE LA TERRE, FACULTÉ DES SCIENCES ET TECHNIQUES, BENI MELLAL, MOROCCO
8 GEOFORSCHUNGSZENTRUM POTSDAM, D-14473 POTSDAM, GERMANY
9 UNIVERSITÀ DEGLI STUDI DI ROMA LA SAPIENZA, DIPARTIMENTO DI SCIENZE DELLA TERRA, PIAZZALE ALDO MORO 5, 00185 ROME, ITALY
10 NOVA SCOTIA DEPARTMENT OF NATURAL RESOURCES, PO BOX 698, HALIFAX, NS, CANADA B3J 2T9
11 DEPARTMENT OF GEOLOGICAL SCIENCE, UNIVERSITY OF VIENNA, A-1090 VIENNA, AUSTRIA
12 DEPARTAMENTO DE CIÊNCIAS DA TERRA, UNIVERSIDADE DO MINHO, 4710-057 BRAGA, PORTUGAL
13 SCHOOL OF GEOLOGY AND GEOPHYSICS, UNIVERSITY OF OKLAHOMA, NORMAN, OK 73019-0628, USA
14 DEPARTAMENTO DE CIENCIAS DA TERRA, UNIVERSIDADE DE COIMBRA, 3000-272 COIMBRA, PORTUGAL
15 DEPARTMENT OF GEOLOGY AND GEOPHYSICS, UNIVERSITY OF CALGARY, CALGARY, AB, CANADA T2N 1N4
16 INSTITUT DES SCIENCES DE LA TERRE D'ORLÉANS (ISTO, UMR 6113), 45071 ORLÉANS CEDEX 2, FRANCE
17 CENTRO DE INVESTIGACIONES GEOLÓGICAS, 644 CALLE NO. 1, 1900 LA PLATA, ARGENTINA
18 INSTITUTE OF MINERALOGY, FREIBERG UNIVERSITY, D-09596 FREIBERG, GERMANY
19 SCHOOL OF GEOSCIENCES, UNIVERSITY OF NEWCASTLE, NEWCASTLE, N.S.W., AUSTRALIA
20 THE COUNCIL FOR GEOSCIENCE, PO BOX 5347, PORT ELIZABETH 6065, SOUTH AFRICA
21 DIPARTIMENTO DI SCIENZE DELLA TERRA E GEOLOGICO-AMBIENTALI, UNIVERSITÁ DI BOLOGNA, 40126 BOLOGNA, ITALY
22 INSTITUTO DE RECURSOS NATURALES Y AGROBIOLOGIA, CSIC, 37071 SALAMANCA, SPAIN
23 NEG-LABISE, DEPARTMENT OF GEOLOGY, FEDERAL UNIVERSITY OF PERNAMBUCO, RECIFE, PE 50670-000, BRAZIL
24 UNIVERSIDAD NACIONAL DE TUCUMAN, FACULTAD CIENCIAS NATURALES, INSTITUTO SUPERIOR CORRELACIÓN GEOLÓGICA, 4000 SAN MIGUEL DE TUCUMAN, ARGENTINA
25 DEPARTAMENTO DE GEOLOGIA, FACULTAD DE CIENCIAS, 37008 SALAMANCA, SPAIN
26 DEPARTMENT OF MINERAL DEPOSITS, FACULTY OF NATURAL SCIENCES, THE COMENIUS UNIVERSITY, MLYSKA DOLINA G, 842 15 BRATISLAVA, SLOVAKIA
27 DEPARTAMENTO DE PETROLOGIA Y GEOQUIMICA, FACULTAD DE CC. GEOLOGICAS, UNIVERSIDAD COMPLUTENSE, 28040 MADRID, SPAIN
28 DEPARTMENT OF GEOLOGY AND GEOPHYSICS, UNIVERSITY OF MINNESOTA, MINNEAPOLIS, MN 55455, USA
29 DEPARTMENT OF MINERALOGY, THE NATURAL HISTORY MUSEUM, LONDON SW7 5BD, UK
30 DEPARTMENT OF GEOLOGY, BELOIT COLLEGE, BELOIT, WI 53511, USA
Andalusite occurs as an accessory mineral in many types of peraluminous felsic igneous rocks, including rhyolites, aplites, granites, pegmatites, and anatectic migmatites. Some published stability curves for And = Sil and the water-saturated granite solidus permit a small stability field for andalusite in equilibrium with felsic melts. We examine 108 samples of andalusite-bearing felsic rocks from more than 40 localities world-wide. Our purpose is to determine the origin of andalusite, including the TPX controls on andalusite formation, using eight textural and chemical criteria: sizecompatibility with grain sizes of igneous minerals in the same rock; shaperanging from euhedral to anhedral, with no simple correlation with origin; state of aggregationsingle grains or clusters of grains; association with muscovitewith or without rims of monocrystalline or polycrystalline muscovite; inclusionsrare mineral inclusions and melt inclusions; chemical compositionandalusite with little significant chemical variation, except in iron content (0·081·71 wt % FeO); compositional zoningconcentric, sector, patchy, oscillatory zoning cryptically reflect growth conditions; compositions of coexisting phasesbiotites with high siderophylliteeastonite contents (Aliv
2·68 ± 0·07 atoms per formula unit), muscovites with 0·574·01 wt % FeO and 0·022·85 wt % TiO2, and apatites with 3·53 ± 0·18 wt % F. Coexisting muscovitebiotite pairs have a wide range of F contents, and FBt = 1·612FMs + 0·015. Most coexisting minerals have compositions consistent with equilibration at magmatic conditions. The three principal genetic types of andalusite in felsic igneous rocks are: Type 1 Metamorphic(a) prograde metamorphic (in thermally metamorphosed peraluminous granites), (b) retrograde metamorphic (inversion from sillimanite of unspecified origin), (c) xenocrystic (derivation from local country rocks), and (d) restitic (derivation from source regions); Type 2 Magmatic(a) peritectic (water-undersaturated, T
) associated with leucosomes in migmatites, (b) peritectic (water-undersaturated, T
), as reaction rims on garnet or cordierite, (c) cotectic (water-undersaturated, T
) direct crystallization from a silicate melt, and (d) pegmatitic (water-saturated, T
), associated with aplitepegmatite contacts or pegmatitic portion alone; Type 3 Metasomatic(water-saturated, magma-absent), spatially related to structural discontinuities in host, replacement of feldspar and/or biotite, intergrowths with quartz. The great majority of our andalusite samples show one or more textural or chemical criteria suggesting a magmatic origin. Of the many possible controls on the formation of andalusite (excess Al2O3, water concentration and fluid evolution, high BeBLiP, high F, high FeMnTi, and kinetic considerations), the two most important factors appear to be excess Al2O3 and the effect of releasing water (either to strip alkalis from the melt or to reduce alumina solubility in the melt). Of particular importance is the evidence for magmatic andalusite in granites showing no significant depression of the solidus, suggesting that the And = Sil equilibrium must cross the granite solidus rather than lie below it. Magmatic andalusite, however formed, is susceptible to supra- or sub-solidus reaction to produce muscovite. In many cases, textural evidence of this reaction remains, but in other cases muscovite may completely replace andalusite leaving little or no evidence of its former existence.
KEY WORDS: andalusite; granite; magmatic; origin; xenocrystic
* Corresponding author. Telephone: (902) 494-2358. Fax: (902) 494-6889. E-mail: clarke{at}dal.ca
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