2006 Philadelphia Annual Meeting (22–25 October 2006)

Paper No. 2
Presentation Time: 8:30 AM

ORDER-DISORDER IN THE OCTAHEDRAL SHEET OF METAMORPHIC 2M1 PHENGITES: A COMBINED EMPA AND AXANES STUDY


CIBIN, Giannantonio, Dipartimento di Scienze Geologiche, Università degli Studi Roma Tre, Largo S. Leonardo Murialdo 1, 00146 Roma, Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, Via Enrico Fermi 40, Frascati RM, 00030, Italy, CINQUE, Gianfelice, Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, Via Enrico Fermi 40, 00030 Frascati RM, Italy, Diamond Light Source, Rutherford Appleton Laboratory, Chilton, Didcot Oxforshire, OX11 0QX, United Kingdom, MARCELLI, Augusto, Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, Via Enrico Fermi 40, Frascati, Roma, 00030, Italy, MOTTANA, Annibale, Dipartimento di Scienze Geologiche, Università degli Studi Roma Tre, Largo S. Leonardo Murialdo 1, Roma, 00146, Italy and SASSI, Raffaele, Dipartimento di Mineralogia e Petrologia, Università degli Studi di Padova, Corso Garibaldi 37, Padova, 35137, Italy, mottana@uniroma3.it

Two types of metamorphic phengites are known: one is linked to HP and is 3T, the other is 2M1: for both the composition is due to rock compositional constraints. This work aims at investigating crystallographic differences between the two phengite types. Six mica samples were studied: 1) one UHP 3T phengite from Dora Maira (P~2.5 Gpa, T~ 750°C); 2) four 2M1 phengites from orthogneisses from Eastern Alps (P= < 0.6 Gpa, T~ 500-600°C); 3) one 2M1 ferroan muscovite from a pegmatite in Antarctica (LP, T ~ 500°C). All studied phengites display significant extents of celadonite substitution. EPMA were carried out at Padua using Cameca-Camebax SX50. XAFS spectra were recorded for Fe at SSRL (U.S.A.) by fluorescence detection mode, and for all other atoms at DAPHNE (Frascati, Italy) by transmission mode. We recorded our AXANES spectra on mosaics of flakes carefully separated and oriented flat on a plastic support. All 2M1 phengites have IVAl > 1 apfu; their VIatom contents are dominated by Al, with variable Fe (partly Fe3+) and Mg. Ti, Mn, and Cr are <0.03 apfu. VIOccupancy in them is slighty > 4 apfu, i.e., there is a partial occupancy of the third VIsheet site. XAFS spectra show complex patterns, which reflect an ordered cation distribution in the VIsheet (and, for Al, in the IVsheet as well). By contrast, the 3T phengite have IVAl just < 1 apfu), and Al and Mg are dominant VIconstituents, being Ti, Cr and Fe (Fe2+) present only at the trace level. XAFS spectra show one broad peak only, indicating Fe2+ in a fully disordered distribution. This is also pointed out by the absence of other XANES features at high-energy i.e., before the onset of EXAFS oscillations. In conclusion: i) 3T phengites from Dora Maira massif, related to UHP, displays complete octahedral disorder; ii) 2M1 phengites unrelated to HP suggest Al and Mg/Fe order over the M1 and (M2,M3) sites in a regular way, as does the 2M1 muscovite from Antarctica pegmatite.