Quick
Search: 
 
advanced search
 GSW Home    GeoRef Home    My GSW Alerts    Contact GSW    About GSW    Journals List    Help 
American Mineralogist Email Content Delivery
JOURNAL HOME HELP CONTACT PUBLISHER SUBSCRIBE ARCHIVE SEARCH TABLE OF CONTENTS

American Mineralogist; July 2007; v. 92; no. 7; p. 1225-1231; DOI: 10.2138/am.2007.2481
© 2007 Mineralogical Society of America
This Article
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
Citing Articles
Right arrow Citing Articles via Google Scholar
Google Scholar
Right arrow Articles by Hålenius, U.
Right arrow Articles by Skogby, H.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation

Galaxite, MnAl2O4, a spectroscopic standard for tetrahedrally coordinated Mn2+ in oxygen-based mineral structures

Ulf Hålenius*, Ferdinando Bosi and Henrik Skogby

Department of Mineralogy, Swedish Museum of Natural History, P.O. Box 50007, SE-104 05 Stockholm, Sweden

Correspondence: * E-mail: ulf.halenius{at}nrm.se

Chemical analyses, crystal structure refinement, cation order determination, and single-crystal optical absorption spectrum of synthetic galaxite are presented. New optical absorption spectra of natural Mn-bearing willemite, rhodochrosite, Mn-rich forsterite, and tephroite are reported for comparative purposes.

The structure of a synthetic galaxite end-member is characterized by a relatively large unit-cell edge, a0 = 8.2104(3) Å, a u-parameter equal to 0.26588(7), a T-O distance of 2.0034(6) Å, and an M-O distance of 1.9310(5) Å. Mn2+ is strongly ordered at the tetrahedral T-site as demonstrated by the refined structural formula T(Mn2+ 0.90Al0.10)M(Mn2+ 0.10Al1.90)O4.

The optical absorption spectrum of galaxite in the range 300–800 nm shows a set of five relatively sharp bands at 20 300, 22 250, 23 390, 25 970, and 27 780 cm–1 marking spin-forbidden transitions in Mn2+ at the tetrahedral site. The molar absorption coefficient of the field-independent 6A1(S) -> 4Eg 4A1g(G) absorption band at 23 390 cm–1 equals 1.90 L/(mol·cm), which is approximately an order of magnitude higher than for corresponding bands in spectra of compounds that contain isolated Mn2+-centered octahedra.

The calculated crystal field splitting, 10Dq, for Mn2+ at the T-site in galaxite equals 5290 cm–1. This compares well with derived 10Dq-values of 5860 and 5510 cm–1 for Mn2+ at the tetrahedral T1- and T2-site in Mn-bearing willemite. In agreement with theory, the 10Dq for Mn2+ in MnO4 tetrahedra is ca. 30% smaller than corresponding values in MnO6 octahedra. The lower Racah B-parameters of the spectroscopic data indicate that the degree of covalency of Mn2+-O bonds is higher in tetrahedra than in octahedra.

Key Words: Crystal structure • galaxite • optical spectroscopy • willemite • tephroite • forsterite







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