A hierachial classification of perovskite super-group minerals

Roger Howard Mitchell, Lakehead University, Geology, Thunder Bay, ON, Canada, Anton Chakhmouradian, University of Manitoba, Department of Geological Sciences, Winnipeg, MB, Canada and Mark Welch, Natural History Museum, Department of Mineralogy, London, United Kingdom

Contact First Author: Roger Howard Mitchell; rmitchel@lakeheadu.ca

Abstract ID#: 34920

 

English Abstract:
Some naturally-occurring oxides, fluorides, hydroxides, arsenides and silicates adopt crystal structures based upon, or which are derivatives of, the aristotypic cubic ternary perovskite structure (ABX3), as exemplified by the synthetic compounds SrTiO3 and KMgF3 and their mineral counterparts, tausonite and parascandolaite. On the basis of the extensive studies of synthetic perovskite-structured compounds it is possible to derive a hierarchy of hettotype structures which are produced by: (1) tilting and distortion of the BX6 octahedra; (2) ordering of A- and/or B-site cations; (3) formation of A-, B- or X-site vacancies. This hierarchical scheme as applied to naturally-occurring minerals results in the proposed recognition of a perovskite super group. Sub-groups include: (1) single ternary (ABX3) ideal (tausonite, isolueshite) and distorted (bridgmanite, perovskite, loparite, lueshite,lakargiite, megawite, neighborite, parascandolaite) perovskites, and others which exhibit second order Jahn-Teller distortions (macedonite, barioperovskite); (2) B-site cation ordered double (A2BBX6) perovskites (elpasolite, cryolite, simmonsite, vapnikite); (3) Anion-deficient (A2B2O5) perovskites (brownmillerite, srebrodolskite); (4) A-site vacant single- and double hydroxyperovskites (dzhalindite, bernalite, schönfliesite, stottite and mopungite subgroups); (5) A-site vacant quadruple perovskites (skutterudite subgroup); (6) B-site vacant double perovskites (diaboleite). Common ternary oxide perovskites typically exhibit space group variations resulting from solid solution between potential end-member compositions, and complete characterization requires single-crystal structure determination. In some ambiguous cases vibrational spectroscopy (Raman, infrared) can provide critical additional information that allows a correct choice of space group.