Nepheline solid solution compositions: stoichiometry revisited, reviewed, clarified and rationalised

Abstract

AbstractMolecular formulae used to recalculate nepheline analyses generally have different numbers of oxygens (e.g. NaAlSiO4(Ne), KAlSiO4,(Ks), CaAl2Si2O8(An) and SiO2(Q)). A 32 oxygen cell has 16 T cations and 8 cavity sites, but ideal nepheline stoichiometry is not necessarily followed. Ca end-member □CaCaAl2Si2O4(CaNe) and excess silica end-member □SiSi2O4(Q’) calculation requires inclusion of both vacancy species as cavity cation values. Q’ parameter calculations can involve different assumptions and four parameters are described: Qxs; QSi; Q(Si–Al); and Qcavity; these should have closely similar values for high-quality, stoichiometric analyses.Representative published compositions are recalculated to assess whether authors followed ideal nepheline stoichiometry. Phenocrysts from peralkaline rocks and nephelinites typically exhibit Al deficiencies reflected in negative Δ(Al – cavity cation) parameters (ΔAlcc), negative ‘normative’ corundum (Al2O3,Cn), and anomalously low or negative Qxsparameters; for such rock types Q(Si–Al)provides a better estimate of excess silica contents. A ΔT-site (cation charge) parameter (ΔTcharge), is closely coupled to ΔAlccand end-member NaAlSiO4has a ΔAlcc/ΔTchargeratio of 1.4296; the derivation of this value is controlled by strict stuffed-tridymite, unit-cell constraints. Natural nephelines all contain excess silica with a mean ΔAlcc/ΔTchargeof ~1.134 reflecting their Si/Al ratio being > 1.Nepheline analyses with relatively low Al and Si and high Na (also Ca) contents are common; this might reflect the presence of small amounts (up to ~5%) of cancrinite as an alteration phase or perhaps even in solid solution. The compositions of alteration lamellae of Ca-rich cancrinite in altered nepheline phenocrysts in phonolites from the Marangudzi alkaline complex, Zimbabwe, are used to define diagnostic parameters for recognising such non-stoichiometry. These alteration lamellae formed hydrothermally from Ca-rich and K-poor fluids.An EXCEL file is provided to help researchers to standardise calculation of nepheline end-member molecular proportions.