A simple IR spectroscopy method for detecting hydrated and dehydrated halloysite in artificial mixtures with kaolinite is described. The method is based on the exclusive ability of RbC1 among the alkali halides to form a complex with haUoysite but not with kaolinite. This complex absorbs at 3500 cm -1 when hydrated halloysite or admixed halloysite is examined in RbCI disks, the limit of detection being 15% in the kaolin admixture. Heating the clay powders or corresponding RbCI disks at 110~ affects the 3500 cm ~ frequency. The development of this absorption band together with a decrease in the intensity ratio of the 3690/3620 cm -~ frequencies is proportional to increasing amounts of halloysite in the kaolin admixtures. This method has an analytical applicability and is relatively rapid.When both kaolinite and halloysite are present in a sample, characterization and crystallinity measurements from X-ray diffraction (XRD) may be misleading (Keller & Haenni, 1978) and other investigative methods are desirable. Electron microscopy can distinguish between the platy morphology of kaolinite and tubular morphology of halloysite. In the present paper it is shown how infrared spectroscopy (IR) can be used to identify halloysite, in its hydrated or dehydrated forms, mixed with kaolinite in different proportions. In contrast to kaolinite, halloysite may form a complex with RbC1 under appropriate conditions, whereas neither of these clays interact with KBr. Thus, the unusual alkali halide RbC1 is used here as a matrix for the preparation of the disks for IR study. The development of the RbC1 complex with increasing concentrations of halloysite can be detected by IR spectroscopy, indicating an analytical potential for this simple and rapid method.
EXPERIMENTALArtificial mixtures of halloysite (Ward's # 13) and kaolinite (Georgia, USA) in different weight proportions (5, 10, 15, 25, 35, 50, 75, 85 and 95% halloysite in kaolinite) were prepared by thoroughly mixing the corresponding amounts of clays. Each mixture was examined by IR absorption spectroscopy in the 4000-1500 cm -1 region with a Perkin Elmer model 567 grating spectrophotometer. Disks of 13 mm diameter were made in a die, after manual gentle mixing (to avoid grinding effects), using 0.1250 g previously dried fine RbC1 powder (Merck) plus 0.0008 g of dried (110~ or undried clay. Spectra of freshly prepared disks were recorded before and after heating the disks at 110~ A dry glove box was used for handling the powders or disks. If heated, they were subsequently cooled under 9 1985 The Mineralogical Society