BASELINE STUDIES OF THE CLAY MINERALS SOCIETY SOURCE CLAYS BY X-RAY PHOTOELECTRON SPECTROSCOPY (original) (raw)

Abstract

This paper presents an overview of the chemical analyses of the Clay Mineral Society Source Clays based on X-ray Photoelectron Spectroscopy. This technique does not require any detailed sample preparation and is therefore easy to perform. In contrast to other common chemical analytical techniques fluorine and chlorine can be analysed together with all the major elements. In addition, the high resolution spectra reveal some details about the local environment of different cations in the clay structure, such as the presence of water, distinction between octahedral and tetrahedral aluminium and the presence of two types of Mg in the octahedral sheets.

Figures (9)

Table 1. The Clay Minerals Society Source Clays analysed in this study.

Table 1. The Clay Minerals Society Source Clays analysed in this study.

Fig. 1. Peak identification in XPS survey scan of montmorillonite SWy-2.  Baseline studies of the Clay Minerals Society Source Clays by X-ray photoelectron spectroscopy

Fig. 1. Peak identification in XPS survey scan of montmorillonite SWy-2. Baseline studies of the Clay Minerals Society Source Clays by X-ray photoelectron spectroscopy

Table 2a. Chemical compositions (in atom %) based on survey XPS analyses with Si as reference.

Table 2a. Chemical compositions (in atom %) based on survey XPS analyses with Si as reference.

Table 2b. Chemical composition data (in atom %) from Datahandbook for Clay Minerals and Other Non-metallic Minerals (van Olphen and Fripiat, 1979) and Clays and Clay Minerals special issue 49(5) Source Clays (2001).  couple of marked differences. Due to the rather low signal strength of iron (Fe 2p) it is difficult to get a very reliable iron analysis and often an over- or under-estimation of the iron content is made. Furthermore, since XPS analyses binding electrons, it is difficult to distinguish between ferric and fer-  rous iron in the crystal structure. In a number of clay samples (Swy-2, SAz-l, SCa-3 and VTx-1) fluorine was observed but  the signal was too weak to obtain an accurate analysis of the amount of fluorine. Chlorine (2.2 at%) was observed for SapCa-2, which has not been observed before.

Table 2b. Chemical composition data (in atom %) from Datahandbook for Clay Minerals and Other Non-metallic Minerals (van Olphen and Fripiat, 1979) and Clays and Clay Minerals special issue 49(5) Source Clays (2001). couple of marked differences. Due to the rather low signal strength of iron (Fe 2p) it is difficult to get a very reliable iron analysis and often an over- or under-estimation of the iron content is made. Furthermore, since XPS analyses binding electrons, it is difficult to distinguish between ferric and fer- rous iron in the crystal structure. In a number of clay samples (Swy-2, SAz-l, SCa-3 and VTx-1) fluorine was observed but the signal was too weak to obtain an accurate analysis of the amount of fluorine. Chlorine (2.2 at%) was observed for SapCa-2, which has not been observed before.

Fig. 2. High resolution Si 2p spectra.

Fig. 2. High resolution Si 2p spectra.

" trace Mg was observed (Mg 1s 1303.99 eV), but is present in the interlayer and not in the clay sheets 2 vw=very weak  Table 3. Binding energies (eV) of the major elements in the clay octahedral and tetrahedral sheets of the Source Clays analysed.

" trace Mg was observed (Mg 1s 1303.99 eV), but is present in the interlayer and not in the clay sheets 2 vw=very weak Table 3. Binding energies (eV) of the major elements in the clay octahedral and tetrahedral sheets of the Source Clays analysed.

Fig. 3. (a) High resolution Al 2p spectrum of beidellite SBCa-1. (b) High resolution Mg |s spectrum of montmorillonite SCa-3.

Fig. 3. (a) High resolution Al 2p spectrum of beidellite SBCa-1. (b) High resolution Mg |s spectrum of montmorillonite SCa-3.

x. 4. (a) High resolution O 1s spectrum of kaolinite KGa-1. (b) O 1s spectrum of beidellite SBCa-1. (c) O 1s spectrum of ripidolite CCa-1. (d) O 1s spectrum of attapulgite PFI-1. (e) O 1s spectrum of sepiolite SepNev-1. (f) O 1 spectrum of corrensite CorWa-1.  Baseline studies of the Clay Minerals Society Source Clays by X-ray photoelectron spectroscopy

x. 4. (a) High resolution O 1s spectrum of kaolinite KGa-1. (b) O 1s spectrum of beidellite SBCa-1. (c) O 1s spectrum of ripidolite CCa-1. (d) O 1s spectrum of attapulgite PFI-1. (e) O 1s spectrum of sepiolite SepNev-1. (f) O 1 spectrum of corrensite CorWa-1. Baseline studies of the Clay Minerals Society Source Clays by X-ray photoelectron spectroscopy

‘ig. 5. (a) Na 1s spectrum of hectorite SHCa-1. (b) Ca 2p spec- Fig. 6. (a) F 1s spectra of Barasym Syn-l, sepiolite SepNev-1 and trum of nontronite NG-1. hectorite SHCa-1. (b) Cl 2p spectrum of saponite SapCa-2.  The Ca 2p transitions for exchangeable Ca are split in two Gaussian shaped bands Ca 2pl and Ca 2p3 bands around 350.7 eV and 347.2 eV (e.g., nontronite NG-1, Figure 5b). Simi- ar to the exchangeable Ca, K is observed as the K 2p transi- ions K 2pl around 297.2 eV and K 2p3 around 294.3 eV but with very low intensity to noise ratio the bands are difficult to accurately fit. Though Adams and Evans (1979) used XPS o determine the cation exchange capacity (CEC) of beidellite using a variety of cations including Ca”* and K*, they did not report the binding energies for these atoms in the interlayer of he beidellite making comparison impossible. A similar type study on micas and illite-smectite clays by Johns and Gier 2001) also used XPS to determine interlayer cation ratios without providing binding energy details for these cations. In contrast K 2p binding energy values similar to those observed in this study have been reported for micas. Bhattacharyya   Despite the fact that corrensite consists of a regular |: 1 in- terstratification of a trioctahedral chlorite and a trioctahedral smectite, this is not reflected in the O 1s spectrum that only shows a single transition at 532.01 eV for oxygen atoms in the structure and a single transition at 533.29 eV for the hydroxyl groups (Figure 4f). The ratio between oxygen and hydroxyls is about 1:2.5 which is slightly on the low side compared to the theoretical ratio of 1 :2. However the peak fit is rather poor and introduces a relatively large error in the determination of the ratio.

‘ig. 5. (a) Na 1s spectrum of hectorite SHCa-1. (b) Ca 2p spec- Fig. 6. (a) F 1s spectra of Barasym Syn-l, sepiolite SepNev-1 and trum of nontronite NG-1. hectorite SHCa-1. (b) Cl 2p spectrum of saponite SapCa-2. The Ca 2p transitions for exchangeable Ca are split in two Gaussian shaped bands Ca 2pl and Ca 2p3 bands around 350.7 eV and 347.2 eV (e.g., nontronite NG-1, Figure 5b). Simi- ar to the exchangeable Ca, K is observed as the K 2p transi- ions K 2pl around 297.2 eV and K 2p3 around 294.3 eV but with very low intensity to noise ratio the bands are difficult to accurately fit. Though Adams and Evans (1979) used XPS o determine the cation exchange capacity (CEC) of beidellite using a variety of cations including Ca”* and K*, they did not report the binding energies for these atoms in the interlayer of he beidellite making comparison impossible. A similar type study on micas and illite-smectite clays by Johns and Gier 2001) also used XPS to determine interlayer cation ratios without providing binding energy details for these cations. In contrast K 2p binding energy values similar to those observed in this study have been reported for micas. Bhattacharyya Despite the fact that corrensite consists of a regular |: 1 in- terstratification of a trioctahedral chlorite and a trioctahedral smectite, this is not reflected in the O 1s spectrum that only shows a single transition at 532.01 eV for oxygen atoms in the structure and a single transition at 533.29 eV for the hydroxyl groups (Figure 4f). The ratio between oxygen and hydroxyls is about 1:2.5 which is slightly on the low side compared to the theoretical ratio of 1 :2. However the peak fit is rather poor and introduces a relatively large error in the determination of the ratio.

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