Supporting information
Crystallographic Information File (CIF) https://doi.org/10.1107/S1600536813001013/br2219sup1.cif | |
Structure factor file (CIF format) https://doi.org/10.1107/S1600536813001013/br2219Isup2.hkl |
Key indicators
- Single-crystal X-ray study
- T = 293 K
- Mean (Sn-S) = 0.002 Å
- Disorder in main residue
- R factor = 0.027
- wR factor = 0.070
- Data-to-parameter ratio = 24.0
checkCIF/PLATON results
No syntax errors found
Alert level C STRVA01_ALERT_2_C Chirality of atom sites is inverted? From the CIF: _refine_ls_abs_structure_Flack 0.910 From the CIF: _refine_ls_abs_structure_Flack_su 0.060 PLAT041_ALERT_1_C Calc. and Reported SumFormula Strings Differ ? PLAT068_ALERT_1_C Reported F000 Differs from Calcd (or Missing)... ? PLAT077_ALERT_4_C Unitcell contains non-integer number of atoms .. ? PLAT915_ALERT_3_C Low Friedel Pair Coverage ...................... 81 Perc.
Alert level G PLAT004_ALERT_5_G Info: Polymeric Structure Found with Dimension . 2 PLAT005_ALERT_5_G No _iucr_refine_instructions_details in the CIF ? PLAT045_ALERT_1_G Calculated and Reported Z Differ by ............ 0.50 Ratio PLAT152_ALERT_1_G The Supplied and Calc. Volume s.1. Differ by ... 3 Units PLAT199_ALERT_1_G Check the Reported _cell_measurement_temperature 293 K PLAT200_ALERT_1_G Check the Reported _diffrn_ambient_temperature 293 K PLAT301_ALERT_3_G Note: Main Residue Disorder ................... 23 Perc. PLAT794_ALERT_5_G Note: Tentative Bond Valency for Sn (IV) 3.91 PLAT794_ALERT_5_G Note: Tentative Bond Valency for Ag1 (I) 1.27 PLAT811_ALERT_5_G No ADDSYM Analysis: Too Many Excluded Atoms .... ! PLAT860_ALERT_3_G Note: Number of Least-Squares Restraints ....... 4 PLAT961_ALERT_5_G Dataset Contains no Negative Intensities ....... !
0 ALERT level A = Most likely a serious problem - resolve or explain 0 ALERT level B = A potentially serious problem, consider carefully 5 ALERT level C = Check. Ensure it is not caused by an omission or oversight 12 ALERT level G = General information/check it is not something unexpected 6 ALERT type 1 CIF construction/syntax error, inconsistent or missing data 1 ALERT type 2 Indicator that the structure model may be wrong or deficient 3 ALERT type 3 Indicator that the structure quality may be low 1 ALERT type 4 Improvement, methodology, query or suggestion 6 ALERT type 5 Informative message, check
The pirquitasite specimen used in this study comes from the type locality, the Pirquitas deposit, Jujuy Province, Argentina and is in the collection of the RRUFF project (http://rruff.info/R061016). The chemical composition, (Ag1.87Cu0.13)(Zn0.61Fe0.36Cd0.03)SnS4, was determined with a CAMECA SX100 electron microprobe. The composition was normalized to four cations.
The structure was refined with the inversion twin (-1 0 0/0 - 1 0/0 0 - 1) to a ratio of 0.91 (6). During refinement, the chemistry was constrained to the empirical formula of (Ag1.87Cu0.13)(Zn0.61Fe0.36Cd0.03)SnS4. The maximum residual electron density in the difference Fourier maps was located at (0.0434, 0.0434, 0.2204), 0.56 Å from Ag2 and the minimum at (0, 0, 0.0693) 0.75 Å from Ag1.
Data collection: APEX2 (Bruker, 2004); cell refinement: SAINT (Bruker, 2004); data reduction: SAINT (Bruker, 2004); program(s) used to solve structure: SHELXS97 (Sheldrick, 2008); program(s) used to refine structure: SHELXL97 (Sheldrick, 2008); molecular graphics: XtalDraw (Downs & Hall-Wallace, 2003); software used to prepare material for publication: publCIF (Westrip, 2010).
(Ag1.87Cu0.13)(Zn0.61Fe0.36Cd0.03)SnS4 | Dx = 4.765 Mg m−3 |
Mr = 520.26 | Mo Kα radiation, λ = 0.71073 Å |
Tetragonal, I4 | Cell parameters from 527 reflections |
Hall symbol: I -4 | θ = 6.3–32.3° |
a = 5.7757 (12) Å | µ = 12.58 mm−1 |
c = 10.870 (2) Å | T = 293 K |
V = 362.60 (13) Å3 | Cuboid, grey |
Z = 2 | 0.05 × 0.05 × 0.04 mm |
F(000) = 470 |
Bruker APEXII CCD area-detector diffractometer | 575 independent reflections |
Radiation source: fine-focus sealed tube | 570 reflections with I > 2σ(I) |
Graphite monochromator | Rint = 0.013 |
ϕ and ω scan | θmax = 32.0°, θmin = 3.8° |
Absorption correction: multi-scan (SADABS; Sheldrick, 2005) | h = −4→8 |
Tmin = 0.572, Tmax = 0.633 | k = −8→7 |
1312 measured reflections | l = −16→12 |
Refinement on F2 | Secondary atom site location: difference Fourier map |
Least-squares matrix: full | w = 1/[σ2(Fo2) + (0.0272P)2 + 2.1498P] where P = (Fo2 + 2Fc2)/3 |
R[F2 > 2σ(F2)] = 0.027 | (Δ/σ)max < 0.001 |
wR(F2) = 0.070 | Δρmax = 1.05 e Å−3 |
S = 1.17 | Δρmin = −0.87 e Å−3 |
575 reflections | Extinction correction: SHELXL, Fc*=kFc[1+0.001xFc2λ3/sin(2θ)]-1/4 |
24 parameters | Extinction coefficient: 0.0061 (6) |
4 restraints | Absolute structure: Flack (1983) |
Primary atom site location: structure-invariant direct methods | Absolute structure parameter: 0.91 (6) |
(Ag1.87Cu0.13)(Zn0.61Fe0.36Cd0.03)SnS4 | Z = 2 |
Mr = 520.26 | Mo Kα radiation |
Tetragonal, I4 | µ = 12.58 mm−1 |
a = 5.7757 (12) Å | T = 293 K |
c = 10.870 (2) Å | 0.05 × 0.05 × 0.04 mm |
V = 362.60 (13) Å3 |
Bruker APEXII CCD area-detector diffractometer | 575 independent reflections |
Absorption correction: multi-scan (SADABS; Sheldrick, 2005) | 570 reflections with I > 2σ(I) |
Tmin = 0.572, Tmax = 0.633 | Rint = 0.013 |
1312 measured reflections |
R[F2 > 2σ(F2)] = 0.027 | 4 restraints |
wR(F2) = 0.070 | Δρmax = 1.05 e Å−3 |
S = 1.17 | Δρmin = −0.87 e Å−3 |
575 reflections | Absolute structure: Flack (1983) |
24 parameters | Absolute structure parameter: 0.91 (6) |
Geometry. All e.s.d.'s (except the e.s.d. in the dihedral angle between two l.s. planes) are estimated using the full covariance matrix. The cell e.s.d.'s are taken into account individually in the estimation of e.s.d.'s in distances, angles and torsion angles; correlations between e.s.d.'s in cell parameters are only used when they are defined by crystal symmetry. An approximate (isotropic) treatment of cell e.s.d.'s is used for estimating e.s.d.'s involving l.s. planes. |
Refinement. Refinement of F2 against ALL reflections. The weighted R-factor wR and goodness of fit S are based on F2, conventional R-factors R are based on F, with F set to zero for negative F2. The threshold expression of F2 > σ(F2) is used only for calculating R-factors(gt) etc. and is not relevant to the choice of reflections for refinement. R-factors based on F2 are statistically about twice as large as those based on F, and R- factors based on ALL data will be even larger. |
x | y | z | Uiso*/Ueq | Occ. (<1) | |
Ag1 | 0.0000 | 0.0000 | 0.0000 | 0.0364 (4) | |
Ag2 | 0.0000 | 0.5000 | 0.2500 | 0.0301 (6) | 0.87 |
Cu | 0.0000 | 0.5000 | 0.2500 | 0.0301 (6) | 0.13 |
Zn | 0.5000 | 0.0000 | 0.2500 | 0.0220 (6) | 0.61 |
Fe | 0.5000 | 0.0000 | 0.2500 | 0.0220 (6) | 0.36 |
Cd | 0.5000 | 0.0000 | 0.2500 | 0.0220 (6) | 0.03 |
Sn | 0.5000 | 0.5000 | 0.0000 | 0.01176 (18) | |
S | 0.7325 (3) | 0.2526 (4) | 0.12847 (11) | 0.0214 (3) |
U11 | U22 | U33 | U12 | U13 | U23 | |
Ag1 | 0.0360 (5) | 0.0360 (5) | 0.0372 (4) | 0.000 | 0.000 | 0.000 |
Ag2 | 0.0274 (7) | 0.0274 (7) | 0.0355 (9) | 0.000 | 0.000 | 0.000 |
Cu | 0.0274 (7) | 0.0274 (7) | 0.0355 (9) | 0.000 | 0.000 | 0.000 |
Zn | 0.0248 (8) | 0.0248 (8) | 0.0163 (9) | 0.000 | 0.000 | 0.000 |
Fe | 0.0248 (8) | 0.0248 (8) | 0.0163 (9) | 0.000 | 0.000 | 0.000 |
Cd | 0.0248 (8) | 0.0248 (8) | 0.0163 (9) | 0.000 | 0.000 | 0.000 |
Sn | 0.0114 (2) | 0.0114 (2) | 0.0125 (3) | 0.000 | 0.000 | 0.000 |
S | 0.0250 (6) | 0.0212 (6) | 0.0181 (6) | 0.0053 (5) | −0.0023 (5) | 0.0044 (5) |
Ag1—Si | 2.5430 (17) | Zn—Siv | 2.383 (2) |
Ag1—Sii | 2.5430 (17) | Zn—Sviii | 2.383 (2) |
Ag1—Siii | 2.5430 (17) | Zn—S | 2.383 (2) |
Ag1—Siv | 2.5430 (17) | Zn—Svii | 2.383 (2) |
Ag2—Siii | 2.485 (2) | Sn—Sii | 2.4070 (16) |
Ag2—Sv | 2.485 (2) | Sn—S | 2.4070 (16) |
Ag2—Svi | 2.485 (2) | Sn—Sv | 2.4070 (16) |
Ag2—Svii | 2.485 (2) | Sn—Six | 2.4070 (16) |
Si—Ag1—Sii | 113.39 (6) | Siv—Zn—Sviii | 107.90 (4) |
Si—Ag1—Siii | 107.55 (3) | Siv—Zn—S | 112.66 (8) |
Sii—Ag1—Siii | 107.55 (3) | Sviii—Zn—S | 107.90 (4) |
Si—Ag1—Siv | 107.55 (3) | Siv—Zn—Svii | 107.90 (4) |
Sii—Ag1—Siv | 107.55 (3) | Sviii—Zn—Svii | 112.66 (8) |
Siii—Ag1—Siv | 113.39 (6) | S—Zn—Svii | 107.90 (4) |
Siii—Ag2—Sv | 115.77 (7) | Sii—Sn—S | 109.67 (4) |
Siii—Ag2—Svi | 106.42 (3) | Sii—Sn—Sv | 109.67 (4) |
Sv—Ag2—Svi | 106.42 (3) | S—Sn—Sv | 109.08 (7) |
Siii—Ag2—Svii | 106.42 (3) | Sii—Sn—Six | 109.08 (7) |
Sv—Ag2—Svii | 106.42 (3) | S—Sn—Six | 109.67 (4) |
Svi—Ag2—Svii | 115.77 (7) | Sv—Sn—Six | 109.67 (4) |
Symmetry codes: (i) −y, x−1, −z; (ii) y, −x+1, −z; (iii) x−1, y, z; (iv) −x+1, −y, z; (v) −x+1, −y+1, z; (vi) y−1/2, −x+3/2, −z+1/2; (vii) −y+1/2, x−1/2, −z+1/2; (viii) y+1/2, −x+1/2, −z+1/2; (ix) −y+1, x, −z. |
Experimental details
Crystal data | |
Chemical formula | (Ag1.87Cu0.13)(Zn0.61Fe0.36Cd0.03)SnS4 |
Mr | 520.26 |
Crystal system, space group | Tetragonal, I4 |
Temperature (K) | 293 |
a, c (Å) | 5.7757 (12), 10.870 (2) |
V (Å3) | 362.60 (13) |
Z | 2 |
Radiation type | Mo Kα |
µ (mm−1) | 12.58 |
Crystal size (mm) | 0.05 × 0.05 × 0.04 |
Data collection | |
Diffractometer | Bruker APEXII CCD area-detector diffractometer |
Absorption correction | Multi-scan (SADABS; Sheldrick, 2005) |
Tmin, Tmax | 0.572, 0.633 |
No. of measured, independent and observed [I > 2σ(I)] reflections | 1312, 575, 570 |
Rint | 0.013 |
(sin θ/λ)max (Å−1) | 0.746 |
Refinement | |
R[F2 > 2σ(F2)], wR(F2), S | 0.027, 0.070, 1.17 |
No. of reflections | 575 |
No. of parameters | 24 |
No. of restraints | 4 |
Δρmax, Δρmin (e Å−3) | 1.05, −0.87 |
Absolute structure | Flack (1983) |
Absolute structure parameter | 0.91 (6) |
Computer programs: APEX2 (Bruker, 2004), SAINT (Bruker, 2004), SHELXS97 (Sheldrick, 2008), SHELXL97 (Sheldrick, 2008), XtalDraw (Downs & Hall-Wallace, 2003), publCIF (Westrip, 2010).
Mineral | Formula | Space Group | Reference |
Stannite | Cu2FeSnS4 | I42m | Hall et al. (1978) |
Hocartite | Ag2FeSnS4 | I42m | Johan & Picot (1982) |
Kuramite | Cu21+Cu2+SnS4 | I42m | Chen et al. (1998) |
Černyite | Cu2CdSnS4 | I42m | Szymański (1978) |
Velikite | Cu2HgSnS4 | I42m | Kaplunnik et al. (1977) |
Famatinite | Cu21+Cu2+SbS4 | I42m | Garin & Parthé (1972) |
Luzonite | Cu21+Cu2+AsS4 | I42m | Marumo & Nowaki (1967) |
Barquillite | Cu2(Cd,Fe2+)GeS4 | I42m | Murciego et al. (1999) |
Briartite | Cu2FeGeS4 | I42m | Wintenberger (1979) |
Permingeatite | Cu21+Cu2+SbSe4 | I42m | Johan et al. (1971) |
Kesterite | Cu2ZnSnS4 | I4 | Kissin & Owens (1979) |
Ferrokesterite | Cu2(Fe,Zn)SnS4 | I4 | Kissin & Owens (1989) |
Pirquitasite | Ag2ZnSnS4 | I4 | This study |
Idaite | Cu2+Cu2+FeS4 | Unknown | Frenzel (1959) |
Pirquitasite is a member of the stannite group of tetragonal sulfides, which exhibit space group I42m or I4, and is an ordered derivative of the sphalerite structure (Johan and Picot, 1982). The stannite group currently contains thirteen species (Table 1), of which only kësterite, ferrokësterite, and pirquitasite are known to display space group I4. Synthetic sulfides with stannite type structures are utilized as the light absorber layer in photovoltaic cells (e.g. Salomé et al. 2012, Sasamura et al. 2012, Tsuji et al. 2010).
Pirquitasite was first described by Johan and Picot (1982), from the Pirquitas deposit, Argentina, as a silver zinc tin sulfide with ideal chemical formula Ag2ZnSnS4 and a stannite-like structure. An extensive solid solution between hocartite (Ag2FeSnS4) and pirquitasite was described by Johan and Picot (1982). Because of the solid solution and the I42m symmetry attributed to hocartite, Johan and Picot (1982) proposed that pirquitasite also exhibits I42m symmetry.
The structure was refined using both I42m and I4, with the R factor for I4 (R = 0.027) significantly lower than for I42m (R = 0.051). The structure of pirquitasite is a derivative of the cubic sphalerite structure that displays cubic closest packed (CCP) layers of S stacked along [111]. Because pirquitasite has a doubled c cell dimension, its stacking direction is [221]. Half of the tetrahedral sites are occupied by Ag, (Zn,Fe), and Sn cations, forming metal layers described by Hall et al. (1978), and it is the arrangement of Ag, (Zn,Fe), and Sn within these layers that differentiates the I4 kësterite structure from the I42m stannite structure.
Stannite and kësterite were originally recognized as distinct species because of different Fe—Zn compositional ratios and different optical properties (Orlova, 1956; Hall et al. 1978). Structural and chemical analyses by Hall et al. (1978) and Kissin and Owens (1979) not only showed a miscibility gap between the pure Fe end-member stannite and the pure Zn end-member kësterite, but found the two minerals differed in symmetry from I42m (stannite) to I4 (kësterite). In I42m, Cu atoms are ordered to the Wyckoff 4d site, (Fe,Zn) atoms are ordered to Wyckoff 2a, Sn is ordered to 2b (Hall et al. 1978). For comparison, the I4 symmetry has Cu atoms ordered to two sites: 2a and 2c, (Zn,Fe) ordered to 2d, Sn ordered to 2b (Hall et al. 1978). As pointed out by Hall et al. (1978), two distinct metal layers perpendicular to [001] result from this ordering in each mineral. Stannite exhibits one layer of Cu atoms only, with the other layer consisting of ordered Fe and Sn atoms, while kësterite exhibits one layer of ordered Cu and Sn atoms and one layer of ordered Zn and Cu atoms (Hall et al. 1978). This is illustrated for pirquitasite versus stannite in Fig. 1, which shows the pirquitasite structure (Fig. 1a) with one layer containing ordered Ag and Sn, the second containing ordered Zn and Ag. For comparison, the two stannite metal layers consist of one layer of Fe and Sn atoms and a second layer containing only Cu atoms (Fig. 1 b). The Ag—Sn layers in pirquitasite and Fe—Sn layers in stannite are ordered identically: Ag—Sn—Ag—Sn and Fe—Sn—Fe—Sn respectively when viewed along (100).
The mineral hocartite (tetragonal Ag2FeSnS4) is reported to exhibit space group I42m (Johan and Picot, 1982), but its structure is as yet unreported. It is likely that the hocartite-pirquitasite series follows the same systematics as the stannite-kësterite series.
An interesting feature is the distortion displayed by the AgS4 tetrahedra, with tetrahedral angle variance of 8.86° displayed by Ag1S4 and 25.40° displayed by Ag2S4. M-S bond lengths are 2.539 Å and 2.497 Å for the Ag1S4 and Ag2S4 tetrahedra, respectively. As our sample contains approximately 13% apfu Cu, this Cu appears to be located in the Ag2 site because the bond lengths are smaller and the tetrahedron can accomodate the distortion. Bond valence calculations gave sums of 1.28 valence units (VU) and 1.35 VU for Ag1 and Ag2, respectively, corroborating that Cu is ordered to the Ag2 site. In a study of the mechanism of incorporation of Cu, Fe, and Zn in the stannite-kësterite series, Bonazzi et al. (2003) studied synthetic crystals, quenched from 1023 Kelvin, of composition Cu2Fe1-XZnXS4 (X = 0, 1/5, 1/2, 0.7, 0.8, 1), which showed decreasing tetrahedral angle distortion with increasing Zn content across the stannite-kësterite compositions.