The Silver(I) Mercury(II) Oxide Nitrate with the Empirical Formula AgHg2N 0 5 Thomas J. Mormann and Wolfgang Jeitschko Anorganisch-Chemisches Institut, Universität Münster, Wilhelm-Klemm-Str. 8, D-48149 Münster, Germany Reprint requests to Prof. Dr. W. Jeitschko. Z. Naturforsch. 54 b, 1489-1494 (1999); received September 7, 1999 Crystal Structure, Silver Mercury(II) Oxide Nitrate The title compound was prepared by solid state reaction of Ag2Ü with Hg(N03)2-H20 in air at 350 °C. Its crystal structure was determined from single-crystal diffractometer data: Pnma, a = 620.1(1) pm, b = 670.1(1) pm, c = 1267.5(2) pm, Z = 4, R = 0.026 for 586 structure factors and 33 variable parameters. The compound may be represented by the formula Ag(Hg0 )2N0 3 . The mercury(II) together with the oxygen atoms form zig-zag chains with linear coordination of the mercury atoms. The oxygen atoms of these chains are linked via silver(I) atoms, thus forming two-dimensionally infinite nets, which contain the trigonal planar nitrate groups in interstices. Thus, only secondary Hg-O and Ag-O bonds are formed between the nets. Introduction Two well-characterized modifications of mercury(II) oxide HgO are known: a trigonal and an orthorhombic modification. The trigonal form crystallizing in the enantiomorphous space groups P3i21 and P3221 - can be prepared by precipita tion at relatively low temperature (50 °C) [1, 2]. It irreversibly transforms on heating above 220 °C to the orthorhombic (Pnma) modification [3], which is identical with the mineral montroydite. Both forms seem to occur with yellow and/or red color, de pending on the particle size; with red for wellcrystallized samples and yellow for microcrystalline precipitates [4], To our knowledge the structure of metastable mercury (I) oxide Hg 2Ü has not been es tablished. It may even exist only in the form of the hydroxide Hg 2(OH )2 [4], Numerous silver oxides have been reported. Well characterized is the silver(I) oxide Ag 2Ü [5, 6] which is isotypic with cuprite CU2O. An appar ently second modification with this formula turned out to be a suboxide with the composition Ag 3 Ü [7], The crystal structures of two modifications of the silver(I, III) oxide AgO have been deter mined. One with monoclinic symmetry, crystalliz ing in the space group P2\/c [8-11], and a tetrago nal form with space group I4\/a [12]. Furthermore, two higher silver oxides are well characterized: the silver(II, III) oxide Ag30 4 [13] and the silver(III) oxide A g203 [14]. Ternary compounds containing only silver, mer cury, and oxygen have not yet been reported. Simi larly, pure mercury nitrates (without water) seem to be unknown. However, there are two well charac terized mercury oxide nitrates. One, with the empir ical formula Hg3N 2 0 g, contains a somewhat folded Hg 30 2 honeycomb net; it may be represented by the formula (H g 0 )2H g(N 03)2 [15]. The other, with the empirical formula Hg 2N 0 4, contains puckered nets formed by HgO zig-zag chains which are linked via Hg2 bridges. This structure also contains dis crete nitrate groups, thus resulting in a formula (H g 0)2H g2(N 03)2 [16, 17]. Three modifications of silver nitrate A g N 0 3 are known: an orthorhombic room temperature form [18-20], a rhombohedral high temperature modifi cation, which ist stable above 159 °C [21], and a rhombohedral metastable modification, which can be obtained by rapid cooling of melted A gN 03 [22]. Furthermore, the crystal structure of a cubic sil ver oxide nitrate AgyNOn has been determined. In this compound most silver atoms - all at the same Wyckoff position - together with most oxygen atoms form a clathrate which contains the remaining silver atoms and the nitrate groups in different cages. It thus was proposed to describe this compound by the formula (AgII’III)60 8 AgIN 0 3 [23], 0932-0776/99/1200-1489 $ 06.00 © 1999 Verlag der Zeitschrift für Naturforschung, Tübingen • www.znaturforsch.com K Dieses Werk wurde im Jahr 2013 vom Verlag Zeitschrift für Naturforschung in Zusammenarbeit mit der Max-Planck-Gesellschaft zur Förderung der Wissenschaften e.V. digitalisiert und unter folgender Lizenz veröffentlicht: Creative Commons Namensnennung-Keine Bearbeitung 3.0 Deutschland Lizenz. This work has been digitalized and published in 2013 by Verlag Zeitschrift für Naturforschung in cooperation with the Max Planck Society for the Advancement of Science under a Creative Commons Attribution-NoDerivs 3.0 Germany License. Zum 01.01.2015 ist eine Anpassung der Lizenzbedingungen (Entfall der Creative Commons Lizenzbedingung „Keine Bearbeitung“) beabsichtigt, um eine Nachnutzung auch im Rahmen zukünftiger wissenschaftlicher Nutzungsformen zu ermöglichen. On 01.01.2015 it is planned to change the License Conditions (the removal of the Creative Commons License condition “no derivative works”). This is to allow reuse in the area of future scientific usage. Th. J. Mormann and W. Jeitschko • A Silver(I) Mercury(II) Oxide Nitrate 1490 Table I. Atomic parameters of AgHg2NOs. X >’ 7 Ba 0.2528(3) 0.19802(6) 0.200(2) 0.1331(14) 0.1069(16) 0.1995(17) 0.320(2) 1/4 0.00003(9) 1/4 0.0920(14) 1/4 1/4 1/4 0.84564(10) 0.09692(2) 0.3561(11) 0.3949(6) 0.0194(8) 0.6704(8) 0.2772(10) 2.76(2) 1.337(9) 1.7(3) 2.4(2) 1.2(2) 1.9(2) 2.9(3) Atom Pnma Ag Hg N 01 02 03 04 4c 8d Atom U ii U2 2 U3 3 U 12 U 13 f/23 Ag Hg 551(8) 209(2) 306(6) 140(1) 193(5) 159(1) 0 -4(4) 18(8) -16(1) 0 4(2) 4c 8d 4c 4c 4c “The last column in the upper part of the table lists the isotropic displacement parameters of the light atoms and the equivalent isotropic displacement parameters of the metal atoms in units of 104 pm2. The anisotropic displacement parameters of the metal atoms (pm- ) are defined by exp(-27r2[/z2(a*)2£/n + ... + 2kIb*c*U2?,]). The up to now only known silver mercury ox ide nitrate was reported more recently [24], It has the empirical formula AgöHgNOn and it is iso typic with cubic AgyNOn [23]. Both compounds have the same AgöOg clathrate cages, and thus the mercury atoms of Ag6HgNOn substitute for those silver atoms of AgyNOn, which are located in the cages. Interestingly, the near-neighbor envi ronments of both compounds suggest that the metal positions in the cages have different oxidation num bers, corresponding to Ag(I) and Hg(II), respec tively. In contrast, the silver mercury oxide nitrate AgHg 2NC>5 , described here, consists of well defined two-dimensionally infinite silver mercury oxygen nets which enclose only nitrate groups. It thus may be represented by the formula Ag(Hg 0 )2N 0 3 . A preliminary account of the presently reported re sults has been given at a conference [25]. Sample Preparation The samples of AgHg2NO.s were prepared in open sil ica tubes by annealing for two weeks at 350 °C. The single crystals used for the structure determination were iso lated from a sample where the starting compounds Ag2Ü (Riedel de Haen, > 99 %) and Hg(N0 3)2-H20 (Fluka, > 99 %) had been mixed in the molar ratio 1:2. This sample contained impurities, which were not further identified. A pure sample of AgHg2NOs was obtained by reaction under the same conditions with the ideal molar starting ra tio of 14, established during the structure determination. The sample was placed in the cold furnace and heated to 350 °C within one hour. At first the silver oxide dissolves in the melted compound Hg(N0 3)2-H20. At higher tem peratures the nitrogen oxides and the water evaporate. Thus the reaction might be formulated by the equation 2Ag20 + 8Hg(N03)2-H20 = 4AgHg2N 0 5 + 12N02 + 3 0 2 + 8H20 ignoring the NO/NO2 equilibrium. After the annealing, the samples were cooled in the furnace to room tempera ture within 5 h. The reaction product at the bottom of the silica tube consisted of yellow needles with easy cleavage along the needle axis. This makes it difficult to isolate compact sin gle crystals. Energy-dispersive X-ray fluorescence analy ses of the samples resulted in atomic ratios Ag:Hg varying between 0.957:2.043 and 1.011:1.989, in good agreement with the ideal ratio of 1:2. No impurity elements heavier than sodium could be detected. Structure Determination A single-crystal of AgHg^NOj with dimensions 20x 20x 100 /./nr was selected for the structure deter mination on the basis of Laue patterns. It was investi gated with an Enraf-Nonius CAD4 diffractometer using graphite-monochromated MoKa radiation and a scintil lation counter with pulse-hight discrimination. The soft ware assigned orthorhombic symmetry with the cell di mensions a = 619.63(6) pm, b = 669.59(10) pm, c = 1265.48(8) pm, V = 0.5251 nm3. These agree reason ably well with the lattice constants obtained from a leastsquares fit of CuKo 1 Guinier powder data using a-quartz (a = 491.30 pm, c = 540.46 pm) as an internal standard: a = 620.1(1) pm. b = 670.1(1) pm. c = 1267.5(2) pm, V = 0.5267 nm3. We consider the latter to be more ac curate, because the lattice constants from the four-circle Th. J. Mormann and W. Jeitschko • A Silver(I) Mercury(II) Oxide Nitrate Ag: 03 02 201 03 Hg: 03 02 01 01 02 04 04 224.6(10) N: 238.1(10) 247.8(9) 277.7(11) 201.9(6) O l: 202.3(6) 277.0(9) 283.5(8) 292.5(8) 293.3(11) 329.3(11) 201 04 04 02 N Ag Hg Hg 124.0(11) 0 2 : 124.5(17) 290.1(19) 297.4(16) 124.0(11) 03: 247.8(9) 277.0(9) 283.5(8) 04: 2Hg Ag 2Hg N 2Hg Ag Ag N N 2Hg 2Hg 202.3(6) 238.1(10) 292.5(8) 297.4(16) 201.9(6) 224.6(10) 277.7(11) 124.5(17) 290.1(19) 293.3(11) 329.3(11) 1491 Table II. Interatomic distances of AgHg2N05, calculated with the lattice constants obtained from the Guinier powder data. All distances shorter than 333 pm are listed. whole reciprocal sphere. An absorption correction was made on the basis of psi scan data. After data averaging for the Laue symmetry nimm 1228 unique reflections were obtained (internal residual for F2 values = 0.080). The structure was determined and refined with the pro gram package SHELX-97 [26]. The positions of the heavy atoms were obtained from a Patterson synthesis, the other positions were located by difference Fourier syntheses. For the structure refinement a full-matrix least-squares program was used with atomic scattering factors, cor rected for anomalous dispersion, as provided by the pro gram. The structure was refined in the space group Pnma (No. 62), the one with the highest symmetry compatible with the space group extinctions. There are Z = 4 formula units in the cell. The calculated density is 7.61 g em-3 . In the final refinement cycles anisotropic displacement pa rameters were used for the metal atoms; the light atoms were refined with isotropic displacement parameters. The final conventional residual is R = 0.026 for 586 structure factors greater than 2 standard deviations. A weighted residual of Rw = 0.064 was obtained for all 1228 unique F2 values. The highest and lowest residual electron den sities are 1.8 and -2.2 e-A-3 , respectively. The atomic parameters and interatomic distances are listed in the Ta bles I and II. Discussion Fig. 1. Near-neighbor coordinations in AgHgaNOs. The thermal ellipsoids of the metal atoms are drawn at the 95 % probability limit. The sizes of the other atoms are not representative of their displacement parameters. For the atoms with labels all neighbors as listed in Table II are shown. diffractometer are affected be systematic errors due to absorption. The intensity data were collected with 0/20 scans and background counts on both ends of each scan. A total of 6136 reflections was collected up to 20 = 70° in the The crystal structure of AgHg 2NC>5 may be rep resented by the formula AgN 0 3 -2 Hg 0 , thus in dicating the oxidation number +1 and +2 for the silver and mercury atoms, respectively. The sil ver atoms have coordination number (CN) 5 with four close oxygen neighbors (at distances between 224.6 and 247.8 pm) forming the transition be tween tetrahedral and square-planar coordination. The O-Ag-O angles of 2x82.9°, 2 x 106.9°, 135.3°, and 149.2° are in between 6x109.5° (tetrahedral) and 4x 9 0 ° and 2x180° (square-planar). The fifth 1492 Th. J. Mormann and W. Jeitschko • A Silver(I) Mercury(II) Oxide Nitrate Fig. 2. Crystal structure o f A gH g 2 N 0 5 . The structure consists o f two- dimensionally infinite lay ers, which are emphazised. At the top only the mercury and their strongly bonded oxygen neighbors are shown. In the next two layers below, the silver atoms and then the nitrate groups are added. Weak secondary metal-oxygen bonds (all greater than 276 pm) are shown be tween the lowest two layers. At the bottom one layer is view ed in a di rection perpendicular to the layer. oxygen neighbor at the somewhat larger Ag-O dis tance of 277.7 pm is situated approximately on the pseudo-fourfold axis (Fig. 1). The average Ag-O distance of 247.2 pm is in excellent agreement with that of 245 pm calculated from the radii given by Shannon for five-coordinated Ag+1 [27], especially if one considers the considerable spread of Ag-O distances in the present compound. The mercury atoms of AgHg2NOs are in approx imately linear oxygen coordination with an O-HgO angle of 177.5(4)°. This linear coordination is most frequently found for Hg+2. The corresponding two H g-0 distances of 201.9(6) and 202.3(6) pm agree well with the H g(II)-0 distances of 203(2) and the average of 205(3) pm for the trigonal [2] and orthorhombic [3] modifications of HgO, re spectively, 202.6(4) pm in HgMoÜ 4 [28], 205(2) pm in Hg5Re20io(I) [29], 201(2) and 203(2) pm in Hg5Re20io(II) [30], as well as the Hg-O distances of 201.0(8) and 202.9(8) pm for the Hg(II) atoms in Hg2Re05 [31]. In all of these compounds the Hg(II) atoms have additional oxygen neighbors sit uated close to a plane perpendicular to the short H g-0 bonds. For the HG(II) atoms in AgHg 2NOs there are five oxygen neighbors at distances ranging between 277.0(9) and 329.3(11) pm. The nitrate groups are practically planar with ON -0 angles of 117.3(1.4)° and 121.3(7)° (2 x ). The N -0 distances of 2 x 124.0( 11) and 124.5( 17) pm are nearly equal. Disregarding the practically nonbond- Th. J. Mormann and W. Jeitschko • A Silver(I) Mercury(II) Oxide Nitrate ing N-O distances of 290 and 297 pm, the oxygen atoms have four or five near neighbors of which some are only weakly bonding (Table II). As already mentioned above, AgHg 2 NOs shows some tendency for cleavage, and indeed the struc ture may be described as consisting of layers which contain all of the strong bonds. This is shown in Fig. 2, produced with the aid of the program DIA MOND [32]. In the top of that figure the mercury atoms of one layer are shown together with their strongly bonded 0 2 and 0 3 atoms, forming O-HgO-Hg zig-zag chains. In the next layer below these chains are linked to each other via the silver atoms of the same layer. Further below, in the third layer from the top we have added the nitrate groups. And fi nally between the next two layers we show the weak Ag-O and Hg-O bonds of 278, 277, and 293 pm, re spectively. A view of one layer perpendicular to its plane is shown at the bottom of Fig. 2. It can be seen that the oxygen atoms of the nitrate group do not form very strong bonds to the silver or mercury atoms, although each nitrate group clearly belongs predominantly only to one Ag(HgO )2 layer. Hence, [1] P. Laruelle, C. R. Acad. Sei. Paris 241, 802 (1955). [2] K. Aurivillius, I.-B. Carlsson, Acta Chem. Scand. 12, 1297 (1958). [3] K. Aurivillius, Acta Chem. Scand. 18, 1305 (1964). [4] Gmelins Handbuch der Anorganischen Chemie, 8. Auflage, System-Nummer 34: Quecksilber Bl (1965). [5] P. Niggli, Z. Kristallogr. 57, 253 (1922). [6] R. W. G. Wyckoff, Am. J. Sei. 3, 184 (1922). [7] W. Beesk, P. G. Jones, H. Rumpel, E. Schwarzmann, G. M. Sheldrick, J. Chem. Soc., Chem. Comm. 1981, 664(1981). [8] J. A. McMillan, J. Inorg. Nucl. Chem. 13, 28 (1960). [9] V. Scatturin, P. L. Bellon, A. J. Salkind, J. Electrochem. Soc. 108, 819 (1961). [10] M. Jansen, P. Fischer, J. Less-Comm. Met. 137, 123 (1988). 1493 the structure can also be represented by the formula A g(H g0) 2 N03. The structure of AgHgoNOs shows some sim ilarity to the structures of (Hg 0 )2 Hg(N 0 3 ) 2 [15], (Hg 0 )2 Hg 2 (N 0 3 )2 [16, 17], and Hg 2 R e 0 5 [31]. In all of these four structures the Hg(II) atoms form zig-zag chains which are parallel to each other. These chains are linked via Ag or Hg atoms or Hg(I)-Hg(I) pairs, thus forming two-dimensionally infinite nets of the compositions AgHg 2 0 2, Hg 3 0 2, and two times Hg 4 0 2 in the four compounds, re spectively. Acknowledgements We thank Mrs. U. Ch. Rodewald and Mr. K. Wagner for the competent collection of the intensity data at the four-circle diffractometer and the work at the scanning electron microscope. We are also indebted to the Heraeus Quarzschmelze for a generous gift of silica tubes. This work was further supported by the Fonds der Chemischen Industrie and by the International Centre for Diffraction Data. [11] N. E. Brese, M. O’Keeffe, B. L. Ramakrishna, R. B. von Dreele, J. Solid State Chem. 89, 184 (1990). [12] K. Yvon, A. Bezinge, P. Tissot, P. Fischer, J. Solid State Chem. 65, 225 (1986); see also J. Solid State Chem. 68, 380(1987). [13] B. Standke, M. Jansen, J. Solid State Chem. 67, 278 (1987). [14] B. Standke, M. Jansen, Z. Anorg. Allg. Chem. 535, 39(1986). [15] H. Behm, Acta Crystallogr. C39, 1319(1983). [16] K. Brodersen, G. Liehr, G. Schottner, Z. Anorg. Allg. Chem. 531, 158 (1985). v [17] B. Kamenar, D. Matokovic-Calogovic, A. Nagl, Acta Crystallogr. C42, 385 (1986). [18] A. Niggli, Z. Kristallogr. 111, 269 (1959). [19] P. F. Lindley, P. Woodward, J. Chem. Soc. A, 123 (1966). 1494 Th. J. Mormann and W. Jeitschko • A Silver(I) Mercury(II) Oxide Nitrate [20] P. Meyer, A. Rimsky, R. Chevalier, Acta Crystallogr. B34, 1457 (1978). [21] P Meyer, J.-J. Capponi, Acta Crystallogr. B38. 2543 (1982). [22] P. Meyer, A. Rimsky. R. Chevalier, Acta Crystallogr. B32, 1143 (1976). [23] C. H. Wong, T. H. Lu, C. N. Chen, T. J. Lee, J. Inorg. Nucl.Chem. 34, 3253 (1972). [24] M. Jansen, U. Bilow, J. Alloys Compd. 183, 45 (1992). [25] Th. Mormann, W. Jeitschko, Bull. Czech. Slovak. Crystallogr. Assn. 5, 372 (1998). [26] G. M. Sheldrick, SHELX-97, A Program System for the Solution and Refinement of Crystal Structures, Universität Göttingen, Germany (1997). [27] R. D. Shannon, Acta Crystallogr. A32, 751 (1976). [28] W. Jeitschko, A. W. Sleight, Acta Crystallogr. B29, 869(1973). [29] J.-P Picard, G. Baud, J.-P. Besse, R. Chevalier, M. Gasperin, Acta Crystallogr. B38, 2242 (1982). [30] M. S. Schriewer-Pöttgen, W. Jeitschko, Z. Naturforsch. 50b, 1335 (1995). [31] M. S. Schriewer-Pöttgen, W. Jeitschko, Z. Anorg. Allg. Chem. 620, 1855 (1994). [32] K. Brandenburg, M. Berndt, DIAMOND, visuelles Informationssystem für Kristallstrukturen, Version 2.1, Universität Bonn, Germany (1999).
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