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Evidence of screw dislocation on gypsum crystals as principal mechanism of growth at low supersaturation

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Evidence of Screw Dislocation on Gypsum as Principal Mechanism of Growth at Low Supersaturation

Joaquín Criado Reyesa, Fermín Otálora Muñoza, Linda Pasterob, Dino Aquilanob and Juan Manuel García Ruiza*

aLaboratorio de Estudios Cristalográficos, IACT, UGR-CSIC, Granada (Spain) bDipatamento di Szience della Terra, Università degli Studi di Torino, Torino (Italy)

Gypsum mineral mainly occurs on evaporitic environment around the world [1, 2]. It has also been reported as a relevant phase in Mars [3-5]. The growth conditions during the growth of gypsum crystals influences the surface growth mechanisms and the habit. Many authors suggest that the growth mechanisms of gypsum crystals at low supersaturation is due to dislocation growth, these studies are based on kinetic data fitted to theoretical equations[6, 7]. However, the observation of hillocks on the surface gypsum crystals has been challenging. A couple of studies on the cleavage face (010) of gypsum by Atomic Force Microscopy (AFM) and Differential Interface Contrast Microscopy (DICM) shown some hillock but only one of them could be clearly identified as a screw dislocation, so the authors conclude that the main growth mechanism at low supersturation on this face is by 2D nucleation[8, 9]. Equivalent studies on the (120) face are missing, mainly due to the roughness of these faces. In a preliminary study of the gypsum (120) face using crystals growing by evaporation, we observed that hillocks spread on (120) at low supersaturation. Those hillocks are made by monolayers with a height of 4.30 Å corresponding to the d-spacing. These hillocks show an asymmetric morphology (figure 1).

Figure 1: Hillock of a spiral growing on (120) face of gypsum crystal. Screw dislocation is the origin of the growth.

1. Krüger, Y., et al., Determining gypsum growth temperatures using monophase fluid inclusions—

Application to the giant gypsum crystals of Naica, Mexico. Geology, 2013. 41(2): p. 119-122.

2. Van Driessche, A.E.S., et al., Ultraslow growth rates of giant gypsum crystals. Proceedings of the National Academy of Sciences, 2011. 108(38): p. 15721-15726.

3. Elwood Madden, M.E., R.J. Bodnar, and J.D. Rimstidt, Jarosite as an indicator of water-limited

chemical weathering on Mars. Nature, 2004. 431: p. 821.

4. Gendrin, A., et al., Sulfates in Martian Layered Terrains: The OMEGA/Mars Express View. Science, 2005. 307(5715): p. 1587-1591.

5. Nachon, M., et al., Calcium sulfate veins characterized by ChemCam/Curiosity at Gale crater,

Mars. Journal of Geophysical Research: Planets, 2014. 119(9): p. 1991-2016.

6. Christoffersen, M.R.C.A.J., Crystal Growth Of Calcium Sulphate Dihydrate Atlow

Supersaturation. Journal of Crystal Growth, 1982. 58: p. 10.

7. G.M. Van Rosmalen, P.J.D.A.W.G.J.M., An Analysis Ofgrowth Experiments Of Gypsum Crystals In

Suspension. Journal of Crystal Growth, 1981. 52: p. 11.

8. Van Driessche, A.E.S., et al., In Situ Observation of Step Dynamics on Gypsum Crystals. Crystal Growth & Design, 2010. 10(9): p. 3909-3916.

[ 43.4 mV ] 98.8 mV Error Signal 3.0 0 µm 3.00 µm 20.0 40.0 60.0 80.0 mV rel. [001] [2-11]

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9. Mbogoro, M.M., et al., Intrinsic Kinetics of Gypsum and Calcium Sulfate Anhydrite Dissolution:

Surface Selective Studies under Hydrodynamic Control and the Effect of Additives. The Journal of

Riferimenti

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