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Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..545v&link_type=abstract
European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a
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Scientific paper
Introduction. The response of carbonate to impact processes has thus far been investigated using a combination of thermodynamic modelling, shock experiments, and impact experiments. Localized shear deformation was suggested to play an important role in the failure of carbonate during some shock experiments [1,2], and was invoked to explain significant degassing of carbonates during oblique impact experiments [3]. The results of the impact experiments are at odds with experiments [4] that show back-reaction of CO2 with CaO and MgO could significantly reduce CO2 degassing during impact events. We performed a frictional-welding experiment in order to investigate the effects of high strain-rate deformation on carbonate-silicate target materials, exclusive of shock deformation effects, and to investigate the differing results of other experiments. Samples and Techniques. A frictional melting experiment was performed using dolomitic marble and quartzite samples to simulate conditions during an impact into carbonate-silicate target rocks. The experiment followed the method of Spray (1995) [5]. The 1.5 cm3 samples were mounted onto separate steel cylinders with epoxy. Using a Blacks FWH-3 axial friction-welding rig, the samples were brought into contact at room temperature and under dry conditions with ~5 MPa applied pressure. Contact was maintained for two seconds at 750 rpm for a sustained strain-rate of 102 to 103 s-1. Results. Vapor or fine dust escaped from the interface during the experiment. Immediately after sample separation, the interfaces were incandescent. Once cooled, opaque white material adhered to both the quartzite and dolomitic marble samples. Quartzite sample. Material was injected into cracks that formed in the quartzite sample. Cooling and crystallization of the friction products resulted in the formation of submicron-sized minerals such as periclase and Ca- and Ca,Mg-silicates (Fig. 1) including merwinite and åkermanite. While periclase was observed as an individual mineral species, no pure lime was observed to be present. In the quartzite sample, CaO is present only as a component of the Ca- and Ca,Mg-silicates. In the fine-grained shear zone materials, however, elemental mapping and EMP analyses reveal an overall segregation of MgO and CaO [6], suggesting that CaO is mostly present in Casilicates and Ca,Mg-silicates with low MgO contents. Dolomitic marble sample. The dolomitic marble section exhibited thinner, shorter fractures than the quartzite sample. Mechanical twinning was induced by the deformation. The adhered friction products were very fine-grained material with larger, untwinned calcite (Fig. 2), and dendritic carbonates with a composition similar to huntite. Most of the secondary calcite had rounded margins, which suggested that they were molten during the experiment. The dendritic huntite-like carbonate, with a CO2 content higher than of these secondary carbonate grains (Fig. 3). However, calcite was the dominant secondary mineral. The finegrained portion of the shear zone material contained pervasive vesicles. The vesicles immediately adjacent to the secondary calcite grains were smaller than those adjacent to the dolomitic marble. This suggests that incorporation of CO2 near the calcite grains facilitated their growth. Discussion. The textures and compositions of the experimental products indicate that the dolomitic marble decarbonated in response to the high temperatures generated during experimental deformation. Simultaneously, the liberated CaO recombined with CO2 to form molten calcite in the shear zone. This effect, in part, is due to the lower decarbonation temperature for dolomite versus calcite [c.f., 7], which allows calcite to survive at higher temperatures than dolomite. In addition, the confining pressure during the experiment was high enough to allow calcite to be present as a liquid [c.f., 8]. Both the calcite and dendritic carbonate are likely products of back-reaction of CaO and MgO with CO2. However, both CaO and MgO were also incorporated into secondary silicates, which reduced the total amount available to back-react with CO2. It appears that all CaO released from the dolomitic marble formed secondary minerals (carbonates and silicates), because it is not present as pure CaO. The MgO released from the dolomitic marble primarily formed secondary silicates, periclase, and minor secondary carbonate. As a result, the secondary carbonates cannot be a sink for all the CO2 gas released from the dolomitic marble, unless a much higher proportion of the huntite-like phase was present. Thus, there was a net release of CO2 gas from the original dolomitic marble. A portion of this CO2 remained trapped in vesicles, but CO2 gas also escaped from the shear zone. This is consistent with compositional measurements of the shear zone that suggest a release of at least 5 wt% CO2 relative to the original dolomitic marble. Comparison with terrestrial craters. Many of the descriptions of deformation features in carbonates at terrestrial craters, such as mechanical twinning and bent fractures [9-11], are similar to those seen in our experimental products. Carbonates that survive impact seem to accommodate both shock and shear deformation primarily through mechanical fracturing and twinning. Impact melts at craters in carbonate-rich targets have been found to contain both silicic and carbonatitic melts [e.g., 12], with mineral phases that are indicative of high temperature reactions between carbonate and silicate rocks [e.g., 9]. Our experiments also showed these characteristics, however, the mineral phases produced were slightly different and we have not observed silicate glass in our experimental products. The segregation of MgO from CaO has been observed, for example, at Haughton [12] and Popigai [13], and was also seen in our experimental products [6]. Implications. The products of high strain-rate deformation experiments with carbonate-silicate rocks are similar in many aspects to impact products at terrestrial craters in mixed carbonate-silicate targets. The experiments show that decarbonation of carbonate targets and high temperature reactions between carbonate and silicates in the target rocks are not exclusive effects of shock deformation. Shear deformation alone can generate temperature and pressure conditions necessary to decarbonate dolomitic marble and generate calcitic melts. Thus, high strain-rate deformation is a potentially major contributor to the total impact-related energy deposited into the target, especially for oblique impacts. Shear deformation occuring during and after shock deformation could, in fact, enhance the release of CO2 as a gas, by creating pathways that allow gases to escape from target materials. Understanding the relative importance and interaction of each CO2 releasing or trapping mechanism is important for the determination of the environmental significance of impacts in targets containing carbonates. References. [1] Lange M. A. and Ahrens T. J. (1986) EPSL 77, 409-418. [2] Tyburczy J. A. and Ahrens T. J. (1986) JGR 91, 4730-4744. [3] Schultz P. H. (1996) GSA Abstracts, A384. [4] Agrinier P., et al. (2001) GCA 65, 2615-2632. [5] Spray J. G. (1995) Geology 23, 1119-1122. [6] van der Bogert C. H., et al. (2007) LPI Contribution No. 1360, 123-124. [7] Martinez I., et al. (1995) JGR 100, 15456-15476. [8] Ivanov B. A. and Deutsch A. (2002) Phys. Earth Planet. Int. 129, 131-143. [9] Martinez I., et al. (1994) EPSL 121, 559-574. [10] Redeker H.-J. and Stöffler D. (1988) Meteoritics 23, 185-196. [11] Skála R. and Jakes P. (1999). In Large Meteorite Impacts and Planetary Evolution II (eds. B. O. Dressler and V. L. Sharpton), pp. 205-214. [12] Osinski G. R. and Spray J. G. (2001) EPSL 194, 17-29. [13] Kenkmann T., et al. (1999) LPS XXX, Abstract #1561.
Schultz Peter H.
Spray John G.
van der Bogert Carolyn H.
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