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Materials 2014, 7(4), 3319-3336; doi:10.3390/ma7043319
Published: 24 April 2014
Abstract: X-ray micro-computer aided tomography (μ-CT), together with optical microscopy and imaging, have been applied to the study of six moldavite samples. These techniques enabled a complete characterization to be made of the textural features of both Muong Nong-type and common splashform moldavites. A detailed study of the size and distribution of pores or bubbles confirmed the marked variability in pore size among the samples, as well as within each sample, and indicated in the Muong Nong-type moldavites the presence of at least two deformation stages which occurred before and after pore formation.
Tektites are natural acid silicate glasses that occur in geographically limited areas, so-called strewn fields. They differ from common volcanic glasses in both chemical and physical properties . Their characteristic features include high silica and very low water content, the presence of lechatelierite (amorphous SiO2) particles, and a low Fe3+/(Fe2+ + Fe3+) ratio [2–8]. Tektites are today generally considered to be products of hypervelocity impacts on Earth; usually they experienced aerodynamic transport and can be deposited at great distances (up to several hundred kilometers) from the presumed source crater. Generally, several morphologically different types of tektites may be recognized: (i) most common are the splashform tektites, found in each of the known strewn fields; (ii) aerodynamically shaped tektites are button-like objects occurring exclusively in Australia; (iii) micro-tektites; and (iv) Muong Nong-type tektites (the rarest type). The Muong Nong-type tektites are named after the city of Muong Nong in Laos where they were first described by Lacroix . Typical features of the archetype Muong Nong-type tektites include blocky shape, highly variable size and weight, layered structure, high content of crystalline inclusions [10–12] and high porosity. Chemical characteristics that distinguish the Muong Nong-type tektites from splashform counterparts include an overall chemical heterogeneity, high volatile trace element abundances  and high water content [14,15].
Moldavites (aka Central European Tektites; CET) are thought to represent distal ejecta formed during the impact event that produced the 24-km diameter Ries crater in Germany. They have been found at distances of 200 km to 450 km from the point of impact in the Czech Republic , Austria , and Germany . The chemical, physical, and morphological properties of moldavites, as well as the data on their geographical distribution, have been reported in numerous papers and books, e.g., [19–29]. Although the link between the Ries crater and moldavites has been generally accepted [26,30–32], the exact formation process and source materials remain a matter of debate [13,27,33–40]. The age of moldavites, as the age of the Ries crater, has been the subject of numerous papers [41–43]. Most recently, Di Vincenzo and Skála  and Buchner et al.  concluded that the age of moldavites and the Ries structure is 14.68 ± 0.11 Ma and 14.59 ± 0.20 Ma, respectively.
Although the vast majority of moldavites are of the splashform type, some authors [46–49] have described Muong Nong–type moldavites from the South Bohemian partial strewn field. The Muong Nong-type moldavites, contrary to the generally larger and considerably blocky Muong Nong-type tektites from Asia, are of much smaller size, similar to splashform moldavites. In some rare cases, some Muong Nong-type moldavites consist of two types of glass, porous and compact, resulting in a layered appearance, which is considered the typical feature of Asian Muong Nong-type tektites. In most cases, however, only the porous layer of a Muong Nong-type moldavite is preserved separately. This highly specific type of moldavite also displays high structural heterogeneity with high content of lechatelierite inclusions, high pore density, and substantial chemical heterogeneity. Since the Muong Nong-type tektites, in general, may carry important information on the tektite-forming process , we decided to characterize the internal structure of four Muong Nong-type moldavites and compare the pore features and the porosity degree with that of two splashform moldavites. We used X-ray micro-computer aided tomography (μ-CT) to extract the 3D pore features on representative portions (about 400–500 mm3) of the samples. This is a relatively new technique allowing the accurate evaluation of the size, shape and distribution of different features of a sample characterized by different X-ray absorption coefficients; in this particular case the micro- and macro-pores or bubbles of the tektites. Since Ketcham and Carlson  first proposed the use of μ-CT to extract 3D features of geological materials, many researchers in the field have applied this technique using either synchrotron or laboratory X-ray sources [51,52]. The technique has also been shown to be a useful tool to study meteorites , especially chondrites. The texture and distribution of mineral phases [54–57], the shape of chondrules , the distribution of pores [59–61], and the different mineralogical phase distribution of chondrites were investigated in order to assess the technique as a possible non-destructive tool for the classification of ordinary chondrites . The technique of μ-CT has also been successfully applied to the study of other planetary related materials, such as the Stardust impact tracks [63,64], the silicate inclusions in meteoritic chromite grains  and splashform moldavites .
2. Materials and Methods
A total of six moldavite samples from the South Bohemian substrewn field (Czech Republic) were selected to be investigated by X-ray micro-computer aided tomography and polarized light microscopy. In particular, the samples Chlum 1 and Chlum 2 (splashform moldavites, chips of about 6 mm × 5 mm × 3 mm) originate from a locality near the village of Chlum nad Malší, 7 km NNE of Kaplice (48°48′2.049″ N, 14°30′52.602″ E), and the four Muong Nong-type moldavite samples (Nos. 2, 7, 8, 23, slices of about 10 mm × 10 mm × 0.8 mm) originate from the village of Slávče, 5 km WSW of Trhové Sviny (48°48′10.887″ N, 14°37′5.851″ E; Figure 1).
2.2. X-ray Micro Computer Aided Tomography (μ-CT) and 3D Data Extraction
Micro-CT data were collected using a Skyscan 1172 high-resolution MicroCT system at the University of Florence (CRIST). This system has a sealed, microfocus tungsten X-ray tube with a 5 μm focal spot size operating at 100 kV, 100 μA, and a 11 Mpixel detector panel with a 16 bit pixel depth. The sample was placed on the pedestal between the X-ray source and the CCD detector, recording the 2D X-ray images by rotating the sample 180° with a slice-to-slice rotation angle of 0.2°. In this way, nine hundred 2D images were recorded for each sample. The total acquisition time was approximately 40 min. Spatial resolution of the single tomogram was kept in a range of 5–10 μm in terms of pixel size, giving a corresponding voxel resolution range between 125 and 1000 μm3.
The 3D image of the object’s internal structure was reconstructed using a modified Feldkamp algorithm for cone-beam acquisition geometry realized in Nrecon v.126.96.36.199 software (Bruker-MicroCT, Kontich, Belgium). The final images were reduced to 8 bit pixel depth. The alignment, beam-hardening and ring artifact corrections were made before starting the reconstruction process.
Morphometric parameters were calculated in 3D on a surface-rendered volume model by using CT-analyzer software v.1.11 (Bruker-MicroCT, Kontich, Belgium). In particular, all calculations were performed on segmented images over selected volumes of interest (VOI) within the tektites. The total volume, density and surface of the pores inside the tektites were calculated on the marching cubes volume model of the pores binarized as solid objects, inside the selected volumes of interest. Average pore diameter was evaluated using the definition of the local thickness for a point within a solid given by Hildebrand and Rüegsegger , which is the diameter of the largest sphere that fulfills two conditions: the sphere encloses the point (but the point is not necessarily the center of the sphere) and the sphere is entirely bounded within the solid surfaces (Figure 2).
In this way the calculated average pore diameter is independent of the object shape. The method that the CT-analyzer uses starts with a “skeletonization” identifying the medial axes of all structures. Then the “sphere-fitting” local thickness measurement is made for all the voxels lying along this axis. The average pore size was larger than the effective pixel size in micro-CT reconstruction and larger than the spot size of the X-ray source.
The visualization of the 3D CT images was created using a model built with a marching cubes 33 algorithm; surface-rendered 3D model of the whole object and the pores were loaded with CT-Vol v.2.1 software (Bruker-MicroCT, Kontich, Belgium). The images of the whole tektites were colored and shown as gray solids or, alternatively, colored images of solid pores were overlaid with the tektites VOI to visualize the pore distribution inside the tektites. All the images were smoothed with the Skyscan software (Bruker-MicroCT, Kontich, Belgium).
2.3. Polarized Light Microscopy
To complement the characterization of the moldavite texture obtained through μ-CT analysis, particularly to retrieve information on strain that cannot be revealed by X-ray tomography, optical microscopy and imaging were performed at the laboratories of the Museo di Scienze Planetarie (Prato) by means of an Axioplan-2 polarizing optical microscope equipped with Axiocam-HR camera and Axiovision 4.1 software (Carl Zeiss Microscopy GmbH, Jena, Germany).
Figure 3A shows a typical X-ray transmission image of a tektite (sample No. 2), located in the microCT sample holder. In this case, pixels of material that have a large X-ray attenuation are dark, whereas pores characterized by lower X-ray attenuation are detectable as light gray spots.
A pre-analysis was made after reconstructing a dataset of each sample, loading it into DataViewer and checking for abnormalities or irregularities that may have occurred during image reconstruction. Three-dimensional portions of materials (VOI, volume of interest) were chosen with the objective of selecting as much volume as possible, avoiding the portions affected by unavoidable irregularities, i.e., beam hardening effect or other artifacts.
The VOI was selected to enable a statistical analysis of the pore size distribution and number to be made. This procedure also allows the largest possible portion of the sample to be selected, but avoids the edges where beam hardening or ring artifacts could lead to misevaluation of the pores. In order to compare the data of samples of different sizes, all the morphometric parameters were normalized with respect to the relative VOI. Tomographic slices, obtained after data reduction and artifact removal on a selected portion (VOI) of the same sample, and are also displayed in Figure 3B. In this case, pixels of material showing a large X-ray attenuation are light gray, whereas pores characterized by lower X-ray attenuation are detectable as dark spots. At each 3D location (shown at the cross-hairs), three orthogonal views are retrieved from the whole dataset as shown:
transaxial view (the normal images, in x-y plane), (B1);
coronal view (x-z plane), (B2);
sagittal view (z-y plane). (B3) Sub-millimeter sized pores, characterized by sharp edges, are clearly detectable in all the images.
Figure 4 displays the isosurface 3D reconstructions of the tektite surface (left) and their pores (right). In particular, the figure displays the three-dimensional distribution of pores (in orange) across the volume of interest (VOI). It is clear that the Muong Nong-type moldavites studied in this work display larger and more numerous pores compared to the splashform samples (Chlum 1 and Chlum 2). Although pores of larger size have been observed in other spashform-like moldavites , the total porosity of these samples was always lower than those of Muong Nong, suggesting that higher porosity levels must be considered a peculiar feature of the Muong Nong-like.
Figure 5 plots the porosity (volume% of pores) determined for the six studied samples. Among the Muong Nong-type moldavites, sample 7 shows the lowest degree of porosity, well below 1%, the other samples are characterized by much larger values up to more than 4% (sample No. 8). In agreement with previous reports , splashform moldavites were found to have very low porosity, as exemplified by Chlum 1 (0.011%) and Chlum 2 (0.006%). Substantial differences were observed in the average number of pores per mm3 (Figure 6). Muong Nong-type moldavite sample No. 7, even though characterized by a low overall porosity, has a very high number of pores, about 100/mm3, similar to the more porous samples No. 2 and 8. Clearly, sample No. 7 contains a large number of very tiny pores, which is highlighted below. Unusual features were also detected for the samples No. 23 and Chlum 1; despite their very different degree of porosity, both display only a relatively low number of pores (about 10/mm3). That is due to the pronounced difference in pore size; tiny pores in Chlum 1 (splashform-type) and much larger pores in No. 23 (Muong Nong-type). The pore size differences are also highlighted in Figure 7, where the average pore size is plotted versus the number of detected pores. Sample No. 23 and Chlum 1 display the largest and smallest average pore size, respectively.
Another useful parameter that provides quantitative information on the type of pores present is the pore surface. It has been calculated as the total surface of closed pores with respect to the VOI volume (Figure 6B). Since only pores that are not intersected by the VOI surfaces (closed pores) were taken into account for the evaluation of pore surface, the values obtained are underestimated for all the samples. Nevertheless, a statistical qualitative indication of the pore shape can be achieved by evaluating the calculated pore surface as a function of the number of closed pores. Small or irregular pores result in a larger calculated pore surface, whereas spherical or subspherical pores translate into smaller values of pore surface. It is interesting to note that sample No. 8 shows the highest value, whereas sample No. 2 is characterized by a much lower surface, about 9 × 10−3 mm2/mm3. Considering that the number of pores is nearly the same for these two samples, it is evident that the pores present in sample No. 8 are larger and less spherical than those present in sample No. 2.
The pore size distribution is shown in Figure 8. The histograms clearly illustrate that there is a large range of pore size distribution among the investigated samples. The largest pores in the splashform moldavites Chlum 1 and Chlum 2 do not exceed 100 μm; the largest pores in the Muong Nong-type moldavite No. 7 do not exceed 150 μm and the largest pores overall are found in sample No. 23 reaching 500 μm. Sample No. 8 is characterized by a large number of large pores, i.e., almost 20% of the pores show diameters between 300 and 350 μm. Table 1 summarizes the data extracted from the porosity analysis.
The studied moldavites also differ on a macroscopic scale. The two splashform moldavites are transparent or translucent, green colored, and rather compact; whereas those of the Muong Nong-type are translucent on the edges only, display generally much darker colors, seem to be composed of various domains (sometimes layer-like), and contain an appreciable amount of pores and pits that possibly represent open pores.
In thin sections, both types are more or less transparent, lightly yellow, yellow-green or yellow-brown colored. The main difference is the presence of at least two intercalated or interwoven melts differing in color and abundance of lechatelierite inclusions and frequency of pores in Muong Nong-type moldavites (see Figures 9 and 10). On the contrary, the splashform moldavites tend to be rather homogeneous. Glass domains in Muong Nong-type moldavites usually form schlieren of various shapes and widths. Furthermore, their pores have very variable sizes and shapes. It is also quite common that individual variably-sized pores aggregate into larger clusters. Between crossed polarizers moldavite glass displays anomalous behavior showing local strong birefringence (Figure 9). Birefringent domains usually occur close to or along the schlieren or lechatelierite inclusions and pores; they are much more frequent in Muong Nong-type moldavites than splashforms.
The application of X-ray micro-computer aided tomography has allowed a statistical analysis to be conducted with high spatial and contrast resolution of a large number of pores of different sizes present inside six moldavite samples on large and representative portions of the samples (about 400–500 mm2). The moldavite samples investigated in this study show highly variable pore content and distribution (Figures 4 and 5), as well as considerable differences in pore shape (Figure 6). The pore sizes display a general trend: the amount of porosity correlates to larger pore sizes (e.g., samples No. 7, Chlum 1 and Chlum 2 show few, small pores). Conversely, in samples No. 8 and No. 23, that have the highest porosity, the pores reach the largest sizes (Figures 4, 5, 7 and 8). This trend is evident from the diagram in Figure 7.
Matsuda et al.  argued that pores formed as a result of gas expansion inside the glass, without being followed by deformation processes, should be spherical. The tomography images (Figure 3) as well as optical images (Figures 9 and 10) show that in the moldavite samples studied many pores, in particular the largest ones, are not spherical. This suggests that a further deformation of moldavites occurred after pore formation.
It is also important to note the mutual relationship among the pores of the schlieren and residual strain. According to Engelhardt and coworkers , each individual moldavite body represents a population of chemically different primary units. The schlieren texture, in the moldavite samples, may represent two subsequent rheological regimes that can be distinguished during the cooling of moldavite bodies, when the temperature is too low to allow mixing. Fluid particles of different composition and viscosity may be extended into thin lamellae in a stress field of laminar flow. At lower temperatures, these arrays were subsequently plastically deformed (also under conditions of compressional stress), probably concomitant with the shaping of individual moldavite bodies .
Neither schlieren nor strain can be revealed by X-ray tomography. Consequently, polarized light microscopy was used to observe these features. As reported by Majmundar and O’Keefe , the tektites display an overall strain pattern as well as that associated with the notches. The strain pattern corresponds to that expected for bodies which were rapidly cooled and, therefore, shows differences between the outer and the inner portions of the bodies: compressional strain in a tangential direction and tensional in the radial direction. Moreover the anomalous strain-induced birefringence may enhance textures connected with the laminar flow as well as those related to plastic deformation. The strain-induced birefringence images of the moldavites are shown in Figure 9. They demonstrate a marked difference among the individual investigated samples, although the strain generally seems to be directly proportional to the porosity. Another interesting feature revealed by Figure 9 is the prevalence of laminar and chaotic flow. The laminar texture is most developed in sample No. 7, whereas it is less apparent in the other samples. On the contrary, significant chaotic flow fabric is evident in sample No. 8. In general, the Muong Nong-type moldavites display more pronounced birefringence, possibly illustrating the presence of much more heterogeneous strain patterns due to considerably higher heterogeneity compared to the splashform moldavites.
The distribution of pores is generally irregular. In most cases, the pores lack any obvious preferential alignment with respect to flow textures. Only locally, the pores seem to be concentrated along the schlieren.
Most of the pores are spherically shaped, however, in sample No. 7 and No. 23 certain pores of different sizes, including the smallest ones, are elongated (Figure 10). It should be noted that elongation axes of the pores in these samples differ in their inclination with respect to the direction of the laminar schlieren. Specifically, in sample No. 7 the pore elongation axes are inclined by about 30 degrees from the direction of the schlieren, whereas in sample No. 23 there are at least two groups of pores whose elongation axes show departures of about 35 and 70 degrees from the direction of the schlieren. Large inclination of the elongation axes of the latter group of pores from the direction of the flow texture indicates that they formed in a completely different stress field compared to the schlieren pattern. Since the pores distinctly displace the thin layers of the schlieren themselves, it is clear that their formation post-dated the formation of flow textures.
On the basis of our observations a possible scenario for the formation of the pores in Muong Nong-type moldavites can be made.
The moldavites history is certainly related to the Ries crater. Regardless of the exact formation process (impact fusion of terrestrial sedimentary material, vapor fractionation of a relatively homogeneous melt, radiation melting of surface sediments, volatilization of elements and formation via plasma), each individual moldavite body was characterized by chemically different primary units destined to experience dissimilar regimes of stress. As shown in this work, at least two regimes are demonstrated by the relationship between schlieren and pores. Firstly, the schlieren was generated by the occurrence of inhomogeneity (probably fluids with different compositions and viscosity ) extended into lamellae in a stress field of laminar flow. Subsequently, as the tektites moved upwards, the temperature and the pressure decreased allowing the growth of the pores that, sometimes, displaced schlieren and were plastically deformed by the same force that shaped the individual moldavites body.
The appearance and relative abundance of the pores represent useful features to distinguish between splashform and Muong Nong-type moldavites. Pores in Muong Nong-type moldavites are much more numerous than in splashforms. Furthermore, in Muong Nong-type moldavites observed the pores agglomerate into clusters, which in limiting cases may result in the so-called frothy appearance absent in their splashform counterparts. The higher values of porosity in Muong Nong-type clearly indicate that the degassing process had not reached completion during the cooling of these tektites.
Combined X-ray micro computer aided tomography (μ-CT) and polarizing optical microscopic study of two splashform and four Muong Nong-type moldavites allowed the detailed characterization of the pore and strain distribution in this type of material. The study revealed the marked variability in pore size, distribution and shape between and within the individual samples. Moreover, the density and distribution of the pores confirmed that it is possible to distinguish between normal and Muong Nong-type moldavites using these parameters. Comparison of the directions of flow texture with those of the elongation axes of certain pores in Muong Nong-type moldavites revealed that the formation of at least a part of the pores post-dates the origin of the schlieren pattern.
The authors would like to thank Regione Toscana for financial support of the project LTSP (Laboratorio Toscano Scienze Planetarie) through the fund POR FSE 2007–2013 (Obiettivo 2, Asse IV). This work was also partially financed by MIUR (Ministero dell’Istruzione dell’Università e della Ricerca) through the fund PRIN2008 “Primitive Extraterrestrial Material as clues to the origin and evolution of the Early Solar System”. Lenka Dziková and Roman Skála acknowledge the support through the Czech Science Foundation (GAČR) projects 205/09/0991 and 13-22351S and Institute of Geology Research Plan RVO:67985831. The studied moldavites were kindly provided by Milan Trnka. Francesca Loglio would like to thank Fondazione Ente Cassa di Risparmio di Firenze for financial support. The authors thank Barry D. Howes for proof reading the English of this paper.
Lenka Dziková and Roman Skála selected the samples based on thorough morphologic, chemical and structural characterization, Roman Skála, in addition, contributed to formulation of the paper.
The Micro-CT data collection and 3D analysis were performed by Stefano Caporali and Francesca Loglio. Giovanni Pratesi carried out the optical microscopy investigation. The manuscript was co-written by all authors.
Conflicts of Interest
The authors declare no conflict of interest.
- Suess, F.E. Die Herkunft der Moldavite. Jahrb. Kais. K. Geol. Reichsanst. Wien 1900, 50, 193–382, (in German). [Google Scholar]
- Fudali, R.F.; Dyar, M.D.; Griscom, D.L.; Schreiber, D. The oxidation state of iron in tektite glass. Geochim. Cosmochim. Acta 1987, 51, 2749–2756. [Google Scholar]
- Dunlap, R.A.; Eelman, D.A.; MacKay, G.R. A Mössbauer effect investigation of correlated hyperfine parameters in natural glasses (tektites). J. Non Cryst. Solids 1998, 223, 141–146. [Google Scholar]
- Rossano, S.; Balan, E.; Morin, G.; Bauer, J.P.; Calas, G.; Brouder, C. 57Fe Mössbauer spectroscopy of tektites. Phys. Chem. Miner 1999, 26, 530–538. [Google Scholar]
- Giuli, G.; Pratesi, G.; Paris, E.; Cipriani, C. Fe local structure in tektites by EXAFS and High resolution XANES spectroscopy. Geochim. Cosmochim. Acta 2002, 66, 4347–4353. [Google Scholar]
- Dunlap, R.A.; Sibley, A.D.E. A Mössbauer effect study of Fe site occupancies in Australasian tektites. J. Non Cryst. Solids 2004, 337, 36–41. [Google Scholar]
- Giuli, G.; Eeckhout, S.G.; Cicconi, M.R.; Koeberl, C.; Pratesi, G.; Paris, E. Iron oxidation state and local structure in North American tektites; Special paper 465. In Large Meteorite Impacts and Planetary Evolution IV; Reimold, W.U., Gibson, R., Eds.; Geological Society of America: Boulder, CO, USA, 2010; pp. 645–652. [Google Scholar]
- Giuli, G.; Pratesi, G.; Eeckhout, S.G.; Koeberl, C.; Paris, E. Iron reduction in silicate glass produced during the 1945 nuclear test at the trinity site (Alamogordo, New Mexico, USA); Special paper 465. In Large Meteorite Impacts and Planetary Evolution IV; Reimold, W.U., Gibson, R., Eds.; Geological Society of America: Boulder, CO, USA, 2010; pp. 653–662. [Google Scholar]
- Lacroix, A. Les tectites sans formes figurées de l′Indochine. Acad. Sci. Paris Comptes Rendus Ser. B Sci. Phys 1935, 200, 2129–2132, (in French). [Google Scholar]
- Glass, B.P. Crystalline inclusions in Muong Nong-type tektite. Meteoritics 1970, 5, 199–200. [Google Scholar]
- Glass, B.P. Zircon and chromite crystals in a Muong Nong-type tektite. Science 1970, 169, 766–769. [Google Scholar]
- Glass, B.P. Relict Zircon Inclusion in Muong Nong-Type Australasian Tektites: Implications Regarding the Location of the Source Crater, Proceedings of 31st Annual Lunar and Planetary Science Conference, Houston, TX, USA, 13–17 March 2000.
- Koeberl, C. Geochemistry and origin of Muong Nong-type tektites. Geochim. Cosmochim. Acta 1992, 56, 1033–1064. [Google Scholar]
- Koeberl, C.; Beran, A. Water content of tektites and impact glasses and related chemical studies, Proceedings of the 18th Lunar and Planetary Science Conference, Houston, TX, USA, 16–20 March 1987.
- Glass, B.P.; Koeberl, C.; Blum, J.D.; Senftle, F.; Izett, G.A.; Evans, B.J.; Thorpe, A.N.; Povenmire, H.; Strange, R.L. A Muong–Nong type Georgia tektite. Geochim. Cosmochim. Acta 1995, 59, 4071–4082. [Google Scholar]
- Skála, R.; Strnad, L.; McCammon, C.; Čada, M. Moldavites from the Cheb Basin, Czech Republic. Geochim. Cosmochim. Acta 2009, 73, 1145–1179. [Google Scholar]
- Koeberl, C.; Brandstätter, F.; Niedermayr, G.; Kurat, G. Moldavites from Austria. Meteoritics 1988, 23, 325–332. [Google Scholar]
- Störr, M.; Lange, J.M. The occurrence of tektites northeast of Dresden, Germany. Geochim. Cosmochim. Acta 1992, 56, 2937–2940. [Google Scholar]
- Bouška, V. Geology and stratigraphy of moldavite occurrences. Geochim. Cosmochim. Acta 1964, 28. [Google Scholar] [CrossRef]
- Bouška, V. Moldavites: The Czech Tektites; Stylizace: Prague, Czech Republic, 1994. [Google Scholar]
- Bouška, V.; Ulrych, J. Electron microprobe analysis of two-coloured moldavites. J. Non Cryst. Solids 1984, 67, 375–381. [Google Scholar]
- Bouška, V.; Povondra, P. Correlation of some physical and chemical properties of moldavites. Geochim. Cosmochim. Acta 1964, 28, 783–791. [Google Scholar]
- Bouška, V. The moldavite strewn field. Chem. Erde Geochem 1998, 58, 321–343. [Google Scholar]
- Philpotts, J.A.; Pinson, W.H. New data on the chemical composition and origin of moldavites. Geochim. Cosmochim. Acta 1966, 33, 253–266. [Google Scholar]
- Barnes, V.E. Petrology of moldavites. Geochim. Cosmochim. Acta 1969, 33, 1121–1134. [Google Scholar]
- Engelhardt, W.V.; Luft, E.; Arndt, J.; Schock, H.; Weiskirchner, W. Origin of moldavites. Geochim. Cosmochim. Acta 1987, 51, 1425–1443. [Google Scholar]
- Engelhardt, W.V.; Berthold, C.; Wenzel, T.; Dehner, T. Chemistry, small-scale inhomogeneity, and formation of moldavites as condensates from sands vaporized by the Ries impact. Geochim. Cosmochim. Acta 2005, 69, 5611–5626. [Google Scholar]
- Trnka, M.; Houzar, S. Moravské Vltavíny; Muzejní a Vlastivědná Společnost v Brně, Západomoravské muzeum v Třebíči: Brno, Czech Republic, 1991. (in Czech). [Google Scholar]
- Trnka, M.; Houzar, S. Moldavites: A Review. Bull. Geosci 2002, 77, 283–302. [Google Scholar]
- Schnetzler, C.C.; Philpotts, J.A.; Hurley, W.H. Rubidium-strontium correlation study of moldavites and Ries crater material. Geochim. Cosmochim. Acta 1966, 33, 1015–1021. [Google Scholar]
- Shaw, H.F.; Wasserburg, G.J. Age and provenance of the target material for tektites and possible impactites from Sm/Nd and Rb/Sr-systematics. Earth Planet. Sci. Lett 1982, 60, 155–177. [Google Scholar]
- Graup, G.; Horn, P.; Köhler, H.; Müller-Sohnius, D. Source material for moldavites and bentonites. Naturwissenschaften 1981, 68, 616–617. [Google Scholar]
- Walter, L.S. Tektite compositional trends and experimental vapor fractionation of silicates. Geochim. Cosmochim. Acta 1967, 31, 2043–2063. [Google Scholar]
- Delano, J.W.; Lindsley, D.H. Chemical systematics among the moldavite tektites. Geochim. Cosmochim. Acta 1982, 46, 2447–2452. [Google Scholar]
- Řanda, Z.; Mizera, J.; Frána, J.; Kučera, J. Geochemical characterization of moldavites from a new locality, the Cheb Basin, Czech Republic. Meteorit. Planet. Sci 2008, 43, 461–467. [Google Scholar]
- Barnes, V.E. Origin of tektites. Tex. J. Sci 1989, 41, 5–33. [Google Scholar]
- Wasson, J.T. Layered tektites: A multiple impact origin for the Australasian tektites. Earth Planet. Sci. Lett 1991, 102, 95–109. [Google Scholar]
- Wasson, J.T. The disintegration of comet Shoemaker-Levy 9 and the Tunguska object and the origin of the Australasian tektites, Proceedings of the 26th Lunar and Planetary Science Conference, Lunar and Planetary Institute, Houston, TX, USA, 13–17 March 1995.
- Žák, K.; Skála, R.; Řanda, Z.; Mizera, J. A review of volatile compounds in tektites, and carbon content and isotopic composition of moldavite glass. Meteorit. Planet. Sci 2012, 47, 1010–1028. [Google Scholar]
- Horn, P.; Müller-Sohnius, D.; Köhler, H.; Graup, G. Rb-Sr systematics of rocks related to the Ries Crater, Germany. Earth Planet. Sci. Lett 1985, 75, 384–392. [Google Scholar]
- Buchner, E.; Seyfried, H.; van den Bogaard, P. 40Ar/39Ar laser probe age determination confirms the Ries impact crater as the source of glass particles in Graupensand sediments (Grimmelfinger Formation, North Alpine Foreland Basin). J. Earth Sci 2003, 92, 1–6. [Google Scholar]
- Gentner, W.; Lippolt, H.J.; Schaeffer, O.A. Argonbestimmungen an Kaliummineralen XI: Die Kalium Argonalter der Gläser des Nördlinger Rieses und der Böhmisch-Mährischen Tektite. Geochim. Cosmochim. Acta 1963, 27, 191–200, (in German). [Google Scholar]
- Laurenzi, A.; Bigazzi, G.; Balestrieri, M.L.; Bouška, W. 40Ar/39Ar laser probe dating of the Central European tektite-producing impact event. Meteorit. Planet. Sci 2003, 38, 887–893. [Google Scholar]
- Di Vincenzo, G.; Skála, R. 40Ar–39Ar laser dating of tektites from the Cheb Basin (Czech Republic): Evidence for coevality with moldavites and influence of the dating standard on the age of the Ries impact. Geochim. Cosmochim. Acta 2009, 73, 493–513. [Google Scholar]
- Buchner, E.; Schwarz, W.H.; Schmieder, M.; Trieloff, M. Establishing a 14.6 ± 0.2 Ma age for the Nordlinger Ries impact (Germany)—A prime example for concordant isotopic ages from various dating materials. Meteorit. Planet. Sci 2010, 45, 662–674. [Google Scholar]
- Koeberl, C. Muong Nong type tektites from the moldavite and north American strewn fields? J. Geophys. Res. Solid Earth 1986, 91, E253–E258. [Google Scholar]
- Rost, R. A Muong Nong–type moldavite from Lhenice in Bohemia. Acta Univ. Carol. Geol 1966, 4, 235–242. [Google Scholar]
- Švardalová, L.; Skála, R.; Trnka, M.; Houzar, S.; Novák, M. Extremely heterogeneous Muong Nong type moldavites, Proceedings of the 39th Lunar and Planetary Science Conference, League City, TX, USA, 10–14 March 2008.
- Meisel, T.; Lange, J.-M.; Krähenbühl, U. The chemical variation of moldavite tektites: Simple mixing of terrestrial sediments. Meteorit. Planet. Sci 1997, 32, 493–502. [Google Scholar]
- Ketcham, R.A.; Carlson, W.D. Acquisition, optimization and interpretation of X-ray computed tomographic imagery: Applications to the geosciences. Comput. Geosci 2001, 27, 381–400. [Google Scholar]
- Moreno-Atanasio, R.; Williams, R.A.; Jia, X. Combining X-ray microtomography with computer simulation for analysis of granular and porous materials. Particuology 2010, 8, 81–99. [Google Scholar]
- Voltolini, M.; Zandomeneghi, D.; Mancini, L.; Polacci, M. Texture analysis of volcanic rock samples: Quantitative study of crystals and vesicles shape preferred orientation from X-ray microtomography data. J. Volcanol. Geotherm. Res 2011, 202, 83–95. [Google Scholar]
- Hezel, D.C.; Friedrich, J.M.; Uesugi, M. Looking inside: 3D structures of meteorites. Geochim. Cosmochim. Acta 2013, 116, 1–4. [Google Scholar]
- Friedrich, J.M. Quantitative methods for three-dimensional comparison and petrographic description of chondrites. Comput. Geosci 2008, 34, 1926–1935. [Google Scholar]
- Ebel, D.S.; Rivers, M.L. Meteorite 3-D synchrotron microtomography: Methods and applications. Meteorit. Planet. Sci 2007, 42, 1627–1646. [Google Scholar]
- Hezel, D.C.; Elangovan, P.; Viehmann, S.; Howard, L.; Abel, R.L.; Armstrong, R. Visualisation and quantification of CV chondrite petrography using micro-tomography. Geochim. Cosmochim. Acta 2012, 116, 33–40. [Google Scholar]
- Uesugi, M.; Uesugi, K.; Takeuchi, A.; Suzuki, Y.; Hoshino, M.; Tsuchiyama, A. Three-dimensional observation of carbonaceous chondrites by synchrotron radiation X-ray CT—Quantitative analysis and developments for the future sample return missions. Geochim. Cosmochim. Acta 2013, 116, 17–32. [Google Scholar]
- Ebel, D.S.; Weisberg, M.K.; Hertz, J.; Campbell, A.J. Shape, metal abundance, chemistry and origin of chondrules in the Renazzo (CR) chondrite. Meteorit. Planet. Sci 2008, 43, 1725–1740. [Google Scholar]
- Sasso, M.R.; Macke, R.J.; Boesenberg, J.S.; Britt, D.T.; Rivers, M.L.; Ebel, D.S.; Friedrich, J.M. Incompletely compacted equilibrated ordinary chondrites. Meteorit. Planet. Sci 2009, 44, 1743–1753. [Google Scholar]
- Friedrich, J.M.; Macke, R.J.; Wignarajah, D.P.; Rivers, M.L.; Britt, D.T.; Ebel, D.S. Pore size distribution in an uncompacted equilibrated ordinary chondrite. Planet. Space Sci 2008, 56, 895–900. [Google Scholar]
- Friedrich, J.M.; Rivers, M.L. Three-dimensional imaging of ordinary chondrite microporosity at 2.6 μm resolution. Geochim. Cosmochim. Acta 2013, 116, 63–70. [Google Scholar]
- Troiano, J.; Rumble, D., III; Rivers, M.L.; Friedrich, J.M. Compositions of three low-FeO ordinary chondrites: Indications of a common origin with the H chondrites. Geochim. Cosmochim. Acta 2011, 75, 6511–6519. [Google Scholar]
- Tsuchiyama, A.; Nakamura, T.; Okazaki, T.; Uesugi, K.; Nakano, T.; Sakamoto, K.; Akaki, T.; Iida, Y.; Kadono, T.; Jogo, K.; et al. Three-dimensional structures and elemental distributions of Stardust impact tracks using synchrotron microtomography and X-ray fluorescence analysis. Meteorit. Planet. Sci 2009, 44, 1203–1224. [Google Scholar]
- Ebel, D.S.; Greenberg, M.; Rivers, M.L.; Newville, M. Three-dimensional textural and compositional analysis of particle tracks and fragmentation history in aerogel. Meteorit. Planet. Sci 2009, 44, 1445–1463. [Google Scholar]
- Alwmark, C.; Schmitz, B.; Holm, S.; Marone, F.; Stampanoni, M. A 3-D study of mineral inclusions in chromite from ordinary chondrites using synchrotron radiation X-ray tomographic microscopy—Method and applications. Meteorit. Planet. Sci 2011, 46, 1071–1081. [Google Scholar]
- Rantzsch, U.; Franz, A.; Kloess, G. Moldavite porosity: A 3-D X-ray micro-tomography study. Eur. J. Mineral 2013, 25, 705–710. [Google Scholar]
- Hildebrand, T.; Rüegsegger, P. A new method for the model-independent assessment of thickness in three-dimensional images. J. Microsc 1997, 185, 67–75. [Google Scholar]
- Matsuda, J.; Matsumoto, T.; Seta, A.; Tsuchiyama, A.; Nakashima, Y.; Yoneda, S. Noble gases in a large bubble in modavite: A comparison with phillippinite, Proceedings of the International Conference on Catastrophic Events & Mass Extinction: Impact and Beyond, Vienna, Austria, 9–12 July 2000.
- Majmundar, H.H.; O’Keefe, J.A. Causes of strain birefringence around the notches in moldavites. Geochim. Cosmochim. Acta 1967, 31, 1533–1534. [Google Scholar]
- Pratesi, G.; Viti, C.; Cipriani, C.; Mellini, M. Silicate-Silicate liquid immiscibility and graphite ribbons in Libyan desert glass. Geochim. Cosmochim. Acta 2002, 66, 903–911. [Google Scholar]
|Table 1. Porosity analysis results of six tektites.|
|Sample||Unit||No. 2||No. 7||No. 8||No. 23||Chlum 1||Chlum 2|
|Total volume (VOI)||μm3||1.68 × 1010||1.35 × 1010||2.48 × 1010||7.53 × 1010||4.76 × 1010||3.36 × 1010|
|Average pore number||Number of pores/mm3||102.9||79.5||105.5||13.8||12||2.1|
|Average pore surface density||mm2/mm3||9.2 × 10−4||4.2 × 10−4||16 × 10−4||8.8 × 10−4||0.18 × 10−4||0.05 × 10−4|
|Average pore size||μm3||0.13 × 106||0.5 × 106||0.4 × 106||2.34 × 106||0.009 × 106||0.03 × 106|
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