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Libyan desert glass

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Journal Article
Published: 01 October 2023
American Mineralogist (2023) 108 (10): 1906–1923.
...Elizaveta Kovaleva; Hassan Helmy; Said Belkacim; Anja Schreiber; Franziska D.H. Wilke; Richard Wirth Abstract The origin of Libyan Desert Glass (LDG) found in the western parts of Egypt close to the Libyan border is debated in planetary science. Two major theories of its formation are currently...
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Journal Article
Published: 01 July 2022
American Mineralogist (2022) 107 (7): 1325–1340.
... or by devitrification. Here we report a study of α-cristobalite in Libyan Desert Glass (LDG), a nearly pure silica natural glass of impact origin found in western Egypt, using electron microprobe analysis (EMPA), laser ablation inductively coupled mass spectrometry (LA-ICP-MS), time-of-flight secondary ion mass...
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Journal Article
Journal: Geology
Published: 02 May 2019
Geology (2019) 47 (7): 609–612.
... environments and, in the case of Chelyabinsk, injured humans. Enigmatic natural glasses have been cited as geologic evidence of the threat posed by large airbursts. Libyan Desert Glass (LDG) is a natural glass found in western Egypt that formed ∼29 m.y. ago, however its origin is disputed; the two main...
FIGURES
Published: 01 January 1999
DOI: 10.1130/0-8137-2339-6.177
Image
Cathodoluminescence images of Libyan Desert Glass. (a) Sample LDG-2018-2a, showing layering. (b) Sample LDG-2018-2b; inset shows the cristobalite grain in Figure 2a.
Published: 01 July 2022
Figure 1. Cathodoluminescence images of Libyan Desert Glass. ( a ) Sample LDG-2018-2a, showing layering. ( b ) Sample LDG-2018-2b; inset shows the cristobalite grain in Figure 2a .
Image
Model of β-cristobalite origin in Libyan Desert Glass (LDG). (a) Silica-rich precursor material (quartz arenite?), pre-impact. Gray and black grains represent Al-bearing phases. (b) Rapid superheating of the precursor formed layered silica melt. (c) Crystallization of magmatic β-cristobalite octahedra with various growth zoning features defined by Al zonation in supercooled silica melt. (d) Dendritic growth of β-cristobalite rims by devitrification in the solid-state. (e) Fracturing due to volume change (ΔV) from the β-α transformation. (f) Formation of α-cristobalite twins; twins in the rim extend across and pre-date fractures; twins in the core are pinned, forming after fractures.
Published: 01 July 2022
Figure 13. Model of β-cristobalite origin in Libyan Desert Glass (LDG). ( a ) Silica-rich precursor material (quartz arenite?), pre-impact. Gray and black grains represent Al-bearing phases. ( b ) Rapid superheating of the precursor formed layered silica melt. ( c ) Crystallization of magmatic β
Image
Map showing location of Libyan Desert Glass (LDG) field in western Egypt (after Koeberl, 1997). Also shown are two regional impact structures, B.P. (2 km diameter) and Oasis (18 km diameter) (Abate et al., 1999).
Published: 02 May 2019
Figure 1. Map showing location of Libyan Desert Glass (LDG) field in western Egypt (after Koeberl, 1997 ). Also shown are two regional impact structures, B.P. (2 km diameter) and Oasis (18 km diameter) ( Abate et al., 1999 ).
Image
Granular zircon from Libyan Desert Glass that preserves evidence of former reidite. A: Backscattered electron (BSE) image showing granular core (neoblastic zircon 1, nz1) surrounded by partially detached corona (rim) consisting of zirconia (baddeleyite) intergrown with a later generation of neoblastic zircon (nz2). B: Orientation map shown with inverse pole figure (IPFy) color scheme. C: Pole figures showing data for granular zircon core (see oval in B). D: Plot showing high-angle (75°–95°) misorientation axes for data in C. Stereonets are equal-area, lower-hemisphere projections in sample x-y-z reference frame.
Published: 02 May 2019
Figure 2. Granular zircon from Libyan Desert Glass that preserves evidence of former reidite. A: Backscattered electron (BSE) image showing granular core (neoblastic zircon 1, nz1) surrounded by partially detached corona (rim) consisting of zirconia (baddeleyite) intergrown with a later
Image
Raman spectra in the frequency range 20–1400 cm−1 of lechatelierite and Libyan Desert Glass (LDG). The frequency position of the main vibrations is reported.
Published: 01 May 2022
Figure 20. Raman spectra in the frequency range 20–1400 cm −1 of lechatelierite and Libyan Desert Glass (LDG). The frequency position of the main vibrations is reported.
Image
SiO2 vs. total alkali (wt.%) diagram for several natural non-magmatic glasses described in this chapter. Glasses deriving from magmatic processes are reported for comparison. Data compilation from Cicconi and Neuville (2019). Combustion glasses from Table 1. LDG = Libyan Desert Glass; mT = microtektites.
Published: 01 May 2022
Figure 1. SiO 2 vs. total alkali (wt.%) diagram for several natural non-magmatic glasses described in this chapter. Glasses deriving from magmatic processes are reported for comparison. Data compilation from Cicconi and Neuville (2019) . Combustion glasses from Table 1 . LDG = Libyan Desert
Image
Simplified pressure-temperature (P-T) diagram (modified after French, 1998) showing hypothetical P-T paths for both airburst (purple) and crater-forming (red) events; dashed portions indicate different possible trajectories. Note that P indicated for airburst path is greatly exaggerated for convenience of illustration; atmospheric overpressures from airburst are in thousands of pascals range (e.g., Aftosmis et al., 2019). Observations from Libyan Desert Glass (LDG) (this study) and Australasian tektites (AT) (see text) are indicated. Neoblastic zircon 1 and 2 refer to different generations of zircon shown in Figure 2. “Reidite-in” and zircon dissociation (dissoc.) curves are from Timms et al. (2017). Cristobalite field is from Swamy et al. (1994).
Published: 02 May 2019
exaggerated for convenience of illustration; atmospheric overpressures from airburst are in thousands of pascals range (e.g., Aftosmis et al., 2019 ). Observations from Libyan Desert Glass (LDG) (this study) and Australasian tektites (AT) (see text) are indicated. Neoblastic zircon 1 and 2 refer to different
Image
Map of location of Libyan glass on the surface of the desert in western Egypt (a poster by V. de Michele at the 57th Meteoritic Conference in Prague, 1994, according to [94]). 1 – sandy dunes, 2 – deflation corridors between the dunes with residual gravel, 3 – Upper Cretaceous Nubian sandstone, 4 – places where glasses were found. The weight of glasses is 100 g to 10 kg over an area of 10,000 m2. It is assumed that the annular contour of 15–22 km in diameter mainly coincides with the primary occurrence of Libyan glass (from the poster legend).
Published: 01 March 1997
Fig. 18. Map of location of Libyan glass on the surface of the desert in western Egypt (a poster by V. de Michele at the 57th Meteoritic Conference in Prague, 1994, according to [ 94 ]). 1 – sandy dunes, 2 – deflation corridors between the dunes with residual gravel, 3 – Upper Cretaceous Nubian
Journal Article
Published: 01 May 2022
Reviews in Mineralogy and Geochemistry (2022) 87 (1): 965–1014.
...Figure 20. Raman spectra in the frequency range 20–1400 cm −1 of lechatelierite and Libyan Desert Glass (LDG). The frequency position of the main vibrations is reported. ...
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Journal Article
Published: 01 April 2012
Earth Sciences History (2012) 31 (1): 50–75.
... colored Libyan desert glass ( George 2000 ). Although the associated pebbles are rounded, the glass shows no signs of having been rolled, though its surface is wind-eroded ( Clayton and Spencer 1934 ). This Libyan desert glass (LDG), as it is now known, is today classified as a tektite ( Müehle 1998...
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Journal Article
Published: 01 March 2002
Geological Magazine (2002) 139 (2): 236–237.
... their terrestrial origin, and provides the evidence linking the tektite strewn fields to particular impact structures. In chapters seven and eight there is a departure from the main tektite theme to discuss occurrences of other natural glasses in relation to impacts, such as Libyan Desert Glass in Egypt, Darwin...
Journal Article
Journal: Geology
Published: 01 October 2001
Geology (2001) 29 (10): 899–902.
... and Boslough, 2000) . A large aerial burst would be accompanied by an intense thermal pulse. Wasson and Moore (1998) speculated that Libyan Desert glass may have been produced by this mechanism. It has also been calculated that intense thermal radiation may be transmitted to the surface along a strip...
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Journal Article
Published: 01 June 2002
The Canadian Mineralogist (2002) 40 (3): 999–1000.
...Michael Zolensky Fairly complete descriptions are given of other types of impact glasses, which are not considered tektites, such as glasses found near Zhamanshin (Kazakhstan) and Wabar (Saudi Arabia) craters, Libyan Desert Glass (Egypt), Darwin Glass (Tasmania), etc. For some reason...
Journal Article
Journal: Geology
Published: 01 February 2007
Geology (2007) 35 (2): 171–174.
... here the composition of CO 2 , CO, and NO contained within the glassy bubbles of a fulgurite from the Libyan Desert. The results show that the fulgurite formed when the ground contained 0.1 wt% organic carbon with a C/N ratio of 10–15 and a δ 13 C of −13.96‰, compositions similar to those found...
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Series: EMU Notes in Mineralogy series
Published: 01 January 2019
DOI: 10.1180/EMU-notes.20.9
EISBN: 9780903056625
... Tutankhamun’s pectoral and Libyan Desert Glass Libyan Desert Glass (LDG) ( Fig. 7 ) is a natural glass consisting mainly of silica (SiO 2 ~98 wt.%) and traces of Al, Fe, Mg and other metals ( Fudali, 1981 ; Koeberl, 1986 , 1997 ; Barrat et al. , 1997 ; Greshake et al. , 2010 , 2018 ). The H 2 O...
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Journal Article
Journal: Geology
Published: 02 August 2018
Geology (2018) 46 (9): 787–790.
... to rhombohedral planes are of minor abundance ( Fig. 4 ). The predominance of PDFs and BTs is therefore a strong indicator of low shock pressure. Previous studies on sandstones from the Libyan Desert Glass strewn field ( Kleinmann et al., 2001 ) and the target rocks from the Mjølnir impact crater...
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