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LZS-1, Lanzarote (Canary Island, Spain) lunar (Apollo 14) basaltic soil simulant
Published 2022-10-01“…Subsequently, they were analysed by different techniques to determine their composition at a mineralogical and geochemical level, and the results were compared with data from other lunar simulants and from the Apollo 14 mission. After that, a set of petrophysical tests was carried out in order to determine its physical properties and evaluate its capacity as an analogous material for use in situ as a resource for further geological and astrobiological (future lunar habitability) essays.…”
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Origin of the Lunar Ultramafic Glasses Constrained by Experiments and Models
Published 2022“…The compositions are designed to produce liquids compositionally similar to the high-Ti Apollo 14 Black (A14B) glass (16.4 wt.% TiO₂) and the high-Al Apollo 14 Very Low Titanium (A14VLT) glass (0.61 wt.% TiO₂, 9.60 wt.% Al₂O₃). …”
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Petrological and rheological controls on volcanism to terrestrial planets
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Using Size and Composition to Assess the Quality of Lunar Impact Glass Ages
Published 2019-02-01“…To understand which properties of lunar impact glasses yield well-constrained ages, we evaluated the compositions and sizes of 119 Apollo 14, 15, 16, and 17 impact glass samples whose compositions and <sup>40</sup>Ar/<sup>39</sup>Ar ages have already been published, and we present new data on 43 others. …”
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The Influence of Variable Oxygen Fugacity on the Source Depths for Lunar High-Titanium Ultramafic Glasses
Published 2022“….% TiO₂), Apollo 15 Red glass (A15R, 13.8 wt.% TiO₂), and Apollo 14 Black glass (A14B, 16.4 wt.% TiO₂). Experimental temperatures and pressures varied from 1420-1590°C and 1.4 to 4.0 GPa. …”
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