Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants

Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants. The objective of the present study is to identify rock lithologies which can be used to produce Mars regolith simulants. It is well known from Curiosity Rover data, t...

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محفوظ في:
التفاصيل البيبلوغرافية
المؤلف الرئيسي: Pavlopoulos, Kosmas (author)
مؤلفون آخرون: Ioannou, Zach (author), Moraetis, Daniel (author)
منشور في: 2021
الوصول للمادة أونلاين:https://depot.sorbonne.ae/handle/20.500.12458/1281
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author Pavlopoulos, Kosmas
author2 Ioannou, Zach
Moraetis, Daniel
author2_role author
author
author_facet Pavlopoulos, Kosmas
Ioannou, Zach
Moraetis, Daniel
author_role author
dc.creator.none.fl_str_mv Pavlopoulos, Kosmas
Ioannou, Zach
Moraetis, Daniel
dc.date.none.fl_str_mv 2021
2022-06-01T11:06:26Z
2022-06-01T11:06:26Z
dc.format.none.fl_str_mv application/pdf
dc.identifier.none.fl_str_mv https://depot.sorbonne.ae/handle/20.500.12458/1281
dc.language.none.fl_str_mv en
dc.title.none.fl_str_mv Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
dc.type.none.fl_str_mv Controlled Vocabulary for Resource Type Genres::text::conference object::conference proceedings
description Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants. The objective of the present study is to identify rock lithologies which can be used to produce Mars regolith simulants. It is well known from Curiosity Rover data, that mafic and ultramafic components are the main constituents of the Martian surface regolith (Blake et al. 2013). We have acquired 9 rock samples taken from different locations and rock outcrops located in the Fujairah, Sharjah and Dubai emirates of the UAE and used to obtain crustal (mafic) and mantle (ultramafic) rock spectral signatures (Philips et al. 2006, Thomas et al. 2006). The samples are analyzed using X-ray fluorescence and X-ray diffraction techniques. Based on their mineralogical composition and characteristics we distinguished two main categories of rocks, close to the Hatta and Kahir areas. The analysis showed a range of SiO2 compatible with ultramafic to mafic rocks (43-46% ±1%) in the Hatta area and some samples with extreme high (73%±1%) or low (21%±1%) values of SiO2. The aforementioned extreme concentrations are possibly correlated to sedimentary or metasedimentary rocks. The mineralogy in the Hatta area comprised mainly of pyroxene and plagioclase and some amorphous material while the metasedimentary rocks are mainly rich in calcite and quartz. The Kahir area samples are showing a SiO2 content between ultramafic to mafic rocks (39-49% ±1%). The mineralogy in the Kahir samples comprised of pyroxene and plagioclase and in several samples the ultramafic rocks are exhibiting strong serpentinization (serpentine mineral). In addition to ground investigations, we have also mapped the extended regions that surround the areas of our rock samples using hyperspectral imagery obtained in 2009 and 2011 by the Hyperion instrument on the Earth Obserbation-1 (EO-1) satellite. Feature extraction and hyperspectral classification such as the supervised Spectral Angle Mapper (SAM) and Spectral Feature Fitting (SFF) methods are carried out to map the different lithologies in the extended regions of interest. We combine the ground truth spectral classification of our samples with the hyperspectral classification of the wider area to improve the accuracy of the mineral map around the Hatta and Kahir regions.
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spelling Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulantsPavlopoulos, KosmasIoannou, ZachMoraetis, DanielHyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants. The objective of the present study is to identify rock lithologies which can be used to produce Mars regolith simulants. It is well known from Curiosity Rover data, that mafic and ultramafic components are the main constituents of the Martian surface regolith (Blake et al. 2013). We have acquired 9 rock samples taken from different locations and rock outcrops located in the Fujairah, Sharjah and Dubai emirates of the UAE and used to obtain crustal (mafic) and mantle (ultramafic) rock spectral signatures (Philips et al. 2006, Thomas et al. 2006). The samples are analyzed using X-ray fluorescence and X-ray diffraction techniques. Based on their mineralogical composition and characteristics we distinguished two main categories of rocks, close to the Hatta and Kahir areas. The analysis showed a range of SiO2 compatible with ultramafic to mafic rocks (43-46% ±1%) in the Hatta area and some samples with extreme high (73%±1%) or low (21%±1%) values of SiO2. The aforementioned extreme concentrations are possibly correlated to sedimentary or metasedimentary rocks. The mineralogy in the Hatta area comprised mainly of pyroxene and plagioclase and some amorphous material while the metasedimentary rocks are mainly rich in calcite and quartz. The Kahir area samples are showing a SiO2 content between ultramafic to mafic rocks (39-49% ±1%). The mineralogy in the Kahir samples comprised of pyroxene and plagioclase and in several samples the ultramafic rocks are exhibiting strong serpentinization (serpentine mineral). In addition to ground investigations, we have also mapped the extended regions that surround the areas of our rock samples using hyperspectral imagery obtained in 2009 and 2011 by the Hyperion instrument on the Earth Obserbation-1 (EO-1) satellite. Feature extraction and hyperspectral classification such as the supervised Spectral Angle Mapper (SAM) and Spectral Feature Fitting (SFF) methods are carried out to map the different lithologies in the extended regions of interest. We combine the ground truth spectral classification of our samples with the hyperspectral classification of the wider area to improve the accuracy of the mineral map around the Hatta and Kahir regions.2022-06-01T11:06:26Z2022-06-01T11:06:26Z2021Controlled Vocabulary for Resource Type Genres::text::conference object::conference proceedingsapplication/pdfhttps://depot.sorbonne.ae/handle/20.500.12458/1281enoai:depot.sorbonne.ae:20.500.12458/12812023-01-05T07:20:55Z
spellingShingle Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
Pavlopoulos, Kosmas
title Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
title_full Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
title_fullStr Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
title_full_unstemmed Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
title_short Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
title_sort Hyperspectral mapping of crust and mantle rocks in the UAE Al-Hajar mountains: Locating raw materials for Martian regolith simulants
url https://depot.sorbonne.ae/handle/20.500.12458/1281