ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars
We evaluated the effectiveness of the ExoMars Raman laser spectrometer (RLS) to determine the degree of serpentinization of olivine-rich units on Mars. We selected terrestrial analogs of martian ultramafic rocks from the Leka Ophiolite Complex (LOC) and analyzed them with both laboratory and flight-...
| Autores: | , , , , , , , , , , , , , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2021 |
| País: | España |
| Recursos: | Universidad de Valladolid |
| Repositorio: | UVaDOC. Repositorio Documental de la Universidad de Valladolid |
| OAI Identifier: | oai:uvadoc.uva.es:10324/46308 |
| Acesso em linha: | https://doi.org/10.1089/ast.2020.2265 http://uvadoc.uva.es/handle/10324/46308 |
| Access Level: | acceso abierto |
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ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on MarsVeneranda ., MarcoLópez Reyes, Guillermo EduardoPascual Sanchez, ElenaKrzesińska, Agata M.Manrique Martínez, José AntonioSanz Arranz, José AurelioLantz, CatelineLalla, Emmanuel AlexisMoral Inza, Andoni GaizkaMedina García, JesúsPoulet, FrancoisDypvik, HenningWerner, Stephanie C.Vago, Jorge L.Rull Pérez, FernandoWe evaluated the effectiveness of the ExoMars Raman laser spectrometer (RLS) to determine the degree of serpentinization of olivine-rich units on Mars. We selected terrestrial analogs of martian ultramafic rocks from the Leka Ophiolite Complex (LOC) and analyzed them with both laboratory and flight-like analytical instruments. We first studied the mineralogical composition of the samples (mostly olivine and serpentine) with state-of-the-art diffractometric (X-ray diffractometry [XRD]) and spectroscopic (Raman, near-infrared spectroscopy [NIR]) laboratory systems. We compared these results with those obtained using our RLS ExoMars Simulator. Our work shows that the RLS ExoMars Simulator successfully identified all major phases. Moreover, when emulating the automatic operating mode of the flight instrument, the RLS ExoMars Simulator also detected several minor compounds (pyroxene and brucite), some of which were not observed by NIR and XRD (e.g., calcite). Thereafter, we produced RLS-dedicated calibration curves (R2 between 0.9993 and 0.9995 with an uncertainty between ±3.0% and ±5.2% with a confidence interval of 95%) to estimate the relative content of olivine and serpentine in the samples. Our results show that RLS can be very effective in identifying serpentine, a scientific target of primary importance for the potential detection of biosignatures on Mars—the main objective of the ExoMars rover mission.Proyecto MINECO Retos de la Sociedad. Ref. ESP2017-87690-C3-1-RMary Ann Liebert, Inc.2021info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://doi.org/10.1089/ast.2020.2265http://uvadoc.uva.es/handle/10324/46308reponame:UVaDOC. Repositorio Documental de la Universidad de Valladolidinstname:Universidad de ValladolidInglésinfo:eu-repo/semantics/openAccessoai:uvadoc.uva.es:10324/463082026-06-13T12:44:47Z |
| dc.title.none.fl_str_mv |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| title |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| spellingShingle |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars Veneranda ., Marco |
| title_short |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| title_full |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| title_fullStr |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| title_full_unstemmed |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| title_sort |
ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars |
| dc.creator.none.fl_str_mv |
Veneranda ., Marco López Reyes, Guillermo Eduardo Pascual Sanchez, Elena Krzesińska, Agata M. Manrique Martínez, José Antonio Sanz Arranz, José Aurelio Lantz, Cateline Lalla, Emmanuel Alexis Moral Inza, Andoni Gaizka Medina García, Jesús Poulet, Francois Dypvik, Henning Werner, Stephanie C. Vago, Jorge L. Rull Pérez, Fernando |
| author |
Veneranda ., Marco |
| author_facet |
Veneranda ., Marco López Reyes, Guillermo Eduardo Pascual Sanchez, Elena Krzesińska, Agata M. Manrique Martínez, José Antonio Sanz Arranz, José Aurelio Lantz, Cateline Lalla, Emmanuel Alexis Moral Inza, Andoni Gaizka Medina García, Jesús Poulet, Francois Dypvik, Henning Werner, Stephanie C. Vago, Jorge L. Rull Pérez, Fernando |
| author_role |
author |
| author2 |
López Reyes, Guillermo Eduardo Pascual Sanchez, Elena Krzesińska, Agata M. Manrique Martínez, José Antonio Sanz Arranz, José Aurelio Lantz, Cateline Lalla, Emmanuel Alexis Moral Inza, Andoni Gaizka Medina García, Jesús Poulet, Francois Dypvik, Henning Werner, Stephanie C. Vago, Jorge L. Rull Pérez, Fernando |
| author2_role |
author author author author author author author author author author author author author author |
| description |
We evaluated the effectiveness of the ExoMars Raman laser spectrometer (RLS) to determine the degree of serpentinization of olivine-rich units on Mars. We selected terrestrial analogs of martian ultramafic rocks from the Leka Ophiolite Complex (LOC) and analyzed them with both laboratory and flight-like analytical instruments. We first studied the mineralogical composition of the samples (mostly olivine and serpentine) with state-of-the-art diffractometric (X-ray diffractometry [XRD]) and spectroscopic (Raman, near-infrared spectroscopy [NIR]) laboratory systems. We compared these results with those obtained using our RLS ExoMars Simulator. Our work shows that the RLS ExoMars Simulator successfully identified all major phases. Moreover, when emulating the automatic operating mode of the flight instrument, the RLS ExoMars Simulator also detected several minor compounds (pyroxene and brucite), some of which were not observed by NIR and XRD (e.g., calcite). Thereafter, we produced RLS-dedicated calibration curves (R2 between 0.9993 and 0.9995 with an uncertainty between ±3.0% and ±5.2% with a confidence interval of 95%) to estimate the relative content of olivine and serpentine in the samples. Our results show that RLS can be very effective in identifying serpentine, a scientific target of primary importance for the potential detection of biosignatures on Mars—the main objective of the ExoMars rover mission. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
https://doi.org/10.1089/ast.2020.2265 http://uvadoc.uva.es/handle/10324/46308 |
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https://doi.org/10.1089/ast.2020.2265 http://uvadoc.uva.es/handle/10324/46308 |
| dc.language.none.fl_str_mv |
Inglés |
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Inglés |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
| dc.publisher.none.fl_str_mv |
Mary Ann Liebert, Inc. |
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Mary Ann Liebert, Inc. |
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reponame:UVaDOC. Repositorio Documental de la Universidad de Valladolid instname:Universidad de Valladolid |
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Universidad de Valladolid |
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UVaDOC. Repositorio Documental de la Universidad de Valladolid |
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UVaDOC. Repositorio Documental de la Universidad de Valladolid |
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