Raman analyses of Al and Fe/Mg‐rich clays: Challenges and possibilities for planetary missions
暂无分享,去创建一个
I. Hutchinson | M. Mchugh | C. Malherbe | G. Eppe | N. Fagel | L. Demaret | H. Lerman
[1] Q. Yao,et al. Reliable spectroscopic identification of minerals associated with serpentinization: Relevance to Mars exploration , 2023, Icarus.
[2] C. Zhou,et al. Enigmatic Issues and Widening Implications of Research on Martian Clay Minerals , 2022, ACS Earth and Space Chemistry.
[3] V. Rajesh,et al. Serpentine-magnesite association of Salem Ultramafic Complex, southern India: A potential analogue for mars , 2022, Planetary and Space Science.
[4] I. Hutchinson,et al. Fe-Rich Fossil Vents as Mars Analog Samples: Identification of Extinct Chimneys in Miocene Marine Sediments Using Raman Spectroscopy, X-Ray Diffraction, and Scanning Electron Microscopy-Energy Dispersive X-Ray Spectroscopy. , 2022, Astrobiology.
[5] A. Molina,et al. Raman spectroscopic peculiarities of Icelandic poorly crystalline minerals and their implications for Mars exploration , 2022, Scientific Reports.
[6] Alian Wang,et al. Crystallinity effects on the vibrational spectral features of saponite: Implications for characterizing variable crystalline phyllosilicates on Mars , 2022, Icarus.
[7] B. Pejcic,et al. Chemistry-dependent Raman spectral features of glauconite and nontronite: Implications for mineral identification and provenance analysis , 2021, American Mineralogist.
[8] C. Cousins,et al. Multiscale spectral discrimination of poorly-crystalline and intermixed alteration phases using aerial and ground-based ExoMars rover emulator data , 2021 .
[9] M. J. Calaway,et al. Perseverance’s Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) Investigation , 2021, Space Science Reviews.
[10] K. Ikehata,et al. Raman microspectroscopic study of reference clay minerals and alteration minerals in volcanic ejecta from the 7 March 2012 phreatic eruption on Ioto Island (Iwo-jima), Izu-Bonin arc, Japan , 2021 .
[11] G. Arana,et al. Characterization of sedimentary and volcanic rocks in Armintza outcrop (Biscay, Spain) and its implication for Oxia Planum (Mars) exploration. , 2021, Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy.
[12] P. Allemand,et al. Oxia Planum: The Landing Site for the ExoMars “Rosalind Franklin” Rover Mission: Geological Context and Prelanding Interpretation , 2021, Astrobiology.
[13] David I. Ellis,et al. Comparability of Raman Spectroscopic Configurations: A Large Scale Cross-Laboratory Study. , 2020, Analytical chemistry.
[14] F. Poulet,et al. ExoMars Raman Laser Spectrometer: A Tool to Semiquantify the Serpentinization Degree of Olivine-Rich Rocks on Mars. , 2020, Astrobiology.
[15] J. T. Kloprogge,et al. Spectroscopic Studies of Synthetic and Natural Saponites: A Review , 2020, Minerals.
[16] R. Léveillé,et al. Data fusion of laser-induced breakdown and Raman spectroscopies: Enhancing clay mineral identification , 2020 .
[17] Honglong Wang,et al. An intensive exploration on structure transformation of talc under γ-ray irradiation at 0–1000 kGy , 2020, Journal of Radioanalytical and Nuclear Chemistry.
[18] G. Christidis,et al. Characterization and origin of two Fe-rich bentonites from Westerwald (Germany) , 2020 .
[19] C. Pilorget,et al. Raman Laser Spectrometer (RLS) calibration target design to allow onboard combined science between the RLS and MicrOmega instruments on the ExoMars rover , 2020 .
[20] H. Edwards,et al. Raman spectra of a graphite–nontronite association in marbles from Oltrek Island (Lake Baikal, Russia) , 2019 .
[21] Gordon R. Osinski,et al. Field and laboratory validation of remote rover operations Science Team findings: The CanMars Mars Sample Return analogue mission , 2019, Planetary and Space Science.
[22] S. F. Vallejuelo,et al. New Raman–visible near‐infrared database of inorganic and mineralogical planetary and terrestrial compounds and its implications for Mars: Phyllosilicates , 2019, Journal of Raman Spectroscopy.
[23] J. Grant,et al. The science process for selecting the landing site for the 2020 Mars rover , 2018, Planetary and Space Science.
[24] E. Jessberger,et al. Raman spectra of hydrous minerals investigated under various environmental conditions in preparation for planetary space missions , 2018, Journal of Raman Spectroscopy.
[25] B. Hynek,et al. Characterization of terrestrial hydrothermal alteration products with mars analog instrumentation: implications for current and future rover investigations , 2017 .
[26] Gianfranco Visentin,et al. Habitability on Early Mars and the Search for Biosignatures with the ExoMars Rover , 2017, Astrobiology.
[27] MedinaJesús,et al. The Raman Laser Spectrometer for the ExoMars Rover Mission to Mars , 2017 .
[28] J. Head,et al. Sedimentological evidence for a deltaic origin of the western fan deposit in Jezero crater, Mars and implications for future exploration , 2017 .
[29] R. Wordsworth. The Climate of Early Mars , 2016, 1606.02813.
[30] J. A. Rodríguez-Losada,et al. Raman-Mössbauer-XRD studies of selected samples from “Los Azulejos” outcrop: A possible analogue for assessing the alteration processes on Mars , 2016 .
[31] L. Vaculíková,et al. Different level of fluorescence in Raman spectra of montmorillonites , 2016 .
[32] B. Jolliff,et al. Understanding the Raman spectral features of phyllosilicates , 2015 .
[33] Jean-Pierre Bibring,et al. Widespread surface weathering on early Mars: A case for a warmer and wetter climate , 2015 .
[34] Ashwin R. Vasavada,et al. Curiosity's Mission of Exploration at Gale Crater, Mars , 2015 .
[35] H. Edwards,et al. Potential for analysis of carbonaceous matter on Mars using Raman spectroscopy , 2014 .
[36] B. Ehlmann,et al. Mineralogy of the Martian Surface , 2014 .
[37] A. Yingst,et al. A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars , 2014, Science.
[38] I. Němec,et al. Microanalysis of clay‐based pigments in painted artworks by the means of Raman spectroscopy , 2013 .
[39] Jean-Pierre Bibring,et al. Subsurface water and clay mineral formation during the early history of Mars , 2011, Nature.
[40] J. Head,et al. Sequence and timing of conditions on early Mars , 2011 .
[41] P. Lucey,et al. A combined remote Raman and LIBS instrument for characterizing minerals with 532 nm laser excitation. , 2009, Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy.
[42] John F. Mustard,et al. Clay minerals in delta deposits and organic preservation potential on Mars , 2008 .
[43] T. Encrenaz,et al. Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data , 2006, Science.
[44] I. R. Lewis,et al. Handbook of Raman Spectroscopy: From the Research Laboratory to the Process Line , 2001 .
[45] R. Frost,et al. Raman Spectroscopy of Nontronites , 2000 .
[46] Ray L. Frost,et al. The structure of the kaolinite minerals−a FT-Raman study , 1997, Clay Minerals.
[47] E. Murad. Identification of minor amounts of anatase in kaolins by Raman spectroscopy , 1997 .
[48] V. Farmer. Infrared spectroscopy in clay mineral studies , 1968, Clay Minerals.
[49] J. Bishop,et al. Surface clay formation during short-term warmer and wetter conditions on a largely cold ancient Mars , 2018, Nature Astronomy.
[50] B. Ehlmann,et al. Geochemical Consequences of Widespread Clay Mineral Formation in Mars’ Ancient Crust , 2013 .