Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload

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Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload. / Allender, E.j.; Cousins, C.r.; Gunn, M.d.; Caudill, C.m.

Yn: Earth and Space Science, Cyfrol 7, Rhif 4, e2019EA000692, 22.04.2020.

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

Harvard

Allender, EJ, Cousins, CR, Gunn, MD & Caudill, CM 2020, 'Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload', Earth and Space Science, cyfrol. 7, rhif 4, e2019EA000692. https://doi.org/10.1029/2019EA000692

APA

Allender, E. J., Cousins, C. R., Gunn, M. D., & Caudill, C. M. (2020). Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload. Earth and Space Science, 7(4), [e2019EA000692]. https://doi.org/10.1029/2019EA000692

Vancouver

Author

Allender, E.j. ; Cousins, C.r. ; Gunn, M.d. ; Caudill, C.m. / Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload. Yn: Earth and Space Science. 2020 ; Cyfrol 7, Rhif 4.

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@article{9062d1b8ed974b228431957fdcce293d,
title = "Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload",
abstract = "In 2020, the European Space Agency and Roscosmos will launch the ExoMars rover, with the scientific objective to detect evidence of life within the martian surface via the deployment of a 2 meter drill. The ExoMars Pasteur payload contains several imaging and spectroscopic instruments key to this objective: the Panoramic Camera (PanCam), Infrared Spectrometer for ExoMars (ISEM), and Close‐UP Imager (CLUPI). These instruments are able to collect data at a variety of spatial (sub‐mm to decimeter) and spectral (3.3 to 120 nm) resolutions across the 440 to 3300 nm wavelength range and collectively will form a picture of the geological and morphological characteristics of the surface terrain surrounding the rover. We deployed emulators of this instrument suite at terrestrial analog sites that formed in a range of aqueous environments to test their ability to detect and characterize science targets. We find that the emulator suite is able to effectively detect, characterize, and refine the compositions of multiple targets at working distances spanning from 2‐18 m. We report on: (i) the detection of hydrothermal alteration minerals including Fe‐smectites and gypsum from basaltic substrates, (ii) the detection of late‐stage diagenetic gypsum veins embedded in exposures of sedimentary mudstone, (iii) multispectral evidence of compositional differences detected from fossiliferous mudstones, and (iv) approaches to cross‐referencing multi‐scale and multi‐resolution data. These findings aid in the development of data products and analysis toolkits in advance of the ExoMars rover mission.",
author = "E.j. Allender and C.r. Cousins and M.d. Gunn and C.m. Caudill",
year = "2020",
month = apr,
day = "22",
doi = "10.1029/2019EA000692",
language = "English",
volume = "7",
journal = "Earth and Space Science",
issn = "2333-5084",
publisher = "Wiley",
number = "4",

}

RIS (suitable for import to EndNote) - Download

TY - JOUR

T1 - Multiscale and multispectral characterization of mineralogy with the ExoMars 2020 rover remote sensing payload

AU - Allender, E.j.

AU - Cousins, C.r.

AU - Gunn, M.d.

AU - Caudill, C.m.

PY - 2020/4/22

Y1 - 2020/4/22

N2 - In 2020, the European Space Agency and Roscosmos will launch the ExoMars rover, with the scientific objective to detect evidence of life within the martian surface via the deployment of a 2 meter drill. The ExoMars Pasteur payload contains several imaging and spectroscopic instruments key to this objective: the Panoramic Camera (PanCam), Infrared Spectrometer for ExoMars (ISEM), and Close‐UP Imager (CLUPI). These instruments are able to collect data at a variety of spatial (sub‐mm to decimeter) and spectral (3.3 to 120 nm) resolutions across the 440 to 3300 nm wavelength range and collectively will form a picture of the geological and morphological characteristics of the surface terrain surrounding the rover. We deployed emulators of this instrument suite at terrestrial analog sites that formed in a range of aqueous environments to test their ability to detect and characterize science targets. We find that the emulator suite is able to effectively detect, characterize, and refine the compositions of multiple targets at working distances spanning from 2‐18 m. We report on: (i) the detection of hydrothermal alteration minerals including Fe‐smectites and gypsum from basaltic substrates, (ii) the detection of late‐stage diagenetic gypsum veins embedded in exposures of sedimentary mudstone, (iii) multispectral evidence of compositional differences detected from fossiliferous mudstones, and (iv) approaches to cross‐referencing multi‐scale and multi‐resolution data. These findings aid in the development of data products and analysis toolkits in advance of the ExoMars rover mission.

AB - In 2020, the European Space Agency and Roscosmos will launch the ExoMars rover, with the scientific objective to detect evidence of life within the martian surface via the deployment of a 2 meter drill. The ExoMars Pasteur payload contains several imaging and spectroscopic instruments key to this objective: the Panoramic Camera (PanCam), Infrared Spectrometer for ExoMars (ISEM), and Close‐UP Imager (CLUPI). These instruments are able to collect data at a variety of spatial (sub‐mm to decimeter) and spectral (3.3 to 120 nm) resolutions across the 440 to 3300 nm wavelength range and collectively will form a picture of the geological and morphological characteristics of the surface terrain surrounding the rover. We deployed emulators of this instrument suite at terrestrial analog sites that formed in a range of aqueous environments to test their ability to detect and characterize science targets. We find that the emulator suite is able to effectively detect, characterize, and refine the compositions of multiple targets at working distances spanning from 2‐18 m. We report on: (i) the detection of hydrothermal alteration minerals including Fe‐smectites and gypsum from basaltic substrates, (ii) the detection of late‐stage diagenetic gypsum veins embedded in exposures of sedimentary mudstone, (iii) multispectral evidence of compositional differences detected from fossiliferous mudstones, and (iv) approaches to cross‐referencing multi‐scale and multi‐resolution data. These findings aid in the development of data products and analysis toolkits in advance of the ExoMars rover mission.

U2 - 10.1029/2019EA000692

DO - 10.1029/2019EA000692

M3 - Article

VL - 7

JO - Earth and Space Science

JF - Earth and Space Science

SN - 2333-5084

IS - 4

M1 - e2019EA000692

ER -

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