The WISDOM Radar onboard the Rover of the ExoMars mission

International audience The most fundamental and basic aspect of the geologic characterization of any environment is understanding its stratigraphy and structure - which provides invaluable insights into its origin, the processes and events by which it evolved, and (through the examination of superpo...

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Main Authors: Ciarletti, Valérie, Corbel, Charlotte, Plettemeier, D., Clifford, S. M., Cais, Ph., Hamran, S.
Other Authors: ESTER - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Technische Universität Dresden = Dresden University of Technology (TU Dresden), Lunar and Planetary Institute Houston (LPI), Observatoire aquitain des sciences de l'univers (OASU), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB), Laboratoire d'Astrophysique de Bordeaux Pessac (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB), Norwegian Defence Research Establishment (FFI)
Format: Conference Object
Language:English
Published: HAL CCSD 2009
Subjects:
Online Access:https://hal.science/hal-00570221
id ftuniversailles:oai:HAL:hal-00570221v1
record_format openpolar
institution Open Polar
collection Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ
op_collection_id ftuniversailles
language English
topic Remote sensing
Instruments and techniques
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
spellingShingle Remote sensing
Instruments and techniques
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
Ciarletti, Valérie
Corbel, Charlotte
Plettemeier, D.
Clifford, S. M.
Cais, Ph.
Hamran, S.
The WISDOM Radar onboard the Rover of the ExoMars mission
topic_facet Remote sensing
Instruments and techniques
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
description International audience The most fundamental and basic aspect of the geologic characterization of any environment is understanding its stratigraphy and structure - which provides invaluable insights into its origin, the processes and events by which it evolved, and (through the examination of superpositional and cross-cutting relationships) their relative timing. The WISDOM GPR onboard the Rover of the ESA ExoMars mission (2016) has the ability to investigate and characterize the nature of the subsurface remotely, providing high-resolution (several cm-scale) data on subsurface stratigraphy, structure, and the magnitude and scale of spatial heterogeneity, to depths in excess of 3 m. Unlike traditional imaging systems or spectrometers, which are limited to characterization of the visible surface, WISDOM can access what lies beneath - providing an understanding of the 3-dimensional geologic context of the landing site along the Rover path. WISDOM will address a variety of high-priority scientific objectives: (1) Understand the geology and geologic evolution of the landing site, including local lithology, stratigraphy and structure. (2) Characterize the 3-D electromagnetic properties of the Landing Site - including the scale and magnitude of spatial heterogeneity - for comparison with those measured at larger scales by MARSIS, SHARAD and any future orbital radars. (3) Understand the local distribution and state of shallow subsurface H2O and other volatiles, including the potential presence of segregated ground ice (as ice lenses and wedges), the persistent or transient occurrence of liquid water/brine, and deposits of methane hydrate and (4) identify the most promising locations for drilling that combine targets of high scientific interest. In addition to these objectives, there are also clear scientific and operational benefits when WISDOM is operated in concert with the rover's drill and its associated analytical instruments, which will determine the compositional and physical properties of retrieved core ...
author2 ESTER - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Technische Universität Dresden = Dresden University of Technology (TU Dresden)
Lunar and Planetary Institute Houston (LPI)
Observatoire aquitain des sciences de l'univers (OASU)
Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Université Sciences et Technologies - Bordeaux 1 (UB)
Laboratoire d'Astrophysique de Bordeaux Pessac (LAB)
Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB)
Norwegian Defence Research Establishment (FFI)
format Conference Object
author Ciarletti, Valérie
Corbel, Charlotte
Plettemeier, D.
Clifford, S. M.
Cais, Ph.
Hamran, S.
author_facet Ciarletti, Valérie
Corbel, Charlotte
Plettemeier, D.
Clifford, S. M.
Cais, Ph.
Hamran, S.
author_sort Ciarletti, Valérie
title The WISDOM Radar onboard the Rover of the ExoMars mission
title_short The WISDOM Radar onboard the Rover of the ExoMars mission
title_full The WISDOM Radar onboard the Rover of the ExoMars mission
title_fullStr The WISDOM Radar onboard the Rover of the ExoMars mission
title_full_unstemmed The WISDOM Radar onboard the Rover of the ExoMars mission
title_sort wisdom radar onboard the rover of the exomars mission
publisher HAL CCSD
publishDate 2009
url https://hal.science/hal-00570221
op_coverage San Francisco, United States
long_lat ENVELOPE(-45.689,-45.689,-60.733,-60.733)
geographic The Landing
geographic_facet The Landing
genre Methane hydrate
genre_facet Methane hydrate
op_source AGU Fall Meeting 2009
https://hal.science/hal-00570221
AGU Fall Meeting 2009, Dec 2009, San Francisco, United States
op_relation hal-00570221
https://hal.science/hal-00570221
BIBCODE: 2009AGUFM.P11D.06C
_version_ 1782336640789774336
spelling ftuniversailles:oai:HAL:hal-00570221v1 2023-11-12T04:20:58+01:00 The WISDOM Radar onboard the Rover of the ExoMars mission Ciarletti, Valérie Corbel, Charlotte Plettemeier, D. Clifford, S. M. Cais, Ph. Hamran, S. ESTER - LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Technische Universität Dresden = Dresden University of Technology (TU Dresden) Lunar and Planetary Institute Houston (LPI) Observatoire aquitain des sciences de l'univers (OASU) Université Sciences et Technologies - Bordeaux 1 (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Université Sciences et Technologies - Bordeaux 1 (UB) Laboratoire d'Astrophysique de Bordeaux Pessac (LAB) Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux (L3AB) Norwegian Defence Research Establishment (FFI) San Francisco, United States 2009-12-14 https://hal.science/hal-00570221 en eng HAL CCSD hal-00570221 https://hal.science/hal-00570221 BIBCODE: 2009AGUFM.P11D.06C AGU Fall Meeting 2009 https://hal.science/hal-00570221 AGU Fall Meeting 2009, Dec 2009, San Francisco, United States Remote sensing Instruments and techniques [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] info:eu-repo/semantics/conferenceObject Conference papers 2009 ftuniversailles 2023-10-31T23:40:04Z International audience The most fundamental and basic aspect of the geologic characterization of any environment is understanding its stratigraphy and structure - which provides invaluable insights into its origin, the processes and events by which it evolved, and (through the examination of superpositional and cross-cutting relationships) their relative timing. The WISDOM GPR onboard the Rover of the ESA ExoMars mission (2016) has the ability to investigate and characterize the nature of the subsurface remotely, providing high-resolution (several cm-scale) data on subsurface stratigraphy, structure, and the magnitude and scale of spatial heterogeneity, to depths in excess of 3 m. Unlike traditional imaging systems or spectrometers, which are limited to characterization of the visible surface, WISDOM can access what lies beneath - providing an understanding of the 3-dimensional geologic context of the landing site along the Rover path. WISDOM will address a variety of high-priority scientific objectives: (1) Understand the geology and geologic evolution of the landing site, including local lithology, stratigraphy and structure. (2) Characterize the 3-D electromagnetic properties of the Landing Site - including the scale and magnitude of spatial heterogeneity - for comparison with those measured at larger scales by MARSIS, SHARAD and any future orbital radars. (3) Understand the local distribution and state of shallow subsurface H2O and other volatiles, including the potential presence of segregated ground ice (as ice lenses and wedges), the persistent or transient occurrence of liquid water/brine, and deposits of methane hydrate and (4) identify the most promising locations for drilling that combine targets of high scientific interest. In addition to these objectives, there are also clear scientific and operational benefits when WISDOM is operated in concert with the rover's drill and its associated analytical instruments, which will determine the compositional and physical properties of retrieved core ... Conference Object Methane hydrate Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ The Landing ENVELOPE(-45.689,-45.689,-60.733,-60.733)