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Potential of Probing the Lunar Regolith using Rover-Mounted Ground Penetrating Radar: Moses Lake Dune Field Analog StudyProbing radars have been widely recognized by the science community to be an efficient tool to explore lunar subsurface providing a unique capability to address several scientific and operational issues. A wideband (200 to 1200 MHz) Ground Penetrating Radar (GPR) mounted on a surface rover can provide high vertical resolution and probing depth from few tens of centimeters to few tens of meters depending on the sounding frequency and the ground conductivity. This in term can provide a better understand regolith thickness, elemental iron concentration (including ilmenite), volatile presence, structural anomalies and fracturing. All those objectives are of important significance for understanding the local geology and potential sustainable resources for future landing sites in particular exploring the thickness, structural heterogeneity and potential volatiles presence in the lunar regolith. While the operation and data collection of GPR is a straightforward case for most terrestrial surveys, it is a challenging task for remote planetary study especially on robotic platforms due to the complexity of remote operation in rough terrains and the data collection constrains imposed by the mechanical motion of the rover and limitation in data transfer. Nevertheless, Rover mounted GPR can be of great support to perform systematic subsurface surveys for a given landing site as it can provide scientific and operational support in exploring subsurface resources and sample collections which can increase the efficiency of the EVA activities for potential human crews as part of the NASA Constellation Program. In this study we attempt to explore the operational challenges and their impact on the EVA scientific return for operating a rover mounted GPR in support of potential human activity on the moon. In this first field study, we mainly focused on the ability of GPR to support subsurface sample collection and explore shallow subsurface volatiles.
Document ID
20090012408
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Horz, F.
(NASA Johnson Space Center Houston, TX, United States)
Heggy, E.
(Institut de Physique du Globe Saint-Maur-des-Fosses, France)
Fong, T.
(NASA Ames Research Center Moffett Field, CA, United States)
Kring, D.
(Lunar and Planetary Inst. Houston, TX, United States)
Deans, M.
(NASA Ames Research Center Moffett Field, CA, United States)
Anglade, A.
(Institut de Physique du Globe Saint-Maur-des-Fosses, France)
Mahiouz, K.
(Institut de Physique du Globe Saint-Maur-des-Fosses, France)
Bualat, M.
(NASA Ames Research Center Moffett Field, CA, United States)
Lee, P.
(Mars Inst. Moffett Field, CA, United States)
Bluethmann, W.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 24, 2013
Publication Date
March 23, 2009
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-18026
Meeting Information
Meeting: 40th Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 23, 2009
End Date: March 27, 2009
Distribution Limits
Public
Copyright
Public Use Permitted.
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