WISDOM GPR Designed for Shallow and High-Resolution Sounding of the Martian Subsurface

The Water Ice Subsurface Deposit Observation on Mars (WISDOM) Ground Penetrating Radar (GPR) is one of the instruments that have been selected as part of the Pasteur payload of the European Space Agency's (ESA's) 2018 ExoMars Rover mission. The main scientific objectives of the mission are to search for evidence of past and present life and to characterize the nature of the shallow subsurface. The Rover is equipped with a drill that can sample the subsurface down to a depth of approximately 2 m. The WISDOM GPR is the only instrumentation capable of obtaining information about the nature of the subsurface along the Rover path before drilling. WISDOM has been designed to explore the first ~3 m of the subsurface with a vertical resolution of a few centimeters. The paper presents a description of the WISDOM instrument with a particular emphasis on the electronic architecture and antenna design that have been chosen to meet the challenging technical objectives. Some preliminary measurements obtained with the prototype are given to illustrate the instrument's potential performance.

[1]  G. G. Stokes "J." , 1890, The New Yale Book of Quotations.

[2]  D. Page Recent low-latitude freeze–thaw on Mars , 2007 .

[3]  John F. Mustard,et al.  Recent ice ages on Mars , 2003, Nature.

[4]  Dirk Plettemeier,et al.  Ultra light-weight antenna system for full polarimetric GPR applications , 2009, IEEE EUROCON 2009.

[5]  Stephen M. Clifford,et al.  The Evolution of the Martian Hydrosphere. , 2001 .

[6]  W. Marsden I and J , 2012 .

[7]  J. Emery,et al.  Young (late Amazonian), near-surface, ground ice features near the equator, Athabasca Valles, Mars , 2005 .

[8]  A. P. Annan,et al.  Impulse radar sounding in permafrost , 1976 .

[9]  D. Ming,et al.  Detection of Perchlorate and the Soluble Chemistry of Martian Soil at the Phoenix Lander Site , 2009, Science.

[10]  T. Parker,et al.  The Evolution of the Martian Hydrosphere: Implications for the Fate of a Primordial Ocean and the Current State of the Northern Plains , 2001 .

[11]  D. Plettemeier,et al.  A prototype for the WISDOM GPR on the ExoMars mission , 2007, 2007 4th International Workshop on, Advanced Ground Penetrating Radar.

[12]  James A. Doolittle,et al.  Detection of subsurface permafrost features with ground‐penetrating radar, Barrow, Alaska , 2001 .

[13]  Steven A. Arcone,et al.  Ground-penetrating radar reflection profiling of groundwater and bedrock in an area of discontinuous permafrost , 1998 .

[14]  M. Carr D/H on Mars - Effects of floods, volcanism, impacts, and polar processes , 1990 .

[15]  D. Burt,et al.  Eutectic Brines on Mars: Origin and Possible Relation to Young Seepage Features , 2002 .

[16]  P. Strevens Iii , 1985 .

[17]  Nicolas Thomas,et al.  Distribution of Mid-Latitude Ground Ice on Mars from New Impact Craters , 2009, Science.

[18]  Gary R. Olhoeft,et al.  Electromagnetic Properties of Martian Analog Minerals at Radar Frequencies and Martian Temperatures , 2006 .

[19]  James W. Head,et al.  Mars: Nature and evolution of young latitude‐dependent water‐ice‐rich mantle , 2002 .

[20]  Jeffrey S. Kargel,et al.  Outwash Plains and Thermokarst on Mars , 1995 .

[21]  G. Brass,et al.  Stability of brines on Mars , 1980 .

[22]  D. T. Gjessing,et al.  Ground penetrating synthetic pulse radar: dynamic range and modes of operation , 1995 .

[23]  B. Clark,et al.  The salts of Mars , 1981 .

[24]  Frances Westall,et al.  Two rovers to the same site on Mars, 2018: possibilities for cooperative science. , 2010, Astrobiology.

[25]  P. Box The Use of Geophysical Methods to Discriminate between Brine Layers and Freshwater Taliks in Permafrost Regions , 2004 .