Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Originally published in Science Express on 30 November 2005
Science 23 December 2005:
Vol. 310. no. 5756, pp. 1925 - 1928
DOI: 10.1126/science.1122165

Research Articles

Radar Soundings of the Subsurface of Mars

Giovanni Picardi,1 Jeffrey J. Plaut,2* Daniela Biccari,1 Ornella Bombaci,3 Diego Calabrese,3 Marco Cartacci,1 Andrea Cicchetti,1 Stephen M. Clifford,4 Peter Edenhofer,5 William M. Farrell,6 Costanzo Federico,7 Alessandro Frigeri,7 Donald A. Gurnett,8 Tor Hagfors,9 Essam Heggy,4 Alain Herique,10 Richard L. Huff,8 Anton B. Ivanov,2 William T. K. Johnson,2 Rolando L. Jordan,2 Donald L. Kirchner,8 Wlodek Kofman,10 Carlton J. Leuschen,11 Erling Nielsen,9 Roberto Orosei,12 Elena Pettinelli,14 Roger J. Phillips,15 Dirk Plettemeier,16 Ali Safaeinili,2 Roberto Seu,1 Ellen R. Stofan,17 Giuliano Vannaroni,13 Thomas R. Watters,18 Enrico Zampolini3

The martian subsurface has been probed to kilometer depths by the Mars Advanced Radar for Subsurface and Ionospheric Sounding instrument aboard the Mars Express orbiter. Signals penetrate the polar layered deposits, probably imaging the base of the deposits. Data from the northern lowlands of Chryse Planitia have revealed a shallowly buried quasi-circular structure about 250 kilometers in diameter that is interpreted to be an impact basin. In addition, a planar reflector associated with the basin structure may indicate the presence of a low-loss deposit that is more than 1 kilometer thick.

1 Infocom Department, "La Sapienza" University of Rome, 00184 Rome, Italy.
2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
3 Alcatel Alenia Space Italia, 00131 Rome, Italy.
4 Lunar and Planetary Institute, Houston, TX 77058, USA.
5 Fakultaet fuer Elektrotechnik und Informationstechnik Ruhr-Universitaet Bochum, D-44780 Bochum, Germany.
6 NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA.
7 Dipartimento di Scienze della Terra, Università degli Studi di Perugia, 06123 Perugia, Italy.
8 Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA.
9 Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany.
10 Laboratoire de Planetologie de Grenoble, 38041 Grenoble Cedex, France.
11 Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA.
12 Istituto di Astrofisica Spaziale e Fisica Cosmica, 00133 Rome, Italy
13 Istituto di Fisica dello Spazio Interplanetario, Istituto Nazionale di Astrofisica, 00133 Rome, Italy.
14 Dipartimento di Fisica, University of Rome 3, 00146 Rome, Italy.
15 Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.
16 Fakultaet fuer Elektrotechnik und Informationstechnik, Technische Universitaet Dresden, D-01062 Dresden, Germany.
17 Proxemy Research, Laytonsville, MD 20882, USA.
18 Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA.

* To whom correspondence should be addressed. E-mail: plaut{at}jpl.nasa.gov

Read the Full Text


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Lunar Radar Sounder Observations of Subsurface Layers Under the Nearside Maria of the Moon.
T. Ono, A. Kumamoto, H. Nakagawa, Y. Yamaguchi, S. Oshigami, A. Yamaji, T. Kobayashi, Y. Kasahara, and H. Oya (2009)
Science 323, 909-912
   Abstract »    Full Text »    PDF »
Radar Sounding Evidence for Buried Glaciers in the Southern Mid-Latitudes of Mars.
J. W. Holt, A. Safaeinili, J. J. Plaut, J. W. Head, R. J. Phillips, R. Seu, S. D. Kempf, P. Choudhary, D. A. Young, N. E. Putzig, et al. (2008)
Science 322, 1235-1238
   Abstract »    Full Text »    PDF »
Mars North Polar Deposits: Stratigraphy, Age, and Geodynamical Response.
R. J. Phillips, M. T. Zuber, S. E. Smrekar, M. T. Mellon, J. W. Head, K. L. Tanaka, N. E. Putzig, S. M. Milkovich, B. A. Campbell, J. J. Plaut, et al. (2008)
Science 320, 1182-1185
   Abstract »    Full Text »    PDF »
Planetary science: Multiple data sets, multiple scales, and unlocking the third dimension.
P. Martin and E. R. Stofan (2007)
Geosphere 3, 435-455
   Abstract »    Full Text »    PDF »
Radar Sounding of the Medusae Fossae Formation Mars: Equatorial Ice or Dry, Low-Density Deposits?.
T. R. Watters, B. Campbell, L. Carter, C. J. Leuschen, J. J. Plaut, G. Picardi, R. Orosei, A. Safaeinili, S. M. Clifford, W. M. Farrell, et al. (2007)
Science 318, 1125-1128
   Abstract »    Full Text »    PDF »
Accumulation and Erosion of Mars' South Polar Layered Deposits.
R. Seu, R. J. Phillips, G. Alberti, D. Biccari, F. Bonaventura, M. Bortone, D. Calabrese, B. A. Campbell, M. Cartacci, L. M. Carter, et al. (2007)
Science 317, 1715-1718
   Abstract »    Full Text »    PDF »
Subsurface Radar Sounding of the South Polar Layered Deposits of Mars.
J. J. Plaut, G. Picardi, A. Safaeinili, A. B. Ivanov, S. M. Milkovich, A. Cicchetti, W. Kofman, J. Mouginot, W. M. Farrell, R. J. Phillips, et al. (2007)
Science 316, 92-95
   Abstract »    Full Text »    PDF »
The carbon cycle on early Earth--and on Mars?.
M. M Grady and I. Wright (2006)
Phil Trans R Soc B 361, 1703-1713
   Abstract »    Full Text »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)