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Originally published in Science Express on 30 May 2002
Science 5 July 2002:
Vol. 297. no. 5578, pp. 75 - 78
DOI: 10.1126/science.1073541

Reports

Global Distribution of Neutrons from Mars: Results from Mars Odyssey

W. C. Feldman,1* W. V. Boynton,2 R. L. Tokar,1 T. H. Prettyman,1 O. Gasnault,1 S. W. Squyres,3 R. C. Elphic,1 D. J. Lawrence,1 S. L. Lawson,1 S. Maurice,4 G. W. McKinney,1 K. R. Moore,1 R. C. Reedy1

Global distributions of thermal, epithermal, and fast neutron fluxes have been mapped during late southern summer/northern winter using the Mars Odyssey Neutron Spectrometer. These fluxes are selectively sensitive to the vertical and lateral spatial distributions of H and CO2 in the uppermost meter of the martian surface. Poleward of ±60° latitude is terrain rich in hydrogen, probably H2O ice buried beneath tens of centimeter-thick hydrogen-poor soil. The central portion of the north polar cap is covered by a thick CO2 layer, as is the residual south polar cap. Portions of the low to middle latitudes indicate subsurface deposits of chemically and/or physically bound H2O and/or OH.

1 Los Alamos National Laboratory, Los Alamos, NM 87545, USA.
2 University of Arizona, Lunar Planetary Laboratory, Tucson, AZ 85721, USA.
3 Cornell University, Center for Radiophysics and Space Research, Ithaca, NY 14853, USA.
4 Observatoire Midi-Pyrénées, 31400 Toulouse, France.
*   To whom correspondence should be addressed. E-mail: wfeldman{at}lanl.gov


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