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Regions of Potential Existence of Free Water (Ice) in the Near-Surface Martian Ground: Results from theMars OdysseyHigh-Energy Neutron Detector (HEND)

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Abstract

We report results of the analysis of the data on global mapping of neutron fluxes from the Martian surface, which have been obtained during the first ten months of measurements carried out by the Russian high-energy neutron detector HEND mounted aboard the AmericanMars Odysseyorbiter. This analysis allowed us to separate regions where free water (in ice form) prevailed in the surface layer (with a thickness of up to 2 m) of the Martian ground from regions where physically and chemically bound ground water was most likely to be the dominant form of water. The global mapping of regions with increased ice content in the ground-surface layer revealed a direct correlation with regions of polygonal terrains morphologically similar to terrestrial polygonal forms of permafrost origin. The potential content of bound water forms in the ground of circumpolar areas of the planet is also estimated.

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REFERENCES

  • Banin, A., Clark, B.C., and Wanke, H., Surface Chemistry and Mineralogy, inMars, Kieffer, H.H.,et al., Eds., Tucson: Univ. of Arizona Press, 1992, pp. 594-625.

    Google Scholar 

  • Boynton, W.V., Feldman, W.C., Squyres, S.W.,et al., Distribution of Hydrogen in the Near-Surface of Mars: Evidence for Subsurface Ice Deposits,Science, 2002, vol. 297, pp. 81-87.

    Google Scholar 

  • Christensen, P.R., Bandfield, J.L., Hamilton, V.E.,et al.,Mars Global SurveyorThermal Emission Spectrometer Experiment: Investigation Description and Surface Science Results,J. Geophys. Res., 2001, vol. 106, pp. 23823-23871.

    Google Scholar 

  • Clark, B.C. and Van Hart, D.C., The Salts of Mars,Icarus, 1981, vol. 45, pp. 370-378.

    Google Scholar 

  • Clifford, S.M. and Hillel, D., The Stability of Ground Ice in the Equatorial Regions of Mars,J. Geophys. Res., 1983, vol. 88, pp. 2456-2474.

    Google Scholar 

  • Clifford, S.V., Bartels, C.J., and Rubenstein, E.F., The Mars Thermal Model (MARSTHERM): A FORTRAN 77 Finite-Difference Program Designed for General Distribution, Houston: LPI, 1987.

    Google Scholar 

  • Fanale, F.P., Martian Volatiles: Their Degassing History and Geochemical Fate,Icarus, 1976, vol. 28, pp. 179-202.

    Google Scholar 

  • Fanale, F.P., The Water and Other Volatiles of Mars,Sci. Technol. Ser Am. Astronautical Soc. Publ., 1986, vol. 71, pp. 157-174.

    Google Scholar 

  • Farmer, C.B. and Doms, P.E., Global and Seasonal Water Vapor on Mars and Implications for Permafrost,J. Geophys. Res., 1979, vol. 84, pp. 2881-2888.

    Google Scholar 

  • Feldman, W.C., Boynton, W.V., and Drake, D.M., Planetary Neutron Spectroscopy from Orbit, inRemote Geochemical Analysis: Elemental and Mineralogical Composition, Piters, C.M. and Englert, A.J., Eds., Cambridge, Cambridge Univ. Press, 1993, pp. 213-234.

    Google Scholar 

  • Feldman, W.C., Boynton, W.V., Tokar, R.L.,et al., Global Distribution of Neutrons from Mars: Results fromMars Odyssey,Science, 2002, vol. 297, pp. 75-78.

    Google Scholar 

  • Greeley, R. and Guest, J.E., Geologic Map of the Eastern Equatorial Region of Mars,US Geologic Survey, Misc. Inv. Map I-802-B, 1987.

  • Kuzmin, R.O., On the Structure of the Martian Cryolithosphere, inProblemy kriolitologii(Problems of Cryolithology), iss. 6, Moscow: Izd. MGU, 1977, pp. 7-23.

    Google Scholar 

  • Kuzmin, R.O.,Kriolitosfera Marsa(Martian Cryolithosphere), Moscow: Nauka, 1983.

    Google Scholar 

  • Kuzmin, R.O., Bobina, N.N., Zabalueva, E.V., and Shashkina, V.P., Structural Inhomogeneities of the Martian Cryolithosphere,Astron. Vestn., 1988, vol. 22,no. 3, pp. 195-212.

    Google Scholar 

  • Kuzmin, R.O., Komarov, I.A., Isaev, V.S.,et al., The Comparative Morphometric Analysis of Polygonal Terrains on Mars and the Earth High Latitude Areas,Lunar Planet. Sci. Conf. XXXII, 2002, Abstract # 2030.

  • Kuzmin, R.O., Specific Character of the Superficial Layer of the Martian Cryolithosphere,Workshop HEND, 2002 May 20–22 (www.iki.rssi.ru/eng/hendws.htm).

  • Kuzmin, R.O., Mitrofanov, I.G., Litvak, M.L.,et al., Mars: Detaching of the Free Water Signature (FTS) Presence Regions on the Base of HEND/OdysseyData and Their Correlation with Some Permafrost Features from MOC Data,Lunar Planet. Sci. Conf. XXXIV, 2003, Abstract # 1369.

  • Kuzmin, R.O. and Zabalueva, E.V., Polygonal Terrains on Mars: Preliminary Results of Global Mapping of Their Spatial Distribution,Lunar Planet. Sci. Conf. XXXIV, 2003, Abstract # 1912.

  • Leighton, R.B. and Murray, B.C., Behavior of Carbon Dioxide and Other Volatiles on Mars,Science, 1966, vol. 153, pp. 136-144.

    Google Scholar 

  • Litvak, M.L., Mitrofanov, I.G., Kozyrev, A.S.,et al., Seasonal Variations of Subsurface Hydrogen as Seen by High Energy Neutron Detector,Mars Odyssey, 36th Brown Vernadsky Microsymposium, 2002.

  • McSween, H.Y., Murchie, S.L., Crisp, J.A.,et al., Chemical, Multispectral, and Textural Constraints on the Composition and Origin of Rocks at theMars PathfinderLanding Site,J. Geophys. Res., 1999, vol. 104, pp. 8679-8716.

    Google Scholar 

  • Mellon, M.T. and Jakosky, B.M., The Distribution and Behavior of Martian Ground Ice during Past and Present Epochs,J. Geophys. Res., 1995, vol. 100, pp. 11781-11800.

    Google Scholar 

  • Mellon, M.T., Kretke, K.A., Smith, M.D.,et al., A Global Map of Thermal Inertia fromMars Global SurveyorMapping-Mission Data,Lunar Planet Sci. Conf. XXXIII, 2002, Abstract # 1416.

  • Mitrofanov, I.G., Anfimov, D., Kozyrev, A.,et al., Maps of Subsurface Hydrogen from the High Energy Neutron Detector, Mars,Science,2002, vol. 297, pp. 78-81.

    Google Scholar 

  • Pollack, J.B., Roush, T., Witteborn, F.,et al., Thermal Emission Spectra of Mars (5.4–10.5 μ),J. Geophys. Res., 1990, vol. 95, pp. 14595-14627.

    Google Scholar 

  • Reider, R., Economov, T., Wanke, H.,et al., The Chemical Composition of Martian Soil and Rocks Returned by the Mobile X-Ray Mode,Science, 1997, vol. 278, pp. 1771-1774.

    Google Scholar 

  • Romanovskii, N.N.,Formirovanie poligonal'no-zhil'nykh struktur(Formation of Polygonal-veined Structures), Novosibirsk: Nauka, 1977.

    Google Scholar 

  • Scott, D. and Tanaka, K., Geologic Map of the Western Equatorial Region of Mars,US Geological Survey, Misc. Inv. Map I-802-A, 1986.

  • Seibert, N.M. and Kargel, J.S., Small-Scale Martian Polygonal Terrain: Implications for Liquid Surface Water,Geophys. Res. Lett., 2001, vol. 28,no. 5, pp. 899-902.

    Google Scholar 

  • Smith, D.E., Zuber, M.T., Frey, H.,et al., The Global Topography of Mars and Implication for Surface Evolution,Science, 1999, vol. 284, pp. 1495-1503.

    Google Scholar 

  • Smith, D.E., Zuber, M.T., and Neumann, G.A., Seasonal Variations of Snow Depth on Mars,Science, 2001, vol. 294, pp. 2141-2146.

    Google Scholar 

  • Soderblom, L., The Composition and Mineralogy of the Martian Surface from Spectroscopic Observations: 0.3 μ–50 μ, inMars, Kieffer, H.H.,et al., Eds., Tucson: Univ. of Arizona Press, 1992, pp. 557-593.

    Google Scholar 

  • Surkov, Yu.A., Shcheglov, O.P., Ryvkin, M.L., and Vinogradova, O.A., Neutron Spectrometry, inRemote Geochemical Analysis: Elemental and Mineralogical Composition, Piters, C.M. and Englert, A.J., Eds., Cambridge: Cambridge Univ. Press, 1998, pp. 427-442.

    Google Scholar 

  • Yoshikawa, K., Contraction Cracking and Ice Wedge Polygons in Mars,Second Mars Polar Sci. Conf., 2000, Abstract # 4045.

  • Zolotov, M.Yu., Water-bearing Minerals in the Martian Soil (Thermodynamic Prediction of Stability),Lunar Planet, Sci. Conf. XX, 1989, pp. 1257-1258.

  • Zolotov, M.Yu., Zabalueva, E.V., and Kuzmin, R.O., Stability of Hydrated Salts and Goethite within the Desiccated Upper Layer of the Martian Regolith,Lunar Planet. Sci. Conf. XXVIII, 1997, pp. 1633-1634.

  • Zurek, R.W., Barnes, J.B., Haberle, R.M.,et al., Dynamics of the Atmosphere of Mars, inMars, Kieffer, H.H.,et al., Eds., Tucson: Univ. of Arizona Press, 1992, pp. 835-933.

    Google Scholar 

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Authors and Affiliations

  1. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, ul. Kosygina 19, Moscow, 117975, Russia

    R. O. Kuzmin & E. V. Zabalueva

  2. Space Research Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117810, Russia

    I. G. Mitrofanov & M. L. Litvak

  3. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, 85721, USA

    W. V. Boynton

  4. Jet Propulsion Laboratory, Pasadena, CA, 91109, USA

    R. S. Saunders

Authors
  1. R. O. Kuzmin
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  2. E. V. Zabalueva
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  3. I. G. Mitrofanov
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  4. M. L. Litvak
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  5. W. V. Boynton
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  6. R. S. Saunders
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Kuzmin, R.O., Zabalueva, E.V., Mitrofanov, I.G. et al. Regions of Potential Existence of Free Water (Ice) in the Near-Surface Martian Ground: Results from theMars OdysseyHigh-Energy Neutron Detector (HEND). Solar System Research 38, 1–11 (2004). https://doi.org/10.1023/B:SOLS.0000015150.61420.5b

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  • DOI: https://doi.org/10.1023/B:SOLS.0000015150.61420.5b

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