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A shallow volatile layer at Chryse Planitia, Mars

Earth, Planets and Space volume 50, pages423–429(1998)Cite this article

Abstract

We have investigated size distribution of rampart craters in the east edge of Chryse Planitia on Mars by Viking high resolution images. Clear existence of the onset diameter of rampart crater, which defines the minimum size of the rampart crater, has been recognized. If this diameter corresponds to the depth to the top of the volatile layer, the converted depth ranges from ∼20 m to 60 m. These values are systematically shallower than the previous estimates (Kuzmin, 1988). Martian volatile layer is thought as a main reservoir of the ancient fluvial processes and atmospheric water vapor. This shallow volatile layer gives us information of the inventory of Martian water and conditions of cryosphere.

References

  1. Boyce, J. M., Distribution of thermal gradient values in the equatorial region of Mars based on impact crater morphology, Reports of Planetary Geology Program-1980 NASA TM 82385, 140–143, 1980.

  2. Carr, M. H., Water on Mars, 229pp., Oxford Univ. Press, New York, 1996.

  3. Carr, M. H., et al., Martian impact craters and emplacement of ejecta by surface flow, J. Geophys. Res., 82, 4,055–4,065, 1977.

  4. Clifford, S. M., A model for the hydrologic and climatic behavior of water on Mars, J. Geophys. Res., 98, 10,973–11,016, 1993.

  5. Costard, F. M., The spatial distribution of volatiles in the Martian hydrolithosphere, Earth Moon Planets, 45, 265–290, 1989.

  6. Costard, F. M. and J. S. Kargel, Outwash plains and thermokarst on Mars, Icarus, 114, 93–112, 1995.

  7. Croft, S. K., Cratering flow fields: Implications for the excavation and transient expansion stages of crater formation, Proc. Lunar Planet. Sci. Conf., 11, 2,347–2,378, 1980. Fanale, F. P. et al., Global distribution and migration of sub-surface ice on Mars, Icarus, 67, 1–18, 1986.

  8. Grieve, R. A. F., Terrestrial impact structures, Ann. Rev. Earth Planet. Sci., 15, 245–270, 1987.

  9. Grieve, R. A. F. and J. B. Garvin, A geometric model for excavation and modification at terrestrial simple craters, J. Geophys. Res., 89, 11,561–11,572, 1984.

  10. Jakosky, B. M. and J. H. Jones, The history of Martian volatiles, Rev. Geophys., 35, 1–16, 1997.

  11. Kuzmin, R. O., Structure inhomogeneities of the Martian cryosphere, Solar System Res., 22, 195–212, 1988 (compiled by S. W. Squyres et al., Chapt. 16 in Mars, 1489pp., Univ. Arizona Press, Tucson, 1992).

  12. McSween, H. Y., What we have learned about Mars from SNC meteorites, Meteoritics, 29, 757–779, 1994.

  13. Melosh, H. J., Impact Cratering, 245pp., Oxford Univ. Press, New York, 1989.

  14. Mouginis-Mark, P. J., Morphology of Martian rampart craters, Nature, 272, 691–694, 1978.

  15. Mouginis-Mark, P. J., Ejecta emplacement and modes of formation of Martian fluidized ejecta craters, Icarus, 45, 60–76, 1981.

  16. Mouginis-Mark, P. J., Water or ice in the Martian regolith?: clues from rampart craters seen at very high resolution, Icarus, 71, 268–286, 1987.

  17. Pike, R. J., Control of crater morphology by gravity and target type: Mars, Earth, Moon., Proc. Lunar Planet. Sci., 11th, 2,159–2,189, 1980.

  18. Pike, R. J., Mercury, Chapt. 7, 794pp., Univ. Arizona Press, Tucson, 1988.

  19. Rotto, S. and K. L. Tanaka, Geologic/geomorphologic map of the Chryse Planitia Region of Mars, U.S. Geological Survey MAP I-2441, 1995.

  20. Scott, D. H. et al., Map of Mars showing channels and possible paleolake basins, U.S. Geological Survey MAP I-2461, 1995.

  21. Sleep, N. H., Martian plate tectonics, J. Geophys. Res., 99, 5,639–5,655, 1994.

  22. Spudis, P. D., The Geology of Multi-Ring Impact Basins, 263pp., Cambridge Univ. Press, Cambridge, 1993.

  23. Stoffler, D. et al., Experimental hypervelocity impact into quartz sand: Distribution and shock metamorphism of ejecta, J. Geophys. Res., 80, 4,062–4,077, 1975.

  24. Tanaka, K. L., Sedimentary history and mass flow structures of Chryse and Acidalia Planitiae, Mars, J. Geophys. Res., 102, 4,131–4,149, 1997.

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Affiliations

  1. Department of Earth and Planetary Physics, University of Tokyo, 7-3-1 Hongou, Bunkyo, Tokyo, 113-0033, Japan
    • Hirohide Demura
    •  & Kei Kurita
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  1. Hirohide Demura
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  2. Kei Kurita
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Correspondence to Hirohide Demura.

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Demura, H., Kurita, K. A shallow volatile layer at Chryse Planitia, Mars. Earth Planet Sp 50, 423–429 (1998). https://doi.org/10.1186/BF03352129

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Keywords

  • Landing Site
  • Impact Crater
  • Atmospheric Water Vapor
  • Lunar Planet
  • Martian Surface