Movatterモバイル変換


[0]ホーム

URL:


Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

Advertisement

Nature
  • Letter
  • Published:

Evidence for recent climate change on Mars from the identification of youthful near-surface ground ice

Naturevolume 412pages411–414 (2001)Cite this article

Abstract

Ground ice in the crust and soil may be one of the largest reservoirs of water on Mars1,2,3. Near-surface ground ice is predicted to be stable at latitudes higher than 40° (ref.4), where a number of geomorphologic features indicative of viscous creep and hence ground ice have been observed5. Mid-latitude soils have also been implicated as a water-ice reservoir6, the capacity of which is predicted to vary on a 100,000-year timescale owing to orbitally driven variations in climate7. It is uncertain, however, whether near-surface ground ice currently exists at these latitudes, and how it is changing with time. Here we report observational evidence for a mid-latitude reservoir of near-surface water ice occupying the pore space of soils. The thickness of the ice-occupied soil reservoir (1–10 m) and its distribution in the 30° to 60° latitude bands indicate a reservoir of (1.5–6.0) × 104 km3, equivalent to a global layer of water 10–40 cm thick. We infer that the reservoir was created during the last phase of high orbital obliquity less than 100,000 years ago, and is now being diminished.

This is a preview of subscription content,access via your institution

Access options

Access through your institution

Subscription info for Japanese customers

We have a dedicated website for our Japanese customers. Please go tonatureasia.com to subscribe to this journal.

Buy this article

  • Purchase on SpringerLink
  • Instant access to full article PDF

Prices may be subject to local taxes which are calculated during checkout

Figure 1: Examples of terrain interpreted to contain near-surface ground ice.
Figure 2: Global distribution of the image locations used in this investigation.
Figure 3: Latitude distribution of MOC frames showing dissection.

Similar content being viewed by others

References

  1. Squyres, S. W. Urey Prize Lecture: Water on Mars.Icarus79, 229–288 (1989).

    Article ADS CAS  Google Scholar 

  2. Carr, M. H.Water on Mars (Oxford Univ. Press, New York, 1996).

    Google Scholar 

  3. Clifford, S. M. A model for the hydrologic and climatic behavior of water on Mars.J. Geophys. Res.98, 10973–11016 (1993).

    Article ADS CAS  Google Scholar 

  4. Fanale, F. P., Salvail, J. R., Zent, A. P. & Postawko, S. E. Global distribution and migration of subsurface ice on Mars.Icarus67, 1–18 (1986).

    Article ADS CAS  Google Scholar 

  5. Squryes, S. W. & Carr, M. H. Geomorphic evidence for the distribution of ground ice on Mars.Science231, 249–252 (1986).

    Article ADS  Google Scholar 

  6. Houben, W., Haberle, R. M., Young, R. E. & Zent, A. P. Modeling the martian seasonal water cycle.J. Geophys. Res.102, 9069–9094 (1997).

    Article ADS  Google Scholar 

  7. Mellon, M. T. & Jakosky, B. M. The distribution and behavior of Martian ground ice during past and present epochs.J. Geophys. Res.100, 11781–11799 (1995).

    Article ADS  Google Scholar 

  8. Malin, M. C. et al. Early view of Martian surface from the mars Orbiter Camera of Mars Global Surveyor.Science279, 1681–1685 (1998).

    Article ADS CAS  Google Scholar 

  9. Edgett, K. S. & Malin, M. C. New views of Mars eolian activity, materials, and surface properties: Three vignettes from the Mars Global Surveyor Mars Orbiter Camera.J. Geophys. Res.105, 1623–1650 (2000).

    Article ADS  Google Scholar 

  10. Christensen, P. R. & Moore, H. J. inMars (eds Kieffer, H. H., Jakosky, B. M., Snyder, C. W. & Matthews, M. S.) 686–729 (Univ. Arizona Press, Tuscon, 1992).

    Google Scholar 

  11. Cooper, C. D. & Mustard, J. F. Criteria for remote sensing detection of sulfate cemented soils on Mars.Lunar Planet. Sci. [online]31, 1747 (2000).

    ADS  Google Scholar 

  12. Mustard, J. F. Recent ground ice on Mars and implications for volatiles and surface processes.Lunar Planet. Sci. [online]32, 1988 (2001).

    ADS  Google Scholar 

  13. Seibert, N. M. & Kargel, J. S. Small-scale martian polygonal terrain: Implications for liquid surface water.Geophys. Res. Lett.28, 899–902 (2001).

    Article ADS CAS  Google Scholar 

  14. Johnson, J. J. & Lorenz, R. D. Thermophysical properties of Alaskan loess: An analog material for the martian polar layered terrain?Geophys. Res. Lett.27, 2769–2772 (2000).

    Article ADS  Google Scholar 

  15. Storrs, A. D., Fanale, F. P., Saunders, R. S. & Stephens, J. B. The formation of filamentary sublimate residues (FSR) from mineral grains.Icarus76, 493–512 (1988).

    Article ADS CAS  Google Scholar 

  16. Haberle, R. M., Houben, W., Barnes, J. R. & Young, R. E. A simplified three-dimensional model for Martian climate studies.J. Geophys. Res.102, 9051–9068 (1997).

    Article ADS  Google Scholar 

  17. Metzger, S. M. et al. Dust devil vortices seen by the Mars Pathfinder camera.Geophys. Res. Lett.26, 2781–2784 (1999).

    Article ADS  Google Scholar 

  18. Renno, N. O. et al. Martian and terrestrial dust devils: Test of a scaling theory using Pathfinder data.J. Geophys. Res.105, 1859–1865 (2000).

    Article ADS  Google Scholar 

  19. Herkenhoff, K. E. & Plaut, J. J. Surface ages and resurfacing rates of the polar layered deposits on Mars.Icarus144, 243–253 (2000).

    Article ADS  Google Scholar 

  20. Kreslavsky, M. A. & Head, J. W. Kilometer scale roughness of Mars: Results from MOLA data analysis.J. Geophys. Res.105, 26695–26712 (2000).

    Article ADS  Google Scholar 

Download references

Acknowledgements

Discussions were provided by J. Head and P. Schultz and formal reviews were provided by M. Carr and B. Jakosky. The efforts of the MOC science team in creating the data base is gratefully acknowledged. This work is supported by grants from NASA.

Author information

Authors and Affiliations

  1. Department of Geological Sciences, Brown University, Providence, 02912, Rhode Island, USA

    John F. Mustard, Christopher D. Cooper & Moses K. Rifkin

Authors
  1. John F. Mustard
  2. Christopher D. Cooper
  3. Moses K. Rifkin

Corresponding author

Correspondence toJohn F. Mustard.

Rights and permissions

About this article

Cite this article

Mustard, J., Cooper, C. & Rifkin, M. Evidence for recent climate change on Mars from the identification of youthful near-surface ground ice.Nature412, 411–414 (2001). https://doi.org/10.1038/35086515

Download citation

This article is cited by

Access through your institution
Buy or subscribe

Advertisement

Search

Advanced search

Quick links

Nature Briefing

Sign up for theNature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox.Sign up for Nature Briefing

[8]ページ先頭

©2009-2025 Movatter.jp