Earth-like sand fluxes on Mars

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Strong and sustained winds on Mars have been considered rare, on the basis of surface meteorology measurements and global circulation models1,2, raising the question of whether the abundant dunes and evidence for wind erosion seen on the planet are a current process. Recent studies3,4,5,6 showed sand activity, but could not determine whether entire dunes were moving—implying large sand fluxes—or whether more localized and surficial changes had occurred. Here we present measurements of the migration rate of sand ripples and dune lee fronts at the Nili Patera dune field. We show that the dunes are near steady state, with their entire volumes composed of mobile sand. The dunes have unexpectedly high sand fluxes, similar, for example, to those in Victoria Valley, Antarctica, implying that rates of landscape modification on Mars and Earth are similar.

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Figure 1: Ripple migration, dune migration and dune elevation.
Figure 2: Linear correlation between ripple migration and dune height.
Figure 3: Dune migration rates.
Figure 4: Comparison of dune migration rates and sand flux on Mars and Earth.


  1. 1

    Arvidson, R. E., Guinness, E. A., Moore, H. J., Tillman, J. & Wall, S. D. Three Mars years: Viking Lander 1 imaging observations. Science 222, 463–468 (1983)

  2. 2

    Haberle, R. M., Murphy, J. R. & Schaeffer, J. Orbital change experiments with a Mars General Circulation Model. Icarus 161, 66–89 (2003)

  3. 3

    Silvestro, S., Fenton, L. K., Vaz, D. A., Bridges, N. T. & Ori, G. G. Ripple migration and dune activity on Mars: Evidence for dynamic processes. Geophys. Res. Lett. 37, L20203 (2010)

  4. 4

    Chojnacki, M., Burr, D. M., Moersch, J. E. & Michaels, T. I. Orbital observations of contemporary dune activity in Endeavour Crater, Meridiani Planum, Mars. J. Geophys. Res. 116, E00F19 (2011)

  5. 5

    Hansen, C. J. et al. Seasonal erosion and restoration of Mars’ northern polar dunes. Science 331, 575–578 (2011)

  6. 6

    Bridges, N. T. et al. Planet-wide sand motion on Mars. Geology 40, 31–34 (2012)

  7. 7

    Malin, M. C. & Edgett, K. S. Mars Global Surveyor Mars Orbiter Camera: Interplanetary cruise through primary mission. J. Geophys. Res. 106, 23,429–23,570 (2001)

  8. 8

    Laity, J. E. & Bridges, N. T. Ventifacts on Earth and Mars: Analytical, field, and laboratory studies supporting sand abrasion and windward feature development. Geomorphology 105, 202–217 (2009)

  9. 9

    Claudin, P. & Andreotti, B. A scaling law for aeolian dunes on Mars, Venus, Earth, and for subaqueous ripples. Earth Planet. Sci. Lett. 252, 30–44 (2006)

  10. 10

    Sullivan, R. et al. Wind-driven particle mobility on Mars: Insights from Mars Exploration Rover observations at “El Dorado” and surroundings at Gusev Crater. J. Geophys. Res. 113, E06S07 (2008)

  11. 11

    Armstrong, J. C. & Leovy, C. B. Long-term wind erosion on Mars. Icarus 176, 57–74 (2005)

  12. 12

    Leprince, S., Barbot, S., Ayoub, F. & Avouac, J. P. Automatic and precise orthorectification, coregistration, and subpixel correlation of satellite images, application to ground deformation measurements. IEEE Trans. Geosci. Rem. Sens. 45, 1529–1558 (2007)

  13. 13

    Vermeesch, P. & Drake, N. Remotely sensed dune celerity and sand flux measurements of the world's fastest barchans (Bodélé, Chad). Geophys. Res. Lett. 35, L24404 (2008)

  14. 14

    McEwen, A. S. et al. The High Resolution Imaging Science Experiment (HiRISE) during MRO’s Primary Science Phase (PSP). Icarus 205, 2–37 (2010)

  15. 15

    Ould Ahmedou, D. et al. Barchan dune mobility in Mauritania related to dune and interdune sand fluxes. J. Geophys. Res. 112, F02016 (2007)

  16. 16

    Andreotti, B., Claudin, P. & Pouliquen, O. Aeolian sand ripples: experimental evidence of fully developed states. Phys. Rev. Lett. 96, 028001 (2006)

  17. 17

    Anderson, R. S. A theoretical model for aeolian impact ripples. Sedimentology 34, 943–956 (1987)

  18. 18

    Andreotti, B. A two-species model of aeolian sand transport. J. Fluid Mech. 510, 47–70 (2004)

  19. 19

    Bourke, M. C., Ewing, R. C., Finnegan, D. & McGowan, H. A. Sand dune movement in Victoria Valley, Antarctica. Geomorphology 109, 148–160 (2009)

  20. 20

    Fenton, L. K. &. M. i. c. h. a. e. l. s. T. J. Characterizing the sensitivity of daytime turbulent activity on Mars with the MRAMS LES: early results. Mars 5, 159–171 (2010)

  21. 21

    Fenton, L. J., Toigo, A. & Richardson, M. I. Aeolian processes in Proctor Crater on Mars: mesoscale modeling of dune-forming winds. J. Geophys. Res. 110, E06005 (2005)

  22. 22

    Spiga, A. & Forget, F. A new model to simulate the Martian mesoscale and microscale atmospheric circulation: validation and first results. J. Geophys. Res. 114, E02009 (2009)

  23. 23

    Bagnold, R. A. The Physics of Blown Sand and Desert Dunes (Dover Publications, 1954)

  24. 24

    Kok, J. F. Difference in the wind speeds required for initiation versus continuation of sand transport on Mars: implications for dunes and dust storms. Phys. Rev. Lett. 104, 074502 (2010)

  25. 25

    Greeley, R. et al. Rate of wind abrasion on Mars. J. Geophys. Res. 87, 10,009–10,024 (1982)

  26. 26

    Malin, M. C. Rates of geomorphic modification in ice-free areas, southern Victoria Land, Antarctica. Antarct. J. US 20, 18–21 (1986)

  27. 27

    Golombek, M. P. et al. Erosion rates at the Mars Exploration Rover landing sites and long-term climate change on Mars. J. Geophys. Res. 111, E12S10 (2006)

  28. 28

    Long, J. T. & Sharp, R. S. Barchan-dune movement in Imperial Valley, California. Geol. Soc. Am. Bull. 75, 149–156 (1964)

  29. 29

    Fryberger, S. et al. Wind sedimentation in the Jafurah sand sea, Saudi Arabia. Sedimentology 31, 413–431 (1984)

  30. 30

    Lancaster, N. Controls on aeolian activity: some new perspectives from the Kelso Dunes, Mojave Desert, California. J. Arid Environ. 27, 113–125 (1994)

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Discussions with R. Ewing, C. Narteau, and S. Silvestro on bedforms and R. Kirk on stereo data significantly improved this research. This research was supported by grants from NASA’s Mars Data Analysis Program, the Keck Institute for Space Studies, and seed funding from the Jet Propulsion Laboratory's Director's Research and Development Fund.

Author information

N.T.B. is the principal investigator of the NASA MDAP grant that partially funded this work, chose the study area, defined major science questions, participated in data analysis, compared results to other Mars and terrestrial data, and led the writing of the paper. F.A. processed all the data with COSI-Corr, produced the figures and Supplementary Information ancillary materials, and played a major role in quantitative analysis and text writing. J-P.A. initiated the project, contributed fundamental ideas on sand flux and dune movement, supervised the data analysis and contributed to text writing. S.L. evaluated all COSI-Corr and quantitative results. A.L. provided expertise in interpretation of bedform movement and sand flux in regards to Mars surface evolution and climate models. S. M. produced the digital elevation model. All authors shared ideas and results and helped produce the final manuscript.

Correspondence to N. T. Bridges.

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The authors declare no competing financial interests.

Supplementary information

Supplementary Information

This file contains Supplementary Figures 1-4, Supplementary Methods, Supplementary Tables 1-2, Supplementary Text and Data and additional references. (PDF 3362 kb)

Supplementary Animation 1

This file contains an animated gif of a sub area of T1 and T2 illustrating the accurate bedrock registration and clear ripple migration. (GIF 369 kb)

Supplementary Animation 2

This file shows Lee front advance (label b on Figure 1) seen in 941 Earth days between image T2 and S1. Lee front advance and bedrock exposure on the stoss side can be observed (white arrows). (GIF 1384 kb)

Supplementary Movie 1

This movie shows the T1 image wrapped on the topography extracted from S1 and S2. Note the vertical exaggeration. (MPG 5152 kb)

Supplementary Movie 2

This movie shows the shaded bedrock-only topography. The bedrock was interpolated beneath the dunes following the method described in SOM Methods: Dune height extraction. (MP4 29559 kb)

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