desert pavement

Several theories have been proposed for the formation of desert pavements.McFadden, L.D., Wells, S.G. and Jercinovich, M.J. 1987. "Influences of aeolian and pedogenic processes on the origin and evolution of desert pavements", Geology 15(6):504-508. A common theory suggests that they form through the gradual removal of sand, dust and other fine-grained material by the wind and intermittent rain, leaving the larger fragments behind. The larger fragments are shaken into place through the forces of rain, running water, wind, gravity, creep, thermal expansion and contraction, wetting and drying, frost heaving, animal traffic, and the Earth's constant microseismic vibrations. The removal of small particles by wind does not continue indefinitely, because once the pavement forms, it acts as a barrier to resist further erosion. The small particles collect underneath the pavement surface, forming a vesicular A soil horizon (designated "Av").

A second theory supposes that desert pavements form from the shrink/swell properties of the clay underneath the pavement; when precipitation is absorbed by clay it causes it to expand, and when it dries it cracks along planes of weakness. Over time, this geomorphic action transports small pebbles to the surface, where they stay through lack of precipitation that would otherwise destroy the pavement by transport of the clasts or excessive vegetative growth.

A newer theory suggests that desert pavements form through depositions of windblown dust atop preexisting rocks. The dust then settles beneath the rocks, forming a layer of soil, while the rocks at the top crack and begin to merge into desert pavement. In 1995, researchers conducted a study in the Mojave Desert using helium-3 dating where they determined the rocks to be of older age than the soil beneath, leading to the conclusion of "stone pavements [being] born at the surface."{{cite journal |author1=Wells S.G. |author2=McFadden L.D. |author3=Poths J. |author4=Olinger C.T. |year=1995 |title=Cosmogenic ³He surface-exposure dating of stone pavements: Implications for landscape evolution in deserts |url=https://faculty.unlv.edu/buckb/Dust%20posters/Wells%20et%20al%201995.pdf |url-status=dead |journal=Geology |volume=23 |issue=7 |pages=613–616 |bibcode=1995Geo....23..613W |doi=10.1130/0091-7613(1995)023<0613:CHSEDO>2.3.CO;2 |archive-url=https://web.archive.org/web/20161006014103/https://faculty.unlv.edu/buckb/Dust%20posters/Wells%20et%20al%201995.pdf |archive-date=2016-10-06 |access-date=2016-02-23}}File:Desert pavement evolution.png

Desert pavement surfaces are often coated with desert varnish, a dark brown, sometimes shiny coating that contains clay minerals. In the US a famous example can be found on Newspaper Rock in southeastern Utah. Desert varnish is a thin coating (patina) of clays, iron, and manganese on the surface of sun-baked boulders. Micro-organisms may also play a role in their formation. Desert varnish is also prevalent in the Mojave desert and Great Basin geomorphic province.Dorn, R. I. and T. M. Oberlander, 1981, "Microbial Origin of Desert Varnish," Science 213:1245-1247

File:Adrar-Reg (1).JPG in Mauritania]]

Stony deserts may be known by different names according to the region. Examples include:

Gibbers: Covering extensive areas in Australia such as parts of the Tirari-Sturt stony desert ecoregion are desert pavements called Gibber Plains after the pebbles or gibbers.East, J.J. 1889. "On the geological structures and physical features of Central Australia", Transactions and Proceedings and Report of the Royal Society of South Australia 12:31-53. Gibber is also used to describe ecological communities, such as Gibber Chenopod Shrublands or Gibber Transition Shrublands.

In North Africa, a vast stony desert plain is known as reg. This is in contrast with erg, which refers to a sandy desert area.Jean Dresch et al., Géographie des régions arides, Presses universitaires de France, Paris, 1982. {{ISBN|2-13-037457-3}}

{{div col}}

• {{annotated link|Aeolian processes}}
• {{annotated link|Desert varnish}}
• {{annotated link|Eduction (geology)}}, a mechanism of surface rock formation
• {{annotated link|Erg (landform)|Erg}}
• {{annotated link|Hamada}}
• {{annotated link|Saltation (geology)}}
• {{annotated link|Ventifact}}

{{div col end}}

{{reflist}}

• Al-Qudah, K.A. 2003. The influence of long-term landscape stability on flood hydrology and geomorphic evolution of valley floor in the northeastern Badin of Jordan. Doctoral thesis, University of Nevada, Reno.
• Anderson, K.C. 1999. Processes of vesicular horizon development and desert pavement formation on basalt flows of the Cima Volcanic Field and alluvial fans of the Avawatz Mountains Piedmont, Mojave Desert, California. Doctoral thesis, University of California, Riverside.
• Goudie, A.S. 2008. The history and nature of wind erosion in deserts. Annual Review of Earth and Planetary Sciences 36:97-119.
• Grotzinger, et al. 2007. Understanding Earth, fifth edition. Freeman and Company. 458–460.
• Haff, P.K. and Werner, B.T. 1996. Dynamical processes on desert pavements and the healing of surficial disturbance. Quaternary Research 45(1):38-46.
• Meadows, D.G., Young, M.H. and McDonald, E.V. 2006. Estimating the fine soil fraction of desert pavements using ground penetrating radar. Vadose Zone Journal 5(2):720-730.
• Qu Jianjun, Huang Ning, Dong Guangrong and Zhang Weimin. 2001. The role and significance of the Gobi desert pavement in controlling sand movement on the cliff top near the Dunhuang Magao Grottoes. Journal of Arid Environments 48(3):357-371.
• Rieman, H.M. 1979. Deflation armor (desert pavement). The Lapidary Journal 33(7):1648-1650.
• Williams, S.H. and Zimbelman, J.R. 1994. Desert pavement evolution: An example of the role of sheetflood. The Journal of Geology 102(2):243-248.

{{Commons category}}

• [https://web.archive.org/web/20030509022609/http://www.tec.army.mil/research/products/desert_guide/lsmsheet/lspave.htm Desert Processes Working Group]

Category:Aeolian landforms

Category:Deserts

Category:Sediments

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