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  Earth Science News
The flowing shapes of the Little Egypt sand dunes in Utah's Escalante Canyon region from when strong, dry winds blow sand. In a desert, there is very little vegetation, because rain is so rare.
CreditJerry Sintz, Bureau of Land Management
Guide to Reading

Water is such an important factor in Earth’s surface processes that the last three chapters have focused on it. The author considered fresh surface water in Chapter 14, ocean water in Chapter 15, and groundwater in Chapter 16. The chapter after this will again deal with water, but in its frozen form, glaciers. Is there no end to water? In this chapter you find it, for the subject is deserts. However, in a sense water is still an issue, for the defining characteristic of all deserts is the lack of water.
The chapter begins by dispelling the popular notion that all deserts are hot and sandy places. It lists and describes the five classes of deserts and points out that their only common factor is their aridity (dryness). The five classes are

    • subtropical: in the hot dry latitudes between 20 and 30°, both north and south
    • rain shadow: on the landward side of coastal mountain ranges
    • coastal: along coasts bordering cold ocean currents
    • continental interior: deep within continents, far from major water sources
    • polar: in the cold dry polar regions, both north and south

Do note the geographic locations given to illustrate the desert types because obviously their geographic locations explain why the regions are deserts and matching desert locations with desert types are frequently asked test questions.

The chapter continues with a discussion of how weathering and erosion processes are modified by desert conditions. Chemical weathering is made minimal and slow, but it does happen and it creates caliche-rich soils and some special desert features like desert varnish. Rainfall is minimal, so streams are intermittent (or ephemeral). Dry water channels and basins (washes, arroyos, wadis, and playas) are common. When water is present, it does a vigorous job of eroding the land and is a more important agent of erosion than the wind is. Flash floods are not rare. They scour the land, produce dramatic steep-sided channels, and polish the canyon walls with their sand-laden waters. Wind, like water, is a fluid and, like water, can carry its load of sediment suspended or as surface load, which it may bounce along the ground in the process of saltation. Wind isn’t as powerful as water and can’t move grains larger than coarse sand. Therefore it creates lag deposits and desert pavement. Wind may abrade rock surfaces to produce smooth faces (facets) on pebble-sized particles called ventifacts or may carve mushroom-shaped columns (yardangs) by the differential erosion of rock strata. Wind erosion can lower the land surface over large areas, a process called deflation, and can produce special circular depressed areas known as blowouts.

Material removed by erosion must be deposited somewhere, so logically deposition in desert environments is the next chapter topic. Deposits may be of varying sizes and may have been transported by a variety of agents. Large angular rocks tumble downhill due to gravity and pile up in talus aprons. Dust-sized particles lifted and then dropped by wind are called loess deposits. Desert streams drop materials when their gradients lessen and produce triangular-shaped structures called alluvial fans. Overlapping alluvial fans may extend for miles along mountain fronts as elongated structures called bajadas. Streams carry various salts into desert lake basins (playas) where they are left as thick salt deposits when the water evaporates. Occasionally these interior basins (lakes with channel inlets but no channel outlets) are very large, like the Great Salt Lake of Utah and the Dead Sea along the Israel-Jordan border.

Desert landscapes are varied, and of course there is special vocabulary to describe all of them. “Hamada,” “reg,” and “erg” are terms used to designate very different aspects of the Sahara Desert region. Rocky desert areas change over time as scarp retreat forms pediments, mesas, buttes, chimneys, hoodoos, cuestas, dip slopes, inselbergs, and bornhardts. Depending on the amount of sand present and the constancy and velocity of the wind, sandy deserts are filled with different-shaped sand dunes. You read about barchan, star-shaped, transverse, parabolic, and longitudinal (seif) dunes, as well as the anatomy of an individual dune (windward slope, lee slope, slip face, angle of repose, and ripples).

Modern scientific thought tends to emphasize the interrelationships between the sciences. Therefore, while this is a geology text and naturally concentrates on inorganic aspects of Earth study, it does point out interactions between the obvious realm of geology, the lithosphere (rocky Earth), and Earth’s other spheres, the atmosphere, the hydrosphere (Chapters 14, 15, and 16), and the biosphere (interwoven through many of the chapters). The last part of this chapter concentrates on the biosphere. It discusses human interactions with desert environments on the Great Plains of North America and in the Sahel region of Africa. The process discussed is desertification, in which semi-arid regions are changed into true deserts, partially due to natural causes, partially due to human activities. It is a somber reminder that geologic happenings influence human society, human society influences geologic happenings, and these interactions may be harmful to some fragile Earth environments and life-forms.

Key Terms
alluvial fan insolation
bajada interior basin lakes
barchan dunes intermittent (or ephemeral) streams
bed load lag deposit
blowout leach
bornhardts loess
buttes longitudinal dunes (or seif dunes)
caliche mesas
chimneys parabolic dunes
continental-interior deserts pediment
convergence zone petroglyphs
Coriolis effect playa
cuestas polar cells
deflation prevailing winds
desert rain shadow deserts
desert pavement reg
desert varnish saltation
desertification scarp retreat
dip slope slip face
divergence zone star-shaped dunes
dust storm suspended load
erg talus apron
Ferrel cells transverse dunes
Hadley cells ventifacts (faceted rocks)
hamada wadis
hoodoos wind abrasion
inselberg yardangs