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Desert
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Sand dunes in the Rub' al Khali ("Empty quarter") of Arabia

A desert is a landscape where little precipitation occurs and, consequently, living conditions create unique biomes and ecosystems. The lack of vegetation exposes the unprotected surface of the ground to denudation. About one-third of the land surface of the Earth is arid or semi-arid. This includes much of the polar regions, where little precipitation occurs, and which are sometimes called polar deserts or "cold deserts". Deserts can be classified by the amount of precipitation that falls, by the temperature that prevails, by the causes of desertification or by their geographical location.[1]

Deserts are formed by weathering processes as large variations in temperature between day and night strain the rocks, which consequently break in pieces. Although rain seldom occurs in deserts, there are occasional downpours that can result in flash floods. Rain falling on hot rocks can cause them to shatter, and the resulting fragments and rubble strewn over the desert floor are further eroded by the wind. This picks up particles of sand and dust, which can remain airborne for extended periods – sometimes causing the formation of sand storms or dust storms. Wind-blown sand grains striking any solid object in their path can abrade the surface. Rocks are smoothed down, and the wind sorts sand into uniform deposits. The grains end up as level sheets of sand or are piled high in billowing dunes. Other deserts are flat, stony plains where all the fine material has been blown away and the surface consists of a mosaic of smooth stones, often forming desert pavements, and little further erosion occurs. Other desert features include rock outcrops, exposed bedrock and clays once deposited by flowing water. Temporary lakes may form and salt pans may be left when waters evaporate. There may be underground water sources in the form of springs and seepages from aquifers. Where these are found, oases can occur.

Plants and animals living in the desert need special adaptations to survive in the harsh environment. Plants tend to be tough and wiry with small or no leaves, water-resistant cuticles, and often spines to deter herbivory. Some annual plants germinate, bloom, and die within a few weeks after rainfall, while other long-lived plants survive for years and have deep root systems that are able to tap underground moisture. Animals need to keep cool and find enough food and water to survive. Many are nocturnal and stay in the shade or underground during the day's heat. They tend to be efficient at conserving water, extracting most of their needs from their food and concentrating their urine. Some animals remain in a state of dormancy for long periods, ready to become active again during the rare rainfall. They then reproduce rapidly while conditions are favorable before returning to dormancy.

People have struggled to live in deserts and the surrounding semi-arid lands for millennia. Nomads have moved their flocks and herds to wherever grazing is available, and oases have provided opportunities for a more settled way of life. The cultivation of semi-arid regions encourages erosion of soil and is one of the causes of increased desertification. Desert farming is possible with the aid of irrigation, and the Imperial Valley in California provides an example of how previously barren land can be made productive by the import of water from an outside source. Many trade routes have been forged across deserts, especially across the Sahara, and traditionally were used by caravans of camels carrying salt, gold, ivory and other goods. Large numbers of slaves were also taken northwards across the Sahara. Some mineral extraction also takes place in deserts, and the uninterrupted sunlight gives potential for capturing large quantities of solar energy.

Etymology

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English desert and its Romance cognates (including Italian and Portuguese deserto, French désert and Spanish desierto) all come from the ecclesiastical Latin dēsertum (originally "an abandoned place"), a participle of dēserere, "to abandon".[2] The correlation between aridity and sparse population is complex and dynamic, varying by culture, era, and technologies; thus the use of the word desert can cause confusion. In English before the 20th century, desert was often used in the sense of "unpopulated area", without specific reference to aridity;[2] but today the word is most often used in its climate-science sense (an area of low precipitation).[3] Phrases such as "desert island"[4] and "Great American Desert", or Shakespeare's "deserts of Bohemia" (The Winter's Tale) in previous centuries did not necessarily imply sand or aridity; their focus was the sparse population.[5]

Major deserts

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global map of deserts
The world's largest non-polar deserts

Deserts occupy about one third of Earth's land surface.[6] Bottomlands may be salt-covered flats. Eolian processes are major factors in shaping desert landscapes. Polar deserts (also seen as "cold deserts") have similar features, except the main form of precipitation is snow rather than rain. Antarctica is the world's largest cold desert (composed of about 98% thick continental ice sheet and 2% barren rock). Some of the barren rock is to be found in the so-called Dry Valleys of Antarctica that almost never get snow, which can have ice-encrusted saline lakes that suggest evaporation far greater than the rare snowfall due to the strong katabatic winds that even evaporate ice.

The ten largest deserts[7]
Rank Desert Area (km2) Area (sqmi)
1 Antarctic Desert (Antarctica) 14,200,000 5,482,651
2 Arctic Desert (Arctic) 13,900,000 5,366,820
3 Sahara Desert (Africa) 9,200,000 3,552,140
4 Great Australian (Australia) 2,700,000 1,042,476
5 Arabian Desert (Middle East) 2,330,000 899,618
6 Gobi Desert (Asia) 1,295,000 500,002
7 Kalahari Desert (Africa) 900,000 347,492
8 Patagonian Desert (South America) 673,000 259,847
9 Syrian Desert (Middle East) 500,000 193,051
10 Great Basin Desert (North America) 490,000 190,000

Deserts, both hot and cold, play a part in moderating Earth's temperature, because they reflect more of the incoming light and their albedo is higher than that of forests or the sea.[8]

Defining characteristics

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A desert is a region of land that is very dry because it receives low amounts of precipitation (usually in the form of rain, but it may be snow, mist or fog), often has little coverage by plants, and in which streams dry up unless they are supplied by water from outside the area.[9] Deserts generally receive less than 250 mm (10 in) of precipitation each year.[9] The potential evapotranspiration may be large but (in the absence of available water) the actual evapotranspiration may be close to zero.[10] Semi-deserts are regions which receive between 250 and 500 mm (10 and 20 in) and when clad in grass, these are known as steppes.[11][6] Most deserts on Earth such as the Sahara Desert, Grand Australian Desert and the Great Basin Desert, occur in low altitudes.[12]

Water

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Atacama Desert in foreground with Andes mountains in distance
Atacama, the world's driest non-polar desert, part of the Arid Diagonal of South America

One of the driest places on Earth is the Atacama Desert.[13][14][15][16][17] It is virtually devoid of life because it is blocked from receiving precipitation by the Andes mountains to the east and the Chilean Coast Range to the west. The cold Humboldt Current and the anticyclone of the Pacific are essential to keep the dry climate of the Atacama. The average precipitation in the Chilean region of Antofagasta is just 1 mm (0.039 in) per year. Some weather stations in the Atacama have never received rain. Evidence suggests that the Atacama may not have had any significant rainfall from 1570 to 1971. It is so arid that mountains that reach as high as 6,885 m (22,589 ft) are completely free of glaciers and, in the southern part from 25°S to 27°S, may have been glacier-free throughout the Quaternary, though permafrost extends down to an altitude of 4,400 m (14,400 ft) and is continuous above 5,600 m (18,400 ft).[18][19] Nevertheless, there is some plant life in the Atacama, in the form of specialist plants that obtain moisture from dew and the fogs that blow in from the Pacific.[13]

muddy stream in Gobi Desert with grass in foreground and desert in background
Flash flood in the Gobi

When rain falls in deserts, as it occasionally does, it is often with great violence. The desert surface is evidence of this with dry stream channels known as arroyos or wadis meandering across its surface. These can experience flash floods, becoming raging torrents with surprising rapidity after a storm that may be many kilometers away. Most deserts are in basins with no drainage to the sea but some are crossed by exotic rivers sourced in mountain ranges or other high rainfall areas beyond their borders. The River Nile, the Colorado River and the Yellow River do this, losing much of their water through evaporation as they pass through the desert and raising groundwater levels nearby. There may also be underground sources of water in deserts in the form of springs, aquifers, underground rivers or lakes. Where these lie close to the surface, wells can be dug and oases may form where plant and animal life can flourish.[20] The Nubian Sandstone Aquifer System under the Sahara Desert is the largest known accumulation of fossil water. The Great Man-Made River is a scheme launched by Libya's Muammar Gaddafi to tap this aquifer and supply water to coastal cities.[21] Kharga Oasis in Egypt is 150 km (93 mi) long and is the largest oasis in the Libyan Desert. A lake occupied this depression in ancient times and thick deposits of sandy-clay resulted. Wells are dug to extract water from the porous sandstone that lies underneath.[citation needed] Seepages may occur in the walls of canyons and pools may survive in deep shade near the dried up watercourse below.[22]

Desert Lake, near Ragtown, Nevada

Lakes may form in basins where there is sufficient precipitation or meltwater from glaciers above. They are usually shallow and saline, and wind blowing over their surface can cause stress, moving the water over nearby low-lying areas. When the lakes dry up, they leave a crust or hardpan behind. This area of deposited clay, silt or sand is known as a playa. The deserts of North America have more than one hundred playas, many of them relics of Lake Bonneville which covered parts of Utah, Nevada and Idaho during the last ice age when the climate was colder and wetter.[23] These include the Great Salt Lake, Utah Lake, Sevier Lake and many dry lake beds. The smooth flat surfaces of playas have been used for attempted vehicle speed records at Black Rock Desert and Bonneville Speedway and the United States Air Force uses Rogers Dry Lake in the Mojave Desert as runways for aircraft and the Space Shuttle.[20]

Classification

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The Sahara is the largest hot desert in the world

Deserts have been defined and classified in a number of ways, generally combining total precipitation, number of days on which this falls, temperature, and humidity, and sometimes additional factors.[6] For example, Phoenix, Arizona, receives less than 250 mm (9.8 in) of precipitation per year, and is immediately recognized as being located in a desert because of its aridity-adapted plants. The North Slope of Alaska's Brooks Range also receives less than 250 mm (9.8 in) of precipitation per year and is often classified as a cold desert.[24] Other regions of the world have cold deserts, including areas of the Himalayas[25] and other high-altitude areas in other parts of the world.[26] Polar deserts cover much of the ice-free areas of the Arctic and Antarctic.[27][28] A non-technical definition is that deserts are those parts of Earth's surface that have insufficient vegetation cover to support a human population.[29]

Potential evapotranspiration supplements the measurement of precipitation in providing a scientific measurement-based definition of a desert. The water budget of an area can be calculated using the formula PPE ± S, wherein P is precipitation, PE is potential evapotranspiration rates and S is the amount of surface storage of water. Evapotranspiration is the combination of water loss through atmospheric evaporation and through the life processes of plants. Potential evapotranspiration, then, is the amount of water that could evaporate in any given region. As an example, Tucson, Arizona receives about 300 mm (12 in) of rain per year, however about 2,500 mm (98 in) of water could evaporate over the course of a year.[30] In other words, about eight times more water could evaporate from the region than actually falls as rain. Rates of evapotranspiration in cold regions such as Alaska are much lower because of the lack of heat to aid in the evaporation process.[31]

Deserts are sometimes classified as "hot" or "cold", "semiarid" or "coastal".[29] The characteristics of hot deserts include high temperatures in summer; greater evaporation than precipitation, usually exacerbated by high temperatures, strong winds and lack of cloud cover; considerable variation in the occurrence of precipitation, its intensity and distribution; and low humidity. Winter temperatures vary considerably between different deserts and are often related to the location of the desert on the continental landmass and the latitude. Daily variations in temperature can be as great as 22 °C (40 °F) or more, with heat loss by radiation at night being increased by the clear skies.[32]

aerial view of ice sheet covered in snow Antarctica
Cold desert: snow surface at Dome C Station, Antarctica

Cold deserts, sometimes known as temperate deserts, occur at higher latitudes than hot deserts, and the aridity is caused by the dryness of the air. Some cold deserts are far from the ocean and others are separated by mountain ranges from the sea, and in both cases, there is insufficient moisture in the air to cause much precipitation. The largest of these deserts are found in Central Asia. Others occur on the eastern side of the Rocky Mountains, the eastern side of the southern Andes and in southern Australia.[11] Polar deserts are a particular class of cold desert. The air is very cold and carries little moisture so little precipitation occurs and what does fall, usually snow, is carried along in the often strong wind and may form blizzards, drifts and dunes similar to those caused by dust and sand in other desert regions. In Antarctica, for example, the annual precipitation is about 50 mm (2 in) on the central plateau and some ten times that amount on some major peninsulas.[32]

Based on precipitation alone, hyperarid deserts receive less than 25 mm (1 in) of rainfall a year; they have no annual seasonal cycle of precipitation and experience twelve-month periods with no rainfall at all.[32][33] Arid deserts receive between 25 and 200 mm (1 and 8 in) in a year and semiarid deserts between 200 and 500 mm (8 and 20 in). However, such factors as the temperature, humidity, rate of evaporation and evapotranspiration, and the moisture storage capacity of the ground have a marked effect on the degree of aridity and the plant and animal life that can be sustained. Rain falling in the cold season may be more effective at promoting plant growth, and defining the boundaries of deserts and the semiarid regions that surround them on the grounds of precipitation alone is problematic.[32]

Semi-arid Niger

A semi-arid desert or a steppe is a version of the arid desert with much more rainfall, vegetation and higher humidity. These regions feature a semi-arid climate and are less extreme than regular deserts.[34] Like arid deserts, temperatures can vary greatly in semi deserts. They share some characteristics of a true desert and are usually located at the edge of deserts and continental dry areas. They usually receive precipitation from 250 to 500 mm (9.8 to 19.7 in) but this can vary due to evapotranspiration and soil nutrition. Semi-deserts can be found in the high elevations of the Tabernas Desert (and some parts of the Spanish Plateau), The Sahel, The Eurasian Steppe, most of Central Asia, the Western US, most of Northern Mexico, portions of South America (especially in Argentina) and the Australian Outback.[35] They usually feature BSh (hot steppe) or BSk (temperate steppe) in the Köppen climate classification.

Coastal deserts are mostly found on the western edges of continental land masses in regions where cold currents approach the land or cold water upwellings rise from the ocean depths. The cool winds crossing this water pick up little moisture and the coastal regions have low temperatures and very low rainfall, the main precipitation being in the form of fog and dew. The range of temperatures on a daily and annual scale is relatively low, being 11 °C (20 °F) and 5 °C (9 °F) respectively in the Atacama Desert. Deserts of this type are often long and narrow and bounded to the east by mountain ranges. They occur in Namibia, Chile, southern California and Baja California. Other coastal deserts influenced by cold currents are found in Western Australia, the Arabian Peninsula and Horn of Africa, and the western fringes of the Sahara.[32]

In 1961, Peveril Meigs divided desert regions on Earth into three categories according to the amount of precipitation they received. In this now widely accepted system, extremely arid lands have at least twelve consecutive months without precipitation, arid lands have less than 250 mm (9.8 in) of annual precipitation, and semiarid lands have a mean annual precipitation of between 250 and 500 mm (9.8 and 19.7 in). Both extremely arid and arid lands are considered to be deserts while semiarid lands are generally referred to as steppes when they are grasslands.[6]

desert behind mountains because of the rain shadow effect
The Agasthiyamalai hills cut off Tirunelveli in India from the monsoons, creating a rainshadow region.

Deserts are also classified, according to their geographical location and dominant weather pattern, as trade wind, mid-latitude, rain shadow, coastal, monsoon, or polar deserts.[36] Trade wind deserts occur either side of the horse latitudes at 30° to 35° North and South. These belts are associated with the subtropical anticyclone and the large-scale descent of dry air. The Sahara Desert is of this type. Mid-latitude deserts occur between 30° and 50° North and South. They are mostly in areas remote from the sea where most of the moisture has already precipitated from the prevailing winds. They include the Tengger and Sonoran Deserts.[36] Monsoon deserts are similar. They occur in regions where large temperature differences occur between sea and land. Moist warm air rises over the land, deposits its water content and circulates back to sea. Further inland, areas receive very little precipitation. The Thar Desert near the India/Pakistan border is of this type.[36]

In some parts of the world, deserts are created by a rain shadow effect. Orographic lift occurs as air masses rise to pass over high ground. In the process they cool and lose much of their moisture by precipitation on the windward slope of the mountain range. When they descend on the leeward side, they warm and their capacity to hold moisture increases so an area with relatively little precipitation occurs.[37] The Taklamakan Desert is an example, lying in the rain shadow of the Himalayas and receiving less than 38 mm (1.5 in) precipitation annually.[38] Other areas are arid by virtue of being a very long way from the nearest available sources of moisture.[39]

A montane desert

Montane deserts are arid places with a very high altitude; the most prominent example is found north of the Himalayas, in the Kunlun Mountains and the Tibetan Plateau. Many locations within this category have elevations exceeding 3,000 m (9,800 ft) and the thermal regime can be hemiboreal. These places owe their profound aridity (the average annual precipitation is often less than 40 mm or 1.5 in) to being very far from the nearest available sources of moisture and are often in the lee of mountain ranges. Montane deserts are normally cold, or may be scorchingly hot by day and very cold by night as is true of the northeastern slopes of Mount Kilimanjaro.[40]

Polar deserts such as McMurdo Dry Valleys remain ice-free because of the dry katabatic winds that flow downhill from the surrounding mountains.[41] Former desert areas presently in non-arid environments, such as the Sandhills in Nebraska, are known as paleodeserts.[36] In the Köppen climate classification system, deserts are classed as BWh (hot desert) or BWk (temperate desert). In the Thornthwaite climate classification system, deserts would be classified as arid megathermal climates.[42][43]

Polar desert

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Polar deserts are a type of cold desert. While they do not lack water, having a persistent cover of snow and ice, this is merely due to marginal evaporation rates and low precipitation.

The McMurdo dry valleys of Antarctica, which lack water (whether rain, ice, or snow) much like a non-polar desert and even have such desert features as hypersaline lakes and intermittent streams that resemble (except for being frozen at their surfaces) hot or cold deserts for extreme aridity and lack of precipitation of any kind. Extreme winds and not seasonal heat desiccate these nearly-lifeless terrains.

Biological desert

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An animation of a year in organism density on Earth. The South Pacific Gyre is an example of a so-called "oceanic desert", visibly low (purple) in organism density. Polar deserts are visible in consistent white and arid deserts in consistent brown, with tundras oscillating between white and brown.

The concept of "biological desert" redefines the concept of desert, without the characteristic of aridity, not lacking water, but instead lacking life. Such places can be so-called "ocean deserts", which are mostly at the centers of gyres, but also hypoxic or anoxic waters such as dead zones.[44][45][46]

Morphology

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Weathering processes

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granite rock with weathered exfoliation Enchanted Rock State Natural Area, Texas
Exfoliation of weathering rocks in Texas, US

Deserts usually have a large diurnal and seasonal temperature range, with high daytime temperatures falling sharply at night. The diurnal range may be as much as 20 to 30 °C (36 to 54 °F) and the rock surface experiences even greater temperature differentials.[47] During the day the sky is usually clear and most of the sun's radiation reaches the ground, but as soon as the sun sets, the desert cools quickly by radiating heat into space. In hot deserts, the temperature during daytime can exceed 45 °C (113 °F) in summer and plunge below freezing point at night during winter.[48]

multicolor grains of sand in a centimeter sample
One square centimeter
(0.16 sq in) of windblown sand from the Gobi Desert

Such large temperature variations have a destructive effect on the exposed rocky surfaces. The repeated fluctuations put a strain on exposed rock and the flanks of mountains crack and shatter. Fragmented strata slide down into the valleys where they continue to break into pieces due to the relentless sun by day and chill by night. Successive strata are exposed to further weathering. The relief of the internal pressure that has built up in rocks that have been underground for aeons can cause them to shatter.[49] Exfoliation also occurs when the outer surfaces of rocks split off in flat flakes. This is believed to be caused by the stresses put on the rock by repeated thermal expansions and contractions which induces fracturing parallel to the original surface.[47] Chemical weathering processes probably play a more important role in deserts than was previously thought. The necessary moisture may be present in the form of dew or mist. Ground water may be drawn to the surface by evaporation and the formation of salt crystals may dislodge rock particles as sand or disintegrate rocks by exfoliation. Shallow caves are sometimes formed at the base of cliffs by this means.[47]

As the desert mountains decay, large areas of shattered rock and rubble occur. The process continues and the end products are either dust or sand. Dust is formed from solidified clay or volcanic deposits whereas sand results from the fragmentation of harder granites, limestone and sandstone.[50] There is a certain critical size (about 0.5 mm) below which further temperature-induced weathering of rocks does not occur and this provides a minimum size for sand grains.[51]

As the mountains are eroded, more and more sand is created. At high wind speeds, sand grains are picked up off the surface and blown along, a process known as saltation. The whirling airborne grains act as a sand blasting mechanism which grinds away solid objects in its path as the kinetic energy of the wind is transferred to the ground.[52] The sand eventually ends up deposited in level areas known as sand-fields or sand-seas, or piled up in dunes.[53]

Features

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see caption
Aerial view of Makhtesh Ramon, an erosion cirque of a type unique to the Negev

Many people think of deserts as consisting of extensive areas of billowing sand dunes because that is the way they are often depicted on TV and in films,[54] but deserts do not always look like this.[55] Across the world, around 20% of desert is sand, varying from only 2% in North America to 30% in Australia and over 45% in Central Asia.[20] Where sand does occur, it is usually in large quantities in the form of sand sheets or extensive areas of dunes.[20]

A sand sheet is a near-level, firm expanse of partially consolidated particles in a layer that varies from a few centimeters to a few meters thick. The structure of the sheet consists of thin horizontal layers of coarse silt and very fine to medium grain sand, separated by layers of coarse sand and pea-gravel which are a single grain thick. These larger particles anchor the other particles in place and may also be packed together on the surface so as to form a miniature desert pavement.[56] Small ripples form on the sand sheet when the wind exceeds 24 km/h (15 mph). They form perpendicular to the wind direction and gradually move across the surface as the wind continues to blow. The distance between their crests corresponds to the average length of jumps made by particles during saltation. The ripples are ephemeral and a change in wind direction causes them to reorganise.[57]

diagram showing movement of sand dune in relation to wind direction
Diagram showing barchan dune formation, with the wind blowing from the left

Sand dunes are accumulations of windblown sand piled up in mounds or ridges. They form downwind of copious sources of dry, loose sand and occur when topographic and climatic conditions cause airborne particles to settle. As the wind blows, saltation and creep take place on the windward side of the dune and individual grains of sand move uphill. When they reach the crest, they cascade down the far side. The upwind slope typically has a gradient of 10° to 20° while the lee slope is around 32°, the angle at which loose dry sand will slip. As this wind-induced movement of sand grains takes place, the dune moves slowly across the surface of the ground.[58] Dunes are sometimes solitary, but they are more often grouped together in dune fields. When these are extensive, they are known as sand seas or ergs.[59]

The shape of the dune depends on the characteristics of the prevailing wind. Barchan dunes are produced by strong winds blowing across a level surface and are crescent-shaped with the concave side away from the wind. When there are two directions from which winds regularly blow, a series of long, linear dunes known as seif dunes may form. These also occur parallel to a strong wind that blows in one general direction. Transverse dunes run at a right angle to the prevailing wind direction. Star dunes are formed by variable winds, and have several ridges and slip faces radiating from a central point. They tend to grow vertically; they can reach a height of 500 m (1,600 ft), making them the tallest type of dune. Rounded mounds of sand without a slip face are the rare dome dunes, found on the upwind edges of sand seas.[59]

Gypsum dune fields, White Sands National Park, New Mexico, United States

In deserts where large amounts of limestone mountains surround a closed basin, such as at White Sands National Park in south-central New Mexico, occasional storm runoff transports dissolved limestone and gypsum into a low-lying pan within the basin where the water evaporates, depositing the gypsum and forming crystals known as selenite. The crystals left behind by this process are eroded by the wind and deposited as vast white dune fields that resemble snow-covered landscapes. These types of dune are rare, and only form in closed arid basins that retain the highly soluble gypsum that would otherwise be washed into the sea.[60]

photograph of desert pavement, small stones left behind by wind
Windswept desert pavement of small, smooth, closely packed stones in the Mojave Desert

A large part of the surface area of the world's deserts consists of flat, stone-covered plains dominated by wind erosion. In "eolian deflation", the wind continually removes fine-grained material, which becomes wind-blown sand. This exposes coarser-grained material, mainly pebbles with some larger stones or cobbles,[53][20] leaving a desert pavement, an area of land overlaid by closely packed smooth stones forming a tessellated mosaic. Different theories exist as to how exactly the pavement is formed. It may be that after the sand and dust is blown away by the wind the stones jiggle themselves into place; alternatively, stones previously below ground may in some way work themselves to the surface. Very little further erosion takes place after the formation of a pavement, and the ground becomes stable. Evaporation brings moisture to the surface by capillary action and calcium salts may be precipitated, binding particles together to form a desert conglomerate.[61] In time, bacteria that live on the surface of the stones accumulate a film of minerals and clay particles, forming a shiny brown coating known as desert varnish.[62]

Other non-sandy deserts consist of exposed outcrops of bedrock, dry soils or aridisols, and a variety of landforms affected by flowing water, such as alluvial fans, sinks or playas, temporary or permanent lakes, and oases.[20] A hamada is a type of desert landscape consisting of a high rocky plateau where the sand has been removed by aeolian processes. Other landforms include plains largely covered by gravels and angular boulders, from which the finer particles have been stripped by the wind. These are called "reg" in the western Sahara, "serir" in the eastern Sahara, "gibber plains" in Australia and "saï" in central Asia.[63] The Tassili Plateau in Algeria is a jumble of eroded sandstone outcrops, canyons, blocks, pinnacles, fissures, slabs and ravines. In some places the wind has carved holes or arches, and in others, it has created mushroom-like pillars narrower at the base than the top.[64] On the Colorado Plateau, it is water that has been the prevailing eroding force. Here, rivers, such as the Colorado, have cut their way over the millennia through the high desert floor, creating canyons that are over a mile (6,000 feet or 1,800 meters) deep in places, exposing strata that are over two billion years old.[65]

Dust storms and sandstorms

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dark brown sand storm about to engulf a motor pool
Dust storm about to engulf a military camp in Iraq, 2005

Sand and dust storms are natural events that occur in arid regions where the land is not protected by a covering of vegetation. Dust storms usually start in desert margins rather than the deserts themselves where the finer materials have already been blown away. As a steady wind begins to blow, fine particles lying on the exposed ground begin to vibrate. At greater wind speeds, some particles are lifted into the air stream. When they land, they strike other particles which may be jerked into the air in their turn, starting a chain reaction. Once ejected, these particles move in one of three possible ways, depending on their size, shape and density; suspension, saltation or creep. Suspension is only possible for particles less than 0.1 mm (0.0039 in) in diameter. In a dust storm, these fine particles are lifted up and wafted aloft to heights of up to 6 km (3.7 mi). They reduce visibility and can remain in the atmosphere for days on end, conveyed by the trade winds for distances of up to 6,000 km (3,700 mi).[66] Denser clouds of dust can be formed in stronger winds, moving across the land with a billowing leading edge. The sunlight can be obliterated and it may become as dark as night at ground level.[67] In a study of a dust storm in China in 2001, it was estimated that 6.5 million tons of dust were involved, covering an area of 134,000,000 km2 (52,000,000 sq mi). The mean particle size was 1.44 μm.[68] A much smaller scale, short-lived phenomenon can occur in calm conditions when hot air near the ground rises quickly through a small pocket of cooler, low-pressure air above forming a whirling column of particles, a dust devil.[69]

diagram of sand particles showing wind entrainment
Wind-blown particles: 1. creep 2. saltation 3. suspension 4. wind current

Sandstorms occur with much less frequency than dust storms. They are often preceded by severe dust storms and occur when the wind velocity increases to a point where it can lift heavier particles. These grains of sand, up to about 0.5 mm (0.020 in) in diameter are jerked into the air but soon fall back to earth, ejecting other particles in the process. Their weight prevents them from being airborne for long and most only travel a distance of a few meters (yards). The sand streams along above the surface of the ground like a fluid, often rising to heights of about 30 cm (12 in).[66] In a really severe steady blow, 2 m (6 ft 7 in) is about as high as the sand stream can rise as the largest sand grains do not become airborne at all. They are transported by creep, being rolled along the desert floor or performing short jumps.[67]

During a sandstorm, the wind-blown sand particles become electrically charged. Such electric fields, which range in size up to 80 kV/m, can produce sparks and cause interference with telecommunications equipment. They are also unpleasant for humans and can cause headaches and nausea.[67] The electric fields are caused by the collision between airborne particles and by the impacts of saltating sand grains landing on the ground. The mechanism is little understood but the particles usually have a negative charge when their diameter is under 250 μm and a positive one when they are over 500 μm.[70][71]

Ecology and biogeography

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Deserts and semi-deserts are home to ecosystems with low or very low biomass and primary productivity in arid or semi-arid climates. They are mostly found in subtropical high-pressure belts and major continental rain shadows. Primary productivity depends on low densities of small photoautotrophs that sustain a sparse trophic network. Plant growth is limited by rainfall, temperature extremes and desiccating winds. Deserts have strong temporal variability in the availability of resources due to the total amount of annual rainfall and the size of individual rainfall events. Resources are often ephemeral or episodic, and this triggers sporadic animal movements and 'pulse and reserve' or 'boom-bust' ecosystem dynamics. Erosion and sedimentation are high due to the sparse vegetation cover and the activities of large mammals and people. Plants and animals in deserts are mostly adapted to extreme and prolonged water deficits, but their reproductive phenology often responds to short episodes of surplus. Competitive interactions are weak.[72]

Flora

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xeroscape of cacti in Baja
Xerophytes: Cardón cacti in the Baja California desert, Cataviña region, Mexico

Plants face severe challenges in arid environments. Problems they need to solve include how to obtain enough water, how to avoid being eaten and how to reproduce. Photosynthesis is the key to plant growth. It can only take place during the day as energy from the sun is required, but during the day, many deserts become very hot. Opening stomata to allow in the carbon dioxide necessary for the process causes evapotranspiration, and conservation of water is a top priority for desert vegetation. Some plants have resolved this problem by adopting crassulacean acid metabolism, allowing them to open their stomata during the night to allow CO2 to enter, and close them during the day,[73] or by using C4 carbon fixation.[74]

Many desert plants have reduced the size of their leaves or abandoned them altogether. Cacti are present in both North and South America with a post-Gondwana origin. The genus is desert specialist, and in most species, the leaves have been dispensed with and the chlorophyll displaced into the trunks, the cellular structure of which has been modified to allow them to store water. When rain falls, the water is rapidly absorbed by the shallow roots and retained to allow them to survive until the next downpour, which may be months or years away.[75] The giant saguaro cacti of the Sonoran Desert form "forests", providing shade for other plants and nesting places for desert birds. Saguaro grows slowly but may live for up to two hundred years. The surface of the trunk is folded like a concertina, allowing it to expand, and a large specimen can hold eight tons of water after a good downpour.[75]

Other xerophytic plants have developed similar strategies by a process known as convergent evolution.[76] They limit water loss by reducing the size and number of stomata, by having waxy coatings and hairy or tiny leaves. Some are deciduous, shedding their leaves in the driest season, and others curl their leaves up to reduce transpiration. Others, such as aloes, store water in succulent leaves or stems or in fleshy tubers.

Desert plants maximize water uptake by having shallow roots that spread widely, or by developing long taproots that reach down to deep rock strata for ground water.[77] The saltbush in Australia has succulent leaves and secretes salt crystals, enabling it to live in saline areas.[77][78] In common with cacti, many have developed spines to ward off browsing animals.[75]

camel thorn tree, Acacia erioloba in the Namib Desert in Namibia
The camel thorn tree (Acacia erioloba) in the Namib Desert is nearly leafless in dry periods.

Some desert plants produce seed which lies dormant in the soil until sparked into growth by rainfall. With annuals, such plants grow with great rapidity and may flower and set seed within weeks, aiming to complete their development before the last vestige of water dries up. For perennial plants, reproduction is more likely to be successful if the seed germinates in a shaded position, but not so close to the parent plant as to be in competition with it. Some seed will not germinate until it has been blown about on the desert floor to scarify the seed coat. The seed of the mesquite tree, which grows in deserts in the Americas, is hard and fails to sprout even when planted carefully. When it has passed through the gut of a pronghorn it germinates readily, and the little pile of moist dung provides an excellent start to life well away from the parent tree.[75] The stems and leaves of some plants lower the surface velocity of sand-carrying winds and protect the ground from erosion. Even small fungi and microscopic plant organisms found on the soil surface (so-called cryptobiotic soil) can be a vital link in preventing erosion and providing support for other living organisms. Cold deserts often have high concentrations of salt in the soil. Grasses and low shrubs are the dominant vegetation here and the ground may be covered with lichens. Most shrubs have spiny leaves and shed them in the coldest part of the year.[79]

Fauna

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A cream-colored courser camouflaging in a desert.
The cream-colored courser is a well-camouflaged desert resident with its dusty coloration, countershading, and disruptive head markings.

Animals adapted to live in deserts are called xerocoles. There is no evidence that body temperature of mammals and birds is adaptive to the different climates, either of great heat or cold. In fact, with a very few exceptions, their basal metabolic rate is determined by body size, irrespective of the climate in which they live.[80] Many desert animals (and plants) show especially clear evolutionary adaptations for water conservation or heat tolerance and so are often studied in comparative physiology, ecophysiology, and evolutionary physiology. One well-studied example is the specializations of mammalian kidneys shown by desert-inhabiting species.[81] Many examples of convergent evolution have been identified in desert organisms, including between cacti and Euphorbia, kangaroo rats and jerboas, Phrynosoma and Moloch lizards.[82]

Deserts present a very challenging environment for animals. Not only do they require food and water but they also need to keep their body temperature at a tolerable level. In many ways, birds are the ablest to do this of the higher animals. They can move to areas of greater food availability as the desert blooms after local rainfall and can fly to faraway waterholes. In hot deserts, gliding birds can remove themselves from the over-heated desert floor by using thermals to soar in the cooler air at great heights. In order to conserve energy, other desert birds run rather than fly. The cream-colored courser flits gracefully across the ground on its long legs, stopping periodically to snatch up insects. Like other desert birds, it is well-camouflaged by its coloring and can merge into the landscape when stationary. The sandgrouse is an expert at this and nests on the open desert floor dozens of kilometers (miles) away from the waterhole it needs to visit daily. Some small diurnal birds are found in very restricted localities where their plumage matches the color of the underlying surface. The desert lark takes frequent dust baths which ensures that it matches its environment.[83]

Water and carbon dioxide are metabolic end products of oxidation of fats, proteins, and carbohydrates.[84] Oxidising a gram of carbohydrate produces 0.60 grams of water; a gram of protein produces 0.41 grams of water; and a gram of fat produces 1.07 grams of water,[85] making it possible for xerocoles to live with little or no access to drinking water.[86] The kangaroo rat for example makes use of this water of metabolism and conserves water both by having a low basal metabolic rate and by remaining underground during the heat of the day,[87] reducing loss of water through its skin and respiratory system when at rest.[86][88] Herbivorous mammals obtain moisture from the plants they eat. Species such as the addax antelope,[89] dik-dik, Grant's gazelle and oryx are so efficient at doing this that they apparently never need to drink.[90] The camel is a superb example of a mammal adapted to desert life. It minimizes its water loss by producing concentrated urine and dry dung, and is able to lose 40% of its body weight through water loss without dying of dehydration.[91] Carnivores can obtain much of their water needs from the body fluids of their prey.[92] Many other hot desert animals are nocturnal, seeking out shade during the day or dwelling underground in burrows. At depths of more than 50 cm (20 in), these remain at between 30 and 32 °C (86 and 90 °F) regardless of the external temperature.[92] Jerboas, desert rats, kangaroo rats and other small rodents emerge from their burrows at night and so do the foxes, coyotes, jackals and snakes that prey on them. Kangaroos keep cool by increasing their respiration rate, panting, sweating and moistening the skin of their forelegs with saliva.[93] Mammals living in cold deserts have developed greater insulation through warmer body fur and insulating layers of fat beneath the skin. The arctic weasel has a metabolic rate that is two or three times as high as would be expected for an animal of its size. Birds have avoided the problem of losing heat through their feet by not attempting to maintain them at the same temperature as the rest of their bodies, a form of adaptive insulation.[80] The emperor penguin has dense plumage, a downy under layer, an air insulation layer next to the skin and various thermoregulatory strategies to maintain its body temperature in one of the harshest environments on Earth.[94]

A desert iguana sunning on a rock
The desert iguana (Dipsosaurus dorsalis) is well-adapted to desert life.

Being ectotherms, reptiles are unable to live in cold deserts but are well-suited to hot ones. In the heat of the day in the Sahara, the temperature can rise to 50 °C (122 °F). Reptiles cannot survive at this temperature and lizards will be prostrated by heat at 45 °C (113 °F). They have few adaptations to desert life and are unable to cool themselves by sweating so they shelter during the heat of the day. In the first part of the night, as the ground radiates the heat absorbed during the day, they emerge and search for prey. Lizards and snakes are the most numerous in arid regions and certain snakes have developed a novel method of locomotion that enables them to move sidewards and navigate high sand-dunes. These include the horned viper of Africa and the sidewinder of North America, evolutionarily distinct but with similar behavioural patterns because of convergent evolution. Many desert reptiles are ambush predators and often bury themselves in the sand, waiting for prey to come within range.[95]

Amphibians might seem unlikely desert-dwellers, because of their need to keep their skins moist and their dependence on water for reproductive purposes. In fact, the few species that are found in this habitat have made some remarkable adaptations. Most of them are fossorial, spending the hot dry months aestivating in deep burrows. While there they shed their skins a number of times and retain the remnants around them as a waterproof cocoon to retain moisture. In the Sonoran Desert, Couch's spadefoot toad spends most of the year dormant in its burrow. Heavy rain is the trigger for emergence and the first male to find a suitable pool calls to attract others. Eggs are laid and the tadpoles grow rapidly as they must reach metamorphosis before the water evaporates. As the desert dries out, the adult toads rebury themselves. The juveniles stay on the surface for a while, feeding and growing, but soon dig themselves burrows. Few make it to adulthood.[96] The water holding frog in Australia has a similar life cycle and may aestivate for as long as five years if no rain falls.[97] The Desert rain frog of Namibia is nocturnal and survives because of the damp sea fogs that roll in from the Atlantic.[98]

Tadpole shrimp facing left on desert sand
Tadpole shrimp survive dry periods as eggs, which rapidly hatch and develop after rain.

Invertebrates, particularly arthropods, have successfully made their homes in the desert. Flies, beetles, ants, termites, locusts, millipedes, scorpions and spiders[99] have hard cuticles which are impervious to water and many of them lay their eggs underground and their young develop away from the temperature extremes at the surface.[100] The Saharan silver ant (Cataglyphis bombycina) uses a heat shock protein in a novel way and forages in the open during brief forays in the heat of the day.[101] The long-legged darkling beetle in Namibia stands on its front legs and raises its carapace to catch the morning mist as condensate, funnelling the water into its mouth.[102] Some arthropods make use of the ephemeral pools that form after rain and complete their life cycle in a matter of days. The desert shrimp does this, appearing "miraculously" in new-formed puddles as the dormant eggs hatch. Others, such as brine shrimps, fairy shrimps and tadpole shrimps, are cryptobiotic and can lose up to 92% of their bodyweight, rehydrating as soon as it rains and their temporary pools reappear.[103]

Human relations

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Humans have long made use of deserts as places to live,[104] and more recently have started to exploit them for minerals[105] and energy capture.[106] Deserts play a significant role in human culture with an extensive literature.[107] Deserts can only support a limited population of both humans and animals.[108]

History

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A human with a group of camels in a desert
A camel shepherd near Marrakech.

People have been living in deserts for millennia. Many, such as the Bushmen in the Kalahari, the Aborigines in Australia and various tribes of North American Indians, were originally hunter-gatherers. They developed skills in the manufacture and use of weapons, animal tracking, finding water, foraging for edible plants and using the things they found in their natural environment to supply their everyday needs. Their self-sufficient skills and knowledge were passed down through the generations by word of mouth.[104] Other cultures developed a nomadic way of life as herders of sheep, goats, cattle, camels, yaks, llamas or reindeer. They travelled over large areas with their herds, moving to new pastures as seasonal and erratic rainfall encouraged new plant growth. They took with them their tents made of cloth or skins draped over poles and their diet included milk, blood and sometimes meat.[109]

Salt caravan of heavy laden camels in desert
Salt caravan travelling between Agadez and the Bilma salt mines

The desert nomads were also traders. The Sahara is a very large expanse of land stretching from the Atlantic rim to Egypt. Trade routes were developed linking the Sahel in the south with the fertile Mediterranean region to the north and large numbers of camels were used to carry valuable goods across the desert interior. The Tuareg were traders and the transported goods traditionally included slaves, ivory and gold going northwards and salt going southwards. Berbers with knowledge of the region were employed to guide the caravans between the various oases and wells.[110] Several million slaves may have been taken northwards across the Sahara between the 8th and 18th centuries.[111] Traditional means of overland transport declined with the advent of motor vehicles, shipping and air freight, but caravans still travel along routes between Agadez and Bilma and between Timbuktu and Taoudenni carrying salt from the interior to desert-edge communities.[112]

Round the rims of deserts, where more precipitation occurred and conditions were more suitable, some groups took to cultivating crops. This may have happened when drought caused the death of herd animals, forcing herdsmen to turn to cultivation. With few inputs, they were at the mercy of the weather and may have lived at bare subsistence level. The land they cultivated reduced the area available to nomadic herders, causing disputes over land. The semi-arid fringes of the desert have fragile soils which are at risk of erosion when exposed, as happened in the American Dust Bowl in the 1930s. The grasses that held the soil in place were ploughed under, and a series of dry years caused crop failures, while enormous dust storms blew the topsoil away. Half a million Americans were forced to leave their land in this catastrophe.[113]

Similar damage is being done today to the semi-arid areas that rim deserts and about twelve million hectares of land are being turned to desert each year.[114] Desertification is caused by such factors as drought, climatic shifts, tillage for agriculture, overgrazing and deforestation. Vegetation plays a major role in determining the composition of the soil. In many environments, the rate of erosion and run off increases dramatically with reduced vegetation cover.[115]

Natural resource extraction

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see description
A mining plant near Jodhpur, India

Deserts contain substantial mineral resources, sometimes over their entire surface, giving them their characteristic colors. For example, the red of many sand deserts comes from laterite minerals.[116] Geological processes in a desert climate can concentrate minerals into valuable deposits. Leaching by ground water can extract ore minerals and redeposit them, according to the water table, in concentrated form.[105] Similarly, evaporation tends to concentrate minerals in desert lakes, creating dry lake beds or playas rich in minerals. Evaporation can concentrate minerals as a variety of evaporite deposits, including gypsum, sodium nitrate, sodium chloride and borates.[105] Evaporites are found in the US's Great Basin Desert, historically exploited by the "20-mule teams" pulling carts of borax from Death Valley to the nearest railway.[105] A desert especially rich in mineral salts is the Atacama Desert, Chile, where sodium nitrate has been mined for explosives and fertilizer since around 1850.[105] Other desert minerals are copper from Chile, Peru, and Iran, and iron and uranium in Australia. Many other metals, salts and commercially valuable types of rock such as pumice are extracted from deserts around the world.[105]

Oil and gas form on the bottom of shallow seas when micro-organisms decompose under anoxic conditions and later become covered with sediment. Many deserts were at one time the sites of shallow seas and others have had underlying hydrocarbon deposits transported to them by the movement of tectonic plates.[117] Some major oilfields such as Ghawar are found under the sands of Saudi Arabia.[105] Geologists believe that other oil deposits were formed by aeolian processes in ancient deserts as may be the case with some of the major American oil fields.[105]

Farming

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aerial view of the Imperial valley showing the pattern of irrigation
Mosaic of fields in Imperial Valley

Traditional desert farming systems have long been established in North Africa, irrigation being the key to success in an area where water stress is a limiting factor to growth. Techniques that can be used include drip irrigation, the use of organic residues or animal manures as fertilisers and other traditional agricultural management practices. Once fertility has been built up, further crop production preserves the soil from destruction by wind and other forms of erosion.[118] It has been found that plant growth-promoting bacteria play a role in increasing the resistance of plants to stress conditions and these rhizobacterial suspensions could be inoculated into the soil in the vicinity of the plants. A study of these microbes found that desert farming hampers desertification by establishing islands of fertility allowing farmers to achieve increased yields despite the adverse environmental conditions.[118] A field trial in the Sonoran Desert which exposed the roots of different species of tree to rhizobacteria and the nitrogen fixing bacterium Azospirillum brasilense with the aim of restoring degraded lands was only partially successful.[118]

The Judean Desert was farmed in the 7th century BC during the Iron Age to supply food for desert forts.[119] Native Americans in the south western United States became agriculturalists around 600 AD when seeds and technologies became available from Mexico. They used terracing techniques and grew gardens beside seeps, in moist areas at the foot of dunes, near streams providing flood irrigation and in areas irrigated by extensive specially built canals. The Hohokam tribe constructed over 500 miles (800 km) of large canals and maintained them for centuries, an impressive feat of engineering. They grew maize, beans, squash and peppers.[120]

A modern example of desert farming is the Imperial Valley in California, which has high temperatures and average rainfall of just 3 in (76 mm) per year.[121] The economy is heavily based on agriculture and the land is irrigated through a network of canals and pipelines sourced entirely from the Colorado River via the All-American Canal. The soil is deep and fertile, being part of the river's flood plains, and what would otherwise have been desert has been transformed into one of the most productive farming regions in California. Other water from the river is piped to urban communities but all this has been at the expense of the river, which below the extraction sites no longer has any above-ground flow during most of the year. Another problem of growing crops in this way is the build-up of salinity in the soil caused by the evaporation of river water.[122] The greening of the desert remains an aspiration and was at one time viewed as a future means for increasing food production for the world's growing population. This prospect has proved false as it disregarded the environmental damage caused elsewhere by the diversion of water for desert project irrigation.[123]

Solar energy capture

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satellite view with solar and renewal energy potential of Sahara and Europe
Desertec proposed using the Saharan and Arabian deserts to produce solar energy to power Europe and the Middle East.

Deserts are increasingly seen as sources for solar energy, partly due to low amounts of cloud cover. Many solar power plants have been built in the Mojave Desert such as the Solar Energy Generating Systems and Ivanpah Solar Power Facility.[124] Large swaths of this desert are covered in mirrors.[125]

The potential for generating solar energy from the Sahara Desert is huge, the highest found on the globe. Professor David Faiman of Ben-Gurion University has stated that the technology now exists to supply all of the world's electricity needs from 10% of the Sahara Desert.[126] Desertec Industrial Initiative was a consortium seeking $560 billion to invest in North African solar and wind installations over the next forty years to supply electricity to Europe via cable lines running under the Mediterranean Sea. European interest in the Sahara Desert stems from its two aspects: the almost continual daytime sunshine and plenty of unused land. The Sahara receives more sunshine per acre than any part of Europe. The Sahara Desert also has the empty space totalling hundreds of square miles required to house fields of mirrors for solar plants.[127]

The Negev Desert, Israel, and the surrounding area, including the Arava Valley, receive plenty of sunshine and are generally not arable. This has resulted in the construction of many solar plants.[106] David Faiman has proposed that "giant" solar plants in the Negev could supply all of Israel's needs for electricity.[126]

Warfare

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Battle of El Alamein
War in the desert: Battle of El Alamein, 1942

The Arabs were probably the first organized force to conduct successful battles in the desert. By knowing back routes and the locations of oases and by utilizing camels, Muslim Arab forces were able to successfully overcome both Roman and Persian forces in the period 600 to 700 AD during the expansion of the Islamic caliphate.[128]

Many centuries later, both world wars saw fighting in the desert. In the First World War, the Ottoman Turks were engaged with the British regular army in a campaign that spanned the Arabian Peninsula. The Turks were defeated by the British, who had the backing of irregular Arab forces that were seeking to revolt against the Turks in the Hejaz, made famous in T.E. Lawrence's book Seven Pillars of Wisdom.[129][130]

In the Second World War, the Western Desert Campaign began in Italian Libya. Warfare in the desert offered great scope for tacticians to use the large open spaces without the distractions of casualties among civilian populations. Tanks and armoured vehicles were able to travel large distances unimpeded and land mines were laid in large numbers. However, the size and harshness of the terrain meant that all supplies needed to be brought in from great distances. The victors in a battle would advance and their supply chain would necessarily become longer, while the defeated army could retreat, regroup and resupply. For these reasons, the front line moved back and forth through hundreds of kilometers as each side lost and regained momentum.[131] Its most easterly point was at El Alamein in Egypt, where the Allies decisively defeated the Axis forces in 1942.[132]

In culture

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drawing of Marco Polo disembarking from ship and entering castle with camels
Marco Polo arriving in a desert land with camels. 14th-century miniature from Il milione.

The desert is generally thought of as a barren and empty landscape. It has been portrayed by writers, film-makers, philosophers, artists and critics as a place of extremes, a metaphor for anything from death, war or religion to the primitive past or the desolate future.[133]

There is an extensive literature on the subject of deserts.[107] An early historical account is that of Marco Polo (c. 1254–1324), who travelled through Central Asia to China, crossing a number of deserts in his twenty four year trek.[134] Some accounts give vivid descriptions of desert conditions, though often accounts of journeys across deserts are interwoven with reflection, as is the case in Charles Montagu Doughty's major work, Travels in Arabia Deserta (1888).[135] Antoine de Saint-Exupéry described both his flying and the desert in Wind, Sand and Stars,[136] and Gertrude Bell travelled extensively in the Arabian desert in the early part of the 20th century, becoming an expert on the subject, writing books and advising the British government on dealing with the Arabs.[137] Another woman explorer was Freya Stark, who travelled alone in the Middle East, visiting Turkey, Arabia, Yemen, Syria, Persia and Afghanistan, writing over twenty books on her experiences.[138] The German naturalist Uwe George spent several years living in deserts, recording his experiences and research in his 1976 book, In the Deserts of this Earth.[139]

The American poet Robert Frost expressed his bleak thoughts in his poem, Desert Places (1933), which ends with the stanza "They cannot scare me with their empty spaces / Between stars – on stars where no human race is. / I have it in me so much nearer home / To scare myself with my own desert places."[140]

Saints associated with the desert include Anthony the Great, also known as "Anthony of the Desert". Pope Benedict XVI linked the metaphorical existence of "internal deserts" with physical and social deserts in his homily inaugurating his papacy: "The external deserts in the world are growing, because the internal deserts have become so vast".[141]

Deserts on other planets

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view of Martian desert showing rock field to the horizon
View of the Martian desert seen by the robotic rover Spirit in 2004

Mars is the only other planet in the Solar System besides Earth on which deserts have been identified.[142] Despite its low surface atmospheric pressure (only 1/100 of that of Earth), the patterns of atmospheric circulation on Mars have formed a sea of circumpolar sand more than 5 million km2 (1.9 million sq mi) in the area, larger than most deserts on Earth. The Martian deserts consist of half-moon dunes in flat areas near the permanent polar ice caps in the north. The smaller dune fields occupy the bottom of many of the craters situated in the Martian polar regions.[143] Examination of the surface of rocks by laser beamed from the Mars Exploration Rover have shown a surface film that resembles the desert varnish found on Earth although it might just be surface dust.[144] The surface of Titan, a moon of Saturn, also has a desert-like surface with dune seas.[145]

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
A desert is an arid landscape or biome defined by extremely low annual precipitation, generally less than 250 millimeters (10 inches), which limits vegetation cover and exposes the terrain to intense solar radiation, high evaporation rates, and wind-driven erosion processes. Deserts encompass about one-third of Earth's continental land surface, spanning every continent from equatorial subtropics to polar latitudes, and include diverse subtypes such as hot deserts with extreme daytime temperatures exceeding 50°C (122°F), cold deserts with freezing winters, coastal fog deserts reliant on marine moisture, and polar deserts where low temperatures inhibit precipitation despite minimal evaporation. These environments form primarily through atmospheric dynamics, including subsidence zones in subtropical high-pressure belts that suppress convection and rainfall, or topographic rain shadows where prevailing winds lose moisture ascending mountain barriers, leaving leeward slopes dry. Despite their harsh conditions, deserts sustain resilient ecosystems with adaptations like deep-rooted xerophytes, nocturnal animals, and ephemeral water-dependent species, while geomorphic features such as shifting sand dunes, deflation hollows, and evaporite basins reveal ongoing aeolian and fluvial processes; only about 20% consist of sand seas, with most areas dominated by gravel plains, rocky plateaus, or salt flats. Human expansion into desert fringes has accelerated desertification via overgrazing and deforestation, though natural variability tied to orbital cycles and solar forcing underscores that aridity is fundamentally driven by causal geophysical mechanisms rather than solely anthropogenic factors.

Definition and Terminology

Etymology

The English word desert, denoting a barren or arid region, originates from the Latin dēsertum, a neuter past participle of dēserere meaning "to abandon" or "to forsake," thus signifying "an abandoned place" or "wasteland." This root emphasized desolation and lack of human habitation rather than aridity per se, as seen in ecclesiastical Latin usage where dēsertum described forsaken territories. The term entered as desert or deserte around the 12th century, retaining the sense of an uncultivated or uninhabited expanse, before adoption into by the late 12th century (first attested c. 1155 in place names and c. 1200 in general use). Early English applications, such as in biblical or exploratory contexts, evoked perceptions of isolation and abandonment, mirroring historical views of such landscapes as divinely or naturally shunned. In contrast to this etymological focus on forsakenness, modern prioritizes measurable criteria like annual below 250 mm (10 inches), decoupling the word from its origins in cultural notions of barren vacancy.

Defining Characteristics

Deserts are regions where extreme aridity prevails, defined quantitatively by the (AI), calculated as the ratio of mean annual (P) to potential evapotranspiration (PET), reflecting the imbalance between water input and atmospheric demand. The (UNEP) establishes hyper-arid conditions at AI < 0.05 and arid at 0.05 ≤ AI < 0.20, thresholds marking environments where evaporative losses chronically exceed , leading to negligible recharge of soil moisture reserves. These criteria prioritize hydrological physics over mere rainfall totals, as high PET—driven by intense solar insolation, elevated temperatures often exceeding 30°C daily maxima, low relative humidity below 30%, and wind speeds averaging 5-10 m/s—amplifies water deficit even when P surpasses simplistic benchmarks. In practice, this manifests as annual P typically below 250 mm in hot deserts, with hyper-arid exemplars like the Atacama receiving under 10 mm, but the AI underscores causal realism: persistent desiccating winds and radiative heating elevate PET to 2000-3000 mm annually, ensuring soil water availability remains below wilting point thresholds (around 0.05-0.10 volumetric content) for most terrestrial plants. Vegetation scarcity follows as a direct outcome, with cover rarely exceeding 10-15% and dominated by xeromorphic adaptations, as sustained moisture deficits preclude competitive growth of mesic species. This excludes transiently barren landscapes, such as post-fire regrowth zones or rain-shadow foothills with episodic recharge, emphasizing chronic atmospheric aridity over perceptual sterility. The UNEP framework thus anchors desert identification in empirical water balance, avoiding overreliance on precipitation alone, which falters in cold deserts where low PET (under 300 mm) permits aridity despite P of 100-200 mm, as in Antarctic interiors. Semi-arid zones (0.20 ≤ AI < 0.50), while dry, support steppes rather than true deserts due to marginally higher moisture retention, highlighting the index's role in delineating biophysical thresholds.

Classification and Types

Climatic and Precipitation-Based

Deserts classified by climatic and precipitation-based criteria emphasize atmospheric circulation patterns and topographic influences that suppress rainfall, typically defined as regions receiving less than 250 millimeters annually. Subtropical deserts form primarily under the descending branch of Hadley cells, where air subsidence around 30° latitude warms adiabatically, increasing relative humidity thresholds and inhibiting convection essential for precipitation. This mechanism, observed in satellite-derived circulation data, results in persistent high-pressure systems that divert moist tropical air equatorward, yielding annual precipitation often below 100 millimeters in core zones. Rain shadow deserts arise from orographic blocking, where prevailing winds encounter mountain barriers, forcing moist air to rise, cool, and precipitate on windward slopes, leaving leeward areas depleted of moisture. In such regimes, the rain shadow effect intensifies aridity through reduced vapor transport, as evidenced by station records showing gradients from wet highlands to hyperarid basins; for instance, Andean topography blocks easterly flows, contributing to precipitation minima under 1 millimeter per year in sheltered valleys. Mid-latitude continental deserts develop in interiors distant from oceanic moisture sources, where air masses traverse vast land expanses, progressively losing humidity via limited evaporation and potential rainout, constrained by weak cyclonic influences. Empirical global precipitation datasets reveal these areas sustain low rainfall regimes, averaging 100-200 millimeters annually, due to the attenuation of maritime air signals over thousands of kilometers. Overall, these subtypes reflect causal interplay of large-scale dynamics and geography, corroborated by long-term observations from weather stations and reanalysis products.

Temperature and Polar Deserts

Deserts exhibit diverse thermal profiles, with hot variants characterized by intense diurnal temperature fluctuations due to low atmospheric moisture and high solar insolation. In regions like the , daytime surface temperatures frequently exceed 40°C, with air temperatures reaching up to 58°C in extreme cases, while nocturnal drops below 0°C are common, yielding diurnal ranges of 14–25°C. These extremes arise from rapid radiative cooling at night absent significant cloud cover or humidity to retain heat. Cold deserts, such as the Gobi, feature pronounced seasonal temperature swings rather than daily extremes, with winter lows averaging -40°C and summer highs up to 45°C. Annual means hover near 0°C or below, reflecting continental interiors distant from moderating oceanic influences, where freezing winters lock precipitation as ice, rendering it unavailable and perpetuating aridity despite occasional snowfall. This contrasts with hot deserts by emphasizing prolonged cold periods over diurnal volatility, yet both underscore aridity's independence from heat, as low moisture limits evaporative moderation in either regime. Polar deserts extend this principle to perpetually low temperatures, classified by annual precipitation below 250 mm water equivalent—often under 50 mm in interior —and mean temperatures in the warmest month under 10°C. In and Arctic high latitudes, scant snowfall undergoes sublimation rather than melting, maintaining effective water scarcity despite ice accumulation. Ice core analyses reveal persistent aridity over millennia, with elevated dust concentrations signaling dry source regions and minimal moisture transport, as dust influx correlates inversely with precipitation en route to polar sites. Thus, polar aridity stems from cold-trapped hydrology, where frozen precipitation evades biological or geomorphic utilization, akin to liquid deficits in warmer deserts.

Specialized Deserts

Coastal deserts represent a specialized category of arid regions where low precipitation persists despite proximity to oceans, primarily due to cold upwelling currents that stabilize the atmosphere and inhibit convective rainfall. These currents, such as the off Namibia and the along Chile, bring nutrient-rich but cold waters to the surface, cooling overlying air and preventing the release of moisture as rain, even as warmer air masses approach. This mechanism overrides the typical moisture availability expected near coastlines, resulting in hyper-arid conditions with annual precipitation often below 25 mm in core areas. The Namib Desert exemplifies this dynamic, stretching over 1,200 km along southwestern Africa's Atlantic coast, where the Benguela Current's influence creates a persistent fog belt but minimal rainfall, with some inland sites recording less than 10 mm annually. Geological evidence indicates the Namib's aridity dates back at least 55 million years, sustained by tectonic stability and consistent oceanographic patterns that limit evaporation and precipitation. Similarly, the in northern Chile combines coastal cold current effects with topographic barriers, yielding zones where no measurable rain has fallen in recorded history, such as Arica experiencing zero precipitation from 1570 to 1971 in some estimates. These deserts support unique ecosystems reliant on fog interception for limited water, highlighting causal factors beyond simple latitudinal climate bands. Biological deserts, characterized by extreme nutrient scarcity or biodiversity deficits rather than precipitation alone, are less commonly applied to terrestrial contexts but draw analogies from oceanic gyres where low primary productivity arises from nutrient poverty in stratified waters. On land, such concepts occasionally describe heavily modified landscapes like monoculture plantations, where species uniformity and soil depletion mimic desert-like ecological barrenness, as seen in eucalyptus or oil palm estates that reduce native biodiversity by over 90% compared to undisturbed habitats. However, verifiable geophysical examples remain sparse, with most terrestrial aridity still tied to hydrological limits rather than isolated nutrient dynamics. Urban heat islands in desert cities, while intensifying local temperatures by 1-5°C through impervious surfaces and reduced vegetation, do not typically create micro-deserts by altering precipitation patterns, though they exacerbate evaporative stress in already arid settings.

Physical Geography

Climate and Hydrology

Deserts exhibit extreme aridity defined by an aridity index (AI) below 0.2, where annual precipitation divided by potential evapotranspiration yields values indicating severe water deficits, often with rainfall under 250 mm per year in hot deserts. This aridity stems from persistent subsidence within high-pressure cells, such as the Hadley circulation, where descending air warms dry-adiabatically at approximately 9.8°C per kilometer, suppressing convection and maintaining low humidity levels typically below 20% relative humidity. The resulting clear skies—often over 300 sunny days annually—permit intense solar insolation exceeding 3,000 kWh per square meter yearly in regions like the , driving daytime surface temperatures above 50°C in summer while enabling efficient longwave radiative cooling at night. Hydrologically, deserts feature negligible sustained surface water due to high potential evapotranspiration rates surpassing precipitation by factors of 5 to over 50, as quantified by the AI, which perpetuates soil moisture deficits and limits vegetation cover. Rare precipitation events, concentrated in convective storms, generate flash floods in ephemeral channels (), where impermeable soils and scant infiltration—often less than 10% of rainfall—cause rapid runoff velocities up to 10 m/s, eroding channels but contributing minimally to perennial streams. These dynamics yield near-zero baseflow, with water balance dominated by evaporation from bare soil and transpiration from sparse , as confirmed by eddy covariance measurements showing actual evapotranspiration rates aligning closely with episodic rainfall inputs rather than potential demands. Deep groundwater sustains isolated oases through fossil aquifers recharged during pluvial periods up to 10,000 years ago, bypassing contemporary aridity. The Nubian Sandstone Aquifer System, spanning 2.6 million km² under the Sahara, contains non-renewable paleowater with radiocarbon ages exceeding 30,000 years, discharging at rates of 0.1-1 m³/s to form oases like those in Egypt's Western Desert. Such systems exhibit confined flow with hydraulic gradients under 0.001, resulting in artesian pressures in some wells, but extraction exceeds recharge—estimated at less than 1% of annual withdrawal—threatening depletion over decades of use. Overall, desert hydrology reflects episodic inputs against chronic deficits, with aquifers buffering but not alleviating the fundamental water scarcity driven by atmospheric persistence.

Landforms and Morphology

Desert landforms arise primarily from aeolian processes of erosion, transportation, and deposition, with episodic fluvial contributions due to infrequent but intense rainfall. Wind-driven abrasion by saltating sand grains shapes resistant bedrock into yardangs, elongated, streamlined ridges oriented parallel to prevailing winds, where softer intervening material is preferentially removed. Ventifacts form as exposed rocks are faceted, pitted, and polished on windward sides by persistent sandblasting, creating flat, sculpted surfaces aligned with dominant wind directions. Deflation, the selective entrainment and removal of fine particles by wind, lowers surfaces and concentrates coarser lags, producing desert pavements—closely packed pebble surfaces that armor the ground and inhibit further erosion. Depositional features dominate in areas of sand supply and reduced wind velocity, forming dunes through accumulation of transported sediment. Barchan dunes exhibit crescentic morphology with trailing arms (horns) extending leeward, migrating downwind at rates up to 20 meters per year via grain saltation and avalanching on slip faces. Longitudinal dunes, or seif dunes, develop as linear ridges parallel to unidirectional winds, elongating at rates around 13 meters per year in some regions. Rare fluvial activity carves wadis, intermittent V-shaped channels incised by flash floods that transport sediment during brief high-discharge events, leaving dry beds flanked by alluvial fans. In closed basins, playas accumulate ephemeral shallow lakes fed by runoff; upon evaporation, dissolved minerals precipitate sequentially as crystals, forming expansive salt flats through cycles of wetting, drying, and crystallization driven by decreasing solubility with water loss. Over millennial timescales, desert landscapes evolve slowly under minimal relief production and sediment flux, with catchment-averaged denudation rates of 1–10 mm per thousand years measured via cosmogenic nuclides like ¹⁰Be in bedrock and fluvial sediments, reflecting limited chemical and physical weathering in hyperarid conditions. These rates underscore the dominance of wind over water in sustaining subdued topography despite prolonged exposure.

Weather and Dynamic Processes

Desert weather features transient convective phenomena driven by intense solar heating of arid surfaces, leading to atmospheric instability. Dust devils arise from localized thermal updrafts in clear skies over flat, barren terrain, where superadiabatic lapse rates generate vertical vorticity and entrain dust particles. These vortices typically form during midday when surface temperatures exceed 40°C, with frequencies peaking under low atmospheric stability rather than maximal heat alone. Larger-scale events, such as sandstorms and , stem from stronger wind gusts, often from thunderstorm downdrafts or frontal passages, propelling dust walls across hundreds of kilometers. , derived from the Arabic term for "blowing wind," manifest as rapidly advancing dust fronts that reduce horizontal visibility to below 100 meters, sometimes approaching zero, posing hazards to transportation. Mechanics involve saltation, where wind lifts sand grains into short trajectories up to 1 meter high, followed by bombardment that liberates finer particles into suspension for long-range transport. These processes contribute substantially to global aeolian dust flux, estimated at 1-2 gigatons annually from desert sources, with saltation accounting for 50-75% of sediment movement near the surface and suspension enabling intercontinental dispersal. Rare haboob-scale events can originate from outflows of distant thunderstorms, as evidenced by satellite observations tracking dust plumes across regions like the U.S. Southwest since 2020. Post-2020 studies integrating lidar, satellite imagery, and machine learning have enhanced detection of such propagating systems, revealing initiation from remote convective cells.

Global Distribution

Major Terrestrial Deserts

The major terrestrial deserts collectively occupy about one-third of Earth's land surface, totaling approximately 33 to 52 million km² based on satellite-derived classifications that account for aridity thresholds in precipitation and vegetation indices. Recent analyses using MODIS and NDVI data reveal fluctuations in desert boundaries over decades, with expansions and contractions driven by interannual precipitation variability rather than uniform trends, as observed in regions like central Asia and Australia. These deserts exhibit significant geographic variability, from subtropical high-pressure dominated hot deserts to continental cold deserts and polar ice deserts, influencing global dust cycles and albedo effects. The Sahara Desert in North Africa is the largest hot desert, spanning 9 million km² from the Atlantic Ocean to the Red Sea, characterized by a hyper-arid core with annual precipitation often below 25 mm in central regions. The Gobi Desert, a cold continental desert in Mongolia and northern China, covers about 1.3 million km², featuring extreme temperature swings and gravel plains interspersed with mountain ranges. The Australian Desert, encompassing subtropical interiors like the Great Victoria and Simpson Deserts, totals roughly 2.1 million km², or about 18% of the continent, with sandy and rocky terrains shaped by episodic rainfall events. The Arabian Desert, stretching across the Arabian Peninsula, includes vast sand seas like the Empty Quarter (approximately 660,000 km²), contributing to a broader arid expanse exceeding 2 million km² overall. Polar deserts represent the largest arid zones by area, with the Antarctic Desert covering an effective dry expanse of 13.8 million km² across the continent, where precipitation equivalents average less than 200 mm annually due to cold trapping of moisture. In contrast, the Atacama Desert along Chile's coast is among the oldest and driest non-polar deserts, with core areas receiving less than 1 mm of rain per year, sustained by the rain shadow of the Andes and persistent coastal upwelling. Other notable deserts include the Kalahari in southern Africa, spanning semi-arid to arid zones of about 900,000 km² with seasonal grass cover variability detectable via NDVI shifts. These inventories highlight how desert extents, mapped via remote sensing, fluctuate naturally by thousands of km² over decades without implying permanent expansion or contraction.
DesertApproximate Area (million km²)Primary LocationKey Aridity Feature
Sahara9.0North AfricaHyper-arid core (<25 mm/year rain)
Antarctic13.8AntarcticaPolar cold desert (<200 mm equiv.)
Australian2.1AustraliaSubtropical interiors
Gobi1.3Mongolia/ChinaCold winters, gravel-dominated
Arabian>2.0Vast erg sand seas
Atacama0.1Northern <1 mm/year in hyperarid zones

Ecology and Biology

Flora and Vegetative Adaptations


Desert flora exhibit specialized adaptations to survive extreme aridity, primarily through strategies that minimize water loss and maximize opportunistic use of scarce resources. Succulent plants, such as cacti, store water in thickened tissues and employ crassulacean acid metabolism (CAM) photosynthesis, where stomata open at night to fix CO₂, reducing transpiration by up to 90% compared to C3 plants during daylight hours. This temporal separation of gas exchange conserves water in hot, dry conditions prevalent in deserts like the Sonoran.
Phreatophytes, including species like mesquite (Prosopis glandulosa) and camel thorn (Acacia erioloba), develop extensive deep root systems extending meters into aquifers to access , bypassing shallow soil drought. These roots can reach depths of over 2 meters within weeks in seedlings, enabling sustained access in arid riparian zones. In contrast, ephemeral annuals complete their life cycles rapidly following infrequent rains, germinating within hours to days after events in fall or spring, as observed in species. Desert seed banks demonstrate remarkable dormancy, with viable seeds persisting for decades or longer, germinating only upon sufficient moisture cues in controlled burial experiments; for instance, seeds of Lepidium potaninii retained 64% after 18 months burial, supporting resilience. Net primary productivity in desert ecosystems remains low, typically 0.1-0.5 g C/m²/day annually, reflecting sparse vegetation and pulsed growth tied to rainfall. Physiological mechanisms like osmotic adjustment further enhance tolerance, allowing such as cold desert shrubs to accumulate solutes and maintain turgor under water deficits, as evidenced in seasonal studies of species like .

Fauna and Animal Adaptations

Desert primarily survive through behavioral strategies such as and burrowing, which mitigate extreme diurnal temperatures exceeding 50°C (122°F), alongside physiological mechanisms for water and energy conservation derived from metabolic processes. Small mammals like kangaroo rats (Dipodomys spp.) remain active only at night, retreating to burrows where soil temperatures can be 20–30°C cooler than surface highs, and obtain approximately 90% of their hydration from oxidizing dry seeds without drinking free water. These rodents' kidneys concentrate up to five times more than those of humans, minimizing evaporative loss in levels below 10% . Reptiles exhibit similar burrow use but incorporate ectothermic advantages; desert iguanas (Dipsosaurus dorsalis) bask briefly in early morning to raise body temperatures to optimal 35–40°C for activity, then seek shade or as heat intensifies, relying on behavioral rather than constant metabolic heat production. Camels (Camelus spp.), adapted for long-distance traversal, store as dorsal fat (yielding 1.1 grams of metabolic water per gram oxidized) and recycle with 94–97% efficiency via ruminal microbes, retaining nitrogen during dehydration periods lasting weeks. Genomic analyses confirm selection for genes enhancing urea transporters and osmoregulatory proteins in camels, enabling survival in hyper-arid zones with annual rainfall under 50 mm. Amphibians counter sporadic water availability through estivation, forming impermeable cocoons from shed skin to reduce cutaneous water loss by over 90% while burrowed; Couch's spadefoot toads (Scaphiopus couchii) can remain dormant up to two years, metabolizing fat reserves at rates as low as 0.1% body weight daily until rains trigger mass emergence and breeding. Birds adapt via migratory nomadism, with many songbirds crossing deserts nocturnally at altitudes above 1,000 meters to exploit cooler air and track ephemeral insect outbreaks or seed pulses, as evidenced by and GPS tracking showing consistent loop patterns synchronized to resource . Invertebrates like desert locusts enter , suspending development during dry phases, while predators in low-density prey environments, such as kit foxes, maintain hunting success through expanded territories (up to 200 km²) and acute olfactory detection thresholds below 10 parts per billion for sparse scents. These adaptations collectively sustain populations at densities as low as 0.1 individuals per , prioritizing survival over reproduction in resource-scarce matrices.

Ecosystem and Biogeographic Patterns

Desert ecosystems exhibit sparse biotic communities dominated by pulsed resource availability, where infrequent precipitation events drive boom-bust cycles in primary production and subsequent trophic cascades. Empirical studies of food webs reveal greater complexity than linear models predict, with detritivores and omnivores playing outsized roles in energy transfer due to slow microbial decomposition rates under low moisture conditions. In arid environments, higher trophic levels adapt through dietary flexibility and opportunistic foraging, sustaining populations amid chronic resource uncertainty. Nutrient cycling in these systems relies on localized hotspots facilitated by symbiotic and biogenic structures, compensating for oligotrophic soils. Mycorrhizal fungi form extensive networks with sparse , enhancing and uptake in water-limited conditions, thereby bolstering resilience and trophic support. colonies engineer fertility islands via mound construction, accelerating decomposition of lignocellulosic material and redistributing nutrients vertically in the profile, which empirical measurements confirm elevates local productivity. Transitional ecotones between deserts and adjacent biomes, such as savannas or shrublands, host elevated despite overall low , as converging environmental gradients foster specialized assemblages. Biogeographic patterns across deserts reflect historical climate oscillations rather than contemporary aridity alone, with Pleistocene refugia enabling persistence of endemic lineages amid glacial-interglacial shifts. Fossil pollen records from the Saharo-Arabian belt indicate recurrent humid corridors during the Pleistocene, supporting refugial habitats that preserved Afro-Asian faunal and floral elements now exhibiting high . These realms, spanning Palearctic and Afrotropical boundaries, show discrete biotic partitions driven by dispersal barriers like hyperarid phases, as evidenced by phylogeographic clustering in endemic taxa. Recent metagenomic analyses of biological soil crusts underscore their role in ecosystem stability, revealing diverse cyanobacterial and fungal assemblages that bind surface particles, mitigate , and fix atmospheric in barren expanses. Surveys from ecotones, conducted post-2023, demonstrate transcriptional responses to wetting events that activate and microbial trophic loops, enhancing cohesion against wind deflation. These crusts, covering up to 70% of some desert soils, integrate abiotic drivers with biotic feedbacks, forming foundational layers for higher trophic persistence.

Human Interactions

Historical Exploration and Settlement

Human presence in arid desert environments dates back to prehistoric times, with evidence of adaptations in regions like the around 12,800 years ago, as indicated by life-size depicting human figures and animals. Early settlements concentrated around oases, where enabled and permanent habitation; for instance, walled oases in northern Arabia supported sedentary communities from the Early onward, approximately 4,000 years ago. emerged with the domestication of the dromedary camel in the around 3000 BCE, facilitating mobility across hyper-arid zones and the rise of Bedouin-like groups who relied on , meat, and transport for survival in environments with minimal sources. Ancient trade routes amplified human traversal of deserts, with the establishing overland connections across Central Asian deserts like the Taklamakan and Gobi starting in 130 BCE under the , exchanging silk, spices, and ideas via camel caravans that navigated extreme aridity. Similarly, across North Africa's vast sands began around 500 BCE, initially on foot or with oxen, but expanded significantly after camel introduction around the 1st century CE, linking West African and salt sources to Mediterranean ports through organized caravans of up to 10,000 animals. In the Americas, indigenous groups adapted to desert conditions through semi-sedentary agriculture; the of the U.S. Southwest constructed cliff dwellings in arid canyons of Mesa Verde between approximately 1150 and 1300 CE, leveraging alcoves for protection against elements and enemies while farming mesa tops with techniques. European-led explorations intensified desert crossings in the , driven by geographic curiosity and imperial ambitions; Scottish explorer reached via routes in 1826, though he perished on the return journey, marking one of the first documented European traversals from north to south. Frenchman René Caillié successfully crossed the from south to north in 1828, disguising himself as an Arab to document after earlier failures highlighted the perils of heat, thirst, and hostile tribes. The saw technological aids for settlement and transit, including the French Trans-Saharan Railway project initiated in the early 1900s to connect Algerian ports to sub-Saharan colonies, though logistical challenges like sand drifts limited completion to partial segments by the 1920s. Oil prospecting post-World War I spurred semi-permanent camps in Middle Eastern deserts, evolving into structured settlements around extraction sites in Arabia starting in the .

Resource Extraction and Economic Value

Deserts contain substantial hydrocarbon deposits, particularly in the Middle East's Arabian and regions, which encompass arid terrains covering much of , the , , , and . As of 2024, these areas hold approximately 48% of global proven crude reserves and over 40% of reserves, with total oil reserves exceeding 800 billion barrels across the region. Extraction from fields like 's Ghawar (the world's largest conventional oil field) and the shared - South Pars/North Dome gas field (holding about 1,800 trillion cubic feet combined) generates revenues that constitute 30-50% of GDP in producer states such as and . These resources drive through exports, funding and diversification efforts, with 2024 production levels from the region supplying around 30% of global output. Mineral extraction further underscores deserts' economic significance, with operations targeting deposits formed under hyper-arid conditions. Morocco controls roughly 70% of worldwide rock reserves, estimated at 50 billion metric tons, primarily in the Saharan regions of and Boucraa; these yield over 30 million tons annually, accounting for 20-25% of national export earnings and supporting global fertilizer production. In South America's , mines from porphyry deposits in northern basins, producing about 5.5 million metric tons yearly as the global leader; major sites like and contribute to the sector's 10-15% share of national GDP, with the region's output alone representing 72% of local economic activity. Such activities employ tens of thousands and spur ancillary industries, though they require substantial water imports in water-scarce environments. Proven reserves data indicate relative stability amid ongoing extraction, as technological advances in seismic imaging, horizontal drilling, and enhanced recovery methods have expanded economically viable volumes; global oil reserves rose slightly to 1,567 billion barrels by end-2024 despite decades of production, reflecting discoveries and gains rather than imminent depletion. This counters narratives of rapid exhaustion by demonstrating how market prices and sustain recoverability, enabling prolonged economic contributions from desert basins without evidence of systemic shortages under current demand trajectories.

Agricultural Innovations and Challenges

Israel developed in the 1950s and 1960s through engineers like and , enabling precise delivery to crop roots in the arid Desert and achieving efficiencies of 90 percent compared to 40-50 percent for . This innovation reduced consumption by 50-70 percent relative to traditional methods, supporting the expansion of field crops, orchards, and greenhouses across the , where now constitutes a key economic sector despite annual rainfall below 250 mm. By 2022, irrigated 75 percent of Israel's crops, demonstrating scalability from smallholder to commercial operations in sandy, low-fertility soils. In , desalination capacity has scaled rapidly in the 2020s to support amid groundwater depletion, with the kingdom operating the world's largest plants and allocating over $80 billion for water projects through 2030. facilities, such as those under the National Water Strategy, aim to raise desalinated water's share in supply to 50 percent by 2030, enabling of staple crops like and dates in hyper-arid regions where natural aquifers yield . These efforts have revolutionized arid farming by blending desalinated output with treated , though energy demands—consuming 20 percent of domestic oil production—underscore trade-offs in dependency. Persistent challenges include salinization from over-irrigation and poor drainage, which accumulates sodium and reduces permeability, leading to yield declines of 20-50 percent in affected desert plots. Reversal strategies employ amendments, which supply calcium to displace sodium ions via , improving infiltration rates by up to 30 percent and aggregate stability in sodic soils; field trials in saline-alkali areas report crop yield increases of 15-25 percent when is applied at 5-10 tons per alongside . These interventions, grounded in chemistry principles, have restored productivity in regions like China's analogs to desert margins, though long-term monitoring reveals variable efficacy based on initial levels exceeding 4 dS/m. Emerging technologies like Liquid Natural Clay (LNC), a nanoclay suspension from Desert Control, have seen 2025 deployments in desert trials, binding sand particles to form water-retaining aggregates that cut needs by 50 percent and boost nutrient holding in permeable soils. Applied at rates of 1-3 liters per square meter, LNC stabilizes structure without , yielding midterm gains in biomass during University of Arizona tests, though scalability depends on cost reductions below $1 per square meter for widespread adoption in sandy expanses.

Energy Production and Infrastructure

Deserts offer exceptional potential for production due to their high solar insolation levels, often exceeding 2,500 kWh/m²/year in regions like the . This geographic advantage stems from clear skies, minimal cloud cover, and intense direct normal irradiance, enabling (CSP) and photovoltaic (PV) systems to achieve high yields compared to temperate zones. Major projects exemplify this: Morocco's Noor Ouarzazate complex, spanning CSP and PV technologies, reached a total capacity of 580 MW by 2018, supplying power to over a million homes while incorporating thermal storage for dispatchable output. Similarly, China's Tengger Desert Solar Park in the Tengger Desert has scaled to multi-gigawatt levels, leveraging vast arid expanses for utility-scale PV deployment. Wind energy complements solar in elevated or coastal desert areas with consistent gusts, such as the Gobi and Atacama, where benefit from low and steady flows. In China's Gobi region, wind farms have integrated with solar to form hybrid installations, with national plans targeting up to 450 GW combined capacity by expanding across desert terrains. These setups mitigate intermittency through diversification, though dust accumulation and extreme temperatures necessitate robust designs and periodic maintenance. Infrastructure development addresses key challenges like remote locations and grid integration via (HVDC) lines, which minimize transmission losses over hundreds of kilometers. For instance, the SunZia project in the U.S. Southwest employs HVDC to convey and solar from desert sources to urban demand centers, spanning over 500 miles with capacities exceeding 3,000 MW. Solutions for site-specific issues include elevated panel mounting to reduce sand abrasion and automated cleaning systems, enabling sustained efficiency despite . These advancements facilitate large-scale renewable export, though upfront costs for grid extensions remain a barrier in undeveloped desert grids.

Military and Strategic Applications

Deserts provide expansive, open terrain conducive to high-mobility , as demonstrated in the of (1940–1943), where Axis and Allied forces exploited vast desert spaces for outflanking operations and rapid armored advances. In these engagements, the lack of natural obstacles allowed tanks and mechanized units to cover hundreds of kilometers, emphasizing tactical flexibility over static defenses, though strains from long supply lines often determined outcomes. Remote desert isolation has made such regions ideal for nuclear weapons testing, with the Nevada National Security Site (formerly Nevada Test Site) hosting the first U.S. atmospheric detonation, Operation Able, on January 27, 1951, followed by 99 more above-ground tests through 1962 to minimize populated-area fallout risks while evaluating weapon yields. Over 900 total tests occurred there until 1992, leveraging the arid expanse to contain blast effects and monitor environmental dispersion. Strategically, deserts like the serve as critical chokepoints linking continents and controlling access to waterways such as the and , providing defensible depth for nations like during conflicts including the 1967 , where capture of the peninsula buffered eastern borders against invasion. Control of these barren corridors enables dominance over trade routes and military transit, historically amplifying geopolitical leverage despite harsh traversal conditions. In contemporary operations, deserts host major forward bases, such as in Qatar's arid interior, established in 1996 and serving as the largest U.S. military installation in the , accommodating over 10,000 personnel for CENTCOM air operations in conflicts like those in and . Military forces integrate with desert sands through specialized camouflage patterns, such as Arid, designed for arid concealment by blending tans, browns, and subtle contrasts to disrupt outlines against sandy backdrops and reduce detection in open terrains.

Environmental Dynamics and Controversies

Desertification: Causes and Debates

refers to in arid, semi-arid, and dry sub-humid areas resulting from various factors, including climatic variations and human activities, as defined by the Convention to Combat (UNCCD) in its 1994 text. This definition, rooted in the 1977 Conference on , emphasizes persistent reduction in biological productivity but has faced criticism for its vagueness, often conflating temporary degradation with irreversible desert formation, which complicates empirical assessment and policy application. Critics note that the term's ambiguity allows inclusion of reversible processes driven by short-term , obscuring distinct causal mechanisms. Primary human-induced causes include overgrazing, which compacts soil and diminishes vegetative cover, and deforestation for fuelwood, reducing infiltration and accelerating erosion in marginal lands. These activities exacerbate vulnerability but interact with natural variability, such as interannual rainfall fluctuations, which empirical data show as dominant drivers of vegetation loss in drylands. Long-term aridity shifts, influenced by Milankovitch orbital cycles—variations in Earth's eccentricity, obliquity, and precession—have historically expanded deserts like the Sahara during low-insolation phases, demonstrating that climatic forcing precedes and modulates human impacts over millennia. In contemporary contexts, studies attribute much observed degradation to rainfall deficits rather than solely anthropogenic pressure, with recovery evident upon precipitation rebound. The Sahel region exemplifies reversible degradation, where severe droughts from the 1970s to 1980s reduced vegetation, but satellite-derived Normalized Difference Vegetation Index (NDVI) data reveal widespread greening since the mid-1980s, correlating strongly with a 20-30% rainfall increase rather than land management alone. This trend, with NDVI rising at rates up to 0.0006 per year in rainy seasons, challenges claims of irreversible loss, as biomass rebounds without permanent soil desertization. Debates persist over NDVI's utility for measuring desertification, as trends often mirror precipitation variability more than degradation, with positive signals in many arid zones confounding narratives of unchecked advance; limitations include sensitivity to seasonal rains and inability to distinguish transient from structural change. Misguided policies stemming from overstated anthropogenic dominance have yielded failures, such as top-down ignoring hydrological limits, which diverts resources from adaptive rotations proven effective in recovery scenarios. Empirical prioritization of variability-driven interventions over alarmist frameworks could mitigate harms like inefficient allocation, as seen in stalled UNCCD initiatives where vague metrics hinder targeted action.

Greening Phenomena and Recovery Evidence

Satellite observations since the 1980s reveal widespread in global , with a significant portion—estimated at 25 to 50 percent of Earth's vegetated lands—exhibiting increased foliage cover primarily due to CO2 fertilization effects that enhance and plant water efficiency in arid conditions. This phenomenon correlates with rising atmospheric CO2 concentrations, which studies attribute as a dominant driver for vegetation gains across 61.4 percent of analyzed global areas showing NDVI trends from 1982 to 2015. Historical evidence from paleoclimate records demonstrates recurrent greening of the Desert during North African Humid Periods, driven by Earth's orbital cycles occurring approximately every 21,000 years, which amplify summer solar insolation and strengthen inflows to support savanna-like ecosystems. The most recent such interval, peaking around 11,000 to 5,000 years ago, transformed arid expanses into vegetated landscapes capable of sustaining lakes, rivers, and human settlements before reverting to desert conditions as waned. In contemporary settings, human interventions have accelerated localized recoveries, as seen in the where farmer-managed natural regeneration— involving pruning of native tree stumps on farmlands—has expanded tree cover across roughly 5 to 7 million hectares in since the 1980s, boosting and soil stability without extensive planting. Similarly, the has greened by 38 percent in vegetation indices from 2001 to 2023, propelled by a 64 percent uptick in rainfall combined with pumping for , though this has raised concerns over depletion. China's exemplifies technology and policy-driven reversal, where the Grain for Green Program, launched in 1999, restored over 35,000 square kilometers of eroded terrain by 2009 through terracing, , and livestock controls, yielding measurable NDVI gains and reduced sediment runoff into the . These efforts underscore causal roles of targeted in countering , distinct from natural climatic oscillations.

Climate Change Interactions

Observations of desert extent in the late 20th and early 21st centuries reveal mixed responses to climatic shifts, with some regions expanding while others exhibit greening. The Desert expanded by approximately 8% between 1950 and 2015, based on analyses of climate indices and vegetation data. This growth has been attributed in part to shifts in sea surface temperatures and atmospheric circulation patterns, including weakening of the African Easterly Jet. Concurrently, elevated atmospheric CO2 concentrations have driven widespread greening in globally, enhancing plant water-use efficiency and reducing , which allows to thrive under limited . Satellite observations indicate an 11% increase in foliage cover across arid regions from the 1980s to the 2010s, primarily due to this rather than precipitation changes alone. Projections from climate models introduce further nuance, forecasting potential increases in over the 's interior under continued warming, contrasting with narratives of uniform . A 2025 study using high-resolution simulations predicts up to 75% more rainfall in parts of the by 2100 compared to historical averages, driven by intensified monsoon dynamics and shifts in the . However, model ensembles vary, with some indicating drying at the desert peripheries due to altered moisture transport, highlighting uncertainties in regional responses. Short-term signals in desert extent are often dominated by natural variability, such as decadal oscillations in ocean-atmosphere systems, which can mask or amplify anthropogenic influences. Proxy records from paleoclimate archives, including lake sediments and aeolian deposits, demonstrate that desert boundaries like the have fluctuated significantly on millennial timescales without industrial-era forcings, as during the mid-Holocene "Green " period when orbital changes and strengthening expanded savannas across . These findings underscore that internal variability has historically driven expansions and contractions, challenging attributions of recent changes solely to human-induced gases as emphasized in IPCC assessments. Analyses attributing desert shifts primarily to anthropogenic forcing may underweight such natural modes, as evidenced by correlations with pre-industrial sea surface temperature patterns.

Extraterrestrial Deserts

Martian Surface Features

The Martian surface exhibits extensive arid terrains dominated by , with vast s mantled in fine basaltic dust particles, expansive fields of sand dunes sculpted by prevailing s, and polar caps that store the planet's primary surface volatiles amid pervasive desiccation. Orbital observations from the Mars Odyssey spacecraft have mapped these dust-covered regions globally, revealing chemical compositions dominated by iron oxides and silicates that contribute to the reddish hue and loose susceptible to mobilization. Syrtis Major Planum stands out as a prominent low-dust basaltic , where has stripped away fine particles to expose darker volcanic , spanning approximately 1,500 km in length and highlighting regional variations in dust accumulation. Dune fields are particularly prominent in the impact basin, the largest such structure on Mars at over 2,300 km in diameter, where and transverse dunes align with multidirectional wind patterns inferred from imagery and atmospheric modeling. These features migrate at rates of up to several meters per Mars year, driven by seasonal slope winds and basin circulation, with dune crest orientations indicating dominant northerly and northwesterly flows along the western rim. Rover anemometers, such as the REMS instrument on , have recorded surface wind speeds exceeding 30 m/s (108 km/h) during dust-lifting events, sufficient to entrain particles and sustain active bedform evolution despite the thin atmosphere. The polar ice caps, situated at latitudes above 70°, comprise perennial water ice layers up to 3 km thick underlying seasonal CO₂ frost, functioning as hyper-arid reserves in a planet where surface temperatures average -60°C and atmospheric pressure permits no stable liquid water. These caps, spanning over 1,000 km across during minima, experience sublimation-driven mass loss during summer, contributing to global dust storm initiation, yet preserve ancient stratified deposits revealing episodic volatile deposition over billions of years. In equatorial regions, the Perseverance rover's investigations since its February 2021 landing in Jezero Crater have identified sedimentary outcrops of ancient fluvial deltas and lakebed strata, dated to the Noachian-Hesperian transition around 3.5–3.8 billion years ago via stratigraphic correlation, underscoring a shift from water-influenced deposition to enduring aridity marked by wind-eroded yardangs and ventifacts.

Deserts on Other Celestial Bodies

Saturn's largest moon, Titan, hosts expansive dune fields resembling terrestrial deserts but composed of solid organic hydrocarbons derived from in its nitrogen-methane atmosphere. Cassini mission observations from 2004 to 2017 mapped these longitudinal dunes, which span thousands of kilometers and reach heights of up to 150 meters, covering at least 13% of the surface and formed by wind-driven transport of particles measuring 100-300 micrometers. The dunes' orientation aligns with from Titan's seasonal methane cycle, with minimal liquid due to sparse hydrocarbon precipitation. Jupiter's moon Io features sulfur-dominated plains akin to volcanic deserts, continuously resurfaced by over 400 active volcanoes ejecting silicate lavas and sulfur compounds. Its thin sulfur dioxide atmosphere enables limited sublimation but no significant fluid flow, resulting in colorful, barren expanses of sulfur frost and basalt flows covering most of the 3,640 km diameter surface. Galileo and Voyager data from the 1970s-1990s, supplemented by Hubble observations, reveal dune-like ridges formed not by wind but by electrostatic levitation of sulfur particles or subsurface lava flows, with tidal heating from Jupiter driving resurfacing rates of up to 1 km³ per year. Mercury's surface is characterized by regolith-blanketed craters and plains, exhibiting desert-like aridity from its negligible —composed primarily of , , and trace oxygen at densities below 10⁴ particles per cm³—precluding atmospheric or retention of volatiles. orbiter data from 2011-2015 mapped smooth northern plains covering 6% of the surface, formed by effusive around 3.5 billion years ago and preserved by micrometeorite gardening without wind or redistribution. Extreme temperature swings from -173°C to 427°C further inhibit surface modification, yielding vast, unchanging expanses of silicate . The Moon's maria represent basaltic flood plains functioning as ancient volcanic deserts, filling impact basins with iron- and titanium-rich lavas that solidified 3-4 billion years ago to form flat, low-albedo terrains covering 16-17% of the near-side surface. Apollo samples and spectroscopy confirm compositions of 40-50% SiO₂ with minimal volatiles, lacking atmosphere for weathering and modified solely by impacts and sputtering. These "seas," misidentified by early telescopic observers, exhibit layers up to 10-20 meters thick, analogous to desert pavements in their resistance to further alteration. James Webb Space Telescope observations since 2023 have identified arid conditions on rocky via transmission spectroscopy, revealing silicate-dominated atmospheres lacking on worlds like LHS 3844 b, a 1.3 Earth-radius with surface temperatures exceeding 1000 K and no evidence of hydration. For TOI-561 b, a lava-covered 50 light-years away, 2023-2024 NIRSpec data detected a possible thin atmosphere of rock vapor but confirmed dry, refractory compositions without oceanic or hydrated features, supporting models of persistent from stellar proximity and volatile loss. These findings, cross-verified with Spitzer archives, indicate causal parallels to solar system deserts through inefficient volatile retention and high insolation.

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