Waw an Namus (also spelled Wau-en-Namus, Arabic: واو الناموس) is a volcano in Libya. Of either Pleistocene or Holocene age, it is located within the eastern Fezzan region. The origin of the volcanism there and at Al Haruj farther north is not clear. Radiometric dating has yielded an age of about 200,000 years, but other circumstantial evidence points to a formation of the volcano during Holocene or even historical times. Waw an Namus is characterized by a caldera surrounded by an apron of dark tephra, which has a notable colour contrast to the surrounding desert terrain of the Sahara. A smaller crater lies northwest of the Waw an Namus caldera. The caldera itself contains a scoria cone. Several small lakes and associated vegetation are located within the caldera.
Name The volcano is also known as Uaw en Namus, Uau en Namus, Wau-en-Namus and Wau Sqair. It means "Oasis of mosquitoes", a reference to the small lakes around it and the numerous mosquitoes that exist at Waw an Namus, nurtured by the lakes at the volcano.
Geography and geomorphology The volcano lies within the Sahara, in the eastern Fezzan and was discovered by scientists a few decades before 1951. The caravan route between Kufra and Sebha passes by the volcano. Ancient graves have been found at Waw an Namus. While the oasis was probably visited by herders and hunters and may have been the source of raw materials, the place is otherwise uninhabited. The landscape around Waw an Namus has been described as "very beautiful" and is reportedly a tourism target but logistical issues and the Libyan Civil War make it difficult to access the area. Waw an Namus is a 100-metre-deep (330 ft), 4-kilometre-wide (2.5 mi) caldera, which has a small relief outwards but a steep margin inwards. During its formation, over 800,000,000 cubic metres (2.8×1010 cu ft) of rock were displaced. Another crater lies 5 kilometres (3.1 mi) northwest from Waw an Namus. That vent was formed by overlapping craters which feature no volcanic rocks and which have produced salty mud; this may have been a site of phreatic activity and of volcanic degassing. The caldera contains ash deposits and some dunes, but also a humid zone with reeds. Within the caldera lies a 140-metre-high (460 ft), 1.3-kilometre-wide (0.81 mi) scoria cone constructed out of phreatomagmatic material with an 80-metre-deep (260 ft), 150-metre-wide (490 ft) crater. Another crater, now reduced to remnants, is located west of the summit crater of the cone. The cone has been modified by gullies. Dark-coloured tephra of basaltic composition has buried the desert sand around the caldera to distances of 10–20 kilometres (6.2–12.4 mi), resulting in a conspicuous colour contrast to the much brighter desert sand. This contrast can be noted even on spaceborne images. The tephra deposit consists of volcanic ash and lapilli and covers a surface of about 300 square kilometres (120 sq mi). 2–150-centimetre-high (0.79–59.06 in) waves are formed by the tephra, which in its western part is baked together by mudflows. The tephra deposit is stratified, implying that it was generated by more than one eruption. Trade winds have blown the tephra over 100 kilometres (62 mi) southwestward, and a large number of megaripples formed by volcanic material occur both inside and outside of the caldera.
Lakes Also within the caldera are three small lakes and additional smaller water bodies, which together form a semicircle around the northern, eastern and southern flanks of the central cone. One of the lakes is north of the scoria cone, the second southeast and south and the third southwest. These lakes cover a total surface of 0.3 square kilometres (0.12 sq mi) and the largest lake has a surface area of 0.146 square kilometres (0.056 sq mi) with a depth of 12.5 metres (41 ft), while the deepest of these waterbodies reaches depths of 15–16 metres (49–52 ft). The water surface reaches 434 metres (1,424 ft) elevation above sea level, although seasonal variations sometimes cause the lakebodies to dry up. These lakes, some of which have red colours, give Waw an Namus a multicoloured appearance. The lakes are probably groundwater-fed, as evaporation in the area greatly exceeds precipitation, with the lakes losing about 1,500,000 cubic metres (53,000,000 cu ft) water per year. Freshwater springs nourish the lakes. At least one water body was reported to be fresh in 1951 while the others are warm and saline. Deuterium isotope ratio analysis indicates that the water at Waw an Namus is recent water, certainly more recent than 8,000 years.
Geology Waw an Namus is an isolated volcano. About 70 kilometres (43 mi) north lie lava flows of basaltic composition and the Haruj volcanic field, of which Waw an Namus is sometimes considered to be a part. These in turn are only two out of several large but little known volcanic fields in the Sahara. A number of theories have been proposed to explain the volcanism in the Sahara, such as the activation of ancient crustal lineaments by the collision between Africa and Europe; in the case of Waw an Namus the magmas originated in the mantle at about 130 kilometres (81 mi) depth, and include both asthenosphere and lithosphere components that underwent metasomatism before melting. The processes at Haruj and Waw an Namus were probably different. The terrain surrounding Waw an Namus is covered by Quaternary sediments. The basement beneath the volcano is crystalline, and is in turn covered by limestone, marl and the Nubian Sandstone.
Alkali basalts have been identified in the scoria, and the occurrence of foidite has been reported. Minerals contained within these rocks include apatite, clinopyroxene, magnetite, nepheline and olivine, and occasionally melilite and sodalite. The rocks contain xenoliths of harzburgite, lherzolite and peridotite. Sulfur occurs within the crater of the scoria cone, as well as white deposits that may be formed by alunite.
Climate Waw an Namus is part of the Sahara desert, one of the world's largest and driest deserts although parts of it were wetter in the past. In some parts of the Sahara it has only rained a few times during a whole century; at Waw an Namus the little precipitation mostly occurs during winter. Wind is the most important weather factor, forming ventifacts and dunes among other structures; at Waw an Namus it mostly blows from the northeast and is sometimes accompanied by dust devils south of the volcano.
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