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Emi Koussi

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High pyroclastic shield volcano in the Sahara

Emi Koussi
Emi Koussi seen from space
Highest point
Elevation3,447 m (11,309 ft)
Prominence2,934 m (9,626 ft)
Ranked 104th
ListingCountry high point
Ultra
Ribu
Coordinates19°47′33″N18°32′47″E / 19.79250°N 18.54639°E /19.79250; 18.54639[1]
Geography
Emi Koussi is located in Chad
Emi Koussi
Emi Koussi
Location in Chad
LocationChad
Parent rangeTibesti Mountains
Geology
Rock ageHolocene
Mountain typePyroclastic shield
Last eruptionunknown
Climbing
Easiest routeHike

Emi Koussi (also known as Emi Koussou[2]) is a highpyroclastic shield[3]volcano that lies at the southeast end of theTibesti Mountains in the centralSahara, in the northernBorkou Region of northernChad. The highest mountain of the Sahara, the volcano is one of several in the Tibesti range, and reaches an elevation of 3,447 metres (11,309 ft), rising 3 km (1.9 mi) above the surroundingsandstone plains. The volcano is 60–70 kilometres (37–43 mi) wide and has a volume of 2,500 cubic kilometres (600 cu mi).

Two nestedcalderas cap the volcano, the outer one being about 15 by 11 kilometres (9.3 mi × 6.8 mi) in size. Within it on the southeast side is a smaller caldera known as Era Kohor, about 2 kilometres (1.2 mi) wide and 350 metres (1,150 ft) deep. Numerouslava domes,cinder cones,maars, andlava flows are found within the calderas and along the outer flanks of the shield. Era Kohor containstrona deposits, and Emi Koussi has been studied as an analogue of theMartian volcanoElysium Mons. Emi Koussi was active more than one million years ago, but some eruptions may be more recent, and there is ongoingfumarolic andhot spring activity.

Geography and geomorphology

[edit]

Emi Koussi lies inChad,Africa, and is part of theTibesti Mountains[4] as well as its highest peak[5] and thus of the Sahara;[6] many peaks of the Tibesti exceed 2,000 metres (6,600 ft) in height.[5] These mountains are formed by a group of volcanoes that grew on top of a largedome of Earth's surface.[7] Volcanism in this area is poorly studied; as the region is remote and access difficult for political reasons.[8]Dirt roads cross the western and eastern margins of the summit caldera,[9] and according to historical reports theTibu people lived in its summit caldera[10] and in artificial caves.[11] In theTedaga language,Emi means "mountains", "massif".[6] The mountain has played an important role in the research and discovery history of the Tibesti.[12]

Emi Koussi rises to a height of 3,415 metres (11,204 ft) on the southern side of the volcano,[13][14] rising between <1 kilometre (0.62 mi)[15] and 3 kilometres (1.9 mi) above the surrounding terrain[16] and forming the highest summit of the Sahara.[17] It is considered by some astronauts to be the most recognizable landmark on Earth, as seen fromorbit.[16] Supposedly the entire Tibesti can be seen from the northern summits.[18]

Topographic map of the Emi Koussi

It is ashield volcano with a diameter of 60–70 kilometres (37–43 mi)[16] or 60–80 kilometres (37–50 mi)[12] and an estimated volume of 150 cubic kilometres (36 cu mi)[15]-2,500 cubic kilometres (600 cu mi).[19] The summit of Emi Koussi is formed by two overlappingcalderas, which together form a[20] 15-by-11-kilometre (9.3 mi × 6.8 mi) wide[16] elliptical caldera that extends from northwest to southeast.[20] The northern caldera formed first, then the southern caldera which is about 50 metres (160 ft) deeper below the northern one. 400–300-metre (1,310–980 ft) highscarps form the inner margin of the southern caldera,[21] with the floor at an elevation of 2,970 metres (9,740 ft).[22] Before the formation of the calderas, the volcano may have reached a height of 4,000 metres (13,000 ft). Emi Koussi has been compared to aMartian volcano,Elysium Mons.[5][23] The caldera rim is cut by oneoutlet, the Porte deModiounga,[24] from whichgorges emanate into the caldera.[25] The highest point of Emi Koussi lies on the southern rim of the caldera.[9]

Nested within this combined caldera is the Era Kohor caldera,[20] which is 300 metres (980 ft) deep and 2 kilometres (1.2 mi) wide, having the appearance of a giant hole.[21] This caldera is also known asNatron Hole[18] or Trou au Natron.[13]Trachytic lava flows are exposed in its walls,[21] andsodium carbonate has been deposited on its floor,[26] which lies at an elevation of 2,670 metres (8,760 ft)[22] and contains a salt lake.[11] The floor of Era Kohor is thus deep white.[24] Threemaars and severalscoria cones are also nested within the combined caldera,[21] along withlava domes andlava flows.[3] Debris fromexplosive eruptions fills the calderas.[27]

The Kohorpumices and two sets ofignimbrites cover the flanks of Emi Koussi,[20] which steepen as they approach the summit.[23] Scoria cones on the slopes are accompanied bylava flows.[20] On the upper sectors of the volcano, lavas are crisscrossed by cracks, which are known as "lappiaz".[28]Sandstone crops out on the terrain surrounding the volcano.[20] North of Emi Koussi lie other volcanoes, such asTarso Ahon andTarso Emi Chi,[29] the former of which is connected to Emi Koussi by a narrow ridge.[13]

Geology

[edit]

Tectonic activity appears to have occurred in the Tibesti already between theCarboniferous and theCretaceous,[5] that is between 358.9 ± 0.4 and 66 million years ago.[30] During the earliest stage of volcanism on Tibesti,alkali basalts formed large plateaus. Later, the central volcanoes developed on top of these plateaus.[16] Volcanism in Tibesti has been explained with amantle plume, as has been proposed for other African volcanoes,[31] although recently tectonic effects of the collision between Africa and Europe and their effects at a distance have also been advanced as an explanation.[32]

The oldest rocks below the Tibesti arePrecambriandiorites,granites andschists,[29] which are probably ofNeoproterozoic age and are differentiated into two units.[32] The volcanic rocks rest on an uplifted basement formed by Cretaceous[5] andPaleozoic sandstone.[16] The latter crop out at the southwestern foot of Emi Koussi, while volcanic rocks dominate north of the volcano, and the Tibesti massif is prevalent east and southeast of Emi Koussi.[29] Older volcanic rocks are exposed in valleys.[33]

Emi Koussi has eruptedphonolite,trachyandesite and trachyte,[16] as well asmafic rocks likebasanite andtephrite. The erupted rocks define two alkaline suites.Phenocryst chemistry and content varies between the various rocks; among the minerals are alkalifeldspar,amphibole,biotite,clinopyroxene,olivine, oxides andplagioclase. Alkali feldspar,apatite, clinopyroxene, olivine,magnetite,mica,nepheline, oxides, plagioclase,quartz,sodalite,titanite andzircon also form thegroundmass ofmicroliths in erupted rocks.[34]Magma genesis mainly involvedfractional crystallization processes.[31] Rocks from Emi Koussi were used asraw material byNeolithic societies of the region.[35]

Until 5,400 years ago[36] during theAfrican humid period (Holocene), Era Kohor was filled with a 4.1 square kilometres (1.6 sq mi) lake whose water reached a depth of 130 metres (430 ft)[17] and a volume of 0.45 cubic kilometres (0.11 cu mi).[36] It was fed in part by water accumulating in the outer caldera and percolating to Era Kohor.[37]Diatom beds have been found 125 metres (410 ft) above the floor of Era Kohor[38] and in depressions without outlet elsewhere in the caldera,[39] they reach thicknesses of 4–5 metres (13–16 ft).[40] Farther down on the mountain, gullies start appearing at 2,800 metres (9,200 ft) elevation and become deepgorges by 2,000–2,500 metres (6,600–8,200 ft) elevation.[19] Elleboewadi originates on Emi Koussi,[41] and several streams on the western flank join into the Enneri Miski which drains southwards and disappears south of the mountains.[42] Small pools of water are found around Emi Koussi.[43]

Eruptive history

[edit]
Emi Koussi caldera,ASTER

Emi Koussi erupted between 2.4 and 1.3 million years ago;[44] it is considered to be ofPliocene-Quaternary age.[45] The volcano was constructed mainly during theMiocene[19][46] within about one million years.[47]Radiometric dating has yielded ages of 2.42 ± 0.03 - 2.33 ± 0.09 million years ago for the oldest Emi Koussi stage. The third stage has yielded ages of 1.4 ± 0.3 - 1.32 ± 0.2 million years ago;[16][48] formerly Era Kohor was considered to be a Holocene centre.[26]

During the first stage, Emi Koussi erupted trachytes and trachyandesites in the form of ignimbrites andbasalticlapilli. This was followed in the second stage by trachytic, green or grey ignimbrites, trachytic and phonolitic lava domes and additional basaltic lava flows.[16] The second stage ignimbrites can be found within the northern caldera and on the southern flank of the volcano.[21] The third stage was dominantly phonolitic, withbreccia,tuffs and ignimbrites including the Kohor ignimbrite.[16] The various ignimbrites containfiamme and often look like lava flows.[49] Each stage was accompanied by the formation of a caldera,[21] and basaltic volcanism continued through all three stages.[16]Phreatic explosions associated with Era Kohor have deposited large blocks within the summit caldera,[21] including beautifully colouredsyenite blocks.[50]

Quaternary volcanism gave rise to the cones on the slopes of Emi Koussi,[20] and the three maars are the most recent vents in the combined caldera,[21] while long lava flows have been interpreted to be the youngest volcanism at Emi Koussi.[51] The most recent volcanic vents show little erosion.[50] Early in thePleistocene,erosion took place on the flanks of Emi Koussi,[5] andcarbonates were deposited in Era Kohor until recent times.[52][53]

On the southern foot of the volcano,fumaroles are active[5] such as at Yi Yerra at 850 metres (2,790 ft) elevation on the southern flanks.[27] At Yi Yerra,hot springs produce water with temperatures of 37 °C (99 °F).[54] Emi Koussi is considered to be a Holocene volcano.[52] Lava flows have buried Holocene diatoms beds in its caldera;[11] dates of 14,790 ± 400 - 12,400 ± 400 yearsbefore present have been obtained byradiocarbon dating on diatom beds which have been penetrated or buried by lava flows.[55]

Climate and vegetation

[edit]

The Tibesti mountains feature a desert mountain climate. There are no weather stations close to Emi Koussi and the stations at lower elevations likely underestimate precipitation at higher elevations,[42] but based oncloud cover data, a yearly precipitation of 80–120 millimetres (3.1–4.7 in) has been estimated for Emi Koussi.[56] Precipitation was higher in the past,it[14] when theAfrican monsoon expanded over the Sahara[17] and drew moisture from theMediterranean Sea to the Tibesti,[57] The climate reflects both northerly and southerly influences and is distinct from that of the surrounding deserts.[55] There is no evidence ofnivation forms on Emi Koussi[58] and the identification ofperiglacial landforms is questionable,[55] although periglacial activity likely occurred in the Pleistocene and may continue to the present-day.[54] Even during the Pleistocene, no part of the mountain had sub-freezing temperatures through the entire year.[59]

A number of diatom species have been identified in sediments left by the Era Kohor lake, includingCocconeis placentula,Cyclotella cyclopuncta,Cyclotella ocellata,Cymbella cistula,Cymbella leptoceros,Cymbella muelleri,Epithemia adnata,Fragilaria construens,Fragilaria pinnata,Gomphonema affine,Gomphonema parvulum,Navicula oblonga andRhopalodia gibba.[60] The diatom fauna appears to be unusual in comparison to other Saharan paleolakes, probably owing to the high elevation of the Emi Koussi lake.[61]Cattail andwater milfoil grew around the lake.[38]

Generally, in the Tibesti vegetation occurs in five different belts depending on elevation.[62] On Emi Koussi,Erica arborea is found up to elevations of 2,900 metres (9,500 ft),[63] in the past it was probably more widespread.[64] The summit region featuresmontane vegetation,[65] includingArtemisia-Ephedrasteppes[66] which cover large parts of the caldera floor.[50] The lava flows high on the mountain have characteristic environmental traits which allow the development of a particular vegetation.[28][67] This vegetation encompassesDichrocephala,Eragrostis,Erodium,Helichrysum as well asferns,liverworts andmosses.[66]Oldenlandia andSelaginella species grow at fumaroles.[68] The caldera floor was used as a pasture forcamels andgoats.[25]

Thewood rushLuzula tibestica isendemic on Emi Koussi.[65] The fernAsplenium quezelii was discovered on Emi Koussi and at first thought to be endemic there[69] before it was found to be identical toAsplenium daghestanicum, a species also previously considered to be endemic toDagestan, more than 3,800 kilometres (2,400 mi) away from Emi Koussi.[70]

Gallery

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  • Another view of it from space
    Another view of it from space
  • Calderas of Emi Koussi
    Calderas of Emi Koussi
  • Emi Koussi inner crater
    Emi Koussi inner crater
  • Natron in the inner caldera of Emi Koussi
    Natron in the inner caldera of Emi Koussi
  • Emi Koussi seen from Apollo 7 in October 1968
    Emi Koussi seen fromApollo 7 in October 1968

See also

[edit]

References

[edit]
  1. ^"Emi Koussi".Peakbagger.com. Retrieved2021-02-12.
  2. ^Hellmich 1972, p. 10.
  3. ^ab"Emi Koussi".Global Volcanism Program.Smithsonian Institution. Retrieved3 November 2013.
  4. ^Gourgaud & Vincent 2004, p. 261.
  5. ^abcdefgMalin 1977, p. 908.
  6. ^abPachur & Altmann 2006, p. 88.
  7. ^Gourgaud & Vincent 2004, p. 262.
  8. ^Permenter & Oppenheimer 2007, p. 609.
  9. ^abJäkel et al. 1972, p. 118.
  10. ^Peel, R. F. (1942). "The Tibu Peoples and the Libyan Desert".The Geographical Journal.100 (2):73–87.doi:10.2307/1789494.JSTOR 1789494.
  11. ^abcPachur & Altmann 2006, p. 103.
  12. ^abJäkel et al. 1972, p. 117.
  13. ^abcGèze et al. 1959, p. 137.
  14. ^abMesserli & Winiger 1992, p. 327.
  15. ^abKarátson, Dávid; Thouret, Jean-Claude (2025). "Chapter 6 Calderas and Caldera Complexes".Volcano Geomorphology: 344.doi:10.1007/978-3-031-77693-9_7.
  16. ^abcdefghijkGourgaud & Vincent 2004, p. 264.
  17. ^abcHoelzmann et al. 2025, p. 1.
  18. ^abTilho 1920, p. 172.
  19. ^abcHellmich 1972, p. 21.
  20. ^abcdefgGourgaud & Vincent 2004, p. 263.
  21. ^abcdefghGourgaud & Vincent 2004, p. 267.
  22. ^abZimmermann, M. (1919). "Chronique Géographique".Annales de Géographie.28 (155):387–400.JSTOR 23439749.
  23. ^abPermenter & Oppenheimer 2007, p. 621.
  24. ^abHellmich 1972, p. 172.
  25. ^abJäkel et al. 1972, p. 119.
  26. ^abMalin 1977, p. 909.
  27. ^abGèze et al. 1959, p. 139.
  28. ^abPoli 1974, p. 225.
  29. ^abcPermenter & Oppenheimer 2007, p. 616.
  30. ^"International Chronostratigraphic Chart"(PDF). International Commission on Stratigraphy. August 2018. Archived fromthe original(PDF) on 31 July 2018. Retrieved4 December 2018.
  31. ^abGourgaud & Vincent 2004, p. 288.
  32. ^abDeniel et al. 2015, p. 3.
  33. ^Gèze et al. 1959, p. 138.
  34. ^Gourgaud & Vincent 2004, pp. 268–269.
  35. ^Smith, Andrew (2001). "Saharo-Sudanese Neolithic".Encyclopedia of Prehistory Volume 1: Africa. Springer, Boston, MA. p. 245.doi:10.1007/978-1-4615-1193-9_19.ISBN 9781468471281.
  36. ^abHoelzmann et al. 2025, p. 4.
  37. ^Hoelzmann et al. 2025, p. 6.
  38. ^abHoelzmann, Philipp (2016-01-01)."Crater palaeolakes in the Tibesti mountains (Central Sahara, North Chad) – New insights into past Saharan climates".ResearchGate. EGU2016.
  39. ^Hellmich 1972, p. 56.
  40. ^Pachur & Altmann 2006, p. 119.
  41. ^Tilho 1920, p. 171.
  42. ^abDumont 1987, p. 135.
  43. ^Dumont 1987, p. 141.
  44. ^Gourgaud & Vincent 2004, p. 266.
  45. ^Gourgaud & Vincent 2004, p. 268.
  46. ^Bruneau de Miré & Quézel 1959, p. 135.
  47. ^Deniel et al. 2015, p. 17.
  48. ^Deniel et al. 2015, p. 18.
  49. ^Deniel et al. 2015, p. 8.
  50. ^abcHellmich 1972, p. 22.
  51. ^Oppenheimer, C. (1997). "Surveillance and Mapping of Volcanoes and their Emissions by Satellite Remote Sensing".Geography.82 (4):317–333.JSTOR 40572950.
  52. ^abPermenter & Oppenheimer 2007, p. 619.
  53. ^Gèze et al. 1959, p. 165.
  54. ^abDumont 1987, p. 134.
  55. ^abc"Hochgebirgsforschung: Tibesti - Zentrale Sahara, Arbeiten aus der Hochgebirgsregion".Zeitschrift für Gletscherkunde und Glazialgeologie.8. 1972.
  56. ^Messerli 1973, p. 146.
  57. ^Hoelzmann et al. 2025, p. 5.
  58. ^Messerli 1973, p. 141.
  59. ^Messerli & Winiger 1992, p. 317.
  60. ^Pachur & Altmann 2006, p. 137.
  61. ^Pachur & Altmann 2006, p. 120.
  62. ^Lézine et al. 2011, p. 1353.
  63. ^Messerli 1973, p. 142.
  64. ^Lézine et al. 2011, p. 1354.
  65. ^abRomo, A.; Boratyński, A. (30 December 2011)."La sección Atlanticae del género Luzula (Juncaceae)".Collectanea Botanica.30: 55.doi:10.3989/collectbot.2011.v30.005.hdl:10261/50024.ISSN 1989-1067.
  66. ^abPoli 1974, p. 226.
  67. ^Bruneau de Miré & Quézel 1959, p. 136.
  68. ^Schnell, R. (10 July 2014)."Réflexion sur les flores africaines".Bulletin de la Société Botanique de France. Actualités Botaniques (in French).136 (3–4): 116.doi:10.1080/01811789.1989.10826963.
  69. ^Viane 1987, p. 143.
  70. ^Viane 1987, p. 147.

Sources

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External links

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