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128 STRUCTURE



                                       Nile                 N                    Nile
                0        250 km
                                               Lake                                      Lake
                                 Lake          Kyoga                       Lake
                                Albert                                    Albert         Kyoga

                           Lake                           Congo       Lake
                           Edward                                    Edward
                Congo
                                                                 Virunga
                      Drainage                                  Mountains
                      from Lake
                     Tanganyika                                           Lake
                                                                          Kivu
                                                Lake               Rusizi                 Lake
                                               Victoria            River                 Victoria






                                                                 Lukuga R.
                                        Lake                                       Lake
                                      Tanganyika                                Tanganyika
                                                          b
                a
               ()                                         ()
              Figure 5.10 Drainage diversion by volcanoes in central Africa. (a) The Nile drainage through the Western Rift before the
              eruptions that built the Virunga Mountains. (b) The Nile drainage after the formation of the Virunga Mountains.
              Source: Adapted from Francis (1993, 366)



              2 km in sedimentary rocks and 4 km in crystalline  features, or a combination of the two (Figure 5.12).
              rocks do not have a simple bowl shape. Rather, they  This is a small total compared with the number iden-
              are complex structures that, in comparison with simple  tified on planets retaining portions of their earliest crust.
              structures, are rather shallow (Figure 5.11b). The most  However, impact structures are likely to be scarce on
              recent examples, such as Clearwater Lakes in Quebec,  the Earth owing to the relative youthfulness and the
              Canada, typically have three distinct form facets. First  dynamic nature of the terrestrial geosphere. Both factors
              a structurally uplifted central area, displaying shock-  serve to obscure and remove the impact record by ero-
              metamorphic effects in the autochthonous target rocks,  sion and sedimentation. Craters would have originally
              that may be exposed as a central peak or rings; second,  marked sites of all impacts. Owing to erosion, older
              an annular depression, partially filled by autochthonous  sites are now obscure, all that remains being signs of
              breccia, or an annular sheet of so-called impact melt  shock metamorphism in the rocks. Thus, impacts will
              rocks, or a mixture of the two; and, third, a faulted  always leave a very long-lasting, though not indelible,
              rim area.                                 signature in rocks, but the landforms (craters) they pro-
                Impact craters occur on all continents. As of 2 Novem-  duce will gradually fade, like the face of the Cheshire
              ber 2004, 172 had been identified as impact craters from  cat. The current list of known impact structures is cer-
              the presence of meteorite fragments, shock metamorphic  tainly incomplete, for researchers discover about five
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