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370   CHAPTER 11



           11.5 THE                                     the plate are re-projected using the same Eulerian rota-
                                                        tion. The continents are then successively shifted along

           SUPERCONTINENT                               fixed latitudes, that is, rotated about the magnetic pole,
                                                        until the overlap of continental margins is minimized.
                                                        Although the paleomagnetic data do not provide a
           CYCLE                                        unique sequence of reconstructions, they clearly indi-
                                                        cate the gross trends of plate movements during ancient
                                                        times. More detailed inferences on the evolution of
           11.5.1 Introduction                          particular regions are then made from their geology
                                                        viewed in terms of plate tectonic mechanisms.
           Geologic evidence for the repeated occurrence of con-  The application of paleomagnetic methods for the
           tinental collision and rifting since the Archean has led   Precambrian is less straightforward than for Phanero-
           to the hypothesis that the continents periodically   zoic times for three main reasons (Dunlop, 1981). First,
           coalesced into large landmasses called supercontinents.   the error limits of isotopic ages typically are larger.
           The best known of the supercontinents include Gond-  Second, isotopic and magnetic records may be partially
           wana (Fig. 3.4) and Pangea (Fig. 11.27), which formed   reset during metamorphism to different degrees, and
           in the latest Proterozoic and late Paleozoic times,   the distinction between pre- and post-orogenic isotopic

           respectively. Other supercontinents, such as Rodinia and   and magnetic overprints can be difficult. Third, over-
           Laurussia, also have been proposed for Late Proterozoic   prints occur during post-orogenic cooling and uplift,
           and late Paleozoic times, respectively. Processes in the   and the temperatures at which isotopic systems close
           mantle that may have led to their assembly and   and magnetizations stabilize are different, so that the
           dispersal are discussed in Section 12.11.    dates may be younger or older than the magnetizations
                                                        by intervals of tens of millions of years. However, even
                                                        given these uncertainties and the gaps in the paleomag-
           11.5.2 Pre-Mesozoic                          netic record arising from the lack of suitable samples of
                                                        certain ages, the data allow investigators to test the valid-
           reconstructions                              ity of paleogeographic reconstructions for pre-Mesozoic
                                                        times based on the geologic record on the continents.
           Paleogeographic maps for the Mesozoic and Cenozoic
           can be computed by the fitting together of continental

           margins or oceanic lineations of the same age on either   11.5.3  A Late Proterozoic
           side of an ocean ridge (Chapters 3, 4). The location of
           the paleopoles can be determined from paleomagnetic   supercontinent
           measurements (Section 3.6) and so the only unknown
           in these reconstructions is the zero meridian of longi-  Similarities between the Late Proterozoic geologic
           tude. These combined techniques cannot be used for   record in western Canada and eastern Australia (Bell &
           reconstructions prior to the Mesozoic because  in situ   Jefferson, 1987; Young, 1992) and between the south-
           oceanic crust is lacking.                    western USA and East Antarctica suggest that these
             Methods of quantifying plate motions in pre-  areas were juxtaposed during Late Proterozoic times
           Mesozoic times involve the use of paleomagnetic data   (Dalziel, 1991, 1995; Moores, 1991; Hoffman, 1991) (Fig.
           coupled with high-precision geochronology. Ancient   11.19a). This seemingly radical suggestion was referred
           plate edges, although somewhat distorted, are marked   to as the SWEAT (South West US and East AnTarctica)
           by orogenic belts and ophiolite assemblages (Sections   hypothesis. The widespread Grenville orogenic belts,
           2.5, 11.4.3), which indicate ancient sutures between   that immediately pre-date the Late Proterozoic, suggest
           welded continents and accreted terranes. Evidence pro-  that many other continental fragments can be added to

           vided from the past distributions of flora and fauna and   this reconstruction to form a Late Proterozoic super-
           indicators of paleoclimate also aid these plate recon-  continent called Rodinia (Fig. 11.19a). Laurentia (North
           structions (Sections 3.4, 3.5). For a particular time the   America and Greenland) forms the core of the

           paleomagnetic pole for each ancient plate is rotated to   supercontinent and is flanked to the north by East
           an arbitrary single magnetic pole and the continents on   Antarctica. The reconstruction shows that the North
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