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PRECAMBRIAN TECTONICS AND THE SUPERCONTINENT CYCLE  373




                                                       South
                                                       China
                              Seychelles  India            Proto-Pacific Ocean  30°N
                                                                       North
                            Madagascar     Australia                   China


                                   Kalahari           Laurentia   Baltica

                                          East
                                        Antarctica                           Siberia
                                                   Rio
                                                   Plata
                                                      Amazonia    Avalonian    30°S
                              Congo                                        Timanian
                                       Brazilide
                                       Ocean
                                                 West
                                                 Africa        Cadomian        60°S

                                             1.3–1.0 Ga Grenville orogenic belts
                                             Cratons with paleomagnetic data ( 750 Ma)


            Fig. 11.20  Reconstruction of Rodinia at ∼750 Ma (after Torsvik, 2003, with permission from Science 300, 1379–81, with
            permission from the AAAS).






            Donnadieu et al., 2004). During break-up, the changing   11.5.4 Earlier supercontinents
            paleogeography of the continents may have led to an
            increase in runoff, and hence consumption of CO 2 ,
            through continental weathering that decreased atmo-  The origin of the fi rst supercontinent and when it may
            spheric CO 2  concentrations (Section 13.1.3). The extreme   have formed are highly speculative. Bleeker (2003)
            glacial conditions may have ended when volcanic out-  observed that there are about 35 Archean cratons today
            gassing of CO 2  produced a suffi ciently large greenhouse   (Plate 11.1a between pp. 244 and 245) and that most
            effect to melt the ice. The resulting “hothouse” would   display rifted margins, indicating that they fragmented
            have enhanced precipitation and weathering, giving rise   from larger landmasses. Several possible scenarios have
            to the deposition of carbonates on top of the glacial   been envisioned for the global distribution of the
            deposits during sea-level (Hoffman et al., 1998). Alterna-  cratons during the transition from Late Archean to
            tively, these transitions may have resulted mainly from   Early Proterozoic times (Fig. 11.21). These possibilities
            the changing configuration of continental fragments   include a single supercontinent, called Kenorland by Wil-

            and its effect on oceanic circulation (Sections 13.1.2,   liams et al. (1991) after an orogenic event in the Cana-
            13.1.3). Whichever view is correct, these interpretations   dian Superior Province, and the presence of either a few
            suggest that the break-up of Rodinia triggered large   or many independent aggregations called supercratons.
            changes in global climate. However, the origin, extent,   Bleeker (2003) concluded that the degree of geologic
            and termination of the Late Proterozoic glaciations, and   similarity among the exposed cratons favors the pres-
            their possible relationship to the supercontinental break-  ence of several transient, more or less independent
            up, remains an unresolved and highly contentious issue   supercratons rather than a single supercontinent or
            (Kennedy et al., 2001; Poulsen et al., 2001).  many small dispersed landmasses. He defi ned  a
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