2
Correspondence Testing the Neoproterozoic glacial models The interval of time immediately preceding the Ediacaran Period (N 635 Ma to 800 Ma) is punctuated by extreme glaciations that appear to extend to low latitudes (Hoffman et al., 1998a; Evans, 2000). Two main models have been forwarded to explain these glaciations. Williams and Schmidt (2004) call on a drastic change in the Earth's obliquity in order to elucidate these low latitude glaciations. Hoffman et al. (1998a) called upon a complete freezing of the Earth dubbed Snowball Earth. The high obliquity model is testable. First, the distribution glacial rocks should be constrained to latitudes less than 45° (Evans, 2000). Secondly, the deposition of latitudinally dependent facies (evaporites, redbeds) should show a spatial distribution consistent with the model. At present, no reliable high latitude paleomagnetic poles have been obtained from Neoproterozoic glacial facies and therefore the high obliquity model cannot be rejected on this basis. In his analysis on 2.5 billion years worth of evaporite facies, Evans (2006) found them to be restricted to latitudes between 10°35°. Because a high obliquity earth would shift evaporite facies equator-ward, the analysis of Evans (2006) falsifies the high obliquity model. The snowball earth model is also falsifiable. These tests can be broken down into two groupsconceptual models and ground truth. Models may examine mechanisms for plunging the earth into a snowball state (e.g. Schrag et al., 2002; Donnadieu et al., 2004), coming out of the snowball state (Hoffman et al., 1998b) or the extent of the glaciations (Hyde et al., 2000). Paleomagnetic tests of the snowball earth are a bit trickier since, in principle, any paleolatitude would fit the snowball earth model. Hoffman et al. (1998a) claim that the initial stages of cap carbonate deposition will be extremely rapid (20 m in only 50 years), thus paleomagnetic directions in cap carbonates should exhibit little secular variation and no reversals (Trindade et al., 2003). The problem with testing the conceptual models of the snowball earth hypothesis is that any failures can be accommodated in a new model. The snowball earth hypothesis implies that the glaciations should be synchronous events. Hoffman et al. (1998a,b) explain that synchroneity is demonstrated by the variation in stable isotopes ( 13 C) before, during and after the glacial events. Knoll (2000) and Halvorsen et al. (2005) argued that the 13 C signal is a robust and near instantaneous recorder of seawater chemistry and therefore useful as a relative geochronometer. The necessary absolute age controls on isotopic curves/glacial Gondwana Research 11 (2007) 573 574 www.elsevier.com/locate/gr Fig. 1. 13 C curve modified from Halvorsen et al. (2005). The dashed lines follow the centerline of the highest density of observations. The ages along the top of the curve along with the extent and length of glaciations follows Halvorsen et al. (2005). The lighter dashed lines represent the 13 C curves for the light-grey lined epochs (Sturtian and Marinoan A). The darker dashed line shows the time-shifted 13 C curve for the second estimate of the glacial episodes (Sturtian and Marinoan B). The 13 C curves are identical for the pre 790 Ma and post 636 Ma periods. The outliergeochronologic ages are listed along the base of the graph. The Trezona and Wonoka negative 13 C anomalies are thought to mark the onset of the Marinoan and Gaskiers glacial epochs respectively. 1342-937X/$ - see front matter © 2006 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved. doi:10.1016/j.gr.2006.11.002

Testing the Neoproterozoic glacial models

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Page 1: Testing the Neoproterozoic glacial models

Gondwana Research 11 (2007) 573–574www.elsevier.com/locate/gr

Correspondence

Testing the Neoproterozoic glacial models

The interval of time immediately preceding the EdiacaranPeriod (N635 Ma to ∼800 Ma) is punctuated by extremeglaciations that appear to extend to low latitudes (Hoffman et al.,1998a; Evans, 2000). Two main models have been forwarded toexplain these glaciations. Williams and Schmidt (2004) call on adrastic change in the Earth's obliquity in order to elucidate theselow latitude glaciations. Hoffman et al. (1998a) called upon acomplete freezing of the Earth dubbed “Snowball Earth”.

The high obliquity model is testable. First, the distributionglacial rocks should be constrained to latitudes less than ∼45°(Evans, 2000). Secondly, the deposition of latitudinallydependent facies (evaporites, redbeds) should show a spatialdistribution consistent with the model.

At present, no reliable high latitude paleomagnetic poleshave been obtained from Neoproterozoic glacial facies andtherefore the high obliquity model cannot be rejected on thisbasis. In his analysis on 2.5 billion years worth of evaporitefacies, Evans (2006) found them to be restricted to latitudesbetween 10°–35°. Because a high obliquity earth would shiftevaporite facies equator-ward, the analysis of Evans (2006)falsifies the high obliquity model.

Fig. 1. 13C curve modified from Halvorsen et al. (2005). The dashed lines follow thecurve along with the extent and length of glaciations follows Halvorsen et al. (2005).(Sturtian and Marinoan A). The darker dashed line shows the time-shifted 13C curve fcurves are identical for the pre ∼790 Ma and post 636 Ma periods. The ‘outlier’ geocnegative 13C anomalies are thought to mark the onset of the Marinoan and Gaskiers

1342-937X/$ - see front matter © 2006 International Association for Gondwana Rdoi:10.1016/j.gr.2006.11.002

The snowball earth model is also falsifiable. These tests canbe broken down into two groups— conceptual models andground truth. Models may examine mechanisms for plungingthe earth into a snowball state (e.g. Schrag et al., 2002;Donnadieu et al., 2004), coming out of the snowball state(Hoffman et al., 1998b) or the extent of the glaciations (Hydeet al., 2000). Paleomagnetic tests of the snowball earth are a bittrickier since, in principle, any paleolatitude would fit thesnowball earth model. Hoffman et al. (1998a) claim that theinitial stages of cap carbonate deposition will be extremely rapid(20 m in only 50 years), thus paleomagnetic directions in capcarbonates should exhibit little secular variation and noreversals (Trindade et al., 2003). The problem with testing theconceptual models of the snowball earth hypothesis is that anyfailures can be accommodated in a new model.

The snowball earth hypothesis implies that the glaciationsshould be synchronous events. Hoffman et al. (1998a,b) explainthat synchroneity is demonstrated by the variation in stableisotopes (13C) before, during and after the glacial events. Knoll(2000) and Halvorsen et al. (2005) argued that the 13C signal isa robust and near instantaneous recorder of seawater chemistryand therefore useful as a relative geochronometer. Thenecessary absolute age controls on isotopic curves/glacial

centerline of the highest density of observations. The ages along the top of theThe lighter dashed lines represent the 13C curves for the light-grey lined epochsor the second estimate of the glacial episodes (Sturtian and Marinoan B). The 13Chronologic ages are listed along the base of the graph. The Trezona and Wonokaglacial epochs respectively.

esearch. Published by Elsevier B.V. All rights reserved.

Page 2: Testing the Neoproterozoic glacial models

574 Correspondence

deposits have yet to be resolved in most cases. If the 13C curvesand the glacial events can be independently correlated withprecise geochronometry, then one of the major criticismsagainst the Snowball hypothesis can be eliminated.

The number of absolute age determinations on theNeoproterozoic glacial deposits has recently increased. Halvor-sen et al. (2005) used many of these ages to develop a global13C curve for the Neoproterozoic glaciations. The growth of thegeochronologic database resulted in questions regarding thenumber and synchroneity of the glacial events. Fig. 1 shows theglobal 13C curve proposed by Halvorsen et al. (2005).Halvorsen et al. (2005) used geochronologic data to definethe limits of the three main glaciations (Sturtian, Marinoan andGaskiers). They suggest that the Sturtian glaciations occurredbetween 700–746 Ma and give two possible ranges for theMarinoan, both ending at 636 Ma. The Gaskiers is thought to bea non-global glaciation that took place ∼580 Ma.

Recent geochronologic data illustrate the difficulties in using13C trends in global correlation. Lund et al. (2003) report an age of∼685 Ma for the Edwardsburg Formation (Idaho) placing theSturtian glaciation∼15Ma younger than shown in Fig. 1. Kendallet al. (2006) report a 657±5 Ma Re–Os age from the AralkaFormation (∼7–9 m above the Areyonga diamictite, Australia)and 643±2.4 Ma from the Tindelpina Formation (Australia).These Re–Os ages are supported by recent 658 Ma U–Pb agesfrom the Merinjina Formation (Australia, Fanning, 2006). Theseages imply that the archetypal ‘Sturtian’ glaciations are eitherdiachronous, have been miscorrelated or that there are more short-lived glacial epochs (Kendall et al., 2006; Fanning, 2006).

The ‘Snowball Earth’ hypothesis assumes that globalglaciations in the Neoproterozoic are represented by synchro-nous and distinct episodes. Correlations between these eventsare based primarily upon features in the 13C record. Theassumption that the features of the 13C curves are distinctenough to allow correlation in the absence of absolute ages ischallenged by a growing geochronologic database. Futuregeochronologic work on these critical sequences may resolvethe current conundrum and alternative explanations for theseenigmatic glaciations should be considered (e.g. Leather et al.,2002; Eyles and Januszczak, 2004).

References

Donnadieu, Y., Goddéris, Y., Ramstein, G., Nédélec, A., Meert, J., 2004. A‘snowball Earth’ climate triggered by continental break-up through changesin run-off. Nature 428, 303–306.

Eyles, N., Januszczak, N., 2004. ‘‘Zipper-rift’’: a tectonic model forNeoproterozoic glaciations during the breakup of Rodinia after 750 Ma.Earth-Science Reviews 65, 1–73.

Evans, D.A.D., 2000. Stratigraphic, geochronological and paleomagnetic con-straints upon the Neoproterozoic glacial paradox. American Journal ofScience 300, 347–433.

Evans, D.A.D., 2006. Proterozoic low orbital obliquity and axial dipolar geo-magnetic field from evaporite paleolatitudes. Nature 444, 51–55.

Fanning, M.C., 2006. Constraints on the timing of the Sturtian glaciation fromsouthern Australia; i.e. for the true Sturtian. Geological Society of AmericaAbstracts with Programs 38 (7), 115.

Halvorsen, G.P., Hoffman, P.F., Schrag, D.P., Maloof, A.C, Rice, A.H.N., 2005.Towards a Neoproterozoic composite carbon isotope record. GeologicalSociety of America Bulletin 117, 1181–1207.

Hoffman, P.F., Kaufman, A.J., Halverson, G.P., Schrag, D.P., 1998a. ANeoproterozoic snowball Earth. Science 281, 1342–1346.

Hoffman, P.F., Kaufman, A.J., Halverson, G.P., 1998b. Comings and goings ofglobal glaciations on a Neoproterozoic tropical platform in Namibia. GSAToday 8 (5), 1–9.

Hyde, W.T., Crowley, T.J., Baum, S.K., Peltier, W.R., 2000. Neoproterozoic‘‘snowball Earth’’ simulations with a coupled climate/ice-sheet model.Nature 405, 425–429.

Kendall, B., Creaser, R.A., Selby, D., 2006. Re–Os geochronology ofpostglacial black shales in Australia: constraints on the timing of ‘‘Sturtian’’glaciation. Geology 34, 729–732.

Knoll, A.H., 2000. Learning to tell Neoproterozoic time. Precambrian Research100, 3–20.

Leather, J., Allen, P.A., Brasier, M.D., Cozzi, A., 2002. Neoproterozoicsnowball Earth under scrutiny: evidence from the Fiq glaciation of Oman.Geology 30, 891–894.

Lund, K., Aleinikoff, J.N., Evans, K.V., Fanning, C.M., 2003. SHRIMP U–Pb geochronology of Neoproterozoic Windermere Supergroup, centralIdaho: implications for rifting of western Laurentia and synchroneity ofSturtian glacial deposits. Geological Society of America Bulletin 115,349–372.

Schrag, D.P., Berner, R.A., Hoffman, P.F., Halverson, G.P., 2002. On theinitiation of a snowball Earth. Geochemistry, Geophysics and Geosystems,3. doi:10.1029/2001GC000219.

Trindade, R.I.F., Font, E., D'Agrella-Filho,M.S., Nogueira, A.C.R., Riccomini, C.,2003. Low-latitude and multiple geomagnetic reversals in the NeoproterozoicPuga cap carbonate, Amazon craton. Terra Nova 15, 441–446.

Williams, G.E., Schmidt, P.W., 2004. Neoproterozoic glaciation: reconcilinglow paleolatitudes and the geologic record. In: Jenkins, G.S., et al. (Ed.),The Extreme Proterozoic: Geology, Geochemistry, and Climate. AmericanGeophysical Union Geophysical Monograph, vol. 146, pp. 145–159.

Joseph G. MeertDepartment of Geological Sciences,

241 Williamson Hall, Gainesville, FL 32611 USAE-mail address: [email protected].

Tel.: +1 352 846 2414; fax: +1 352 392 9294.

6 November 2006