Paper No. 9
Presentation Time: 10:00 AM
STRATIGRAPHIC TESTS FOR THE ORIGIN OF THE DEEPEST CARBON-ISOTOPE ANOMALY IN EARTH HISTORY - THE WONOKA FORMATION OF SOUTH AUSTRALIA
The deepest carbon isotope excursion in Earth history is recorded in Ediacaran carbonates from Oman, South Australia, south China, southern Siberia, southwest USA, Namibia and Scotland. Called the ‘Shuram’ excursion, two end member hypotheses seek to explain the observed trend. The first interprets the carbonate isotopes as a primary seawater signal, and postulates the existence of a large, relict DOC pool (much larger than today) based upon remarkably invariant δ13Corg during the δ13Ccarb excursion. Remineralization of this pool during the Ediacaran would push global DIC to very low δ13C values. The second holds that the isotopic signal is not primary, but rather is a diagenetic overprint. The depleted δ13C values and observed covariation between δ13C and δ18O might have resulted from migrating, high pCO2 fluids that interacted with the sediments during burial diagenesis at elevated temperatures. The second hypothesis is of critical importance, as δ13C has become the backbone for the correlation of pre-fossil stratigraphy. In order to test these hypotheses, we present a program of integrated mapping, physical stratigraphy, and paired δ13Ccarb - δ18Ocarb - δ13Corg analyses of the Wonoka Formation of South Australia. The Wonoka outcrops over 100s of kilometers, enabling us to map the carbon isotopic profiles in a range of paleodepositional environments - from stormy open shelf and microbialite reef to deep submarine canyon. We are thus able to assess the relationship between δ13C and sedimentary environment, geographic location, and primary porosity. We find covariation between δ13C and δ18O only in the lower part of the Wonoka. Furthermore, at some localities, the base of the Wonoka is marked by deep (>1km) paleocanyons; a possible relationship between canyon formation, local sea level change and the Shuram excursion has never been explored. We find that the Wonoka was a prograding carbonate ramp that cut into itself (and recycled itself into the canyon fill) towards the end of its deposition, and that canyon formation postdated the nadir of the Shuram excursion. As canyon incision occurred during Wonoka deposition, this observation requires that the morphology of the deep negative δ13C excursion was acquired early, and must have preceded any significant heating or burial diagenesis.