2007 GSA Denver Annual Meeting (28–31 October 2007)

Paper No. 5
Presentation Time: 2:45 PM

IS THERE A SECULAR CHANGE IN OXYGEN ISOTOPE COMPOSITION OF CRUSTAL FLUIDS TRACKING THAT OF SEAWATER?


MUEHLENBACHS, Karlis, Earth and Atmospheric Sciences, University of Alberta, 1-26 ESB, Edmonton, AB T6G 2E3, FURNES, Harald, Centre for Geobiology & Department of Earth Science, University of Bergen, Allegate 41, Bergen, 5007, Norway, DE WIT, Maarten, AEON-Africa Earth Observatory Network, and Department of, University of Cape Town, Rondebosch, 7700, South Africa, ROSING, Minik, Nordic Centre for Earth Evolution (NordCEE) & Geological Museum, University of Copenhagen, Copenhagen, 1350, Denmark and STAUDIGEL, Hubert, Scripps Insitution of Oceanography, Univ of California, UCSD-0225, La Jolla, CA 9209309 0225, karlis.muehlenbachs@ualberta.ca

The δ18O of seawater directly or indirectly sets the starting composition of almost all crustal fluids, with the possible exception of magmatic fluids. If δ18O of seawater changed over geological time, so all crustal fluids and their subsequent rock or brine products would exhibit a secular change in δ18O. Most fossil brachiopods and sediments do show a secular trend of decreasing δ18O, which some explain as reflecting an ever lower δ18O ocean. However, the δ18O ophiolites and ore deposits do not change indicating a constant δ18O of seawater. The secular trend in sediments can be explained if the temperature of the oceans were higher. A 40 year controversy has continued on this point but has recently reignited as a result of the recent suggestion that the Archean oceans were very hot, a conclusion incompatible with some models of atmosphere and seawater compositions. Critics of a hot Archean invoke moderate temperatures but a very low δ18O ocean (-13 ppt SMOW) as the explanation for the low δ18O Archean cherts. A -13 ‰ ocean would impose a clear signal on any product of rock alteration by the hydrosphere, with much lower values in higher alteration temperature products. The recently discovered sheeted dike complex at Isua, Greenland provides insights into the 3.8 Ga ocean and may finally resolve the long standing controversy the δ18O of ancient oceans. The Isua dikes range in δ18O from 5.7 to 6.9 ppt giving no evidence of a low, but rather a slightly enriched 18O seawater at 3.8 Ga. The data from Isua as well as previous studies on 18O-enriched pillows from Pilbara (3.5 Ga.), Barberton (3.5 Ga) and Kid Creek (2.7 Ga) show that the suggestion of a very low δ18O, early ocean is untenable. We can conclude from the oxygen isotope analyses of the pillows and dykes that the earliest ocean had already reacted with the sea floor. This has great implications to the composition of the oceans themselves because seawater/seafloor rock reactions are known to massively affect if not control the chemical make up of seawater.