Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published September 2012 | public
Journal Article

Origin of giant wave ripples in snowball Earth cap carbonate

Abstract

The most extreme climate transitions in Earth history are recorded by the juxtaposition of Neoproterozoic glacial deposits with overlying cap carbonate beds. Some of the most remarkable sedimentary structures within these beds are sharp-crested (trochoidal) bedforms with regular spacing of as much as several meters that are often interpreted as giant wave ripples formed under extreme wave conditions in a nonuniform postglacial climate. Here we evaluate this hypothesis using a new bedform stability diagram for symmetric oscillatory flows that indicates that the first-order control on the formation of trochoidal rather than hummocky bedforms is sediment size, not wave climate. New measurements of bedform wavelengths and particle sizes from the ca. 635 Ma Nuccaleena Formation, Australia, indicate that the giant ripples are generally composed of coarse to very coarse sand; most are within the trochoidal bedform stability phase space for normal wave climates. Moreover, numerical simulations of flow over fixed bedforms show that symmetric trochoidal ripples with a nearly vertical angle of climb may be produced over long time periods with variable wave climates in conjunction with rapid seabed cementation. These data reveal that, rather than extreme wave conditions, the giant wave ripples are a consequence of the unusual mode of carbonate precipitation during a global carbon cycle perturbation unprecedented in Earth history.

Additional Information

© 2012 Geological Society of America. Manuscript received 6 December 2011; Revised manuscript received 26 March 2012; Manuscript accepted 2 April 2012. First published online July 23, 2012. Lamb acknowledges support from the donors of the American Chemical Society Petroleum Research Fund. Fischer acknowledges support from the Agouron Institute. Raub was supported by National Science Foundation grant EAR-0739105. We thank Tony Prave, John Southard, and Paul Hoffman for informal reviews and delightful discussions. David Mohrig and Bob Dalrymple provided formal reviews that strengthened the final manuscript.

Additional details

Created:
August 22, 2023
Modified:
October 19, 2023