Distinguishing base-level change and climate signals in a Cretaceous alluvial sequence

  1. T. White1,
  2. B. Witzke2,
  3. G. Ludvigson2 and
  4. R. Brenner3
  1. 1Earth and Environmental Systems Institute, Pennsylvania State University, University Park, Pennsylvania 16802, USA
  2. 2Iowa Geological Survey, Iowa City, Iowa 52242, USA
  3. 3Geoscience Department, University of Iowa, Iowa City, Iowa 52240, USA

Abstract

We present the results of oxygen isotope and electron-microprobe analyses of sphaerosiderites obtained from Cretaceous paleosols in Iowa. The sphaerosiderite δ18O values record Cretaceous meteoric groundwater chemistry and an overall waning of brackish groundwater inundation during alluvial-plain aggradation and soil genesis. We focus on horizons that precipitated from freshwater, in which δ18O values ranging from −3.3‰ to −6.8‰ relative to the Peedee belemnite standard are interpreted to record variations in the Cretaceous atmospheric hydrologic cycle. During relative sea-level highstands, moisture was derived from the Cretaceous Western Interior Seaway, whereas during lowstands, when the seaway narrowed and occasionally withdrew from the Midcontinent, the dominance of hemispheric-scale atmospheric moisture transport initiated in the tropical Tethys Ocean led to decreased precipitation rates. These processes did not operate like a switch, but rather as a continuum of competing moisture sources and mechanisms of transport between the nearby epicontinental sea and the distant tropics. The sphaerosiderite data demonstrate (1) temporal variation in the intensity of hemispheric-scale atmospheric moisture transport and (2) long-term amplification of the global hydrologic cycle marked by extreme 18O depletion at the Albian-Cenomanian boundary.

    • Received 14 July 2004.
    • Accepted 1 October 2004.
    • Revision received 27 September 2004.
« Previous | Next Article »Table of Contents