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Brugia Malayi - Clark Science Center - Smith College

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Distribution and Origin of Caliche Crusts in Ancient Sand Dunes on San<br />

Salvador Island, Bahamas<br />

Sarah Brisson<br />

In January I conducted geological fieldwork on San Salvador to examine unusual features of eolian dune deposits formed by<br />

sedimentation and lithification of wind-blown carbonate sand. This summer I carried out petrographic and stable isotope analyses<br />

of collected samples. I described and photographed my samples, then cut them and made thin sections for examination under a<br />

petrographic microscope. Using a microscope-mounted drill I collected powder for stable isotope (oxygen and carbon) analysis. I<br />

will be presenting my results at the Annual Meeting of the Geological Society of America in Charlotte, NC this fall.<br />

My research focused on numerous thin caliche crusts present in eolianites of the upper North Point Member of the Rice Bay<br />

Formation exposed along the northeastern coast of San Salvador. These eolianites formed during Holocene sea-level rise about 6<br />

to 5 ka and consist of complexly stratified deposits produced by wind-ripple migration, grainfall and sandflow processes. 1 Such<br />

caliche crusts are not present in the lower part of these Holocene deposits or in the older Pleistocene eolianites. I examined the<br />

distribution and composition of caliche and compared them with Pleistocene deposits to better understand the formation of these<br />

unique features.<br />

Caliche is a hard microcrystalline crust formed by dissolution and subsequent reprecipitation of carbonate. In the upper<br />

part of the exposure caliche coats all prominent bedding planes, including dune crests, gently sloping windward sides, and steep<br />

(up to 34°) leeward surfaces. In weathered exposures caliche also forms a step-like pattern of up to twelve crusts, 1-4 mm thick,<br />

separating 3-32 cm thick eolian beds that thin upsection. Most of these crusts are parallel to lamination and vary in orientation<br />

from horizontal to 18°. Others encrust cross-laminated beds and vertical fractures forming caliche dikes. Caliche crusts have a<br />

sharp, smooth upper surface with varying degrees of weathering which impart a pitted, irregular appearance. In most cases caliche<br />

crusts are associated with dense, laterally extensive rhizoliths that form by carbonate precipitation around plant roots.<br />

Multiple caliche horizons represent coeval precipitation as penetrative caliche. 2 Plant roots penetrated through the eolianite,<br />

then spread laterally along firmly lithified laminae in search of water and nutrients. The presence of water and plant material<br />

facilitated caliche formation and produced a unique stratification pattern with numerous thin crusts delineating distinct beds<br />

of mainly wind-ripple laminated strata. This distinguishes the Holocene deposits from their Pleistocene counterparts, which<br />

commonly have thicker eolian strata separated by more varied and better-developed ancient soil horizons. Stable isotope analysis<br />

also demonstrated important differences in the composition of caliche and host eolian sediment from these strata. These<br />

differences reflect varying climatic and environmental conditions as well as differing duration and styles of eolian sedimentation<br />

and post-depositional modifications in the Pleistocene versus the Holocene in the Bahamas. (Supported by the Schultz<br />

Foundation)<br />

Advisor: Bosiljka Glumac<br />

References:<br />

1<br />

White, B. and H.A. Curran. 1988. Mesoscale physical sedimentary structures and trace fossils in Holocene carbonate eolianites from San Salvador Island, Bahamas.<br />

Sedimentary Geology, 555: 168-184.<br />

2<br />

Rossinsky Jr., V., H.R. Wanless and P.K. Swart. 1992. Penetrative calcretes and their stratigraphic implications. Geology, 20: 331-334.<br />

2012<br />

130

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