Genesis of active sand-filled polygons in lower and central Beacon Valley, Antarctica

Nonsorted polygons with sand-filled wedges were investigated in Beacon Valley, Antarctica (77.82°S, 160.67°E) using field observations coupled with 2-m resolution aerial photography. A gasoline-powered concrete breaker was employed to expose the sediments of four polygon centres and six wedges from...

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Bibliographic Details
Published in:Permafrost and Periglacial Processes
Main Authors: Bockheim, James G., Kurz, Mark D., Soule, S. Adam, Burke, Andrea
Format: Article in Journal/Newspaper
Language:English
Published: 2009
Subjects:
Ice
Online Access:https://risweb.st-andrews.ac.uk/portal/en/researchoutput/genesis-of-active-sandfilled-polygons-in-lower-and-central-beacon-valley-antarctica(41ecd500-a57f-447f-bbfc-0ae85b40402f).html
https://doi.org/10.1002/ppp.661
http://onlinelibrary.wiley.com/doi/10.1002/ppp.661/abstract
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Summary:Nonsorted polygons with sand-filled wedges were investigated in Beacon Valley, Antarctica (77.82°S, 160.67°E) using field observations coupled with 2-m resolution aerial photography. A gasoline-powered concrete breaker was employed to expose the sediments of four polygon centres and six wedges from geomorphic surfaces containing tills of two different ages. The excavated polygons ranged from 9 to 16 m in diameter; the sand-filled wedges ranged from 0.2 to 2.5 m in width. The top of ice-bonded permafrost ranged from 12 to 62 cm in depth in the polygon centres and from 64 to >90 cm in wedges. One active thermal-contraction fissure generally was apparent at the surface, but excavations revealed numerous inactive fissures. The wedges contain sand laminations averaging 3 mm in width when viewed in cross-section. Although most of the polygons were of the sand-wedge type, some contained ice veins up to 1 cm in width and could be classed as composite wedges. Three stages of polygon development were observed, including well-developed polygons on Taylor II surfaces (ca. 117 ka), moderately developed polygons on Taylor III surfaces (ca. 200 ka) and poorly expressed polygons on Taylor IVa and older (ca. >1.1 Ma) surfaces. This retrogressive development may be due to sublimation of ice-bonded permafrost following thermal cracking. With the drop in ice content, the thermal coefficient of expansion of the permafrost may be lowered, which would result in a reduction in tensile stresses.