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Tidewater glacier beds: insights from iceberg debris in Kongsfjorden, Svalbard

Published online by Cambridge University Press:  08 September 2017

Neil F. Glasser
Affiliation:
Centre for Glaciology, Institute of Geography and Earth Sciences, University of Wales, Aberystwyth SY23 3DB, Ceredigion, Wales
Michael J. Hambrey
Affiliation:
Centre for Glaciology, Institute of Geography and Earth Sciences, University of Wales, Aberystwyth SY23 3DB, Ceredigion, Wales
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Abstract

The sediment in icebergs offers an opportunity to sample the otherwise inaccessible beds of modern tidewater glaciers. This paper presents a discussion of the benefits and problems of using iceberg debris to make inferences about the nature of the beds of modern tidewater glaciers. As an example, we present data obtained from icebergs calved from fast-flowing tidewater glaciers in Kongsfjorden, Svalbard. Sediment samples obtained from 12 icebergs show that clast-rich muddy diamicton is the dominant facies, although muddy gravel and mud are also present in some debris layers. Sediment texture and clast-shape analyses indicate that most debris in the icebergs is of basal origin. Micro-morphological analyses of thin sections of the diamicton also indicate pervasive deformation of the sediment. Although individual icebergs only represent small samples of the bed of a tidewater glacier, and problems remain in linking iceberg sediments to their precalving transport history beneath the glacier, this method provides a potentially fruitful way of linking sediments to glacier dynamics.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2001
Figure 0

Fig. 1. Location map of Kongsfjorden, showing major tidewater glacier termini and the position of the icebergs sampled. Simplified bedrockgeology in the catchments of the glaciers is taken from Hjelle (1993). The Proterozoic rocks consist of schist, psammite and marble; the Devonian rocks are sandstone and siltstone; and the Carboniferous and Permian rocks consist of sandstones, limestone and chert.

Figure 1

Fig. 2. (a) Photograph of debris in iceberg KF06 in Kongsfjorden, showing debris melting out of the iceberg and streaking the surface below. The tidewater front of Kronebreen can be seen in the background. (b) Close-up of debris in iceberg KF02. Note the sharp contact between the coarse clear ice (left) and the debris layer (right). The debris layer is about 0. 4 m thick.

Figure 2

Table 1. Principal characteristics of the icebergs and associated debris in Kongsfjorden. Clast lithologies are based on samples of 50 clasts: C chert; CL, cherty limestone; SP, schist/psammite; L, limestone; SA, sandstone; VQ vein quartz; Q quartz; SI, siltstone; MG, microgranite; G, gneiss; MA, marble; O, others

Figure 3

Fig. 3. Covariant plots of the RA index (% of angular and very angular clasts) against the C40 index (% of clasts with c/a axial ratio ≤0.4) for clast-shape data obtained from debris-rich icebergs in Kongsfjorden. Each symbol represents a sample of 50 clasts. The subglacial, supraglacial and glaciofluvial facies envelopes are from Bennett and others (1997). The moraine-complex envelope contains 44 samples of clasts in diamicton emplaced on land by the 1948 surge of the Kongsvegen/Krone-breen tidewater glacier (Bennett and others, 1999).

Figure 4

Fig. 4. Iceberg KF07 displaying the nature of part of the bed beneath Kronebreen. (a) Close-up of the iceberg showing slick-ensides and grooves on the base of the diamicton. (b) The diamicton and its texture, showing dispersed clasts and brecciation.

Figure 5

Fig 5. Histograms showing particle-size data for the 11 debris-rich icebergs sampled in this study. Intervals are in half Samples KF01–KF11 are diamicton, whilst KF12 is mud.

Figure 6

Table 2. Clast-shape data (in%) for samples of 50 clasts from each of the debris-rich icebergs (VA, very angular; A, angular; SA, subangular; SR, subrounded; R, rounded; WR, well rounded)

Figure 7

Fig. 6. Microstructures observed in thin sections of diamicton from iceberg KF07, interpreted as representing the presence of a deformable bed. Photomicrographs are taken from the flow-parallel section, and both images show a field of view measuring 16 mm across. (a) Galaxy structure, comprising silt grains arranged around a small pebble (cross-polarized light). (b) Fractured clast, centre left of photograph (normal light).