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Stratigraphy and glaciotectonic structures of permafrost deformed beneath the northwest margin of the Laurentide ice sheet, Tuktoyaktuk Coastlands, Canada

Published online by Cambridge University Press:  08 September 2017

Julian B. Murton
Affiliation:
Department of Geography, University of Sussex, Brighton BN19QJ, England E-mail: j.b.murton@sussex.ac.uk
Richard I. Waller
Affiliation:
School of Earth Sciences and Geography, Keele University, Keele, Staffordshire ST5 5BG, England
Jane K. Hart
Affiliation:
School of Geography, University of Southampton, Highfield, Southampton SO17 1BJ, England
Colin A. Whiteman
Affiliation:
School of the Environment, University of Brighton, Brighton BN2 4GJ, England
Wayne H. Pollard
Affiliation:
Department of Geography, McGill University, 805 Sherbrooke Street West, Montreal, Quebec H3A 2K6, Canada
Ian D. Clark
Affiliation:
Department of Earth Sciences, University of Ottawa, 140 Louis Pasteur, Ottawa, Ontario K1N 6N5, Canada
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Abstract

The upper 20—30 m of ice-rich permafrost at three sites overridden by the northwest margin of the Laurentide ice sheet in the Tuktoyaktuk Coastlands, western Arctic Canada, comprise massive ice beneath ice-rich diamicton or sandy silt. The diamicton and silt contain (1) truncated ice blocks up to 15 m long, (2) sand lenses and layers, (3) ice veins dipping at 20—30°, (4) ice lenses adjacent and parallel to sedimentary contacts, and (5) ice wedges. The massive ice is interpreted as intrasedimental or buried basal glacier ice, and the diamicton and silt as glacitectonite that has never thawed. Deformation of frozen ground was mainly ductile in character. Deformation was accompanied by sub-marginal erosion of permafrost, which formed an angular unconformity along the top of the massive ice and supplied ice clasts and sand bodies to the overlying glacitectonite. After deformation and erosion ceased, postglacial segregated ice and ice- wedge ice developed within the deformed permafrost.

Type
Research Article
Copyright
Copyright © International Glaciological Society 2004

Introduction

An opportunity to examine glacier—bed interactions beneath cold-based ice is provided by field investigations of Pleistocene permafrost in formerly glaciated regions. Previous work in such regions has provided evidence for glacier-ice thrusting near the northwest limit of the Laurentide ice sheet (LIS) (Reference Mathews and MackayMathews and Mackay, 1960; Reference Mackay, Rampton and FylesMackay and others, 1972), and for a deformable bed of permafrost beneath the southern Kara ice sheet (Reference Astakhov, Kaplyanskaya and TarnogradskiyAstakhov and others, 1996). Observations of the stratigraphy and structural geology of near-surface, glacially deformed permafrost provide basic information about the rheology of sub-marginal permafrost, and thus are essential for modelling and reconstructing ice sheets with cold-based margins. Because recent numerical models suggest that subglacial permafrost was probably more extensive than previously assumed (Reference Cutler, MacAyeal, Mickelson, Parizek and ColganCutler and others, 2000), acquiring information about its former existence is of vital importance.

The aim of this paper is two-fold: (1) to examine the evidence for glacier—permafrost interactions beneath the northwest margin of the LIS, and (2) to infer the rheological conditions during sub-marginal deformation of permafrost. To this end, the paper describes the stratigraphy and glaciotectonic structures in the upper –5—20 m of permafrost at three sites in the Tuktoyaktuk Coastlands, western Arctic Canada (Fig. 1). The paper focuses on permafrost that is ice-rich, because glacially deformed ground ice within the stratigraphic sequences indicates that the ground has not thawed since the time of deformation.

Fig. 1. Location map of the Tuktoyaktuk Coastlands and Yukon Coastal Plain. Ice-flow directions and ice limits of the Toker Point Stade and Sitidgi Stade are according to Rampton (1988a).

Permafrost and Glacial History

The Tuktoyaktuk Coastlands form that part of the Arctic Coastal Plain between the Mackenzie Delta and Amundsen Gulf, Northwest Territories (Fig. 1; Reference Rampton and SennesetRampton, 1988a). They are in the zone of continuous permafrost, the maximum thickness of which is –750 m beneath northeast Richards Island (Reference Judge, Pelletier and NorquayJudge and others, 1987; Reference Taylor, Dallimore and JudgeTaylor and others, 1996).

Glacier ice of the northwest sector of the LIS overrode most of the Tuktoyaktuk Coastlands during the Toker Point Stade. The age of theToker Point Stade is disputed: an early- Wisconsin (>35 kyr BP) age has been inferred from regional Quaternary mapping (Fig. 1; Reference RamptonRampton, 1982,1988a; cf. Reference Vincent, Clark and LeaVincent, 1992), whereas a mid- or late-Wisconsin age has been suggested from studies of aeolian and glaciofluvial deposits (<35 kyr BP; Reference Dallimore, Wolfe, Matthews and VincentDallimore and others, 1997; Reference Murton, French and LamotheMurton and others, 1997). The ice flowlines and glacial limits reconstructed by Rampton (1982, 1988a) are shown in Figure 1. One major ice lobe flowed north-northwestward along the Mackenzie Valley, before fanning out northwest across the Yukon Coastal Plain and northeast across Richards Island and the southwest end of the Tuktoyaktuk Peninsula (Fig. 1). Another large ice lobe, in the vicinity of the Kugaluk and Anderson Rivers, flowed northward and then north-north eastward towards Nicholson Point. The interior of the Mackenzie Valley lobe is inferred to have been warm-based from the occurrence of eskers, drumlins, extensive spreads of ice-marginal glaciofluvial sediments and the reconstructed low glacier profile (Reference BegetBeget, 1987; Reference Rampton and SennesetRampton, 1988a). The western and eastern margins of these lobes have been placed by Rampton (1982, 1988a) near ice-thrust elevated ground at Herschel Island and at Nicholson Point, respectively (Fig. 1). Buried glacier ice from the LIS has been identified on Richards Island, Summer Island, Herschel Island and in the Eskimo Lakes Fingerlands (Fig. 1; Reference Dallimore, Wolfe and SennesetDallimore and Wolfe, 1988; Reference Rampton and SennesetRampton, 1988a; Reference French and HarryFrench and Harry, 1990; Reference PollardPollard, 1990; Murton and others, in press).

Permafrost existed in the Tuktoyaktuk Coastlands and the Yukon Coastal Plain prior to the last Laurentide glaciation. Its existence is inferred from glacially-folded and faulted icy layers reported by Reference Mackay, Rampton and FylesMackay and others (1972) at Herschel Island, Stokes Point, Kay Point, King Point, Garry Island, Pelly Island, Hooper Island, Kendall Island, Rae Island, Richards Island, nearTuktoyaktuk and at Nicholson Point (Fig. 1). This deformation has been attributed to glacier-ice thrusting (Reference Mackay, Rampton and FylesMackay and others, 1972) and appears similar in nature to the deformation discussed in this paper.

Methods

Stratigraphic sections ~5—20 m high and ~20—300 m long were logged sedimentologically and sketched in order to determine the stratigraphy of the deformed permafrost. Descriptions of ice and sediment facies follow those of Reference Murton and FrenchMurton and French (1994).

Clast fabrics were measured in three samples of diamicton and one sample of underlying massive ice in order to (1) compare them with fabrics reported from basal glacier ice (Reference LawsonLawson, 1979a; Reference Ham and MickelsonHam and Mickelson, 1994; Reference Bennett, Waller, Glasser, Hambrey and HuddartBennett and others, 1999), and (2) assess if the diamicton and massive ice displayed similar strain signatures. The orientation and dip of at least 30 clasts with a: b axis ratios of ≥3:2 were measured and plotted on Schmidt equal-area stereonets. From these data were calculated the three principal eigenvalues (S 1, S 2 and S 3; Reference MarkMark, 1973), as well as fabric isotropy (I = S 3/S i) and fabric elongation (E = 1 — (S 2/S 1)) (Reference BennBenn, 1994).

Petrographic analysis of one sample of massive ice from Pullen Island (Fig. 1) was carried out in order to determine the characteristics of the ice crystals and sediment inclusions, and the crystal c-axis orientations. The analyses were carried out in the McGill University Geocryology Laboratory, following methods described by Reference LangwayLangway (1958). The sample block was trimmed and cut into thick slices to facilitate examination of cryogenic structure and inclusion patterns. Vertical thin sections were prepared from subsamples of the block sample and examined under cross-polarized light to determine crystal size and shape, and plane light to examine structural characteristics. Crystal c-axis orientations were measured using a standard Rigsby stage. The high sediment content made thin-section and systematic c- axis orientation problematic. Approximate fabric patterns were obtained by partially melting and refreezing oriented chip samples and were plotted as lower-hemisphere projections on a Schmidt equal-area net (see Fig. 2).

Fig. 2. Lower-hemisphere projection of c-axis orientations on a Schmidt net of a vertical thin section of massive ice from Pullen Island.

Oxygen and deuterium isotopic analysis of ground ice within permafrost was undertaken in order to (1) determine the water source for the ice and the conditions of freezing, and (2) test the hypothesis that blocks of ice dispersed within diamicton derive from underlying massive ice and are therefore isotopically similar. The analyses were carried out in the G. G. Hatch Stable Isotope Laboratories, University of Ottawa, to an analytical precision of ±1% for δD and ±0.1 ‰ for δ18O.

Observations

The stratigraphy of ice-rich permafrost in glaciated terrain of the Tuktoyaktuk Coastlands is described below from three sites that provide large vertical sections through terrain veneered by Toker Point till (Reference Rampton and SennesetRampton, 1988a, map 1647A) and that contain abundant deformation structures and ground ice. Site 1 is on the southern shore of Liverpool Bay, extending from the mainland directly southwest of Nicholson Island for ~5 km to the west (Figs 1 and 3a). Site 2 is located on northern ‘Crane Island’ (informal name), in the central Eskimo Lakes (Figs 1 and 3b). Site 3a is on western Pullen Island (Figs 1 and 3c), and site 3b is on the northwest bluff of an adjacent island at North Head (Figs 1 and 3c).

Fig. 3. Location of sites at (a) Liverpool Bay; (b) ‘Crane Island’, central Eskimo Lakes; and (c) Pullen Island and North Head. Locations are shown in Figure 1.

The permafrost stratigraphy of these sites comprises massive ice beneath ice-rich diamicton or sandy silt. The massive ice is at least ~2.5—8.0 m thick, and either (i) white and bubble-rich, or (ii) grey, debris-rich and banded. Its upper contact is a planar to irregular angular unconformity. The overlying diamicton and sandy silt is >4 to ~12 m thick, and contains (1) ice blocks, many of which have internal debris bands that are truncated along block margins; (2) sand lenses and layers, some of which show boud- inage and some that contain recumbent, isoclinal and Z- shaped folds; (3) ice veins that are aligned and dipping at 20—30°; (4) ice lenses adjacent and parallel to sedimentary contacts; and (5) ice wedges. The stratigraphy, sedimentol- ogy, deformation structures, ice petrography and stable isotopes for each site are listed in Tables 1-3 and illustrated in Figures 2 and 4-11.

Table 1. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 1, Liverpool Bay

Table 2. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 2, ‘Crane Island’

Table 3. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 3a, Pullen Island

Fig. 4. Co-isotope plot of full dataset for ground ice from Liverpool Bay, ‘Crane Island’ and Pullen Island. Also shown are oxygen isotope data for massive ice and ice blocks from North Head. The massive ice at all of the sites is of the dark-grey, bubble-poor, banded type, except where white, bubble-rich massive ice is indicated in five of the six samples from Liverpool Bay. V-SMOW: Vienna StandardMean OceanWater.

Fig. 5. Stratigraphy at Liverpool Bay. Locations of sections are shown in Figure 3a.

Fig. 6. Schmidt equal-area stereonets of clast fabrics from ice-rich diamicton at Liverpool Bay (a, b), and massive ice (c) and overlying ice-rich diamicton at ‘Crane Island’ (d).

Fig. 7. Co-isotope plots showing regression lines for (a) massive ice at Liverpool Bay, and (b) massive ice and ice blocks at Pullen Island.

Fig. 8. Ice blocks (ice clasts) in near-surface permafrost. (a) Ice blocks within ice-rich diamicton, Liverpool Bay, 8 July 1998. One block comprises the hinge of a truncatedfold. Spade for scale, (b) Block of massive ice (~15 m long) within ice-rich diamicton, Liverpool Bay, 8 July 1998; location shown in Figure 5a. (c) Chaotic arrangement of ice blocks (arrows) in sandy silt unit, Pullen Island, 4 May 1999. Person with ice axefor scale, (d) Elongate ice blocks aligned parallel to glaciotectonic lenses and pinch-and-swell structures of sand and clay, North Head, 10 August 1991. Trowelfor scale. (e) Large ice block showing truncated bands along its sides, North Head, 10 August 1993. Spade for scale. (f) Excavated ice block with streamlined form, North Head, 11 August 1993.

Fig. 9. Schematic stratigraphy at ‘Crane Island’.

Fig. 10. Schematic stratigraphy at Pullen Island.

Fig. 11. Glacitectonite at North Head. (a) Lenses and layers of sand within silty clay. Note the various stages of attenuation of in homogeneities into fold noses and allochthonous folds. Pencil for scale. (b) Close-up of lenses within a pinch-and-swell structure of sand. Pencil for scale.

Interpretation

In order to evaluate the evidence for glacially deformed permafrost, we must first consider the origin of the massive ice, because this comprises a major element of the exposed stratigraphy and a potential source of ice blocks within the overlying sediments. Secondly, we discuss the evidence for subglacial deformation and erosion. Finally, we interpret the features associated with postglacial processes.

Origin of massive ice

The white, bubble-rich massive ice at Liverpool Bay probably formed within pre-existing sediment (i.e. intrasedimental ice) rather than being buried by younger sediment (i.e. buried ice). Intrasedimental massive ice forms in situ by growth of segregated to intrusive ice during downward permafrost aggradation in regions where subpermafrost groundwater is under high pressure (Reference MackayMackay, 1971; Reference Mackay and DallimoreMackay and Dallimore, 1992). The high pressure may arise from (1) pore-water expulsion during freezing of saturated, coarse-grained sediment such as sand, as occurs during the growth of hydrostatic pingos, but on a larger scale (Reference MackayMackay, 1971); and/or (2) subglacial meltwater driven towards aggrading permafrost near the edge of an ice sheet in response to a gradient in ice overburden pressure (Reference Rampton and SennesetRampton, 1988a, b). The pressurized groundwater feeds a lens of massive ice growing at or near the contact of frost-susceptible sediment (e.g. silty clay till) and underlying sand.

Although a buried glacier origin for the white, bubble- rich massive ice at Liverpool Bay cannot be discounted, the ice resembles neither contemporary basal nor firnified glacier ice in terms of all its observed field characteristics. Instead, an intrasedimental interpretation is preferred for three reasons: (1) the massive ice isotopically matches segregated ice in the underlying Kittigazuit Formation sand (Fig. 4); (2) the observed lower contact of the massive ice is conformable with this underlying segregated ice; and (3) the massive ice contains layers of suspended sand grains similar to those in the Kittigazuit Formation. All three observations are consistent with downward freezing through the sand. In addition, the ice closely resembles massive intrasedimental ice at Peninsula Point (Fig. 1), both being bubble-rich and relatively sediment-poor (Reference Mackay and DallimoreMackay and Dallimore, 1992). An intrasedimental origin for massive ice directly south of Nicholson Island and therefore in sections near those described here has been proposed independently by French and Harry (1990, Fig. 7B).

The origin of the grey, banded massive ice at Liverpool Bay is less certain. Possibly, the ice resulted from shearing- induced regelation along the upper boundary of the white massive ice. This might account for (1) the occurrence of the banded ice directly above the white ice (Fig. 5c); (2) the abundant cracks (shear planes) within the white ice; and (3) the intercalation of debris-rich layers comprising suspended aggregates of sandy silty clay and debris-poor layers, similar to regelation ice in contemporary glaciers (Reference Kamb and LaChapelleKamb and LaChapelle, 1964; Reference Hubbard and SharpHubbard and Sharp, 1995). Alternatively, the intercalation of the white and banded ice types (Fig. 5e) may reflect subsequent folding and shearing during glacial overriding (Reference HartHart, 1995; Reference Hart and WallerHart and Waller, 1999).

The debris-rich massive ice at ‘Crane Island’and Pullen Island is interpreted as buried basal glacier ice. At ‘Crane Island’, the sediment dispersed within the bands of aggregate-poor ice is a diamicton visually identical to that in the overlying, ice-rich diamicton, previously mapped as till (Reference Rampton and SennesetRampton, 1988a). The bands of aggregate-poor ice with suspended rock clasts closely resemble basal stratified suspended sub-facies ice from Matanuska Glacier, Alaska, U.S.A. (Reference LawsonLawson, 1979b), and from the southwest Greenland ice sheet (Reference KnightKnight, 1997; Reference Waller, Hart and KnightWaller and others, 2000). The clast fabric in the massive ice (Fig. 6c) displays a strongly preferred orientation similar to that characteristic of contemporary basal glacier ice (Reference LawsonLawson, 1979a; Reference Bennett, Waller, Glasser, Hambrey and HuddartBennett and others, 1999). The massive ice at both ‘Crane Island’ and Pullen Island lacks the white, bubble-rich ice facies common in massive intrasedimental ice at Liverpool Bay and Peninsula Point.

The oxygen isotope composition of the massive ice at sites 1-3 (mean = -30.2‰, std dev. = 2.0‰, n = 16) is similar to that of other massive ice in the Tuktoyaktuk Coastlands (e.g. -28 to -35‰; Reference MackayMackay, 1983) and to that of Laurentide ice identified at the base of the Barnes Ice Cap, Baffin Island, Canada (mean = -34.6‰; Reference Zdanowicz, Fisher, Clarke and LacelleZdanowicz and others, 2002). The oxygen isotope composition of the massive ice suggests a very cold water source. Refrozen meltwater may be enriched in 18 O by as much as 3‰, and that would displace intrasedimental massive ice to values more enriched than Laurentide meltwater from, for example, the Barnes Ice Cap. However, the co-isotopic plots for the white, bubble-rich massive ice at Liverpool Bay and the banded massive ice at Pullen Island do not assist in the determination of their origin due to their poorly constrained distributions (Fig. 7).

Evidence for subglacial deformation and erosion

Angular unconformity

The upper contact of the banded massive ice at all three sites is an angular unconformity resulting from erosion of the ice. Had the contact formed by downward freezing, we would expect a conformable relationship between the ice and the overlying sediments, i.e. where bands in the massive ice run parallel to the upper contact of the ice (Reference MackayMackay, 1989, Fig. 1). The conformable relationship would reflect alignment ofice and sediment bands orthogonal to the direction of heat flow, a feature characteristic of ice segregation. Alternatively, had the contact formed by downward thaw of the massive ice, the allochthonous blocks of ice (discussed below) in the overlying sediment would have melted. Instead, the contact is attributed to decollement that truncated the banded massive ice and supplied the ice blocks to the overlying sediment.

Ice blocks (ice clasts)

The ice blocks are interpreted as ice clasts eroded from preexisting ice. In situ formation of segregated or intrusive ice is discounted where bands within ice blocks are truncated along block margins. Although some ice blocks may conceivably derive from toppling of ice down crevasses or from the ice front, we have not observed blocks of stratified, bubble-rich ice characteristic of firnified glacier ice; but we cannot discount the possibility that small clear ice blocks may be remnants of such ice. More likely, however, is the interpretation that many or all of the ice blocks were eroded from pre-existing ice, particularly massive ice. Erosion from massive ice would account for (1) the large size of some ice blocks (≤15 m long × ≤ 1.5 m high; Figs 5a and 8b); (2) the similarity of ice facies in many blocks to those in the banded massive ice; (3) the stratigraphic occurrence of ice blocks above or laterally adjacent to massive ice; (4) the angular unconformity (erosion surface) along the top of the massive ice; and (5) those ice blocks with δ18O values of -28 to —30‰, which are within the δ18O range obtained from massive ice in the present study (—28.0 to —33.1‰; Fig. 4) and by Reference MackayMackay (1983). In addition, the similar size, shape and alignment of many ice blocks to adjacent sand lenses derived from pre-existing sand, as discussed below, are consistent with subglacial erosion and deformation.

Those ice blocks from North Head with δ18O values of —22‰ are isotopically too heavy to derive from massive ice. They are also too heavy to derive from single-stage refreezing of meltwater from massive ice, which could produce δ518O values no heavier than about —25‰, and may account for ice blocks with intermediate δ18O values of ~ —27 to —25‰ (Fig. 4). Instead, the ice blocks with δ18O values of —22‰ may derive from a different climate regime because shifts of 5—10‰ for δ18O usually correspond with glacial- to-interglacial or stadial-to-interstadial changes. Hence, the isotopically heaviest ice blocks may be fragments of preglacial ground ice dating from a warm climatic period. Another process that will enrich the ice is the contribution of ambient precipitation, which falls at lower elevation than in the higher catchments of the LIS and is likely summer- dominated off the Beaufort Sea.

The alignment of elongate ice blocks more or less parallel to adjacent sand lenses and laminae, and the smooth deflection of some sand lenses around them are attributed to movement within a shear zone. The rounded and streamlined shape of many ice blocks may reflect partial melting and/or erosion within the shear zone.

Folds within ice blocks developed either before or during movement within the shear zone. The unusual truncated fold shown in Figure 8a was probably eroded from a fold similar to those common in the banded massive ice at Liverpool Bay. If such folding developed after blocks were eroded, we would expect to observe many more examples of ice blocks containing similar folds.

Glacitectonite

The ice-rich diamicton at Liverpool Bay and ‘Crane Island’ (see Fig. 9) and the sandy silt at Pullen Island (see Fig. 10) are interpreted as glacitectonite. An origin as till is discounted because these frozen sediments contain ice clasts and do not overlie a thaw unconformity; hence the sediment has never melted out and been finally deposited (cf. Reference Kaplyanskaya and TarnogradskiyKaplyanskaya and Tarnogradskiy, 1986; Reference Dyke and SavelleDyke and Savelle, 2000). Instead, an origin as glacitectonite is consistent with (1) the evidence for a lack of thaw, (2) the occurrence of striated and/or faceted rock clasts at ‘Crane Island’, and (3) the inclusions of sand or ice blocks. The brown, fine sand in some sand lenses and layers at Liverpool Bay has clearly been eroded from the underlying, preglacial Kittigazuit Formation. The streamlined shape to some sand lenses, similar to augen and boudins in metamorphic rocks (Reference Passchier and TrouwPasschier and Trouw, 1996), is attributed to erosion and deformation of the edges of stiff sand pods during shear within more rapidly deforming finer-grained sediment in the surrounding diamicton. Similar lenses and laminations have been reported in subglacially deformed Pleistocene sediments in Canada (Reference MenziesMenzies, 1990) and the U.K. (Reference Hart and BoultonHart and Boulton, 1991; Reference Benn and EvansBenn and Evans, 1996).

The sites display a variety of structures commonly observed within subglacially deformed sequences. Recumbent folds are present at all sites and indicate simple shear and ductile deformation, forming where there is a perturbation in the junction between two layers of differing rheology. As strain increases, the fold becomes more attenuated in the direction of principal shear, producing a tectonic lamination. Figure 11a shows various stages in the attenuation of inhomogeneities into fold noses and allochthonous folds. The pinch-and-swell structures at North Head reflect horizontal extension parallel to layering and brittle failure of the sand layer within a more ductile matrix. Their incomplete separation suggests only a slight difference in competency between the two units (Reference RobertsRoberts, 1989). The small sand lenses observed within one such pinch-and-swell structure (Fig. 11b) are interpreted as shear lenses, similar to those reported from the B1 horizon of subglacially deformed, unfrozen sediment from Svalbard (Reference BoultonBoulton, 1970) and Iceland (Reference Boulton, Menzies and RoseBoulton, 1987). Additional evidence for brittle failure is provided by (1) ice veins within the ice-rich diamicton and (2) cracks within the white, bubbly massive ice at Liverpool Bay. The ice veins probably mark tension cracks formed in a shear zone. Similar features, often comprising quartz or cal- cite veins and interpreted as en echelon tension gashes, define brittle shear zones in rock (cf. Reference RobertsRoberts, 1989). In the case of the structures reported here, fracturing is inferred during shear, with segregated ice infilling the fractures during or after shear.

Clast fabrics are commonly used to reconstruct the strain history of sheared materials, and have been applied both to sediment-rich basal glacier ice (e.g. Reference LawsonLawson, 1979a; Reference Ham and MickelsonHam and Mickelson, 1994; Reference Bennett, Waller, Glasser, Hambrey and HuddartBennett and others, 1999) and to subglacial sediments (Reference HartHart, 1994; Reference BennBenn, 1995; Reference Bennett, Waller, Glasser, Hambrey and HuddartBennett and others, 1999). As the ice-rich diamictons have been deformed in a frozen state, comparisons with the former are more appropriate. Both Lawson (1979a) and Reference Ham and MickelsonHam and Mickelson (1994) suggest that sediment-rich basal glacier ice is characterized by very strong, flow-parallel fabrics with Si values mostly >0.8; they group tightly near the cluster apex of triangular eigenvalue plots (Reference BennBenn, 1994). Although the fabrics recorded from ice-rich diamicton at Liverpool Bay display similar strengths (S 1 = 0.843 and 0.797), consistent with their interpretation as a glacially deformed ice—sediment mixture, the sample from ‘Crane Island’ displays a much weaker orientation (S 1 = 0.605). Although this result falls outside the range of data for basal ice presented by Lawson (1979a) and Reference Ham and MickelsonHam and Mickelson (1994), it does lie within the range of values presented by Reference Bennett, Waller, Glasser, Hambrey and HuddartBennett and others (1999) and therefore is consistent with a glacially deformed ice—sediment mixture. The mean vectors from the ice-rich diamic- ton and massive ice (Fig. 6) are all approximately parallel to the ice-flow direction independently inferred by Ramp- ton (1988a) (Fig. 1).

The range of oxygen isotope values obtained from reticulate ice within the ice-rich diamicton at Liverpool Bay and ‘Crane Island’ (—29.4 to —31.2‰) is within the range typical of massive ice in the Tuktoyaktuk Coastlands, and indicates a very cold water source. This discounts thaw of the ice-rich diamicton during the Holocene and mixing with isotopically heavier water from warmer climatic conditions.

Postglacial processes

Ice segregation

The large ice lenses in the ice-rich diamicton at Liverpool Bay and the silty sand at Pullen Island formed by ice segregation after glacial deformation had ceased. If the ice lenses pre-dated deformation, we would expect them to have been boudinaged or eroded, to form ice clasts. At Liverpool Bay the location of the ice lenses within or directly above sand lenses was clearly influenced by the orientation of sand—dia- micton contacts, i.e. between frost-susceptible and nonfrost-susceptible sediment. The δ18O values of the segregated ice at both sites (Fig. 7) suggest a very cold water source, and discount mixing with isotopically heavier water associated with warmer climatic conditions during the Holocene.

Active-layer deepening and mass movement

The ice-rich silt at ‘Crane Island’ is interpreted as Holocene colluvium, consistent with burial of organic matter by downslope soil movement. The sharp base of the silt is a thaw unconformity that probably marks the base of the early-Holocene active layer, when the active layer was regionally deeper than at present, melting the tops of the buried ice wedges (Fig. 9; cf. Reference MackayMackay, 1975; Reference BurnBurn, 1997).

Discussion

Our observations allow us to make some important inferences about deformation, rheology and erosion of permafrost beneath the cold-based margin of a former ice sheet.

Glaciotectonic deformation at sites 1—3 occurred beneath the margin of the LIS. Proglacial deformation is discounted because the glaciotectonic structures described, in particular the isoclinal recumbent folds and pinch-and- swell structures, indicate simple shear and extension, which are characteristic of subglacial deformation, as discussed above, rather than compressive strains associated with proglacial deformation (cf. Reference Hart and BoultonHart and Boulton, 1991). In addition, the ice clasts resemble in size and shape sediment inclusions characteristic of subglacially deformed sediment (e.g. Reference Benn and EvansBenn and Evans, 1996), and it is difficult to understand how they could have been eroded proglacially. However, subglacial deformation beneath the warm-based interior of the ice sheet is discounted because the glacitectonite has never thawed. Instead, deformation took place beneath the cold-based margin of the LIS. The possibility that glacier overriding was preceded or followed by proglacial deformation cannot be excluded.

Deformation occurred while the sediment was frozen but contained limited amounts of liquid water. Pervasive unfrozen conditions during deformation are precluded because (1) massive ice and (2) eroded and deformed ice blocks interpreted as ice clasts are preserved within the deformed permafrost. However, the glacitectonite must have contained some liquid water, because segregated ice could not otherwise have formed within it after deformation had ceased. The unfrozen water probably resulted from freezing-point depression in clay-rich sediments such as the ice- rich diamicton and/or from local pressure melting during deformation, for example, at the top of the white massive ice at Liverpool Bay. It is well documented in the permafrost literature that ice and unfrozen water can coexist, and that ice segregation can occur in fine-grained frozen soils at temperatures of a few degrees below 0°C (Reference Williams and SmithWilliams and Smith, 1989).

The presence and quantity of liquid water are key determinants of the mechanical properties of frozen ground. Liquid water reduces the strength of both ice-ice and ice- sediment bonds and, in the case of ice-sediment mixtures, substantially reduces cohesion (Reference Williams and SmithWilliams and Smith, 1989). In addition to temperature, the amount of liquid water present strongly depends on grain-size, with clay retaining significant quantities down to temperatures well below the freezing point. Frozen, fine-grained sediments thus display much lower yield stresses than frozen coarse-grained sediments, and at temperatures between 0°C and —2°C are more susceptible to creep deformation than is pure ice (Reference Johnston, Ladanyi, Morgenstern, Penner and JohnstonJohnston and others, 1981). These experimental results concerning variations in unfrozen water content provide a theoretical explanation for the competency contrasts inferred from the permafrost stratigraphy at sites 1—3: the ice clasts and layers and lenses of frozen sand constituted relatively competent units within a more rapidly deforming shear zone of partially frozen, ice-rich diamicton. Such warm conditions (i.e. close to the pressure-melting point) result in a reduction in the yield stress of both the ice and frozen sediment and thereby promote pervasive creep deformation (Reference VialovVialov, 1965; Reference Mellor and TestaMellor and Testa, 1969). Reference TsytovichTsytovich (1975) terms this type of easily deformable permafrost ‘plastic-frozen ground’, as opposed to ‘hard-frozen ground’, which is comparatively rigid.

Rheologically, the deformed permafrost is dominated by structures indicative of ductile or creep deformation, including a variety of fold types (recumbent and S-shaped). This style of deformation is common in relatively warm, ice-rich materials subjected to low deviatoric stresses over long time periods. There is, however, evidence for brittle failure in the form of pinch-and-swell structures at North Head and en echelon tension gashes at Liverpool Bay and Pullen Island. The tension gashes may have resulted from variations in the strain rate (personal communication from G. D. Williams, 2003) and/or temperature within the deforming permafrost. Alternatively, they may reflect local extension and the tendency of ice to fail in a brittle fashion when subjected to tensile stress (Reference Williams and SmithWilliams and Smith, 1989). The clast-fabric data, featuring a range of weak and strongly orientated fabrics, may also indicate the occurrence of both pervasive, ductile deformation and brittle or brittle/ductile shear (Reference HartHart, 1994; Reference BennBenn, 1995).

Erosion of permafrost accompanied deformation. Erosion is indicated by (1) the angular unconformity along the top of the massive ice and (2) the abundant ice clasts within the overlying glacitectonite. The unconformity marks a de- collement surface beneath a shear zone. At Liverpool Bay and ‘Crane Island’ this surface was irregular (Figs 5 and 9), but at Pullen Island it was subhorizontal (Fig. 10). The nature of this contact is consistent with erosion of pre-existing irregularities in the ice, as discussed by Reference Boulton, Menzies and RoseBoulton (1987) in the case of subglacial deformation of unfrozen sediment. Shear at this contact may also have promoted regelation and deformation within the underlying massive ice and the formation of the banded ice facies at Liverpool Bay.

A schematic model of permafrost deformation beneath the northwest margin of the LIS is shown in Figure 12. The model is broadly consistent with that inferred by Reference Astakhov, Kaplyanskaya and TarnogradskiyAstakhov and others (1996) in western Siberia, because both models involve (1) subglacial extension over a weak zone of finegrained and/or ice-rich permafrost, and (2) significant subglacial erosion of frozen materials. The model also supports Reference Mathews and MackayMathews and Mackay’s (1960) suggestion that glacial- induced shearing may occur in clayey beds in permafrost. However, our observations, which are confined to near-surface permafrost, do not allow testing of Reference Mathews and MackayMathews and Mackay’s (1960) inference that high pore-water pressures beneath subglacial permafrost facilitated glacial thrusting by reducing the shear strength of unfrozen soil.

Fig. 12. Schematic model of deforming, warm, ice-rich permafrost beneath the northwest margin of the LIS. The approximate thickness of the ice sheet is based on Rampton’s (1988a) reconstruction.

Conclusions

The main conclusions from this study are as follows:

  1. (1) Ice-rich permafrost in the Tuktoyaktuk Coastlands was deformed to depths of at least 5-20 m beneath the northwest margin of the LIS. The deformed permafrost examined comprised frozen glacitectonite above intra- sedimental massive ice or buried basal glacier ice. Because this mixture of ice and sediment moved subglacially, the deformed permafrost could be considered to represent either a frozen subglacial deforming layer or a debris-rich basal ice layer.

  2. (2) Rheologically, the deformed permafrost is dominated by glaciotectonic structures (recumbent and S-shaped folds, sand lenses and layers) indicative of ductile deformation and common in warm, ice-rich materials. The ice clasts and sand layers and lenses within the gla- citectonite constituted relatively competent, frozen units within a more rapidly deforming shear zone of finer sediment that contained both ice and limited amounts of liquid water.

  3. (3) Subglacial erosion of permafrost formed an angular unconformity along the top of the massive ice, and supplied frozen Pleistocene sediment and ice clasts to the glacitectonite. The ice clasts were eroded from pre-existing ground ice.

  4. (4) Two types of ground ice occur in the deformed permafrost: (i) massive ice and ice clasts, both of which have been glacially deformed, eroded or moved; and (ii) segregated ice and ice-wedge ice that have not been glacially disturbed because they post-date deformation.

Acknowledgements

J.B.M.’s fieldwork between 1989 and 1993 was supported by grants (to Professor H. M. French) from the Natural Sciences and Engineering Research Council, Canada, and the Geological Survey of Canada (GSC). Logistical support was provided by the Polar Continental Shelf Project, Natural Resources Canada; the GSC; and the Inuvik Research Centre, Aurora College. Fieldwork in 1998 and 1999 was funded by grants (toJ.B.M.) from the Leverhulme Trust and theTyrell Fund of the Geological Society. R.I.W’s participation was supported by the University of Greenwich. C.A.W. was supported by the University of Brighton Research Support Fund. A. D. Green, B. P. Lowe and F. Wolki assisted with fieldwork. S. Rowland and H. Lintott produced the figures. D. J. A. Evans and an anonymous referee are thanked for their constructive comments on the paper. This is Polar Continental Shelf Project contribution No. 02403.

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Figure 0

Fig. 1. Location map of the Tuktoyaktuk Coastlands and Yukon Coastal Plain. Ice-flow directions and ice limits of the Toker Point Stade and Sitidgi Stade are according to Rampton (1988a).

Figure 1

Fig. 2. Lower-hemisphere projection of c-axis orientations on a Schmidt net of a vertical thin section of massive ice from Pullen Island.

Figure 2

Fig. 3. Location of sites at (a) Liverpool Bay; (b) ‘Crane Island’, central Eskimo Lakes; and (c) Pullen Island and North Head. Locations are shown in Figure 1.

Figure 3

Table 1. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 1, Liverpool Bay

Figure 4

Table 2. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 2, ‘Crane Island’

Figure 5

Table 3. Stratigraphy and glaciotectonic structures of near-surface permafrost at site 3a, Pullen Island

Figure 6

Fig. 4. Co-isotope plot of full dataset for ground ice from Liverpool Bay, ‘Crane Island’ and Pullen Island. Also shown are oxygen isotope data for massive ice and ice blocks from North Head. The massive ice at all of the sites is of the dark-grey, bubble-poor, banded type, except where white, bubble-rich massive ice is indicated in five of the six samples from Liverpool Bay. V-SMOW: Vienna StandardMean OceanWater.

Figure 7

Fig. 5. Stratigraphy at Liverpool Bay. Locations of sections are shown in Figure 3a.

Figure 8

Fig. 6. Schmidt equal-area stereonets of clast fabrics from ice-rich diamicton at Liverpool Bay (a, b), and massive ice (c) and overlying ice-rich diamicton at ‘Crane Island’ (d).

Figure 9

Fig. 7. Co-isotope plots showing regression lines for (a) massive ice at Liverpool Bay, and (b) massive ice and ice blocks at Pullen Island.

Figure 10

Fig. 8. Ice blocks (ice clasts) in near-surface permafrost. (a) Ice blocks within ice-rich diamicton, Liverpool Bay, 8 July 1998. One block comprises the hinge of a truncatedfold. Spade for scale, (b) Block of massive ice (~15 m long) within ice-rich diamicton, Liverpool Bay, 8 July 1998; location shown in Figure 5a. (c) Chaotic arrangement of ice blocks (arrows) in sandy silt unit, Pullen Island, 4 May 1999. Person with ice axefor scale, (d) Elongate ice blocks aligned parallel to glaciotectonic lenses and pinch-and-swell structures of sand and clay, North Head, 10 August 1991. Trowelfor scale. (e) Large ice block showing truncated bands along its sides, North Head, 10 August 1993. Spade for scale. (f) Excavated ice block with streamlined form, North Head, 11 August 1993.

Figure 11

Fig. 9. Schematic stratigraphy at ‘Crane Island’.

Figure 12

Fig. 10. Schematic stratigraphy at Pullen Island.

Figure 13

Fig. 11. Glacitectonite at North Head. (a) Lenses and layers of sand within silty clay. Note the various stages of attenuation of in homogeneities into fold noses and allochthonous folds. Pencil for scale. (b) Close-up of lenses within a pinch-and-swell structure of sand. Pencil for scale.

Figure 14

Fig. 12. Schematic model of deforming, warm, ice-rich permafrost beneath the northwest margin of the LIS. The approximate thickness of the ice sheet is based on Rampton’s (1988a) reconstruction.