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Science

Glacial geomorphology between the Gran Campo Nevado and Estrecho de Magallanes, Chile (52–53°S, 73°W)Open DataOpen Materials

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Article: 2153091 | Received 29 Aug 2022, Accepted 21 Nov 2022, Published online: 03 May 2023

ABSTRACT

We present the first extensive high-resolution glacial geomorphic map west of the Andean Cordillera in southernmost Chile (52.8–53.1°S, 73.0–73.9°W). The map extends over 1565 km2 and is based on high-resolution satellite images and aerial photographs. At selected locations, the remotely mapped geomorphology was corroborated by field observations. The study area is dominated by glacial erosional landforms (77%) over depositional landforms (23%), with published submarine depositional landforms having been included (e.g. moraines). Glacial drift, kettle kame topography and lateral and frontal moraines form the primary depositional landforms and sediment associations. Glacial cirques, wide U-shaped valleys, whalebacks, roches moutonnées and scoured bedrock characterize most of the mapped area. The spatial distribution of whalebacks and roches moutonnées in the study area indicates a lack of lithological control on their formation and a warm-based, dynamic ice velocity and thickness regime during Patagonian Ice Sheet cover and retreat during the last glacial cycle.

1. Introduction

The well-preserved terrestrial geomorphology east of the Andean divide has led to numerous glacial geomorphic mapping efforts (e.g. Bendle et al., Citation2017; Caldenius, Citation1932; Clapperton, Citation1983; CitationClapperton, 1992; Darvill et al., Citation2014; Glasser & Jansson, Citation2008; Izagirre et al., Citation2018; Lovell et al., Citation2011; Soteres et al., Citation2020) and geochronological studies (e.g. CitationClapperton et al., 1995; Blomdin, Citation2012; Darvill et al., Citation2015; García et al., Citation2012, Citation2018; McCulloch et al., Citation2005; Sagredo et al., Citation2011) covering over one million years of Patagonian glacial history (Hein et al., Citation2009). During the last glacial cycle (110.8–11.7 ka; CitationHughes et al., 2013), the Patagonian Ice Sheet extended between 38° and 56°S (Glasser & Jansson, Citation2008). Geochronological data indicate regional variations in the timing of maximum Patagonian Ice Sheet expansion between 75 and 28 ka (e.g. Darvill et al., Citation2015; García et al., Citation2018; Geiger, Citation2015; Glasser et al., Citation2011; Mendelová et al., Citation2020). Glacier lobes drained eastward and westward from the Andes, with maximum ice sheet widths of ∼350 km at 46°S and 52–53°S (see Davies et al., Citation2020). Based on current glacial geomorphic and geochronological data, the total ice-covered area at 35 ka has been estimated to be ∼492,600 km2 with sea level equivalent contributions estimated to ∼1.5 m (Davies et al., Citation2020), which is more than the modeled last glacial maximum (LGM: 33–26.5 ka; Clark et al., Citation2009) equivalent sea level contribution of ∼1.2 m (Hulton et al., Citation2002).

One remnant of the former Patagonian Ice Sheet is known as the Gran Campo Nevado (GCN, 52.7–52.9°S, 72.9–73.2°W; and ). The GCN is an ice cap located in southern Patagonia with a mean elevation of 880 m a.s.l. and an area of 189 km2 (Koch & Kilian, Citation2005). At present, the GCN is composed of 75 glaciers predominantly draining into tidal fjords towards the west and proglacial lakes towards the east (Schneider et al., Citation2007). The GCN is located in the southern sector of the Peninsula Muñoz Gamero () and is the largest ice body between the Campo de Hielo Patagónico Sur (HPS; engl. Southern Patagonian Ice Field) and the Estrecho de Magallanes (EDM; engl. Strait of Magellan, ).

Figure 1. Research area and published studies. (a) Study area indicated by box west of the Gran Campo Nevado, located ca. 130 km south of the Campo de Hielo Patagónico Sur. (b) Mapped area includes overlap rectangles of locations studied previously. Solid black symbols correspond to marine sediment records (MSR), hollow symbols indicate lake sediments cores (LS), CitationBiester et al. (Citation2002) utilize peat records (PR), CitationLamy et al. (Citation2010) include MSR, LS and PR data while CitationSchimpf et al. (Citation2011) use cave and stalagmites samples (CS). Blue squares indicate the closest automatic weather stations.

Figure 1. Research area and published studies. (a) Study area indicated by box west of the Gran Campo Nevado, located ca. 130 km south of the Campo de Hielo Patagónico Sur. (b) Mapped area includes overlap rectangles of locations studied previously. Solid black symbols correspond to marine sediment records (MSR), hollow symbols indicate lake sediments cores (LS), CitationBiester et al. (Citation2002) utilize peat records (PR), CitationLamy et al. (Citation2010) include MSR, LS and PR data while CitationSchimpf et al. (Citation2011) use cave and stalagmites samples (CS). Blue squares indicate the closest automatic weather stations.

Figure 2. Spatial coverage of imagery used for geomorphological mapping. Planet satellite orthorectified images (Imagery © 2019 Planet Labs Inc.) form the base-map. Mosaics from these satellite images and from Sentinel-2 images cover the entire mapped area so are not indicated. The UAV footage area represents total area visualized during the flight. Colored hillshade of 45° is from ALOS PALSAR DEM and delimits the mapped area. Selected codes from the DGA inventory provided for Gran Campo Nevado glaciers (see Table S1). Islands mentioned in the text are labeled with numbers: 1: Isla Tamar (∼10 km2), 2: Isla Emiliano Figueroa (∼170 km2), 3: Isla Providencia (∼25 km2), 4: Isla Eleodoro (∼8 km2), 5: Isla Merino (∼11 km2).

Figure 2. Spatial coverage of imagery used for geomorphological mapping. Planet satellite orthorectified images (Imagery © 2019 Planet Labs Inc.) form the base-map. Mosaics from these satellite images and from Sentinel-2 images cover the entire mapped area so are not indicated. The UAV footage area represents total area visualized during the flight. Colored hillshade of 45° is from ALOS PALSAR DEM and delimits the mapped area. Selected codes from the DGA inventory provided for Gran Campo Nevado glaciers (see Table S1). Islands mentioned in the text are labeled with numbers: 1: Isla Tamar (∼10 km2), 2: Isla Emiliano Figueroa (∼170 km2), 3: Isla Providencia (∼25 km2), 4: Isla Eleodoro (∼8 km2), 5: Isla Merino (∼11 km2).

The GCN is located on the Andean cordillera's axis, which is the only continuous orographic barrier between 46 and 56°S, intersecting oceanic as well as meteorological global circulation systems such as the Southern Westerly Winds (Garreaud et al., Citation2009; Kilian & Lamy, Citation2012; Lamy et al., Citation2010). These westerlies have a strong control on local precipitation and temperature patterns (Garreaud et al., Citation2013) directly impacting geomorphic processes. Precipitation comparisons at 53°S show that precipitation at sea level on the Pacific coast is 59% of the precipitation measured at sea level within the mountains, while to the east, precipitation drastically drops to 25% and 8% at Seno Skyring (to ∼70 km) and Punta Arenas (to ∼150 km), respectively (Schneider et al., Citation2003; see (a)). This barrier leads to high annual precipitation contrasts between >4,000 mm/a over the Pacific, ∼10,000 mm/a in the highly elevated cordillera and <500 mm/a east of the GCN (Möller et al., Citation2007; Schneider et al., Citation2003).

Whilst previous research in the study area has focused on the GCN’s glaciology (Davies & Glasser, Citation2012; Koch & Kilian, Citation2005; Meier et al., Citation2018; Möller et al., Citation2007; Schneider et al., Citation2007), marine geological mapping efforts to identify submerged glacial landforms (CitationBreuer et al., 2013b; Kilian et al., Citation2007b), and the extraction of marine, lake and peat sediment records for palaeoclimate reconstructions (Biester et al., Citation2002; CitationBreuer et al. 2013a; CitationBreuer et al., 2013b; Kilian et al., Citation2006; Lamy et al., Citation2010; Shiroya et al., Citation2013), no comprehensive study of the glacial geomorphology in the fjords and islands west of the GCN has been conducted until present ((b)).

In general, there is a lack of glacial geomorphic mapping west of the Andean divide between 44 and 55°S, with the exception of the Gualas, San Rafael, San Tadeo/Quintín (46.4–46.9°S; e.g. Heusser, Citation1960; Winchester & Harrison, Citation1996; Glasser et al., Citation2006; Winchester & Harrison, Citation1996), the Isla Wellington/Puerto Edén (∼49.1°S; Ashworth et al., Citation1991) and surrounding the Cordillera Darwin proglacial area (Hall et al., Citation2013; Izagirre et al., Citation2018). The limited terrestrial and marine glacial geomorphic data along 1600 km of the Patagonian Ice Sheet’s western margin (see Davies et al., Citation2020) considerably restricts our understanding of its palaeo-glaciological dynamics, manner of subsequent demise and associated climate feedbacks in the region. We present the first glacial geomorphic map between the GCN and the EDM to address this data gap between 52° and 53°S. This research provides the foundation for future geochronological studies that require a sound knowledge of the glacial geomorphology for targeted sampling. In addition, the methodologies developed here can be used to guide and extend future glacial geomorphic mapping efforts in the Chilean fjords to increase our understanding of Patagonian glacier dynamics along the Pacific coast during the last glacial cycle.

1.1. Study area

The mapped area is delimited by the GCN to the east, Bahia Beaufort and Seno Icy in the N/NW and the EDM in the S/SW, covering an area of 1,565 km2 ( and ). The landscape is characterized by deeply incised fjords and islands. The highest peaks in the field area are protruding the GCN up to 1500 m a.s.l. Fjord depths range between ∼700 m NE of Isla Tamar in Bahía Beaufort (CitationBreuer et al., 2013b) and up to ∼1,100 m south of Punta Cummings in the EDM (SHOA, Citation1998; see ). There are multiple small islands (<1 km2) in the study area and 10 larger than 1 km2. There are four main islands ranging between 8 and 172 km2 in size (). The Islands are named Emiliano Figueroa, Providencia, Tamar and Eleodoro, and account for 32% of the field area, while the rest is mainland.

The study area was covered by the Patagonian Ice Sheet during the last glacial cycle (see CitationDavies et al., 2020). Though there are no published terrestrial glacial geochronological datasets available to determine deglaciation rates, the marine transgression at 14,000 yr BP in the western Strait of Magellan (CitationKilian et al., 2007a) and identification of the Mount Burney Tephra (4150 yr BP) in the northern sections of Canal Sweet ((b); see CitationBreuer et al. 2013a) indicates that the last deglaciation of the study area occurred between the end of the last glacial and likely finished by the mid-Holocene.

2. Map production

2.1. Imagery

The glacial geomorphic map was produced using remote sensing data, field observations and published bathymetry data (see , ; see CitationBreuer et al., 2013a and supplemental material). Mapping was conducted manually and without automatic mapping procedures utilizing QGIS 3.28. Remote sensing data include optical and radiometric data sources which were integrated and manipulated in the GIS environment. In total, 19 optical high-resolution Planet satellite orthorectified images (PI; Imagery © 2019 Planet Labs Inc.) taken between 2017 and 2019 were used, as well as two Sentinel-2 satellite images (SI; 2018, bands 8-11-4 & 8-4-3, see also supplemental material), and 26 aerial photographs at 1:60,000 scale taken by the Servicio Aerofotogramétrico de Chile (SAF; flights in 1978 and 1982). Data from the Advanced Land Observing Satellite Digital Elevation Model (ALOS DEM; 12.5 m e.r.) was used as the topographic base and to map landforms and sediment deposits in excess of 500 meters. To improve landform delimitations, high-resolution images from the 3D Google Earth Pro software Version 7.0 (GE-v7.0) and very high-resolution Bing images (BI), available through the QGIS OpenLayers plugin, were used where images were freely available (). The mapped landforms in GE-v7.0 and BI were recognized and mapped onto the planet satellite images (PSI), which has an orthorectified pixel size of three meters and forms the base for the entire map. The aerial photographs were analyzed using traditional stereoscopy and georeferenced to the PIs using a mean of 72 control points per photograph (see supplementary material for detailed methodology).

Table 1. Remote sensing data used.

2.2. Field observations

Selected remotely mapped sites were visited during the #ChileFjords18 cruise in November 2018 to corroborate mapped features using direct field measurements, photography and unmanned aerial vehicle footage (UAV: DJI Mavic PRO 4 K HD; ; see the main map for flight route details). The use of a non-tripulated tool and the high-resolution field photographs and videos obtained from the UAV footage were used in two ways: (1) to observe areas of restricted access, and (2) to capture different angles of landforms between 1 m and ∼1 km2 (e.g. and (c,d)).

Figure 3. Examples of erosional landforms mapped (see and for location): (a) Hillshade from ALOS PALSAR DEM illuminated from northwest showing glacial cirques in the area close to Punta Pedro. (b) Map of coalescing cirques and arêtes, with a tarn at the base of the most north-eastern cirque. Lakes are shown in blue. (c) Infrared Sentinel image showing eroded bedrock as a gray surface. (d) Interpreted whalebacks (continuous line) and roche moutonnées (dashed line). Ice flow from east to west, selected landform long profiles shown in meters (not to scale). Profiles 1 and 2 show asymmetric cross profile with smooth stoss and steep lee side, whilst profile 3 is symmetric. (e) Planet image showing the clearest asymmetric roche moutonnée example in Falso Martinez Valley. (f) Same location as image 3e with hillshade. Ice flow from SE to NW, long profile of rouche moutonnée plotted in meters (not to scale).

Figure 3. Examples of erosional landforms mapped (see Figures 1 and 2 for location): (a) Hillshade from ALOS PALSAR DEM illuminated from northwest showing glacial cirques in the area close to Punta Pedro. (b) Map of coalescing cirques and arêtes, with a tarn at the base of the most north-eastern cirque. Lakes are shown in blue. (c) Infrared Sentinel image showing eroded bedrock as a gray surface. (d) Interpreted whalebacks (continuous line) and roche moutonnées (dashed line). Ice flow from east to west, selected landform long profiles shown in meters (not to scale). Profiles 1 and 2 show asymmetric cross profile with smooth stoss and steep lee side, whilst profile 3 is symmetric. (e) Planet image showing the clearest asymmetric roche moutonnée example in Falso Martinez Valley. (f) Same location as image 3e with hillshade. Ice flow from SE to NW, long profile of rouche moutonnée plotted in meters (not to scale).

Figure 4. Examples of whalebacks mapped in the field (see for locations). (a) Micro-scale whaleback at Seno Icy. (b) Micro-scale fractured whaleback at Isla Tamar. (c,d) Back and side view of a meso-scale whaleback colonized by vegetation on its stoss side, image captured during a UAV flight at Seno Glaciar.

Figure 4. Examples of whalebacks mapped in the field (see Figure 2 for locations). (a) Micro-scale whaleback at Seno Icy. (b) Micro-scale fractured whaleback at Isla Tamar. (c,d) Back and side view of a meso-scale whaleback colonized by vegetation on its stoss side, image captured during a UAV flight at Seno Glaciar.

3. Glacial landform and sediment description

In this section, we describe landform and sediment accumulations associated with (de)glaciation. All of the mapped landforms, commonly meso-scale (1 m–2 km), are listed and defined in with corresponding shape files provided as supplemental material. The high-resolution remote sensing data facilitated the identification of landforms with a minimum size of ∼30 m. Glacial erosional landforms and depositional landforms and sediment deposits cover an area of 77% and 23%, respectively.

Table 2. Identification criteria for landforms mapped from satellite/aerial imagery.

3.1. Glacial erosional landforms

A total of 463 meso-scale landforms related to glacial erosion were identified and mapped with criteria detailed in .

3.2. Cirques

In total, 70 armchair-shaped hollows with steep sides and back walls were identified in the study area and interpreted as cirques ((b) and main map). The majority of cirques or cirque clusters are located proximal to the GCN. The number of cirques reduces significantly westward likely as a function of lower elevation ((a,b)). The base of ice-free cirques ranges in altitude from 32 to 539 m a.s.l. with a mean base altitude of ∼270 m a.s.l. While 52% of ice-free cirques show a clear south-facing aspect, the remainder have no preferred aspect direction. Cirques developed facing westward or eastward are rare (<7%).

3.2.1. U-shaped valleys

Macro to micro-scale negative relief created by glacial erosional action is visible on remote sensing images in form of U-shaped valleys. Twenty-eight valleys with a clear U-shape transversal profile were mapped. These range from 0.5 to 8.3 km in length with preferred direction toward NW (azimuth 290°), in agreement with the principal structural geology in the area (NW/SE; CitationBreuer et al., 2013b). U-shaped valley widths range from 100 to 600 m.

3.2.2. Areal scouring

Areal scouring refers to areas of ice-scoured bedrock with undulating positive and negative relief. Areal scouring can feature an assemblage of streamlined bedrock features (whalebacks), stoss and lee forms (e.g. roches moutonnées) and rock basins (Rea & Evans, Citation1996). About 30% of the total ice-free land mapped corresponds to ice-scoured bedrock. In the study area, regions of scoured bedrock often include rocky basins containing shallow ponds or marshes in the hollows, with whalebacks and roches moutonnées separating them.

3.2.3. Whalebacks

Whalebacks are positive relief landforms produced in the subglacial environment and were principally identified using aerial photographs and during field work (). They are defined as bedrock knolls that have been smoothed and rounded on all sides by glacier ice (Glasser & Bennett, Citation2004). Whalebacks represent 78% of all mapped positive eroded landforms (n = 51) in the study area. Their mean perimeter polygon altitude, i.e. the base is at 126 m a.s.l., but they have been mapped up to an elevation of 669 m a.s.l. The whalebacks a-axes range between 200 and 2,300 m in length. During fieldwork whalebacks of >10 m in length were identified ().

3.2.4. Roches moutonnées

Roches Moutonnées are positive relief landforms with a pronounced asymmetric longitudinal profile, abraded slope on the stoss side and a plucked lee side indicating glacier flow direction (Glasser & Bennett, Citation2004). This clear asymmetry is not easily visible on the DEM ((d)), with confidence reached only with landforms exceeding ∼600 m in length ((f)). In contrast, with the AP stereoscopic analysis, it is possible to identify and map roches moutonnées a-axes from ∼150 m in length. When APs were unavailable (see ), we use the BI to determine whether the stoss side was abraded or plucked. A total of eighteen roches mountonées were identified between 53 and 344 m a.s.l. and the mean base altitude is 136 m a.s.l.

3.2.5. Micro-features

Glacial striations are produced by entrained subglacial sediment abrading bedrock. Chatter marks are crescentic-shaped gauges, formed by rock fragments being dragged across subglacial bedrock. Both erosional micro-features were identified in the field at elevations up to 700 m a.s.l.

3.3. Glacial depositional landforms and sediment

Glacial depositional landforms are scarce in the study area (22%). Undifferentiated glacial drift is common over bare rock and spatially related to modern glacial activity (total area coverage: 1.28 km2, see and (d)). In total, 128 glacial depositional landforms and sediment accumulations were identified and mapped (; Map).

Figure 5. Bing Satellite Image (2019) over ALOS PALSAR DEM view in 3D, east of Seno Glaciar. The terminus of glacier 007 is at ∼160 m a.s.l. (DEM elevation). Glacial meltwater is actively flowing 600 m down valley before producing a well-developed outwash plane. Northeast of Glacier 007, a frozen lake is at ∼485 m a.s.l. and a GLOF deposit is located downhill. Scoured bedrock is observed as gray polished surfaces in the whole area.

Figure 5. Bing Satellite Image (2019) over ALOS PALSAR DEM view in 3D, east of Seno Glaciar. The terminus of glacier 007 is at ∼160 m a.s.l. (DEM elevation). Glacial meltwater is actively flowing 600 m down valley before producing a well-developed outwash plane. Northeast of Glacier 007, a frozen lake is at ∼485 m a.s.l. and a GLOF deposit is located downhill. Scoured bedrock is observed as gray polished surfaces in the whole area.

Figure 6. Examples of depositional landforms. (a) High-resolution GI image north of Seno Northbrook showing spotted deposits. (b) PI image showing same site as (a) with area of kettle kame topography delimited (full line). (c) Hillshade from DEM ALOS PALSAR illuminated from 45°, south–west GCN (see for location). (d) Mapping output of (c) site. Moraine area indicated with purple hollow polygons, respective moraine crests in black lines. More than one crest inside a polygon indicates a moraine complex. Lakes in blue and glacier margins in stippled white line (see Table S1).

Figure 6. Examples of depositional landforms. (a) High-resolution GI image north of Seno Northbrook showing spotted deposits. (b) PI image showing same site as (a) with area of kettle kame topography delimited (full line). (c) Hillshade from DEM ALOS PALSAR illuminated from 45°, south–west GCN (see Figure 2 for location). (d) Mapping output of (c) site. Moraine area indicated with purple hollow polygons, respective moraine crests in black lines. More than one crest inside a polygon indicates a moraine complex. Lakes in blue and glacier margins in stippled white line (see Table S1).

3.3.1. Moraines

Ice marginal moraines are ridges formed at the lateral and/or frontal margin of glaciers, typically with asymmetric profiles (Benn & Evans, Citation2010; ). The moraines are composed of glacial till ranging between silt to boulder-sized rounded to very angular sediments. We distinguish individual moraine crests from the entire moraine complex, the latter can include more than one moraine crest. In our map, the moraine complex area and moraine crests are represented by polygons and lines, respectively ((d)). In total, 118 individual terrestrial and seven submarine moraine crests were mapped, corresponding to seventy-one moraine complexes. The majority of moraine crests/complexes cover a small area (5,400 – 400,000 m2) with a relative relief of 7–80 m between the crest and the surrounding topography. In general, the moraines crests/complexes are located in one of two locations: (I) between 2 and 10 km from ice-free cirques, with a relief of <20 m and emerging from the fjords; (II) ∼1 km down-valley from active glacier margins, located between 30 and 420 m a.s.l. with a relief of 30–60 m (e.g. moraines located in the three glacial valleys SW of the GCN; and (c,d)).

3.3.2. Kettle kame topography (KKT)

KKT is generated through supraglacial or ice-contact glaciofluvial sediment deposition around in-situ ice, wastage and ice-block melt out (Gordon & Mcewen, Citation1993) or following GLOF events (CitationIribarren et al., 2015). As the ice melts over time, a pitted topography remains. Twenty-eight KKT areas have been mapped ((a,b)) and are dispersed across the study area. The KKTs are located between 20 and 511 m a.s.l. and cover an area of 0.01–1.52 km2.

3.3.3. Outwash plains

Outwash plains are relatively flat deposits at the valley base composed of sub-rounded to rounded sediment and dissected by active/inactive fluvial processes (). A total of four outwash plains were identified. Three have active proglacial meltwater channels from GCN glaciers (). One outwash plain is located ca. 2 km from the current glacier 008 margin, indicating a former glacial still-stand down-valley, which represents the ice limit in 1942 AD (Kilian et al., Citation2007b).

4. Hydrological features

4.1. Contemporary glaciers

Present-day glaciers were mapped using the National Glacier Inventory of Chile as a reference (DGA, Citation2014). The glacier names used in the map follow the DGA numbering, excluding their shared first eight-digit prefix code CL112422 (e.g. CL112422005 = Glacier 005). Table S1 lists the glacier names used here with those from other glacier inventories. The boundaries have been updated with Sentinel 2 (IR band combination of 2017) and PSI from 2018 (). In total, 54 glaciers were mapped with surface areas ranging from 0.02 to 22.83 km2.

4.2. Fluvial channels

We differentiate fluvial channels as active or inactive according to the surface runoff observed in the remote sensing images.

4.2.1. Active rivers and streams

Present-day river activity was inferred from the images covering 2018–2019 (). Flowing water with no glacial source was considered as active and defined as river or stream depending on their respective widths (n = 1456).

4.2.2. Meltwater channels

Meltwater channels are active channels formed in the proglacial area by glacial meltwater (e.g. Izagirre et al., Citation2018; Lovell et al., Citation2011), of which 271 were identified in the study area.

4.3. Water bodies

We mapped 1637 fresh water bodies in the study area (), ranging from 3 to 2750 m2, of which 47 correspond to bedrock-floored tarns.

5. Non-glacial landforms and sediment

Several non-glacial landforms and sediment accumulations were mapped for completeness and are provided in the final map. Items mapped are marine terraces, alluvial deposits (Gutiérrez-Elorza, Citation2008), landslides (Hungr et al., Citation2014) and peat bogs. More detailed differentiation of non-glacial deposits is beyond the scope of this work.

6. Geology

We provide the only geological map available of the study area as a shape file in the supplemental materials (scale: 1:1,000,0000; SERNAGEOMIN, Citation2003). It is outwith the scope of this paper to create a more detailed geological map. The local geology is dominated by Cretacious intrusives, mainly tonalites, diorites and granodiorites. Jurassic-Cretacious mafic complexes outcrop locally (see supplemental material). The principal structural control in the area corresponds to the NW/SE Magallanes–Fagnano lateral slip fault system which controls the common structural lineaments’ orientation (CitationBreuer et al., 2007b). Observations in the field and remote sensing analysis were used to establish a better overlap and relationship between the local geology and the glacial landforms discussed.

7. Discussion

In terms of methodology where precise changes in the relief needed to be identified (e.g. discriminating between whalebacks and roches mountonnées), the DEM and 3D visor GE-v7.0 were used together (). However, when comparing the output to aerial photograph (AP) stereographic analysis, it became clear that the DEM and 3D GE visor overestimate the number of whalebacks and underestimated the number of roches moutonnées in the study area. The resolution of the DEM and 3D GE visor hampers the clear discrimination between both landforms; thus, only through the use of the APs could landforms be accurately mapped. We also used the very high-resolution BI images () to discriminate if the stoss side looked abraded (smooth) or plucked (high presence of fractures and shadows, and lack of detrital material). This is a time-consuming method but produces higher confidence in landform discrimination and final geomorphic map output.

From our map, it is clear that the peninsulas and islands located between the GCN and the EDM have been impacted by late Pleistocene glacial expansion and recession to varying degrees. Glacial erosional landforms account for 78% of all mapped features. From micro-scale striations and chatter marks to meso-scale whalebacks and roches moutonnées to macro-scale aerial scouring of bedrock, the occurrence of these features indicates efficient subglacial erosion due to warm-based, debris loaded, potentially fast-flowing ice. Glacier retreat was likely rapid and continuous due to a relative lack of marine and terrestrial depositional landforms marking glacier stabilization (28× kame and kettle topography, 71× moraine complex, 5× outwash plains; see Map).

Meso-scale glacial erosional landforms in the study area are dominated by whalebacks (74%) and roches moutonnées (26%). CitationKrabbendam and Glasser (Citation2011) suggest that lithology (hardness) and joint spacing exerts a strong control on the distribution of whalebacks and roches moutonnées. In our study area, 67% of whalebacks and 67% of roches moutonnées occur on harder intrusive granitoids and 33% of each landform on softer mafic rocks. The lack of lithological preference for either landform suggests that lithology does not exert a strong control on landform distribution in the fjords of southwestern Chile. To investigate the influence of joint spacing on landform distribution requires a more detailed analysis of the structural geology and paleo-channel distribution, which is beyond the scope of this work.

The distribution of whalebacks and roches mountonnées may represent different subglacial conditions. Whalebacks are generally associated with warm-based thicker ice, low sliding velocities and available basal meltwater, whereas roches moutonnées preferentially form underneath warm-based thin fast-flowing ice (Hallet, Citation1996), with abundant subglacial meltwater (Glasser & Bennett, Citation2004). Whalebacks were mapped up to 700 m a.s.l. whilst roches moutonnées were only identified up to 344 m a.s.l. We hypothesis that each landform is associated with a different glacier flow regime, either during the same or multiple glacial cycles. Whalebacks were likely produced when ice cover in the fjords was more extensive, i.e. thicker, whilst the roches moutonnées were formed during phases of thinner ice. Such thinner ice likely occupied the area during the last glacial to de-glacial transition, potentially exacerbated by the de-glacial marine transgression (∼14 ka BP; CitationKilian et al., 2007a), leading to potentially thinner fast-flowing outlet glaciers from the Patagonian Ice Sheet.

8. Conclusions

  • We present the first terrestrial glacial geomorphic map between the Gran Campo Nevado and EDM (52° to 53°S), to address the data gap in reconstructing Patagonian Ice Sheet dynamics west of the Cordillera de los Andes in southwestern Patagonia.

  • All features were mapped manually without automatic mapping procedures, eliminating the errors related to automation and increasing our mapping accuracy using a number of different remote sensing products.

  • In total 4290 individual features were mapped in the study area (1565 km2) of which 862 are directly related to glacial activity. The most relevant are:125 terrestrial and submarine moraine crests, 71 moraine complexes, 70 cirques, 51 whalebacks, 40 scarps, 28 kettle kame topography, 28 U-shaped valleys and 18 roches moutonnées,

  • The spatial distribution of whalebacks and roches moutonnées indicates a lack of lithological control on their formation, which may alternatively be related to glacier bed conditions and/or joint spacing.

  • Glacial erosional landforms dominate over depositional landforms indicating a warm-based, sediment laden and meltwater-rich subglacial environment. In addition, the occurrence of whalebacks and roches moutonnées suggests a dynamic and changing ice velocity and thickness regime during Patagonian Ice Sheet cover and retreat.

Software

We use Sentinel Application Platform (SNAP, v.5.0) by ESA to work with Sentinel data sets. Google Earth Pro 7.3.2 (©2019 Google LLC) was useful to observe different perspectives of landforms. Finally, all mapping and data manipulation were conducted in the Open Source Geospatial Foundation Project software QGIS 3.280 [https://qgis.org] while the final map design was improved in Adobe Illustrator (AI).

Open scholarship

This article has earned the Center for Open Science badge for Open Data. The data are openly accessible at http://dx.doi.org/10.5525/gla.researchdata.1384

Supplemental material

Supplemental Material

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Supplemental Material

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Acknowledgements

Special thanks go out to Captain Hugo Cardenas and the entire Mary Paz II crew for making nearly everything possible, Juan-Carlos Aravena and Marcelo Arevalo for logistical support at Universidad de Magallanes and in Punta Arenas, and everyone who helped during fieldwork preparations in Santiago and Punta Arenas. We would also like to thank the thorough and thoughtful comments provided by reviewers Federico Ponce, Andy Hein, Thomas Pingle and associate editor Jasper Knight which considerably improved the manuscript.

Disclosure statement

No potential conflict of interest was reported by the author(s).

Data availability statement

The data that support the findings of this study are available from the Glasgow University online repository at the following link: https://dx.doi.org/10.5525/gla.researchdata.1384. The primary data has the following license: CC-BY-SA. See supplemental materials for further information.

Correction Statement

This article has been corrected with minor changes. These changes do not impact the academic content of the article.

Additional information

Funding

This study was supported by research grants from the Royal Geographical Society with IBG, British Society for Geomorphology, Quaternary Research Association, FONDECYT [grant number 3170869], and a Hanse-Wissenschaftskolleg Institute for Advanced Studies Junior Fellowship awarded to A.J.G.; FONDECYT [grant number 1161110] of J-L.G & A.J.G.; University of Liverpool Early Career Researchers Grant awarded to R.K.S. We would like to thank AMG Group for sponsoring field gear for the #ChileFjords18 expedition.

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