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Downloaded By: [Swets Content Distribution] At: 10:00 20 June 2007 Younger Dryas cirque glaciers in western Spitsbergen: smaller than during the Little Ice Age JAN MANGERUDAND JON Y. LANDVIK BOREAS Mangerud, J. & Landvik, J. Y. 2007 (July): Younger Dryas cirque glaciers in western Spitsbergen: smaller than during the Little Ice Age. Boreas, Vol. 36, pp. 278 285. Oslo. ISSN 0300-9483. The outermost moraines in front of the Scottbreen glacier in Spitsbergen date from c. AD 1900. These moraines rest on top of a marine shoreline radiocarbon-dated to about 11 200 14 C yr BP and demonstrate that the AD-1900 moraines show the maximum glacier extent since late Allerød time. This means that Scottbreen was smaller during the Younger Dryas than at AD 1900, in contrast with glaciers on mainlandwestern Europe, which were all much largerduring the Younger Dryas. The explanation is probably starvation of precipitation on western Spitsbergen during the Younger Dryas. In contrast, ice sheets and glaciers in Spitsbergen reacted moreor less in concert with glaciers in western Europe, during the global Last Glacial Maximum and the Little Ice Age. Jan Mangerud (e-mail: [email protected]), Department of Earth Science and Bjerknes Centre for Climate Research, University of Bergen, Alle ´gt. 41, NO-5007 Bergen, Norway; Jon Y. Landvik (e-mail: jon.landvik@ umb.no), Norwegian University of Life Sciences, Department of Plant and Environmental Sciences, P.O.Box 5003, NO-1432 A ˚ s, Norway; received 11th August 2006, accepted 31st October 2006. The Younger Dryas (YD) in western Europe, i.e. downwind of the North Atlantic, is characterized by extensive glacier growth, and all glaciers were much larger during the YD than at any time during the Holocene (Gray & Coxon 1991; Andersen et al. 1995; Kerschner et al. 2000; Geirsdottir 2004; Denton et al. 2005). On the other hand, further north along the same seaboard the opposite situation has been reported, i.e. that glaciers on western Spitsbergen were smaller during the YD than during the Little Ice Age (LIA) (Salvigsen 1979; Mangerud & Svendsen 1990; Svendsen & Mangerud 1992). However, this has been documented at only a few sites. During the Last Glacial Maximum (LGM), the Barents ( Svalbard) Ice Sheet reached the shelf edge west of our study site (Fig. 1) (Landvik et al. 1998). The ice margin retreat started about 15 000 14 C yr BP and the study area became ice-free at about 12 000 14 C yr BP (Landvik et al. 1992; Mangerud et al. 1992). The deglaciation dates of 12 830 and 12 570 14 C yr BP (T-6000 and Ua-280), performed on sediment-feeding molluscs collected close to Scottbreen, are now con- sidered to be too old (Mangerud et al. 2006). In this paper we present radiocarbon dates demon- strating that Scottbreen, a cirque glacier on the west coast of Spitsbergen in the Svalbard archipelago (Figs 1, 2), was smaller during the YD than during its LIA maximum extent at c. AD 1900. Study area and observations Svalbard is located at 77 808N. The archipelago is therefore characterized by an arctic climate, and about 60% of the land area is covered by glaciers (Fig. 1) (Hagen et al. 1993). However, because of advection of warm Atlantic water and southwesterly winds, the climate, in particular the winter climate, is exception- ally warm compared with other areas at this latitude. At Isfjord Radio, located on the coast 55 km north of Scottbreen (Fig. 1), the mean annual temperature (1961 1990) is /5.18C (Førland et al. 1997). The means for the coldest and warmest months are /12.48C and /4.88C, respectively. At Sveagruva, situated some 70 km inland, the corresponding tem- peratures are /7.18C, /17.08C and /5.88C, respec- tively. Annual precipitation is 480 mm at Isfjord and 260 mm at Sveagruva (Førland et al. 1997). Scottbreen (‘breen’ /glacier) (77833?N, 14822?E) is a 4.4-km long cirque glacier stretching from 700 to 90 m a.s.l. (Hagen et al. 1993). It is located close to the open ocean on the west coast of Spitsbergen (Figs 1, 2). The regional equilibrium line altitude (ELA) for glaciers along this coast is /400 m a.s.l. (Hagen et al. 2003a, b) and the present Scottbreen ELA is estimated to be 450 500 m a.s.l. (J. O. Hagen, pers. comm. 2006). In front of the glacier there is a belt of up to 50 60-m high ice-cored end moraines (Figs 3, 4) that were clearly formed during the LIA. Oblique air photographs from 1936 (Fig. 2) show that the glacier reached the proximal slope of the outermost moraine at that time (Norsk Polarinstitutt, S36, photographs 1694 and 3189). The small glaciers on western Spitsbergen generally reached their maximum LIA position around AD 1900 (Hagen & Liestøl 1990; Lefauconnier & Hagen 1990) and this was probably the case for Scottbreen. The present ice margin is some 800 m behind the LIA moraine, and the lower part of the DOI 10.1080/03009480601134827 # 2007 Taylor & Francis

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Page 1: Younger Dryas cirque glaciers in western …oi/AG-326 2006 readings/Svalbard...Downloaded By: [Swets Content Distribution] At: 10:00 20 June 2007 Younger Dryas cirque glaciers in western

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Younger Dryas cirque glaciers in western Spitsbergen: smaller thanduring the Little Ice Age

JAN MANGERUD AND JON Y. LANDVIK

BOREAS Mangerud, J. & Landvik, J. Y. 2007 (July): Younger Dryas cirque glaciers in western Spitsbergen: smaller thanduring the Little Ice Age. Boreas, Vol. 36, pp. 278�285. Oslo. ISSN 0300-9483.

The outermost moraines in front of the Scottbreen glacier in Spitsbergen date from c. AD 1900. These morainesrest on top of a marine shoreline radiocarbon-dated to about 11 200 14C yr BP and demonstrate that the AD-1900moraines show the maximum glacier extent since late Allerød time. This means that Scottbreen was smaller duringthe Younger Dryas than at AD 1900, in contrast with glaciers on mainland western Europe, which were all muchlarger during the Younger Dryas. The explanation is probably starvation of precipitation on western Spitsbergenduring the Younger Dryas. In contrast, ice sheets and glaciers in Spitsbergen reacted more or less in concert withglaciers in western Europe, during the global Last Glacial Maximum and the Little Ice Age.

Jan Mangerud (e-mail: [email protected]), Department of Earth Science and Bjerknes Centre for ClimateResearch, University of Bergen, Allegt. 41, NO-5007 Bergen, Norway; Jon Y. Landvik (e-mail: [email protected]), Norwegian University of Life Sciences, Department of Plant and Environmental Sciences, P.O. Box 5003,NO-1432 As, Norway; received 11th August 2006, accepted 31st October 2006.

The Younger Dryas (YD) in western Europe, i.e.downwind of the North Atlantic, is characterized byextensive glacier growth, and all glaciers were muchlarger during the YD than at any time during theHolocene (Gray & Coxon 1991; Andersen et al. 1995;Kerschner et al. 2000; Geirsdottir 2004; Denton et al.2005). On the other hand, further north along the sameseaboard the opposite situation has been reported,i.e. that glaciers on western Spitsbergen were smallerduring the YD than during the Little Ice Age(LIA) (Salvigsen 1979; Mangerud & Svendsen 1990;Svendsen & Mangerud 1992). However, this has beendocumented at only a few sites.

During the Last Glacial Maximum (LGM), theBarents (�Svalbard) Ice Sheet reached the shelf edgewest of our study site (Fig. 1) (Landvik et al. 1998). Theice margin retreat started about 15 000 14C yr BP andthe study area became ice-free at about 12 000 14C yrBP (Landvik et al. 1992; Mangerud et al. 1992). Thedeglaciation dates of 12 830 and 12 570 14C yr BP(T-6000 and Ua-280), performed on sediment-feedingmolluscs collected close to Scottbreen, are now con-sidered to be too old (Mangerud et al. 2006).

In this paper we present radiocarbon dates demon-strating that Scottbreen, a cirque glacier on thewest coast of Spitsbergen in the Svalbard archipelago(Figs 1, 2), was smaller during the YD than during itsLIA maximum extent at c. AD 1900.

Study area and observations

Svalbard is located at 77�808N. The archipelago istherefore characterized by an arctic climate, and about

60% of the land area is covered by glaciers (Fig. 1)(Hagen et al. 1993). However, because of advection ofwarm Atlantic water and southwesterly winds, theclimate, in particular the winter climate, is exception-ally warm compared with other areas at this latitude.At Isfjord Radio, located on the coast 55 km north ofScottbreen (Fig. 1), the mean annual temperature(1961�1990) is �/5.18C (Førland et al. 1997). Themeans for the coldest and warmest months are�/12.48C and �/4.88C, respectively. At Sveagruva,situated some 70 km inland, the corresponding tem-peratures are �/7.18C, �/17.08C and �/5.88C, respec-tively. Annual precipitation is 480 mm at Isfjord and260 mm at Sveagruva (Førland et al. 1997).

Scottbreen (‘breen’�/glacier) (77833?N, 14822?E) is a4.4-km long cirque glacier stretching from 700 to 90 ma.s.l. (Hagen et al. 1993). It is located close to the openocean on the west coast of Spitsbergen (Figs 1, 2). Theregional equilibrium line altitude (ELA) for glaciersalong this coast is�/400 m a.s.l. (Hagen et al. 2003a, b)and the present Scottbreen ELA is estimated to be450�500 m a.s.l. (J. O. Hagen, pers. comm. 2006). Infront of the glacier there is a belt of up to 50�60-m highice-cored end moraines (Figs 3, 4) that were clearlyformed during the LIA. Oblique air photographs from1936 (Fig. 2) show that the glacier reached theproximal slope of the outermost moraine at that time(Norsk Polarinstitutt, S36, photographs 1694 and3189). The small glaciers on western Spitsbergengenerally reached their maximum LIA position aroundAD 1900 (Hagen & Liestøl 1990; Lefauconnier &Hagen 1990) and this was probably the case forScottbreen. The present ice margin is some 800 mbehind the LIA moraine, and the lower part of the

DOI 10.1080/03009480601134827 # 2007 Taylor & Francis

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glacier has a significantly lower surface slope thanshown on the air photographs from 1936.

Most important for the present discussion is that thedistal part of the LIA moraine was deposited on top

of a well preserved beach terrace of about 57 m a.s.l.(Figs 4, 5). Thus the LIA moraine shows the maximumextent of Scottbreen after the formation of this terrace,which, as we will demonstrate, is of Allerød age.

Fig. 1. The inset map shows the location of Svalbard. Present-day glaciers are shown in white on the main map. The maximum extent (LastGlacial Maximum�/LGM) of the Barents Ice Sheet is shown beyond the west coast (Landvik et al. 1998; Ottesen et al. 2005). Theapproximate limit of the Younger Dryas ice sheet on Svalbard (modified from Svendsen et al. 2004) is indicated as a line separatingdeglaciation dates of Younger Dryas and early Holocene ages. We assume errors rarely exceeded 30 km along the west coast. In the easternareas the ice margin was beyond the coast and cores with relevant dates were only obtained from far out in the Barents Sea. Therefore the lineis more generalized here and errors may exceed 100 km. Norwegian Polar Institute, digital map.

BOREAS 36 (2007) Younger Dryas cirque glaciers in western Spitsbergen 279

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The beach terraces in front of Scottbreen aredissected by meltwater channels from the glacier(Figs 3, 4) that have exposed sandy gravelly beachdeposits with shell fragments, predominantly of Myatruncata. Four radiocarbon dates from the molluscshells have yielded uncorrected ages in the range of11 6259/50 to 11 7509/80 14C yr BP (Table 1). Assum-ing a marine reservoir age of 440 years, which is thestandard used for Svalbard (Mangerud & Gulliksen1975), the corrected ages are in the range 11 185�11 310 14C yr BP, i.e. a late Allerød age. A new estimateof the present-day reservoir age of 3809/80 (Mangerudet al. 2006) indicates that the ages are slightly older.Precise Allerød�YD reservoir ages have not beendetermined from Svalbard, but three pairs of molluscshell/driftwood dates from eastern Svalbard coveringthe period 7000�9200 14C yr BP gave reservoir ages ofabout 400 years (J. Mangerud, unpublished). Along the

west coast of Norway the reservoir age was also closeto the present day during most of the Allerød, andsome 300 years higher during parts of the YD(Bondevik et al. 2006). We conclude that the datesindicate a late Allerød or possibly an early YD age forthe shells.

In theory, the molluscs may have lived at severalmetres of water depth or they may have been redepos-ited from higher and older terraces. If so, the 57-mterrace could be younger than the shells. However, thesouthern flank of the moraine cross-cuts a distinctbeach terrace at 61 m a.s.l. as well as beach sedimentsat 66 m a.s.l. According to a relative sea level curvefrom the area immediately to the west (Salvigsen et al.1991), the latter altitude represents the marine limitdated to c. 12 000 14C yr BP and the 57-m terracerepresents a late Allerød sea level, and thus supportsour inference that the shells accurately date the terrace.

Fig. 2. Oblique air photo of Scottbreen (Fig. 1) taken on 28th July 1936, approximately towards the southwest. The arrow shows the locationof Fig. 4. Norwegian Polar Institute, photograph no. S36-1694.

280 Jan Mangerud and Jon Y. Landvik BOREAS 36 (2007)

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Fig. 3. Scottbreen with the large Little Ice Age moraines (oblique arrows). As seen from Fig. 2, the glacier front reached the foot of thismoraine as late as 1936. The vertical arrow indicates the dated marine terrace overrun by the glacier (Fig. 4). Younger terraces are seen ashorizontal lines below. Photograph taken 27th August 2002.

Fig. 4. The person is standing on the Allerød-age shoreline, 57 m a.s.l. The dated shells were found by excavating this terrace. The Little IceAge moraine is seen on top of the terrace to the right of the person, and as the large ridge behind and to the left of the person. The glacier islocated to the right of the photograph.

BOREAS 36 (2007) Younger Dryas cirque glaciers in western Spitsbergen 281

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The marine limit was formed during the deglaciation ofthe Barents�Svalbard Ice Sheet (Landvik et al. 1987;Mangerud et al. 1992), meaning that Scottbreenremained inside the position of the LIA morainesfrom the deglaciation at about 12 000 14C yr BP untilabout AD 1900, i.e. also during the YD.

Discussion

One question arising is whether Scottbreen couldhave been cold-based during the YD and overrun theterrace without depositing any till. Today, a noticeablepart of the bouldery material deposited by the glacieris debris originating from rock falls from the steepmountain slopes onto the glacier surface, a supply thatmust have existed even if the glacier was cold-based.However, we could not find any such debris on topof the terraces and we consider it unlikely that theglacier overran the terrace without depositing at leastsome blocks from englacial or supraglacial transport.

During the YD, a remnant of the Barents�SvalbardIce Sheet still covered much of Svalbard further to theeast (Fig. 1) (Landvik et al. 1998; Svendsen et al. 2004).In that sense the glacial history of Svalbard is similar tothe development in Scandinavia, Scotland and the

Alps, where ice sheets or ice caps also existed duringthe YD. However, there are two major differences inthe glacial behaviour.

First, prominent YD moraines have not been foundon Svalbard, even if a slow-down in glacio-isostaticrebound indicates that the retreat of the ice sheet halted(Landvik et al. 1987, 1998). The YD ice sheet extent inFig. 1 is mainly mapped as the up-fjord limit of YDshorelines and from the distribution of deglaciationages in stratigraphical successions (Mangerud et al.1992). A probable reason for the lack of YD morainesis simply that the ice sheet over Svalbard did not re-advance towards the west, in contrast with theScandinavian, Scottish and Alp ice sheets/ice caps.The last ice sheet over Svalbard comprised fast-flowingice along the fjords and less dynamic, possibly cold-based, ice between these ice streams (Landvik et al.2005). Thus any moraines formed during the YD maybe confined to the floors of fjords or even to valleyspresently occupied by fjord-head glaciers. Some mor-aines of postulated YD age, and interpreted as theresult of a glacial re-advance, have indeed beendescribed recently from the floors of Isfjorden and itstributaries (Forwick & Vorren 2005).

Second is the difference demonstrated in this paperand earlier by Salvigsen (1979), Mangerud & Svendsen

Table 1. Radiocarbon dates from the marine terrace in front of the Scottbreen Little Ice Age moraine. All dates were performed on fragmentsof marine shells, probably Mya truncata. d13C was not measured but a value of 1.0� rel. PDB was assumed and used for correction. Thereservoir age is according to Mangerud & Gulliksen (1975).

Field sample no. Lab. no. 14C ageAssumedreservoir age

Reservoirage-corrected 14C age

JM1995-12a Tua-4270 11 7509/80 440 11 3109/80JM1995-12b Tua-4271 11 7609/70 440 11 3209/70JM1995-12c Tua-4272 11 6509/50 440 11 2109/50JM1995-12d Tua-4273 11 6259/50 440 11 1859/50

±±±±

A B

Fig. 5. A. Longitudinal profile of Scottbreen drawn from the 1:100 000 map sheet Van Keulenfjorden, which was constructed from airphotographs taken in 1936 and has contour intervals of 50 m. Issued by Norsk Polarinstitutt 1985. B. Stratigraphical relationship between thedated shoreline and the Little Ice Age moraine. The radiocarbon dates are corrected for a marine reservoir age of 440 years.

282 Jan Mangerud and Jon Y. Landvik BOREAS 36 (2007)

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(1990) and Svendsen & Mangerud (1992), that gla-ciers located west of the ice sheet on Svalbard(Fig. 1) were smaller during the YD than the LIA.In contrast, all glaciers in western Europe were, asalready mentioned, much larger during the YD thanLIA (Fig. 6). The surprisingly small YD glaciers onSvalbard could be the result of warm summers and/orlimited precipitation (snowfall). The YD summerinsolation at this latitude was about 10% higher thantoday (Berger & Loutre 1991), but this was also thecase for northern Scandinavia and therefore it cannotexplain the difference in glacial response between thetwo areas. Unfortunately, there are no observations onSvalbard that can be used to construct the YD summertemperatures but, according to a compilation by Birkset al. (2005), the summer sea surface temperaturessouth of Svalbard were 2�108C colder than today. It istherefore reasonable to assume that summers werecolder on Svalbard too, and we conclude that theglaciers on western Svalbard remained small be-cause of limited snow accumulation. Regional glacierre-advances in northern Norway during the YD(Andersen et al. 1995; Vorren & Plassen 2002) showthat the latitudinal boundary between the dry climatefavouring glacier starvation and the climate withenough precipitation for glacial advances was locatedbetween Svalbard and the northern tip of Norway(Fig. 6). The explanation for the dry climate may be thehypothesis proposed by Birgel & Hass (2004): prevail-ing easterly winds over Svalbard during the YD.Western Svalbard would then be in the precipitationshadow, whereas there would be more precipitation ineastern Svalbard and the Barents Sea. This pattern isconsistent with the snow accumulation postulated fromthe slow-down of isostatic rebound, as mentionedabove. This is also consistent with modelling experi-ments that produce a YD air pressure pattern givingwesterly winds over all of Scandinavia and east-erly winds over Svalbard, particularly during winter(Renssen et al. 2001).

The YD glaciers in northwest Europe were mainlyfed by precipitation brought in with westerly or south-erly winds from the Atlantic Ocean and the Nordic seas

(Sissons 1980; Larsen et al. 1984). However, it is clearthat the glacial re-advances that took place across sucha large and climatically diverse region as westernEurope and Iceland were mainly caused by coldsummers. Precipitation differences would regionallymodify the large-scale pattern, as in Scotland whereglaciers grew in the west whereas the east was in theprecipitation shadow (Gray & Coxon 1991). Benn &Lukas (2006) found that precipitation in northwestScotland was c. 26% higher during the YD than today,whereas in the mountains further east it was close topresent-day levels (Benn & Ballantyne 2005). TheScandinavian Ice Sheet had its largest growth in itssouthwest sector, as a result of the underlying topo-graphy (Mangerud 1980) and, perhaps more impor-tantly, a larger winter precipitation than in other areas(Mangerud 2004). In our interpretation, Svalbardwould be almost a mirror image of Scotland: an icecap in the east and a precipitation shadow in the west.

The glaciers on Svalbard and the Barents Sea grew inconcert with the Scandinavian, British and Alp glaciersduring the period before and around the global LGM(Landvik et al. 1998), in contrast with what we havedescribed for the YD. This could indicate differenttypes of glacial climates between the two cold periods.However, it should be borne in mind that YD was ashort period of about 1300 yr, whereas the LGM wasalmost 10 times longer when the period of ice build-upis included. Conditions for snow accumulation couldtherefore have varied over time during the LGM.Nevertheless, if precipitation was the main factorcausing the difference between mainland Europe andSvalbard during the YD, then less difference in theprecipitation pattern during the LGM ice growthwould be expected. Open water, at least periodicallyand during summers, has been described during theLGM in the North Atlantic and the Norwegian Sea asa source for precipitation on the Scandinavian andBarents ice sheets (Hebbeln et al. 1994; Hald et al.2001). However, open waters have also been reportedfor the YD (Koc et al. 1993; Birgel & Hass 2004)and were probably required for the ice growth inScandinavia.

ELA

dep

ress

ion

(m)

4000 km

Fig. 6. Estimation of how muchlower the equilibrium line altitude(ELA) was during the Little IceAge and the Younger Dryas relativeto the present day ELA. Note thevery different situation inSpitsbergen compared withmainland western Europe.Modified from Mangerud &Svendsen (1990) and Svendsen &Mangerud (1992).

BOREAS 36 (2007) Younger Dryas cirque glaciers in western Spitsbergen 283

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Conclusions

. Scottbreen and other glaciers on western Spitsber-gen were smaller during the YD than the LIA(c. AD 1900), in contrast with all glaciers in westernEurope.

. The explanation for the small YD glaciers inSpitsbergen is starvation of precipitation (snowfall),although higher insolation may have contributed toincreased summer melting.

Acknowledgements. � J. M. thanks co-leaders and students on theUNIS excursion 1995 for help in digging and finding molluscs. Wealso thank John Inge Svendsen and Øystein Lohne, who gave criticalcomments on an earlier version of the manuscript, Jane Ellingsen,who completed the drawings, and Mike Talbot, who corrected theEnglish language. Comments from the journals editor, Jan A.Piotrowski, and reviewers, Jon Ove Hagen and Matthias Forwick,also improved the manuscript and are appreciated.

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