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HindawiPublishingCorporation JournalofGeologicalResearch Volume2011,ArticleID247983,11pages doi:10.1155/2011/247983 Research Article Thessaloniki Mud Volcano, the Shallowest Gas Hydrate-Bearing Mud Volcano in the Anaximander Mountains, Eastern Mediterranean C.Perissoratis,1Chr.Ioakim,1S.Alexandri,2J.Woodside,3P.Nomikou,2A.Da¨hlmann,4 D.Casas,5K.Heeschen,6H.Amman,7G.Rousakis,2andV.Lykousis2 1InstituteofGeologyandMineralExploration,EntranceC,SpyrouLouis1,OlympicVillage,Acharne,13677Athens,Greece 2HellenicCentreforMarineResearch,46thkmAthens-SounionBP712,19013Anavyssos,Greece 3Department of Sedimentary and Marine Geology, Vrije Universiteit Amsterdam, De Boelelaan 1085, 1081 HV Amsterdam, The Netherlands 4DepartmentofGeochemistry,FacultyofEarthSciences,UtrechtUniversity,80021Budapestla-an4,3508TAUtrecht,TheNetherlands 5InstitutdeSciencesdelMar,PaseoMaritimodelaBarceloneta37-49,08003Barcelona,Spain 6Bundesanstaltfu¨rGeowissenschaftenundRohstoffeGeozentrumHannover,Stilleweg2,D-30655Hannover,Germany 7TechnischeUniversita¨tBerlin,MullervBresslauStrasse,10623Berlin,Germany CorrespondenceshouldbeaddressedtoC.Perissoratis,[email protected] Received2June2011;Revised16August2011;Accepted12September2011 AcademicEditor:MichelaGiustiniani Copyright©2011C.Perissoratisetal.ThisisanopenaccessarticledistributedundertheCreativeCommonsAttributionLicense, whichpermitsunrestricteduse,distribution,andreproductioninanymedium,providedtheoriginalworkisproperlycited. A detailed multibeam survey and the subsequent gravity coring carried out in the Anaximander Mountains, Eastern Mediterranean, detected a new active gas hydrate-bearing mud volcano (MV) that was named Thessaloniki. It is outlined by the1315mbathymetriccontour,is1.67km2 inarea,andhasasummitdepthof1260m.Theseabottomwatertemperatureis 13.7◦C.Thegashydratecrystalsgenerallyhavetheformofflakesorrice,somelargeraggregatesofthemareupto2cmacross. A pressure core taken at the site contained 3.1 lt. of hydrocarbon gases composed of methane, nearly devoid of propane and butane.Thesedimenthadagashydrateoccupancyof0.7%ofthecorevolume.Thesecharacteristicsplacethegashydratefieldat ThessalonikiMVattheupperboundaryofthegashydratestabilityzone,pronetodissociationwiththeslightestincreaseinsea watertemperature,decreaseinhydrostaticpressure,orchangeinthetemperatureoftheadvectingfluids. 1.Introduction:PurposeofThisStudy theirdiscoveryinthelate1970s[13].Mudvolcanoesarealso known for their high methane fluxes, advecting methane- The occurrence of mud volcanoes (MVs), mud diapirs, richfluidsatseafloorseeps,gashydrates,andfavorableenvi- and fluid seeps has long been known in various different ronmentsforchemosyntheticsymbioticfauna[5,10,12]. geological environments of the Eastern Mediterranean [1] The Anaximander Mountains are situated between the and in the Aegean Sea [2]. They occur not only in regions Hellenic and Cyprus Arcs at the junction of the African of compressional stress present in subduction zones (e.g., Plate with the Anatolian and the Aegean microplates, Calabrian Arc [3], Mediterranean Ridge [4], and orogenic an area accommodating the relative motion between the belts[1,5–7]),butalsoonpassiveriftedmarginssuchasthe African and Eurasian plates [6,10,14]. The mountains Egyptianoffshore[8,9]andareasofmixedtectonicsignature have thus undergone a complex deformation including liketheANAXIMANDERMountainswheremudvolcanism southwarddirectedthrusting,northeast-southwestshearing is related to faults with normal and transcurrent faulting in the west (Strabo Trough trend) and northwest-southeast components [10–12]. Especially the accretionary prism of shearingintheeast(FlorenceRisetrend),andcross-cutting the Hellenic Arc (Mediterranean Ridge) is an area where a normal faulting, all defining the current structure of the largenumberofmudvolcanoeshavebeenstudiedfollowing mountains [10,12,15,16]. They are comprised of three 2 JournalofGeologicalResearch mainseamounts:Anaximander,Anaximenes,andAnaxago- deck the autoclave corer was placed upright for controlled ras(Figure1(a)). degassing and kept in an ice bath to prevent warming The setting of the Anaximander Mountains is clearly to deck temperatures. The degassing, gas collection, and favorable for the occurrence of mud volcanoes (Figure1) gas-subsampling were carried out using a valve system as thanks to the presence of overpressured fluids and faults described by Heeschen et al. [19], a method used and that act as conduits for the fluids to escape [12, 17, 18]. described also by others [18]. The pressure was constantly Discovered during the Dutch ANAXIPROBE project by monitored and the increasing volume of released gas was multibeam surveying in 1995, seven large mud volcanoes read off from a converted graduated cylinder. Gas sub- were sampled in 1996 [6, 7, 11] when the first gas hydrates samples were taken via a three-port valve and were stored samplesintheMediterraneanSeawerecollectedfromKula for analysis in the laboratory [22]. A total of four gravity MV. By 2002 the Amsterdam and Kazan MVs were also cores and one autoclave core were collected at Thessaloniki discovered to have hydrates. Between 2003 and 2005 the MV (Figure2, Table1). The trace and main elements were EC-funded project ANAXIMANDER targeted these mud analyzedbytheX-raydiffractionmethodusingaSIEMENS volcanoes in a study of the gas hydrates and associated D-500 instrument. The crystalline phases were determined deep biosphere in the area, and this was followed by the using the Joint Committee Power Diffraction Standards HERMES project (2005–2009). During these projects gas and their final semiquantitative analyses by using the EVA hydrates from Amsterdam and Kazan MVs were collected programfromSiemens/Bruker/Socabimo. and studied, and two new mud volcanoes named Athina andThessalonikiwerealsodiscovered,sampled,andstudied 3.ResultsandDiscussion (Figure1(b)[17,19–21]). Since Thessaloniki MV is the shallowest known GH 3.1. Bathymetry and Backscattering Imaging. Anaximenes bearing MV in the Eastern Mediterranean, very briefly Mountain (Figure1) is a slightly northwestward concave describedearlier[17,21],thepurposeofthisstudyistocarry feature occupying the shallowest (680m) and smallest area outdetailedanalysesandexaminationofalldatacollectedin in the Anaximander Complex, and therefore is character- thisareaanddiscusstheconditionsandcharacteristicsofthe ized by steep slopes and rugged relief. To the south the GHpresent. Mediterranean Ridge is terminated in the form of a flat slightly wavy or folded area lying at a water depth of about 2.MaterialsandMethods 2800m. It is separated from Anaximenes Mountain by a deep valley (>3000m). The study of the combined 3D The data examined in this study were acquired mainly seabed morphology and backscatter intensity revealed in during two cruises of the R/V Aegaeo in May 2003 and the southeastern slope of Anaximenes Mountain numerous October-November 2004. During the first cruise detailed dome-like morphological features with strong backscatter swath bathymetry and backscatter imagery of the study thatconstitutepotentialmudvolcanosites.Followingimage area was obtained using a hull-mounted SEABEAM 2120 processing of the backscatter data, a number of high swath system operating at 20KHz. It has an angular sector backscatter areas implying potential active mud volcanism of 150◦, with 159 beams and a swath width from 7.5- to wereidentified.Oneofthesesitesatadepthof1798mwas 11.5- times the water depth, for depths from 1 to 5km subsequently surveyed in 2003 and discovered to be a mud respectively. Navigation was carried out with a Trimble volcano which was named Athina MV (Figure1, [17, 20]). 4000 GPS providing the ships position to within ±10m. Inthesamearea,about9kmnortheastofAthinaMV(at35◦ The bathymetric map of Thessaloniki MV (Figure2) was 28.60N–30◦15.06E),andatwaterdepthsbetween1320and produced using a 20m grid interval and plotted with a 1260mtheThessalonikiMVwasdiscoveredaftersurveying Mercatorprojectionatascaleof1:20.000with5mcontours. andsamplinginNovember2004(Figures1and2[17,21]). Sediment was sampled with a 3m long 73cm i.d. Benthos Thismudvolcanohadnotbeenfullyexaminedinprevious InstrumentsGravityCorerwithpresplitsleevestoreducethe cruisesbecauseofitssmallsizeandlocationatthebaseofa timeneededtoopenandsamplethecores.Thetimebetween very steep sloping cliff (Figure2), although its eastern side coring the seafloor and on board sampling of cores from was crossed during the ANAXIPROBE ORETech side scan a depth of 2000m was thus reduced to between 20 and 25 survey [7] (Figure2). It is an oval submarine hill with its minutestoensuretheleastpossiblegashydratedissociation long axis about 1750m as defined by the 1315m isobath, andsedimentdistortion.Assoonasthecoreswereopened, withsteepnorthernandeasternslopesandanareaofabout the temperature of the sediments was measured, and any 1.67km2. In the inner part, near the summit, it becomes gashydrateswerecollectedandplacedinafreezerat–70◦C. morecircularwherethreepeaksaredistinguished,twointhe Detailedsamplingofthesedimentfollowed. west outlined by the 1260m contour and one in the east at The pressure coring was carried out using the APCA 1265m. Its small size and location on a steep slope made (Autoclave Piston Corer Anaximander) [22] designed and it a lower priority for investigation during earlier research fabricated by Technical University of Berlin as part of projects. the ANAXIMANDER project. The APCA retrieves cores of 10cm diameter and up to a length of 250cm in water depths of up to 2500m. It preserves the sediment cores 3.2. Sedimentology. Five cores were collected from Thes- under in situ pressure conditions [22]. Upon retrieval on saloniki MV: four gravity cores (AX46-GC1, AX47-GC1, JournalofGeologicalResearch 3 29◦00 29◦20 29◦40 30◦00 30◦20 30◦40 31◦00 Kastelorizo TurkishContinentalMargin Antalya Island Basin 36◦00 B asin 36◦00 Finik e 2500 3000 Rhodes Basin 35◦40 2500 1500 35◦40 3500 The Great Slid e Fold 3000 A n a x2i0m00a n d e r menes Anaxagoras 2000 Belt xi 35◦20 Ana Florence 35◦20 Rise 40◦20◦ 25◦ 30◦ 40◦ Mediterranean Ridge Province Turkey 2500 PREOCJcoEnCtraTctEVAKN3-CAT-X20I0M2−A00N06D8ER 35◦00 Greece ChiefscientistV.Likousis 35◦00 Swath bathymetry map 35◦ Anaximander 35◦ S.Alexandri,P.Nomikou,D.Ballas Mountains Cyprus PErlloipjescotiido:nW:MGeSr-c8a4torat35◦N MSyisntedmepUthse:d6:0S0EmABMEaAxMde2p1t2h0:3(02000kmHz) Gridinterval:100meters Datacollectedby:R/VAEGAEO 30◦20◦ Africa25◦ 30◦ −30◦4500 −3500 −2500 −1500 −500Isobaths:100HmelleniccentreformInaMrinaeyr2e0s0e3aracnhdOctober-November2004 29◦00 29◦20 29◦40 30◦00 30◦20 30◦40 31◦00 (a) Kula N ◦ 5 6 3 5 Thessaloniki Kazan ◦ 4 8 3 5 Athina ◦ 4 0 3 5 Amsterdam ◦ 3 2 3 5 3 5◦ 2345◦ 1365◦ 0 8 29◦−43800029◦ 5−6260300◦ 04− 23200◦012 −310◦80200 3−0◦124800 30◦−31600030◦ 44− 60300◦ 52 31◦ 00 (b) Figure 1: Bathymetry-physiography of the Anaximander complex (a), and swath bathymetry with locations of the five surveyed mud volcanoes((b)from[17]supplementedwithANAXIPROBEdatatooutlineeachMVarea[11]). 4 JournalofGeologicalResearch Thessalonikimudvolcano 30◦15 30◦16 N −−11130000 1 3 6 0 35◦29 −1500 60 0 1340 5 8 0 1 4 0 0 − −1 −14 132 240 60 0 35◦30 35◦30 35◦28− −1 −11 −108 −1000 1320 1300 1216208 0 3355◦◦2298 1100 1150 12130000 12501300 1350 114400510500 3355◦◦2298 30◦15 1300 4gravitycores 35◦27 1300 35◦27 30◦14 30◦15 30◦16 GHsites Figure2:SwathbathymetrymapofThessalonikiMVandlocationofthecollectedcores(blackdots).Upperleft,greaterswathmapwith thevolcanoatthecenter,lowerright,ORETechsidescanimagefromANAXIPROBEcruiseontopofSEABEAMbackscatterintensitymap. GravitycoresAX46-GC1,AX47-GC1,andautoclavecoreAX49-AP1wereretrievedfromthenorthernpeak,nearlyatthesamelocation. GravitycoresAX-48andAX-49wereretrievedfromthesouthernpeak(from[17]supplementedwithbackscatterdataandlocationof APCAcore). Table1:(a)Gravitycores.(b)Autoclavecore. (a) Waterdepth Sediment Length G.H.presence Smellof Coreno. Latitude Longitude (m) temperature (cm) (visualidentification) H2Sgas AX46-GC1 35◦28.603(cid:3) 30◦15.113(cid:3) 1263 14,4◦C 110 No Yes AX47-GC1 35◦28.562(cid:3) 30◦15.123(cid:3) 1265 12,3◦C 167 No Yes AX48-GG1 35◦28.729(cid:3) 30◦15.052(cid:3) 1264 8.4–10.7◦C 130 Yes Yes AX49-GC1 35◦28.728(cid:3) 30◦15.060(cid:3) 1264 Nodata 228 Yes Yes (b) Waterdepth Length Pressure Gasvol. Coreno. Latitude Longitude GHpresence (m) (cm) (bars) (litres) AX49-AP1 35◦28.728(cid:3) 30◦15.060(cid:3) 1.264 0.70 105 Yes 3.1 AX48-GC1,andAX49-GC1)andoneautoclavecore(AX49- been dissociating gas hydrates present). These observations AP1).Theyarelocatedinsimilarsedimentaryenvironments confirmedthatthisMVisanactivegashydratebearingmud on the two western highs on the summit of Thessaloniki volcano,thefourthdiscoveredintheMediterranean. MV(Figure2),inwaterdepthsfrom1263to1265m.Table1 The general appearance of typical mud breccia cores presents the details of the core locations and characteris- (Figure3) is of a very poorly sorted sediment with muddy tics, with the initial deck observations made to determine matrix-supported angular to subangular clasts (xenoliths) whether there were gas hydrates (even if not actually of different compositions and grain sizes (0.5 to 2.5cm). observed; for example, with sediment temperatures below The clasts reflect the geological units through which the the seafloor temperature, ∼13.7◦C, there is likely to have overpressured sediment passed before erupting on the JournalofGeologicalResearch 5 seafloorasmudbreccia.Inthiscasetheyrepresentbasement units associated with the Lycian Nappes and Bey Dag˘ları to the north in Turkey [6, 7, 23–25]. Porous gas-release structuresarecommoninthesedimentweobservedbecause Thessalonikimudvolcano much of the disseminated gas hydrates, associated with AX46-GC1 AX47-GC1 AX48-GC1 AX49-GC this type of sediment, dissociated during the sampling 0 operationorminuteslateronboard,wheretheambientP-T 5 10 conditions indicate that gas hydrates are unstable [26, 27]. 15 Similar sediment has been described in other mud volca- 20 noes(Amsterdam,Kula,andKazan)inthearea[17,24,28]. 25 Core AX46-GC1 (Figure3) was retrieved from the 30 southernpeak(1263mwaterdepth;corelengthof119cm). 35 Thetop5cmiscomposedofayellowishgrayoxidizedmud 40 layer with faint laminae supporting dispersed small clasts 45 50 <1.5cm in diameter. There is a gradual change in color 55 downwards toward the next 5 to 19cm section which is a 60 greenish-gray reduced mud containing a few clasts up to 65 3cm in diameter. The following 19–119 section is simi- 70 lar in color with the overlying section but with larger 75 clasts, up to 5cm in diameter and increasing in the 80 lower 10cm. Evidence of dewatering features associated 85 with a strong gas smell were also noted. The sediment 90 temperature upon opening of the core was 14.4◦C, roughly 95 100 (actually, just above) seafloor temperature. No gas hydrates 105 weredetected. cm) 110 Gassmell On the same southern peak at a distance of about 80m pth ( 111250 T=14.4◦C to the north and at a depth of 1265m core AX47-GC1 was De collected with a length of 167cm (Figure3). The sediment 125 temperature upon opening was 12.3◦C. At the top of the 130 135 PresenceofGH core there was a 3cm thick yellowish gray oxidized layer 140 T=8.4◦C− followed by a 3–78cm section of dark reduced greenish- 145 10.7◦C graymudwithoccasionalclasts.Thesedimentismoresoupy 150 in the top 41cm of the section becoming stiffer below, 155 withfaintlaminaeat64to65cm.Thenext78to167cmsec- 160 Gassmell tioncontainslargerrockclasts,upto2.5cmacross,andtwo 165 T=12.3◦C dark gray-colored laminated layers at 79–85cm and at 96– 170 99cm.Thesedimentbecomesstiffatthebottomofthelayer. 175 NoGHwerefound. 180 185 On the northern peak a 130cm long core (AX48-GC1, 190 Figure3) was retrieved from a water depth of 1264cm. 195 The sediment temperature when measured on deck varied 200 between 8.4 and 10.7◦C. No oxidized layer was observed 205 at the top of the core, indicating relatively recent mud 210 volcanic activity in this area (because the upper part of the 215 mud breccias had not had time to oxidize nor to be over- 220 225 lain by semipelagic sediment typical of the local seafloor). 230 Thesedimentconsistsofgreenish-graymudwithlargerock PresenceofGH clasts dispersed throughout the whole length of the core. The GH were observed mainly between 110 and 120cm Yellowish mud - oxidized layer where their dissociation produced many degassing features Greenish gray mud resulting in the soft and sometimes soupy texture of the Clasts sediment (Figure4). Most of the large rock clasts occur in the lower section of the core, where the sediment becomes GH dissociation features stifferbelowacoredepthof55cm. Gradual change in color or composition Core AX49-GC1 (Figure3) was the longest core taken Sharp change in color or composition (228cm)andalsocomesfromthenorthernpeakatthesame Presence of gas hydrates location and water depth as core AX48-GC1. It consists of Figure3:Descriptionofthegravitycores. gray mud with foamy mousse-like texture and consistency, 6 JournalofGeologicalResearch It is possible that observations of gas hydrates in one core, butnotinanotherwithsimilarconcentrationsofmethane, canbeexplainedbydifferencesinthesizeofthegashydrate depositsbetweenthetwocores,withthesmallerGHcrystals disappearingmorequickly. Theinsitumethaneconcentrationintheautoclavecore at northern site AX49 (core AX49-AP1) was calculated to be about 180mmoL/kg pore water at depths where there is no sulfate present. To calculate gas hydrate volumes from methane concentrations in(cid:2)relation to the core volume, the amount of collected gas ( CH = 3.1L) is related to the 4 4cm corevolumebetweenthebottomofthecoreandthesulfate depletiondepth,assuminganevendistributionthroughout Figure 4: Section 99–124cm of core AX48-GC1. Note the soft this depth range with dissolved and hydrate-bound CH to characterofsection110–120cmwhichcontainedgashydrates. 4 be present. The saturation concentration (c ) of CH is eq 4 subtractedbeforecalculatinggashydratevolumes.Fordetails see[30].IncoreAX49-AP1gashydratesoccupyabout0.7% withmanydegassingfeaturesproducedfromthedissociation of the core volume. The gas collected from the pressure ofGHdispersedthroughoutthewholelengthofthecore. core is nearly devoid of propane and butane thus allowing structureIgashydratestobeformed[19].Nopressurecorer 3.3. Geochemical Results. A geochemical analysis was made wastakenonthesouthernpeakofthiswesternhigh. of both the mud flow (trace element) and the rock clasts (mainelement)ofthegravitycores. Theresultsofthetraceelementanalysisinthemudflow 3.4.StudyoftheMudBrecciaRockClasts. Thepresenceofa oftwogravitycores(Table2(a))indicatethatorganiccarbon yellowish-brownoxidizedlayerintheupperfewcentimetres (C ),Na O,Mg,Rd,Sr,andCudonotvarydowncore.The of the two gravity cores, where there were no gas hydrates org 2 total carbon (C ) is higher at the top of the cores than in observed,probablyindicatesthatatthesetwositesmudvol- tot thelowersectionswhereasthevaluesofSandZnareusually canoactivitywaslowtoabsentduringthelastfewhundred loweratthetopofthecoresthanbelow. years. Freshly erupted mud breccia is characterised by grey Calcite is the dominant mineral in the rock clasts from reduced sediment and the lack of an oxidised hemipelagic gravity core AX 48-GC1 (Table2(b)). This combined with sediment cover. An estimate of the age of eruptions can thepresenceoftheothermainelementsshowninTable2(b), sometimes be made using the thickness of the overlying andthelowdolomitecontent,supportearlierinterpretations sedimentandagoodestimateoftherateofsedimentation,in that bedrock here is related to the Miocene flysch deposits thisareaabout2–5cm/ka[24].Thecompositionofthemud presentonlandtothenorth([6]seeSection3.4). inallcoreswasmainlysiltyclayswithasandfractionbetween These results also indicate that the composition of 5 to 7% and a mean grain size between 6.2 and 7.8 phi; it the Thessaloniki MV sediments are comparable to those is consisted of terrigenous material with minor amounts of reportedinotherMediterraneanmudvolcanoeslikeAthina biogeniccomponents,mainlyplanktonicforaminifera. [20]andeventhosefromtheGulfofCadiz[29]. As noted previously, rock clasts that erupted through a The methane concentration was measured in both mudvolcanoarecomprisedofachaoticmixtureofmaterial gravitycores.NogashydrateswereobservedincoreAX47- from the overpressurized source formation and the rock GC1butthesedimentwaswetandinsomeplaces“soupy.” units through which the eruption occurred. This material On the other hand, gas hydrates were observed throughout can provide significant geological information about the core AX49-GC1 when it was opened on deck (Figures 3 deepergeologicalunitsunderlyingthemudvolcano,aswell and 4). Methane concentrations in core AX47-GC1 were as the stratigraphy. A litho-micropalaeontological study of about 2800µmoL/kg wet sediment, with a maximum of 39samplesofmudbrecciaclastsfromThessalonikiMVwas 4000µmoL/kgwetsedimentatacoredepthbelowseafloorof undertaken. 100cm.IncoreAX49-GC1,themethaneconcentrationwas These rock clasts of various size (2–5cm in length) 3000µmoL/kg wet sediment, decreasing to 2000µmoL/kg andsupportedinahomogeneousmudbrecciamatrixwere wet sediment below this maximum at 100cm down core sampled from the gravity cores collected during the second (Figure5).Thusthemethaneconcentrationsatbothwestern cruise of the ANAXIMANDER project. They were subse- highsonthesummitofthemudvolcanowerehighdespite quentlywashedandclassifiedbytheirgeneralcharacteristics the apparent differences in gas hydrate content seen in (composition, color, grain size, reaction with HCl, and the sediment. However, due to the degassing of these roundness). Several clasts were selected then for further conventionalcoresduringrecovery,andtheconsequentloss thinsectionanalysisusingaNIKONpolarizingpetrographic ofup to 90% of themethane [19],wecouldnot determine microscope.Themostinformativesampleswerealsowashed significant differences in methane concentrations because and sieved through a 150µm sieve. This fraction is also the concentrations are far below methane saturation in the usedforanalyzingtheplanktonicforaminiferaassemblages. presence of gas hydrates (∼100mmoL/kg pore water [19]). TypicalexamplesofthinsectionsareshowninFigure6. JournalofGeologicalResearch 7 Table2:(a)TraceelementanalysisofthemudflowincoresAX48GC1andAX49GC1.(b)Mainelementanalysis(%)oftherockclastsfrom coreAX48-GC1. (a) Core Sampledepth(cm) Ctot∗% Corg∗% S% Na2O% Mg% Sr% Rb% Znppm Cuppm AX48GC1 9cm 2,57 0,37 0,27 1,48 0,142 0,022 0,08 87 56 (cid:3)(cid:3) 30cm 2,05 0,35 0,44 1,75 0,146 0,019 0,10 94 78 (cid:3)(cid:3) 65cm 2,20 0,32 0,48 1,62 0,134 0,027 0,08 100 74 (cid:3)(cid:3) 110cm 1,70 0,32 0,40 1,75 0,137 0,023 0,08 104 78 AX49GC1 12cm 2,85 0,44 0,58 1,75 0,151 0,024 0,09 89 73 (cid:3)(cid:3) 50cm 2,25 0,48 0,62 1,75 0,150 0,023 0,09 102 72 (cid:3)(cid:3) 70cm 1,45 0,39 0,48 1,75 0,158 0,016 0,08 86 69 (cid:3)(cid:3) 105cm 1,75 0,43 0,58 1,62 0,146 0,023 0,08 94 76 (b) Mineral % Calcite 57 Quartz 12 Montmorillonite 5 Kaolinite 8 Glaucophane 4 Albite 6 SiO 5 2 Dolomite 3 ∗ Ctotistotalcarbon,Corgisorganiccarbon. Methane(µmol/kgwetsediment) an angular-subangular form, are small in size, have light- gray colour, are consolidated, and contain (10–60%) well- 0 2000 4000 6000 8000 preserved pelagic foraminifera in a micritic calcite matrix. 0 The foram chambers are usually filled by sparitic calcite or pyrite.TheplanktonicspeciespresentareOrbulinasuturalis, 50 Globigerinoidestrilobus,Globigerinoidessp.,andGloboquad- rina dehiscens, which indicate a Lower to Middle Miocene ) bsf 100 age and an open marine environment [17, 24, 31]. The m detrital biomicrites are angular-subangular in form, gray- c h( brown in colour, contain tests and fragments of planktonic ept 150 foraminifera,withfinegrainedaggregatesofcalciteandsilty D sized angular quartz grains in a micritic arenite matrix. 200 AmongthemainfossilsrecognizedarethespeciesOrbulina universa, Orbulina suturalis, Globigerinoides trilobus, Globo- quadrina nepethens, and Globigerinoides obliquus. which 250 indicate an Upper Miocene age [31], and an open marine AX47GCI depositionalenvironment. Comparable microfaunal associations of Miocene AX49GCI depositswerealsoidentifiedintheclastssampledbygravity Figure5:Methaneconcentrationsofoneofthesouthern(AX47- coring in the upper parts of mud flows in Amsterdam, GG1) and northern (AX49-GG1) gravity core stations at Thessa- Athina, Kazan, and Kula MVs. These data support the lonikiMV. conclusion that part of the basement of the Anaximander Mountains in this area contains Miocene deposits that are comparable in age and facies with the geological units of the neighbouring land area of SW Turkey. RockclastsfromtheThessalonikiMVcores(AX46GC1, Considering that these units are probably in situ, it can AX47GC1, AX48GC1, AX49GC1, and AX49AP1) belong be concluded that the onshore Miocene flysch deposits of to two rock groups: fossiliferous micrites and detrital the Antalya Complex [24, 31] extend southward into the biomicrites. Both these two groups were recognized also AnaximenesandAnaximanderMountains,thussupporting in the other ANAXIMANDER mud volcanoes during this similar conclusions by Woodside et al. and other authors project [24, 25]. The fossiliferous micrites exhibit mainly [6,7,12,32,33]. 8 JournalofGeologicalResearch (a) (b) (c) (d) Figure6:(a–d)Polarizedmicroscopepicturesofthinsectionsofmudbrecciarockclasts;bioclasticcarbonatepack/wackestones(grading intomudstones/claystones)withGlobigerinidaeplanktonicforaminifera. 4.GasHydrateStabilityField forexample,wereashighas2.78◦C/mintheactivecentreof Isismudvolcano[35]. As noted above, the sediment cores with gas hydrates were Agashydratestabilitydiagram,basedontheparameters allfromrelativelyrecentlyeruptedmudbreccia,asindicated justdescribed,indicates(Figures7(a)and7(b),[27,36])that bythelackofhemipelagiccoverorsurfaceoxidationofthe thegashydratesatThessalonikiMVarejustatthelimitfor mud flow. Thessaloniki MV is the shallowest mud volcano theoccurrenceofstablemethanehydrate,anddonotextend bearinggashydratesintheMediterranean(1265m).Atthis morethanafewmetersabovetheknownThessaloniki MV depth the gas hydrates are just within, and near the edge depth.Thismeansthatwithonlysmallchangesintheenvi- of the gas hydrate stability zone (Figures 7(a) and 7(b)) as ronmental parameters the gas hydrates could disassociate determinedbythepressure(12.9Mpaat1265mdepth)and releasingwaterandmethane.Suchchangescouldresultfrom seafloor temperature (∼14◦C). The field data collected at adecreaseinseafloorpressure(e.g.,bytectonicupliftorsea ThessalonikiMVindicatedthattheGHoccurat1265msea leveldecrease)orbyslightincreaseinthebottomwatertem- floordepthandinsubbottomsedimentarylayersatleastto perature(e.g.,fromaneventliketherecentincreaseinbot- 220cm below seafloor. The sea bottom water temperature tomwatertemperatureintheIonianSea[37]).Thesesmall is 13.75◦C and the geothermal gradient is expected to be changes in temperature and sea level are both possible and 30–35◦C/Km or more, based on heat flow measurements sufficienttodestabilizethegashydratesatThessalonikiMV. made in the Olimpi mud diapir field [34]. During the Although the amount of methane produced from the MIMEScruisein2004,oneheatflowmeasurementmadeby autoclave core from Thessaloniki MV is minor in quantity, Feseker and Foucher on Amsterdam Mud Volcano showed andthevolumeofgashydratesisunlikelytobelargeatthis a significant warming of the sediments by over 3◦C in the site (based on the maximum depth at which gas hydrates upper10mofmud[35,36].Inothermudvolcanoareasthe in this area can be stable, as indicated in Figures 7(a) and heatflowimpliesmuchhighergeothermalgradientswhich, 7(b)),wedo not know thepotential arealextent of the GH JournalofGeologicalResearch 9 Temperature(◦C) 5 10 15 20 25 0 50 Methanegasand Methanegasand water water ice 200 Hydrothermal curve 100 Permafrost hydrate 400 Methane hydrate andwater ice 600 m) m) 500 Methane ( ( Depth 800 Depth 1000 Xhydrate Oceanic hydrate Hydrate 1000 phase +N+aNCalCl N 2N2 ++CCOo22,, CC22HH66 boundary HH22SS,, C C33HH88 1200 5000 Water/sediment Geothermal BaseofGH 10000 curve −10 0 10 20 30 40 1400 Temperature(◦C) (a) (b) Figure7:(a)GashydratestabilitydiagramfortheThessalonikiMVgreaterarea(basedon[36]),(b)gashydratestabilitydiagram[27] depictingwithanXthelocationofThessalonikigashydratefield. at these water depths in the Eastern Mediterranean. Since at Thessaloniki MV indicate that the GH there are at the these GH are at the upper boundary of the GH stability upper limit of the stability zone, and prone to dissociation diagram their distribution and presence should be studied withtheslightesttemperatureincreaseorpressuredecrease. morethoroughly. Thereforeitcouldbeaparticularlysuitablesiteforstudying not only the mud volcano activity, but also the stability of natural gas hydrates and their potential environmental 5.Conclusion impactshouldtheydissociate. AnewgashydratebearingmudvolcanonamedThessaloniki Acknowledgments wasdiscoveredintheAnaximanderMountainsonthebasis ofitsseafloorexpressionandananalysisofcorescontaining The field and office work was supported by the EC-funded gas hydrates in a matrix of mud breccia typical of mud projectsANAXIMANDER(EVK-CT-2002-20068)andHER- volcanoes. It is the shallowest mud volcano there, lying at MES(GOCE-CT-2005-511234-1)whichtheauthorsgreatly depths between 1315 and 1260m, with an areal extend of appreciate.Theauthorsthanktheofficersandthecrewofthe about 1.67km2 and comprising three peaks on its summit. R/V Aegaeo for their important and effective contribution GH were collected from three cores (two conventional during the field work. They also thank the anonymous gravity cores and one autoclave core). The GH crystals reviewersfortheusefulcommentsandsuggestions. have the form of flakes or rice. The degassing of the 228cmlongautoclavecoreprovided3.1litersofgas(mostly References methane).Rockclastsfromthemudbrecciasindicatealower middleMioceneageforthesourcerockformation.Thesea [1] A. H. F. Robertson and A. 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like the ANAXIMANDER Mountains where mud volcanism is related to faults with .. They are located in similar sedimentary environments on the two
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