Petrology,
Geochemistry
(Geochronology)
U–Pb
laser
ablation
ICP-MS
zircon
dating
across
the
Ediacaran–Cambrian
transition
of
the
Montagne
Noire,
southern
France
Maxime
Padel
a,*
,
J.
Javier
A´lvaro
b,
Se´bastien
Clausen
a,
Franc¸ois
Guillot
c,
Marc
Poujol
d,
Martim
Chichorro
e,
E´ric
Monceret
f,
M.
Francisco
Pereira
g,
Daniel
Vizcaı¨no
haUMR8198EEPCNRS,universite´ deLille-1,baˆtimentSN5,avenuePaul-Langevin,59655Villeneuve-d’Ascqcedex,France b
InstitutodeGeociencias(CSIC-UCM),Novais12,28040Madrid,Spain
c
UMR8187LOGCNRS,universite´ deLille–universite´ duLittoralCoˆted’Opale,SN5SciencesdelaTerre,59655Villeneuve-d’Ascqcedex, France
d
Ge´osciencesRennes,UMR6118,universite´ deRennes-1,campusdeBeaulieu,35042Rennes,France
e
GEOBITEC/DepartamentodeCieˆnciasdaTerra,UniversidadeNovadeLisboa,Portugal
f18,ruedesPins,11570Cazilhac,France
gIDL/DepartamentodeGeocieˆncias,ECT,UniversidadedeE´vora,Portugal h
7c/oJean-BaptiseChardin,Maquens,11090Carcassonne,France
C.R.Geoscience349(2017)380–390
ARTICLE INFO Articlehistory: Received28July2016
Acceptedafterrevision25November2016 Availableonline1August2017
HandledbyMarcChaussidon Keywords: Ediacaran Cambrian U–Pbdating MontagneNoire ABSTRACT
U–Pblaserablationinductivelycoupledplasmamassspectrometrywasusedfordating
zircongrainsextractedfromfour sedimentaryandvolcanosedimentaryrocks ofthe
Montagne Noireencompassing thepresumedEdiacaran–Cambrianboundaryinterval.
MagmaticzirconfromtwosamplesfromthebasalandmiddlepartsoftheRivernous
Formation(arhyolitictuff)weredepositedat542.51Maand537.12.5Ma,bracketing
the541MaagepresentlyadmittedasbeingattheEdiacaran–Cambrianboundary.Inaddition,
apieceofsandstonefromtheunderlyingRivernousFormationcontainingmostlyeuhedral
zircongrains,suggestingproximalmagmaticsources,yieldsNeoproterozoicdatesranging
from574Mato1Ga,and subsidiaryolderdates from1.25to2.75Ga.Anotherpieceof
sandstone fromthe overlyingMarcoryFormation yielded mostly roundedzircon grains
probablyissuedfrommoreremoteareas,withalargespectrumdominatedbyNeoproterozoic
datesaswellasolderagesupto3.2Ga.Acomparisonofbothkindsofsandstonesuggestsa
significantchangeinprovenance,changingfromarestrictedsourceareaduringtheEdiacaran
toamuchlargersourcedomainduringtheCambrianEpoch2thatrecordedcontributions
fromdifferentcratonsofGondwana.
C 2017Acade´miedessciences.PublishedbyElsevierMassonSAS.Thisisanopenaccess
articleundertheCCBY-NC-NDlicense(http://creativecommons.org/licenses/by-nc-nd/
4.0/).
* Correspondingauthor.
E-mailaddresses:maxime.padel@etudiant.univ-lille1.fr(M.Padel),jj.alvaro@csic.es(J.J.A´lvaro),sebastien.clausen@univ-lille1.fr(S.Clausen),
Francois.Guillot@univ-lille1.fr(F.Guillot),marc.poujol@univ-rennes1.fr(M.Poujol),ma.chichorro@fct.unl.pt(M.Chichorro),eric.monceret@orange.fr
(E´.Monceret),mpereira@uevora.pt(M.F.Pereira),daniel.vizcaino@wanadoo.fr(D.Vizcaı¨no).
ContentslistsavailableatScienceDirect
Comptes
Rendus
Geoscience
ww w . sci e nc e di r e ct . com
http://dx.doi.org/10.1016/j.crte.2016.11.002
1631-0713/ C 2017Acade´miedessciences.PublishedbyElsevierMassonSAS.ThisisanopenaccessarticleundertheCCBY-NC-NDlicense(http://
1. Introduction
The pre-Variscan succession of the Montagne Noire
cropsoutasafold-and-thrustcomplexdividedintotwo
sedimentary-dominated, northern and southern flanks
fringinganessentiallymetamorphic,AxialZone(Arthaud,
1970; Ge`ze, 1949). Several tectonic models have been
proposedfortheMontagneNoireandarestillsubjectof
debate(BrunandVanDenDriessche,1994;Charlesetal.,
2009; Faure and Cottereau, 1988; Fre´ville et al., 2016; Mattaueretal.,1996;Poujoletal.,inpress;Soulaetal., 2001;VanDenDriesscheandBrun,1992).The
Precambri-an–Cambrianboundaryhastraditionallybeententatively
located in the lowermost formation exposed in the
southernMontagneNoire,namelytheMarcoryFormation
(A´lvaro et al., 1998). However, recent reviews of the
northernsuccessionschallengedtheformerstratigraphic
chart (A´lvaro et al., 2014b; Devaere et al., 2013) and
establishedalowerstratigraphicpositionforthe
volcano-sedimentarysuccessionsoftheGrandmont,Rivernousand
Layrac formations, exclusively exposed in the northern
MontagneNoire.Theonlypreviousradiometricdatafrom
theRivernousFormation(Fm.)yieldedanOrdovicianage,
ranging from 47319Ma to 44340 (Rb/Sr method;
Demange, 1982), which was subsequently ruled out by
biostratigraphicagesyieldedbyacritarch-bearing,laterally
equivalent deposits (the so-called ‘‘Schistes X’’) from the
Axial Zone (Fournier-Vinas and Debat, 1970). There, the
‘‘SchistesX’’arecappedbytheSe´rie`sTuff(‘‘Se´rie`s’’isavillage
name) tentatively correlated with the Rivernous Fm. The
Se´rie`sTuffwasdatedat54515MabyPb-evaporationon
zircon from a metadacite (Lescuyer and Cocherie, 1992).
Somescarcezirconcrystalsweresampledinagarnet-grade
Cambrianmeta-siltstonefromthesouthernMontagneNoire,
givingamaximumdepositionalageof556Mabasedonlyon
asinglezircon(Gebaueretal.,1989).Thisageattributionmay
lookdisputable,giventhemorerecentstatisticalguidelines
for provenance studies (see below) and also taking into
accountthemarkedmetamorphiccharacterofthisrock.In
fact,inapreviouspaper,GebauerandGru¨nenfelder(1977)
admittedthatabout80%oftheprimitiveradiogenicPbmight
havebeenlostduetoPhanerozoicthermalevents.Inorderto
improvethestratigraphicframeworkoftheNeoproterozoic–
Cambrian boundary interval, and the lithostratigraphic
nomenclaturallinksbetweentheAxialZoneandthenorthern
andsouthern flanksof theMontagneNoire, zircongrains
weresampledfromtheRivernous,GrandmontandMarcory
formationsanddatedbyinsituLA-ICP-MSU–Pbanalysis.Our
results place new constraints upon the palaeogeographic
affinitiesofthedifferenttectonostratigraphicunitsthatform
theMontagneNoire,aswellasonthedetritalprovenanceof
theEdiacaran–Cambriansedimentspreservedin
neighbour-ingtectonostratigraphicareas.
2. Geologicalandstratigraphicsetting
LocatedinthesouthernpartoftheFrenchMassifCentral
(Fig.1A),theMontagneNoirerepresentsasegmentofthe
external,southwesterncomponentoftheVariscanBeltin
Europe(Demange,1998;Poujoletal.,inpress;Rogeretal.,
2004).Assummarizedabove,thisENE–WSW-strikingrange
isdividedintothreetectonicunits:acentralmetamorphic
dome,theso-calledAxialZone,fringedbyitsnorthernand
southernflanks(Demange,1985;Ge`ze,1949).
TheAxialZoneisessentiallycomposedofmicaschist,
minor marble, paragneiss and migmatized orthogneiss
(Ge`ze,1949).Theprotolithageoftheorthogneissandits
relationshipwiththemetasedimentaryrocks havebeen
disputed.Someauthorsinterpretedtheorthogneissasa
granitic Precambrian basement (Demange,1975, 1998),
whereas others considered it as Palaeozoic intrusions
(BardandLoueyit,1978).Recentconventional(ID-TIMS),
SHRIMP and LA-ICP-MS U–Pb datings of various
ortho-gneisssamples(Cocherieet al.,2005;Pitra etal.,2012;
Rogeretal.,2004)suggestthatthegraniticprotolithwas
emplacedduringtheOrdovician.
The southern and northern sedimentary-dominated
flanksoftheAxialZoneareafold-and-thrustcomplexof
nappes (Fig. 1). The Precambrian–Cambrian boundary
interval, only reported in thenorthern MontagneNoire
(A´lvaro et al., 2014b), comprises four formations, from
bottom to top, the Grandmont, Rivernous, Layrac and
Marcou formations(Fig. 2). The Grandmont Fm., about
700m thick, consists of grey to black shales with
subsidiary sandstone interbeds (Fig. 2). The Rivernous
Fm.,upto200mthick,comprisesslightlymetamorphosed
rhyolitictuffsthatincluderarebrecciaandshaleinterbeds
(Fig.2). Bothformationscrop out intheAve`ne–Mendic
parautochthon,whichincludestheLode´voisinlierandthe
Lacaunethrustslice(Murat,Fig.1B).IntheLacauneunit,a
lateral equivalent of the Rivernous Fm. (locally named
Murat Fm.),withbaseand toptruncatedby faults,was
datedat53212Ma(U–Pbonzircon;Demangeetal.,1995;
Ducrotet al., 1979). In the Ave`ne–Mendicparautochthon
(Fig.1),therhyoliticpalaeorelief formedbytheRivernous
Fm.(uptoabout300mhigh,afterA´lvaroetal.,2014b)is
unconformably onlapped by the volcano sedimentary
conglomerates andsandstones of the LayracFm. (Fig. 2).
TheLayracFm.isitselfoverlainbythecarbonate-dominated
MarcouFm.,about400mthickandassignedtotheCambrian
Stage2byrecentbiostratigraphic studies(Fig.2,Devaere
etal.,2013).
Theabove-reportedformationsarenotexposedinthe
southern Montagne Noire, where the oldest outcrop is
represented by the up to 1000m-thick Marcory Fm.
(Fig. 2), a monotonous alternation of sandstones and
shaleswithsubordinatecarbonatenodulesandlayers.The
upperpartoftheMarcoryFm.hasbeenassigned tothe
CambrianStage2–3transitionduetotheoccurrenceofthe
ichnogenera Psammichnitesand Taphrelmintopsis (A´lvaro
andVizcaı¨no,1999),andtheoldesttrilobitesfoundinthe
Montagne Noire, i.e. Blayacina miqueli (Cobbold, 1935;
Geyer, 1992). The MarcoryFm., although absent in the
Ave`ne–Mendicparautochthon,isexposedinotherthrust
slicesandnappesofthenorthernMontagneNoire.
3. Materialandmethods
3.1. Material
TheGrandmontandRivernousFormationshavebeen
(about4kmtotheeastofLode`ve):asandstonefromthe
baseoftheexposedGrandmontFm.(sampleMN1),anda
rhyolitictufffromthebaseoftheRivernousFm.(sample
MN2).TheRivernousFm.wasalsosampledatitsmiddle
partneartheColduLayrac(sampleMN3).MN1toMN3
samplesbelongtotheso-calledAve`ne–Mendic
parautoch-thon.InordertoinvestigatetheprovenanceoftheMarcory
Fm.,asandstone(sampleMN4)wasalsoselectedfromthe
Psammichnitesgigas-bearinglevelinthesouthern
Monta-gneNoire (A´lvaroand Vizcaı¨no,1999),along theOrbiel
riversectionoftheMinervoisnappe(Fig.1).
3.2. Samplespreparation
Zirconseparationfromfreshsamplesstartedwithrock
grindingusingasteelcrusher.Theresultingpowderswere
sievedintherangeof50–250
m
m.Grainswereseparatedfirstusinga heavyliquid (sodium heteropolytungstates,
density 2.85gcm–3), then using a Frantz magnetic
separator.FollowingSla´maandKosˇler(2012),theselected
grainswereobtainedfromrandomhandpickingundera
binocularmicroscopewhatevertheirsize,shape,orcolor,
inordertoavoidanyoperatorbias.Theywerefinallysetin
anepoxyresinpuckandpolishedtoexposetheircore.
3.3. LA-ICP-MSinsituU–Pbdating
Toidentifyinternalgrowthtexturesandmorphologies,
zircongrainswereimagedbyscanningelectronmicroscopy
(SEM) to get cathodoluminescence and back-scattered
electron images (atthe ‘‘Laboratoire d’oce´anologie etde
ge´osciences’’,UniversityofLille,France).TheU–Pbagesof
zirconsweredeterminedinsituattheGe´osciencesRennes
laboratoryby LA-ICP-MSusingan ICP-MSAgilent 7700x
coupled with an ESI laser Excimer system producing a
radiationwithawavelengthof193nm(NWR193UC),with
ablationspotdiametersof25
m
m,energypulsesof7Jcm–2,and repetitionratesof5Hz.Ablations wereoperated on
both grain rims and cores. Where necessary, distinct
domainsofazircongrainwereanalyzedtocomparetheir
ages.TheresultingablatedmaterialwasmixedinaHe,N
andArgasmixturebeforebeingtransferredintotheplasma
sourceoftheICP-MSdevice.Eachanalysislasted80sand
consisted of a first 20-s background measurement
Fig.1.SimplifiedgeologicalmapoftheMontagneNoire;modifiedfromDevaereetal.(2014).A,LocationoftheFrenchMassifCentral(grey)andMontagne Noire(rectangle)inFrance.B,Structuralunitsandpreviousradiometricages:(a)Demange,1982(Rb/Sr)discardedbyourresults(seetext);(b)Ducrotetal., 1979(U–Pb)inDemangeetal.,1995;(c)LescuyerandCocherie,1992(U–Pb);(d)Rogeretal.,2004.
M.Padeletal./C.R.Geoscience349(2017)380–390 382
followed by 60-s ablation with measurements of
204
(Hg+Pb), 206Pb, 207Pb, 208Pb, 232Th, and 238U, and a
15swash-outdelaybeforethenextacquisition.Thedata
werecollectedinbatchof43analysesdividedinthreesetsof
10unknowns,bracketedbytwomeasurementsoftheGJ-1
primaryzirconstandard(Jacksonetal.,2004)tocorrectfor
U–Pb and Th–Pb laser-induced fractionation and for
instrumentalmassdiscrimination,followedbyoneanalysis
of thePlesovice secondaryzircon standard(Sla´ma etal.,
2008)inordertochecktheprecisionandaccuracyofthe
measurements. During the course of this study, the
Plesovice zircon standard yielded a Concordia age of
336.80.67Ma (N=32). The operating conditions forthe
LA-ICP-MSequipmentcanbefoundinSupplementaryTable
1. For more information on the acquisition protocol, see
Manzottietal.(2015).Datatreatmentwasperformedwiththe
GLITTERsoftware(VanAchterberghetal.,2001)andplotted
using the Isoplot 3.75 software (Ludwig, 2012) in both
Wetherill and Tera-Wasserburg Concordia diagrams. For
rhyolitic tuffs, theages werecalculated using theTuffZirc
Agealgorithm(LudwigandMundil,2002)togetherwiththe
SambridgeandCompston(1994)algorithm.Forthe
sandsto-nes,agedistributioncurveswithprobabilitydensityplotwere
obtained using the density plotter freeware proposed by
Vermeesch(2004).Fordates>1Ga,wereportedthe207Pb/
206Pbdatesandforages<1Ga,weusedthe206Pb/238Udates.
The analyses out of the [90–110%] concordance interval,
calculated with 100(207Pb/235Uage)/(207Pb/206Pbage) for
ages>1Ga(Meinholdetal.,2011)and100(206Pb/238Uage)/
(207Pb/235Uage) forages <1Ga, wererejected (Faure and
Mensing, 2005 and Talavera et al., 2012). The age ofthe
youngestzirconpopulationisderivedfromaclusterofatleast
threeanalysesfromthreedifferentgrainsoverlappinginageat
2
s
(standarddeviation),asproposedbyDickinsonandGehrels(2009) to ensure a statistically robust estimate of the
maximum depositional ages. Percentages of concordance,
isotopicratiosandageswith1
s
errors,aswellasUandPbconcentrations are providedin Supplementary Table 2. In
sedimentaryrocksamples(MN1andMN4),about110grains
wereanalyzedinordertogetthebestrepresentationofthe
detritalzirconpopulations.Fortuffs(MN2andMN3),about
50grainswereanalyzed,followingthesuggestionsofBowring
etal.(2006),togivearobustestimateofthebestageforthe
relatedvolcanicevent(s).
4. Results
4.1. GrandmontFormation(MN1)
ZirconsfromthesampleMN1,medium-grained
sand-stone, are mostly in the 100–250
m
m range, euhedral,facetted,rarelysub-rounded,colourlessandgenerallywell
zoned(Supplementarydata,Fig.S1).107ofthe114MN1
analyseswereconcordant [90–110%],amongwhich94%
are Neoproterozoic (101 grains), 3% Mesoproterozoic
(3 grains), 2% Paleoproterozoic (2 grains) and 1 grain
(1%)isArcheaninage(Fig.4B).Intheintervalrangingfrom
500to1100Ma,theprobabilitycurveshowsadominant
Ediacaran group within the cluster 550–850Ma, which
displaysamainpeakaround605Maandasecondaryone
around 635Ma (Fig. 4B). In this same cluster, four
subsidiary peaks are identified around 690Ma, 760Ma,
805Ma and 835Ma. The Tonian-aged zircon grains are
characterized by one peak around 906Ma, in an 890–
920Maclusterandanotherpeakaround1Gainthe950–
1050Macluster.Thefouryoungestandconcordantzircon
grains from this group rangingfrom 567.26.12Ma to
579.56.28Ma,yieldanaveragedateof5746Ma (95% conf.,Fig.3E).
4.2. RivernousFormation(MN2andMN3)
Samples MN2 and MN3 are both rhyolitic tuffs.
Accordingly,zircon grains fromsamplesMN2 andMN3
areeuhedral,clearandcolourless.Rarelycored,internal
structures highlighted by the CL-imaging show clear
magmaticzoning(Supplementarydata,Fig.S1).
InsampleMN2,59zircongrainswereanalysed,among
which 50 gave concordant dates [90–110% as defined
above]. Seven of the 50 analyses wererejected due to
possibleleadloss.Thustheyoungestandmainpopulation
fromthissamplerepresent65%ofthese43zircongrains
with individual 206Pb/238U dates ranging from
534.86.01Mato5466.02Ma.Thesecondgroup
repre-sents23%ofthetotalpopulation,andgives206Pb/238Udates
ranging from 576.96.3Ma to 600.86.7Ma (Fig. 3A).
Finally, five inherited core grains were dated at
Fig.3. LA-ICP-MSresultsforallsamplesusing206
Pb/238
Uages.DiagramA:mixtureanalysisforsampleMN2usingSambridgeandCompston’s(1994) approach;theage579.84.3Maisconsideredasinheritedage.DiagramB:mixtureanalysisforsampleMN3usingSambridgeandCompston(1994)approach; theage5247.2Maisconsideredasgeologicallymeaningless,duetoleadloss.DiagramsCandD:datapointagedistributionforsamplesMN2andMN3,resp., usingTuffZircAge(LudwigandMundil,2002);chosenemplacementagefortherhyolitictuffsoftheRivernousFm.are:5423Ma(2s)forsampleMN2and 5373Ma(2s)forsampleMN3.DiagramsEandF:averageagecalculatedfortheyoungestconcordantzirconpopulationofGrandmontandMarcoryFm.(sample MN1andMN4),derivedfromaclusterofatleastthreeanalysesfromthreedifferentgrainsoverlappinginageat2s(standarddeviation)asproposedbyDickinson andGehrels(2009).
M.Padeletal./C.R.Geoscience349(2017)380–390 384
651.67.2Ma,661.87.1Ma,66237.1Ma,685.87.6Ma
and704.77.6Ma(SupplementaryTable2).
Looking attheyoungestpopulation, theTuffZircAge
algorithmreturnedadateof542.5+0.7/–0.6Ma,whilethe
SambridgeandCompstonalgorithmyieldedacomparable
dateof541.92.3Ma(Fig.3AandC).Therefore,choosing
between those two within error identical results, we
concludethatthisrhyolitictuffwasemplaced542.5+0.7/–
0.6Ma.
InsampleMN3,58zircongrainswereanalysed,among
which 52 yielded concordant results [90–110%]: two
compositegrainswithcores(Zr1andZr27)yieldingU–
Pb datesof1837.719.1Maand583.16.37Ma
respec-tively. The youngest zircon population suggested by the
SambridgeandCompstonapproachforsampleMN3returned
adatearound524Ma(Fig.3B),whichispoorlyconstrained,
by only one concordant zircon among seven somewhat
discordantdatapoints(onaConcordiaplot).Therefore,this
dateisinterpretedasgeologicallymeaninglessasitcouldbe
linkedtoapossibleleadloss.
Keepingonlyagroupcomprisingthreeconcordantdata
points(greybars in Fig.3B),theTuffZircAge algorithm
yielded adate of537.35+2.35/–1.25Mawhile the
Sam-bridge and Compston approach returned a comparable
date of 537.12.5Ma. This second rhyolitic samplewas
thereforeemplaced537.12.5Maago(2
s
)(Fig.3BandD).4.3. MarcoryFormation(MN4)
SampleMN4isafine-grainedand maturesandstone.
Accordingly, its zircon crystals are mostly anhedral,
rounded to subrounded, often broken and rarely
bi-pyramidal, largely in the 50–100-
m
m size range. Theyare colourless to yellowish, though the biggest zircon
grainsarereddishincolour.Intheanalysedfraction,104of
the112MN4analyseswereconcordant[90–110%],among
which 87%are Neoproterozoic(90grains), 4%
Mesopro-terozoic (4 grains), 5% Paleoproterozoic (6 grains), 2%
Neoarchean(2grains),onegrainisMesoarcheanandthe
oldestoneisPaleoarcheaninageat3.2Ga(Fig.4A).
Theprobabilitydensitycurve(Vermeesch,2004)shows
a dominant Ediacaran group (clustered across 550–
850Ma),withamainpeakaround614Maandasecondary
peak around 575Ma (Fig. 4A). In this same cluster, six
otherpeaksareidentifiedaround651Ma,678Ma,700Ma,
737Ma, 800Ma and 850Ma. The Tonian-aged zircon
grains are characterized byone peak around900Ma in
an 890–920Ma cluster and another distinctive peak
around 1Ga in the 950–1050Ma cluster. The three
youngest dates obtained from this sample that are
concordantyieldanaveragedateof602.57.3Ma(Fig.3F).
5. Discussion
5.1. TheRivernousvolcanicactivitymarkingthe
Precambrian–Cambrianboundaryinterval
Thetwodates(537.12.5Maand542.5+0.7/–0.6Ma)
obtainedfromtheRivernousrhyolitictuffsaremucholder
than previouslyestimated(47319Ma and44340Ma;
Demange, 1982). These results allow us to confidently
identify the Precambrian–Cambrian boundary (541Ma,
Gradstein et al., 2012) in the basal succession of the
MontagneNoire.Bycomparisonwiththepreviously
deter-mined age of the Se´rie`s Tuffs from the Axial Zone
(54515Ma;LescuyerandCocherie,1992)andthe
River-nous(formerMurat)Fm.intheLacaunethrustsliceofthe
northernflank (53212Ma, interceptsuperior; Demange
etal.,1995andreferencestherein;Figs.1–2),theseresults
supportthelateralequivalenceoftheSe´rie`svolcanicepisode
(AxialZone)andRivernousrhyolitictuffdeposition(northern
flank),asalreadysuggested(Poucletetal.,inpress).
InotherVariscanunitsoftheIbero-ArmoricanArc,some
plutonicbodieshaverecentlybeendatedaround540Maby
LA-ICPMS(Supplementarydata,Fig.S2;seealsoCasasetal.,
2015;Castin˜eirasetal.,2008;Gutie´rrez-Alonsoetal.,2004; Melletonetal.,2010;Rubio-Ordo´n˜ezetal.,2015):the
Arc-de-FixandArde´choisaugengneissesintheMassifCentral,
with respective Concordia age of 541.83.1 and
542.53.1Ma (Couzinie´ et al., this issue), as well as the
LaparanorthogneissintheCentralPyrenees,withaConcordia
age of 5453Ma (Mezger and Gerdes, 2016). All these
plutonicandvolcanicevents,overlappinginagewithinerror,
shouldbelinkedtoacommonepisodeassociatedwiththe
voluminousmagmaticandanatecticCadomianevents
repor-tedforWestGondwana,amongothers,byLinnemannetal.
(2007, 2008). According to these authors, the numerous
plutonic and volcanic to volcano sedimentary complexes
identifiedintheOssa-Morena,Saxo-ThuringianandAnti-Atlas
zones(A´lvaroetal.,2014a;Bleinetal.,2014)canresultfroma
slabbreakoffofasouthwardsubductedoceanicplateending
withtheCadomiancycleatabout545–540Ma.Theendofthe
Pan-African/CadomiancycleledtotheonsetofaCambrian
magmaticcycle(Supplementarydata,Fig.S2),relatedtothe
riftingoftheNorthGondwanamargin(A´lvaroetal.,2014a,
2014b;Poucletetal.,inpress).
5.2. AgeandpotentialprovenancesoftheGrandmontand
Marcoryformations
Depositionalages.Theyoungestgroupofconcordant
zircongrainsfromtheGrandmontFm.(sampleMN1)yield
anaveragedateof5746Mathatisinterpretedhereasits
maximumdepositionalage(i.e.lateEdiacaran;Fig.3E).This
resultiscoherentwiththestratigraphicframeworkproposed
byA´lvaroetal.(2014b)andtheNeoproterozoicagebasedon
acritarchsreportedfromthe‘‘SchistesX’’ Fm.oftheAxial
Zone (Fournier-Vinas and Debat, 1970). As a result, this
maximum age of deposition supports their correlation
betweentheGrandmontand‘‘SchistesX’’formations(A´lvaro
etal.,2014b).
Theaveragedatecalculatedfromtheyoungestgroupof
concordant data for the Marcory Fm. at 602.57.3Ma
(Fig.3F)mightbeconsideredasamaximumdepositionalage.
However, it is far from the real depositional age, as
mentioned above. Indeed, this samplewas selected from
the Psammichnitesgigas-bearing level (Fig. 2), and
conse-quently must be assigned to the Cambrian Stage 2–3
transition,i.e.itislessthan521Maold.
Sourceofthepre-ca.1Gadetritalzircongrains.The
(MN4)andGrandmont(MN1)formationsaresomewhat
similar, but display some differences. Although each
individualsingleton-dateshouldbetreatedwithcaution,
the distributions of pre-1 Ga ages are plainly distinct
(Figs.4and5).
Asmentionedabove,zircongrains fromtheMarcory
Fm.(sampleMN4)aremuchsmalleranddefinitelymore
rounded(Supplementarydata,Fig.S1)thanthosefromthe
GrandmontFm.(sampleMN1),suggestingalongdistance
oftransportfortheformergrains.Wehaveseparateddata
frominheritedcores(whiteboxesinFig.4),meaningless
regardingthesourceage,fromdatafromzonedmagmatic
rims(blackboxes,Fig.4)thatrepresentmostprobablythe
ageofthesource-rock.Fromthisrespect,theoldestzircon
rim from the Grandmont Fm. (MN1) is only Late
Paleoproterozoic(180619Ma),andonlytwograinrims
are older than 1 Ga.By contrast,the presence ofseveral
ArcheanzirconrimsinMN4pointstoamajorchangeinthe
sourceareas.MN1zircongrainscouldpossiblybederived,
ultimately,fromtheAmazoniancraton(Rhyacian,Orosirian
andStatherianevents),moreprobably fromthe Eburnean
WestAfricancraton,orfromtheSaharanmetacraton(Fig.5).
By contrast,eight pre-1Gazircon rims fromsampleMN4
form a Paleoproterozoic group (cluster ranging from
Fig.4.Frequencyandprobabilitydensityplotsofdetritalzircongrainsintherange500–3300MaforsamplesMN1(B)andMN4(A).Agegroupsofeach samplearepresentedinapiediagram.SectionCshowsacomparisonofagegroupswherewhiteboxesrepresentdatesfrominheritedcoreandblackboxes relatetodatesfromzonedrims.
M.Padeletal./C.R.Geoscience349(2017)380–390 386
210919Mato178720Ma)andanArcheangroup.Those
groupsfitmuch betterwithan Africansourcecomprising
EburneanareasplusArcheanWestAfricancraton(Fig.5).
However,weshouldnotexcludethattheavailabilityof
zircon to erosion and transport from either primary
crystalline orrecycled sources requiresthat the
zircon-bearing rocks be exposed at the appropriate time, and
recyclingfromoldersedimentarydepositsmayconstitute
a more significantsourcethan fromprimarycrystalline
rocks.
SourcesoftheStenian–Toniandetritalzircons.The
clusterpointingtotheStenian–Toniantransition(950to
1100Ma)insamplesMN1andMN4couldshareacommon
origin (Fig. 4). Oneshould expectanAmazoniancraton
affinity (Linnemann et al., 2011) with detrital sources
related totheSan Ignacioand Sunsasevents andon its
eastern margin (Pereira et al., 2012). However, many
studies on sandstones from Lower Palaeozoic
peri-GondwananexposuresaroundtheMediterraneanregion
(e.g.,Israel,Jordan,Libya,Pyrenees,Sardinia,Greeceand
Sicily) rule out an Amazonian provenance and suggest
insteadaneasterntosoutheasternAfricanorigin(Altumi
et al., 2013; Avigad et al., 2003; Avigad et al., 2012; Kydonakisetal.,2014;Margalefetal.,inpress;Meinhold etal.,2011;Meinholdetal.,2013;Williamsetal.,2012).
Therefore,theArabian–Nubianshield,theSaharan
meta-craton, possibly the western edge of the Congo craton
(Tacketal.,2001),aswellasitseasternpartrecordingthe
‘‘Kibaran Event’’(Tacketal.,2010)andtheIrumidebelt
(Meinholdet al.,2011), fit wellaspotentialsources for
MesoproterozoicandStenian–Tonianzircongrains.These
zircon-formingeventsoccurred simultaneouslywiththe
assembly of the supercontinent Rodinia (Grenvillian
orogeny). Different hypotheses have been advanced to
explainthisinputofMesoproterozoicandStenian–Tonian
zircon crystals (Altumi et al., 2013), including: (i) the
transportoflargeamountsofsedimentthrough
Neopro-terozoicglaciersfollowinganoriginalsouth–north
tran-sect,later reworkedanddeposited(Avigadetal.,2003);
and (ii) a sourceregion linked tothe Transgondwanan
supermountain range resulting from the East African–
AntarcticOrogenandformedduringtheprotractedLate
Neoproterozoic docking of East and West Gondwana
(Williamset al., 2012), involving the development of a
super-fan system (Kydonakis et al., 2014; Squire et al.,
2006).
SourcesofNeoproterozoicdetritalzircons.
Neopro-terozoic grains display similar age distributions in the
GrandmontandMarcoryformations:amain
Neoprotero-zoicpopulation of zircongrains (with onepredominant
Ediacarangroup)followedbyfivesimilarpeaksacrossthe
Tonian–Cryogenianinterval(Fig.4).Potentialsourcesfor
thesedetritalzirconsarelocatedintheeastern(Saharan
metacraton,Arabian-Nubianshield)andwestern
(Trans-Saharanbelt, Pan-Africansutureof theAnti-Atlas,early
and lateCadomianarcs, and AvalonianArc)area of the
North-Gondwanamargin(Fig.5).Theprobabilitydensity
curve of the Marcory Fm., as well as the shape and
roundnessofitszircongrains,impliesmoreremoteorigins
forthemthanfortheGrandmontFm.ones.Therefore,a
Fig.5.PotentialsourcesforsamplesMN1andMN4(modifiedafterDrostetal.,2011;Linnemannetal.,2011;Pereiraetal.,2011;Pereiraetal.,2012;Tack etal.,2001;Tacketal.,2010).AC1:SiderianeventoftheAmazoniancraton;AC2:Rhyacian,OrosirianandStatherianeventsoftheAmazoniancraton;AC3: SanIgnacioandSunsaseventsoftheAmazoniancraton;AC4:easternmarginoftheAmazoniancraton;Av:Avalonia;Cd:Cadomia;Bo:Bohemianmassif; AA:Anti-Atlas;WAC1:EburneaneventoftheWestAfricancraton;WAC2:LiberianeventoftheWestAfricancraton;WAC3:LeonaneventoftheWest Africancraton;TSB1:Trans-Saharanbelt,Benin-Nigerianshield;TSB2:Trans-Saharanbelt,Tuaregshield;SMC:Saharanmetacraton;ANS:Arabian–Nubian shield;CC:Congocraton.
comparisonof themorphologicalandagedifferencesof
thesezircongrainssuggestsanevolution ofthe
deposi-tional basinand it sourcing froma narrow basinbeing
infilledbytheGrandmontFm.,probablyaback-arcbasin
resulting from the Panafrican/Cadomian orogeny, to a
moreevolved andopened basininfilledby theMarcory
Formation, represents a more evolved and widespread
basinwithwiderpotentialsourceareas,developedduring
thebreak-upofWestGondwana.
AcompositezircongrainoftheGrandmontsandstone
(sampleMN1;ZR49)demonstrates thatcrustwithca.
586Maoldrocksbecamerecycledduringmagmatismat
ca.567Ma,and underlinestheexistenceoftwodistinct
Ediacaranmagmaticeventsinthesourcearea.
One should expect to identifythe Ediacaran
River-nous volcanic event as reworked zircon grains in the
overlying Cambrian Marcory Fm. However, this is not
the case. A rapid burial of the Rivernous volcano
sedimentary palaeorelief, related to high rates of
sedimentationandavailableaccommodationspace due
to active thermal subsidence, has been proposed for
FurongiantoEarlyOrdoviciantimesinWestGondwana
(Linnemannetal.,2011;Pereiraetal.,2012)andthelate
Neoproterozoic–earlyCambrianintheANS(Avigadand
Gvirtzman, 2009) or post-Cadomian rifting extension (Poucletetal.,inpress;VonRaumerandStampfli,2008),
whichshouldprecludereworkingoftheRivernousfrom
distal(northern)toproximalareas(southernMontagne
Noire).
6. Conclusions
TheEdiacaran–Cambrianboundaryhasbeen
confident-lyidentifiedwithinerror,basedonU–Pbzircondating,into
theRivernous Fm.ofthenorthernMontagneNoire.The
Rivernous volcanic event is indicated to be the lateral
equivalentoftheSe´rie`sTuffoftheAxialZone.Thisfitswell
with a latest Ediacaran depositional age (ca. 574Ma)
estimatedwithdetritalzirconU–Pbgeochronologyforthe
underlyingGrandmontFm.Thelatter shouldbe
consid-eredas a time-stratigraphicequivalentof the
acritarch-bearing‘‘SchistX’’Fm.oftheAxialZone(Supplementary
data,Fig.S3).
U–PbanalysisofthedetritalzirconsfromtheEdiacaran
GrandmontFm.and theCambrianSeries2 MarcoryFm.
suggestsachangeovertimeinthesourcing.TheEdiacaran
sedimentsweredepositedinanarrowback-arcbasinfar
from the influence of far cratonic sources, whereas
CambrianSeries2detritalsedimentswerederivedfrom
maturesourcerocksinvolvingthedenudationofdifferent
Gondwanancratons.
Acknowledgements
The authors thank constructive criticism made by
O. Bleinand B. Laumonier, and founding fromthe RGF
program of theFrench Geological Survey (BRGM). This
paperisacontributiontoprojectCGL2013-48877-Pfrom
SpanishMINECO.
AppendixA. Supplementarydata
Supplementarydataassociated withthisarticlecanbe
found,intheonlineversion, athttp://dx.doi.org/10.1016/j.
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