A Laurentian provenance for the Dalradian rocks of north Mayo, Ireland, and evidence for an original...
Transcript of A Laurentian provenance for the Dalradian rocks of north Mayo, Ireland, and evidence for an original...
doi:10.1144/0016-76492009-147 2010; v. 167; p. 1033-1048 Journal of the Geological Society
Claire A. McAteer, J.Stephen Daly, Michael J. Flowerdew, Martin J. Whitehouse and Chris L. Kirkland
ComplexGneissevidence for an original basement�cover contact with the underlying Annagh
A Laurentian provenance for the Dalradian rocks of north Mayo, Ireland, and
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Journal of the Geological Society, London, Vol. 167, 2010, pp. 1033–1048. doi: 10.1144/0016-76492009-147.
1033
A Laurentian provenance for the Dalradian rocks of north Mayo, Ireland, and
evidence for an original basement–cover contact with the underlying Annagh
Gneiss Complex
CLAIRE A. MCATEER1*, J. STEPHEN DALY 1, MICHAEL J. FLOWERDEW 2,
MARTIN J. WHITEHOUSE 3 & CHRIS L. KIRKLAND3
1UCD School of Geological Sciences, University College Dublin, Belfield, Dublin 4, Ireland2British Antarctic Survey, High Cross, Madingley Road, Camfbridge CB3 0ET, UK
3Laboratory for Isotope Geology, Swedish Museum of Natural History, S-104 05, Stockholm, Sweden
*Corresponding author (e-mail: [email protected])
Abstract: Metasediments of the early Dalradian Grampian Group (Erris Group) and probable equivalents
(Inishkea Division) structurally overlie Palaeoproterozoic to Neoproterozoic Annagh Gneiss Complex
orthogneisses in NW Mayo, Ireland. Sm–Nd isotopic data suggest a Palaeoproterozoic source for the
metasediments. K-feldspar and granitoid clasts from the Doonamo Formation, Erris Group, record U–Pb
zircon ages of c. 1740 Ma and c. 980 Ma, respectively. These ages are within error of the c. 1730–1750 Ma
Mullet gneisses and c. 990 Ma Grenvillian migmatitic leucosomes in the underlying Annagh Gneiss Complex.
U–Pb detrital zircon data reveal that the Erris Group was deposited after c. 955 Ma, with predominant input
from c. 1640, c. 1500 and c. 990 Ma interpreted Laurentian sources (Labradorian, Pinwarian and Grenvillian
terranes, respectively). Limited detrital zircon data from the Inishkea Division yield similarly aged detritus
and a tentative maximum depositional age of c. 1005 Ma. Correlation of both sequences with the Scottish
Dalradian Grampian Group is considered valid based on detrital zircon U–Pb and whole-rock Sm–Nd data.
The clast ages support the hypothesis that the Dalradian unconformably overlies the Annagh Gneiss Complex
in north Mayo, whereas the detrital zircon data imply more distal Laurentian sources. Dalradian deposition is
thereby tied to the margins of Laurentia.
Supplementary material: U–Pb zircon (secondary ion mass spectrometry) data and descriptions of dated
zircon grains are available at http://www.geolsoc.org.uk/SUP18414.
Basement–cover relationships are crucial in reconstructing pa-
laeogeography as they link younger cover sequences to older
basement rocks at the time of deposition. However, these
relationships can be obscured by deformation, possibly leading to
misinterpretations, inappropriate tectonic models and erroneous
past continental configurations. In north Mayo, Ireland, the
Dalradian Supergroup, a major continental margin sequence,
thought to have been deposited on the Laurentian margin of the
Iapetus ocean (Cawood et al. 2003; Banks et al. 2007),
structurally overlies its postulated basement, the Palaeoprotero-
zoic to Neoproterozoic Annagh Gneiss Complex (Max & Long
1985; Kennedy & Menuge 1992; Fitzgerald et al. 1994;
Winchester & Max 1996; Daly 2001, 2009). Western Ireland is
one of the few places where the potential basement to the
Dalradian can be observed. The only other exposures are in the
Central Highlands, Scotland, where the Dalradian may rest
unconformably on the Glen Banchor and Dava Successions of
possible Moine affinity (Piasecki 1980; Robertson & Smith
1999; Strachan et al. 2002), and in the Inner Hebrides, Scotland,
where the Colonsay Group (possible lower Dalradian) rests
unconformably on the Palaeoproterozoic Rhinns Complex
(McAteer et al. 2010).
Early Dalradian deposition took place in the Neoproterozoic
(Dempster et al. 2002), a critical interval in Earth’s history that
saw the break-up of the supercontinent Rodinia, possible glacia-
tion of the entire planet and the emergence of the first hard-
bodied organisms (Grotzinger et al. 1995; Dalziel 1997; Hoffman
et al. 1998; Karlstrom et al. 2000). A better understanding of the
Neoproterozoic palaeogeography of Rodinia may help establish
how the past continental configurations evolved and how an
evolving palaeogeography influenced these phenomena. However,
in the case of north Mayo, Caledonian tectonics (Sanderson et al.
1980) has hampered efforts to decipher the relationship between
the Dalradian metasediments and the structurally underlying
Annagh Gneiss Complex. In the absence of clear field relation-
ships, other methods need to be employed.
In this paper U–Pb detrital zircon data are presented for the
lower Dalradian Grampian Group (Erris Group) and probable
equivalents (Inishkea Division), which structurally overlie the
Annagh Gneiss Complex in north Mayo. The data are compared
with possible source areas whose chronology is well established
(including the Annagh Gneiss Complex) and with U–Pb detrital
zircon data from the Grampian Group of Scotland (which has a
unique detrital zircon signature distinct from the rest of the
Dalradian; Cawood et al. 2003, 2007; Banks et al. 2007). Other
potential correlatives (i.e. the upper part of the Dalradian and
other major Neoproterozoic stratigraphic sequences such as the
Moine Supergroup and the Torridonian; Rainbird et al. 2001;
Cawood et al. 2003, 2004; Friend et al. 2003; Kinnaird et al.
2007; Kirkland et al. 2008) are also examined.
In addition to the detrital zircon study, whole-rock geochem-
istry and Sm–Nd isotopic analyses are presented for both the
Erris Group and the Inishkea Division as well as U–Pb zircon
ages for K-feldspar and granitoid clasts from pebbly horizons
within the Erris Group, which are petrographically similar to
lithologies within the Annagh Gneiss Complex.
The data are used to investigate the source(s) of the metasedi-
ments, possible correlatives and their relationship to the under-
lying Annagh Gneiss Complex. On a broader scale the data shed
some light on Neoproterozoic palaeogeography at the time these
rocks were deposited.
Geological setting
Metasediments of the Erris Group and Inishkea Division structu-
rally overlie the Palaeoproterozoic to Neoproterozoic Annagh
Gneiss Complex in north Mayo, Ireland (Fig. 1). Winchester &
Max’s (1996) unified stratigraphy for the Erris Group in Mayo is
adopted in this work (Table 1). Although there has been no
formal stratigraphic subdivision of the Inishkea Division, single
occurrences are ascribed informal stratigraphic names based on
location (e.g. Kinrovar Schist, Scotch Port Schist). The metasedi-
ments, the Annagh Gneiss Complex and basement–cover rela-
tionships are discussed sequentially below.
Metasediments (Erris Group and Inishkea Division)
The banded quartz–plagioclase–mica psammites and locally
pebbly horizons of the Erris Group (Winchester et al. 1988;
Winchester & Max 1996; Daly 2001, 2009; Fig. 1) pass
stratigraphically upwards into Dalradian (Appin Group) rocks
(Winchester et al. 1988; Winchester & Max 1996). Thus the
Erris Group is generally accepted to belong to the Dalradian
Grampian Group (Winchester & Max, 1996; Table 1).
Fig. 1. Schematic geological map of the study area adapted from Kennedy & Menuge (1992), Max et al. (1992), Winchester & Max (1996) and Daly &
Flowerdew (2005). Sample numbers and Sm–Nd model ages (Ma) are shown in white text with black boxes. White stars denote XRF and Sm–Nd
analyses only. Black stars denote XRF, Sm–Nd and U–Pb zircon analyses. Clasts C61B-1, C61B-10, C61D-30 and C61G-7 are from the same locality as
C61A. Inset map adapted from Chew et al. (2008). MT, Moine Thrust; GGF, Great Glen Fault; HBF, Highland Boundary Fault; FCBL, Fair Head–Clew
Bay Line; SUF, Southern Uplands Fault.
C . A. McATEER ET AL .1034
The relationship between the Inishkea Division and the
Dalradian Supergroup has proven more controversial. First recog-
nized by Trendall & Elwell (1963), the strongly foliated schists
and psammitic gneisses of the Inishkea Division were originally
believed to be part of an older, pre-Dalradian, Erris Complex
(Crow et al. 1971; Max & Sonet 1979; Winchester & Max
1984), which also included the Annagh Gneiss Complex. They
were later described as the products of Caledonian reworking of
rocks similar to the Annagh gneisses (Sutton & Max 1969; Crow
& Max 1976). Ambiguous structural evidence (Crow & Max
1976; Max & Long 1985; Winchester & Max 1987) and Rb–Sr
data (Max et al. 1983) then led to the suggestion that the
Inishkea Division metasediments were younger than the Annagh
gneisses but older than the Dalradian.
Kennedy & Menuge (1992, 1993) argued that there is no
evidence, structural or isotopic, to support a pre-Dalradian age
for the Inishkea Division (Yardley et al. (1987) also questioned
previous structural evidence). Furthermore, they recorded a
stratigraphic contact between the Inishkea Division and overlying
Erris Group north of Scotch Port and with rocks of possible
Appin Group affinity at Kildun (Fig. 1; Kennedy & Menuge
1992). This led them to infer that parts of the Inishkea Division
(namely the Kinrovar Schist) may belong to the Appin Group
(Kennedy & Menuge 1992). The rocks at Kildun, however, were
placed in the Erris Group by Winchester & Max (1996; and are
depicted as such in Fig. 1). Whereas Max & Winchester (1993)
maintained that all contacts between the Inishkea Division and
the Dalradian are tectonic, Daly (2001) also reported strati-
graphic contacts between them.
Interpretations of the depositional setting for both the Erris
Group and the Inishkea Division are complicated by Caledonian
metamorphism and deformation, which also inhibit rigorous
basin analysis (Daly 2001). The Erris Group is thought to have a
fluviatile to marginal marine setting (Winchester et al. 1988;
Daly 2001), whereas the Inishkea Division may represent a suite
of greywackes deposited in a restricted basin (Winchester & Max
1987). Cross-bedding, channelling and compaction structures
have been recorded in the Erris Group (Winchester et al. 1988;
this study). Graded bedding, slump conglomerates and bottom
compaction structures have been reported in the Inishkea Divi-
sion (Max & Winchester 1993).
The Inishkea Division and the Erris Group are geochemically
similar to the Grampian Group in Scotland (Max & Winchester
1993; Winchester & Max 1996) and both sequences have similar
whole-rock Sm–Nd depleted mantle model ages (tDM; Inishkea
Division 1609–1986 Ma; Erris Group 1619–1754 Ma; Kennedy
& Menuge 1992; J. S. Daly & J. F. Menuge, unpubl. data) to the
Scottish Grampian Group (Banks et al. 2007; J. S. Daly & J. F.
Menuge, unpubl. data). When combined with the stratigraphic
relationships outlined above, these geochemical and isotopic
similarities suggest that the Inishkea Division and the Erris
Group are probable correlatives and that both probably correlate
with the Scottish Grampian Group. Based on geochemical
characteristics, an Appin Group affinity for the Kinrovar Schist
(Inishkea Division; Kennedy & Menuge 1992, 1993), is, how-
ever, unlikely (Max & Winchester 1993).
Annagh Gneiss Complex
The predominantly Palaeoproterozoic, granodioritic to granitic
orthogneisses (Winchester & Max 1984; Daly 2001) of the
Annagh Gneiss Complex (Kennedy & Menuge 1992; Menuge &
Daly 1994) structurally underlie the Erris Group and the Inishkea
Division in north Mayo (Fig. 1). Formerly part of the Erris
Complex (Crow et al. 1971), and originally considered to be of
Archaean age (Hull 1882), the Annagh gneisses were later
reinterpreted as Caledonian migmatites developed from the
surrounding metasedimentary rocks (Kilroe 1907; Trendall &
Elwell 1963; Phillips et al. 1969). This interpretation prevailed
until Sutton & Max (1969) recognized that the Annagh gneisses
were intensely deformed prior to the Caledonian orogeny and
Brindley (1969) suggested that Hull’s (1882) interpretation be re-
examined. It has since been demonstrated that the Annagh
Gneiss Complex, the protoliths of which were shown to be of
plutonic origin (based on geochemistry and field evidence;
Winchester & Max 1984), was deformed during the Grenville
orogeny (van Breemen et al. 1976, 1978; Max & Sonet 1979;
Aftalion & Max 1987). Menuge & Daly (1990) suggested that
the Annagh gneisses represented crust that formed in two distinct
episodes, one at c. 1.9 Ga and the other at c. 1.35 Ga.
The chronology of the Annagh Gneiss Complex is now well
established (Table 2; Daly 1996, 2001, 2009; Daly & Flowerdew
2005) and it can be divided into the c. 1.75 Ga Mullet gneiss, c.
1.28 Ga Cross Point gneiss and c. 1.18 Ga Doolough gneiss (Fig.
1; Daly 1996). The Mullet gneisses are characterized by
migmatized quartzofeldspathic orthogneisses and locally darker
micaceous bands. Compositionally they are I-type metaluminous
monzodiorites, granodiorites (which predominate) and granites
with a magmatic arc chemistry (Daly 1996). The syenitic to
granitic Cross Point gneiss displays A-type, within-plate geo-
chemistry (Fitzgerald et al. 1996). Pre-Grenville amphibolite
bodies occur in both the Mullet and Cross Point gneisses (Daly
1996). The Doolough gneisses consist of subalkaline granites
and trondhjemites with some amphibolite. These juvenile
gneisses, which are very highly strained, are cut by the c.
1015 Ma Doolough Granite (Daly 1996). Several generations of
Grenville-aged granite–pegmatite sheets cut the Annagh Gneiss
Complex (Daly 1996; Table 2).
Grenville deformation of the Annagh Gneiss Complex oc-
curred in three phases (Daly 1996). The first two phases occurred
between c. 1177 and c. 1015 Ma (Daly 1996). The third event
took place between c. 995 and c. 960 Ma (Daly 1996). There is
no evidence to suggest that the Annagh Gneiss Complex was
affected by a post-Grenville, pre-Grampian orogeny (Daly &
Table 1. Simplified stratigraphy of the north Mayo Dalradian adapted from Winchester & Max (1996) with likely position of the Inishkea Division
North Mayo Dalradian Scottish Dalradian Dalradian Supergroup
Benmore FormationBroad Haven Formation
9>>=>>;
9=; Glen Spean Subgroup
9>>>>=>>>>;
Belderg FormationErris Group
Grampian GroupDoonamo Formation
�Corrieyairack Subgroup
Inishkea Division
PROVENANCE OF THE NORTH MAYO DALRADIAN 1035
Flowerdew 2005). The pre-Caledonian history of the Annagh
Gneiss Complex is summarized in Table 2.
Detailed descriptions of the Annagh Gneiss Complex ortho-
gneisses have been given by Winchester & Max (1984, 1988)
and Daly (1996, 2001, 2009). Details of field relationships have
been given by Sutton (1969, 1972), Sutton & Max (1969), Max
(1970) and Menuge & Daly (1990).
Basement–cover relationships
All contacts between the Erris Group, the Inishkea Division, and
other parts of the Dalradian with the Annagh Gneiss Complex
are tectonic. However, the metasediments consistently face away
from the orthogneisses (Max & Long 1985; Winchester et al.
1988; Winchester & Max 1996), and post-Grenville metadoler-
ites cutting the Annagh Gneiss Complex are similar to pre-
deformational dykes in both the Erris Group and the Inishkea
Division (Sutton 1972; Winchester & Max 1988; Menuge &
Daly 1990; Kennedy & Menuge 1992; Fitzgerald et al. 1994;
Daly 1996). This suggests that the metasediments were stitched
together with the older ‘basement’ prior to deformation. Sm–Nd
isotopic data demonstrate that both the Inishkea Division and the
Erris Group were derived from a Palaeoproterozoic source
similar to the Annagh Gneiss Complex (Kennedy & Menuge
1992; J. S. Daly & J. F. Menuge, unpubl. data). Moreover, K-
feldspar and granitic clasts, from pebbly horizons within the
Erris Group, petrographically resemble lithologies within the
Annagh Gneiss Complex (Fig. 2). All of these observations
suggest that the Annagh Gneiss Complex represents the deposi-
tional basement to the Dalradian of NW Ireland.
Sample descriptions and localities
One psammite and four clasts (three K-feldspar clasts and one
granitoid clast) were sampled from the stratigraphically lowest
subdivision of the Erris Group, the Doonamo Formation. In
addition, four mica schists from the Inishkea Division were also
sampled (Fig. 1).
Samples of the Doonamo Formation were collected along a
shoreline exposure at Spinkadoon (Fig. 1). At this locality beds
up to 1 m thick of tabular, laterally continuous psammites are
interbedded with thin bands of mica schist (up to c. 20 cm thick)
and occasional pebble beds (eight pebble horizons were identi-
fied). Bedding strikes roughly east–west, dips c. 508 to the south
and youngs to the south away from the structurally underlying
Annagh Gneiss Complex. The rocks are foliated, more intensely
so in the finer-grained mica-schist horizons. The foliation dips
shallowly to the north, cutting bedding at an angle of c. 408.
Channelling, cross-bedding, trough cross-bedding and hummocky
cross-stratification were observed in the psammites (Fig. 2b).
The pebble beds are matrix-supported, display erosive bases
and appear to pinch out laterally. The pebbles occur predomi-
nantly towards the tops of the beds and are elongated as a result
of strain during the Caledonian orogeny (Sanderson et al. 1980).
In the thicker pebble horizons (Fig. 2a), the pebbles are
distributed throughout the bed. Granitoid and quartzo-feldspathic
gneissic pebbles are common as well as centimetre-sized quartz
and K-feldspar clasts. The pelitic matrix of these beds consists of
quartz (33%), biotite (28%), epidote (14%), muscovite (9%),
opaque minerals (9%) and minor amounts of apatite, plagioclase,
orthoclase, microcline and titanite.
The sedimentary structures in the psammites suggest a shallow
marine depositional setting, with the hummocky cross-stratifica-
tion indicative of deposition between fair-weather wave base and
storm wave base. The pebble beds may represent transgressive
lag deposits, which would have formed as the shoreline retreated
causing a winnowing of coarser material and reworking of some
of the material below. This seems to be the case for the pebble
horizon displayed in Figure 2a, where a small lens of coarser
material in the underlying psammite might suggest a reworking
event. However, the frequency of these pebble horizons (eight
occurrences over c. 35 m) suggests that they are unlikely to be
entirely controlled by transgressive events. An alternative expla-
nation is that the pebble horizons may represent interfingering
between a deltaic front and shoreline deposits, where debris
flow-like deltaic deposits are interspersed with shallow marine
deposits. This would account for the frequency of pebble
horizons. A combination of these scenarios is also possible.
One psammite (C61A) and four pebbles (K-feldspar clasts
C61B-1, C61B-10 and C61D-30, and C61G-7, a granitoid clast)
were collected at Spinkadoon. C61B-1 and C61B-10 were
sampled from a pebble horizon [F681391] c. 4 m above C61A.
C61D-30 was sampled 4 m above this and C61G-7 was collected
from a stratigraphically lower pebble horizon almost 40 m below
C61A [F682392]. C61A is a quartz-rich (55%) psammite
(average grain size c. 200 �m) with muscovite (15%), biotite
(5%), epidote (10%), K-feldspar (5%; mostly orthoclase with
minor microcline) and minor amounts of plagioclase, opaque
minerals, titanite, zircon and apatite. The micas define a weak
foliation. Clasts C61B-1, C61B-10 and C61G-7 are coarse-
grained K-feldspar crystals and probably represent fragments of
granitic pegmatite. They are petrographically similar to Grenville
pegmatites in the Annagh Gneiss Complex and older K-feldspar
megacrystic sections of the Mullet gneisses (Fig. 2c). C61B-1
consists of a large, centimetre-sized perthite crystal (with some
clay and chlorite alteration) with inclusions of fine-grained white
Table 2. Pre-Grampian history of the Annagh Gneiss Complex
Age (Ma) Event
1753 � 3 Formation of Mullet gneiss protolith (crustal addition of juvenile magma); c. 1730–1750 Ma zircon alsoreported*
1271 � 6, 1287 +38/�35 Formation of Cross Point gneiss protolith at Tristia and Cross Point (anorogenic magmatism)1177 � 4 Formation of Doolough gneiss protolith (crustal addition of juvenile magma)
DG1 and DG2 Grenville deformation events1015 � 4 Intrusion of peralkaline Doolough Granite at Dooloughc. 999–980 Migmatization and pegmatite injection958 +17/�19 Metamorphic zircon defining DG3 Grenville foliation943 � 8† Post-tectonic titanite growth
Data from Daly (1996); additional data sources: * J. S. Daly (unpubl. data); † Daly & Flowerdew (2005).
C . A. McATEER ET AL .1036
mica, quartz, K-feldspar, epidote, zircon, opaque minerals and
small veinlets of finer-grained quartz, K-feldspar, epidote and
opaque minerals. C61B-10 consists of a microcline crystal (with
clay and chlorite alteration), c. 1.5 cm in size with inclusions of
white mica, opaque minerals, quartz, orthoclase, zircon and
epidote. C61G-7 is made up of a large, fractured orthoclase
crystal (with clay and chlorite alteration) about 1.2 cm in size
with inclusions of quartz, orthoclase, plagioclase, epidote, white
mica, zircon and opaque minerals and cross-cutting veinlets of
quartz, orthoclase, and plagioclase. C61D-30 is petrographically
similar to c. 990 Ma migmatitic leucosomes from Annagh Head
(Daly 1996) and consists of large microcline crystals up to
0.5 cm in size with finer-grained recrystallized quartz and K-
feldspar, some opaque minerals and fine-grained white mica and
minor amounts of zircon and biotite, partly replaced by chlorite.
Schists from the Inishkea Division (C62, C63, C66B, C67)
were collected at Carricklahan, Kinrovar, Tiraun Point and
Scotch Port (Fig. 1). Unlike the Doonamo Formation at Spinka-
doon, these rocks are strongly deformed and as a result
sedimentary structures, including bedding, are difficult to distin-
guish. Sample C62, of Carricklahan Schist (Max et al. 1992; Fig.
1), consists of quartz, biotite, muscovite, feldspar porphyroblasts
(plagioclase and K-feldspar with inclusions of quartz and white
mica), epidote and minor amounts of apatite, opaque minerals,
titanite and zircon. A strong foliation, defined by quartz, biotite,
muscovite and epidote, wraps around the feldspar porphyroblasts,
suggesting that they formed before the foliation. Compositional
layering, possibly defining original bedding, strikes roughly
NW–SE and dips about 608 northeastwards.
Sample C63, from the Kinrovar Schist (Fig. 1) is a coarse-
grained porphyroblastic schist comprising quartz, biotite, musco-
vite, garnet, feldspar porphyroblasts (plagioclase and K-feldspar
with inclusions of quartz, white mica, opaque minerals and
garnet), zircon and apatite. Biotite (with inclusions of zircon and
some chlorite replacement) and muscovite define a foliation that
wraps around the feldspar porphyroblasts. Garnet occurs as
inclusions within the feldspar porphyroblasts but can also be
found occasionally defining the foliation, possibly suggesting two
generations of garnet growth. Kennedy & Menuge (1992)
described the rocks from this locality, which are layered on a
scale of 5–30 cm, as pelitic porphyroblastic oligoclase or albite
garnet schists with muscovite and biotite. Sample C66B was
collected from the coast at Tiraun Point (Fig. 1) and is
petrographically similar to C63. A sample of the Scotch Port
Schist, C67 (Fig. 1), contains quartz, biotite, muscovite, garnet
porphyroblasts and some apatite, zircon and titanite. A strong
foliation, defined by biotite and muscovite, wraps around the
garnet porphyroblasts (which have fine-grained inclusions of
white mica and quartz), implying that the foliation post-dates
porphyroblast growth.
Sample preparation and analytical methods
Whole-rock major and trace element analyses and Sm–Nd
isotopic analyses were carried out on all samples, excluding
clasts, for which there was insufficient material. The Doonamo
Formation clasts (C61B-1, C61B-10, C61D-30, C61G-7) were
dated by the U–Pb zircon method and a U–Pb detrital zircon
study was carried out on samples C61A (Doonamo Formation
psammite, Erris Group), C63 (Kinrovar Schist, Inishkea Divi-
sion) and C67 (Scotch Port Schist, Inishkea Division).
Weathered material and veins were removed from samples
prior to crushing in a Retsch tungsten carbide jaw-crusher.
Whole-rock aliquots (c. 100 g) were milled in a tungsten carbide
Fig. 2. Doonamo Formation (Erris Group), Spinkadoon and Mullet
gneiss, Annagh Head. (a) A c. 20 cm thick pebble bed from the
Doonamo Formation (C61B-1 and C61B-10 sampled from this horizon)
overlying a cross-bedded psammite with lenses of coarser-grained
material at Spinkadoon. Photograph looking east; beds young to the
south. (b) Cross-bedding and hummocky cross-stratification, Spinkadoon.
(c) K-feldspar megacrystic orthogneiss (Mullet gneiss) and later
Grenville pegmatite, Annagh Head.
PROVENANCE OF THE NORTH MAYO DALRADIAN 1037
Tema mill. Major and trace element analyses (Table 3) were
carried out by X-ray fluorescence (XRF) spectrometry at the
Department of Geology, University of Leicester on fusion beads
and pressed powder pellets respectively.
Chemical separation of Sm and Nd for isotopic analysis
followed Pin et al. (1994) using TruSPEC and LN resins. Sm–
Nd isotope analyses (Table 4) were carried out on spiked samples
using a multi-collector VG 354 mass spectrometer at the School
of Geological Sciences, University College Dublin. Concentra-
tions were calculated offline from the measured ratios, following
correction for mass fractionation and spike addition. 143Nd/144Nd
ratios are relative to a 143Nd/144Nd ratio of 0.511850 for the La
Jolla standard (see Table 4).
Zircon grains were separated from �250 �m fractions using
di-iodomethane. Detrital mineral grains were randomly selected,
whereas those from clasts were selected by grain size, turbidity
and state of alteration in view of their expected igneous protolith.
Zircon grains were cast in an epoxy mount, polished and imaged
in both reflected and transmitted light. The gold-coated mount
was imaged by scanning electron microscopy (SEM) using
secondary electron (SE) and cathodoluminescence (CL) detectors
to determine the internal structure of the grains so as to guide in
situ analysis.
Zircon grains were analysed by secondary ion mass spectro-
metry (SIMS) on the NORDSIM Cameca IMS 1270 ion micro-
probe at the Swedish Museum of Natural History, Stockholm,
Sweden. U–Th–Pb zircon analyses followed the methods de-
scribed by Whitehouse & Kamber (2005). Pb/U calibration was
carried out using the 1065.4 � 0.3 Ma Geostandards zircon
91500, with U and Pb concentrations of 80 ppm and 15 ppm
respectively (Wiedenbeck et al. 1995). Common Pb corrections
were applied to a minority of data with 206Pb/204Pb ratios ,3000
(indicating significant common Pb), using the present-day terres-
trial common Pb estimate of Stacey & Kramers (1975). This
Table 3. Whole-rock major and trace element data for the Erris Group and the Inishkea Division
Erris Group Inishkea Division
Doonamo Formation Carricklahan Schist Kinrovar Schist Tiraun Point Scotch Port SchistC61A C62 C63 C66B C67
Oxides (wt %)SiO2 73.49 65.16 62.08 60.40 59.85TiO2 0.47 1.06 0.89 0.84 0.80Al2O3 11.84 13.77 16.60 17.25 17.77Fe2O3 3.53 6.45 6.62 6.74 6.63MnO 0.05 0.10 0.10 0.11 0.11MgO 0.78 1.63 2.10 2.43 2.80CaO 1.95 3.25 2.08 2.02 1.54Na2O 2.79 3.07 3.88 2.45 2.41K2O 3.11 3.19 2.93 4.10 4.70P2O5 0.06 0.20 0.26 0.27 0.23LOI 0.67 0.86 1.20 1.62 1.76Total 98.74 98.74 98.79 98.25 98.61Trace elements (ppm)Ba 934 893 767 1008 1192Cr 37 42 51 55 53Cu b.d. 9 24 34 18Ga 12 16 19 21 24Mo 1 1 1 2 1Nb 11 21 17 16 14Ni 8 14 23 31 29Pb 16 19 19 20 57Sc 8 13 16 16 17Th 4 14 13 15 16U 2 4 4 3 4V 42 90 93 97 99Y 20 43 37 23 34Zn 30 68 85 100 153Zr 167 563 301 205 164La 21 51 51 30 47Ce 46 114 105 64 90Sm 4 10 8 5 7Nd 23 54 43 27 40Cs b.d. 2 5 3 6Rb 92 117 115 157 189Sr 326 314 292 218 208SiO2/Al2O3 6.21 4.73 3.74 3.50 3.37Fe2O3/K2O 1.14 2.02 2.26 1.64 1.41Cr/Zr 0.22 0.07 0.17 0.27 0.32Rb/Sr 0.28 0.37 0.39 0.72 0.91Y/Sr 0.06 0.14 0.13 0.11 0.17Zr/Sc 19.71 43.81 18.78 12.76 9.82
LOI, loss on ignition. b.d., concentration below the lower limit of detection. Sm and Nd concentrations determined by TIMS.
C. A. McATEER ET AL .1038
assumes that any common Pb detected was due to surface
contamination during sample preparation.
All ages were calculated and plots generated using Isoplot
3.00 (Ludwig 2003). All ages are concordia ages (Ludwig 1998)
unless otherwise stated. All errors in ages presented and
discussed in the text are quoted at the 2� level; concordia age
errors are 2� except for those .100 Ma, which represent 95%
confidence levels. For U–Pb zircon geochronology of clasts only
data whose error ellipse intersects concordia are used to calculate
a concordia age. The same criterion was adopted to screen
analyses of detrital grains prior to plotting on age distribution
diagrams. Discordant data are discussed below. Where core and
rim ages are available for the same detrital grain only the rim
age is included in the age distribution plot. The significance of
corresponding cores is discussed below.
Results
Whole-rock geochemistry
Major and trace element analyses are listed in Table 3. Samples
C63, C66B and C67 (Inishkea Division from Kinrovar, Tiraun
Point and Scotch Port, respectively) plot as shales on a
log(Fe2O3/K2O) v. log(SiO2/Al2O3) plot (Herron 1988; Fig. 3).
Using the same parameters, C62 (Carricklahan Schist, Inishkea
Division) plots as a greywacke and C61A (Doonamo Formation,
Erris Group) plots as a borderline arkose–litharenite–greywacke.
Cr/Zr ratios (Table 3) are low, consistent with predominant input
from an acidic source region (Winchester & Max 1996). In
addition, low Rb/Sr and Y/Sr ratios (Table 3) suggest that these
sediments are immature (Winchester & Max 1996). Excluding
sample C62, Zr/Sc ratios are less than 30, consistent with
minimal sedimentary recycling (McLennan et al. 2003). Whereas
trace element signatures are similar for all samples (Fig. 4a), the
psammitic sample C61A is less enriched in REE than the more
pelitic samples. The trace element signatures of the analysed
samples are similar to average values for the Scottish Grampian
Group (Winchester & Glover 1988; Fig. 4b).
Sm–Nd data
Results are listed in Table 4. The single Erris Group sample from
the Doonamo Formation (sample C61A) yields a whole-rock
Sm–Nd model age (tDM) of 1723 Ma, Inishkea Division rocks
(samples C62, C63, C66B, C67) yield tDM ranging from 1728 to
1829 Ma (Fig. 1) and �Nd values for all samples lie within the
Sm–Nd evolutionary field of the Annagh Gneiss Complex (Fig.
5; Menuge & Daly 1990).
U–Pb zircon geochronology
C61B-1, K-feldspar clast, Doonamo Formation, Erris Group,
Spinkadoon. Zircon grains from C61B-1 (Fig. 6) comprise sub-
rounded, oscillatory-zoned prisms of 48–110 �m width and 82–
232 �m length, with a mean Th/U value of c. 0.3 consistent with
an igneous origin (Belousova et al. 2002). Eight out of 18
analyses (from five out of 12 zircon grains) define a concordia
age of 1743 � 4 Ma (Fig. 7a). This age is interpreted as the
magmatic age of the clast. Analyses of zircon rims are discordant
and, in common with the other discordant analyses, have been
variably influenced by recent Pb loss, all but four of which define
a weighted mean 207Pb/206Pb age (1744 � 6 Ma) within error of
the concordia age. These four analyses (spots 11, 2a, 3 and 7a),Table4.Whole-rock
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PROVENANCE OF THE NORTH MAYO DALRADIAN 1039
when anchored to 1743 Ma, define a discordia with a lower
intercept of 690 � 4 Ma (Fig. 7a).
C61B-10, K-feldspar clast, Doonamo Formation, Erris Group,
Spinkadoon. Zircon grains from C61B-10 comprise mainly pink
prismatic, oscillatory-zoned grains (Fig. 6) of 50–65 �m width
and 87–105 �m length. Six out of 10 analyses (from three out of
six zircon grains dated) yield a concordia age of 1744 � 6 Ma
(Fig. 7b). All analyses have Th/U ratios (c. 0.3) consistent with a
magmatic origin and, as such, the concordia age is interpreted as
dating the clast. Discordance of the remaining data (spots 2, 4b,
5 and 5b) may be explained by Pb loss (Fig. 7b).
C61G-7, K-feldspar clast, Doonamo Formation, Erris Group,
Spinkadoon. Only two analyses were obtained from a single
oscillatory-zoned prismatic zircon grain from sample C61G-7
(Fig. 6). One of these intersects concordia whereas the other is
reversely discordant. The data define a weighted mean 207Pb/206Pb age of 1750 � 12 Ma, which is interpreted as the magmatic
age of the clast, given its petrography and Th/U ratio (c. 0.27).
C61D-30, granitoid clast, Doonamo Formation, Erris Group,
Spinkadoon. Zircon grains from C61D-30 comprise mainly pink
and brown broken, rounded and sub-rounded prisms, most of
which display oscillatory zoning (Fig. 6). Five out of six grains
have low Th/U ratios (,0.02) and generally high U contents.
Five out of 13 analyses (spots 3, 3b, 6, 4 and 4b) plot near one
another on concordia but overlap insufficiently to define a
concordia age (Fig. 7c). Three of these (spots 3, 3b and 6) yield
a concordia age of 982 � 13 Ma. Alternatively a concordia age
of 973 � 13 Ma can be calculated from spots 3, 3b and 4. Spots
2a, 2c and 7 are reversely discordant, probably as a result of their
high U concentrations (3464 ppm, 3620 ppm and 3165 ppm,
respectively), which invalidates the standard calibration (91500
has only 81 ppm U; Fig. 7c). However, this does not affect the207Pb/206Pb ratios, and all eight analyses define a weighted mean207Pb/206Pb age of 972 � 8 Ma (MSWD ¼ 3.6, Fig. 7c). This age
is interpreted as dating the formation of the zircon in this clast,
possibly in a metamorphic event in view of the low Th/U ratios.
Given the high U concentrations of these grains, however, the
Th/U ratios could be misleading as an indicator of zircon growth
conditions. Of the remaining discordant data, spots 2b, 3c and 4c
are consistent with recent Pb loss (Fig. 7c) and yield a weighted207Pb/206Pb age within error of the age of the clast
(953 � 13 Ma). Spot 5 yields a 207Pb/206Pb age of 1022 � 49 Ma
and may indicate the presence of an inherited component (Fig.
7c). When plotted with the concordant analyses, spot 1 lies along
a discordia with lower and upper intercepts of 477 � 79 Ma and
964 � 12 Ma, respectively, consistent with Grampian Pb loss
(Fig. 7c).
C61A, detrital zircon, Doonamo Formation, Erris Group, Spinka-
doon. Zircon grains from C61A are 63–185 �m wide and 110–
285 �m long, colourless, pink and brown in colour, and rounded
to sub-rounded in shape. Most exhibit oscillatory zoning but
some sector-zoned grains are also present (Fig. 6). Zircon age is
independent of zircon colour and morphology. Of the grains
analysed 84 out of 99 yield a range of concordant ages between
c. 950 Ma and c. 1740 Ma, with peaks at c. 990 Ma, 1500 Ma
and 1640 Ma (Fig. 8). The youngest concordant detrital zircon
(grain 103, a CL-dark, unzoned grain) yields a concordia age of
955 � 12 Ma (Fig. 9). Another, possibly younger grain (grain
57), whose error ellipse barely touches concordia (Fig. 9), has a206Pb/238U age of 919 � 21 Ma (and a concordia age of
928 � 310 Ma). This grain is interpreted to have experienced Pb
loss, however, and is not deemed a reliable constraint on the
maximum depositional age of the Doonamo Formation. Its 207Pb/206Pb age of 986 � 51 is within error of that of the more robust
analysis of grain 103 (i.e. c. 955 Ma). We therefore interpret that
deposition of the Doonamo Formation took place after c.
955 Ma.
Dating cores and rims can potentially yield additional insight
into provenance by identifying inherited zircon components; how-
ever, this is rarely possible because of grain size limitations and
the diverse opportunities for discordance. Corresponding cores
and rims were dated in three grains; however, only one, grain 1,
yielded concordant data for both parts. Grain 1 has an oscillatory-
zoned core dated at 1377 � 19 Ma (spot 1b), and a CL-bright,
zoned rim (spot 1a) with an age of 998 � 15 Ma (Fig. 6).
Sixteen analyses were excluded from the age distribution plot
(Fig. 8) on the basis of discordance. All are within the same age-
range as the concordant data except for grain 3 (207Pb/206Pb age
of 1848 � 12 Ma), grain 57 (206Pb/238U age of 919 � 21 Ma)
and grain 87 (206Pb/238U age of 891 � 16 Ma) (Fig. 9). Grains
Fig. 3. Classification of Erris Group
(C61A) and Inishkea Division (C62, C63,
C66B, C67) samples after Herron (1988)
using log (Fe2O3/K2O) v. log (SiO2/Al2O3).
C. A. McATEER ET AL .1040
57 and 87 are interpreted as having suffered Pb loss and are
probably the same age, within error, as the youngest cluster of
concordant data at c. 1 Ga. (Fig. 9). Grain 3 has also experienced
Pb loss but possibly indicates the presence of an older, c.
1850 Ma component (Fig. 9).
C63, detrital zircon, Kinrovar Schist, Inishkea Division, Kinro-
var. Detrital zircon grains from sample C63 are 60–178 �m wide
and 78–265 �m long, pink or colourless, and exhibit rounded to
sub-rounded morphologies. There is no obvious correlation
between zircon size, type or colour and age. Of the detrital grains
analysed, 12 of 15 yield concordant ages ranging from c.
1110 Ma to c. 1650 Ma (Figs 8 and 9). The zircon yield for this
sample was particularly low, possibly owing to it having a pelitic
protolith (Fig. 3). Grain 9 constrains the maximum depositional
age of the Kinrovar Schist to 1112 � 67 Ma (weighted mean207Pb/206Pb age of core (spot 9a, concordant but large error) and
rim (spot 9b, discordant) analyses, which are interpreted to be
the same age; Fig. 9). However, a younger maximum deposi-
tional age is possible, as grain 1 (Fig. 6) yields a discordant rim
analysis (spot 1b) interpreted as Pb loss from c. 1000 Ma (Figs 8
and 9; 207Pb/206Pb age for this analysis is 1025 � 44 Ma).
Discordant core data from the same grain suggest Pb loss from c.
1650 Ma (spot 1a), indicating an inherited component (Figs 6
and 9).
Analysis of the zoned rim of grain 8 (spot 8c) yields a
concordia age of 468 � 12 Ma. This rim has a very low Th/U
ratio (0.009) and is interpreted as a post-depositional meta-
morphic overgrowth (Fig. 6), formed during the Grampian
orogeny (Daly & Flowerdew 2005).
Fig. 4. Multi-element plots showing trace
element distributions for (a) C61A,
Doonamo Formation (Erris Group), C62,
Carricklahan Schist (Inishkea Division),
C63, Kinrovar Schist (Inishkea Division),
C66B, Inishkea Division (Tiraun Point) and
C67, Scotch Port Schist (Inishkea Division)
and (b) average values for the samples
plotted in (a) and semipelites from the
Corrieyairack and Glen Spean subgroups of
the Scottish Grampian Group (data from
Winchester & Glover 1988). Data
normalized to Average Upper Crust (AUC;
Taylor & McLennan 1981). Black bar
indicates lower limit of detection.
PROVENANCE OF THE NORTH MAYO DALRADIAN 1041
C67, detrital zircon, Scotch Port Schist, Inishkea Division, Scotch
Port. Zircon grains from sample C67 are 79–110 �m wide and
95–220 �m long, oscillatory-zoned and mostly pink or pinkish
brown, sub-rounded prisms. This sample had a poor zircon yield,
which, as for sample C63, is probably attributable to it having a
pelitic protolith (Fig. 3). Four grains from seven yield concordia
ages of 1186 � 22 Ma, 1252 � 26 Ma, 1264 � 26 Ma and
1520 � 15 Ma (spots 6, 1, 7 and 3, respectively; Fig. 9). The
youngest of these provides a reliable maximum age for the
deposition of the Scotch Port schist. The remaining three grains
(grains 2, 4 and 5), when corrected for the presence of common
Pb, yield concordia ages of 1005 � 22 Ma, 1178 � 27 Ma and
1450 � 25 Ma, respectively (spots 2b, 4a and 5b). The youngest
of these, spot 2b, extends the age limit on the time of deposition
to 1005 � 22 Ma. Ages for grains 2 and 5 are based on analyses
of zircon rims (spots 2b and 5b). Corresponding core analyses
for these grains (spots 2a and 5a) indicate c. 1150 Ma and c.
1620 Ma, inheritance, respectively (Fig. 6).
Discussion
Provenance
Palaeoproterozoic whole-rock Sm–Nd tDM values (1723–
1829 Ma) suggest a similar source for the Erris Group and the
Inishkea Division and all ages are within range of previously
determined Sm–Nd data (Kennedy & Menuge 1992; J. S. Daly
& J. F. Menuge, unpubl. data). �Nd values for both sequences are
consistent with an Annagh Gneiss Complex-type source (Fig. 5;).
The samples analysed have similar chemical compositions with
low Cr/Zr ratios indicative of predominant input from an acidic
source (Winchester & Max 1996). In addition, the samples have
relatively low Zr/Sc ratios suggesting minimal sedimentary
recycling (McLennan et al. 2003), which would suggest that the
detrital zircons are probably first cycle.
U–Pb zircon data from four clasts (K-feldspar and granitoid
clasts) within the Doonamo Formation at Spinkadoon are
consistent with derivation from the structurally underlying
Annagh Gneiss Complex. Two of the K-feldspar clasts (C61B-1,
C61B-10) have identical concordia ages with a weighted mean
value of 1743 � 3 Ma, whereas the third (C61G-7) has a 207Pb/206Pb age of 1750 � 12 Ma. These ages are comparable with the
U–Pb thermal ionization mass spectrometry (TIMS) age of 1753
� 3 Ma for the Mullet gneiss of the Annagh Gneiss Complex
(Daly 1996), which also records c. 1730–1750 Ma crystallization
ages (J. S. Daly, unpubl. data). The clasts are coarser-grained
than the samples dated by Daly (1996), although K-feldspar
megacrystic gneisses are common within the Mullet gneiss (Fig.
2c). Rocks of similar age occur on Rockall Bank (Daly et al.
1995; Fig. 10), but these are characterized by polygonal granular
textures, which are not present in the analysed clasts.
Clast C61D-30 yields a weighted mean 207Pb/206Pb age of 972
� 8 Ma. This age falls within the time range of late Grenville
(Rigolet phase) pegmatite formation and metamorphism recorded
in the Annagh Gneiss Complex (Daly 1996, 2009). An older
discordant zircon in this sample, with a 207Pb/206Pb age of 1022
� 49 Ma (spot 5), is consistent with inheritance from the c.
1015 Ma Doolough Granite (Daly 1996, 2009).
The detrital zircon data tell an entirely different story. The
Erris Group was deposited after c. 955 Ma (concordia age of
youngest detrital zircon from the Doonamo Formation, C61A)
with age peaks of c. 990 Ma, c. 1500 Ma and c. 1640 Ma
dominating the zircon spectra. Deposition of the Inishkea Divi-
sion is tentatively constrained to have been later than c. 1005 Ma
(youngest detrital zircon from the Scotch Port Schist, C67), and
although based on limited data also consists of Mesoproterozoic
detritus with some Neoproterozoic and late Palaeoproterozoic
grains. A single discordant analysis from the Doonamo Forma-
tion (sample C61A, grain 3) points to a detrital contribution from
a c. 1850 Ma source; otherwise, early Palaeoproterozoic and
Archaean detrital zircons are absent in both the Erris Group and
Inishkea Division. However, the absence of age peaks in limited
datasets (e.g. the Inishkea Division) cannot reliably be used to
exclude particular age populations. Conversely, grains present in
small datasets may represent a significant component of the
sediment (Vermeesch 2004; Andersen 2005). The available
sparse detrital zircon data for the Inishkea Division are similar to
those of the Doonamo Formation and a similar provenance for
the two is not unlikely.
The detrital zircon signature of the Doonamo Formation, for
which there are sufficient data for assessment (Andersen 2005),
suggests a more distal source for the majority of the psammitic
detrital zircons than the more locally derived clasts. However,
some grains are compatible with a source similar to the Annagh
Gneiss Complex. Grains from C61A, which fall in the age
bracket of c. 960–1000 Ma, are consistent with Grenville mag-
Fig. 5. Nd evolution diagram showing �Nd
values for Erris Group (C61A) and Inishkea
Division (C62, C63, C66B and C67)
metasediments at inferred time of
deposition (c. 900 Ma). Annagh Gneiss
Complex Nd evolution lines from Menuge
& Daly (1990).
C. A. McATEER ET AL .1042
matic and metamorphic events in the Annagh Gneiss Complex.
A single grain in C61A (grain 92, 1184 � 20 Ma) and another
from C67 (grain 4, 1178 � 27 Ma) may correlate with the c.
1177 Ma Doolough gneiss, whereas c. 1270 Ma grains (two in
C61A, five in C63 and two in C67) and c. 1750 Ma grains (three
in C61A) are consistent with derivation from the Cross Point and
Mullet gneisses, respectively (Daly 1996, 2009). Paired core and
rim ages from grain 2 (1152 � 27 Ma and 1005 � 22 Ma,
respectively) from the Scotch Port Schist (C67, Inishkea Divi-
sion), suggest derivation from the c. 1015 Ma Doolough Granite
Fig. 6. CL images of selected zircon grains showing ion microprobe
spots as numbered ellipses labelled with U–Pb ages. White continuous-
line scale bars represent 100 �m; white dashed scale bars represent
50 �m. Single spot ages are given for detrital zircons (all concordia ages
except for those with asterisks, which are 207Pb/206Pb ages and represent
discordant analyses). Concordia ages are shown for zircon from
Doonamo Formation clasts (except C61G-7 and C61D-30, which
represent weighted mean 207Pb/206Pb ages).Fig. 7. Tera–Wasserburg concordia diagrams for zircon from Doonamo
Formation clasts. Ages are concordia ages, except for C61D-30, which is
a weighted mean 207Pb/206Pb age. All errors are 2�. (a) C61B-1: black
continuous-line ellipses represent concordant data used to calculate
concordia age; grey ellipses represent discordant data displaying Pb loss
from c. 1744 Ma; black dashed ellipses with spot numbers represent
discordant data defining discordia age (MSWD ¼ 2.2). (b) C61B-10:
concordant data (black continuous-line ellipses) used to calculate
concordia age (inset); discordant data (grey-filled dashed ellipses with
spot numbers) are the result of Pb loss. (c) C61D-30: concordant data
(black continuous-line ellipses with black spot numbers) and discordant
data (grey-filled ellipses, reversely discordant; dashed ellipses with grey
spot numbers, Pb loss). Weighted mean 207Pb/206Pb age of clast from
concordant and reversely discordant data. Concordant data and spot 1
define discordia (MSWD ¼ 1.5).
PROVENANCE OF THE NORTH MAYO DALRADIAN 1043
with inheritance from the c. 1177 Ma Doolough gneiss (Daly
1996; Fig. 6).
Metamorphism
All post-Grenville deformational events in the Annagh Gneiss
Complex can be matched with events in the overlying metasedi-
ments (Yardley et al. 1987; Kennedy & Menuge 1992; Daly &
Flowerdew 2005) and are demonstrably Grampian (c. 470 Ma) in
age (Daly & Flowerdew 2005). Furthermore, metadolerites that
share the same deformational history as their enclosing metasedi-
ments (the Doonamo Formation and the Scotch Port Schists)
experienced post-metamorphic cooling at c. 450 Ma (Ar–Ar age,
Daly & Flowerdew 2005). In addition, a Grampian (c. 470 Ma)
overgrowth is recorded by one zircon from the Inishkea Division
(Kinrovar Schist, C63, spot 8c) and is interpreted as a post-
depositional overgrowth, consistent with the Rb–Sr muscovite
age of c. 450 Ma obtained from the main foliation by Chew et
al. (2003). A c. 470 Ma Pb loss event is also suggested in the c.
980 Ma clast C61D-30 (discordant data lie along a discordia with
upper and lower intercepts of 965 � 12 Ma and 477 � 79 Ma,
respectively). The geological significance, if any, of the c.
690 Ma lower discordia intercept, recorded in the c. 1740 Ma
clast C61B-1, is unclear at present.
Correlation
Correlation between the Erris Group and the Inishkea Division
seems valid on the basis of whole-rock geochemistry, Sm–Nd
isotopic data and U–Pb detrital zircon ages. The U–Pb detrital
zircon data, although limited for the Inishkea Division, permit
correlation of the Erris Group and the Inishkea Division with the
lowest subdivision of the Dalradian, the Grampian Group
(Cawood et al. 2003; Banks et al. 2007), and with the Moine
Supergroup (Friend et al. 2003; Cawood et al. 2004; Kirkland et
al. 2008). Both the Dalradian Grampian Group and the Moine
Supergroup are characterized by late Palaeoproterozoic peaks,
Mesoproterozoic detritus, some Neoproterozoic detritus and little
if any early Palaeoproterozoic or Archaean detritus (Cawood et
al. 2003, 2004; Friend et al. 2003; Banks et al. 2007; Kirkland et
al. 2008). A correlation with the Moine Supergroup is unlikely
for the Erris Group, however, given its stratigraphic relationship
to the upper parts of the Dalradian in north Mayo (Winchester et
al. 1988; Winchester & Max 1996). Kennedy & Menuge’s (1992)
interpretation of a stratigraphic contact between the Inishkea
Division and overlying Erris Group north of Scotch Port also
supports a Grampian Group affinity for the Inishkea Division.
The lack of Archaean detritus in the Inishkea Division detrital
zircon age spectrum suggests that a correlation with the Dalra-
dian Appin Group, or even the Torridonian, is unlikely (Rainbird
et al. 2001; Cawood et al. 2003; Kinnaird et al. 2007). It must be
pointed out, however, that the detrital zircon data for the Inishkea
Division are not sufficient to reliably rule out possible correla-
tives, as only a small amount of detritus has been sampled in this
study. However, given that detrital grains present in very small
datasets are likely to represent a significant constituent of the
sediment (Vermeesch 2004; Andersen 2005), some Archaean
grains, which are the dominant mode in the Appin Group
(Cawood et al. 2003), might be expected in the Inishkea Division
if an Appin Group correlation was appropriate. Using this
argument, albeit a circular one, it is unlikely that the Kinrovar
Schist has an Appin Group affinity (as suggested by Kennedy &
Menuge 1992). This concurs with geochemical evidence
(Winchester & Max 1988; Max & Winchester 1993) that the
Inishkea Division is compatible only with the lower Dalradian
Grampian Group. The original argument that the Kinrovar Schist
belonged to the Appin Group was based on the assumption that
the rocks at Kildun (Fig. 1), in stratigraphic contact with the
Inishkea Division, were part of the Appin Group (Kennedy &
Menuge 1992). These rocks have since been included in the Erris
Group (Winchester & Max 1996; Fig. 1).
Fig. 8. Number v. zircon age distribution plots for C61A, Doonamo
Formation (Erris Group), C63 Kinrovar Schist (Inishkea Division) and
C67 Scotch Port Schist (Inishkea Division), north Mayo. Ages are
concordia ages except for the youngest grain in C63 (grain 9, 207Pb/206Pb
age). Black boxes with white text denote the age of the youngest zircon
for each sample (2� errors). Dashed rectangle for C63 depicts a
discordant analysis from grain 1 (spot 1b), interpreted as Pb loss from c.
1000 Ma. All other data are concordant (i.e. error ellipses intersect
concordia). Grey bars denote Sm–Nd whole-rock model ages (tDM, Ma)
for each sample. n, number of grains.
C. A. McATEER ET AL .1044
Fig. 9. Tera–Wasserburg concordia
diagrams for detrital zircons in sample
C61A, Doonamo Formation (Erris Group)
(black ellipses denote concordant data,
n ¼ 84/99 grains; black-filled ellipse
indicates grain 103, the youngest
concordant analysis; grey-filled ellipses
denote discordant data discussed in the text,
with spot numbers); C67, Scotch Port
Schist (Inishkea Division) (concordant data
with spot numbers, n ¼ 7/7 grains, and spot
5a, an inherited core analysis; grey-filled
ellipses denote common Pb corrected data);
C63, Kinrovar Schist (Inishkea Division)
(black ellipses denote concordant data,
n ¼ 12/15 grains; grey-filled ellipses denote
discordant data discussed in the text, with
spot numbers).
Fig. 10. Rodinia palaeogeography and source regions. (a) Reconstruction of Rodinia at c. 900 Ma adapted from Li et al. (2008). ES, East Svalbard; G,
Greenland; R, Rockall Bank; S, Scotland. Dashed rectangle highlights area in (b). (b) Schematic palaeogeographical reconstruction of the North Atlantic
region c. 900 Ma showing potential source regions for the Dalradian of north Mayo, Ireland. Arrow indicates likely sedimentary transport route. Age of
crustal elements from Ahall & Gower (1997), Rivers (1997) and Daly et al. (2001). Distribution of crustal elements as given by Li et al. (2008). K-M,
Ketilidian–Makkovikian.
PROVENANCE OF THE NORTH MAYO DALRADIAN 1045
Winchester & Max (1996) correlated the Doonamo Formation
with the Corrieyairack Subgroup of the Scottish Grampian Group
on the basis of whole-rock geochemistry (Table 1). As the
chemistry of the Inishkea Division is similar to that of the
Doonamo Formation (Max & Winchester 1993; Fig. 4) and both
have detrital zircon signatures consistent with those of the
Corrieyairack Subgroup (i.e. late Palaeoproterozoic, Mesoproter-
ozoic and early Neoproterozoic detritus; see Banks et al. 2007) it
is proposed that they represent the Irish equivalents to the
Corrieyairack Subgroup (Table 1). However, more data are
needed from the Inishkea Division to properly characterize its
detrital zircon age spectrum. The younger Erris Group forma-
tions (not included in this study) are geochemically similar to the
Glen Spean Subgroup of the Grampian Group (Winchester &
Max 1996; Table 1).
Deposition of the Grampian Group in Ireland is constrained
to have taken place after c. 955 Ma (youngest detrital zircon)
and before c. 470 Ma (Grampian metamorphism of the metase-
diments, Daly & Flowerdew 2005). A Sm–Nd mineral iso-
chron age of 625 � 47 Ma for the Mam Sill that cuts the
Appin Group near Horn Head in Donegal, and a U–Pb zircon
age of c. 590 Ma for a gabbro–pegmatite of a correlative sill
at Dooros Point, Donegal (Kirwan et al. 1989; Daly 2009),
suggests a minimum depositional age of c. 590 Ma for the
Appin Group and, by inference, the Grampian Group in north
Mayo.
Source regions and Neoproterozoic palaeogeography
The Neoproterozoic site of Dalradian deposition is thought to
have occupied a triple-junction position between three major
cratons within the supercontinent Rodinia, Laurentia, Baltica and
Amazonia (Soper 1994; Cawood et al. 2003; Banks et al. 2007;
Fig. 10). The locally derived clasts from the Erris Group (C61B-
1, C61B-10, C61G-7 and C61D-30) support other lines of
evidence, discussed above, that the Annagh Gneiss Complex
represents the depositional basement to the Dalradian in NW
Ireland. Furthermore, the detrital zircon data for the Erris Group
are consistent with a Laurentian provenance with age peaks at c.
1640 Ma, c. 1500 Ma and c. 990 Ma corresponding to Labrador-
ian (c. 1.71–1.60 Ga), Pinwarian (c. 1.51–1.45 Ga) and Grenvil-
lian (c. 1.3–0.95 Ga) terranes, respectively (Rivers 1997;
Wasteneys et al. 1997; Fig. 10). Although the detrital zircon data
for the Inishkea Division are limited they are also consistent with
similar Laurentian sources. Although most of the detrital zircon
grains analysed as part of this study seem to have a more distal
source than the locally derived clasts, some are consistent with
derivation from the Annagh Gneiss Complex (discussed above).
The c. 1300 Ma detritus in both the Erris Group (C61A) and the
Inishkea Division (C63) may have been derived locally from a c.
1310 Ma granitic orthogneiss from the northern Porcupine High,
offshore western Ireland (Daly et al. 2008).
Paired core and rim ages can potentially allow more accurate
identification of their source. However, care must be taken not to
include older core ages in zircon age distribution plots where the
age of the source is constrained by a younger rim analysis. Grain
1 from the Doonamo Formation (C61A; see Fig. 6), with a c. 1.0
Ga overgrowth around a c. 1380 Ma core, is consistent with
derivation from the c. 1.4–1.3 Ga Dysart–Mt. Holly Granitoids
in the western Grenville Province (Rivers & Corrigan 2000).
Grain 2 from the Scotch Port Schist was probably derived from
the Doolough Granite (it yields a rim age within error of the c.
1015 Ma Doolough Granite and a core age within error of the c.
1177 Ma Doolough gneiss; Daly 1996; discussed above) whereas
grain 5, also from the Scotch Port Schist, yields a c. 1620 Ma
Labradorian core and a c. 1450 Ma overgrowth, and was
probably derived from the Pinware Terrane (Wasteneys et al.
1997; Rivers & Corrigan 2000; Heaman et al. 2004; Fig. 10).
Although Baltica offers another possibility for Labradorian-,
Grenville- and Pinwarian-aged sources (within the Sveconorwe-
gian and Svecofennian provinces; Puura & Floden 1999; Ahall &
Connelly 2008; Fig. 10), a Laurentian provenance concurs with
previous interpretations of a westerly derived source for both the
Inishkea Division and the Erris Group (Winchester & Max
1987). Local derivation for the K-feldspar and granitoid clasts
also seems more likely than a Svecofennian origin. Amazonia
can also be excluded for this reason, but more importantly as it
lacks c. 1.7–1.6 Ga magmatic activity (Banks et al. 2007, and
references therein) that could account for the strong c. 1640 Ma
peak in the detrital data. Dalradian deposition is therefore tied to
the margins of Laurentia.
Conclusions
K-feldspar and granitoid clasts from the Erris Group yield U–Pb
zircon ages of c. 1740 Ma and c. 980 Ma, consistent with local
derivation from the underlying Annagh Gneiss Complex. The c.
1640 Ma, c. 1500 Ma and c. 990 Ma peaks in the Erris Group U–
Pb detrital zircon age spectra record more distant Laurentian
sources (Labradorian, Pinwarian and Grenvillian, respectively).
Detrital zircon grains from the Inishkea Division are also
consistent with a Laurentian provenance, but the data are too few
to distinguish any notable peaks. Deposition of the Erris Group
occurred after c. 955 Ma, whereas deposition of the Inishkea
Division is more tentatively constrained to after c. 1005 Ma.
Correlation of the Erris Group and Inishkea Division with the
lower Dalradian Grampian Group is considered valid on the basis
of whole-rock geochemistry and Sm–Nd data, and U–Pb detrital
zircon data (although more detrital zircon data are needed from
the Inishkea Division). The clast data support other lines of
evidence that the Annagh Gneiss Complex represents the deposi-
tional basement to the lower Dalradian in north Mayo, one of the
few such ‘basement–Dalradian cover’ examples preserved. Dalra-
dian deposition can therefore be tied to the margins of Laurentia.
Thanks go to T. Culligan, M. Murphy and P. Haughton (UCD School of
Geological Sciences, University College Dublin) for thin sections,
assistance with TIMS isotopic analysis and sedimentology advice, respec-
tively. L. Ilyinsky and K. Linden are thanked for their help at the
NORDSIM facility, Stockholm. We also thank N. Marsh (University of
Leicester) for XRF analyses. I. Millar and B. Wade are thanked for
careful and insightful reviews. This research was funded by a UCD
Research Demonstratorship and an EU ‘SYNTHESYS’ grant awarded to
C.A.M. and an IRCSET Basic Research grant SC/2002/248 awarded to
J.S.D. This paper is NORDSIM Contribution 253.
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Received 13 October 2009; revised typescript accepted 2 April 2010.
Scientific editing by Chris Clark.
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