Geochemical
evidence for atmospheric pollution derived from prehistoric copper mining at
Copa Hill, Cwmystwyth, mid-Wales, U.K.
Mighall, T.M.,1
Abrahams, P.W.2 Grattan, J.,2 Hayes, D.2
Timberlake, S.3. & Forsyth, S.1
1. Centre for Quaternary Science, Geography, School of
Natural and Environmental Sciences, Coventry University, Priory Street,
Coventry, CV1 5FB, U.K. (corresponding author: t.mighall@cov.ac.uk)
2. Institute of Geography and Earth Science, University of Wales, Aberystwyth, Wales, SY23 3DB, U.K.
3.
98 Victoria Road, Cambridge, CB4, U.K.
ABSTRACT
This paper presents geochemical data from a blanket peat located close
to a Bronze Age copper mine located on the northern slopes of the Ystwyth
valley, Ceredigion, mid-Wales, U.K. The research objectives were twofold;
firstly to test the comparability of different geochemical analytical
techniques, and secondly to explore the possibility that the peats contained a
geochemical record of the pollution generated by the mining activity. Four peat monoliths were extracted from the
blanket peat to reconstruct the pollution history of the prehistoric mine.
Three different geochemical measurement techniques were employed and 4 copper
profiles have been reconstructed, one of which is radiocarbon-dated. Three of these
profiles, located close to the mine, recorded copper enrichment of the peat during the known
period of exploitation of the mine. In
contrast copper did not enrich the fourth monolith, extracted approximately 1.5
km north of the mine. Whilst other possible
explanations to explain the copper concentrations are discussed, it is argued
that the high copper concentrations represent the first evidence of localised
atmospheric pollution caused by Bronze Age copper mining in the British Isles.
INTRODUCTION
In northern and western Europe Roman and subsequent mining and smelting
activity has been detected in the records of geochemical deposition in
ombotrophic peat bogs. Less attention, however, has been given to European
prehistoric mining and smelting despite the fact that ‘the detection of early
mineral exploitation in sediments of this kind is an important step in
understanding the extent and nature of mining and smelting in the past’ (West et al., 1997:343). In Britain, prehistoric metal mining sites
have been difficult to identify and, until recently, there was a widespread
belief that evidence of early mining was destroyed by subsequent
activities. This view has been recently
overturned by the discovery of several prehistoric copper mines in the British
Isles including Copa Hill Cwmystwyth in west Wales (between 3500±50 and 3070±50
BP); Great Orme’s Head, Llandudno, north Wales (2940±80 BP); Mount Gabriel, Co.
Cork, Ireland (3450±120 BP. and 3130±80 BP) (Timberlake, 1990a,b; Timberlake
& Switsur 1988; Dutton and Fasham, 1994; O’Brien, 1994).
This paper aims to identify evidence for prehistoric copper mining
pollution at Copa Hill, Cwmystwyth, mid-Wales, by (i) replicating copper
profiles at four sites located within 600 metres of a prehistoric mine, using a
variety of analytical methods and (ii) comparing these proximal profiles with a
relatively distal profile located 1.5 km from the mine.
The prehistoric mining site of Copa Hill is situated 30 km ENE of
Aberystwyth, mid-Wales (SN811751) on a copper/lead mineral vein on the northern
slopes of the Ystwyth valley at approximately 420 m OD. Charcoal, recovered
from the mineworking debris, has been dated to a period within the early to mid
Bronze Age (Timberlake, 1990a,b, 1995).
Metal mining for probably resumed in the Ystwyth valley, during Roman
times when lead was the focus of activity and from the 16th century until the
early 20th century for lead and zinc (Hughes, 1981). Thus, this location
provides an ideal site to investigate pollution histories for mining activities
spanning three millennia.
METHODS
An extensive area of blanket peat occupies the northern plateau of the
Ystwyth valley. Four peat monoliths were extracted from freshly exposed
sections. In order to
detect any atmospheric pollution and to attempt to replicate the data four
monoliths CH1, CH2 and CH4 were extracted 600 metres to the north of the mine,
and are within 30 metres of each other. A fourth monolith CH3 was recovered from a
freshly exposed section approximately 1.5 km NE from the prehistoric mine to
act as a spatial control.
Three methods were employed to reconstruct metal concentrations. These were, a) Inductively Coupled Plasma Mass Spectrometry using a partial acid digestion of the peat, b) Atomic Absorption Spectrophotometry using a Kjeldahl total digestion method to produce the aliquot c) Absorption Spectrophotometry using a microwave digestion method to produce the aliquot.
RESULTS and DISCUSSION
In all three proximal profiles copper distribution within the monolith
followed a similar pattern. Copper is
clearly concentrated towards the base of each core reaching 110 µg g-1 and are higher
than a local mean background figure for local peats which may be extrapolated
from CH3 of ~15 µg g-1. In complete contrast to the previous three
sets of results copper concentrations at site CH3 show little stability in this
monolith. Values range between 0 and 38
µg g-1. Copper in this monolith appears to be distributed entirely
randomly. It is clear that each of the three proximal monoliths CH1, CH2 and
CH4 record a similar pattern of copper deposition. Each of the extraction techniques and analytical methods used
have produced broadly similar results.
However, it is clear that the partial acid digest method used on CH1
dramatically reduced the concentrations detected, though not the pattern of
distribution, which limits its comparative value as an extraction method.
Although the exact timespan of prehistoric mining cannot be determined,
a basal radiocarbon date of the CH2 peat profile, from 134 to 133 cm depth,
places peat initiation at 3470 + 35 years BP during the early Bronze
Age. A second radiocarbon date of 2395 +
35 years BP was derived from peat between 105 and 106 cm. It is clear that the copper enrichment
evident between 124–138 cm depth in monolith CH2 corresponds with the
established dates of Bronze Age mining at Copa Hill 600 metres to the
south. The different lengths of all
three proximal monoliths suggest that since initiation peat accumulation has
occurred at a slightly differing rate.
However, the clear similarity of the geochemical profiles and their
proximity to each other suggest that it is reasonable to propose that the
copper enrichment indicated in all three monoliths is the result of the same
depositional processes occurring at approximately the same time.
The replication of elevated copper concentrations three times using three different extraction and analytical methods suggests that the concentration of copper towards the base of each the proximal monoliths is unlikely to be an artefact of the chemical method. In fact, the pattern for copper throughout the peat profiles is fairly consistent although the values do vary slightly. The basal peak in copper concentrations described at sites CH1, CH2 and CH4 is not evident at site CH3. One explanation for the absence of high copper concentrations is that the site lies outside the atmospheric dispersion halo of prehistoric mining activity. It is likely that the pattern of copper deposition recorded in monoliths CH1, CH2 and CH4 reflects prehistoric copper mining activity ca. 3000 years ago in the remote uplands of central Wales. Having established the existence of this record it is probable that other geochemical records of ancient mining activity may be detected in upland blanket peats.
References
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