Heterogeneity, cyclicity and diagenesis in a Mississippian brachiopod shell of palaeoequatorial...
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Transcript of Heterogeneity, cyclicity and diagenesis in a Mississippian brachiopod shell of palaeoequatorial...
Heterogeneity, cyclicity and diagenesis in a Mississippian
brachiopod shell of palaeoequatorial Britain
Lucia Angiolini,1 Michael Stephenson,2 Melanie Leng,3 Flavio Jadoul,1 Dave Millward,4 AnthonyAldridge,5 Julian Andrews,6 Simon Chenery2 and Gareth Williams21Dipartimento Scienze della Terra �A. Desio� Via Mangiagalli 34, 20133 Milano, Italy; 2British Geological Survey, Keyworth, Nottingham,
NG12 5GG, UK; 3NERC Isotope Geosciences Laboratory, British Geological Survey, Keyworth, Nottingham, NG12 5GG, UK; 4British
Geological Survey, Murchison House, West Mains Road, Edinburgh EH9 3LA, UK; 5PO Box 19576, Woolston, Christchurch 8241, New
Zealand; 6School of Environmental Sciences, University of East Anglia, Norwich, NR4 7TJ, UK2
Introduction
Fossil shells are high-resolution ar-
chives which vary in response to
growth, environmental conditions
and diagenetic changes. Isotope pro-
files across growth lines of recent fossil
shells allow assessment of seasonality
(e.g. Schone et al., 2005; Johnson
et al., 2009). Only a handful of studies
have been conducted in the Palaeozoic
which relate isotope data and growth,
to unravel environmental variation
(Mii and Grossman, 1994; Ivany and
Runnegar, 2010). Fewer studies have
been undertaken on patterns of alter-
ation ⁄preservation and on the hetero-
geneous distribution of chemistry and
isotope composition within fossil
shells (e.g. Samtleben et al., 2001).
Brachiopods are excellent proxies
for ancient ocean conditions (e.g.
Compston, 1960; Popp et al., 1986;
Parkinson & Cusack in Williams
et al., 2007; Grossman et al., 2008),
because they record the primary sea-
water isotope composition with no
known vital effect in their innermost
shell layers. Also, brachiopod shells
grow episodically rather than contin-
uously, and major growth lines or
bands may form due to seasonal
perturbations (Hiller, 1988), making
them good recorders of past climate.
Recent studies show chemical hetero-
geneity in the shells of extant brachio-
pods (Cusack et al., 2008; Brand
et al., 2011), which reflects natural
environmental variation.
ABSTRACT
A shell of Gigantoproductus okensis shows twenty growth lines
with marked changes of fabric, indicating periodical reduction
of growth rates caused by environmental perturbations. The
number of growth lines suggests a lifespan of 20 years in
agreement with the survival rates of extant brachiopods, and
with spiral deviation analysis. Geochemical analyses across the
growth profile show a heterogeneous distribution of stable
isotopes and trace elements. It is possible to distinguish
primary from altered carbonate, and to interpret the isotopic
data. The oxygen isotope signal in the unaltered parts is
periodical and annual, with oscillation of �1.1&. The higher
values are at the growth lines (winter), and therefore most
likely related to monsoon circulation during the Visean. The
annual periodicity seems also present in the altered part of the
shell, suggesting that diagenesis could have reset the primary
values, but preserved their cyclicity.
Terra Nova, 00, 1–11, 2011
T E R 1 0 3 2 B Dispatch: 19.10.11 Journal: TER CE: Bharani
Journal Name Manuscript No. Author Received: No. of pages: 11 PE: Revathi
Sheffield
Derby
Buxton
Stoke-
on-
Trent
Bakewell
Chapel
En Le
Frith
Matlock
Permian & Triassic
Peak limestone group (Visean)
Millstone grit group (Serpukhovian-Bashkirian)
Pennine coal measures group (Bashkirian- Moscovian)
10 km Sample site
Fig. 1 Geological map of the Carboniferous rocks of the Derbyshire High region of
central England. The Monsal Dale Limestone Formation is part of the Peak
Limestone Group. The star indicates the sample location.
Correspondence: Lucia Angiolini, Diparti-
mento Scienze della Terra �A. Desio� Via
Mangiagalli 34, 20133 Milano, Italy.
e-mail: [email protected]
� 2011 Blackwell Publishing Ltd 1
doi: 10.1111/j.1365-3121.2011.01032.x
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Herein we present the geochemistry
of a Mississippian brachiopod shell
from palaeoequatorial Britain and
show relationships with growth, envi-
ronmental change and diagenesis.
Material and methods
The specimen is a productid brachio-
pod of the species Gigantoproductus
okensis (Sarytcheva) (CA6866, BGS
collection) from Monsal Dale Lime-
stone Formation of Derbyshire, UK
(Bridges, 1982) of early Brigantian D2
(= late Visean) age (Fig. 1). The
specimen was sectioned parallel to
growth and screened by SEM,
cathodoluminescence and trace ele-
ment analysis. One hundred and four-
teen samples were taken using a
0.5 mm drill across the growth lines
for geochemistry and isotopes. Subs-
amples for geochemical analysis were
dissolved in a few ml of 1 M ultra-pure
acetic acid, taken up in 1% (c. 0.16 M)
nitric acid, and measured for Mn, Sr
and Fe using Inductively Coupled
Plasma-Atomic Emission Spectros-
copy (ICP-AES) on a Fison ⁄ARL
3580 simultaneous ⁄ sequential spec-
trometer. The instrument was cali-
brated with NIST solutions and
precision is >10%.
Trace elements were also measured
along a transverse section of the shell
in situ using a New Wave Research
213 nm Nd-YAG laser ablation (LA)
system attached to a Thermo X Series
ICPMS. The laser was optimized and
calibrated with the NIST 610 silicate
glass. Laser ablation pits were then
cross correlated with the samples
drilled for geochemistry and isotopes;
each drilled hole corresponded to 2–4
LA-ICPMS pits.
Isotope analysis was undertaken
using a GV IsoPrime mass spectro-
meter with Multiprep device. Isotope
values (d13C, d18O) are reported as per
mil (&) deviations of the isotopic
ratios (13C ⁄12C, 18O ⁄
16O) calculated
to the VPDB scale using a within-run
laboratory standard (KMC) cali-
brated against international NBS
standards (NBS18 and 19). Analytical
reproducibility was better than 0.1&
for d13C and d18O.
Fourier analysis was carried out on
O and C time series data of sequen-
tially collected sample numbers 40–97
to investigate periodicity. Samples
which are out of sequence of growth
because they either represent the
same growth increment or a time
reversal were not considered. Spectral
analysis of unevenly sampled data is
frequently achieved by interpolating
data to a uniform scale, which can
have the undesirable consequence of
aliasing high frequencies into the low
frequencies of a spectrum. Lomb
(1976) and Scargle (1989) modified
the traditional Fourier transform to
account for the effects of uneven time
sampling. This study adopts the pro-
cedure of Schulz and Stattegger
(1997).
Twenty years growth of the shell
Gigantoproductid brachiopods are
abundant in the upper Visean shallow
marine bioclastic limestones of central
England (Ferguson, 1978; Pattison,
1981; Bridges, 1982). These brachio-
pods lived semi-infaunally in coarse
sediments, stabilized by their extended
ears and postero-ventral shell thicken-
ing, in normal saline marine settings.
The large size and thick shell of
Gigantoproductus okensis (Sarytcheva)
(Fig. 2) make it suitable for analysis
of shell growth, structure and geo-
chemical composition. In longitudinal
section (Fig. 3), it shows conspicuous
growth lines indicating slowing of
growth caused by regular environmen-
tal perturbations. Twenty major
growth lines cross the well-preserved
prismatic shell layer of the ventral
valve and are weakly inclined anteri-
orly towards the inner shell surface.
At the growth lines, the fabric changes
from calcite prisms to irregular lami-
nae (Fig. 4), confirming periodical
mantle-reversal and reduction of
growth rate. The spacing of the
growth lines varies from 300 lm to
more than 1 mm (c.f. Mii et al., 2001).
According to Hiller (1988) a seasonalFig. 3 Longitudinal section through Gigantoproductus okensis. The shell is orientated
with dorsal valve up and the umbo to the right.
Fig. 2 Ventral view of an articulated specimen of Gigantoproductus okensis. Maxi-
mum width = 15.6 cm, length = 12.1 cm.
Heterogeneity, cyclicity and diagenesis 1• L. Angiolini et al. Terra Nova, Vol 00, No. 0, 1–11
.............................................................................................................................................................
2 � 2011 Blackwell Publishing Ltd
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fall in temperature ⁄nutrient supply
(winter) would reduce or stop growth
causing a change in the direction of
the axes of the secondary layer fibres
or a halt in the growth of regularly
stacked tertiary prisms.
There are few controlled growth
studies in extant brachiopods (Buen-
ing, 2001), but estimates suggest a
lifespan of 3–20 years (Buening and
Spero, 1996). Recent Tyrrhenian Sea
brachiopods have a lifespan
>40 years (Taddei Ruggiero, 2001).
The growth lines in our specimen
suggest a lifespan of at least 20 years
in agreement with these estimates.
To further constrain the age of our
brachiopod we used spiral deviation
analysis, which studies deviations
from the secular component of accre-
tionary growth of the shells (Aldridge
and Gaspard, 2011). Logarithmic spi-
rals were fitted to the inner ventral
valve surface of our shell (Aldridge,
1999) with deviations from spiral fit
analysed for periodicity. Deviations
were nonrandom (P < 0.01 4, mean
square successive difference test,
Bissell and Williamson, 1988), and
subjected to an empirical mode
decomposition (Wu et al., 2007;
implemented as R code by Donghoh
and Hee-Seok, 2008). The first four
minima of an empirical mode function
(Fig. 5) represented distances from the
umbo that were then located on the
actual shell. Two internal growth lines
were discerned between each of the
first four minima of spiral deviations,
which were then interpreted as 2-year
increments. The indicated age at the
first four minima, their arc length
from umbo, and a 100 unit maximum
length were used to fit a two para-
meter logistic growth function
(Fig. 6). Age at death was inversely
calculated from the fitted logistic
curve to be 20.2 years, which is con-
sistent with the age estimated by
counting the growth lines.
Geochemistry and preservation of the
accretionary shell
One hundred and fourteen samples
(for O and C isotopes and trace
elements) were taken across the
20 year period of growth within the
mostly non- or slightly luminescent
(indicative of low alteration, e.g. Popp
et al., 1986; Grossman et al., 1993)
parts of the shell interior, which con-
sists of a well developed prismatic
layer (Figs 4, 7 and 8 and Table 1).
The samples typically show Sr
>1000 ppm, Mg >3000 ppm, Na
�1000 ppm, Mn �60 ppm and Fe
<300 ppm, with a heterogeneous dis-
tribution throughout the shell. Trace
elements are consistent with data from
extant species (Brand et al., 2003) and
from well-preserved Carboniferous
and Permian brachiopods (Bruckshen
et al., 1999; Korte et al., 2003; Van
Geldern et al., 2006); their hetero-
geneous distribution reflects the natu-
ral variations observed in recent
brachiopods (Cusack et al., 2008;
Fig. 4 Ultrastructure of the shell at the growth lines showing a change in fabric at the
growth halts from stacked prisms to irregular laminae.
Fig. 5 Deviations from spiral growth as
an empirical mode function plotted
against distance from ventral umbo
(maximum shell length fixed at 100
units). Solid symbols denote the minima
used in fitting the two parameter logistic
growth curve.
Fig. 6 Logistic growth curve fitted to
distance and age of four minima identi-
fied from spiral deviations (Fig. 5). The
solid square symbol locates the length of
the inner ventral valve (98.85 image
units) and the calculated age at death
(20.2 years).
Colouronline,B&W
inprint
Terra Nova, Vol 00, No. 0, 1–11 L. Angiolini et al. • Heterogeneity, cyclicity and diagenesis 1
.............................................................................................................................................................
� 2011 Blackwell Publishing Ltd 3
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Brand et al., 2011). Except for small
areas, the non-luminescent or slightly
luminescent inner prismatic shell has
d18O varying from )4.4& to )6.4&
and d13C from )2.6& to +1.3&.
There are a few values in common
with those of Popp (1986) who inves-
tigated Gigantoproductus of the As-
bian-Brigantian of Britain and
Belgium. Popp�s (1986) data came
from spot-analysis on material which
was either undetermined at specific
level or belongs to different species of
the genus, and thus may be influenced
by heterogeneous distribution of TE
in the shell, and interspecific variation.
In the luminescent parts, which are
characterized by diagenetic quartz
replacing original calcite, d18O values
are very low ()11.9& to )7&). The
quartz is in the form of small idio-
morphic crystals or, more frequently,
as mm-sized aggregations of idiomor-
phic ⁄ subidiomorphic crystals and par-
tially silicified nuclei with calcitic
inclusions (Fig. 9). These very low
d18O values are coupled with high
d13C values, and so are not indicative
of early diagenetic alteration related
to sub aerial exposure (Bridges, 1982).
Also d13C values do not fit the �mete-
oric calcite line� (Lohmann, 1988).
Luminescent samples (e.g. samples 5–
38; 65–71; Table 1) show Na, Mg and
Sr lower than the unaltered material,
but higher Fe; Mn is generally low.
Samples at the anterior margin of the
shell (samples 86–92) have relatively
low Mg and Sr, but higher Mn and
Fe; these trace elements suggest alter-
ation, although the d18O values for
these samples are in the range of those
from the unaltered shell material or
only slightly lower. This suggests a
different type of alteration affecting
the posterior part of the shell with
respect to the anterior margin, prob-
ably related to the occurrence of voids
in the umbonal cavity, later filled by
equant calcite (Fig. 3).
In addition, trace element variabil-
ity through a transverse section of the
shell (from the inside to outside edge
of the shell between sample positions
46–47 of the series shown in Fig. 7)
was measured using laser ablation to
investigate the change from the inner
unaltered to the outer altered portions
of the shell (Tables 2 and 3). Diage-
netic alteration in the outer shell is
identified by d18O values lower than
)6.4&, generally lower Sr and higher
Mn. This suggests that the fossil
retains primary material within the
inner most part of the shell. Alteration
of the posterior, anterior and external
part of the shell may have been caused
by locally confined circulation of rel-
atively hot fluids of hydrothermal
origin, since the region was affected
by Mississippi-Valley type Late Car-
boniferous-Early Permian mineraliza-
tion with fluid temperatures of
100 �C–150 �C (Kendrick et al., 2002).
The central inner part of the shell may
Fig. 7 Plane-polarized light (below) and corresponding CL images (above) of the
ventral valve of Gigantoproductus okensis, umbo to the right. The shell is luminescent
around quartz aggregates (left side) and along the external margin. Numbers indicate
samples 26–97 (Table 1).
Fig. 8 Non-luminescent shell interior (external part of the shell bottom down), transmitted light and CL.
Colouronline,B&W
inprint
Colouronline,B&W
inprint
Heterogeneity, cyclicity and diagenesis 1• L. Angiolini et al. Terra Nova, Vol 00, No. 0, 1–11
.............................................................................................................................................................
4 � 2011 Blackwell Publishing Ltd
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Table 1 Isotopes and trace elements for the samples collected along the internal surface of the shell.
Sample no. d13C (&) d
18O (&) SEM CL Ca lg ⁄g Mg lg ⁄g Ba lg ⁄g Sr lg ⁄g Mn lg ⁄g Fe lg ⁄g
1 1.1 )5.2 P III
2 0.7 )6.0 P III
3 0.1 )6.5 P III
4 0.9 )6.1 P III
5 0.9 )7.3 P III
6 1.1 )7.4 P III
7 0.8 )8.2 P III
8 0.6 )8.9 P III
9 0.4 )10.5 P III
10 0.4 )11.9 P III 400 000 2884 <DL 534 131 <DL
11 0.6 )11.8 P III
12 0.7 )11.9 P III
13 0.1 )11.7 P III 400 000 2530 <DL 515 111 <DL
14 )0.1 )11.9 P III 400 000 2393 <DL 540 107 <DL
15 )0.2 )11.5 P III
16 0.1 )11.4 P III
17 0.0 )11.6 P III
18 0.3 )11.7 P III
19 0.2 )11.4 P III 400 000 2453 <DL 393 141 <DL
20 0.4 )11.3 P III L 400 000 2332 <DL 413 136 <DL
21 0.1 )11.3 P III L
22 0.2 )11.4 P III L 400 000 2234 <DL 541 130 <DL
23 )0.5 )10.6 P III L 400 000 2208 <DL 628 136 <DL
24 )0.4 )10.6 P III L
25 )0.4 )10.9 P III L
26 )0.1 )11.1 P III L
27 )0.5 )10.6 P III L
28 )0.7 )9.9 P III L
29 )1.5 )7.6 P III L
30 )1.9 )7.8 P III L
31 )0.5 )10.2 P III L
32 )0.4 )9.8 P III L
33 )0.8 )9.0 P III L
34 )1.2 )9.3 P III L
35 )1.5 )9.2 P III L
36 )0.5 )10.5 P III L
37 )0.4 )10.8 P III L
38 )1.7 )7.5 P III SL
39 )2.2 )6.4 P III NL 400 000 4719 <DL 1338 15 <DL
40 )1.5 )5.9 P III NL
41 )1.5 )5.6 P III NL 400 000 4566 <DL 1288 <DL <DL
42 )0.4 )5.3 P III NL 400 000 4044 <DL 1228 <DL <DL
43 0.3 )4.9 P III NL 400 000 4214 <DL 1274 9 <DL
44 )0.8 )5.1 P III NL 400 000 4192 <DL 1289 <DL <DL
45 )1.3 )5.6 P III NL 400 000 3459 <DL 1201 19 <DL
46 )1.2 )5.7 P III NL 400 000 3529 <DL 1249 <DL <DL
47 )0.3 )5.5 P III NL 400 000 3477 <DL 998 <DL <DL
48 )0.5 )5.5 P III NL 400 000 3636 <DL 1111 36 <DL
49 )0.9 )5.4 P III NL
50 )0.3 )9.2 P III SL
51 0.8 )10.4 P III L
52 )0.6 )5.5 P III NL
53 )0.3 )4.9 P III NL
54 )1.5 )5.5 P III NL
55 )1.5 )5.2 P III NL 400 000 3432 <DL 1168 69 <DL
56 0.2 )4.8 P III NL 400 000 3154 <DL 996 86 157
57 )1.3 )5.0 P III NL 400 000 3467 <DL 1175 28 <DL
58 )0.4 )4.7 P III NL
59 )0.5 )4.4 P III NL 400 000 2581 <DL 793 195 <DL
60 )2.5 )5.8 P III NL 400 000 3531 <DL 1187 29 <DL
61 )2.6 )6.0 P III NL 400 000 3822 <DL 1228 <DL <DL
Terra Nova, Vol 00, No. 0, 1–11 L. Angiolini et al. • Heterogeneity, cyclicity and diagenesis 1
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� 2011 Blackwell Publishing Ltd 5
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Table 1 Continued
Sample no. d13C (&) d
18O (&) SEM CL Ca lg ⁄g Mg lg ⁄g Ba lg ⁄g Sr lg ⁄g Mn lg ⁄g Fe lg ⁄g
62 )2.2 )6.0 P III NL 400 000 3735 <DL 1219 41 <DL
63 )2.6 )5.9 P III NL 400 000 3856 <DL 1273 54 <DL
64 )2.4 )6.2 P III NL 400 000 3873 <DL 1268 33 <DL
65 0.1 )7.9 P III L 400 000 3192 <DL 918 48 <DL
66 0.1 )10.5 P III L
67 0.1 )8.5 P III SL
68 )0.7 )7.0 P III SL
69 )0.6 )7.0 P III SL
70 0.3 )9.7 P III SL
71 0.4 )9.9 P III L
71.5 )0.4 )7.9 P III L
72 0.0 )6.2 P III SL 400 000 3178 <DL 889 152 279
72.5 )1.1 )6.3 P III SL
73 )1.0 )5.8 P III SL
73.5 )0.9 )6.4 P III SL
74 )1.4 )6.1 P III NL 400 000 3648 <DL 1120 46 <DL
74.5 )0.9 )5.7 P III NL
75 )1.0 )6.2 P III NL 400 000 3525 <DL 1043 101 85
75.5 )2.1 )8.2 P III NL
76 )1.3 )5.9 P III NL 400 000 3924 <DL 1115 55 646
76.5 )1.1 )6.1 P III NL
77 )1.1 )6.0 P III NL 400 000 3766 <DL 1090 82 85
78 )0.7 )6.5 P III SL 400 000 3225 <DL 917 130 239
79 )0.5 )6.3 P III SL 400 000 2701 <DL 733 214 338
80 0.2 )6.5 P III NL
81 0.2 )6.4 P III NL 400 000 3194 <DL 852 123 356
82 0.2 )6.0 P III NL
83 0.6 )6.2 P III SL 400 000 2827 <DL 722 149 439
84 0.9 )7.3 P III L
85 0.5 )7.0 P III L
86 0.8 )6.1 P III L 400 000 2054 <DL 442 328 918
87 1.2 )5.9 P III L 400 000 1972 <DL 399 454 954
87.5 0.8 )6.8 P III L
88 1.1 )6.4 P III L 400 000 1567 <DL 310 548 872
88.5 +1.0 )8.2 P III L
89 1.2 )6.2 P III L 400 000 1754 <DL 374 516 965
89.5 1.0 )5.8 P III L
90 1.0 )6.5 P III L 400 000 1993 <DL 463 405 785
90.5 1.0 )6.4 P III L
91 1.1 )6.2 P III L
91.5 1.1 )7.1 P III L
92 1.0 )6.3 P III SL 400 000 2149 <DL 567 191 225
92.5 1.1 )6.2 P III SL
93 0.9 )7.3 P III SL 400 000 1760 <DL 448 254 233
93.5 1.3 )7.0 P III SL
94 1.3 )6.5 P III NL 400 000 1961 <DL <DL <DL <DL
94.5 1.3 )6.2 P III SL
95 1.3 )6.2 P III SL
95.5 1.3 )6.9 P III SL
96 1.4 )6.9 P III L
96.5 1.2 )7.0 P III L
97 1.3 )7.0 PII ⁄ III L
97.5 1.2 )7.7 PII ⁄ III L
Equant calcite 0.1 )8.4
Calcite cement 0.1 )8.2
Calcite cement 0.4 )12.1
Echinoderm 1 2.1 )8.3
Echinoderm 2 2.0 )6.1
Peloidal packstone 3.0 )4.9
Equant calcite inside the posterior filling of the shell. Calcite cements outside the shell. Echinoderm in the matrix outside the shell. Peloidal packstone in the
anterior geopetal filling of the shell. SEM ultrastructure: PIII = preserved tertiary layer, PII ⁄ III = preserved secondary ⁄ tertiary layers. CL, cathodolumi-
nescence; DL, detection limit; L, luminescent; NL, non-luminescent; SL, (dull orange) slightly luminescent.
Heterogeneity, cyclicity and diagenesis 1• L. Angiolini et al. Terra Nova, Vol 00, No. 0, 1–11
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have been protected from diagenetic
fluids, being in the shadow of the
convex ventral valve.
Analyses of the matrix of the sam-
ple (Table 1) show that the d18O
values of the equant calcite filling the
umbo and the Mg-calcite of associated
echinoderm fragments are lower than
those of unaltered brachiopod shell.
Is the geochemical record of the
accretionary growth periodical?
Not only is shell growth periodical,
but also regular oscillations of d18O
and d13C occur (Table 1 and Fig. 10).
d18O varies more regularly than d13C,
as has been previously observed in the
Lower Permian bivalve Eurydesma
cordatum (Ivany and Runnegar,
2010). If the growth lines represent
halts in the growth of the tertiary layer
during a seasonal fall in temperature
and ⁄or nutrient supply, the oscillation
of d18O can be tested against their
pattern. Considering only possibly
unaltered values, d18O is higher when
the sample coincides with a growth
line, whereas lower values occur in the
tertiary layer between growth lines
(Figs 10 and 11). This suggests that
growth lines represent winter halt of
growth as higher d18O values corre-
spond to lower sea temperature. As
the average oscillation of d18O is
about 1.1&, the sea surface tempera-
ture (SST) variation may have been
�5 �C (using )0.24& ⁄ �C after Craig,
1965). However, as there are still
many uncertainties about the isotopic
composition of Palaeozoic seawater
(e.g. Muehlenbachs and Clayton,
1976; Veizer et al., 1999; Came et al.,
2007; Ivany and Runnegar, 2010), we
cannot interpret absolute tempera-
tures.
To test the oscillation of the d18O
data we applied Fourier transform
analysis to the sequence of altered and
unaltered samples 40–97, which were
sampled sequentially to record up
to 230 month�s growth (Table 4
and Fig. 4). Following Schulz and
Fig. 9 Local diagenetic replacement of calcite by authigenic quartz. The authigenic quartz are subhedral crystal aggregates, mm-
sized, with the original calcareous shell at the nuclei. Transmitted ⁄polarized light and CL.
Table 2 Comparison of trace element data by LA-ICPMS (University of East Anglia)
and ICP (British Geological Survey) on different low luminescent parts of the shell.
n Na lg ⁄g Mg lg ⁄g Sr lg ⁄g Mn lg ⁄g Fe lg ⁄g
LA-ICPMS
(corrected) UEA
8 937 2868 1055 67 354
ICP BGS 25 na 3670 1135 65 249
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Stattegger (1997), we computed a
power spectrum (Fig. 12), which
shows peaks at 0.91, 1.602 and
2.83 years. Regression (least squares)
of sine and cosine terms for part of the
data sequence with a high sampling
rate confirmed that the 0.91 year cycle
is significant (F = 4.53 on 2, 23 d.f.;
P = 0.02) and consistent with a
12 month cycle (Fig. 13). Fourier
analysis on the altered and unaltered
parts seems thus to show that d18O
periodicity is annual and thus sea-
sonal, although other interannual
periodicity is also present (Fig. 12).
Carbon and oxygen isotopes
–2.0
–4.0
–6.0
–8.0
–10.0
–12.0
0.0
2.020 40 60 80 100
δ13C
an
d
18O
13C
18O
Fig. 10 d18O and d13C data for Gigantoproductus okensis. Numbers on the x-axis
represent samples from the umbo (0) to the anterior margin (97). The shell was
originally sampled sequentially at 97 points across growth lines; the shell was
subsequently re-sampled (between 71–77 and 87–97) to obtain 114 data points in total
(Table 1). Shading on the d18O plot shows altered parts of the shell based on CL, TE
and d18O values <)6.4&. The position of the growth lines relative to the isotopic
data is shown by the vertical dotted lines for samples which are in order of growth.
Table 3 Data table for the transverse section. Depth scale is in microns from the
inside edge of the shell where 0 = sample 1.
Depth (lm) Na lg ⁄g Mg lg ⁄g Mn lg ⁄g Fe lg ⁄g Sr lg ⁄g d18O& d
13C&
0 1587 2339 58 85 979 )5.24 0.92
200 1034 2607 116 77 978 )5.24 0.92
400 637 2990 56 357 1160 )5.24 0.92
600 750 3521 68 481 903 )5.30 )1.12
800 751 2634 110 764 919 )5.30 )1.12
1000 929 2523 56 435 1089 )5.30 )1.12
1200 657 3009 47 376 1162 )6.23 )1.74
1400 1150 3321 26 258 1250 )6.23 )1.74
1600 1177 3365 11 51 1185 )6.23 )1.74
1800 639 3517 51 175 1106 )7.25 )1.02
2000 230 2780 105 168 1082 )7.25 )1.02
2200 117 2190 165 220 828 )7.25 )1.02
2400 725 2411 134 140 893 )7.25 )1.02
2600 1490 3027 85 145 1019 )9.81 )0.54
2800 2162 3904 23 181 1149 )9.81 )0.54
3000 2252 4091 18 56 1296 )9.81 )0.54
3200 1090 2510 88 48 832 )10.30 )0.09
3400 252 3130 130 466 793 )10.30 )0.09
3600 81 2257 219 278 583 )10.69 )0.36
3800 )49 2389 138 204 660 )10.69 )0.36
4000 242 1721 350 545 497 )10.74 0.18
4200 218 1646 416 557 530 )10.74 0.18
4400 562 1872 24 36 700 )7.79 )0.28
4600 1285 2093 78 130 718 )7.79 )0.28
4800 452 1492 240 765 633 )6.49 0.39
5000 820 1269 259 687 478 )6.49 0.39
Table 4 Estimates of the age (expressed
in months) of sample points 40–97
considering their position with respect
to growth lines. Out of sequence of
growth samples have been excluded.
d13C d18O
1.3 )7.0 97 5 months
1.4 )6.9 96 9 months
1.3 )6.2 95 11 months
1.3 )6.5 94 16 months
0.9 )7.3 93 20 months
1.0 )6.3 92 22 months
1.1 )6.2 91 23 months
1.0 )6.5 90 27 months
1.2 )6.2 89 30 months
1.1 )6.4 88 34 months
1.2 )5.9 87 35 months
0.8 )6.1 86 37 months
0.5 )7.0 85 39 months
0.9 )7.3 84 42 months
0.6 )6.2 83 44 months
0.2 )6.0 82 46 months
0.2 )6.4 81 47 months
0.2 )6.5 80 49 months
)0.5 )6.3 79 53 months
)0.7 )6.5 78 56 months
)1.1 )6.0 77 58 months
)1.3 )5.9 76 59 months
)1.0 )6.2 75 61 months
)1.4 )6.1 74 66 months
)1.0 )5.8 73 71 months
0.0 )6.2 72 78 months
0.3 )9.7 70 85 months
)0.6 )7.0 69 90 months
)0.7 )7.0 68 95 months
0.1 )8.5 67 107 months
)2.6 )5.9 63 119 months
)2.2 )6.0 62 122 months
)2.6 )6.0 61 125 months
)2.5 )5.8 60 129 months
)0.5 )4.4 59 131 months
)0.4 )4.7 58 134 months
)1.3 )5.0 57 138 months
0.2 )4.8 56 143 months
)1.5 )5.2 55 160 months
)0.3 )4.9 53 167 months
)0.6 )5.5 52 179 months
0.8 )10.4 51 181 months
)0.3 )9.2 50 186 months
)0.9 )5.4 49 191 months
)0.5 )5.5 48 197 months
)0.3 )5.5 47 203 months
)1.2 )5.7 46 210 months
)0.8 )5.1 44 213 months
0.3 )4.9 43 218 months
)1.5 )5.6 41 222 months
)1.5 )5.9 40 225 months
)0.4 )5.3 42 230 months
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Heterogeneity, cyclicity and diagenesis 1• L. Angiolini et al. Terra Nova, Vol 00, No. 0, 1–11
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These periodicities may have been
caused by a seasonal climate affecting
palaeoequatorial Britain in the late
Mississippian (Scotese and McKer-
row, 1990). Indeed, monsoon rainfall
seasonality at this time has already
been deduced from palaeosols
(Wright, 1990) and fossil plant mor-
phology (Falcon-Lang, 1999). Also
Tucker et al. (2009) reported d18O
cyclicity in the Pendlelian Great Lime-
stone, interpreted as arid–humid
climate cycles.
Can a primary chemical and isotopic
signal be retained even after
diagenesis?
Both the raw data presented in Fig. 10
and the Fourier analysis (Figs 12 and
13) show that the annual periodicity
seems to be preserved as a residual
signal within the altered parts of the
shell, suggesting that cyclicity, if not
primary values, were retained when
diagenetic fluids locally permeated the
shell. d18O is systematically lower by
4–6&, but has the same periodicity in
the primary portion (inner shell) and
in the altered parts of the posterior,
anterior and external shell. Preserva-
tion of the original isotopic signal is
more common in carbon isotope data,
as the amount of C in the rock buffers
secondary C introduced within the
diagenetic fluid (Tucker, 1990; Sharp,
2007). Similar data on preserved iso-
tope cyclicity have been shown by
Rasser and Fenninger (2002), Valen-
cio et al. (2003), and Tucker et al.
(2009) though over a longer (millen-
nial) time-scale and with large rock
mass involved. This mechanism for
signal preservation in diagenetic rocks
is however, not fully understood.
Conclusions
This study reveals periodical variation
in growth and geochemistry of a
brachiopod shell, which may have
been linked to a seasonal climate, as
indicated by other proxies (e.g.
Wright, 1990; Falcon-Lang, 1999;
Tucker et al., 2009). The evidence
suggests that great variation in pres-
ervation ⁄alteration, as well as physical
and geochemical features can be seen
in a single shell, suggesting caution in
the interpretation of isotopic data
derived from spot-analyses, especially
in fossil shells. We also show that even
in diagenetically altered parts of the
shell, primary periodicity signals can
be preserved, even if primary values
are not. Thus, the results of the studyFourier transform analysis
0
0.5
1
1.5
2
2.5
3
3.5
0 1 2 3 4
Periodicity/frequency
Po
we
r/str
en
gth
of
pe
rio
dic
ity
Fig. 12 Power spectrum of the d18O time
series (Table 4) with signal peaks at 0.91,
1.602 and 2.83 years. The input data had
a maximum, minimum and mean sample
rate of 1.42, 0.08 and 0.37 years respec-
tively. At mean sampling rate, the Sam-
pling Theorem predicts a resolution of
0.74 cycles ⁄year, which is less than the
cycle of 0.91 years. Application of the
Siegel Test (Schulz and Stattegger, 1997)
was significant (P < 0.05) rejecting the
null hypothesis of white noise (random
variation) for the alternative of at least
three spectrum peaks.
Fig. 13 d18O values for altered (solid round symbols) and unaltered (solid square
symbols) densely sampled locations from umbo to the median part of the shell. Fitted
sine and cosine regression with a trend (continuous line) confirms the yearly cycle
(F = 4.53 on 2, 23 df; P = 0.02) and is consistent with a 12-month cycle both for
altered and unaltered samples.
–7.9 –6.2–5.9
–6.0–6.0
–5.8–4.4 –4.7 –4.8 –4.9–5.0
–5.2–5.5
–5.5–10.8 –9.2
–5.4
–5.5–5.7
1 mm
Fig. 11 Distribution of d18O data with respect to growth lines in the central part of the shell (data points 45–65). Bold italicized
numbers represent unaltered d18O data sampled at the growth lines, regular numbers represent unaltered d18O data sampled in the
growth increment and underlined numbers represent altered d18O data. Samples 65–67 represent a time reversal and they have not
been considered in the Fourier analysis (Table 4).
Colouronline,B&W
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Terra Nova, Vol 00, No. 0, 1–11 L. Angiolini et al. • Heterogeneity, cyclicity and diagenesis 1
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may have implications for under-
standing Palaeozoic climate dynamics
and far-reaching effects for isotope
proxy studies in general.
Acknowledgements
We are grateful to C. Malinverno and A.
Rizzi for sample preparation and SEM
assistance. Hilary Sloane at NIGL under-
took the stable isotope analysis. This
research was funded by the British Geo-
logical Survey. Stephenson, Leng, Mill-
ward and Williams publish this article
with the permission of the Director British
Geological Survey (NERC). This paper
benefitted from insightful reviews by Ethan
Grossman, the Editor and Associated Edi-
tors of Terre Nova and an anonymous
reviewer.
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Received 15 April 2011; revised version
accepted 24 September 2011
Terra Nova, Vol 00, No. 0, 1–11 L. Angiolini et al. • Heterogeneity, cyclicity and diagenesis 1
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