New chronostratigraphy of the Cretaceous–Paleogene boundary interval at Bidart (France
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Transcript of New chronostratigraphy of the Cretaceous–Paleogene boundary interval at Bidart (France
www.elsevier.com/locate/epsl
Earth and Planetary Science Letters 224 (2004) 19–32
New chronostratigraphy of the Cretaceous–Paleogene boundary
interval at Bidart (France)
Bruno Galbrun*, Silvia Gardin
Universite Paris VI, CNRS FR 32 ‘‘Centre Parisien de Geologie’’ Case 117, 4 place Jussieu, 75252 Paris cedex 5, France
Received 24 November 2003; received in revised form 24 April 2004; accepted 26 April 2004
Abstract
The Cretaceous–Paleogene boundary section at Bidart (French basque coast) was prevented for a long time to be considered
as a reference section for the K–T boundary due to a suspected hiatus comprising most of Chron C29r.
In our new magneto- and biostratigraphic study of this section we discovered that the underlying primary magnetic polarity
is not revealed in the vector directions but in a small, but consistent, intensity excursion during laboratory demagnetization
trends. Magnetite and maghemite are the main carriers of remanence, with contribution of hematite to the magnetic mineralogy
of the red-brown lowermost Danian and Maastrichtian marly limestones. Magnetite is the main magnetic mineral in the white to
pink Danian limestones. The NRM of marls and marly limestones is characterized by: (1) a present-day field overprint, (2) a
medium-temperature (300–400 jC) reversed component interpreted as a relic of the characteristic remanent magnetization
(ChRM) carried by magnetite grains which are not completely oxidized into maghemite, and (3) a high temperature (up to 590
jC) normal component due to late diagenesis hematite growth. The NRM of Danian limestones is characterized by (1) a
present-day field overprint and (2) a ChRM component of normal or reversed polarity.
The ChRM directions allow a new correlation of the magnetic polarity sequence with the Geomagnetic Polarity Time Scale
(GPTS): Chron C29r corresponds to the Maastrichtian unit and extends up to 3.5 m above the K–T boundary, and Chron C29n
occurs at the top of the section. There is no evidence for a hiatus at or below the K–T boundary, and the section does not extend
up to Chron C28r as previously suggested. These new chronostratigraphic assignments are in good agreement with the previous
biostratigraphic data and from the new biostratigraphic analyses based on calcareous nannofossils presented in this paper.
Our study demonstrates that the section of Bidart can be considered as a key section to study the K–T boundary event(s).
D 2004 Elsevier B.V. All rights reserved.
Keywords: magnetostratigraphy; Chron C29r; K–T boundary; calcareous nannofossils; Bidart; France
1. Introduction
Paleomagnetic interpretation is often an art; and
different people can analyze the same data and reach
0012-821X/$ - see front matter D 2004 Elsevier B.V. All rights reserved.
doi:10.1016/j.epsl.2004.04.043
* Corresponding author. Fax: +33-1-44273831.
E-mail addresses: [email protected] (B. Galbrun),
[email protected] (S. Gardin).
entirely different conclusions. The Bidart section
(French basque coast) (Fig. 1), one of the most
important Cretaceous–Paleogene boundary section
in Europe, is a good example to illustrate diverging
interpretations of the same data. A long-standing
apparent discrepancy between biostratigraphic and
paleomagnetic data [1] prevented this section to be
considered as a reference one for the K–T boundary
Fig. 1. Location map and lithology of the K–T boundary Bidart
section in SW France, south of town of Biarritz.
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3220
time interval. Our careful magneto- and biostrati-
graphic study shows that the published normal polar-
ity (interpreted as Chron C30n) and an associated K–
T boundary hiatus is, instead, an expanded record of
the K–T boundary interval with reversed polarity
(Chron C29r).
2. The Bidart section
In the Basque–Cantabric Basin of southwest
France a flysch zone persisted from Albian to Eocene
time allowing the accumulation of very thick forma-
tions of marl and marly limestone with some turbiditic
events [2]. Given the regional tectonics, all sections in
the basin are extremely faulted and discontinuous
[3,4].
The Bidart section crops out along the beach a few
kilometers south of Biarritz. This section, which dis-
plays Campanian and Maastrichtian formations, has
been subject to numerous stratigraphic and paleonto-
logic investigations [5–11], especially for the K–T
boundary interval [1,12–14].
The Bidart section was divided by Clauser [8] into
16 subunits separated by major faults. The K–T
boundary is easily identifiable between the Danian
white to pink massive limestone and the Maastrichtian
red-brown marls and marly limestones (Fig. 1). This
Maastrichtian unit is approximately 8 m thick and is
interrupted by a fault at the base. It consists of red-
brown marls and marly-limestones which become
grey 30 cm below the K–T boundary. This boundary
is marked by an abrupt lithological change: it consists
of a 15-cm-thick clay layer which is green at its base
and passes up to grey-brown and red at the top. The
clay horizon is overlain by red marly limestones,
followed by massive pink-white limestone 0.3 m
above the K–T horizon. A 60-cm-thick slump occurs
1.6 m above the K–T boudary. The Danian unit is
approximatively 20-m thick and is terminated by a
diapir of Triassic salt, but only 4 m of the unit can be
sampled for a magnetostratigraphic study before a
gully which make correlations somewhat difficult.
The magnetostratigraphy of this section was in-
vestigated by Delacotte et al. [1] who recognized
normal and reversed magnetozones and proposed
correlations with the reference section of Gubbio
(Italy). According to these authors, the uppermost
Maastrichtian was assigned to Chron C30n. Thus, a
large hiatus corresponding to the Cretaceous part of
Chron C29r was suspected below the K–T boundary
although the biostratigraphic data did not confirm its
occurrence.
Recently morphometry of coccoliths and geo-
chemical analyses were performed on this section
[15–17], but the controversy between biostrati-
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 21
graphic and magnetostratigraphic results remained
unsolved.
3. Biostratigraphy
3.1. Planktonic foraminifera
Premoli-Silva [1] reported that Abatomphalus
mayaroensis, the uppermostMaastrichtian index fossil,
was not encountered in the 8 m of sediments studied.
According to Haslett [9] the 8 m of the studied section
belong to the uppermost Maastrichtian Pseudotextu-
laria deformis zone. This planktonic foraminifer zone
was defined by Keller [18] when A. mayaroensis is
very rare or missing in the uppermost Maastrichtian
sediments, especially in low latitude sections. More
recently Apellaniz et al. [14] recognized the A. mayar-
oensis zone on the (rare) presence of the index species.
The basal 10 cm of the Danian portion of the
section contain only benthic foraminifera (Premoli-
Silva in [1],[14]). According to Haslett [9] and Apel-
laniz et al. [14] this thin interval belongs to the
Guembelitria cretacea zone of Smit [19]. This is
followed by the Parvularugoglobigerina eugubina
zone at about 10 cm above the boundary ([9,14],
Premoli Silva in [1]) and by the Parasubbotina
pseudobulloides zone from 70 cm (Premoli Silva in
[1]). Haslett [9] and Apellaniz et al. [14] found a
younger first occurrence (FO) of P. pseudobulloides at
about 2 m above the boundary.
3.2. Calcareous nannofossils
Perch-Nielsen [1] recorded the upper Maastrichtian
Micula prinsii subzone [20] from the base of the section
she studied (8 m below the Maastrichtian-Danian
boundary). Due to different sampling strategies, the
FO of M. prinsii was reported at different levels
according to the authors who studied this section:
Gorostidi and Lamolda [10] found it at about 7 m
below the boundary; Manivit [8] reported the FO ofM.
prinsii at about 20 m below the boundary. The Danian
sediments belong to the Biantholithus sparsus Zone of
Perch-Nielsen [21] up to the limestone bed just below
the slump and to the Cruciplacolithus primus zone of
Perch-Nielsen [21] from this slump up to the top of the
studied section (Perch-Nielsen in [1], [10,13]).
In our study, splits of samples used for magneto-
stratigraphy were processed to obtain standard smear-
slides for calcareous nannofossils analysis, in order to
establish first order correlations between the nanno-
fossil datums and the magnetic polarity pattern. Cal-
careous nannofossils were investigated on more than
350 fields of view per slide using a light microscope
at 1350� to detect presence/absence of key species.
Assemblages are in general abundant and moderately
preserved.
Our study confirms the occurrence of M. prinsii in
the 8 m of Maastrichtian strata below the K–T
boundary, though its occurrence may be discontinuous
due to preservation because this taxon is dissolution
prone and difficult to confidently identify if poorly
preserved. Nephrolithus frequens is rare but present in
the Maastrichtian samples together with more com-
mon Litraphidites quadratus, Micula murus, and
sparse Ceratholithoides kamptneri. These data are a
further confirmation of the late Maastrichtian age
recorded by previous authors.
The Danian age of the upper part of the section is
also confirmed by our data and a more detailed
succession of calcareous nannofossil events is provid-
ed : the FO (first occurrence) of C. primus (both small
and regular morphotypes; see Appendix A) and
Futuyana petalosa (sample + 1.64), the FO of Cruci-
placolithus intermedius (sample + 2.43), the FO of
Coccolithus pelagicus (sample + 2.49), the FO of
Praeprinsius dimorphosus (sample + 3.30), and the
FO of Cruciplacolithus tenuis (early morphotypes;
sample + 3.59) (Plate 1, Appendix A). This succes-
sion of nannobiohorizons, directly correlated with
magnetochrons in our study, is similar to the nanno-
fossil succession found in the basal Danian in most of
middle to low latitude sections ([21–23] and refer-
ences herein). The presence of a sedimentary slump in
the Danian sequence is biostratigraphically shown to
be associated with a hiatus based on the following
evidence: (1) the FOs of C. primus (both small and
regular morphotypes) and F. petalosa in the same
sample while they normally occur delayed, and (2) the
lack of the «dwarf Biscutum bloom» interval [24],
which normally occurs in most of low latitudes
sections. The marker species of Zone CP2 [25] and
NP3 [26], Chiasmolithus danicus, was not encoun-
tered in the 4 m of Danian strata, either in this study or
in the previous ones.
Plate 1. Key species of calcareous nannofossils. All micrographs are under polarized light. (1) Micula murus, sample �8.05 m. (2) Micula
prinsii (overgrowth specimen), sample �8.05 m. (3) Cruciplacolithus primus < 5Am (small morphotypes), sample + 1.64 m. (4–5)
Cruciplacolithus primus > 5Am, sample + 1.64 m. (6) Cruciplacolithus intermedius, sample +2.43 m. (7) Neobiscutum parvulum, sample + 0.60
m. (8) Futuyania petalosa, sample + 1.64 m. (9) Coccolithus pelagicus, sample + 2.49 m. (10–11) Cruciplacolithus tenuis (early morphotypes),
samples + 3.59 and + 3.70 m. (12) Praeprinsius dimorphosus, sample + 3.30 m.
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3222
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 23
4. Paleomagnetic analysis
Samples were collected using a portable gasoline
powered drill, and oriented with a magnetic compass.
Average sampling spacing was dependent on the lithol-
ogy and was generally 10–30 cm; the soft Cretaceous
marly limestone was sampled with a larger interval. A
total of 49 samples was collected and analyzed.
4.1. Rock magnetism
A set of rock magnetic experiments was conducted
to characterise and identify the magnetic mineralogy of
the two main lithologies. We first analyzed the acqui-
sition of IRM (Isothermal Remanent Magnetization)
up to 1.6 T and its subsequent thermal demagnetiza-
tion. Following the procedure described by Lowrie
[27], magnetic fields of 1.6, 0.4 and 0.12 T were
successively applied to each of the three perpendicular
directions prior to thermal demagnetization (Fig. 2).
For the white to pink Danian limestone, 90% of the
maximum IRM is acquired below 0.2 T and saturation
was achieved at 0.4 T (Fig. 2A). Thermal demagneti-
zation shows that the low field (0.12 T) component is
dominant and decreases up to a maximum unblocking
temperature of approximately 580 jC indicating mag-
Fig. 2. IRM acquisition of two typical samples (A, C) and thermal demagne
field strenghs (B, D) (stratigraphic levels refer to K/T boundary level as 0
netite (Fig. 2B). The harder components, less than 5%
of the total IRM, decrease regularly up to temperature
of 300–350 jC and suggest the presence of a Fe-
sulphide (pyrrhotite or greigite).
The acquisition of IRM for the Maastrichtian marly
limestones shows also an initial steep rise until approx-
imatively 0.2 T (80%) and saturation do not complete-
ly occur in applied field up to 1.6 T (Fig. 2C). The low
coercivity component corresponds to a maximum
unblocking temperature of approximately 580 jCwhich indicates magnetite (Fig. 2D). However, the
decreasing intensity curve of this component displays
an intermediate unblocking temperature of 200–250
jC which probably corresponds to the presence of
maghemite [28]. The presence of maghemite is possi-
bly the result of low-temperature oxidation of magne-
tite, likely explained by intense weathering of these
beach outcrops. The relative contribution of these two
low coercivity components to the IRM is difficult to
estimate. The high coercivity component shows an
unblocking temperature of 100 jC indicating the
presence of goethite. Unblocking temperatures greater
than 600 jC for the medium blocking field component
may indicate low coercivity hematite.
Hysteresis loops in fields up to 0.8 T were estab-
lished for some samples. A typical Maastrichtian marly
tization of IRM acquired in three orthogonal directions with different
m.).
Table 1
Fitted IRM component parameters for a typical Maastrichtian marly
limestone
Sample Component SIRM
(A/m)
B1/2
(mT)
Range
(mT)
Contribution
(%)
–4.3 m 1 0.18 21 16.2–27 11
2 1.46 66 49–112 87
3 0.04 372 310–447 2
The fitting procedure used was that of Kruiver et al. [30].
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3224
limestone shows a strong paramagnetic signal caused
by clay minerals (Fig. 3a). After subtracting this
paramagnetic component, the ferrimagnetic compo-
nent appears clearly (Fig. 3b): it is mostly due to low
coercivity minerals, confirming the previous IRM
analysis. Given the weakness of the magnetization in
Danian limestones no reliable hysteresis loop could be
established from these samples.
To estimate the relative contribution of the indi-
vidual magnetic minerals to the bulk IRM, especially
the red-brown marly limestone, we tried to decompose
the IRM acquisition curves into their magnetic com-
ponents [29]. We used the IRM fitting program of
Kruiver et al. [30]. Each magnetic component can be
described by: (1) its saturation IRM (SIRM) and thus
its contribution to the bulk IRM curve; (2) B1/2, the
applied field at which half of the SIRM is reached;
Fig. 3. Hysteresis loop up to 0.8 T of a typical Maastrichtian marly
limestone (a), and ferrimagnetic hysteresis loop after subtracting the
paramagnetic contribution (b).
and (3) DP, the dispersion parameter of the cumulative
log-normal distribution. The procedure requires inter-
active analysis towards the final model fit by optimis-
ing the IRM components parameters to minimize the
residuals between the measured data and fitted curves.
Different solutions with two or three components
were tested. The three-component fits are significantly
better, as statistically tested, than the two component
fits; they are also more in accordance with the
previous results of IRM thermal demagnetization
curves. The three-component fit of a typical sample
(Table 1) reveal a high coercivity component (mean
372 mT), as well as the differentiation of two separate
low coercivity components (means 21 and 66 mT).
The high coercivity magnetic component corresponds
most probably to hematite, and perhaps to goethite, as
suggested from the thermal demagnetization curves of
the IRM medium (0.4 T) and high field (1.6 T)
components on Fig. 2D. No distinction can be made
between hematite and goethite because of their coer-
civity overlap. The two low coercivity components
are in accordance with the results suggested by the
thermal demagnetization curves of the IRM 0.12 T
field component (Fig. 2D), in which two components
were discriminated by their unblocking temperatures.
Component 1 of lower coercivity (mean 21 mT) is
probably magnetite with an unblocking temperature of
approximately 580 jC (Fig. 2D), and component 2
(mean 66 mT) corresponds probably to magnetite
partially oxidized to maghemite with intermediate
unblocking temperature of 200–250 jC.
4.2. Natural remanent magnetization (NRM) analysis
The NRM of all samples analyzed was measured
with a three-axis RS-O1 LETI/CEA cryogenic mag-
netometer. Each sample was measured in eight ori-
entations, using four readings at each orientation for
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 25
weak samples. The NRM intensities display a large
variation depending on lithology. The red-brown
Maastrichtian marly limestone has an average inten-
sity of 15 mA/m; the NRM intensity drops to 0.2–0.4
mA/m in a 15-cm-thick grey bed 30 cm below the K–
T boundary, and then increases again until the bound-
ary. The lowermost Danian marly limestone shows the
Fig. 4. Susceptibility changes during thermal demagnetization of
two typical white Danian limestones (A) and three red-brown
Maastrichtian marly limestones (B).
highest NRM intensities values of the section, up to
35 mA/m. The NRM decreases in the white to pink
Danian limestone to 0.4 mA/m, with the exception of
the slump which displays NRM intensity values quite
similar to the Maastrichtian marly limestone. Usually
slumps are avoided by paleomagnetists, but the Dan-
ian slump of the K–T boundary Bidart section was
previously studied by Delacotte et al. [1] who defined
a normal polarity for this unit and correlated it to
Chron C29n. We studied it also to test this chrono-
stratigraphic assignment.
To determine characteristic remanent magnetization
directions and to establish the magnetostratigraphy of
the section, we thermally demagnetised one sample
from each stratigraphic level. Since heating often
induces chemical changes, we have monitored the
intial susceptibility Xin during thermal demagnetiza-
tion for a set of samples of each lithology (Fig. 4). For
the Danian white to pink limestone the Xin does not
display any variation up to 400 jC (Fig. 4A). Suscep-
tibility strongly increases in the range 400–500 jCand then decreases at temperature higher than 500 jC.Such increasing trends have been attributed to oxida-
tion of pyrite and formation of magnetite [31]. The
variations of magnetic susceptibility during heating of
Maastrichtian brown marly limestones are different
(Fig. 4B). Xin decreases up to 300 jC, remains stable,
increases from 400 to 500 jC, and finally decreases
again slowly. The decay of susceptibility up to 300 jCcould indicate the presence of maghemite as suspected
from IRM analysis. The increasing of Xin at 400 jCcan be interpreted as the transformation of pyrite to
magnetite. Despite this increasing of Xin in all lithol-
ogies, no creation of large amount of single domain
magnetite and induced large viscous remanent mag-
netization were observed. Thus the thermal demagne-
tization can be used without any problem as an
effective magnetic cleaning for all the samples.
Thermal demagnetization was performed up to 450
jC with 50 jC steps, and up to 590 jC with steps of
25–30 jC. A multicomponent behaviour of the NRM
is clear in the majority of the samples (Figs. 5 and 6),
especially in the red-brown marly limestone. The
directions of the components of magnetization were
analyzed by a least-squares fit of a line through
selected data points [32].
Representative thermal demagnetization diagrams
of the Maastrichtian and lowermost Danian samples
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3226
show up to four components (Fig. 5): (1) a viscous
component, removed at 100 jC, (2) a low-temperature
(LT) component ranging 100–300 jC, with a present
day field direction (declination 6j and inclination
60j), (3) a reversed polarity medium-temperature
(MT) component, removed between 300 and 400
jC, and (4) a normal polarity high temperature (HT)
component ranging from 400–450 to 560–590 jC.The MT and HT components are antiparallel. In the
levels displaying the highest NRM intensities—i.e.,
lowermost Danian marly limestones and some levels
in the last meter of Maastrichtian—only the LT and
HT components are visible, the MT component is
missing or forms a cluster (Fig. 5, sample + 0.38 m).
This type of behaviour is also seen in samples from
the Danian slump, 1.6 m above the K–T boundary
(Fig. 6, sample + 2.03 m).
The Danian white to pink limestone shows a more
common behaviour (Fig. 6, samples + 0.93, + 2.22
and + 3.69m) : (1) a very soft component is removed at
100 jC, (2) a normal polarity, low temperature (LT)
component removed between 100 and 250/300 jC, and(3) a normal (sample + 3.69 m) or reversed (samples
+ 0.93 and + 2.22 m) high temperature (HT) compo-
nent removed between 300/350 and 500/590 jC.
5. Discussion
The results of the magnetic mineralogy and NRM
analysis require to discuss the origin of each magnetic
component and to assess which one is the character-
istic remanent magnetization (ChRM) representing the
Earth’s magnetic field at the time of deposition.
For the Maastrichtian and lowermost Danian red-
brown marls and marly limestones (Fig. 5), the LT
component is a recently acquired overprint, contribut-
ing most of the NRM. It likely corresponds to the low
coercivity (0.12 T) component with an unblocking
temperature of 250–350 jC (Fig. 2D), and to compo-
nent 2 of the IRM analysis (Table 1). This component is
Fig. 5. Orthogonal demagnetization plots of typical samples of
Maastrichtian and lower Danian red marls and marly limestones
(stratigraphic levels � 8.05, � 5.05 and � 0.05 m below the K–T
boundary, and + 0.38 m above the boundary). Open and closed
circles represent projections on the vertical and horizontal planes,
respectively.
Fig. 6. Orthogonal demagnetization plots of typical samples of
Danian white to pink limestones (stratigraphics levels + 0.93,
+ 2.22 and + 3.69 m above the K–T boundary), and of the Danian
slump ( + 2.03 m). Open and closed circles represent projections
on the vertical and horizontal planes, respectively.
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 27
most probably carried by maghemite due to weathering
and seems more prominent approximatively 1 m below
and above the K–T boundary, an interval of soft marls
which is more susceptible to weathering.
The MT component, of reversed polarity, is defined
only between 300 and 400 jC; we are confident that
this component represents a relic of the primary
magnetization. It is probably carried by magnetite
grains which are not completely oxidized into maghe-
mite. Magnetite appears on the thermal demagnetiza-
tion curves of the IRM 0.12 T field component (Fig.
2D) with a maximum unblocking temperature of 580
jC, and is probably the component 1 on IRM compo-
nents analysis (B1/2 = 20 mT) (Table 1). The HT
component of normal polarity, ranging from 400–
450 to 560–590 jC, is possibly due to authigenic
pigmentary hematite as evident from the red-brown
colour of the marly limestones. This hematite compo-
nent corresponds to the component 3 of the IRM
analysis component (Table 1). From a relative large
spectrum of grain sizes, it results in a large spectrum of
unblocking temperature and field coercivity [33] that
seems to be the case here. Such hematite growth could
occur early in the diagenetic evolution and continue for
several hundreds of thousand years after the deposition
of the host sediment. In the case of the Bidart section,
the uppermost Maastichtian and lowermost Danian
marl and marly limestone were deposited during a
period of reversed polarity (C29r). The growth of
pigmentary hematite, which occured in late diagenesis,
recorded a normal polarity corresponding to the field
of a subsequent normal period, probably C29n.
Only the LT and HT components are present in
some levels around the K/T boundary, which were
more subject to weathering (Fig. 5, sample + 0.38 m),
and in the Danian slump (Fig. 6, sample + 2.03 m).
Likely the slump stayed longer time in an unconsol-
idated state than the massive Danian limestones and
so it may have acquired the secondary normal polarity
overprint due to hematite. The white to pink Danian
limestone is more easy to interpret (Fig. 6). The
normal polarity LT component, ranging from 100 to
250/300 jC, is again an overprint due to weathering,
while we interpret the normal or reversed HT com-
ponent, removed between 300/350 and 590 jC, to be
the primary component.
Thus, the directions of MT component from Maas-
trichtian and lowermost Danian marls and marly
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3228
limestones and of HT component from white to pink
Danian limestones are the ChRM directions and are
used to define the magnetic polarity sequence of the
section (Fig. 7). Not all the samples studied could give
a reliable ChRM, but the mean directions computed
on those we are confident are ‘‘quite antiparallel’’
Fig. 7. Lithology of the K–T boundary section at Bidart, calcareous n
directions (declination, inclination), polarity sequence (black/white is norm
of Delacotte et al. [1]. ChRM directions (Middle temperature component
and high temperature component in the Danian limestone) are plotted as b
Maastrichtian marly limestones, the lower Danian limestones and the Dan
(Table 2). On these two populations we applied the
reversal test of McFadden and McElhinny [34]: the
critical angle cc is 21.16j and the observed angle cobetween the two mean polarities is 5.4j. The reversaltest is thus positive and classified as class B according
to [34]. This supports the primary origin of these
annofossil biostratigraphic events, NRM intensity, paleomagnetic
al/reversed polarity) and Chron assignment, previous interpretation
in the Maastrichtian marly limestones and lower Danian limestones
lack circles; the high temperature normal overprint directions in the
ian slump are plotted as open circles.
Table 2
Means characteristic remanent magnetization directions. (a) Normal
polarity samples at the top of the section excluding those from the
Danian slump, (b) all reversed polarity samples, (c) reversed samples
with reliable ChRM directions
N D I k a95
Normal (a) 4 14.9 46 41.3 14.5
Reversed (b) 34 204.4 � 51 6.6 10.4
Reversed (c) 27 197.0 � 51 16.8 7
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 29
ChRM directions. The established magnetic polarity
sequence is characterized by a reversed magnetozone
which includes the entire Maastrichtian part of the
section and up to 3.5 m above the K–T boundary, and
a normal magnetozone at the top of the section (Fig.
7). Considering the reliable biostratigraphic data and
the position of the K–T boundary it is possible to
correlate the proposed magnetic polarity sequence to
the GPTS: the reversed magnetozone corresponds to
Chron C29r and the subsequent normal magnetozone
belongs to Chron C29n.
This interpretation differs substantially from the
one provided by Delacotte et al. [1]. These authors
recognized a normal polarity for most of the Maas-
trichtian unit of the section and assigned it to Chron
C30n (Fig. 7). Thus, a long hiatus corresponding to
the Cretaceous part of Chron C29r was suspected
below the K–T boundary. Such a long hiatus is not
supported by the biostratigraphic data: the 8 m studied
below the K/T boundary belong to the uppermost
Fig. 8. Summary of paleomagnetic and biostratigraphic data across the late
[23,35–40]).
Maastrichtian planktonic foraminifera zone, the P.
deformis Zone [9]. The calcareous nannofossil M.
prinsii occurs within the 8 m studied, while its FO
is defined near the Chrons C29r–C30n boundary [35]
(Fig. 8). The present section can thus be attributed to
Chron C29r, though we cannot completely rule out the
hypothesis that this reversed interval does not repre-
sent the entire late Cretaceous part of the Chron. The
absence of the planktonic foraminifer Plummerita
hantkeninoides (Premoli-Silva in [1]) [9], its FO
defining the uppermost Maastrichtian CF1 Zone of
Keller [18] and within the M. prinsii subzone, might
indicate a missing uppermost Maastrichtian. However
the planktonic foraminifera assemblages of this sec-
tion are scarce and poorly preserved (Premoli-Silva in
[1],[9]) and thus do not represent the best means of
identifying a missing/absent uppermost Maastrichtian
interval.
In the lowermost Danian, Delacotte et al. [1]
defined some levels of reversed polarity as Chron
C29r (Fig. 7). They assigned a normal polarity for
the Danian slump and correlated it with Chron C29n.
The next polarity intervals were thus assigned to
Chrons 28r and 28n. However, the calcareous nanno-
fossil events found in this investigation and in previous
studies are more indicative of an earliest Danian age
and correlate well with the upper part of Chron C29r
and Chron C29n for the following reasons: (1) assemb-
lages are dominated by abundant Thoracosphaera spp.
and F. petalosa with few Cruciplacolithus species and
Maastrichtian–early Danian considered in this work (data are from
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–3230
Cretaceous species still present, these assemblages are
typical of earliest Danian [21]; (2) the FOs of C.
pelagicus and P. dimorphosus were recorded within
the lowest Paleocene NP2 and CP1 zones of Martini
[26] and Okada and Bukry [25] by previous authors
([23] and references herein); (3) early morphotypes of
C. tenuis were observed from sample + 3.59, which is
indicative of a normal polarity interval (interpreted
here as C29n), in agreement with the findings of
Berggren et al. [23]; (4) the calcareous nannofossil
C. danicus, whose FO lies in the uppermost part of
Chron C29n [23], was not encountered. Thus, the
interpretation of the normal interval at the top of the
studied section and the slump to Chrons C28n and
C29n respectively is highly unlikely.
Delacotte et al. [1] interpreted their paleomagnetic
data from the marl and marly limestone using the
directions of the high temperature (HT) component as
the primary directions. They have not detected the
medium temperature (MT) component, mainly be-
cause they used a spinner magnetometer which did
not allow precise measurements.
6. Conclusion
Rock magnetic analysis, careful thermal demagne-
tization and analysis of NRM components allow us to
propose a new magnetostratigraphic interpretation of
the K–T boundary Bidart section (France).
Magnetite, maghemite, and hematite are the car-
riers of remanence in the red-brown lowermost Dan-
ian and Maastrichtian marly limestones. The NRM of
these strata is dominated by a double normal overprint
due to, (1) a low-temperature (100–300 jC) present-day field overprint probably resulting from weather-
ing and its resultant maghemitisation and, (2) a high
temperature (up to 590 jC) normal component caused
by late diagenesis hematite growth. The characteristic
remanent magnetization (ChRM) carried by magnetite
grains which are not completely oxidized into maghe-
mite appears only as a relic reversed component of
medium temperature ranging from 300 to 400 jC.Magnetite is the main magnetic mineral in the
white to pink Danian limestones in which the NRM
is characterized by a secondary present day field
overprint and a ChRM component of normal or
reversed polarity.
A new magnetic polarity sequence is established,
and we propose a new correlation with the GPTS. The
Maastrichtian unit and the limestone beds up to 3.5 m
above the K–T boundary are of reversed polarity and
correspond to Chron C29r. A normal magnetozone
occurring at the top of the section is correlated with
Chron C29n.
These chronostratigraphic assignments are well in
accordance with the previously established biostrati-
graphic data and the new calcareous nannofossil data
presented in this paper. The calcareous nannofossil M.
prinsii, whose FO is defined around the boundary
between Chrons C29r and C30n occurs in the entire
8 m below the K–T boundary. This allows the
confident correlation of the Maastrichtian sediments
with Chron C29r. The succession of calcareous nan-
nofossil FOs above the K–T boundary (FO of C.
primus, C. intermedius, C. pelagicus, P. dimorphosus
and early morphotypes of C. tenuis), indicates an
earliest Danian age correlating well with Chrons
C29r and C29n. On the contrary, C. danicus, whose
FO lies at the base of Chron C28r [23], was not
encountered either in this or in the previous studies.
From the magnetostratigraphic and biostratigraphic
point of view, there is no evidence for a hiatus at
the K–T boundary section at Bidart. This section is
thus suitable to carry out high-resolution studies of
the paleoenvironmental changes across the K–T
boundary.
Acknowledgements
We are grateful to our collegues Xixi Zhao
(University of Santa Cruz) and Mark Leckie (Univer-
sity of Massachussets) for their suggestions and
careful review of an early draft of the paper. Jim
Ogg (Purdue University) is warmly thanked for
comments and opening paragraph, we are grateful to
Cor Langereis (Utrecht University) for his very
detailed and constructive review. The rock magnetism
analysis were performed at the Institut de Physique du
Globe de Paris, we thank Maxime Legoff for
assistance. Thanks to Pauline Kruiver (Utrecht
University) who helped us by mail to use her IRM
fitting program while we were on the ODP Leg 210 in
the Atlantic Ocean. We thank Eric Robin and Robert
Rocchia for assistance in the field. [VC]
B. Galbrun, S. Gardin / Earth and Planetary Science Letters 224 (2004) 19–32 31
Appendix A. Taxonomy of calcareous nannofossil
species cited in the text
� Ceratolithoides kamptneri Bramlette and Martini,
1964� Coccolithus pelagicus (Wallich, 1871), Schiller,
1930� Cruciplacolithus intermedius van Heck and Prins,
1987
Remarks: In this study we considered as C. inter-
medius a Cruciplacolithus having a length of more
than7Amanda thick, robust cross in the central area.
� Cruciplacolithus primus Perch-Nielsen, 1977
Remarks: The first C. primus to occur in basal
Danian are 3–4 Am in length (early morphotypes).
‘‘Regular’’ morphotypes are 5–7 Am in length.
Both morphotypes display a thin, weakly birefrin-
gent cross in the central area.
� Cruciplacolithus tenuis (Stradner 1961), Hay and
Mohler in Hay et al., 1967
Remarks: InthisworkC.tenuis isintendedastheform
having «feet» (calcite blocks) at the end of the central
cross (shown by Romein, 1979). The specimens
shown in Plate 1 (10,11) having incoming, small,
calcite blocks visible when the specimen is rotated at
45j,areconsideredasearlymorphotypesofC.tenuis.
� Futuyania petalosa (Ellis and Lohmann, 1973),
Varol 1989� Lithraphidites quadratus Bramlette and Martini,
1964� Micula murus (Martini, 1971), Bukry, 1973� Micula prinsii Perch-Nielsen, 1979a� Nephrolithus frequens Gorka, 1957� Neobiscutum (Romein, 1979) Varol 1989� Praeprinsius dimorphosus (Perch-Nielsen 1969),
Varol and Jakubowsky, 1979� Thoracosphaera Kamptner, 1967, spp.
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