Marine Micropaleontology 51 (2004) 95 – 128
www.elsevier.com/locate/marmicro
Age and paleoenvironment of the Cenomanian–Turonian
global stratotype section and point at Pueblo, Colorado
Gerta Keller a,*, Alfonso Pardo b
a
Department of Geosciences, Princeton University, Guyot Hall, Princeton, NJ 08544-1003, USA
b
Fundacion San Valero, Violeta Parra N 9, E-50015 Saragossa, Spain
Received 4 February 2003; received in revised form 1 July 2003; accepted 15 August 2003
Abstract
Biostratigraphy and stable isotopes indicate that the global stratotype section and point (GSSP) at Pueblo contains an
essentially complete sedimentary record across the global ocean anoxic event (OAE 2) and the Cenomanian – Turonian
boundary. The OAE 2 d13C shift occurred over a period of about 90 ky and was accompanied by a major sea level transgression,
which at its peak was marked by an incursion of oxygen-rich waters creating a benthic oxic zone that lasted about 100 ky. A
mid-Cenomanian d13C shift, sea level transgression and faunal turnover occurred about 2 my before OAE 2. d18O values of the
planktic foraminifer Hedbergella planispira and its relative abundance changes reveal cyclic variations in surface salinity due to
alternating freshwater influx and marine incursions, whereas dominance by the low oxygen tolerant Heterohelix species
indicates a well-developed oxygen minimum zone (OMZ) for most of the middle to late Cenomanian and early Turonian.
Profound faunal changes accompanied these oceanographic events, including the extinction of 30% of the species
assemblage and an equal gain in evolutionary diversification, though the overall combined relative abundances of outgoing and
incoming species were less than 2% and 4%, respectively, of the total assemblages. The faunal turnover began with the sea level
transgression and rapid increase in d13C values, and accelerated with the influx of oxygen-rich deep water, increased water mass
stratification and competition during the benthic oxic zone. The incursion of oxygen-rich deep waters at this time was also
observed in Morocco and may represent a global event of a still unknown source.
D 2003 Elsevier B.V. All rights reserved.
Keywords: Cenomanian – Turonian; Pueblo GSSP; paleoenvironment; planktic foraminifera
1. Introduction
During the late Cenomanian, the Western Interior
Sea (WIS) was characterized by generally low sea
levels, high terrigenous influx and low salinity, an
* Corresponding author. Tel.: +1-609-258-4117; fax: +1-609258-1671.
E-mail address: gkeller@princeton.edu (G. Keller).
0377-8398/$ - see front matter D 2003 Elsevier B.V. All rights reserved.
doi:10.1016/j.marmicro.2003.08.004
environment that supported few marine invertebrates
or foraminifera (Kauffman, 1984; Cobban, 1985;
Elder, 1985). Benthic foraminifera were generally rare
(Eicher, 1969a) and low-diversity assemblages of
planktic foraminifera persisted in the deepest parts
of this seaway (Eicher and Diner, 1989; Leckie et al.,
1998). During the late Cenomanian to early Turonian
a major sea level transgression expanded the WIS
(Greenhorn Sea) northward to the Arctic slope, transporting normal, saline, subtropical marine waters and
96
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 1. Location of the Pueblo GSSP in the Rock Canyon Anticline area of Lake Pueblo State Park, Colorado. The section is exposed along the
road on the lakeside.
Fig. 2. Outcrop of the Pueblo section exposed on the road along Lake Pueblo showing exposure of the Hartland Shale and Bridge Creek
Limestone.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
97
Plate 1. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. All specimens are from the R. cushmani zone. Scale
bar = 200 Am. Specimens 1 – 4: R. greenhornensis (Morrow). Specimens 5 – 7: R. cushmani (Morrow). Specimens 8 and 12: R. deekei (Franke).
Specimens 9 and 11: R. montsalvensis Mornod. Specimens 13, 14, 15 and 16: Rotalipora-A. multiloculata transition.
98
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Plate 2. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. All specimens from the R. cushmani zone. Scale bar = 100
Am for specimens 1 – 5, all others 200 Am. Specimens 1 – 5: A. multiloculata (Morrow), A. multiloculata subzone of R. cushmani zone.
Specimens 6 – 8: Praeglobotruncan aumalensis (Sigal). Specimens 9 – 11: P. stephani (Gandolfi). Specimens 12 – 14, 15 and 16: P. gibba Klaus.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
99
Plate 3. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. Scale bar = 200 Am for specimens 1 and 2, all others 100
Am. Specimens 1 and 2: P. praehelvetica (Trujillo), upper R. cushmani zone. Specimens 3 and 4: H. helvetica (Bolli), base H. Helvetica zone
(Bed 89, Pueblo). Specimens 5 – 7: P. inornata (Bolli), upper R. cushmani zone. Specimens 8 and 11. D. algeriana (Caron), upper R. cushmani
zone. Specimens 9 and 10: D. imbricata (Mornod), lower W. archaeocretacea zone. Specimens 12 – 14, 15 and 16: Whiteinella archaeocretacea
Pessagno, lower W. achaeocretacea zone, D. hagni subzone.
100
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Plate 4. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. Scale bar = 100 Am, specimens 1 – 9; 200 Am for specimens
10 – 15. Specimens 1 and 2: W. archaeocretacea Pessagno, lower W. achaeocretacea zone, D. hagni subzone. (Specimens 3, 4, 7, 8): W. baltica
Douglas and Rankin, R. cushmani zone. (Specimens 5, 6, 9): W. aprica (Loeblich and Tappan), W. achaeocretacea zone, H. moremani subzone.
Specimens 10 – 14 and 15: W. brittonensis (Loeblich and Tappan), R. cushmani zone.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
101
Plate 5. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. Scale bar = 100 Am. Specimens 1 – 4: W. paradubia (Sigal),
upper R. cushmani zone. Specimens 5 – 9: H. delrioensis (Carsey), R. cushmani zone. Specimens 10 and 11: H. simplex (Morrow), R. cushmani
zone. Specimens 12 – 14: G. ultramicra (Subbotina). Specimens 15 – 18: G. bentonensis (Morrow), W. archeocretacea zone, G. bentonensis
subzone.
102
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Plate 6. SEM illustrations of planktic foraminifera from the Pueblo GSSP, Colorado. Scale bar = 100 Am for specimens 1 – 614, R. cushmani zone.
Scale bar = 50 Am for specimens 15 and 16, W. archaeocretacea zone. Specimens 1 – 5: H. planispira (Tappan). Specimens and 7: Heterohelix cf.
moremani (morphotype with compressed chambers). Specimens 8 – 10: H. moremani (Cushman). Specimens 11 – 14: H. reussi (Cushman).
Specimens 15 and 16: G. cenomana (Keller).
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
their biotas (Kauffman, 1984; Caldwell and Kauffman, 1993; Leckie et al., 1998). With the onset of this
transgression during the latest Cenomanian, bottom
water conditions abruptly improved as observed by
the establishment of diverse warm water mollusk and
calcareous benthic foraminiferal assemblages (‘‘benthic zone’’ of Eicher, 1969b). A positive excursion in
d13C values of organic carbon marks a major increase
in productivity, the onset of low oxygen conditions
and a major turnover in planktic foraminifera (Elder,
1985). These events have been studied extensively
and summarized by Pratt et al. (1993) and Leckie et al.
(1998).
The Ceonomanian – Turonian transition is exposed along the Rock Canyon Anticline to the north
and northeast of Lake Pueblo State Park, Colorado
(USA), with well-known outcrops in the Rock
Canyon, Pueblo and Liberty Point localities (Fig.
1). The best and most easily accessible outcrops are
exposed along a railroad cut and nearby road cut at
the Pueblo locality (Fig. 2). In this area of the Rock
Canyon Anticline, the Cenomanian – Turonian
boundary Stratotype Section and Point (GSSP) has
been designated (Kennedy and Cobban, 1991, Kennedy et al., 2000, official designation expected in
2003).
We collected and examined the road cut sequence at
Pueblo, which spans 15 m of Cenomanian and 3.5 m of
lower Turonian sediments (Fig. 1). This section was
analyzed as reference point for comparison with sections in Europe and North Africa. Our study focused
on (l) high-resolution age control based on planktic
foraminiferal biostratigraphy, (2) paleoecology of
planktic foraminiferal species based on quantitative
abundance data and carbon and oxygen isotope variations recorded in the monospecific planktic foraminifer Hedbergella planispira (as reported in Keller et al.,
in press), and (3) evaluation of faunal turnovers based
on depth stratification of species and implied changes
in water mass stratification.
2. Methods
A total of 100 samples were collected and
analyzed at 10 cm intervals in the changing lithologies of the Bridge Creek Limestone, and at 20 – 25
cm intervals in the more monotonous shales of the
103
Hartland Shale Member. For foraminiferal analysis
shale, marly limestone and bentonite samples were
processed for small (38 – 63 Am) and larger (>63
Am) size fractions by standard methods (Keller et
al., 1995). Both size fractions were analyzed quantitatively based on representative splits of 150 –250
specimens per sample for biostratigraphic and environmental analyses. Species from each sample
split were picked, identified and mounted on microslides for a permanent record and illustrated by
SEM (Plates 1– 6). The remaining sample residues
were examined for rare species.
Foraminiferal preservation is relatively good in
shale and marl samples, but difficult to free of
adhering carbonate in more chalky lithologies.
All foraminiferal shells show some degree of
recrystallization. In general, shells of small species (hedbergellids, globigerinellids, guembelitrids
and heterohelicids) are less recrystallized than
shells of larger species that may be infilled with
blocky calcite. The identification of species and
classification of genera follows that of Robaszynski and Caron (1979), Caron (1985) and Eicher
(1972).
3. Lithology
The collected Pueblo section from the Rock
Canyon Anticline area forms a road cut at the
northeastern end of Lake Pueblo (Figs. 1 and 2).
At this locality about 18.5 m of gray shales,
bentonites and tan-colored limestones of the Greenhorn Formation are exposed (Cobban, 1985; Elder
and Kirkland, 1985). The Greenhorn Formation is
divided into Hartland Shale and Bridge Creek
Limestone Members. The Hartland Shale Member
at this outcrop consists of 11.2 m of rhythmically
bedded thin calcarenite or nodular calcarenite layers
and 30 to 100 cm thick gray shale layers. Bentonite
layers are common and vary from 1– 2 to 20 cm
thick (Fig. 3).
The Bridge Creek Limestone Member is about
6.5 m thick. A prominent 40 – 50 cm thick bioturbated micritic limestone (Bed 63) marks the base of
the Bridge Creek Limestone and contains an upper
Cenomanian ammonite assemblage of the Metoicoceras geslinianum zone (Kennedy et al., 2000), and
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G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 3. Lithology, biostratigraphy, planktic foraminiferal and ammonite datum events of the Pueblo section in the Rock Canyon Anticline area of Lake Pueblo State Park, Colorado.
Ages for datum events are from age/depth graph of Fig. 4. The sea-level curve is based on lithologic, mineralogical, paleontological and stable isotopic data discussed in Keller et al.,
in press. The larger sample ticks on the lithological column mark samples analyzed for this study; whereas shorter sample ticks mark additional limestone and bentonite (B) samples
for geochemical and mineralogical analyses.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
planktic foraminiferal assemblage indicative of the
uppermost Rotalipora cushmani zone (Leckie, 1985;
this study). Previous studies have identified this
limestone facies as the main sea-level transgression
near the end of the Cenomanian (Hancock and
Kauffman, 1979; Kauffman, 1984; Sageman et al.,
1998). Upsection, the lithology consists of rhythmically bedded 10 – 20 cm thick bioturbated micritic
limestones alternating with 10 – 60 cm thick organicrich dark shales (Figs. 2 and 3). Bentonite layers are
common and of variable thickness ranging from 1–
2 to 20 cm, similar to the underlying Hartland Shale
Member. Prominent sediment layers of the Bridge
Creek Limestone have been labeled as marker beds
and in this study we follow the numbering system
of Cobban and Scott (1972, Fig. 3).
Sea level changes for the Pueblo section have
been inferred from paleontological, mineralogical
and sedimentological investigations as well as stable
isotopes (e.g., Hancock and Kauffman, 1979; Kauffman, 1984; Arthur et al., 1985; Pratt et al., 1993;
Leckie et al., 1998; Keller et al., in press). The
Hartland Shale was deposited in a shallow epicontinental sea in proximity to shoreline, which provided
periodic freshwater influx and clastic debris during
wet and humid climate conditions. A sea level rise
and transgression occurred during the lower part of
the Hartland Shale coincident with a d13C excursion
that marks the mid-Cenomanian event (MCE) (Coccioni and Galeotti, 2003; Keller et al., in press). A
major sea level transgression began near the top of
the Hartland Shale and culminated in the Bridge
Creek Limestone Bed 63 (Fig. 3), coincident with
the d13C excursion that marks a global oceanic
anoxic event (OAE 2) discussed below. Both sea
level transgressions appear to have been eustatic
(Hardenbol et al., 1998). A generally high though
fluctuating sea level accompanied deposition of the
Bridge Creek Limestone.
4. Age and depositional rates
The age of the Pueblo section is well constrained
based on planktic foraminiferal and ammonite biostratigraphies, and details of the OAE 2 d13C excursion that indicate relatively continuous sediment
deposition across the Cenomanian – Turonian (C – T)
105
transition. The stable isotope data is from Keller et al.
(in press) and based on monospecific samples of the
planktic foraminifer H. planispira from the same
sample splits used for this study. Age estimates for
species first and last appearances, d13C excursions,
depositional and environmental events have been
calculated based on ages of various ammonite and
planktic foraminiferal datum events extrapolated from
the paleomagnetic time scale and radiometric dates by
Hardenbol et al. (1998) (Fig. 4, Table 1). Three
40
Ar/39Ar ages determined from bentonite layers by
Obradovich (1993) and Kowallis et al. (1995) are
compatible with these dates. On the basis of the
40
Ar/39Ar data, these workers estimated the CT
boundary level at 93.3 F 0.2 and 93.1 F 0.3 Ma,
respectively, as compared with 93.49 F 0.2 Ma based
on the first appearance of Watinoceras devonense,
which is the preferred marker for the CT boundary,
and 93.29 F 0.2 Ma for the last appearance of Helvetoglobotruncana helvetica, the planktic foraminiferal
marker species (Hardenbol et al., 1998; Kennedy et
al., 2000).
Sedimentation rates calculated based on the age/
depth plot for the Pueblo section indicate no major
sedimentary breaks or discontinuities. From the base of
the Bridge Creek Limestone Bed 63 to Bed 79, sediment accumulation rates average 1.23 cm/ky (1.11 cm/
ky excluding bentonite layers), whereas in the upper
part they average 0.87 cm/ky (0.75 cm/ky excluding
bentonite layers), assuming that limestone and shale
layers were deposited at roughly equal rates (Fig. 4).
Based on cycle analysis, Meyers et al. (2001) concluded that there is a hiatus of about 25,000 years in the
upper part of Bed 78, though no hiatus is apparent in
outcrops or faunal analyses. This short hiatus does not
significantly affect the sediment accumulation rate, nor
change the slope of the age/depth curve.
Estimated sedimentation rates for the Bridge Creek
Limestone by Elder and Kirkland (1985) average
0.5– 1.0 cm/ky, by Scott et al. (1998) 0.9 cm/ky and
by Sageman et al. (1998) 0.57 cm/ky. In comparison,
the comparable interval at Eastbourne averages 2.4
cm/ky. The lower sediment accumulation rate at
Pueblo is probably due to cyclic climate variations
and periods of nondeposition between shale/limestone
couplets (Sageman et al., 1998). Shale deposition
occurred during humid wet periods accompanied by
high sediment and freshwater influx. Limestone de-
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G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 4. Age/depth plot of the Pueblo section in the Rock Canyon Anticline area of Lake Pueblo State Park, Colorado, based on planktic
foraminiferal and ammonite datum events from Hardenbol et al. (1998) and other datum events for which ages have been extrapolated from the
age/depth and sediment accumulation rates. Calculated datum events are coeval at Pueblo and Eastbourne sections within errors of 10 to 20 ky,
except for the last appearance of G. bentonensis for which a 50 ky difference occurs due to the condensed interval in Bed 68 at Pueblo.
40
Ar/39Ar ages for bentonite layers are from Obradovich (1993) and Kowallis et al. (1995).
position occurred during more arid periods accompanied by reduced sedimentary influx and increased
production of biogenic carbonate (foraminiferal tests,
coccoliths, invertebrates; Keller et al., in press). These
dilution/productivity cycles have been interpreted as
obliquity and precession cycles, respectively (Sageman et al., 1998).
Meyers et al. (2001) estimated that overall sedimentation rates for the Hartland Shale average 2.7 cm/
ky. Sedimentation appears to have been significantly
lower, about 0.5 cm/ky, for the top 10 m of the
Hartland shale, which is estimated to span a 2 my
interval between the d13C shifts of the mid-Cenomanian event (MCE) and late Cenomanian OAE 2
(Coccioni and Galeotti, 2003). The lower sediment
accumulation rate, compared with the Bridge Creek
Limestone, may be due to lower biogenic productivity
in a shallower epeiric sea and nondeposition associated with cyclic sea level fluctuations.
The age/depth plot and sediment accumulation
rates at Pueblo provide age estimates for foraminiferal
datum events and oceanographic events marked by
the d13C excursion (Fig. 4). A similar age/depth plot
for the Eastbourne section (Keller et al., 2001) has
been used to cross-calibrate ages for the two-peaked
d13C shifts, the Heterohelix shift, and the last appearance data (LAD) of G. bentonensis, Rotalipora deekei
and Rotalipora greenhornensis. The ages of these
datum events in these two sections are comparable
within error margins of 0.01 to 0.02 my, except for G.
bentonensis where ages differ by 50 ky as a result of a
condensed interval at the top of Bed 68 at Pueblo
(Table 1). This condensed interval is also evident by
the juxtaposition of the first appearance datum (FAD)
Table 1
(a) Relative percent abundance of the middle to late Cenomanian planktic foraminifera in the Hartland Shale Member at Pueblo, Colorado
Biozones
R. cushmani
Subzones
Sample
1
Depth (cm) from section base 0
7
10
85
145 195 215 245 260 300 325 355 395 420 450 495 540 570 595
13
16
19
22
24
25
26
27
28
30
31
x
2
27
18
5
5
18
x
x
1
x
2
27
10
34
4
3
41
11
50
4
8
9
x
x
1
x
1
3
2
1
x
31
35
x
40
67
5
15
4
56
5
x
x
4
2
x
14 11
4
x
x
x
x
x?
195 172 223 172
x
32
33
x
34
35
36
37
625
660
685
x
x
1
33
2
58
2
1
24
x
1
x
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
A. multiloculata
Anaticinella cf. multiloculata
Dicarinella algeriana
D. hagni
D. cf. imbricata
D. imbricata
Globigerinelloides bentonensis
G. ultramicra
Gümbelitria cenomana
G. albertensis
Hedbergella delrioensis
20
H. planispira
66
H. simplex
Heterohelix moremani
5
H. reussi
4
H. sp. A
H. sp. B
Praeglobotruncana aumalensis
P. gibba
P. inornata
P. praehelvetica
P. stephani
Rotalipora cushmani
R. deekei
R. greenhornensis
R. montsalvensis
Whiteinella aprica
W. archaeocretacea
W. baltica
4
W. brittonensis
x
W. paradubia
Total specimens counted
156
4
30
x
6
22
35
6
56
x
3
44
1
8
6
7
76
63
x
2
28
1
3
1
x
6
x
40
1
x
45
x
x
x
x
1
55
2
1
33
10
31
3
3
34
10
x
3
x
2
x
3
x
x
2
1
x
1
x
x
x
x
x
1
x
2
x
x
215
13
x
x
150
5
x
x
229
7
1
x
x
161 166
2
3
x
215
2
2
2
x
x
260 211
1
1
x
265
1
40
3
36
3
50
3
46
4
x
x
x
x
2
x
x
189
x
x
48
x
x
40
1
1
x
x
x
x
1
x
x
x
x
1
x
x
208
3
2
1
273
1
27
x
3
55
4
1
2
x
3
44
4
3
x
x
x?
3
x
1
x
2
1
1
x
x
x
4
x
2
186
4
1
x
213
21
1
x
65
2
2
x
1
7
257
x
x
9
x
x
183
(continued on next page)
107
108
Table 1 (continued)
(b) Relative percent abundance of late Cenomanian planktic foraminifera in the Hartland Shale Member at Pueblo, Colorado
Biozones
R. cushmani
Subzones
P. praehelvetica
Sample
38
39
40
W. archeocretacea
A. multiloculata
41
42
43
44
45
46
47
48
49
Rotalipora extinct. G. bentonensis D. hagni
50
51
52
53
54
57
59
60
61
63
64
65
67
69
A. multiloculata
Anaticinella cf. multiloculata
Dicarinella algeriana
D. hagni
D. cf. imbricata
D. imbricata
Globigerinelloides bentonensis 1
G. ultramicra
Gümbelitria cenomana
G. albertensis
Hedbergella delrioensis
3
H. planispira
49
H. simplex
x
Heterohelix moremani
1
H. reussi
25
H. sp. A
13
H. sp. B
1
Praeglobotruncana aumalensis
P. gibba
2
P. inornata
1
P. praehelvetica
x
P. stephani
x
Rotalipora cushmani
x
R. deekei
R. greenhornensis
x
R. montsalvensis
x
Whiteinella aprica
W. archaeocretacea
W. baltica
1
W. brittonensis
1
W. paradubia
Total specimens counted
159
1
x
x
x
x
x
x
1
2
x
x
3
4
1
x
2
19
27
4
4
21
6
2
2
2
1
7
22
1
5
41
x
3
2
1
x
1
x
x
x
4
x
2
29
1
4
35
3
7
2
8
34
x
1
36
2
9
x
7
13
3
7
33
2
7
x
x
x
28
x
1
50
3
6
3
2
1
40
1
4
48
5
5
x
1
2
51
x
5
37
x
x
x
x
x
1
x
1
x
x
x
1
x
3
3
3
x
x
x
x
x
x
x
x
x
x
x
x
1
x
x
6
2
27
x
2
38
11
1
x
x
2
9
1
10
7
7
46
x
13
6
1
16
1
6
49
7
2
x
4
17
2
5
44
12
x
x
x
4
x
x
1
9
x
5
1
x
x
x
x
x
6
x
5
11 4
4
13 5
4
x
3
4
x
2
1
x
4
x
x
x
1
2
2
x
x
x
x
x
x
257 184 251 181 185 125 182 210 211 229 144
3
3
x
x
224
5
4
19
x
4
30
1
12
x
x
6
x
x
x
2
9
3
1
7
29
2
2
44
1
x
x
x
2
3
5
3
4
23
3
5
20
5
12
2
x
x
6
1
x
x
1
1
x
4
x
188 216
8
2
2
6
5
2
1
x
x
8
7
x
x
7
4
1
2
x
x
2
12
3
15
39
1
1
5
11
41
1
1
10
1
1
x
3
1
1
x
9
2
25
1
6
47
3
15
x
12
36
x
x
x
x
x
x
x
x
x
x
x
x
x
x
1
2
x
2
5
8
12
8
x
44
10
x
x
x
x
x
4
5
8
4
7
36
x
1
24
x
4
11
1
9
22
x
9
34
x
x
x
x
1
1
2
3
x
x
1
5
x
x
x
12
3
2
7
38
x
2
x
5
39
2
22
8
33
2
10
5
4
35
1
3
27
x
x
1
x
x
x
x
1
2
3
2
x
2
x
x
239 188 170
169
10
7
x
x
288
x
3
2
x
x
183
3
2
5
x
6
4
x
1
x
3
x
315 185 226 215
x
6
6
x
x
247
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Depth (cm) from section base 715 740 765 795 825 855 875 885 895 930 975 985 1020 1050 1075 1100 1125 1175 1180 1185 1190 1210 1225 1230 1260 1280
(c) Relative percent abundance of late Cenomanian to early Turonian planktic foraminifera in the Bridge Creek Limestone Member at Pueblo, Colorado
Biozones
W. archeocretacea
H. helvetica
Subzones
D. hagni H. moremani
Sample
70
72
74
76
77
78
79
80
81
82
83
84
85
86
88
89
90
94
96
98
100
Depth (cm) from section base 1295 1320 1335 1355 1375 1400 1425 1445 1475 1500 1530 1555 1580 1600 1645 1665 1680 1735 1775 1800 1825
x
x
x
x
x
x
x
x
x
x
x
x
4
2
5
34
2
9
29
x
x
3
3
7
1
x
208
2
5
2
22
1
5
41
1
2
3
1
1
3
2
x
6
3
2
x
5
2
x
x
x
2
1
1
x
5
3
5
2
x
196
3
4
5
1
x
196
5
4
5
4
1
201
4
10
4
4
2
195
9
4
9
3
67
5
65
4
53
1
45
3
42
1
55
x
3
60
x
3
60
x
1
51
2
x
61
5
2
64
8
61
4
x
1
x
x
x
x
x
x
x
x
x
x
x
x
x
x
2
x
x
1
4
4
x
183
3
3
10
13
3
78
poor
x
1
3
x
x
181
1
4
2
1
1
3
1
2
3
1
179
x
1
2
2
1
259
x
2
x
1
x
x
x
x
310 249
2
46
7
3
x
6
x
4
3
x
1
56
10
3
x
x
x
2
3
x
2
11 1
x
x
266 99
1
14
x
1
48
x
4
x
x
22
1
x
1
3
48
8
x
1
x
1
19
x
1
3
15
2
35
x
x
x
1
8
2
39
x
x
x
4
2
35
1
x
6
6
2
34
x
1
x
10
3
26
x
x
2
x
3
23
x
x
1
4
6
x
x
x
5
x
x
209 183
4
x
x
1
x
1
x
3
x
x
2
8
x
x
10
8
3
173
1
x
6
2
x
165 203
63
1
1
x
1
x
6
2
x
5
71
5
1
x
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
A. multiloculata
Anaticinella cf. multiloculata
Dicarinella algeriana
D. hagni
D. cf. imbricata
1
D. imbricata
Globigerinelloides bentonensis
G. ultramicra
Gümbelitria cenomana
1
G. albertensis
Hedbergella delrioensis
3
H. planispira
3
H. simplex
Heterohelix moremani
5
H. reussi
8
H. sp. A
x
H. sp. B
Helvetoglobtruncana helvetica
Praeglobotruncana aumalensis
P. gibba
2
P. inornata
P. praehelvetica
P. stephani
x
Rotalipora cushmani
R. deekei
R. greenhornensis
R. montsalvensis
Whiteinella aprica
5
W. archaeocretacea
1
W. baltica
54
W. brittonensis
13
W. paradubia
x
Total specimens counted
110
Preservation
poor
6
3
2
3
x
197
109
110
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Table 2
Ages for planktic foraminiferal and ammonite first (FAD) and last
(LAD) appearance data, and d13C shifts at the Pueblo GSSP
93.29 F 0.2 Ma
Helvetoglobotruncan
helvetica FAD
Watinoceras devonense FAD
93.49 F 0.2 Ma
Neocardioceras juddii LAD
93.49 F 0.2 Ma
Neocardioceras juddii LAD
93.59 Ma
Calycoceras geslineanum
LAD
Neocardioceras juddii FAD
93.73 F 0.2 Ma
Heterohelix shift
OAE 2 d13C peak (2)
excursion max.
Globigerinelloides
bentonensis LAD
Dicarinella hagni FAD
Rotalipora cushmani LAD
93.78 F 0.02 Ma*
93.86 F 0.05 Ma*
Hardenbol
et al. (1998)
Hardenbol
et al. (1998)
Hardenbol
et al. (1998)
this study at
Pueblo
Hardenbol
et al. (1998)
Hardenbol
et al. (1998)
this study
this study
93.86 F 0.05 Ma*
this study
93.86 F 0.05 Ma*
93.90 F 0.02 Ma*
93.91 F 0.02 Ma*
94.00 F 0.02 Ma*
93.95 F 0.02 Ma*
this study
Hardenbol
et al. (1998)
this study
this study
this study
93.95 Ma
94.50 Ma
this study
this study
94.88 Ma
this study
95.71 Ma
this study
95.85 Ma
this study
OAE 2 d13C peak 1
OAE 2 d13C excursion onset
Rotalipora greenhornensis
LAD
Rotalipora deekei LAD
Whiteinella archeocretacea
FAD
Praeglobotruncana
praehelvetica FAD
Mid-Cenomanian d13C
shift (MCE)
Whiteinella paradubia FAD
93.73 F 0.2 Ma
Asterisks mark datum events at Pueblo that have been crosscorrelated with Eastbourne, England. Error margins reflect uncertainty between these two sections.
of Dicarinella hagni and peak 2 of the d13C excursion. The ages for datum events calculated by Hardenbol et al. (1998) also indicate good agreement with
Eastbourne, except for H. helvetica which appears
earlier at Eastbourne possibly because this species is
diachronous and/or the evolutionary transition from
praehelvetica to helvetica is difficult to determine
(Table 2).
5. Biostratigraphy
The Cenomanian –Turonian transition in the Western Interior is stratigraphically defined by ammonite
and inoceramid zones, which provide reliable regional
correlations and have been discussed in various publications (e.g., Cobban and Scott, 1972; Cobban, 1985;
Elder, 1985; Kennedy and Cobban, 1991). Biostratigraphic correlation based on planktic foraminifera has
received little attention due to the scarcity or low
diversity of microfossils in these mostly very shallow
Western Interior marine sequences. Early studies by
Eicher (1969a,b, 1972) formed the critical groundwork
for foraminiferal biostratigraphy and paleoecology,
whereas Leckie (1985, 1989) and Leckie et al.
(1998) significantly advanced the paleoclimatic and
paleoceanographic applications. This study documents
the planktic foraminiferal species ranges and applies
the standard planktic foraminiferal biozones (Robaszynski and Caron, 1979) to achieve global integration
of the Pueblo GSSP, and incorporates Keller et al.’s
(2001) three-part subdivision of the Whiteinella archeocretacea zone to achieve a higher age resolution.
Additional biomarkers are considered for subdivision
of the R. cushmani zone, which after testing in other
geographic regions may provide further biostratigraphic refinement and age control. The proposed planktic
foraminiferal biostratigraphic scheme at Pueblo is
shown in Fig. 5 along with the d13C excursion and
ammonite zones. Species ranges and assemblages as
well as the d13C excursion at Pueblo are very similar to
those at Eastbourne and can be easily correlated (Paul
et al., 1999; Keller et al., 2001).
5.1. H. helvetica zone
The first appearance (FA) of H. helvetica defines
the base of this zone and is considered the planktic
foraminiferal biomarker for the Cenomanian– Turonian (C/T) boundary. However, this species is a
problematic biomarker and needs to be reevaluated.
The problems are primarily due to the rarity of this
species, potential diachronous occurrence, and identification and separation of the H. helvetica morphotype
from its evolutionary ancestor P. praehelvetica (Hart
and Bigg, 1981; Hilbrecht et al., 1986; Jarvis et al.,
1988; Keller et al., 2001). At Pueblo, this species first
appears in the shale above limestone Bed 90 about 75
cm above the FA of the ammonite W. devonense (Bed
86), which marks the C/T boundary, though transitional forms of praehelvetica – helvetica are present in
Beds 85, 86 and 89. At Eastbourne the first appearance
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 5. High-resolution correlation scheme for the Cenomanian – Turonian transition based on planktic foraminifera and the carbon isotope curve of the planktic foraminifer H.
planispira at the Pueblo GSSP. See Fig. 4 for ages of datum events.
111
112
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
of H. helvetica was observed 20 cm above the FA of W.
devonense (Keller et al., 2001). The discrepancies in
the observed first appearance of H. helvetica is largely
due to the difficulty in finding a uniform criterion for
determining the point at which the transition from P.
praehelvetica to H. helvetica can be considered to have
been completed. Such problems are commonly encountered for biomarkers based on evolutionary transitions in adaptation to changing environments and
therefore can result in diachronous datum events.
5.2. Heterohelix moremani subzone
(93.29 – 93.78 Ma)
This subzone defines the interval from the first
appearance of Heterohelix dominated assemblages
(Heterohelix shift) after the initial OAE 2 d13C excursion to the FA of H. helvetica. This Heterohelix shift
has previously been used as correlation tool in the US
WIS by Leckie et al. (1998), but it also marks an
interval of global heterohelicid dominance (H. moremani and H. reussi) in the W. archeocretacea zone
after the d13C excursion reached its peak (Figs. 5 and
6, Nederbragt and Fiorentino, 1999; Keller et al.,
2001). The Heterohelix shift is a reliable global
biomarker that reflects the expansion of the oxygen
minimum zone after the major sea level transgression
and d13C excursion. At Pueblo, the onset of the
Heterohelix shift occurs 50 cm below Bed 79, near
the base of the ammonite Neocardioceras zone.
5.3. Dicarinella hagni subzone (93.78 –93.86 Ma)
This subzone defines the interval from the last
appearance (LA) of Globigerinelloides bentonensis
to the Heterohelix shift (Fig. 5). In addition, D. hagni
first appears just prior to the extinction of G. bentonensis. At Pueblo, this subzone forms the upper part
of the benthic oxic zone and spans from Bed 68 to
Bed 78. Note that the D. hagni subzone replaces the
A. multiloculata subzone of Keller et al. (2001),
because examination of the Pueblo section revealed
that the acme of development of A. multiloculata is in
the upper R. cushmani zone.
5.4. Globigerinelloides bentonensis subzone
(93.86 –93.90 Ma)
This subzone defines the interval from the extinction of R. cushmani to the extinction of G. bentonen-
Fig. 6. Relative abundances of Heterohelix at Eastbourne, England, Pueblo, Lohali Point and Rock Canyon in Lake Pueblo State Park, and
Kalaat Senan, Tunisia. At each locality, there is a shift to Heterohelix-dominated assemblages which follows the d13C shift and benthic oxic
zone. The Heterohelix is an excellent biomarker for global correlations.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
sis. The interval spans Beds 66 to 68 and corresponds
to the trough between the first and second d13C peaks
at Pueblo and Eastbourne (see also Keller et al.,
2001).
5.5. Rotalipora extinction subzone (93.90 – 93.94 Ma)
This subzone spans the interval of extinction of the
genus Rotalipora and is marked by the extinctions of
R. greenhornensis and R. deekei at the base and R.
cushmani at the top (Fig. 5). In addition, this subzone
corresponds to the interval of d13C excursion and sea
level transgression at both Pueblo and Eastbourne and
is correlative with the M. geslinianum zone.
5.6. Anaticinella multiloculata subzone
(93.94 –94.50? Ma)
This subzone marks the interval from the FA of W.
archeocretacea to the LA of R. greenhornensis. The
nominate taxon is most abundant at the top of this
zone and near the onset of the d13C excursion (Fig.
5). In this interval, A. multiloculata peaks in morphologic diversity showing gradations from its ancestor R. greenhornensis to A. multiloculata by
losing its keel and inflating chambers, probably in
adaptation to a shallower subsurface habitat in the
lower photic zone (see Appendix, Eicher, 1972). The
last occurrence of R. greenhornensis was observed at
the same stratigraphic interval at Eastbourne (Keller
et al., 2001).
5.7. Praeglobotruncana praehelvetica subzone
(94.50 –94.88? Ma)
This subzone spans the interval from the FA of P.
praehelvetica to the FA of W. archeocretacea (Fig. 5).
6. Planktic foraminiferal turnovers
During the late Cenomanian to early Turonian at
Pueblo planktic foraminifera experienced a major
faunal turnover associated with the OAE 2 positive
d13C excursion and major sea level transgression (e.g.,
Eicher, 1969a; Leckie, 1985; Leckie et al., 1998; West
et al., 1998). A smaller faunal turnover occurred
earlier in the R. cushmani zone and is also associated
113
with a positive d13C excursion and sea level transgression termed the mid-Cenomanian event (MCE)
(Coccioni and Galeotti, 2003). The nature of these
faunal turnovers can be evaluated based on species
richness and relative species abundances.
At the base of the Pueblo section prior to the MCE
d13C excursion, only seven species are consistently
present and four show sporadic occurrences. During
and immediately after the d13C shift, six species
appeared, including Praeglobotruncana aumalensis,
Whiteinella paradubia, Heterohelix sp. A (a large
morphotype with inflated chambers), R. cushmani,
R. greenhornensis and R. montsalvensis (Fig. 7).
The absence of the latter three deeper dwelling Rotalipora species prior to the MCE may be ecological
and related to the shallow environment at Pueblo. In
the 4 m above this interval, species richness gradually
increased to a maximum of 20 species between 7 and
8 m with the appearance of P. inornata, P. praehelvetica, A. multiloculata and Guembelitria, but decreased
again below the OAE 2 d13C shift (Fig. 7).
With the onset of the major OAE 2 d13C shift and
marine transgression that spans the top of the Hartland
Shale and base of the Bridge Creek Limestone, four
Rotalipora species disappeared (R. montsalvensis, R.
deekei, R. greenhornensis, R. cushmani) followed by
G. bentonensis and Praeglobotruncana inornata
resulting in a loss of about 30% (Fig. 7). In the same
interval and immediately following the Rotalipora
extinction six species appeared (Dicarinella algeriana,
D. imbricata, D. hagni, W. archaeocretacea, W. aprica
and G. albertensis, Fig. 7). This faunal turnover thus
results in no net loss in species diversity. Relative
species abundances indicate that both outgoing and
incoming species were rare and endangered species
and thus a minor components of the total planktic
foraminiferal population with < 2% and < 4%, respectively. No significant change in species diversity is
observed above the OAE 2 d13C shift. However, a
sharp drop in species richness is observed in the lower
part of the H. moremani subzone, Bed 78 of the Bridge
Creek Limestone, coincident with maximum Heterohelix abundance. This event was also observed at the
same stratigraphic interval at Eastbourne (Keller et al.,
2001) and appears to be associated with a global
expansion of the oxygen minimum zone.
Relative species abundances, dominant species
groups, size and morphology yield further clues to
114
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 7. Species ranges of planktic foraminifera, species richness and the d13C curve at Pueblo, Colorado. Note that species extinctions and
originations are about equal and there is no net loss in diversity during the OAE 2 d13C shift. A sharp drop in species richness to seven species in
the lower part of the H. moremani subzone is also observed at this stratigraphic interval at Eastbourne (Keller et al., 2001) and is associated with
maximum Heterohelix abundance and intensified oxygen minimum zone. A smaller d13C shift and faunal turnover occurred during the middle
Cenomanian.
the nature and degree of stress conditions during these
faunal turnovers. For example, species in high stress
environments documented from the early Danian globally and restricted environments of the late Maastrichtian tend to be morphologically smaller by up to 50% or
more as a result of early sexual maturation and high
reproductive rates (Keller, 1993, 2002; MacLeod et al.,
2000; Abramovich et al., 2003). For this reason, the
small size fraction (38 – 63 Am) was investigated at
Pueblo to assess the presence of small species (e.g.,
Guembelitria, Globigerinella, Hedbergella, Heterohelix) and quantify relative abundances. The results
reveal a constant dominance of biserial species
(f 80%) and a smaller component of hedbergellids
(Fig. 8). Guembelitrids appear only at the time of
maximum d13C values after the OAE 2 d13C shift and
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
115
Fig. 8. Relative abundances of planktic foraminiferal species in the small size fraction (38 – 63 Am) at Pueblo. Note that low oxygen tolerant
Heterohelix species (H. reussi, H. moremani) dominate ( f 80%) through most of the middle to late Cenomanian and early Turonian at Pueblo,
suggesting that a well-developed OMZ was present most of the time. The opportunistic Guembelitria species appeared after at the onset of the
benthic oxic zone, probably in response to upwelling and nutrient-rich surface waters.
coincident with a marked temporary decrease in heterohelicids (Fig. 8). This indicates that high stress conditions prevailed at Pueblo throughout the middle and
late Cenomanian, but that the maximum OAE 2 d13C
excursion and sea level transgression provided the
ecologic conditions for the opportunist Guembelitria.
116
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Relative species abundances in the >63 Am size
fraction provide a more comprehensive assessment of
the diversity and variations in foraminiferal habitats.
This data set reveals faunal assemblages dominated by
the same two species groups, Heterohelix and H.
planispira, as in the smaller size fraction (Fig. 9).
All other species are sporadically common (10 – 20%)
or rare to few. This pattern reveals high stress conditions for the entire water column and suggests
reduced water mass stratification, and variations in
salinity, oxygen, temperature and nutrients. Examination of species habitats can provide information as to
the nature and probable cause of the high stress
environment in the Western Interior Sea during the
middle Cenomanian to early Turonian.
7. Planktic foraminiferal paleoecology
The evolution, diversification and extinction of
planktic foraminifera are generally associated with
stratification of the water column, variations in the
trophic structure, vertical temperature and density
gradients and the associated niche differentiation
Fig. 9. Relative abundances of planktic foraminiferal species in the >63 Am size fraction and the d13C curve of H. planispira at Pueblo,
Colorado. Note that the assemblages are dominated by low oxygen tolerant Heterohelix and low salinity tolerant H. planispira reflecting a welldeveloped OMZ and low surface salinity due to freshwater influx. There are two d13C shifts, the OAE 2 and mid-Cenomanian event (MCE) and
each is associated with a sea level transgression (see Fig. 3) and increased water mass stratification as indicated by reduced Heterohelix
populations. Note that extinctions and originations of the OAE 2 faunal turnover affected only rare and endangered species whose combined
relative abundances account for less than 2% and 4% of the total foraminiferal population, respectively.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
(Lipps, 1979; Leckie et al., 1998; Price and Hart,
2002; Keller, 2002). Fundamentally important in
maintaining diverse planktic foraminiferal communities is stratification of the upper water column, which
is affected by seasonal changes in thermocline, nutrient cycling, and productivity. Species diversity is proportional to the water mass stratification, with highest
diversity in a stable stratified water column with
normal salinity and nutrients, and year-round temperature gradients that provide a variety of ecological
niches and a stable nutrient supply.
Water mass stratification and the type of ecological niches occupied by different species can be
inferred from the diversity and relative species
abundances, morphologies of species, biogeographic
distribution, and carbon and oxygen isotope ranking.
Although stable isotopic ranking of species is the
best single method to elucidate species depth habitats
and has been successfully applied to Cretaceous
species (e.g., Corfield et al., 1990; Norris and
Wilson, 1998; Price and Hart, 2002; Abramovich et
al., 2003), best results depend on excellent preservation, which is often difficult to find, and strong
d18O and d13C gradients. Therefore, a combined
approach integrating available isotopic, biogeographic and quantitative faunal data provides the most
reliable results.
7.1. Deepwater dwellers—keeled species
Stable isotope ranking of large, complex, keeled
and flattened morphotypes indicate that globotruncanids and rotaliporids generally occupied deeper oligotrophic habitats at or below thermocline depth
during the late Cretaceous (e.g., Corfield et al.,
1990; Price and Hart, 2002; Norris and Wilson,
1998; Abramovich et al., 2003). Faunal analysis
indicates that these species are generally present in
low abundances in high diversity species assemblages, suggesting adaptation in a stable and wellstratified water mass (Caron and Homewood, 1983;
Leckie, 1987; Keller et al., 2001). In the Hartland
Shale at Pueblo, keeled species are absent prior to the
MCE d13C shift probably due to the shallow water
environment. Above the MCE d13C shift keeled
species are very rare ( < 1%) and include R. greenhornensis, R. montsalvensis, R. deekei and R. cushmani (Fig. 9, Plate 1). The rarity of rotaliporids can be
117
explained by the shallow water depth, low thermal
gradients, reduced water mass stratification and welldeveloped oxygen minimum zone (OMZ) in the
Western Interior Sea. All rotaliporids disappeared
during the first phase of the OAE 2 d13C shift. Leckie
(1985) suggested this might have been due to an
expanding OMZ. However, the relative abundance
of low oxygen tolerant heterohelicids remained relatively constant through the upper Hartland Shale and
the extinction of the last rotaliporids actually coincided with a dramatic drop in heterohelicids indicating a
strongly reduced OMZ, more oxygenated water column and increased water stratification (Fig. 9). This is
also indicated by the presence of diverse benthic
assemblages, including Cibicidoides, which mark the
only interval with oxic bottom waters in the Pueblo
section (benthic zone of Eicher, 1969b). The Rotalipora extinction is therefore more likely due to increased competition from evolving dicarinellids and
praeglobotruncanids that accompanied increased water mass stratification.
7.2. Lower photic zone dwellers—weakly keeled
species
This group is characterized by inflated chambers
and weak or poorly developed keels and includes A.
multiloculata, all praeglobotruncanids (e.g., P. praehelvetica, P. helvetica, P. inornata, P. aumalensis, P.
stephani), and some dicarinellids (D. algeriana, D.
hagni, Fig. 9; Plates 1 –3). These species may have
descended from keeled morphotypes by inflating
chambers and losing keels in response to adaptation
to shallower and less oxygenated habitats (Eicher,
1972; Leckie, 1985). This interpretation gains support
from isotopic analysis that indicates generally lighter
d18O values for P. stephani than for Rotalipora
species (Price and Hart, 2002), though the isotopic
ranking of most other species has not yet been
adequately documented.
Most of these adaptations were ultimately unsuccessful, as is evident with P. inornata and A. multiloculata that are reported extinct at the same time as
R. cushmani (Eicher, 1972; Leckie, 1985), though
we observed a recurrence of A. multiloculata in the
upper W. archeocretacea zone at Pueblo and Eastbourne (H. moremani subzone, Fig. 9; Keller et al.,
2001). Praeglobotruncanids fared little better, with
118
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
most species rare and sporadically present through
the studied interval. We interpret these species as
having occupied habitats in the lower photic zone
but above the OMZ. In this ecologic niche, they
would have thrived only at times when water mass
stratification increased and the OMZ decreased. Such
conditions prevailed only intermittently in the WIS
and most notably immediately after the first phase of
the OAE 2 d13C excursion with the appearance of
oxygenated bottom water (oxic benthic zone), which
favored the evolutionary diversification of dicarinellids (Fig. 9). Weakly keeled species fared little better
in the more open sea environment at Eastbourne
(Keller et al., 2001).
7.3. Oxygen minimum zone dwellers—heterohelicids
During the late Cretaceous heterohelicids thrived
in low oxygen marine environments with well-developed oxygen minimum zones (OMZ) (Hart and Ball,
1986; Resig, 1993; Keller, 1993, 2002; Leckie et al.,
1998). At Pueblo, this biserial group is dominated by
H. moremani and H. reussi, with more restricted
occurrences of H. sp. A, a large morphotype with
globular chambers (Fig. 9, Plate 6). Heterohelix
reussi and H. moremani dominated the faunal assemblages, averaging 40 –50% in the Hartland Shale
and 60– 70% in the Bridge Creek Limestone, except
for a short interval in the lower W. archeocretacea
zone (subzones G. bentonensis and D. hagni). In the
small size fraction (38 –63 um), Heterohelix species
average 80% throughout the section, except for two
brief intervals at the base of the W. archeocretacea
zone (G. bentonensis subzone) and at the base of the
H. moremani subzone (Fig. 8). This suggests that the
OMZ was well developed during deposition of the
Hartland Shale and Lower Bridge Creek Limestone,
except for the interval of the benthic oxic event (Figs.
9 and 10).
Heterohelix abundances largely covary with d18O
values. In general, high negative d18O values correspond to significantly reduced Heterohelix abundances in 86% of the time (19 out of 22 intervals),
whereas high positive d18O values correspond to
increased abundances 60% of the time (12 out of 20
intervals, Fig. 10). The lower correlation for positive
d18O values occurs largely within the benthic oxic
zone of OAE 2 and MCE. In addition, fewer isotope
data points in some intervals prevent point-by-point
evaluation. Since highly negative d18O values reflect
subsaline surface waters (Pratt, 1985; Pagani and
Arthur, 1998; Keller et al., in press), this suggests
that heterohelicids thrived at times of more normal
marine salinity, but decreased during times of subsaline surface waters. However, at times of a more
oxygenated water column and increased stratification,
Heterohelix populations also decreased apparently due
to a reduced OMZ.
This is apparent during OAE 2 where a major
decrease in the Heterohelix population to < 10%
occurred following the sea level transgression and
first peak in d13C shift (Fig. 11). The decrease in
Heterohelix parallels a nearly 3xnegative shift in
d18O values and 1xshift in d13C values of the
surface dweller H. planispira (Keller et al., in press).
This interval also coincides with the first appearances
of four planktic species (Figs. 7 and 9) and diverse
benthic assemblages including Cibicidoides that mark
the lower part of the ‘‘benthic zone’’ of Eicher
(1969b) and Eicher and Worstell (1970). A likely
interpretation is a well-oxygenated and stratified water
column with a reduced OMZ probably due to upwelling of oxygen-rich deeper waters. The negative d18O
values suggest increased freshwater runoff (Fig. 11).
Species richness is generally high in the d13C shift
interval and oxic zone (Fig. 7). Above this short oxic
zone, a shift to Heterohelix dominance signals the
return to an expanded OMZ, which is associated with
a dramatic 2/3 drop in species richness. The same
reduction in species richness at this time interval was
observed at Eastbourne and suggests that this is a
globally intensified OMZ event. A negative excursion
in d18O values about 50 cm below the C – T boundary
suggests a lower sea level and increased freshwater
influx (Fig. 11).
7.4. Subsaline surface dweller—Hedbergella
planispira
Stable isotope ranking indicates that all Hedbergella species lived in surface or near-surface waters
(Price and Hart, 2002), as also indicated by paleogeographic distribution and abundance patterns in open
ocean and shallow epeiric sea environments (Hart and
Bailey, 1979; Leckie, 1985; Hart, 1999). In the
Western Interior Seaway, H. planispira alternately
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
119
Fig. 10. Relative abundance of Heterohelix compared with the d18O curve of H. planispira at the Pueblo section. There is an 86% correlation
between high negative d18O values and significantly reduced Heterohelix abundances, and a 60% correlation between high positive d18O values
increased Heterohelix. The lower correlation occurs largely within the benthic oxic zone of OAE 2 and MCE. These data indicate that
heterohelicids thrived at times of more normal marine salinity and low oxygen, but decreased at times of sea level transgressions and the arrival
of oxic deeper waters.
dominates with low oxygen tolerant biserial species
(Eicher, 1969b; Eicher and Worstell, 1970; Leckie,
1987). Assuming that H. planispira calcified its shell
in equilibrium with seawater, similar to other planktic
foraminiferal species (Corfield et al., 1990; Norris and
Wilson, 1998; Price and Hart, 2002), the cyclic
variations in d18O values of this surface dweller
record alternating periods of more normal marine
salinity with freshwater influx in the WIS (Fig. 12).
Hence, 2 –4xnegative d18O excursions reflect freshwater influx at times of humid and wet periods with
high runoff, as supported by correlative peaks in
detrital input, whereas positive d18O excursions reflect
dry periods with low runoff, or marine incursions at
times of rising sea levels (Pratt et al., 1993; Pagani
and Arthur, 1998; Keller et al., in press).
120
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 11. Heterohelix abundance, d18O and d13C across OAE 2 at Pueblo. The d13C shift is accompanied by a sea level transgression, which is
followed by an influx of oxygen-rich deep water forming a benthic oxic zone, upwelling, increased water mass stratification and strongly
reduced OMZ. Most extinctions and radiations take place in the benthic oxic zone.
Population abundances of H. planispira covary
with the d18O signal of their shells. Relatively high
population abundances of H. planispira correlate
with 2 – 4xnegative d18O excursions 91% of the
time (20 out of 22 data points, Fig. 12) and suggest
a high tolerance for subsaline surface waters. A
similarly high correlation is observed between relatively low H. planispira abundances and positive
d18O excursions, which indicate a low tolerance for
more normal marine surface water salinity. H. planispira is thus an excellent proxy for surface salinity. However, this relationship does not hold at times
when relative abundances of H. planispira drop
below 15% and signal more normal surface salinity,
as is the case in the A. multiloculata subzone and
early Turonian (upper H. moremani to H. helvetica
zones). There is also a notable exception in sample
79 where stable isotope values of a high H. planispira population (35%) indicate a positive d18O
excursion (Fig. 12). The reason for this discrepancy
is not clear.
7.5. Surface dwellers—normal marine salinity
7.5.1. Hedbergellids
As noted above, paleobiogeographic distribution
patterns (Hart and Bailey, 1979; Leckie, 1985; Hart,
1999) and stable isotope ranking of Hedbergella
species indicate that this group inhabited surface or
near-surface waters during the middle to late Cenomanian (Corfield et al., 1990; Price and Hart, 2002).
At Pueblo, the low relative abundances of Hedbergella simplex and H. delrioensis, as compared with H.
planispira, indicates different habitats. Hedbergella
delrioensis reached a maximum of 31% near the base
of the section, but only intermittent peaks of 10%
thereafter, whereas H. simplex is generally rare, but
both species covary suggesting similar habitats (Fig.
12). Their peak abundances coincide with heavier
d18O values, indicating a preference for normal marine salinity. These species are more abundant at
Eastbourne where more normal marine conditions
prevailed (Keller et al., 2001).
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
121
Fig. 12. Relative abundance of H. planispira compared with the d18O curve of this species at the Pueblo section. There is excellent (91%)
correlation between relatively high H. planispira abundance and negative d18O excursions, which indicates that this species has a high tolerance
for subsaline surface waters and can be used as proxy for low surface salinity. However, this relationship does not hold at times when relative
abundances of H. planispira drop below 15% and signal more normal surface salinity. Other Hedbergella species show no tolerance for
subsaline waters.
7.5.2. Globigerinellids
Globigerinelloides bentonensis and Globigerinelloides ultramicra thrived in surface waters in marginal
or open marine environments. At Pueblo, G. bentonensis is rare in the lower part of the Hartland Shale
examined, but increased to about 5% in the upper part
of this unit and disappeared coincident with the OAE
2 d13C shift in the lower part of the Bridge Creek
Limestone, as also observed at Eastbourne (Fig. 9,
Plates 5 and 6, Keller et al., 2001). Globigerinelloides
ultramicra is also rare and sporadically present, reaching a maximum of 3% in the interval of the d13C
excursion. In contrast, this species is relatively common at Eastbourne where it reached peak abundance
of 20%, suggesting a preference for normal salinity
(Keller et al., 2001).
122
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
7.5.3. Whiteinellids
The globular, large Whiteinella species are morphologically similar to the rugoglobigerinids of the
Maastrichtian and may have occupied similar habitats
in the lower part of the surface mixed layer, as
suggested by stable isotope depth ranking (Norris
and Wilson, 1998). At Pueblo, Whiteinella species
are always present in low abundances (5 –15%, Fig. 9;
Plates 3– 5), but Whiteinella abundance peaks coincide with decreased abundances of the low salinity
tolerant H. planispira, suggesting a preference for
normal marine salinity.
7.6. Opportunists—eutrophic surface: Guembelitria
Late Cretaceous Guembelitria species thrived in
eutrophic surface waters of shallow marginal marine
environments with variable salinities at times of
severe ecological stress when few other species
survived (e.g., Keller, 2002; Keller et al., 2002).
Although Hedbergella and Globigerinella species
also thrived in surface waters, there is no evidence
that they occupied the same ecological niche with
Guembelitria (Hart and Ball, 1986; Leckie et al.,
1991; Keller et al., 2002). At Pueblo, Guembelitria
cenomana and G. albertensis are absent in the
shallow subsaline surface waters of the Hartland
Shale in both the small (38 – 63 um) and larger
(>63 Am) size fractions, but they appeared in relatively low abundance during the sea level transgression and benthic oxic interval of OAE 2 (Figs. 8 and
9). The low abundance of heterohelicids in this
interval and high d13C values suggest upwelling of
oxic nutrient-rich waters, though surface waters appear to have remained subsaline, as suggested by a
negative shift in d18O values and abundant H.
planispira. This implies that late Cenomanian Guembelitria species have a preference for eutrophic
surface waters and tolerate salinity variations, similar
to late Maastrichtian and early Danian morphotypes.
Cenomanian should in principle have fostered relatively high species diversity, but three factors
worked against it: (a) relatively shallow water depth
that reduced the ecologic niches available for deeper
dwelling species, (b) variable salinity due to periodic
freshwater influx, and (c) low oxygen condition
associated with a well-developed oxygen minimum
zone (OMZ). These factors significantly influenced,
and for the most part reduced, ecologic niche
availability for plankton communities in the WIS
and the resultant assemblages reflect a complex
interaction between salinity, oxygen, nutrients and
depth. This can be seen in the abundance changes of
the two dominant species, the low oxygen tolerant
Heterohelix, which reflects changes in the oxygen
minimum zone (Fig. 11), and the low salinity
tolerant H. planispira (Fig. 12), which reflects
freshwater influx.
Temperature also played a key role in limiting
species habitats, but is not considered in this study
because temperature estimates based on salinity influenced d18O data are not reliable. However, some
inferences can be made based on cephalopod Sr and
O isotope data by Cochran et al. (2003) who estimated
a 10 jC increase in temperature (from f 13 to 23 jC)
associated with a change from marine to brackish
water in the WIS during the late Maastrichtian. If this
estimate is correct and can be used as yardstick for
similar conditions during the late Cenomanian, such
major temperature changes at the frequencies indicated by d18O data would have severely limited plankton
habitats throughout the studied interval. Perhaps this
was the case at Pueblo where faunal assemblages are
dominated by just two stress tolerant species (low
oxygen and low salinity). Superimposed on these
overall high stress conditions of the WIS are the
two major oceanographic events MCE and OAE 2,
which forced many ecologically specialized species to
adapt or die out.
8.2. Mid-Cenomanian d13C event (95.71 – 95.80 Ma)
8. Discussion
8.1. Faunal turnovers
The warm low latitude location of Pueblo in the
Western Interior Sea during the middle and late
The mid-Cenomanian event (MCE) at Pueblo is
characterized by a 1xpositive d13C shift in the
planktic foraminifer H. planispira in the lower R.
cushmani zone. Near the onset of the d13C shift is a
nearly 3xnegative shift in d18O values that reflects
freshwater influx. The subsequent d13C shift is ac-
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
companied by a positive 3.5xd18O shift that likely
reflects a marine incursion and sea level transgression
(Fig. 13, Keller et al., in press). Based on sediment
accumulation rates, the d13C shift occurred over
about 90 ky (95.71 – 95.80 Ma). A likely cause for
this d13C shift is increased terrestrial input as suggested by high detrital and terrestrial organic matter
(Keller et al., in preparation). The same oceanographic event has been identified from sections in Italy and
southeastern England (Jenkyns et al., 1994; Coccioni
and Galeotti, 2002). The MCE at Pueblo is associated with a significant faunal turnover, though not of
the same magnitude as OAE 2 (Fig. 13). During the
freshwater influx H. planispira dominates and
reflects subsaline surface waters, whereas during the
transgression Heterohelix dominates and indicates an
expanded OMZ. Four species appeared before and
two species after the peak Heterohelix abundance and
transgression and inhabited surface (Whiteinella),
subsurface (Praeglobotruncan, Heterohelix sp. A),
and deeper waters (Rotalipora). There are no extinctions. This diversification reflects a deeper marine
environment and increased water mass stratification
123
as a result of the sea level transgression. The appearance of Rotalipora, and possibly also the other
species at Pueblo at this time, is likely due to
transport from the western Tethys during the marine
incursion, rather than evolutionary diversification.
The three Rotalipora species (R. cushmani, R. greenhornensis, R. montsalvensis) are known to have
evolved prior to the MCE (Coccioni and Galeotti,
2003).
8.3. Late Cenomanian OAE 2 d13C shift
The major features of the late Cenomanian global
oceanic anoxia event (OAE 2) at Pueblo are a nearly
3xpositive d13C shift in the uppermost R. cushmani zone accompanied by a positive 5.5xd18O
excursion that reflects a major sea level transgression
(Fig. 14). The likely cause for this d13C shift is
increased productivity and enhanced preservation, as
suggested by high organic matter of marine origin
(Pratt et al., 1993; Keller et al., in press). Based on
sediment accumulation rates the d13C shift occurred
over about 90 ky (93.91 – 94.00 Ma) and has been
Fig. 13. The mid-Cenomanian d13C shift event (MCE) and faunal turnover at Pueblo, Colorado. A freshwater influx in the lower part of the d13C
shift is followed by a marine transgression. No species extinctions occurred. The increased species diversity is partly due to originations in
subsurface and surface waters and partly due to immigration of deeper dwelling Rotalipora species during the sea level transgression.
124
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
Fig. 14. The OAE 2 d13C shift and faunal turnover at Pueblo, Colorado. Species extinctions primarily occurred in subsurface and deeper waters, whereas originations occurred
primarily in surface and subsurface waters. About 30% of the species disappeared and 30% originated, but their combined relative abundances are less than 2% and 4% of the total
population, respectively. There is no net loss in diversity. The major faunal turnover occurs in the benthic oxic zone, whereas the lowest species diversity coincides with the return of
dominant Heterohelix populations (Heterohelix shift) signaling an expanded OMZ.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
recognized in late Cenomanian sequences globally. A
major faunal crisis is associated with this environmental change at Pueblo. During the first phase of
the d13C excursion (initiation to first peak, Fig. 14)
two deeper dwelling Rotalipora species (R. deekei,
R. greenhornensis) disappeared and one surface (W.
archeocretacea) and two subsurface dwellers (P.
aumalensis, P. praehelvetica) appeared. Further
extinctions and evolutions occurred at the top of this
interval and transition to the benthic oxic zone (Fig.
14). At this transition, the last deep dweller (R.
cushmani) and a subsurface dweller (P. inornata)
disappeared, followed by the temporary disappearance of several other subsurface dwellers (e.g., P.
aumalensis, P. praehelvetica, A. multiloculata, D.
algeriana, Plates 1 and 2). At the same time diversification occurred in surface (Whiteinella aprica, G.
albertensis) and subsurface waters (D. imbricata, D.
hagni), though one surface dweller (G. bentonensis)
disappeared coincident with the peak d13C shift in
the benthic oxic zone (93.86 Ma).
This faunal turnover indicates major changes in
water mass stratification from surface to deep, and
struggling populations trying to adapt to these changing conditions. The deeper water rotaliporids died
out, though not before trying to adapt to living in
shallower subsurface habitats by losing keels and
inflating chambers for greater buoyancy. Such
experiments in adaptations included A. multiloculata
as well as early praeglobotruncanids and dicarinellids
(Eicher, 1972). Only one surface dweller disappeared
(G. bentonensis) and several new species evolved
(mostly whiteinellids). This is not surprising since
surface dwellers are more adapted to variable conditions, whereas subsurface and deep dwellers inhabit relatively stable habitats and adapt poorly to
changing habitats.
What caused the change in water mass stratification and what was its nature? Clues can be
obtained from the stable isotope record. After the
first phase of the d13C shift and sea level transgression there is a rapid decrease in both d13C and
d18O values (93.91 Ma, Fig. 14), coincident with
the first diverse benthic assemblages (including
Cibicidoides) indicating well oxygenated bottom
waters. These oxic bottom waters and lower d18O
values persisted for about 100 ky, though d13C
values remained high and suggest high surface
125
productivity. The benthic oxic zone has been observed throughout the WIS (Eicher, 1969a,b; Eicher
and Worstell, 1970; West et al., 1998) and may
reflect an influx of oxygenated deeper water from
the Tethys as a result of the sea level transgression.
However, a benthic oxic zone at this interval is also
observed in Morocco (Thomas Wagner, personal
communication, 2002) and suggests a global event,
though the actual source of this oxic deep water
still needs to be investigated.
Upwelling of oxygen-rich waters is the likely cause
for the weak oxygen minimum zone during the
benthic oxic zone, as suggested by the strongly
reduced Heterohelix populations. Surface water
appears to have remained largely subsaline due to
freshwater influx, as suggested by the 2.5xlower
d18O values and high abundance of H. planispira
(Fig. 14). However, the appearance of significant
populations of the eutrophic surface opportunist
Guembelitria (G. cenomana, G. albertensis) suggests
that surface waters are nutrient enriched, probably due
to upwelling. By 93.78 Ma, a major shift to Heterohelix dominated assemblages and rare low oxygen
tolerant benthic assemblages mark the return of an
expanded OMZ and dysoxic or anoxic bottom waters.
This OMZ event is associated with a 2/3 drop in
species diversity at both Pueblo and Eastbourne,
indicating severely restricted habitats. In the early
Turonian strongly reduced H. planispira populations
reflect more normal marine surface salinity and increased abundance of deeper dwelling dicarinellids
and praeglobotruncanids indicate a deeper marine
environment.
9. Conclusions
1. The global stratotype section and point (GSSP) at
Pueblo contains an essentially complete sedimentary record across the global ocean anoxic event
(OAE 2) and the Cenomanian –Turonian boundary.
Sediment accumulation rates average 1.23 cm/ky
for the lower part and 0.87 cm/ky for the upper part
of the Bridge Creek Limestone and about 0.5 cm/
ky during deposition of the Hartland Shale
Member.
2. A high-resolution biostratigraphic scheme is introduced that integrates the d13C shift and new
126
3.
4.
5.
6.
G. Keller, A. Pardo / Marine Micropaleontology 51 (2004) 95–128
subdivisions of W. archeocretacea and R. cushmani
zones; the same zonal subdivisions are coeval at
Eastbourne.
H. planispira is a proxy for subsaline surface
waters as indicated by covariance in negative d18O
shifts (freshwater influx) and peak abundance in H.
planispira populations. Heterohelix, a proxy for
low oxygen waters, dominates at times of positive
d18O shifts (incursion of more normal marine
salinity) and is an indicator of the strengths of the
oxygen minimum zone.
A benthic oxic zone begins after the maximum sea
level transgression and OAE 2 d13C shift and
persist for about 100 ky. Low Heterohelix
abundance indicates a well-oxygenated water
column, and the appearance of Guembelitria
suggests nutrient-rich surface waters. These conditions can be explained by an influx of oxygenated deeper water from the Tethys and
upwelling during the sea level transgression.
The OAE 2 faunal turnover, characterized by 30%
species extinctions and 30% evolutionary diversification, results in no net loss in diversity and the
combined relative abundances of outgoing and
incoming species are less than 2% and 4%,
respectively, of the total assemblages. This faunal
turnover is related to a major sea level transgression, the influx of oxygen-rich bottom waters,
increased productivity associated with a major
positive excursion in d13C values. Lowest species
diversity coincides with a shift to Heterohelix
dominance that marks an expanded OMZ after the
benthic oxic zone.
A mid-Cenomanian d13C shift and sea level
transgression in the Hartland Shale (95.71 –95.80
Ma) is associated with a significant faunal turnover, though not of the magnitude of OAE 2. The
increased species diversity reflects the deeper
marine environment and increased water mass
stratification.
Acknowledgements
We thank Jake Hancock who graciously offered his
time to drive Thierry Adatte and GK to the outcrop
during a meeting on Cretaceous Climate in Florissant,
Colorado, in July of 2002. We gratefully acknowledge
the review comments and suggestions by Don Eicher,
and thank Thierry Adatte, Zsolt Berner and Doris
Stueben for sharing the isotope data, and Sigal
Abrmaovich for assistance with SEM illustrations.
This study was supported by NSF INT-0115357.
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