Sites
U1402 |
U1404 |
U1405 |
U1406 |
U1407 |
U1408 |
U1409 |
U1410 |
U1411
IODP Expedition 342: Paleogene Newfoundland Sediment Drifts
Site U1403 Summary
PDF file is available for download.
Background and objectives
Site
U1403 (proposed site JA-01) is the first and the deepest water site to be
drilled on the J Anomaly Ridge, pinning the deep end of the Paleogene
Newfoundland sediment drifts depth transect. The site is positioned to capture
deep excursions of the calcite compensation depth (CCD) during the Paleogene
and to help improve stratigraphic control on the sediments to be drilled on J
Anomaly Ridge. A secondary goal at Site U1403 was to identify the age and
lithology of a reflector-rich sediment package that lies beneath the
acoustically homogenous unit that is a primary drilling target for Expedition
342.
Principal Results
After
a 946 nmi transit from Site U1402 the vessel
stabilized over Site U1403 at 1708 h (UTC-2.5h) on 11 June 2012. The original
plan called for three holes to a depth of ~250 m DSF (driller's depth below seafloor),
but the science decision was ultimately to complete operations with two holes:
Hole U1403A to 253.3 m DSF, and Hole U1403B to 265.1 m DSF. Hole U1403A was
spudded at 1020 h on 12 June. The water depth based on the 5.85-m long mudline core was 4944.3 m. The APC system recovered Cores
U1403A-1H through 17H, where a hard layer was encountered at ~148 m DSF. The
XCB system was deployed for Cores U1403A-18X through 29X to a final depth of 253.3
m DSF. The seafloor was cleared at 1240 h on 14 June, ending Hole U1403A.
Overall core recovery for Hole U1403A was 231.82 m for the 253.3 m interval
cored (91% recovery).
The
vessel was offset 20 m to the east and Hole U1403B was spudded at 1730 h on 14
June. The intent was to recover ~8 m in the mudline
core. The 3.9 m core recovery was a surprise, yielding a water depth of 4948.7
m, 4.4 m deeper than recorded in Hole U1403A. This, and correlation of features
across the two holes, led to the suspicion that the water depth estimate for
Hole U1403A was incorrect for unknown reasons. The APC coring system was used
for Cores U1403B-1H through16H. The XCB system was deployed for Cores
U1403B-17X through 18X, until we broke through the chert layers at 150.4 m DSF.
The APC coring system was again deployed for Cores U1403B-19H through 22H to a
depth of 175.9 m DSF. After a partial stroke core with a 2.97 m recovery, the
XCB system was again deployed for Cores U1403B-23X through 32X, to a final
depth of 265.1 m DSF. Overall, core recovery for Hole U1403B was 229.81 m for
the 265.1 m cored interval (87% recovery).
Site
U1403 yielded diverse types of deep-sea pelagic sediments within five lithologic units of Pleistocene to Late Cretaceous (Campanian) age. Core recovery and condition were excellent
overall and included records of the K-Pg Boundary
Extinction Event, the Late Eocene Chesapeake Bay impact and the Eocene hyperthermals ETM2 and PETM. The majority of the Paleogene
is carbonate poor but relatively rich in siliceous microfossils. This record is
consistent with paleo-depths below the local calcite
compensation depth (CCD), and anchors the deepest water site of the Expedition
342 depth transect. Initial results reveal episodic
deepening of the calcite compensation depth (CCD), which may be evidence of
carbonate compensation ÒovershootsÓ that enhance carbonate deposition in the
deep sea, a predicted response to transient global warming and ocean
acidification events.
The
downhole lithostratigraphy at Site U1403 includes
foraminifer sandy clay, unfossiliferous clay, red,
brown, and black chert, clay with radiolarians, clay with nannofossils
and radiolarians, nannofossil ooze and chalk. Uppermost sediments
include foraminifer sand with manganese nodules that overly a succession of unfossiliferous clay, and clay with nannofossils and radiolarians. Chert horizons are present below 150 m between intervals of radiolarian clay and nannofossil ooze and chalk. The chert horizons are
typically poorly recovered. A thin, graded, green spherule horizon is present
at the K-Pg boundary and interpreted as debris from the Chicxulub impact event. Underlying sediments largely consist of color banded nannofossil chalk to
a depth of ~262 m.
Site
U1403 recovered a sequence of Holocene-Pleistocene to Campanian
sediments. Quaternary calcareous nannofossils and planktic
foraminifers are present in the uppermost 2 m of the section, but from 2 to 70
m the sediments contain no age-diagnostic fossils. Calcareous nannofossils and radiolarians indicate a middle Eocene
(44.5 Ma) and lower Eocene to K-Pg boundary sequence
from ~70 to 220 m. Radiolarian assemblages are diverse and well preserved in
the middle and lower Eocene and provide the only age control between 70 and 119
m CSF-A. Preliminary biostratigraphic analysis
suggests that minor hiatuses may exist in the lower Eocene and middle-upper
Paleocene. Fossiliferous sequences of both the PETM
and ETM-2 hyperthermal events were recovered and
include ÒexcursionÓ calcareous nannofossil assemblages.
The K-Pg boundary section appears to be biostratigraphically complete. A high diversity uppermost Maastrichtian calcareous nannofossil
assemblage occurs below the K-Pg impact ejecta bed and very low diversity, post–mass-extinction assemblages occur above this bed. Earliest Danian
assemblages are dominated by calcareous dinoflagellates
and a handful of Cretaceous calcareous nannofossil
survivor species, and are followed up-section by a record of nannoplankton recovery and diversification. Hole U1403B bottomed at ~262 m in upper Campanian sediments consisting largely of nannofossil chalk. Planktic foraminifers are absent or very poorly preserved
through most of the succession, except for an interval of well-preserved
assemblages in the lowermost Danian and uppermost Maastrichtian. Benthic foraminiferal assemblages characterized by calcareous taxa are present throughout the Paleocene to Cretaceous.
Paleomagnetic results from Site U1403 revealed a
continuous series of normal and reverse magnetozones between
Sections U1403A-6H-1 and 16H-1 (~46-140 m CFS-A) and between Sections U1403B-6H-5
and 16H-5 (~41-137 m CFS-A). This magnetic stratigraphy correlates well to Chrons C16n.1r through C22n on the geomagnetic polarity
timescale, and indicates that we have collected a continuous Early to Late
Eocene section (35.892-49.344 Ma). Site U1403 magnetostratigraphy
also indicates that the distinctive gray-blue interval at U1403A-6H-2, 80-120 cm
and U1403B-6H-5, 50-90 cm was deposited during C16n.1n (35.706-35.892 Ma).
Thus, this stratigraphic interval, which is characterized by the occurrence of euhedral feldspars and a large spike in natural gamma ray
radiation, marks the Chesapeake Bay Impact event.
A
partially spliced composite depth record was produced for Holes U1403A and
U1403B. The mudlines could not be reliably aligned
owing to an inconsistency in the apparent seafloor depths between the two
holes. A composite spliced record was achieved between Holes U1403A and U1403B
from ~20 and 150 m CCSF (core composite depth below seafloor). Below 150 m
CCSF, where chert layers were encountered in both holes, floating composite
sections for the ETM2, PETM, and the K-Pg boundary
and upper Maastrichtian were constructed.
Age-depth
relationships are based largely upon biostratigraphic
datums for radiolarians and calcareous nannofossils in Hole U1403A and a combination of paleomagnetic data from Holes U1403A and U1403B. The upper
~46 m of the sediment column at Site U1403 is undated other than an ~2 m-thick
layer of Holocene-Pleistocene sediment. The magnetostratigraphic
identification of C16n.1n (35.706-35.892 Ma) in Core U1403-6H (and discovery of
the same interval in Hole U1403B) represents the first of a series of dated
Paleogene horizons at Site U1403.
Our correlation indicates that average clay accumulation rates from
~40-50 Ma were ~1 cm/ky, and diminished to ~0.2 cm/ky from ~35-40 Ma. Average linear rates of sedimentation of ~0.6 cm/ky are relatively stable to ~148 m
CSF-A. Between 148 and 149 m CSF-A, a ~3 million year-long interval from 50.5 to 53.7 Ma
is recorded by a series of chert horizons. The lower Eocene to the PETM
sequence accumulated at average linear sedimentation rates of ~1.4 cm/ky. Immediately underlying the PETM, a highly condensed
chert-rich interval with at least one hiatus between 182 and 189 m CSF-A
corresponds to ~56-62 Ma. Average linear sedimentation rates of ~0.8 cm/ky are recorded in the interval spanning the K-Pg boundary (~62-69 Ma).
Headspace
gas analysis for the purpose of safety monitoring yielded low concentrations of
methane that gradually increased to 17 ppmv with
depth. Other higher hydrocarbon gases were not detected. TOC content was quite
low in the upper 34 m of Hole U1403A, ranging from 0.14 to 0.46
wt %, except for the interval 27-31 m where TOC content ranged from 1.4 to 1.7 wt%. Carbonate content varied between 0.04 and 0.80 wt% in Cores
U1403A-1H through 13H. In the
bottom of Core U1403A-13H (~137 m) carbonate increases to 60% and fluctuates
between about 2 and 40% to the bottom of the recovered sequence.
Grain
density values are typically low (~1.5 g/cm3) in lithologic
Units I to IV that are dominated by clay and then increase to 1.6 g/cm3 and gradually to 1.8 g/cm3 in lithologic
Unit V toward the deepest recovered sequences in the site. Porosity values are
generally high (80%) in the radiolarian-rich sediments of lithologic
Unit III and decrease (~60%) in the carbonate-rich section of lithologic Unit V.
Magnetic susceptibility (MS) falls from lithologic Unit I into the upper 18 m CSF-A of lithologic Unit II. Below 150 m CSF-A magnetic susceptibility shows large fluctuations between ~20
to values over 120 instrument units. These large amplitude increases in MS are
linked with major events such as the ETM-2, PETM, K-Pg
boundary and Campanian-Maastrichtian boundary. A
further large amplitude MS peak was documented in Paleocene sediments at Site
U1403. P-wave velocity increases progressively downhole in the upper 150 m
CSF-A to 1550 m/s, takes a step to a velocity of 1600 m/s in the chert at the
top of lithologic Unit V and continues to increase to
~1650 m/s at the bottom of the recovered section. NGR measurements average 30
cps until 110 m CSF-A, fall to 20 cps in the nannofossil
clays of lithologic Unit VI, and then show high
frequency fluctuations in carbonate sediments of lithologic Unit V.
At
the conclusion of coring at 2200 h on 16 June, the hole was swept clean with 30
barrels of high viscosity mud and the drill string was pulled from the hole to
78.43 m DSF for logging with the triple combo string and FMS-Sonic string. Two
attempts to deploy the logging tools failed and the tools became firmly stuck
inside the BHA with ~17 m of the tool string extending out from the bit. After
working the tools for several hours with no progress, the wireline was severed
and the pipe tripped to the surface. When the tools arrived on the rig floor it
was discovered that the triple combo tool string had parted, leaving ~17 m of
tools missing from the bottom of the tool string, including the density and
porosity tools.
A
video and sonar survey was planned to find and recover the lost tools. During
deployment, the camera was shaking, vibrating and rotating around the pipe due
to strong ocean currents. At 2145 h, with the bit ~30 m above the seafloor, the
signal from the subsea camera and the Mesotech Sonar
were lost. The pipe was tripped back to the rig floor with the camera frame
resting on top of the bit. Our suspicion that the co-axial cable supporting the
camera system had failed was confirmed when the camera cable arrived at the rig
floor.
Repair
of the camera system would have taken 1-2 days, and redeployment was likely to
result in the same problems. In addition, the potential loss of the only
re-entry system available for this vessel would have been detrimental to future
operations. The decision not to deploy the camera system again at this site
meant that we were unable to locate the lost logging tool or Hole U1403B. The
drill floor was secured at 1415 h on 19 June, ending Site U1403 (JA-1A) and
Hole U1403B.
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