HR: 16:30h
AN: PP14A-03 [Abstracts]
TI: An early Eocene transient warming ($\sim $53 Ma): Implications for
astronomically-paced early Eocene hyperthermal events.
AU: * Sluijs, A
EM: A.Sluijs@bio.uu.nl
AF: Laboratory of Palaeobotany and Palynology, Utrecht University, Budapestlaan 4, Utrecht, 3584 CD
Netherlands
AU: Lourens, L J
EM: llourens@geo.uu.nl
AF: Department of Geology, Faculty of Earth Sciences, Utrecht University, Budapestlaan 4, Utrecht, 3584 CD
Netherlands
AU: Kroon, D
EM: kroo@geo.vu.nl
AF: Faculty of Earth and Life Sciences, Vrije Universiteit, De Boelelaan 1085, Amsterdam, 1081 HV
Netherlands
AU: Zachos, J C
EM: jzachos@emerald.ucsc.edu
AF: Earth Sciences Department, University of California at Santa Cruz, Earth and Marine Sciences Building,
Santa Cruz, CA 95064
United States
AU: Thomas, E
EM: ethomas@wesleyan.edu
AF: Wesleyan University, 265 Church Street, Middletown, CT 06459-0
United States
AU: R”hl, U
EM: uroehl@allgeo.uni-bremen.de
AF: Department of Geosciences, Universit„t Bremen, Postfach 33 04 40, Klagenfurter Strasse, Bremen, 28334
Germany
AB:
Here we report on a pronounced hyperthermal event approximately 2 Myrs after
the Paleocene-Eocene thermal maximum (PETM) and place both events in a new
orbitally-tuned framework. This previously unrecognized transient event and
the underlying PETM were both recovered at five sites along a 2km depth
transect on the Walvis Ridge (southeast Atlantic) during Ocean Drilling
Program Leg 208. Similar to the PETM, this event, \textit{Elmo}, is marked by a red clay
layer, associated with severe drop in CaCO$_{3}$ concentrations, suggesting
a $\sim $2 km rise in the lysocline. High-resolution (1cm) bulk carbonate
$\delta ^{13}$C measurements of the shallowest, and hence most complete
Site 1263 revealed a $\sim $1.5% drop in $\delta ^{13}$C and $\delta
^{18}$O. The negative $\delta ^{13}$C excursion is composed of three
steep steps of which the last one corresponds to the base of the red clay
layer. The post-\textit{Elmo} interval mirrors the typical PETM signature with an
exponential recovery to pre-excursion $\delta ^{13}$C values. The
planktonic foraminiferal $\delta ^{13}$C record (measured on single
specimens of the surface dweller \textit{Acaranina soldadoensis}) confirms the bulk pattern, although the
amplitude of the excursion, $\sim $-2.5, is larger. The planktonic
foraminiferal $\delta ^{18}$O record shows the same $\sim $-1% excursion
as the bulk, suggesting a fast increase in sea surface temperature of $\sim
$4 degrees C. The case of conditions similar to the PETM during the ELMO
event is further strengthened by the occurrence of low diversity, diminutive
benthic foraminifer assemblages, and a decrease in planktonic foraminifer
diversity. Examination of published isotope, X-ray fluorescence and magnetic
susceptibility records further indicates that this event is global in nature
and recorded in other marine and terrestrial basins. Orbital tuning of the
deepest Sites 1262 magnetic susceptibility and Sites 1262 and 1267 color
reflectance records to the La2004 and R7 astronomical solutions shows that
the \textit{Elmo} is five 400-kyr eccentricity cycles younger than the PETM and that both
events are linked to eccentricity-maxima. This, and the subtle resemblance
between the \textit{Elmo} and PETM mentioned above, suggests that similar, astronomically
modulated, mechanisms are at the root of them. The leading hypothesis to
explain the PETM climatic event and its $\delta ^{13}$C excursion is the
dissociation of submarine methane hydrates. If the \textit{Elmo} shares a similar origin,
its less extreme appearance may be associated with the ability of the
methane hydrate reservoir to recharge after the PETM, especially under the
warm conditions that prevailed in the interval spanning the two events.
DE: 1610 Atmosphere (0315, 0325)
DE: 1615 Biogeochemical processes (4805)
DE: 1620 Climate dynamics (3309)
SC: Paleoceanography and Paleoclimatology [PP]
MN: 2004 AGU Fall Meeting