HR: 11:20h
AN: OS42A-05 [Abstracts]
TI: Towards Determining the Upper Temperature Limits to Life on Earth: An In-situ Sulfide-Microbial
Incubator
AU: * Kelley, D
EM: kelley@u.washington.edu
AF: University of Washington, School of Oceanography
Box 357940, Seattle, WA 98195
United States
AU: Baross, J
EM: jbaross@u.washington.edu
AF: University of Washington, School of Oceanography
Box 357940, Seattle, WA 98195
United States
AU: Delaney, J
EM: jdelaney@u.washington.edu
AF: University of Washington, School of Oceanography
Box 357940, Seattle, WA 98195
United States
AU: Girguis, P
EM: girguis@mbari.org
AF: Monterey Bay Aquarium Research Institute, 7700 Sandholdt Road, Moss Landing, CA 95039
United States
AU: Schrenk, M
EM: mos@ocean.washington.edu
AF: University of Washington, School of Oceanography
Box 357940, Seattle, WA 98195
United States
AB:
Determining the maximum conditions under which life thrives, survives, and expires is critical to understanding how and where
life might have evolved on our planet and for investigation of life in extraterrestrial environments. Submarine black smoker
systems are optimal sites to study such questions because thermal gradients are extreme and accessible within the chimney
walls under high-pressure conditions. Intact cells containing DNA and ribosomes have been observed even within the most
extreme environments of sulfide structure walls bounded by 300\deg C fluids. Membrane lipids from archaea have been detected
in sulfide flanges and chimneys where temperatures are believed to be 200-300\deg C. However, a balanced inquiry into the
limits of life must focus on characterization of the actual conditions in a given system that favor reactions necessary to
initiate and/or sustain life. At present, in-situ instrumentation of sulfide deposits is the only effective way to gain
direct access to these natural high-temperature environments for documentation and experimentation. With this goal in mind,
three prototype microbial incubators were developed with funding from the NSF, University of Washington, and the W.M. Keck
Foundation. The incubators were deployed in 2003 in the walls of active black smoker chimneys in the Mothra Hydrothermal
Field, Endeavour Segment of the Juan de Fuca Ridge. All instruments were successfully recovered in 2004, and one was
redeployed for a short time-series experiment. Each 53-cm-long titanium assembly houses 27 temperature sensors that record
temperatures from 0 to 500\deg C within three discrete incubation chambers. Data are logged in a separate housing and
inductively coupled links provide access to the data loggers without removal of the instruments. During the initial
deployment, data were collected from 189 to 245 days, with up to $\sim478\deg$ K temperature measurements completed for an
individual instrument. Temperatures within the chimney walls ranged from near ambient conditions to $\sim280\deg$ C. Distinct
thermal gradients were delineated extremely well in each of the three discrete environmental chambers in all instruments. In
one instrument numerous perturbations were recorded simultaneously on all 27 probes showing temperature increases of up to
$\sim30\deg$ C. Smaller-scale fluctuations resulting from tidal perturbations were ubiquitous in all instruments. Tidal
pumping that mixes oxygenated seawater and reduced, volatile-rich hydrothermal fluids may be critical for development of
dense and diverse microbial communities within the outer chimney walls. Preliminary examination of some sterile mineral
surfaces emplaced within the chambers shows extensive biofilm development. Culturing experiments are ongoing and DNA has been
successfully extracted from many of the chambers for genetic characterization. This experiment is a component of the W.M.
Keck Foundation-funded proto-NEPTUNE Observatory and Ridge R2K program at Endeavour.
DE: 4832 Hydrothermal systems
DE: 4200 OCEANOGRAPHY: GENERAL
DE: 4294 Instruments and techniques
SC: Ocean Sciences [OS]
MN: 2004 AGU Fall Meeting