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Applied and Environmental Microbiology, November 2001, p. 5179-5189, Vol. 67, No. 11
Exobiology Branch, NASA Ames Research Center,
Moffett Field, California 940351;
Lehrstuhl für Mikrobiologie and Archaeenzentrum,
Universität Regensburg, D-93053 Regensburg,
Germany2; Australian Geological Survey
Organisation, Canberra, ACT 2601, Australia3; Department of Geology and
Geophysics, Woods Hole Oceanographic Institution, Woods Hole,
Massachusetts 025434; and Department of
Geology, Portland State University, Portland, Oregon
972015
Received 10 May 2001/Accepted 20 August 2001
The molecular and isotopic compositions of lipid biomarkers of
cultured Aquificales genera have been used to study the
community and trophic structure of the hyperthermophilic pink streamers and vent biofilm from Octopus Spring. Thermocrinis
ruber, Thermocrinis sp. strain HI 11/12,
Hydrogenobacter thermophilus TK-6,
Aquifex pyrophilus, and Aquifex aeolicus
all contained glycerol-ether phospholipids as well as acyl glycerides.
The n-C20:1 and
cy-C21 fatty acids dominated all of the
Aquificales, while the alkyl glycerol ethers were mainly
C18:0. These Aquificales biomarkers were
major constituents of the lipid extracts of two Octopus Spring samples,
a biofilm associated with the siliceous vent walls, and the well-known
pink streamer community (PSC). Both the biofilm and the PSC contained
mono- and dialkyl glycerol ethers in which C18 and
C20 alkyl groups were prevalent. Phospholipid fatty acids included both the Aquificales n-C20:1 and
cy-C21, plus a series of
iso-branched fatty acids
(i-C15:0 to
i-C21:0), indicating an additional bacterial
component. Biomass and lipids from the PSC were depleted in
13C relative to source water CO2 by 10.9 and
17.2
0099-2240/01/$04.00+0 DOI: 10.1128/AEM.67.11.5179-5189.2001
Copyright © 2001, American Society for Microbiology. All rights reserved.
Signature Lipids and Stable Carbon Isotope Analyses of Octopus
Spring Hyperthermophilic Communities Compared with Those of
Aquificales Representatives
, respectively. The C20-21 fatty acids of the PSC
were less depleted than the iso-branched fatty acids,
18.4 and 22.6
, respectively. The biomass of T. ruber
grown on CO2 was depleted in 13C by only 3.3
relative to C source. In contrast, biomass was depleted by 19.7
when
formate was the C source. Independent of carbon source, T.
ruber lipids were heavier than biomass (+1.3
). The depletion
in the C20-21 fatty acids from the PSC indicates that
Thermocrinis biomass must be similarly depleted and too
light to be explained by growth on CO2. Accordingly,
Thermocrinis in the PSC is likely to have utilized
formate, presumably generated in the spring source region.
*
Corresponding author. Mailing address: M/S 239-4, NASA
Ames Research Center, Moffett Field, CA 94035. Phone: (650) 604-3221. Fax: (650) 604-1088. E-mail:
ljahnke{at}mail.arc.nasa.gov.
Present address: Department of Earth, Atmospheric and Planetary
Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139.
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