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25th International Meeting on Organic Geochemistry IMOG 2011

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P-182<br />

The influence of hydrogen <strong>on</strong> organic matter cycling at the lost<br />

city hydrothermal field<br />

Susan Lang 1 , Gretchen Früh-Green 1 , Stefano Bernasc<strong>on</strong>i 1 , Marvin Lilley 2<br />

1 ETH Zürich, Zürich, Switzerland, 2 University of Washingt<strong>on</strong>, Seattle, United States of America<br />

(corresp<strong>on</strong>ding author:susanqlang@gmail.com)<br />

Fluids from the Lost City Hydrothermal Field are rich<br />

in hydrogen and methane, with high pHs (9 – 11), as<br />

a result of serpentinizati<strong>on</strong> reacti<strong>on</strong>s at moderate<br />

temperatures of approximately 120-200°C [1].<br />

Carb<strong>on</strong>ate chimneys in the middle of the field vent<br />

fluids that are warmer (up to 91�C) and have higher<br />

hydrogen c<strong>on</strong>centrati<strong>on</strong>s (up to 14 mmol/kg) than<br />

those <strong>on</strong> the periphery of the field (as low as 47�C,<br />

1.3 mmol/kg) [2]. The decreases of hydrogen<br />

c<strong>on</strong>centrati<strong>on</strong>s have been attributed to sulfate<br />

reducti<strong>on</strong>. To gain insight into organic matter cycling<br />

under these different chemical c<strong>on</strong>diti<strong>on</strong>s, the organic<br />

matter incorporated into high-hydrogen chimneys was<br />

compared to that in low-hydrogen and extinct<br />

chimneys that were no l<strong>on</strong>ger venting fluids. Chimney<br />

samples were decarb<strong>on</strong>ated and the residual was<br />

analyzed for total organic carb<strong>on</strong>, total organic<br />

nitrogen, stable isotopic compositi<strong>on</strong> ( 13 C, 15 N), and<br />

radiocarb<strong>on</strong> c<strong>on</strong>tent (Δ 14 C).<br />

Residuals from actively venting chimneys had C/N<br />

ratios similar to that of fresh microbial biomass, and<br />

low � 15 N values that could be attributed to either<br />

nitrogen fixati<strong>on</strong> or assimilati<strong>on</strong> of seawater nitrate.<br />

No significant variati<strong>on</strong>s between chimneys hosting<br />

low- or high- hydrogen fluids were found in C/N or<br />

� 15 N values. Residuals from extinct structures had, <strong>on</strong><br />

average, higher C/N ratios and higher � 15 N values<br />

than those of actively venting structures. While it may<br />

not be the sole processes, these trends are c<strong>on</strong>sistent<br />

with diagenesis.<br />

In general, chimneys hosting high hydrogen fluids<br />

were extremely low in total biomass. That biomass<br />

was significantly more enriched in 13 C than typical<br />

marine organic matter, as has been observed in other<br />

studies [1,3]. Comparatively, chimneys hosting low<br />

hydrogen fluids had higher biomass and were more<br />

depleted in 13 C. Initial results also indicate differences<br />

in the radiocarb<strong>on</strong> c<strong>on</strong>tent of the biomass between<br />

high- and low- hydrogen chimneys, suggesting there<br />

is variability in the amount of mantle carb<strong>on</strong><br />

incorporated into microbial cellular comp<strong>on</strong>ents.<br />

Further radiocarb<strong>on</strong> analyses are underway and will<br />

help to c<strong>on</strong>strain the processes that result in these<br />

distinct signatures.<br />

References:<br />

[1] Kelley et al., (2005) Science 307:1428-1434.<br />

[2] Proskurowski et al., (2006) Chemical Geology<br />

229(4) 331-343.<br />

[3] Bradley et al., (2009) Geochim. Cosmochim. Acta<br />

73(1): 102-118<br />

322

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