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25th International Meeting on Organic Geochemistry IMOG 2011

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P-174<br />

Distinct microbial inventories in terrestrial mud volcanoes of<br />

Northern Italy c<strong>on</strong>trolled by the source and compositi<strong>on</strong> of<br />

emitted fluids<br />

Christina Heller 1 , Martin Blumenberg 1 , Christoph Wrede 2 , Michael Hoppert 2 , Marco<br />

Taviani 3 , Joachim Reitner 1<br />

1 Geoscience Centre, University of Goettingen, Goettingen, Germany, 2 Institute of Microbiology and Genetics,<br />

University of Goettingen, Goettingen, Germany, 3 ISMAR-CNR, Bologna, Italy (corresp<strong>on</strong>ding<br />

author:cheller1@gwdg.de)<br />

Mud volcanoes are geological structures that occur in<br />

terrestrial and marine envir<strong>on</strong>ments worldwide and<br />

are caused by various geological processes e.g.<br />

tect<strong>on</strong>ic accreti<strong>on</strong> and faulting. In Italy such fluid<br />

venting structures occur al<strong>on</strong>g the external<br />

compressi<strong>on</strong>al margin of the Apennine chain, where<br />

the mud volcanoes are distributed al<strong>on</strong>g two belts [1].<br />

The natural Salse di Nirano (near Modena) is <strong>on</strong>e of<br />

the largest mud volcano areas in Italy, emitting gas<br />

with approximately 99 % methane and <strong>on</strong>ly minor<br />

amounts of higher hydrocarb<strong>on</strong>s. The fluids seeping<br />

out in Nirano pass through geological formati<strong>on</strong>s from<br />

the Jurassic to the lower Pleistocene [2]. In doing so,<br />

the mud is getting enriched in various electr<strong>on</strong><br />

acceptors (e.g. SO4 2- , NO2 - /NO3 - , O2), potentially<br />

fueling microbial aerobic and anaerobic oxidati<strong>on</strong> of<br />

hydrocarb<strong>on</strong>s, in particular methane [3,4,5]. A<br />

sec<strong>on</strong>d, smaller and geologically distinct mud volcano<br />

area is situated in Puianello (near Modena). In<br />

Puianello methane c<strong>on</strong>centrati<strong>on</strong>s in the gases are<br />

lower ~48 % and, in c<strong>on</strong>trast to Nirano, the fluids do<br />

not cross Messinian formati<strong>on</strong>s, thus, i<strong>on</strong>s like sulfate<br />

are relatively lower in c<strong>on</strong>centrati<strong>on</strong>.<br />

Our biomarker and molecular microbiological (16S<br />

rDNA) data show that microbial communities in the<br />

different mud volcanoes are distinct. We found signals<br />

of various eukaryotes, bacteria and archaea at both<br />

sites. In Nirano, however, specific bacterial dialkyl<br />

glycerol diethers (DAGE; in particular ai15/ai15- and<br />

16/16-DAGE) were found which are putatively<br />

sourced by sulfate-reducing bacteria (SRB) [6,7,8].<br />

The presence of archaea is evidenced by archaeol<br />

and hydroxyarchaeol and isotopic analyses of SRBderived<br />

bacterial DAGE as well as hydroxyarchaeol<br />

dem<strong>on</strong>strated 13 C-depleti<strong>on</strong>s with δ 13 C values low as -<br />

54‰, suggesting an involvement of the source<br />

organisms in the sulfate-dependent anaerobic<br />

turnover of methane. By c<strong>on</strong>trast, typical SRBbiomarkers<br />

were absent in sulfate-poor mud<br />

volcanoes in Puianello. But, various 13 C-depleted<br />

hopanoids e.g. 17β(H)21β(H)-bishomohopanol<br />

17β(H)21β(H)-bishomohopanoic acid and 3Me-<br />

17β(H)21β(H)-bishomohopanol were highly abundant.<br />

Since the latter are typical biomarkers for aerobic<br />

methanotrophs, those bacteria appear to be keyplayers<br />

in this envir<strong>on</strong>ment.<br />

Our data dem<strong>on</strong>strate a high microbial and metabolic<br />

diversity in terrestrial mud volcanoes in Italy, which is<br />

most likely c<strong>on</strong>trolled by different geological settings<br />

and thus mud compositi<strong>on</strong>s.<br />

[1] Minissale, A., Magro, G., Martinelli, G., Vaselli, O.,<br />

Tassi G.F. (2000). Tect<strong>on</strong>ophysics 319, 199-222.<br />

[2] B<strong>on</strong>ini, M. (2008). Geology 136, 131-134.<br />

[3] Nauhaus, K., Albrecht, M., Marcus Elvert, Boetius,<br />

A., Widdel F. (2007). Envir<strong>on</strong>. Microbiol. 9, 187–196.<br />

[4] Wrede, C. Brady, S., Dreier, A., Rockstroh, S.,<br />

Kokoschka, S., Heinzelmann, S.M., Heller, C, Reitner,<br />

J., Taviani, M., Daniel, R., Hoppert, M. (<strong>2011</strong>). Sed.<br />

Geol. (in revisi<strong>on</strong>).<br />

[5] Alain, K., Holler, T., Musat, F., Elvert, M., Treude,<br />

T., and Krüger, M. (2006). Envir<strong>on</strong>. Microbiol. 8, 574-<br />

590.<br />

[6] Pancost, R.D., Bouloubassi, I., Aloisi, G.,<br />

Sinninghe Damsté, J.S., Party, T.M. S. (2001a). Org.<br />

Geochem. 32, 695-707.<br />

[7] Pancost, R.D., Hopmans, E. C., Sinninghe<br />

Damsté, J. S., Party, T.M.S. (2001b). Geochim.<br />

Cosmochim Acta 65, 1611-1627.<br />

[8] Blumenberg, M., Seifert, R., Reitner, J., Pape, T.,<br />

and Michaelis, W. (2004). Proc. Nat. Acad. Sci. 101,<br />

30, 11111-11116.<br />

314

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