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Sub-millimeter structure and internal architecture of ODP 204

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DAVID FISCHER1,2, GERHARD BOHRMANN1, THOMAS PAPE1, STEPHAN A. KLAPP1,3, FRIEDER ENZMANN3, WERNER F. KUHS4, THOMAS HUTHWELKER5

BREMERHAVEN Am Handelshafen 12 27570 Bremerhaven Telefon 0471 4831-0 www.awi.de

Sub-millimeter structure and internal architecture of ODP 204

(Hydrate Ridge) gas hydrates revealed by Synchroton Radiation X-Ray Cryo-Tomographic Microscopy (SRXCTM)

Introduction

Although recognized worldwide in different environmental settings including the seafloor, natural hydrocarbon-gas hydrates (GH) remain rather exotic materials

whose interplay between chemical and physical parameters is still not fully under- stood. We radiographed gas hydrate specimen obtained during ODP Leg 204 to the renowned Hydrate Ridge offshore Oregon with Synchroton radiation provided by the Swiss Light Source in Villingen, Switzerland, in order to gain insight into their sub-millimeter scale internal structure. The project was conducted in the frame of the DFG-Schwerpunktprogramm “IODP”. In contrast to earlier studies focussing on shape parameters of hydrocarbon gas hydrates, our approach enabled us to investi- gate specific areas of interest within small samples and to identify internal, architec- tural particularities of single gas hydrate grains, grain boundaries and matrix mate- rials in the micometer to several hundreds of micrometers range.

With this study we provide a new and unique dataset of the sub-millimeter scale in- ternal structure of gas hydrates from Hydrate Ridge and show that Synchroton radi- tation is very helpful in investigating the architecture of natural hydrocarbon gas

hydrates. Future investigations are needed to 1) adapt, establish and refine the used method for examining gas hydrates and 2) compare samples from different envi-

ronmental settings and samples of different crystallographic compositions (e.g., sI and sII hydrates).

Contact: David Fischer david.fischer@awi.de 0049-471-48312389

1MARUM – Center for Marine Environmental Sciences and Department of Geosciences at the University of Bremen, Leobener Straße, D-28359 Bremen, Germany 2 Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research, Am Handelshafen 12, D-27570 Bremerhaven, Germany

3 Springer, Tiergartenstraße 17 | 69121 D-Heidelberg, Germany

4 GZG, Abt.Kristallographie, Georg-August-Universität Göttingen, Goldschmidtstr.1, D-37077 Göttingen, Germany 5 Swiss Light Source, Paul Scherrer Institute, CH-5232 Villigen, Switzerland

Study area (a) and ODP 204 sampling sites at Hy- drate Ridge (b). Figure (a) is from Goolge Earth (Inc.) and (b) originally appeared in Tréhu et al.

(2006).

Initial step in sample analysis: 3-D arrangement of grey- value tomographic slices produced using Synchroton ra- diation X-ray cryo-tomographic microscopy. Certain fea- tures are visible based on density differences. a) gas hy- drate, b) small boundary pore network, c) boundary pore network.

a

b c

Second step in sample analysis: Use 3-D visualization soft- ware to identify and mark segments of same/similar com- position or structure (purple: GH, green/yellow: pores).

Final step in sample analysis: Create and interpret 3-D vi- sualizations and understand the internal architecture of specimens.

Post-measurement workflow

1

2

3

Geographical and geological setting

Tubes (yellow), GH (purple translucent and blue). What are these tubes and is there a structural control on their dis- tribution?

Conclusions

1) SRXTCM provides essential insights into internal architecture of sub-millimeter scale gas hydrate

samples

2) Many samples contain gas-filled tubular structures of unknown origin

--> perhaps pressure release features?

3) Although not proven, we suggest that density dif- ferences between sI and sII gas hydrates might be vi- sible in SRXTM images

100 µm

200 µm 200 µm

200 µm

300 µm 300 µm

Preliminary results

Cited literature: Tréhu, A.M., Torres, M.E., Bohrmann, G., and Colwell, F.S., 2006. Leg 204 synthesis: gas hydrate distribution and dynamics in the central Cascadia accretionary complex. In Tréhu, A.M., Bohrmann, G., Torres, M.E., and Colwell, F.S. (Eds.), Proc. ODP, Sci. Results, 204: College Station, TX (Ocean Drilling Program), 1–40. doi:10.2973/odp.proc.sr.204.101.2006

a b

Distinct density differences within one piece of GH appear as different shades of grey: structures I and II?

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