24.02.2013 Views

25th International Meeting on Organic Geochemistry IMOG 2011

25th International Meeting on Organic Geochemistry IMOG 2011

25th International Meeting on Organic Geochemistry IMOG 2011

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

P-290<br />

On the problem of preservati<strong>on</strong> of hydrocarb<strong>on</strong>s (HC) and<br />

organic matter (OM) at high pressures (HP) and temperatures<br />

(HT) (experimental data)<br />

Vasily Melenevskiy 1 , Yury Palyanov 2 , Alexander Sokol 2 , Vladislav Maly 3<br />

1 Institute of Petroleum Geology and Geophysics, Siberian Branch of the Russian Academy Science (SB<br />

RAS), Novosibirsk, Russian Federati<strong>on</strong>, 2 Institute of Geology and Mineralogy SB RAS, Novosibirsk, Russian<br />

Federati<strong>on</strong>, 3 Institute of Hydrodynamics SB RAS, Novosibirsk, Russian Federati<strong>on</strong> (corresp<strong>on</strong>ding<br />

author:vmelenevsky@yandex.ru)<br />

We studies the behavior of HC and coal in<br />

the c<strong>on</strong>diti<strong>on</strong>s of supercritical fluid at HP and HT,<br />

which account for diam<strong>on</strong>d stability c<strong>on</strong>diti<strong>on</strong>s, and<br />

that of dispersed OM and coal under shock-wave<br />

loading. The reacti<strong>on</strong> products were examined by<br />

means of chemical, X-ray and pyrolytic (Rock – Eval)<br />

methods. The analysis technique, and the experiment<br />

procedures, and, partly, the findings of the studies<br />

are described in the works [1 - 4].<br />

Supercritical fluids Experiments were<br />

carried out in a multi-anvil high-pressure apparatus of<br />

the ‗‗split-sphere‖ type at temperature 1200 ’ 1420 о С<br />

and pressure 5,2 ÷ 5,7 GPa [3, 4]; eicosane,<br />

anthracene and bituminous coal (R o vt=0.94 %, HI=<br />

225 mg HC/g Соrg) were used as the objects of the<br />

study.<br />

When heated in HT-HP c<strong>on</strong>diti<strong>on</strong>s, the first<br />

processes starting to proceed in coal is cracking,<br />

followed by further decompositi<strong>on</strong> of the hydrocarb<strong>on</strong><br />

products yielded and ending by the build-up of<br />

metamorphized residuals. The data analysis showed<br />

that the coal has metamorphically altered to pass to<br />

the metaanthracitic stage of coalificati<strong>on</strong> (atomic ratio<br />

(Н/С)at was shown to decrease against the initial<br />

value of 0.84 to 0.24). X-ray diffracti<strong>on</strong> data for the<br />

residual solid OM after the experiment <strong>on</strong> HCs have<br />

proven it to be represented by graphite. The<br />

accuracy of establishing the HC decompositi<strong>on</strong><br />

degree was defined with the analysis blank value in<br />

the experiment. Under the HT-HP experiment<br />

c<strong>on</strong>diti<strong>on</strong>s, the decompositi<strong>on</strong> degree value might not<br />

exceed 0.999, according to our estimati<strong>on</strong>s.<br />

However this estimati<strong>on</strong> proved correct <strong>on</strong>ly<br />

for HC with nCi>10. For the light HC additi<strong>on</strong>al<br />

investigati<strong>on</strong>s are needed.<br />

Shock wave experiment. To model the<br />

impact processes going <strong>on</strong> when a meteorite hits the<br />

surface of the Earth, we used explosi<strong>on</strong> technique in<br />

the geometrical versi<strong>on</strong> of cylindrical symmetry [1, 2].<br />

Maximum (calculated) pressure within the fr<strong>on</strong>t of a<br />

det<strong>on</strong>ati<strong>on</strong> wave varied within the interval 2.0÷ 6.0<br />

GPa. OM proved to have morphed into graphite<br />

during the experiment; neither gaseous or heavy<br />

hydrocarb<strong>on</strong> have been detected in the sample after<br />

the experiment.<br />

8 cm<br />

Fig. This picture shows l<strong>on</strong>gitudinal secti<strong>on</strong><br />

of the c<strong>on</strong>tainer with the sample subjected to<br />

explosi<strong>on</strong> with intensity of 2.00 Gpa. The upper arrow<br />

indicates the det<strong>on</strong>ati<strong>on</strong> wave directi<strong>on</strong>.<br />

In the left porti<strong>on</strong> of the picture we can see a<br />

c<strong>on</strong>e-shaped darkened area, an indicati<strong>on</strong> of the<br />

largest transformati<strong>on</strong>s, c<strong>on</strong>sisting in graphitizati<strong>on</strong> of<br />

OM; whereas, the starting OM has hardly been<br />

altered outside this area. Thus after the explosi<strong>on</strong><br />

there was formed practically n<strong>on</strong>-gradient boundary<br />

between high and low maturity OM.<br />

References<br />

[1] Melenevsky V. N., et al. (2003) Geokhimia, №12,<br />

p.1332-1336.<br />

[2] Melenevsky V. N. et al. (2005) DAN, v. 405, p. 1-<br />

3.<br />

[3] Melenevsky V., K<strong>on</strong>torovich. A. (2007) Problemy<br />

TEC (In Russian), #1, p.18-21.<br />

[4] Alexander G. Sokol et al. (2009) Geochim. et<br />

Cosmochim. Acta, v. 73, p.5820–5834.<br />

423

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!