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.

O-84<br />

Predicti<strong>on</strong> of gas volume and dryness in shale gas systems:<br />

kinetic modeling of kerogen and retained hydrocarb<strong>on</strong>s thermal<br />

cracking in Barnett And Posid<strong>on</strong>ia shales<br />

Françoise Behar 1 , Daniel Jarvie 2<br />

1 IFP Energies Nouvelles, Rueil-Malmais<strong>on</strong>, France, 2 Worldwide <strong>Geochemistry</strong> Company, Humble, United<br />

States of America (corresp<strong>on</strong>ding author:francoise.behar@ifpenergiesnouvelles.fr)<br />

The aim of the present study is to predict the volumes<br />

of the different sources of gas generated during<br />

kerogen cracking in the Ro range 0.5 to 3.0 and to<br />

add the c<strong>on</strong>tributi<strong>on</strong> of generated gas from sec<strong>on</strong>dary<br />

cracking of retained hydrocarb<strong>on</strong> compounds in<br />

source rocks after the main phase of primary<br />

expulsi<strong>on</strong>. For that purpose, two immature kerogens<br />

from the Barnett Shale (US) and from the Posid<strong>on</strong>ia<br />

Shale (Germany) were selected. First they were<br />

artificially matured by closed system pyrolysis in the<br />

temperature range 250-350°C and with durati<strong>on</strong>s<br />

between 1 to 216h. Then, for late gas generati<strong>on</strong>,<br />

kerogens already matured at 375°C/24h, were heated<br />

between 400 and 600°C.<br />

The following kinetic schema was optimised (Behar et<br />

al., 2008a) :<br />

Kerogen = n<strong>on</strong> HC gas + HC1 + Asp. + kerogen 2<br />

Asphaltenes = n<strong>on</strong> HC gas + HC1 + Resins + prechar<br />

Resins = HC1 + prechar<br />

HC1 = HC2 + prechar<br />

The optimised kinetic parameters show that the<br />

asphaltenes are as unstable as the kerogen from<br />

which they originate. Their maximum yields are 64 –<br />

65% for the two samples, with those of the resins<br />

being respectively 19 and 28% for the Barnett and<br />

Posid<strong>on</strong>ia. The associated gas generated with oil<br />

does not exceed 5% and is mainly wet. The maximum<br />

yield of late gas is respectively 6% and 4% for the<br />

Barnett and Posid<strong>on</strong>ia kerogens. It is almost pure<br />

methane since the ethane yield does not exceed<br />

0.4% and neither propane and butane are produced.<br />

For the two shale gas kerogens, a full compositi<strong>on</strong>al<br />

kinetic model (Behar et al., 2008b) was used to<br />

predict both the mass balance and chemical<br />

compositi<strong>on</strong> of the retained compounds after the main<br />

phase of oil generati<strong>on</strong> and expulsi<strong>on</strong>. Then, from this<br />

mass balance, it was possible to predict the gas<br />

volume and dryness during further thermal maturati<strong>on</strong><br />

for Ro range between 1.0 and 2.7 %Ro. Results are<br />

shown <strong>on</strong> Fig. 1 for the Barnett shale. In the Ro range<br />

between 1 and 1.5%, the gas dryness rapidly<br />

increases from 65 to 80% with a maximum yield of<br />

4%. Then, an additi<strong>on</strong>al c<strong>on</strong>tributi<strong>on</strong> of 3% of dry gas<br />

leads to a final gas dryness at almost 90% These<br />

results are in excellent agreement with observed data.<br />

dryness dryness (%) (%)<br />

yield yield (%) (%)<br />

6.0<br />

4.5<br />

3.0<br />

1.5<br />

Gas generati<strong>on</strong><br />

0.0<br />

1.0 1.5 2.0 2.5<br />

100<br />

90<br />

80<br />

70<br />

60<br />

Ro (%)<br />

Gas dryness<br />

50<br />

1.0 1.5 2.0 2.5<br />

Ro (%)<br />

wet gas<br />

dry gas<br />

Fig. 1: Predicti<strong>on</strong> of gas volume and dryness under<br />

geological c<strong>on</strong>diti<strong>on</strong>s in the Ro range from 1 to 3%.<br />

References :<br />

Behar, F., Lorant, F., Lewan, M.D., 2008a.<br />

Elaborati<strong>on</strong> of a new compositi<strong>on</strong>al kinetic schema for<br />

oil cracking. <strong>Organic</strong> <strong>Geochemistry</strong> 39, 764-782.<br />

Behar, F., Lorant, F., Mazeas, L., 2008b. Elaborati<strong>on</strong><br />

of a new compositi<strong>on</strong>al kinetic schema for oil<br />

cracking. <strong>Organic</strong> <strong>Geochemistry</strong> 39, 764-782.<br />

146

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

Saved successfully!

Ooh no, something went wrong!