Martin J Blunt Department of Earth Science and Engineering, Imperial College London Two hundred barrels left: an analysis of population growth, oil reserves.

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Presentation transcript:

Martin J Blunt Department of Earth Science and Engineering, Imperial College London Two hundred barrels left: an analysis of population growth, oil reserves and carbon dioxide emissions

Big question? Volatile oil prices Financial crisis Rising food prices Growing population Peak oil Global warming Where are we heading?

World population

Growth rates

Population growth

Growth rate as a function of population

US population to the present day

US population growth rate

Swedish population

Swedish population growth rate

Population of Saudi Arabia

Growth rate for Saudi Arabia

Population of Rwanda

Growth rate for Rwanda

Global population growth rates fit to linear models Logistic equation K is carrying capacity

Logistic equation

Population projections Green line – my estimate Other lines and crosses: more detailed estimates from the UN, US Census Bureau and the World Bank

Hubbert analysis of oil production NNNN

US oil production to 1960

US oil production – data and prediction

US oil production to 1960

Hubbert analysis for world oil production

Hubbert prediction – peak in 2010!

Total volume of discoveries worldwide, From Tertzakian, 2006; based on Harper, 2003

Comments Oil is integral to our society – think of something that doesn’t use oil in its manufacture or distribution. We are not about to run out of oil, but it is a precious resource. So what will happen?

Fossil fuels and global warming What is the greenhouse effect? What does it have to do with carbon dioxide? What has carbon dioxide to do with the oil industry? Are we likely to damage the climate? Should we be worried? Don’t listen to opinions – work this out for yourselves.

What determines climate? Radiative heat transfer from the sun (which is influenced by orbital mechanics, solar variations) Flow of warm and cold water in the ocean Flow of warm and cold air in the atmosphere Reflection of sunlight back to space Greenhouse gases Feedbacks (much more about this later) Source: Lamb & Singleton, Earth Story, Princeton U. Press, 1998

(ORNL 1997) Carbon exchange with the environment

Atmospheric CO 2 concentration - Last glacial maximum to present

Radiation energy balance Source: IPCC Third Assessment Report, 2001

Greenhouse gases Water is the most important GHG. CO 2, CH 4, N 2 O and CFCs are other important GHGs. Sulfur emissions (aerosol precursors have also risen). Surface ocean pH has declined by 0.1 due to dissolving CO 2. Source: IPCC Third Assessment Report, 2001

The Earth is a greenhouse planet The combination of solar irradiance and greenhouse effect determines the mean surface temperatures of Mars, Earth and Venus. In the absence of the natural greenhouse effect, the average surface temperature of Earth would be -19 o C o C15 o C 452 o C Average Surface Temperatures MarsEarth Venus Source: C.T. Bowman, Mechanical Engineering, Stanford

Source: IPCC, “Climate Change 2001: The Scientific Basis, Cambridge Univ. Press, UK (2001)

How much carbon dioxide?

Concentration in the atmosphere

Fossil fuel reserves

Population growth

How much oil per person?

Carbon dioxide concentrations

What can we do? We do still need the oil industry. Yes, we will continue to use fossil fuels – like it or not. There is only one technology that can save us…..?

Carbon capture and storage How much can be stored? 920 Gt – 45% of emissions to 2050 in oil and gas fields ,000 Gt in aquifers % of emissions to 2050 IEA estimates. 700 Gt in North Sea alone (DTI) ≈ CO 2 produced by all UK population for >50 years

Critical point of CO 2 is 31 o C and 72 atm (7.2 MPa). CO 2 will be injected deep underground at supercritical conditions (depths greater than around 800 m). CO 2 is relatively compressible; density less than water, similar to oil. Low viscosity – around10% of that of water. Carbon dioxide properties

Current emissions are around 30 Gt CO 2 per year (8.5 Gt carbon). Say inject at 10 MPa and 40 o C – density is kgm -3. This is around 10 8 m 3 /day or around 700 million barrels per day. Current oil production is around 85 million barrels per day. Huge volumes – so not likely to be the whole story, but could contribute 1-2 Gt carbon/yr…. Costs: 1-2p/KWh for electricity for capture and storage; £25-60 per tonne CO 2 removed – Shackley and Gough, Could help fill the UK emissions gap in Some numbers

North Sea storage Large capacity in mature oil and gas fields. Oil and gas field relatively small traps in much larger aquifers. Engineering challenge to construct the capture, transport and injection infrastructure. Most current infrastructure would need to be replaced.

Trapping background How can you be sure that the CO 2 stays underground? Dissolution, chemical reaction, cap-rock and capillary trapping. Capillary trapping is rapid (decades): CO 2 as pore-scale bubbles surrounded by water. host rock

Pore-scale CO 2 trapping CO 2 bubbles

Design of CO 2 storage Injector Producer SPE 10 reservoir model, 1,200,000 grid cells (60X220X85), 7.8 Mt CO 2 injected. Qi et al., SPE A case study on a highly heterogeneous field representative of an aquifer below the North Sea:  Inject brine and CO 2 together and then use chase brine to trap CO 2  1D results are used to design a stable displacement  Simulations are used to optimize trapping

3D results for aquifer storage Mobile CO 2 saturation Z 170m X 3200m Y 2280m Trapped CO 2 saturation X 3200m Y 2280m Z 170m 20 years of water and CO 2 injection followed by 2 years of water injection in realistic geology 95% of CO 2 trapped after 4 years of water injection Qi et al., SPE

Conclusions and thanks Do your own analysis! Many students and post-docs and research funders: