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ENERGY R. E. Smalle Rice Univers SAM Distinguished Lecture iversity of Houston rch 17, 2003
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Page 1: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

ENERGY

R. E. Smalley Rice University

TCSAM Distinguished LectureUniversity of HoustonMarch 17, 2003

Page 2: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

• ENERGY is the single most important problem facing humanity today.

• WE CAN SOLVE THIS PROBLEM with revolutionary breakthroughs at the frontiers of Physical Sciences

& Engineering, and particularly in Nanotechnology

• We need a new APOLLO PROJECT to do this.

• The problem is huge, but it is also a magnificent opportunity.

• Success will revolutionize the largest industry in the world, Energy.

• American boys and girls will enter the physical sciences to do this, inspired by their idealism, their sense of mission, and their desire to be “where the action is”.

• In the process this new Apollo Project will produce a cornucopia of new technologies, and provide the underpinnings for vast new economic prosperity for the US and the world.

Page 3: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Humanity’s Top Ten Problemsfor next 50 years

1. ENERGY

2. WATER

3. FOOD

4. ENVIRONMENT

5. POVERTY

6. TERRORISM & WAR

7. DISEASE

8. EDUCATION

9. DEMOCRACY

10. POPULATION2003 6.3 Billion People2050 9-10 Billion People

Page 4: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

0

5

10

15

20

25

30

35

40

45

50

OilCoa

lGas

Fission

Biomas

s

Hydro

electr

ic

Solar,

wind, g

eothe

rmal

0.5%

Source: Internatinal Energy Agency

2003

0

5

10

15

20

25

30

35

40

45

50 2050

The ENERGY REVOLUTION (The Terawatt Challenge)

14 Terawatts

210 M BOE/day 30 -- 60 Terawatts450 – 900 MBOE/day

The Basis of Prosperity 20st Century = OIL 21st Century = ??

Page 5: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Projected Demand for Carbon-Free Energy

• M.I. Hoffert et. al., Nature, 1998, 395, 881, “Energy Implications of Future Atmospheric Stabilization of CO2 Content”

Possible Sources of Carbon-Free Energy

• M.I. Hoffert et. al., Science, 2002, 298, 981, “Advanced Technology Paths to Global Climate Stability: Energy for a

Greenhouse Planet”

Page 6: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Population Growth to 10 Billion People in 2050

Per Capita GDP Growthat 1.6% yr-1

Energy consumption perUnit of GDP declinesat 1.0% yr -1

Page 7: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Energy Demand & Source(in Terawatts)

2000 2020 2040 2060 2080 2100 YEARSource: M.I. Hoffert et. al., Nature, 1998, 395, 881,

20

30

40

10

0

50

TW million BOE/day

-- 200

-- 400

-- 600

Page 8: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Tonight’s Reading Assignment

“Hubbert’s Peak” by Kenneth Deffeyes (2001)

• King Hubbert predicted US oil production would peak in 1970. It did.

• The same approach predicts World Oil production will peak within this decade. It will.

• The days of cheap energy from oil will then be gone.

(See also Colin Campbell’s interview athttp://www.globalpublicmedia.com/INTERVIEWS/COLIN.CAMPBELL/)

Page 9: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

World Energy Millions of Barrels per Day (Oil Equivalent)

300

200

100

01860 1900 1940 1980 2020 2060 2100

Source: John F. Bookout (President of Shell USA) ,“Two Centuries of Fossil Fuel Energy” International Geological Congress, Washington DC; July 10,1985. Episodes, vol 12, 257-262 (1989).

Page 10: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

World Proven OIL Reserves 

Proven Oil Reserves(2000)

Iran9%

Mexico3%

Nigeria2%

Libya3%

China2%

Russia5%

UAE10%

Kuw ait9%

Iraq11%

Saudi Arabia25%

USA3%

Venezuela8%

Qatar1%

Other9%

THE REMAINING OIL RESERVES ARE NOT WHERE WE WANT THEM.

FOR TRANSPORTATION FUELS WE CURRENTLY HAVE NO CHOICE.

Page 11: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Tomorrow’s Reading Assignment

“The Hydrogen Economy: The Next Great Economic Revolution” by Jeremy Rifkin

(Tarcher/Putnam, 2002)

H2 is not a primary energy source.

But, after natural gas, it probably will be our future transportation fuel

and energy storage medium.

(also check out http://www.eere.energy.gov/ )

Page 12: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

PRIMARY ENERGY SOURCESAlternatives to Oil

• Conservation / Efficiency-- not enough• Hydroelectric -- not enough• Biomass -- not enough• Wind -- not enough• Wave & Tide -- not enough • Natural Gas -- sequestration?, cost?• Clean Coal -- sequestration?, cost?

• Nuclear Fission -- radioactive waste?, terrorism?, cost?

• Nuclear Fusion -- too difficult?, cost?

• Geothermal HDR -- cost ?• Solar terrestrial -- cost ?• Solar power satellites -- cost ?• Lunar Solar Power -- cost ?

Page 13: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Solar Cell Land Area Requirements

20 TW

3 TW

Graphic fromNate LewisCal Tech

165,000 TWof sunlighthit the earthevery day

Page 14: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Solar Cell Land Area Requirements

6 Boxes at 3.3 TW Each

Page 15: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Sun-Moon-Beam-Rectenna

KEY PROMOTER: DAVID CRISWELL

( Institute of Space Systems Operations, University of Houston)

Solar Power -> Lunar BaseS -> Power BeamS -> Earth ReceiverS

Page 16: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

≥ 20 TWe from the Moon

Page 17: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

14 Enabling Nanotech Revolutions1. Photovoltaics -- a revolution to drop cost by 10 to100 fold.

2. H2 storage -- a revolution in light weight materials for pressure tanks , and/or a new light weight, easily reversible hydrogen chemisorption system

3. Fuel cells -- a revolution to drop the cost by nearly 10 to 100 fold

4. Batteries and supercapacitors -- revolution to improve by 10-100x for automotive and distributed generation applications.

5. Photocatalytic reduction of CO2 to produce a liquid fuel such as methanol.

6. Direct photoconversion of light + water to produce H2

7. Super-strong, light weight materials to drop cost to LEO, GEO, and later the moon by > 100 x, to enable huge but low cost light harvesting structures in space; and to improve efficiency of cars, planes, etc.

8. Nanoelectronics to revolutionize computers, sensors and devices.

Page 18: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

9. High current cables (superconductors, or quantum conductors) with which to rewire the electrical transmission grid, and enable continental, and even worldwide electrical energy transport; and also to replace aluminum and copper wires essentially everywhere -- particularly in the windings of electric motors (especially good if we can eliminate eddy current losses).

10. Thermochemical catalysts to generate H2 from water that work efficiently at temperatures lower than 900 C.

11. CO2 mineralization schemes that can work on a vast scale, hopefully starting from basalt and having no waste streams.

12. Nanoelectronics based Robotics with AI to enable construction maintenance of solar structures in space and on the moon; and to enable nuclear reactor maintenance and fuel reprocessing.

13. NanoMaterials/ coatings that will enable vastly lower the cost of deep drilling, to enable HDR (hot dry rock) geothermal heat mining.

14. Nanotech lighting to replace incandescent and fluorescent lights

14 Enabling Nanotech Revolutions

Page 19: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

The People Problem

Number of Physics Ph.D. Degrees Awarded in the U.S.

0

200

400

600

800

1000

1200

1400

1600

1800

1900 1920 1940 1960 1980 2000

Year

Nu

mb

er

of

Ph

.D.s

TOTAL U.S. Citizens Permanent Visa Temporary Visa

Sputnik

End of WW II

Page 20: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Doctoral Sciences & Engineering Degrees

0

2000

4000

6000

8000

10000

12000

14000

16000

18000

1985 1990 1995 2000

Year

Nu

mb

er o

f D

egre

es G

ran

ted

Asians in Asian Institutions

Asians in US Institutions

US citizens in US Institutions

All nationalities in US Institutions

Source: Science and Engineering Doctorate Awards, 1996 and 2000, NSF; Science and Engineering Indicators,

NSB, 2002Sciences = Physics, chemistry, astronomy, earth, atmospheric, and ocean sciencesEngineering = Aeronautical, astronautical, chemical, civil, electrical, industrial, material, metallurgical, and mechanical.

By 2010, if current trends continue, over 90% of all physical scientists and engineers in the worldwill be Asians working in Asia.

Page 21: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Ph.D. Degrees in Physical Science and Engineering

0

5

10

15

20

25

30

1985 1990 1995 2000 2005

Year

Nu

mb

er

of

de

gre

es

gra

nte

d (

in

tho

us

an

d)

Asian Citizens

U.S. Citizens

Sources: Science and Engineering Doctorate Awards, NSF, 2001. Science and Engineering Indicators, NSB, 2002.

Sciences = Physics, chemistry, astronomy, earth, atmospheric, and ocean sciencesEngineering = Aeronautical, astronautical, chemical, civil, electrical, industrial, material, metallurgical, and mechanical.

Page 22: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

Ph.D. Degrees in Physics as a Percentage of GDP

0.01

0.02

0.03

0.04

0.05

1950 1960 1970 1980 1990 2000 2010

Year

Pe

rce

nt

GDP is expressed in constant 1996 dollars (in million) Source: American Institute of Physics & National Science Board, Science and Engineering Indicators, 2002.

The Sputnik Generation

Physical Scientist Production in the US is not keeping up with GDPeven though the physical sciences are the basis of most wealth creation.

We Need a NewSputnik Event to inspire US citizens into the Physical Sciences and Engineering.

We have one:

9/11

Page 23: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

The biggest single challenge for the next few decades:

ENERGY for 1010 people

• . At MINIMUM we need 10 Terawatts (150 M BOE/day) from some new clean energy source by 2050

• For worldwide peace and prosperity we need it to be cheap.

• We simply can not do this with current technology.

• We need Boys and Girls to enter Physical Science and Engineering as they did after Sputnik.

• Inspire in them a sense of MISSION( BE A SCIENTIST SAVE THE WORLD )

• We need a bold new APOLLO PROGRAM to find the NEW ENERGY TECHNOLOGY

Page 24: ENERGY R. E. Smalley Rice University TCSAM Distinguished Lecture University of Houston March 17, 2003.

New Energy Research Program(The Nickel & Dime Solution)

• For FY04-FY09 collect 5 cents from every gallon of oil product Invest the resultant > $10 Billion per year as additional funding in

frontier energy research distributed among DOE, NSF, NIST, NASA, and DoD.

• For the next 10 years collect 10 cents from every gallon; invest the >$20 Billion per year in frontier energy research.

• Devote a third of this money to New Energy Research Centers located adjacent to major US Research Universities.

• At worst this endeavor will create a cornucopia of new technologies and new industries.

• At best, we will solve the energy problem before 2020, and thereby lay the basis for peace and prosperity worldwide.


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