2. Energy Systems & Sustainability Freshman Seminar 2008

3. The Issue Before Us “One of the greatest challenges facing humanity during the twenty-first century must surely be that of giving everyone on the planet access to safe, clean & sustainable energy supplies.”

4. Some basic definitions (1) Energy… modern sense of this word appeared in the 1800’s :  Described transfer of heat  Motion of planets  Operation of machinery  Flow of electricity

5. Some basic definitions (2) TODAY… Energy = capacity to do work. That is, to move an object against a resisting force  Unit --- Joules Power = the rate of doing work or rate at which energy is converted from one form to of energy to another  Unit -- Watts = Joules/second

6. Some basic definitions (3) What about sustainable? Word introduced by the UN report “Our Common Future” Brundtland Commission in 1987 sustainable = development that meets the needs of the present without compromising the ability of future generations to meet their own needs

7. Some basic definitions (4) Sustainable energy sources means:  that are not substantially depleted by continues use;  the use of which does not entail the emission of pollutants or other hazards to the environment on a substantial scale; and  the use of which does not involve the perpetuation of substantial health hazards or social injustices. P.S. Others prefer the emphasize renewable energy instead

8. Energy Sources Fossil Fuels –Coal –Oil –Natural gas Nuclear energy –Fission –Fusion Bioenergy –Burning wood –Animal dung –Wastes –Alcohol (ethanol) Gasohol Hydroelectric Solar energy Wind energy Wave power Tidal energy Geothermal –Earth internal heat originates mainly from the decay of long lived radioactive elements

9. % contributions of energy sources to world’s consumption (2000)

10. Why bother to learn about this now? Problems with current energy producing fuels It is hypothesized that by 2050 we will have run out of economically recoverable fossil fuels

11. Growing Population

12. No More Fossil Fuel? Need For New Energy Sources If we continue to burn fossil fuels for energy, they will only last another few hundred years. This means that an energy shortfall could occur within the next fifty years.

13. Some basic facts about Fossil Fuels –Coal –Oil –Natural gas  75% of our current source of energy

14. Coal Abundant Burns dirty Causes acid rain and air pollution –Greenhouse gas problems

15. Oil Flexible fuel source with many derivatives Transportable Finite supply Causes air pollution

16. Natural Gas Burns cleanly Transportable Finite supply Dangerous to handle

17. Nuclear Power (7%) Clean No CO 2 No immediate pollution Problems with waste disposal Safety concerns

18. Other Alternative Sources (18%) Water Power Solar Power Tidal Power Wind Power Geothermal Power 20% of the energy needed for an estimated world population of 10 Billion in 2050 WHY?

19. We need to look at each source in more detailed

20. Few comments about... Nuclear Fusion

21. Introduction “Every time you look up at the sky, every one of those points of light is a reminder that fusion power is extractable from hydrogen and other light elements” -Carl Sagan, 1991

22. Our Sun

23. Fusion Advantages Abundant fuel, available to all nations –Deuterium and lithium easily available for thousands of years Environmental Advantages –No carbon emissions, short-lived radioactivity Modest land usage –Compact relative to solar, wind and biomass Can’t blow up –Resistant to terrorist attack –Less than 5 minutes of fuel in the chamber Not subject to daily, seasonal or regional weather variation –No large-scale energy storage nor long-distance transmission Can produce electricity and hydrogen –Compliments other nearer-term energy sources

24. Fusion Disadvantages Huge research and development costs Radioactivity

25. Background Fusion Basics

26. Basic Physics

27. Energy-Releasing Reactions ChemicalFissionFusion Sample Reaction C + O 2  CO 2 n + 235 U  143 Ba + 91 Kr + 2 n 2 H + 3 H  4 He + n Typical Inputs (to Power Plant) Bituminous CoalUO 2 (3% 235 U+ 97% 238 U)Deuterium & Lithium Typical Reaction Temp. (K) 700100010 8 Energy Released per kg of Fuel (J/kg) 3.3 x 10 7 2.1 x 10 12 3.4 x 10 14

28. What is an atom?

29. Nuclear Power Nuclear fission –Where heavy atoms, such as uranium, are split apart releasing energy that holds the atom together Nuclear fusion –Where light atoms, such as hydrogen, are joined together to release energy

30. States of Matter Plasma is sometimes referred to as the fourth state of matter

31. Plasma makes up the sun and the stars

32. Plasma Atoms In plasma the electrons are stripped away from the nucleus Like charges repel –Examples of plasma on earth: Fluorescent lights Lightning Neon signs

33. Other Typical Plasmas Interstellar Solar Corona Thermonuclear Laser

34. Characteristics of Typical Plasmas

35. Basic Characteristics Particles are charged Conducts electricity Can be constrained magnetically

36. Fusion Fuel Tritium Deuterium

37. The fuel of fusion

38. Inexhaustible Energy Supply Deuterium –Constitutes a small percentage of the hydrogen in water Separated by electrolysis 1 barrel (42 gallons) water  ¾ oz. Tritium –n + Li T + He –Lithium is plentiful Earth’s crust Oceans –Savannah, Georgia –Canada, Europe, Japan

39. Fusion Fuel: Deuterium

40. Other Possible Fusion Fuels Helium-3 Nuclear Fusion Proton NeutronProton

41. Where is Helium-3? Helium-3 comes to us from the sun on the solar wind It cannot penetrate the magnetic field around the earth, so it eventually lands on the moon One shuttle load- 25 tons- would supply the U.S. with enough fuel for one year

42. HOW FUSION REACTIONS WORK

43. Two Main Types of Fusion Reactions: P-P "P-P": Solar Fusion Chain

44. Two Main Types of Fusion Reactions: D-T D + T => 4 He + n

45. More on Fusion Reactions

47. An enormous payoff The fraction of “lost” mass when H fuses into He is 38 parts out of 10,000 This lost mass is converted into energy The energy released from 1 gram of DT = the energy from about 2400 gallons of oil

49. The result Inexhaustible fuel source –Seawater & Lithium The MOST “bang for your buck” Inexpensive to produce Widely distributed fuel source –No wars No pollution –Helium is not polluting Fuel that is non-radioactive –Residue Helium-4 is non-radioactive Waste reduction

50. More of Fusion Radioactivity Stray Tritium –Relatively benign Doesn’t emit strong radioactivity when it decays –So only dangerous when ingested or inhaled Shows up in one’s body as water –Easily and frequently flushed out Half-life of 12 years –No long-term waste problem –Won’t decay while in one’s body –Less than natural exposure to radon, cosmic rays and much less than man-made x-rays

51. More on Fusion Radioactivity Reactor Structure –Development of special “low-activation” structural materials Vanadium Silicon-carbide –Wait ten to fifteen years after shutdown The reactor will be less radioactive than some natural materials (particularly uranium ores) Recycle into a new fusion reactor

52. Waste Reduction Power Source Total Waste (m3) High-Level RAD Waste Coal 10,000 (ashes) 0 Fission 440 120 Fusion: Today’s Materials 2000 30 Advanced Materials 2000 0

53. So why aren’t fusion plants already in operation? How fusion works and the obstacles in the way

54. The Problems Harnessing the Energy Achieving & sustaining high temperatures –The reaction takes place at a temperature hotter than the surface of the sun –0.1 seconds Containing the fuel & the reaction Money for research and development

55. Harnessing the Energy

56. Achieving ignition temperatures 45