Energy Systems & Sustainability Freshman Seminar 2013 Mayda M. Velasco Oct. 1, 2013.

Slides:



Advertisements
Similar presentations
Transmutations involve more than just the conversion of one element into another—they also involve the conversion of mass into energy. Nuclear energy released.
Advertisements

Nuclear Reactions, Transmutations, Fission and Fusion
Nuclear Reactions: AN INTRODUCTION TO FISSION & FUSION Farley Visitors Center.
Nuclear Physics Notes CP Physics Ms. Morrison.
NUCLEAR ENERGY PRESENT BY:OLUWATOBI BAKARE :LUMANA HALAN BAYARO.
Atomic Energy 3U Physics. Mass-Energy Equivalence All matter is a form of stored energy.
Chapter 13 Nuclear Reactions.
Nuclear Chemistry Unstable Nuclei and Radioactive Decay.
Nuclear Physics Year 13 Option 2006 Part 2 – Nuclear Fusion.
Power of the Sun. Conditions at the Sun’s core are extreme –temperature is 15.6 million Kelvin –pressure is 250 billion atmospheres The Sun’s energy out.
Nuclear Energy Fission and Fusion
23.4 Nuclear energy NUCLEARNUCLEAR POWERPOWER Millstone Station.
23.4 Nuclear energy NUCLEARNUCLEAR POWERPOWER Millstone Station.
Nuclear Reactions.
Chapter 40 Nuclear Fission & Fusion
Nuclear Fusion The Possibility Introduction “Every time you look up at the sky, every one of those points of light is a reminder that fusion power is.
Section 10–4: Fission and Fusion
1 X - Nuclear 2 Stability of isotopes is based on the ratio of neutrons and protons in its nucleus. Although most nuclei are stable, some are unstable.
Nuclear Fusion - SAMI Introduction “Every time you look up at the sky, every one of those points of light is a reminder that fusion power is extractable.
Nuclear Fusion Katharine Harrison. Why Are We Interested? There are great challenges that are associated with fusion, but there are also very large possible.
Radioisotope: an unstable isotope that spontaneously changes its nuclear structure and releases energy in the form of radiation. Isotopes Stable Radioisotopes.
Energy Systems & Sustainability Freshman Seminar 2008.
40 Nuclear Fission and Fusion After fusion, the total mass of the light nuclei formed in the fusion process is less than the total mass of the nuclei that.
Nuclear Fusion Reactors
Nuclear Chemistry.
Nuclear Reactions Dr. G. Maynes Illustrations from Brown, LeMay and Bursten.
The energy of future. World’s reserves of fuel are going to be exhausted in about 50 years. It’s also predicted that the gas and the coal resources will.
Nuclear Symbols Element symbol Mass number (p + + n o ) Atomic number (number of p + )
For each atom, in its natural state, the number of electrons and the number of protons is equal. This number may or may not be the same as the number.
Nuclear Power. Locations of Nuclear Power plants in the US.
1 Nuclear Changes Physical Science Chapter Radioactive decay  The spontaneous breaking down of a nucleus into a slightly lighter nucleus, accompanied.
Radiation. Atomic Anatomy Atoms –electrons (e-) –protons (p+) –neutrons (n)
Fission Lise Meitner- Austrian physicist during time of WWII. Discovered that bombardment of uranium with neutrons can split the nucleus into two pieces.
Nuclear Energy. A. What does radioactive mean? 1. Radioactive materials have unstable nuclei, which go through changes by emitting particles or releasing.
Fundamental Forces of the Universe. There are four fundamental forces, or interactions in nature.  Strong nuclear  Electromagnetic  Weak nuclear 
Fusion: Basic Principles, Current Progress and ITER Plans
Section 1Nuclear Changes Section 1: What is Radioactivity?
Fusion in the Stars Nunez & Panogalinog. Nuclear Fusion in stars is one of the most important reasons which make life on Earth possible! ○ HOW IS THAT.
Chapter 16 notes.
Neeraj Dhiman. DEFINITION Nuclear physics is the field of physics that studies the building blocks and interactions of atomic nuclei.
Radioactivity Nucleus – center of the atom containing protons and neutrons –How are the protons and neutrons held together? Strong Force - an attractive.
Presented by: - POOJA SHRESTHA What is Fusion? When two light nuclei fuse together to form heavy nucleus, the process is known as Fusion. When two light.
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Essential Questions 1)Identify four types of nuclear radiations and compare and contrast their properties.
Chapter 10 Nuclear Chemistry.
1 Clip. 1. Differentiate among alpha and beta particles and gamma radiation. 2. Differentiate between fission and fusion. 3. Explain the process half-life.
Nuclear Reactions: FISSION & FUSION ã Nuclear reactions deal with interactions between the nuclei of atoms ã Both fission and fusion processes deal with.
Chapter 10 Fission and Fusion. Fission The splitting of an atomic nucleus into smaller parts. Huge amounts of energy can be produced from a very small.
Chapter 9 Book Nuclear Changes #20. I. Nuclear Radiation Radioactivity – Nucleus emits one or more particles – Unstable nuclei Unstable – Nuclei has to.
The mass of the nuclei produced is less than the mass of the original two nuclei The mass deficit is changed into energy We can calculate the energy released.
1. What is radioactivity? Radioactivity is the process in which an unstable atomic nucleus emits charged particles and energy. 2. What is a radioisotope?
Nuclear fission Nuclear fission: heavy nuclei split into two smaller parts in order to become more stable proton neutron Kr-90 nucleus U-235 nucleus energy.
The Atomic Nucleus & Radioactive Decay (Chapter 10)
Ch. 28 Nuclear Chemistry C. Smith. I. Nuclear Radiation A. Radioactivity 1. Radioisotopes are unstable isotopes that have unstable nuclei. 2. They gain.
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Nuclear Radiation Strong Nuclear force – the force that holds protons and neutrons together. Remember that.
Nuclear Power Ps 5c: I will compare and contrast Fission and Fusion.
Nuclear Fission and Fusion. Nuclear Reactions Nuclear reactions deal with interactions between the nuclei of atoms Both fission and fusion processes deal.
Nuclear Energy Britney Chance Dusty Ely Roland 8 th Grade Science Mrs. Miller.
MEASURING RADIATION Large doses of radiation are harmful to living tissue. Radiation can be measured with a Geiger counter – a device that measures radioactivity.
Integrated Science C Mrs. Brostrom. Describe the availability, current uses and environmental issues related to the use of fossil and nuclear fuels to.
Nuclear Radiation NC Essential Standard Types of Radiation, Penetrating Ability of Radiation, Nuclear Equations, Nuclear Decay, Half-Life, Fission.
Nuclear Fusion Katharine Harrison.
The Atomic Nucleus & Radioactive Decay
The Atomic Nucleus & Radioactive Decay
Nuclear Energy – Learning Outcomes
MEASURING RADIATION Large doses of radiation are harmful to living tissue. Radiation can be measured with a Geiger counter – a device that measures radioactivity.
Nuclear Reactions.
Unit 5.4 Nuclear Fission and Fusion
Nuclear Fusion vs. Nuclear Fission
Fission and Fusion Chp 24.
Nuclear Fusion vs. Nuclear Fission
Presentation transcript:

Energy Systems & Sustainability Freshman Seminar 2013 Mayda M. Velasco Oct. 1, 2013

Few comments about... Nuclear Fusion

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

Our Sun

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

Fusion Disadvantages Huge research and development costs Radioactivity

Background Fusion Basics

Energy-Releasing Reactions ChemicalFissionFusion Sample Reaction C + O 2  CO 2 n 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) Energy Released per kg of Fuel (J/kg) 3.3 x x x 10 14

What is an atom?

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

Fusion process

Stability Band – Lifetime  Radioactive waste

Nuclear Binding Energy Fusion favored Fission favored

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

Plasma makes up the sun and the stars

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

Other Typical Plasmas Interstellar Solar Corona Thermonuclear Laser

Characteristics of Typical Plasmas

Basic Characteristics Particles are charged Conducts electricity Can be constrained magnetically

Fusion Fuel Tritium Deuterium

The fuel of fusion

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

Fusion Fuel: Deuterium

Other Possible Fusion Fuels: Helium-3 Nuclear Fusion Proton NeutronProton

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

HOW FUSION REACTIONS WORK?

Two Main Types of Fusion Reactions: #1 = Proton-Proton "P-P": Solar Fusion Chain

Two Main Types of Fusion Reactions: #2 = D-T D + T  4 He + n

More on Fusion Reactions

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

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

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

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

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

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

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

Harnessing the Energy

Achieving ignition temperatures 45