Fission & Fusion.

Slides:



Advertisements
Similar presentations
Nuclear Fission and Fusion
Advertisements

Radioactivity and Nuclear Reactions
Fission & Fusion. Forces What holds an atom together? Why doesn’t the nucleus of an atom fly apart if it’s made of positively charged protons?
UNIT FOUR: Matter and its Changes  Chapter 12 Atoms and the Periodic Table  Chapter 13 Compounds  Chapter 14 Changes in Matter  Chapter 15 Chemical.
Integrated Science Chapter 25 Notes
 What is the mole and how does it relate to Avagadro’s number. How many atoms are in 2 moles of NaCl. Explain with complete sentences and show any calculations.
Objective  I will be able to identify and compare the difference between fission and fusion reactions and cite specific examples of how they are used.
1 Nuclear Changes Physical Science Chapter Radioactive decay  The spontaneous breaking down of a nucleus into a slightly lighter nucleus, accompanied.
Three Types of Atomic Nuclear Changes
Nuclear Energy. A. What does radioactive mean? 1. Radioactive materials have unstable nuclei, which go through changes by emitting particles or releasing.
Radioactivity Nucleus – center of the atom containing protons and neutrons –How are the protons and neutrons held together? Strong Force - an attractive.
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Essential Questions 1)Identify four types of nuclear radiations and compare and contrast their properties.
Nuclear Chemistry. Nuclear Chemistry looks at the number of protons and neutrons in an atom Radioactive Decay = Spontaneous disintegration of a nucleus.
Nuclear Chemistry. ATOMIC REVIEW: Atomic number = # of protons # of neutrons = mass # - atomic # protons & neutrons are in the nucleus.
Fission & Fusion. Forces What holds an atom together? Why doesn’t the nucleus of an atom fly apart if it’s made of positively charged protons?
Chapter 9 Book Nuclear Changes #20. I. Nuclear Radiation Radioactivity – Nucleus emits one or more particles – Unstable nuclei Unstable – Nuclei has to.
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Nuclear Radiation Strong Nuclear force – the force that holds protons and neutrons together. Remember that.
 In nuclear fission, large atoms are split apart to form smaller atoms, releasing energy.  Fission also produces new neutrons when an atom splits. 
Fission and Fusion. Nuclear Reactions Two types of nuclear reactions that release energy.  Fission  Fusion.
Nuclear Chemistry and Radioactivity Unit 13 Notes.
Nuclear Chemistry. Radioactivity  Radioisotopes – isotopes that are unstable, who’s nucleus undergoes changes to gain stability  Radiation – the penetration.
1) How is the mass number calculated (2).
Fission & Fusion.
Unit 4 Lesson 3 Nuclear Reactions
Radioactivity Clip.
Radioactivity Nucleus – center of the atom containing protons and neutrons How are the protons and neutrons held together? Strong Force - an attractive.
Radioactivity Clip.
Chapter 9.2 Nuclear Radiation.
Chapter 9 – Radioactivity and Nuclear Reactions
Chapter 19 Radioactivity
Unit 4 Lesson 3 Nuclear Reactions
Physical Science Honors
Radioactivity Clip.
The Atomic Nucleus.
Radioactivity.
E = mc2 If you can’t explain it simply, you haven’t learned it well enough. Einstein.
Chain Reactions Chain Reaction - the series of repeated fission reactions caused by the release of neutrons in each reaction.
Nuclear Reactions.
Nuclear Chemistry Physical Science.
14.4 Chemical vs. Nuclear Reactions
Nuclear Chemistry.
Radioactivity Clip.
Radioactivity Clip.
Radioactivity.
RADIOACTIVITY SPS4. Obtain, evaluate, and communicate information to explain the changes in nuclear structure as a result of fission, fusion and radioactive.
Nuclear Decay Song on Youtube
Nuclear Chemistry.
5.2 - Nuclear Chemistry.
Chapter 16 Nuclear Energy
Chapter 16 Radioactivity.
What is a nuclear reaction?
NUCLEAR CHEMISTRY NUCLEONS – The particles found in the nucleus
Unit 4 Lesson 3 Nuclear Reactions
Radioactivity.
Nuclear Decay.
Radioactivity.
Chapter 14.4 Learning Goals
Radioactivity Clip.
Nuclear Chemistry Chapter 21.
Fission & Fusion.
Fundamental Forces of the Universe
Unit 4 – Nuclear Reactions
Nuclear Radiation.
Three kinds of particle emission
Nuclear Chemistry Bravo – 15,000 kilotons.
Should New Zealand remain ‘nuclear power’ free?
Nuclear Chemistry Vocabulary.
Nuclear Energy Nuclear Structure and Radioactivity.
Presentation transcript:

Fission & Fusion

Radioactive Elements Any element over atomic number 83 is radioactive. Radioactive materials have unstable nuclei (too few or too many neutrons). When an unstable nucleus decays, it breaks apart emitting particles and energy as it decays. Three types of nuclear radiation: Alpha particles Beta particles Gamma radiation electromagnetic wave

Fission The process used to release nuclear energy by splitting nuclei is called fission. + ENERGY

What nuclei can split during nuclear fission? Only large nuclei like U or plutonium can split apart during nuclear fission. Click on image for animation

What nuclei can split during nuclear fission?                                                U-236 is so unstable that it immediately splits into barium & krypton nuclei, several neutrons & a large amount of energy

Chain Reaction Free neutrons produced by fission can hit other nuclei emitting more neutrons repeating the reaction over and over. A series of fission reactions is called a chain reaction. Can only be slowed by using materials that will absorb the neutrons.

Chain Reaction An uncontrolled chain reaction releases a huge amount of energy in a short time & requires a critical mass of starting material to produce more reactions.

Fusion The sun is powered by nuclear fusion. In a nuclear fusion reaction, two small, light nuclei combine to form one larger, heavier nucleus. Two hydrogen atoms combine under extreme heat and pressure to form a helium atom. (H-2 + H-2→He-4)

Fusion Why would we want to use the fusion reaction in a nuclear power plant? 1. Hydrogen is the most common element in the universe. 2. Could meet energy demands for millions of years

How are temperature & fusion related? How can two nuclei get close enough to combine? They must be moving very fast. All nuclei positively charged Thus repel each other KE must overcome electric force to push them close enough to combine KE increases as temperature increases Temp must be millions of °C like Sun & other stars

How does the Sun produce energy? The Sun, made mostly of H produces its energy by fusion of H nuclei 2 protons (H-1) fuse to make a H isotope (H-2); then H-1 + H-2 form an isotope of He-3. positron Light light neutrino The emission of a positron or a positive electron is referred to as beta decay. The positron is accompanied by a neutrino, a massless and chargeless particle. Positrons are emitted with the same kind of energy spectrum as electrons in negative beta decay because of the emission of the neutrino.

How does the Sun produce energy? To complete the process, 4 H nuclei combine into 1 He nucleus during which a small amount of matter changes into a huge amount of energy.

Fusion on the Sun The heat & light Earth receives comes from this process. About 1% of the Sun’s hydrogen has been changed into energy. Sun has enough H to continue fusion reactions for another 5 billion years.

Fusion vs. Fission Comparison Chart Fission vs. Fission

Radiation Background radiation can come from Sun Water Plants ***Radon is the largest source of radiation in the earth’s crust.***

Radiation Damage Mutate hemoglobin Mutate cells, lose function Destroy immune system Burn skin, destroy bone

Radioactive Tracer What is a radioactive tracer? - short lived isotope that can be observed with a sensitive detector

Radioactive Tracer How are they used? - Agriculture – measure water flow - Medicine – locate tumors - Medical research – trace drug paths thru body - Geology – trace underground water flow