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Section 2 Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas • Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

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Page 1: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Section 2: Nuclear Fission and Fusion

Preview• Key Ideas• Bellringer• Nuclear Forces• Nuclear Fission• Chain Reaction• Nuclear Fusion

Page 2: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Key Ideas

〉What holds the nuclei of atoms together?

〉What is released when the nucleus of a heavy atom is split?

〉What happens when the nuclei of small atoms are joined?

Page 3: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Bellringer

In your study of chemical reactions, you learned that one convenient way to classify reactions was as synthesis or decomposition. In synthesis reactions, the products are larger and more complex than the reactants. In decomposition reactions, the opposite is true.

In some situations, nuclear reactions can occur. These reactions can also be categorized by how the product nuclei compare to the reactant nuclei. Study the models of the nuclei shown on the next slide, and answer the following questions.

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Section 2Nuclear Changes

Bellringer, continued

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Bellringer, continued

1. In which of the diagrams did a complex nucleus form simpler nuclei?

2. In which of the diagrams did simple nuclei combine to form a complex nucleus?

3. Each year, scientists around the world attempt to “discover” new elements using nuclear reactions. Which of the reactions shown in the diagrams above most likely would be useful for this type of research? Explain your answer.

Page 6: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

SPS3.b Differentiate between fission and fusion.

Page 7: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

EQ: How do fission and fusion differ?

Page 8: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Nuclear Forces

What holds the nuclei of atoms together?

Page 9: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-1 Nuclear Forces

The stability of a nucleus depends on the nuclear forces that act between protons and neutorons and hold the nucleus together.

Page 10: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-2 Nuclear Forces, continued

• strong nuclear force: causes protons and neutrons in the nucleus to attract each other

Page 11: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

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10-2-3 Nuclear Forces, continued

• Neutrons contribute to nuclear stability.

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10-2-4 Nuclear Forces, continued

Nuclei with more than 83 protons are always unstable.

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Section 2Nuclear Changes

Nuclear Forces, continued

Page 14: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Nuclear Fission

What is released when the nucleus of a heavy atom is split?

Page 15: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-5 Nuclear Fission

• fission: the process by which a nucleus splits into two or more fragments and releases neutrons and energy

Page 16: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-6 Nuclear Fission, continued

• Fission of Uranium-235: 235 1 140 93 1

92 0 56 36 0U n Ba Kr 3 n energy

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Section 2Nuclear Changes

10-2-7 Nuclear Fission, continued

• According to Einstein’s equation, E = mc2 , mass is converted to energy in a fission reaction.

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10-2-8 Nuclear Fission, continued

–mass defect: the difference in the total measured mass of a nucleus and the sum of the individual masses of the neutrons and protons that make up the nucleus

Page 19: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-9 Nuclear Fission, continued

The mass defect is the amount of mass that has been changed to energy.

Page 20: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-9 Nuclear Fission, continued

–nuclear chain reaction: a continuous series of nuclear fission reactions caused by the release of electrons

Page 21: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

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10-2-10 Nuclear Fission, continued

–critical mass: the minimum mass of a fissionable isotope that provides the number of neutrons needed to sustain a chain reaction

Page 22: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Chain Reaction

Page 23: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

Nuclear Fusion

What happens when the nuclei of small atoms are joined?

Page 24: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-11 Nuclear Fusion

• fusion: the process in which light nuclei combine at extremely high temperatures, forming heavier nuclei and releasing energy

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10-2-12 Nuclear Fusion, continued

• In stars, energy is produced when hydrogen nuclei combine.

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10-2-13 Nuclear Fusion, continued

A large amount of energy and a very high temperature is needed to start a fusion reaction.

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Section 2Nuclear Changes

10-2-14 Nuclear Fusion, continued

Four hydrogen atoms combine to make a helium atom and high-energy gamma rays in a three-step process.

1 1 21 1 1

2 1 3 01 1 2 0

3 3 4 1 12 2 2 1 1

H H H other particles

H H He

He He He H H

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Section 2Nuclear Changes

10-2-15 Nuclear Fusion, continued

Fusion reactions are not practical now because of the difficulty of containing such a high temperature reaction.

Page 29: Section 2Nuclear Changes Section 2: Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2Nuclear Changes

10-2-16 Nuclear Fusion, continued

Two big advantages of fusion are they produce more energy than fission and they don’t make hazardous wastes.

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Section 2Nuclear Changes

Nuclear Fusion, continued