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Page 1: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic EnergyAtomic EnergyAtomic EnergyAtomic Energy

Page 2: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

AgendaAgenda

Atomic EnergyAtomic EnergyWarm-up:

What do you know about radiation?

Homework: Reread pages 80-87.

OBJ 1: Compare alpha, beta, and gamma decay

Atomic EnergyAtomic EnergyWarm-up:

What do you know about radiation?

Homework: Reread pages 80-87.

OBJ 1: Compare alpha, beta, and gamma decay

1.What do you know about radiation?2.Intro to atomic

energy3.Let’s read up on

it!4.Watch your “headsium”.

5.Alpha, Beta, Gamma6.Project

1.What do you know about radiation?2.Intro to atomic

energy3.Let’s read up on

it!4.Watch your “headsium”.

5.Alpha, Beta, Gamma6.Project

Page 4: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Nuclear Radiation Nuclear Radiation

high-energy particles and rays that are emitted by the nuclei of some atoms

radioactivity: the ability to give off nuclear radiation

high-energy particles and rays that are emitted by the nuclei of some atoms

radioactivity: the ability to give off nuclear radiation

Page 5: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

History!!History!!

• http://www.neok12.com/Nuclear-Power.htm• http://www.neok12.com/Nuclear-Power.htm

Page 6: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

3 different types of radiation. 3 different types of radiation.

Page 7: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Nuclear radiation is produced through decay

Nuclear radiation is produced through decay

Radioactive decay- the process in which the nucleus of a radioactive atom releases nuclear radiation

3 types of decay:

alpha

beta

gamma

Radioactive decay- the process in which the nucleus of a radioactive atom releases nuclear radiation

3 types of decay:

alpha

beta

gamma

Page 8: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Alpha DecayAlpha Decay

• Release of an alpha particle from a nucleus

• Alpha particle = 2 protons and 2 neutrons; has a mass of 4 and charge of 2+ (is identical to nucleus of a helium atom) *Large radioactive nuclei give off alpha particles to become nuclei of atoms of different elements.

• Release of an alpha particle from a nucleus

• Alpha particle = 2 protons and 2 neutrons; has a mass of 4 and charge of 2+ (is identical to nucleus of a helium atom) *Large radioactive nuclei give off alpha particles to become nuclei of atoms of different elements.

Page 9: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

ReminderReminder

mass number = ___ + ___ mass number = ___ + ___

Page 10: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Radium - 226Radium - 226

atomic number =

proton number =

neutron number =

electron number =

atomic number =

proton number =

neutron number =

electron number =

Page 11: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

ConservationConservation

sum of mass number of starting material = sum of mass number of products

charge is conserved . . .sum of charges of starting is always equal to sum of charges of products

sum of mass number of starting material = sum of mass number of products

charge is conserved . . .sum of charges of starting is always equal to sum of charges of products

Page 12: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Radium-226 undergoes alpha decay

Radium-226 undergoes alpha decay

Radium 226 ----> Radon 222

Charge 88+ ----> Charge 86+

Radium 226 ----> Radon 222

Charge 88+ ----> Charge 86+

He - 4He - 4Charge- 2+ Charge- 2+

the decay the decay into 2 products into 2 products

Page 13: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• Americium- Atomic Number : 95

• Neptunium- Atomic Number: 93

• Alpha Particle: 2 protons & 2 neutrons

• Americium- Atomic Number : 95

• Neptunium- Atomic Number: 93

• Alpha Particle: 2 protons & 2 neutrons

Page 14: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Beta DecayBeta Decay

• Release of a beta particle from a nucleus.

• Beta particle = an electron (having a charge of 1- and mass of almost 0) OR a positron (having a charge of 1+ and a mass of almost 0). *Because electrons and positrons do

NOT contain protons or neutrons, mass number is 0.

• Release of a beta particle from a nucleus.

• Beta particle = an electron (having a charge of 1- and mass of almost 0) OR a positron (having a charge of 1+ and a mass of almost 0). *Because electrons and positrons do

NOT contain protons or neutrons, mass number is 0.

Page 15: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

two types of beta decaytwo types of beta decay

A proton breaks down into a positron (1+) & a neutron

Neutron breaks down into a proton & an electron

So if there’s 1 more proton in the nucleus…

A proton breaks down into a positron (1+) & a neutron

Neutron breaks down into a proton & an electron

So if there’s 1 more proton in the nucleus…

Page 16: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• Beta decay occurs when the neutron to proton ratio is too great in the nucleus and causes instability. In basic beta decay, a neutron is turned into a proton and an electron. The electron is then emitted. Here's a diagram of beta decay with hydrogen-3:

• (taken from http://library.thinkquest.org/3471/radiation_types_body.html)

• Beta decay occurs when the neutron to proton ratio is too great in the nucleus and causes instability. In basic beta decay, a neutron is turned into a proton and an electron. The electron is then emitted. Here's a diagram of beta decay with hydrogen-3:

• (taken from http://library.thinkquest.org/3471/radiation_types_body.html)

Page 17: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• There is also positron emission when the neutron to proton ratio is too small. A proton turns into a neutron and a positron and the postiron is emitted. A positron is basically a positively charged electron. Here's a diagram of positron emission with carbon-11:

• There is also positron emission when the neutron to proton ratio is too small. A proton turns into a neutron and a positron and the postiron is emitted. A positron is basically a positively charged electron. Here's a diagram of positron emission with carbon-11:

Page 18: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Gamma DecayGamma Decay

• Release of gamma rays from a nucleus. Occurs after alpha or beta decay as particles shift in nucleus to a more stable position. *Gamma rays alone do not cause one element to change into another.

• Release of gamma rays from a nucleus. Occurs after alpha or beta decay as particles shift in nucleus to a more stable position. *Gamma rays alone do not cause one element to change into another.

Page 19: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Gamma DecayGamma Decay

• The release of gamma rays from the nucleus

• Energy that is released during alpha or beta decay in the form of gamma rays

• No mass

• No charge

• Does not cause 1 element to change into another like alpha & beta

• The release of gamma rays from the nucleus

• Energy that is released during alpha or beta decay in the form of gamma rays

• No mass

• No charge

• Does not cause 1 element to change into another like alpha & beta

Page 20: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Watch Your “Headsium”Watch Your “Headsium”

page 79 in book.

follow the instructions.

you will need graph paper

page 79 in book.

follow the instructions.

you will need graph paper

Page 21: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Please copy the following

Please copy the following

Trials Number of “headsium” nuclei remaining

0 100

1

2

3

4

5

6

7

8

Page 22: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic EnergyAtomic Energy•OBJ 1: Compare alpha, beta, and gamma decay.

•OBJ 2: Describe the penetrating power of the 3 types of nuclear radiation.

•OBJ 3: Identify uses of radiation.

•Warm-up: Take several minutes and complete the Section Review on page 84.

•Homework: Read and take notes on pages 84-87.

Atomic EnergyAtomic Energy•OBJ 1: Compare alpha, beta, and gamma decay.

•OBJ 2: Describe the penetrating power of the 3 types of nuclear radiation.

•OBJ 3: Identify uses of radiation.

•Warm-up: Take several minutes and complete the Section Review on page 84.

•Homework: Read and take notes on pages 84-87.

Agenda

1. Let’s watch!

2. Gamma decay

3. Watch your “headsium”.

Agenda

1. Let’s watch!

2. Gamma decay

3. Watch your “headsium”.

Page 23: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

3 different types of radiation: What does this mean? 3 different types of radiation: What does this mean?

Page 24: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Alpha (α): could barely pass through a single sheet of paper. Deflected as a positive particle in a magnetic field.

Beta (β): can pass through about 3mm of aluminum. Deflected as a negative particle in a magnetic field.

Gamma (γ): can pass through several centimeters of LEAD! Not deflected in a magnetic field.

Page 25: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Some more history!Some more history!Some more history!Some more history!• Wilhelm Conrad Roentgen (1845-1923) Drawn to a glowing fluorescent screen on a nearby table. He determined that the fluorescence was caused by invisible rays originating from the partially evacuated glass tube he was using to study cathode rays (i.e., electrons). Surprisingly, these mysterious rays penetrated the opaque black paper wrapped around the tube. Roentgen had discovered X rays!

• Antoine Henri Becquerel (1852-1908) Becquerel chose to work with was potassium uranyl sulfate,, which he exposed to sunlight and placed on photographic plates wrapped in black paper. When developed, the plates revealed an image of the uranium crystals. Becquerel initially concluded "that the phosphorescent substance in question emits radiation which penetrates paper opaque to light.“ He believed this was due to the presence of the sun's energy which was being absorbed by the uranium which then emitted X rays. Further investigation, revealed that X rays were emitted without the presence of the sun. Thus Becquerel had discovered radioactivity, the spontaneous emission of radiation by a material.

• Wilhelm Conrad Roentgen (1845-1923) Drawn to a glowing fluorescent screen on a nearby table. He determined that the fluorescence was caused by invisible rays originating from the partially evacuated glass tube he was using to study cathode rays (i.e., electrons). Surprisingly, these mysterious rays penetrated the opaque black paper wrapped around the tube. Roentgen had discovered X rays!

• Antoine Henri Becquerel (1852-1908) Becquerel chose to work with was potassium uranyl sulfate,, which he exposed to sunlight and placed on photographic plates wrapped in black paper. When developed, the plates revealed an image of the uranium crystals. Becquerel initially concluded "that the phosphorescent substance in question emits radiation which penetrates paper opaque to light.“ He believed this was due to the presence of the sun's energy which was being absorbed by the uranium which then emitted X rays. Further investigation, revealed that X rays were emitted without the presence of the sun. Thus Becquerel had discovered radioactivity, the spontaneous emission of radiation by a material.

Page 26: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• Pierre Curie (1859-1906) Marie Curie (1867-1934) Together, they began investigating the phenomenon of radioactivity recently discovered in uranium ore. Although the phenomenon was discovered by Henri Becquerel, the term radioactivity was coined by Marie. After chemical extraction of uranium from the ore, Marie noted the residual material to be more "active" than the pure uranium. She concluded that the ore contained, in addition to uranium, new elements that were also radioactive. This led to their discoveries of the elements of polonium and radium, but it took four more years of processing tons of ore under oppressive conditions to isolate enough of each element to determine its chemical properties.

• Ernest Rutherford (1871-1937) Named and characterized the alpha particle, beta particle and proton. Even the neutron, discovered by James Chadwick, owes its name to Rutherford. The exponential equation used to calculate the decay of radioactive substances was first employed for that purpose by Rutherford and he was the first to elucidate the related concepts of the half-life and decay constant. With Frederick Soddy at McGill University, Rutherford showed that elements such as uranium and thorium became different elements (i.e., transmuted) through the process of radioactive decay.

• Pierre Curie (1859-1906) Marie Curie (1867-1934) Together, they began investigating the phenomenon of radioactivity recently discovered in uranium ore. Although the phenomenon was discovered by Henri Becquerel, the term radioactivity was coined by Marie. After chemical extraction of uranium from the ore, Marie noted the residual material to be more "active" than the pure uranium. She concluded that the ore contained, in addition to uranium, new elements that were also radioactive. This led to their discoveries of the elements of polonium and radium, but it took four more years of processing tons of ore under oppressive conditions to isolate enough of each element to determine its chemical properties.

• Ernest Rutherford (1871-1937) Named and characterized the alpha particle, beta particle and proton. Even the neutron, discovered by James Chadwick, owes its name to Rutherford. The exponential equation used to calculate the decay of radioactive substances was first employed for that purpose by Rutherford and he was the first to elucidate the related concepts of the half-life and decay constant. With Frederick Soddy at McGill University, Rutherford showed that elements such as uranium and thorium became different elements (i.e., transmuted) through the process of radioactive decay.

Page 27: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

A Closer LookA Closer Look

Page 28: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic EnergyAtomic Energy•OBJ 4: Calculate ages of objects using half-life.

•Warm-up: To determine the age of an antler which has one-fourth of its original carbon-14 unchanged, we must : multiply the number of half-lives that have passed by the length of the half life for that element (in this case 5,730 years). THUS: 2 x 5,730 yrs = 11,460 yrs.

YOUR TURN: what is the age of a spear containing one-eighth its original amount of carbon-14?

•Homework: Read and take notes on pages 88-94.

Atomic EnergyAtomic Energy•OBJ 4: Calculate ages of objects using half-life.

•Warm-up: To determine the age of an antler which has one-fourth of its original carbon-14 unchanged, we must : multiply the number of half-lives that have passed by the length of the half life for that element (in this case 5,730 years). THUS: 2 x 5,730 yrs = 11,460 yrs.

YOUR TURN: what is the age of a spear containing one-eighth its original amount of carbon-14?

•Homework: Read and take notes on pages 88-94.

Agenda

1. R. decay and Half-life

2. Watch your “headsium”

Agenda

1. R. decay and Half-life

2. Watch your “headsium”

Page 29: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Half-lifeHalf-life

• The amount of time it takes for one-half of the nuclei of a radioactive isotope to decay.

• The amount of time it takes for one-half of the nuclei of a radioactive isotope to decay.

Page 30: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Radium

0 1620

3240

6480 12960

25920

51840

% Remaining

100%

50% 25% 12.5%

6.25%

3.125%

1.56%

Iodine

% Remaining

100%

50% 25% 12.5%

6.25%

3.125%

1.56%

Uranium % Remaining

100%

50% 25% 12.5%

6.25%

3.125%

1.56%

Page 31: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Radioactive Decay & the Radioactive Decay & the Half-lifeHalf-life

Radioactive Decay & the Radioactive Decay & the Half-lifeHalf-life

• Using the information on page 86, answer the following questions:

1. A 20 g nitrogen-13 sample is prepared for an experiment. If a scientist begins the experiment 20 minutes later, how many grams of nitrogen-13 remain?

2. At the end of the experiment, if only 2.5 g of nitrogen-13 remain, how much time has passed from the time the sample was prepared?

3. Sodium-24 has a half-life of 15 hours. There are 5 grams of Sodium-24 at time 0. How long will it take to have 1.25 grams remaining?

• Handout

• Using the information on page 86, answer the following questions:

1. A 20 g nitrogen-13 sample is prepared for an experiment. If a scientist begins the experiment 20 minutes later, how many grams of nitrogen-13 remain?

2. At the end of the experiment, if only 2.5 g of nitrogen-13 remain, how much time has passed from the time the sample was prepared?

3. Sodium-24 has a half-life of 15 hours. There are 5 grams of Sodium-24 at time 0. How long will it take to have 1.25 grams remaining?

• Handout

Page 32: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Please copy the following

Please copy the following

Trials Number of “headsium” nuclei remaining

0 100

1

2

3

4

5

6

7

8

Take several minutes and complete the Section Review on page 87

Take several minutes and complete the Section Review on page 87

ConclusionConclusion

Page 33: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic EnergyAtomic Energy•OBJ 5: Understand the difference Understand the difference between nuclear fusion & fission. between nuclear fusion & fission.

•OBJ 6: Identify advantages and OBJ 6: Identify advantages and disadvantages of energy from the disadvantages of energy from the nucleus.nucleus.

•Warm-up: Complete the Section Review on page 93.

•Homework: Complete the Chapter Review on pg 98 #1-10 (this will be graded!) *Possible POP QUIZ next week!

Atomic EnergyAtomic Energy•OBJ 5: Understand the difference Understand the difference between nuclear fusion & fission. between nuclear fusion & fission.

•OBJ 6: Identify advantages and OBJ 6: Identify advantages and disadvantages of energy from the disadvantages of energy from the nucleus.nucleus.

•Warm-up: Complete the Section Review on page 93.

•Homework: Complete the Chapter Review on pg 98 #1-10 (this will be graded!) *Possible POP QUIZ next week!

Page 34: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

AgendaAgenda

• Finish QuickLab questions/ graph

• Finish worksheet

• Nuclear Fusion/Fission

• Finish QuickLab questions/ graph

• Finish worksheet

• Nuclear Fusion/Fission

Page 35: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• Nuclear Fission: when a large nucleus splits into two smaller nuclei with the release of energy

• Some nuclei can undergo fission naturally

• Hit with neutrons

• Chain reaction

• Nuclear Fission: when a large nucleus splits into two smaller nuclei with the release of energy

• Some nuclei can undergo fission naturally

• Hit with neutrons

• Chain reaction

Page 36: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• Nuclear Fusion: 2 or more nuclei with small masses join together to form a larger, more massive nucleus

• The repulsion of + + has to be overcome…only way is with high temps (100,000,000 degrees)

• Occurs naturally in the sun’s core

• Nuclear Fusion: 2 or more nuclei with small masses join together to form a larger, more massive nucleus

• The repulsion of + + has to be overcome…only way is with high temps (100,000,000 degrees)

• Occurs naturally in the sun’s core

Page 37: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Can we use nuclear fusion?

Can we use nuclear fusion?

Page 38: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

• 1. When you wrap the Mobium in a few sheets of paper, your instruments cannot detect its radiation. What kind of radiation is Mobium probably emitting?

• 2. 24 hours after isolating Mobium, you determine that all but 6.25% of it has turned into iron. What is Mobium’s half-life?

• 3. Rounding to the nearest whole number percentage point, after how many hours will ~100% of the Mobium have turned into iron?

• 1. When you wrap the Mobium in a few sheets of paper, your instruments cannot detect its radiation. What kind of radiation is Mobium probably emitting?

• 2. 24 hours after isolating Mobium, you determine that all but 6.25% of it has turned into iron. What is Mobium’s half-life?

• 3. Rounding to the nearest whole number percentage point, after how many hours will ~100% of the Mobium have turned into iron?

Page 39: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic EnergyAtomic Energy•OBJ 5: Understand the difference Understand the difference between nuclear fusion & fission. between nuclear fusion & fission.

•OBJ 6: Identify advantages and OBJ 6: Identify advantages and disadvantages of energy from the disadvantages of energy from the nucleus.nucleus.

•Warm-up: Turn in Chapter Review.

•Homework: Possible POP QUIZ next week!

Atomic EnergyAtomic Energy•OBJ 5: Understand the difference Understand the difference between nuclear fusion & fission. between nuclear fusion & fission.

•OBJ 6: Identify advantages and OBJ 6: Identify advantages and disadvantages of energy from the disadvantages of energy from the nucleus.nucleus.

•Warm-up: Turn in Chapter Review.

•Homework: Possible POP QUIZ next week!

Page 40: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

AgendaAgenda

• Check worksheet

• Nuclear Fusion/Fission

• Domino Chain Reaction Lab

• Check worksheet

• Nuclear Fusion/Fission

• Domino Chain Reaction Lab

Page 41: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

The Effects of RadiationThe Effects of Radiation

• Can knock electrons out of atoms

• Break chemical bonds between atoms

• Can cause damage to living and non-living matter

• Radiation sickness

• Can knock electrons out of atoms

• Break chemical bonds between atoms

• Can cause damage to living and non-living matter

• Radiation sickness

Page 42: Atomic Energy. Agenda Atomic Energy Warm-up: What do you know about radiation? Homework: Reread pages 80-87. OBJ 1: Compare alpha, beta, and gamma decay.

Atomic Energy in Real Life

Atomic Energy in Real Life


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