2 ch 28 nuclear chemistry (def radioactivity)

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Nuclear Chemistry Chapter 28

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Page 1: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear ChemistryNuclear Chemistry

Chapter 28Chapter 28

Page 2: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Comparison of Chemical and Nuclear Reactions

Comparison of Chemical and Nuclear Reactions

Chemical Reactions Nuclear Reactions

Occur when bonds are broken or formed

Occur when nuclei combine, split, & emit radiation

Involve only valence electrons

Can involve protons, neutrons, & electrons

Associated with small energy changes

Associated with large energy changes

Atoms keeps same identity although they may gain, lose, or share electrons, and form new substances

Atoms of one element are often converted into atoms of another element

Temperature, pressure, concentration, and catalysts affect reaction rates

Temperature, pressure, and catalysts do not normally affect reaction rates

Page 3: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

RadioactivityRadioactivity Radioisotopes are isotopes that have an

unstable nucleus. They emit radiation to attain more stable atomic configurations in a process called radioactive decay.

Radioactivity is the property by which an atomic nucleus gives off alpha, beta, or gamma radiation. Marie Curie named the process. In 1898, Marie & Pierre Curie identified 2

new elements, polonium & radium. The penetrating rays and particles

emitted by a radioactive source are called radiation.

Radioisotopes are isotopes that have an unstable nucleus. They emit radiation to attain more stable atomic configurations in a process called radioactive decay.

Radioactivity is the property by which an atomic nucleus gives off alpha, beta, or gamma radiation. Marie Curie named the process. In 1898, Marie & Pierre Curie identified 2

new elements, polonium & radium. The penetrating rays and particles

emitted by a radioactive source are called radiation.

Page 4: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Radioactivity (cont)Radioactivity (cont) The presence of too many or too

few neutrons, relative to the number of protons, leads to an unstable nucleus.

The types of radiation are alpha (α), beta (β), or gamma (γ).

An unstable nucleus loses energy by emitting radiation during the process of radioactive decay. Spontaneous and does not require any

input of energy.

The presence of too many or too few neutrons, relative to the number of protons, leads to an unstable nucleus.

The types of radiation are alpha (α), beta (β), or gamma (γ).

An unstable nucleus loses energy by emitting radiation during the process of radioactive decay. Spontaneous and does not require any

input of energy.

Page 5: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

The effect of an electric field on α,β, and γ, radiation. The radioactive source in the shielded box emits radiation, which passes between two electrodes. Alpha radiation is deflected toward the negative electrode, β radiation is strongly deflected toward the positive electrode, and γ radiation is undeflected.

Page 6: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 7: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear EquationsNuclear Equations For a nuclear reaction to be

balanced, the sum of all the atomic numbers and mass numbers on the right must equal the sum of those numbers on the left.

To figure out the unknown isotope, you need to balance the equation.

For a nuclear reaction to be balanced, the sum of all the atomic numbers and mass numbers on the right must equal the sum of those numbers on the left.

To figure out the unknown isotope, you need to balance the equation.

Page 8: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

ExampleExample

Page 9: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Natural Radioactive DecayNatural Radioactive Decay Why

The nucleus has many positively charged protons that are repelling each other.

The forces that hold the nucleus together can’t do its job and the nucleus breaks apart.

All elements with 84 or more protons are unstable and will eventually undergo nuclear decay.

How Alpha particle emission Beta particle emission Gamma radiation emission Positron emission (less common) Electron capture (less common)

Why The nucleus has many positively charged

protons that are repelling each other. The forces that hold the nucleus together

can’t do its job and the nucleus breaks apart. All elements with 84 or more protons are

unstable and will eventually undergo nuclear decay.

How Alpha particle emission Beta particle emission Gamma radiation emission Positron emission (less common) Electron capture (less common)

Page 10: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Alpha radiationAlpha radiation A type of radiation called alpha radiation

consists of helium nuclei that have been emitted from a radioactive source.

These emitted particles, called alpha particles, contain 2 protons and 2 neutrons and have a double positive charge.

A type of radiation called alpha radiation consists of helium nuclei that have been emitted from a radioactive source.

These emitted particles, called alpha particles, contain 2 protons and 2 neutrons and have a double positive charge.

Page 11: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Alpha Radiation (cont)Alpha Radiation (cont) Because of their large mass and

charge, alpha particles do not tend to travel very far and are not very penetrating. They are easily stopped by a piece of

paper or the surface of skin.Radioisotopes that emit alpha

particles are dangerous when ingested.

Because of their large mass and charge, alpha particles do not tend to travel very far and are not very penetrating. They are easily stopped by a piece of

paper or the surface of skin.Radioisotopes that emit alpha

particles are dangerous when ingested.

Page 12: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Alpha radiation occurs when an unstable nucleus emits a particle composed of 2 protons and 2 neutrons. The atom giving up the alpha particle has its atomic number reduced by two. Of course, this results in the atom becoming a different element. For example, Rn undergoes alpha decay to Po.

Page 13: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 14: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Beta ParticlesBeta Particles A beta particle is essentially an

electron that’s emitted from the nucleus.

A neutron is converted (decayed) into a proton & electron…so the atomic number increases by 1 and the electron leaves the nucleus.

Isotopes with a high neutron/proton ratio often undergo beta emission, because this decay allows the # of neutrons to be decreased by one & the # of protons to be increased by one, thus lowering the neutron/proton ratio.

A beta particle is essentially an electron that’s emitted from the nucleus.

A neutron is converted (decayed) into a proton & electron…so the atomic number increases by 1 and the electron leaves the nucleus.

Isotopes with a high neutron/proton ratio often undergo beta emission, because this decay allows the # of neutrons to be decreased by one & the # of protons to be increased by one, thus lowering the neutron/proton ratio.

Page 15: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 16: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Beta radiation occurs when an unstable nucleus emits an electron. As the emission occurs, a neutron turns into a proton.

Page 17: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Positron EmissionPositron Emission

A positron is essentially an electron that has a positive charge instead of a negative charge.

A positron is formed when a proton in the nucleus decays into a neutron & a positively charged electron.

It is then emitted from the nucleus. The positron is a bit of antimatter (seen in

Star Trek). When it comes in contact with an electron, both particles are destroyed with the release of energy.

A positron is essentially an electron that has a positive charge instead of a negative charge.

A positron is formed when a proton in the nucleus decays into a neutron & a positively charged electron.

It is then emitted from the nucleus. The positron is a bit of antimatter (seen in

Star Trek). When it comes in contact with an electron, both particles are destroyed with the release of energy.

Page 18: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 19: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Positron emission occurs when an unstable nucleus emits a positron. As the emission occurs, a proton turns into a neutron.

Page 20: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Positron emission tomography, also called PET imaging or a PET scan, is a diagnostic examination that involves the acquisition of physiologic images based on the detection of radiation from the emission of positrons. Positrons are tiny particles emitted from a radioactive substance administered to the patient.

Page 21: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

AntimatterAntimatter National Geographic Article When a particle and its antiparticle meet,

they annihilate each other and their entire mass is converted into pure energy.

Compared to conventional chemical propulsion systems, antimatter energy would slash the travel time to Mars and back from roughly two years to a few weeks.

The world's largest maker of antimatter, the Fermi National Accelerator Laboratory in Batavia, Illinois, makes only one billionth of a gram a year at a cost of $80 million.

National Geographic Article When a particle and its antiparticle meet,

they annihilate each other and their entire mass is converted into pure energy.

Compared to conventional chemical propulsion systems, antimatter energy would slash the travel time to Mars and back from roughly two years to a few weeks.

The world's largest maker of antimatter, the Fermi National Accelerator Laboratory in Batavia, Illinois, makes only one billionth of a gram a year at a cost of $80 million.

Page 22: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

This artist's concept of an antimatter-powered rocket ship looks like a big space-borne linear accelerator. Credit: Laboratory for Energetic Particle Science at Pennsylvania State University.

An artist's concept of a robotic antimatter-powered probe sailing past planets in an imaginary nearby solar system. Credit: Laboratory for Energetic Particle Science at Pennsylvania State University.

Page 23: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Gamma RadiationGamma Radiation Gamma radiation is similar to x-rays –

high energy, short wavelength emissions (photons).

The symbol is γ, the Greek letter gamma. It commonly accompanies alpha and

beta emission, but it’s usually not shown in a balanced nuclear reaction.

Some isotopes, such as Cobalt-60, give off large amounts of gamma radiation. Co-60 is used in the radiation treatment of

cancer…the gamma rays focus on the tumor, thus destroying it.

Gamma radiation is similar to x-rays – high energy, short wavelength emissions (photons).

The symbol is γ, the Greek letter gamma. It commonly accompanies alpha and

beta emission, but it’s usually not shown in a balanced nuclear reaction.

Some isotopes, such as Cobalt-60, give off large amounts of gamma radiation. Co-60 is used in the radiation treatment of

cancer…the gamma rays focus on the tumor, thus destroying it.

Page 24: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Gamma radiation occurs when an unstable nucleus emits electromagnetic radiation. The radiation has no mass, and so its emission does not change the element. However, gamma radiation often accompanies alpha and beta emission, which do change the element's identity.

Page 25: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Electron CaptureElectron Capture Electron capture is a rare type of

nuclear decay in which an electron from the innermost energy level (1s) is captured by the nucleus.

This electron combines with a proton to form a neutron.

The atomic number decreases by one but the mass stays the same.

Electrons drop down to fill the empty space in the 1s orbital, releasing energy.

Electron capture is a rare type of nuclear decay in which an electron from the innermost energy level (1s) is captured by the nucleus.

This electron combines with a proton to form a neutron.

The atomic number decreases by one but the mass stays the same.

Electrons drop down to fill the empty space in the 1s orbital, releasing energy.

Page 26: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 27: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Man-Made Radioactive Decay on Earth

Man-Made Radioactive Decay on Earth

Fission Fusion

Occurs naturally in spacePowers the sunSupernovas allow atoms to fuse

into heavier elements, this is how the other elements came into existence

Fission Fusion

Occurs naturally in spacePowers the sunSupernovas allow atoms to fuse

into heavier elements, this is how the other elements came into existence

Page 28: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

FissionFission

Nuclear fission occurs when scientists bombard a large isotope with a neutron.

This collision causes the larger isotope to break apart into two or more elements.

These reactions release a lot of energy. You can calculate the amount of

energy produced during a nuclear reaction using an equation developed by Einstein: E=mc2

Nuclear fission occurs when scientists bombard a large isotope with a neutron.

This collision causes the larger isotope to break apart into two or more elements.

These reactions release a lot of energy. You can calculate the amount of

energy produced during a nuclear reaction using an equation developed by Einstein: E=mc2

Page 29: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 30: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

EinsteinEinstein

"The intuitive mind is a sacred gift and the rational mind is a faithful servant. We have created a society that honors the servant and has forgotten the gift." 

"The intuitive mind is a sacred gift and the rational mind is a faithful servant. We have created a society that honors the servant and has forgotten the gift." 

Page 31: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Chain ReactionsChain Reactions A chain reaction is a continuing

cascade of nuclear fissions. This chain reaction depends on the

release of more neutrons then were used during the nuclear reaction.

Isotopes that produce an excess of neutrons in their fission support a chain reaction - fissionable.

There are only two main fissionable isotopes used during nuclear reactions – uranium-235 & plutonium-239.

A chain reaction is a continuing cascade of nuclear fissions.

This chain reaction depends on the release of more neutrons then were used during the nuclear reaction.

Isotopes that produce an excess of neutrons in their fission support a chain reaction - fissionable.

There are only two main fissionable isotopes used during nuclear reactions – uranium-235 & plutonium-239.

Page 32: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Chain Reactions (cont)Chain Reactions (cont) The minimum amount of

fissionable material needed to ensure that a chain reaction occurs is called the critical mass.

Anything less than this amount is subcritical.

The minimum amount of fissionable material needed to ensure that a chain reaction occurs is called the critical mass.

Anything less than this amount is subcritical.

Page 33: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Chain Reaction FigureChain Reaction Figure

Page 34: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Atomic BombsAtomic Bombs Because of the tremendous amount of

energy released in a fission chain reaction, the military implications of nuclear reactions were immediately realized. The first atomic bomb was dropped on

Hiroshima, Japan, on August 6, 1945. In an atomic bomb, two pieces of a

fissionable isotope are kept apart. Each piece by itself is subcritical.

When it’s time for the bomb to explode, conventional explosives force the two pieces together to cause a critical mass.

The chain reaction is uncontrolled, releasing a tremendous amount of energy almost instantaneously.

Because of the tremendous amount of energy released in a fission chain reaction, the military implications of nuclear reactions were immediately realized. The first atomic bomb was dropped on

Hiroshima, Japan, on August 6, 1945. In an atomic bomb, two pieces of a

fissionable isotope are kept apart. Each piece by itself is subcritical.

When it’s time for the bomb to explode, conventional explosives force the two pieces together to cause a critical mass.

The chain reaction is uncontrolled, releasing a tremendous amount of energy almost instantaneously.

Page 35: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Mushroom CloudMushroom Cloud

Page 36: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear Power PlantsNuclear Power Plants If the neutrons can be controlled,

then the energy can be released in a controlled way. Nuclear power plants produce heat through controlled nuclear fission chain reactions.

The fissionable isotope is contained in fuel rods in the reactor core. All the fuel rods together comprise the critical mass.

Control rods, commonly made of boron and cadmium, are in the core, and they act like neutron sponges to control the rate of radioactive decay.

If the neutrons can be controlled, then the energy can be released in a controlled way. Nuclear power plants produce heat through controlled nuclear fission chain reactions.

The fissionable isotope is contained in fuel rods in the reactor core. All the fuel rods together comprise the critical mass.

Control rods, commonly made of boron and cadmium, are in the core, and they act like neutron sponges to control the rate of radioactive decay.

Page 37: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear Power Plants (cont)

Nuclear Power Plants (cont)

In the U.S., there are approximately 100 nuclear reactors, producing a little more than 20% of the country’s electricity.

Advantages No fossil fuels are burned. No combustion products (CO2, SO2, etc) to

pollute the air and water. Disadvantages

Cost - expensive to build and operate. Limited supply of fissionable Uranium-235. Accidents (Three Mile Island & Chernobyl) Disposal of nuclear wastes

In the U.S., there are approximately 100 nuclear reactors, producing a little more than 20% of the country’s electricity.

Advantages No fossil fuels are burned. No combustion products (CO2, SO2, etc) to

pollute the air and water. Disadvantages

Cost - expensive to build and operate. Limited supply of fissionable Uranium-235. Accidents (Three Mile Island & Chernobyl) Disposal of nuclear wastes

Page 38: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

A nuclear power plant. Heat produced in the reactor core is transferred by coolant circulating in a closed loop to a steam generator, and the steam then drives a turbine to generate electricity.

Page 39: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Three Mile IslandThree Mile Island

Page 40: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

ChernobylChernobyl

Page 41: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 42: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear FusionNuclear Fusion

Fusion is when lighter nuclei are fused into a heavier nucleus.

Fusion powers the sun. Four isotopes of hydrogen-1 are fused into a helium-4 with the release of a tremendous amount of energy.

On Earth, H-2 (deuterium) & H-3 (tritium) are used.

Fusion is when lighter nuclei are fused into a heavier nucleus.

Fusion powers the sun. Four isotopes of hydrogen-1 are fused into a helium-4 with the release of a tremendous amount of energy.

On Earth, H-2 (deuterium) & H-3 (tritium) are used.

Page 43: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 44: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

PlasmaPlasma Plasmas are conductive assemblies of

charged particles, neutrals and fields that exhibit collective effects.

Further, plasmas carry electrical currents and generate magnetic fields.

Plasmas are the most common form of matter, comprising more than 99% of the visible universe, and permeate the solar system, interstellar and intergalactic environments.

Plasmas are conductive assemblies of charged particles, neutrals and fields that exhibit collective effects.

Further, plasmas carry electrical currents and generate magnetic fields.

Plasmas are the most common form of matter, comprising more than 99% of the visible universe, and permeate the solar system, interstellar and intergalactic environments.

Page 46: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear Fusion (cont)Nuclear Fusion (cont) The first demonstration of nuclear fusion –

the hydrogen bomb – was conducted by the military. A hydrogen bomb is approximately 1,000 times

as powerful as an ordinary atomic bomb. The goal of scientists has been the

controlled release of energy from a fusion reaction. If the energy can be released slowly, it can be

used to produce electricity. It will provide an unlimited supply of energy that

has no wastes to deal with or contaminants to harm the atmosphere.

The 3 problems are: temperature, time, containment

The first demonstration of nuclear fusion – the hydrogen bomb – was conducted by the military. A hydrogen bomb is approximately 1,000 times

as powerful as an ordinary atomic bomb. The goal of scientists has been the

controlled release of energy from a fusion reaction. If the energy can be released slowly, it can be

used to produce electricity. It will provide an unlimited supply of energy that

has no wastes to deal with or contaminants to harm the atmosphere.

The 3 problems are: temperature, time, containment

Page 47: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 48: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Nuclear Fusion (cont)Nuclear Fusion (cont) Temperature

Hydrogen isotopes must be heated to 40,000,000 K (hotter than the sun).

Electrons are gone…all that’s left is positively charged plasma.

TimeThe plasma needs to be held together

for about one second at 40,000,000 K. Containment

Everything is a gas…ceramics vaporize. A magnetic field could be used but the plasma leaks from those as well.

TemperatureHydrogen isotopes must be heated to

40,000,000 K (hotter than the sun). Electrons are gone…all that’s left is

positively charged plasma. Time

The plasma needs to be held together for about one second at 40,000,000 K.

ContainmentEverything is a gas…ceramics vaporize.

A magnetic field could be used but the plasma leaks from those as well.

Page 49: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 50: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 51: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Half – Life Half – Life A half-life (t1/2) is the time required for

one-half of the nuclei of a radioisotope sample to decay to products.

Half-lives may be as short as a fraction of a second or as long as billions of years.

This is an example of exponential decay. If you want to find times or amounts that

are not associated with a simple multiple of a half-life, you can use this equation:

ln(N0/N) = (.6963/t1/2)t

ln=natural log, N0=amnt iso start, N=amnt iso left

t=time, t1/2=half-life

A half-life (t1/2) is the time required for one-half of the nuclei of a radioisotope sample to decay to products.

Half-lives may be as short as a fraction of a second or as long as billions of years.

This is an example of exponential decay. If you want to find times or amounts that

are not associated with a simple multiple of a half-life, you can use this equation:

ln(N0/N) = (.6963/t1/2)t

ln=natural log, N0=amnt iso start, N=amnt iso left

t=time, t1/2=half-life

Page 52: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 53: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 54: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Radioactive DatingRadioactive Dating Radioactive dating is a useful

application of half-lives. Carbon-14 is produced in the upper

atmosphere by cosmic radiation. Plants absorb C-14 during

photosynthesis. Animals eat plants. C-14 is part of the cellular structure of all living things.

As long as an organism is alive, the amount of C-14 remains constant.

When the organism dies, the C-14 begins to decrease.

The half-life of C-14 is 5,730 years. For nonliving substances, another

isotope is used. Usually potassium-40.

Radioactive dating is a useful application of half-lives.

Carbon-14 is produced in the upper atmosphere by cosmic radiation.

Plants absorb C-14 during photosynthesis. Animals eat plants. C-14 is part of the cellular structure of all living things.

As long as an organism is alive, the amount of C-14 remains constant.

When the organism dies, the C-14 begins to decrease.

The half-life of C-14 is 5,730 years. For nonliving substances, another

isotope is used. Usually potassium-40.

Page 55: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Is this the face of Christ? A new study reignites the argument that the Shroud

of Turin, from which this impression was taken, is the burial cloth of Jesus of

Nazareth. A 1988 carbon-dating study determined that a piece of the shroud was created

between A.D. 1260 and 1390. Ever since, the conventional wisdom has been that the shroud, which resides in Turin, Italy,

was a medieval fake. But new tests show that the piece that

was tested is of a different material from the rest of the shroud, says chemist

Raymond Rogers—it was a patch added in medieval times. Published in the

journal Thermochimica Acta, the findings greatly increase the possibility

that the shroud may be as old as Christianity itself.

Page 56: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)

Human Exposure to Radiation

Human Exposure to Radiation

Page 57: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)
Page 58: 2 Ch 28 Nuclear Chemistry (Def Radioactivity)