25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Chapter 25
Nuclear Chemistry
25.1 Nuclear Radiation
25.2 Nuclear Transformations
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
What is the source of radon in homes?
CHEMISTRY & YOUCHEMISTRY & YOU
Radon may
accumulate in a
basement that is
not well ventilated.
Test kits are
available to
measure the
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Nuclear Stability and Decay
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
The
nuclear force
is an attractive force
that acts between
all
nuclear particles that
are extremely close together, such as
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
The
nuclear force
is an attractive force
that acts between
all
nuclear particles that
are extremely close together, such as
protons and neutrons in a nucleus.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
The stability of a nucleus depends on the
ratio of neutrons to protons.
Interpret Data
Interpret Data
• This graph shows the number of
neutrons vs. the number of
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
The stability of a nucleus depends on the
ratio of neutrons to protons.
Interpret Data
Interpret Data
• The region of the graph in which these points are located is called the band of
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
The stability of a nucleus depends on the
ratio of neutrons to protons.
Interpret Data
Interpret Data
• For elements of low atomic number
(below about 20), this ratio is about 1. • Above atomic
number 20, stable nuclei have more neutrons than
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
A nucleus may be unstable and undergo
spontaneous decay for different reasons.
The neutron-to-proton ratio in a
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Some nuclei are unstable because they
have too many neutrons relative to the
number of protons.
• When one of these nuclei decays, a neutron
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Some nuclei are unstable because they
have too many neutrons relative to the
number of protons.
• When one of these nuclei decays, a neutron
emits a beta particle (fast-moving electron) from the nucleus.
– A neutron that emits an electron becomes a proton.
n
1
0 p +
1
1 e
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Some nuclei are unstable because they
have too many neutrons relative to the
number of protons.
• When one of these nuclei decays, a neutron
emits a beta particle (fast-moving electron) from the nucleus.
– A neutron that emits an electron becomes a proton.
n
1
0 p +
1
1 e
0 –1
– This process is known as beta emission. – It increases the number of protons while
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Radioisotopes that undergo beta emission
include the following.
Cu
66
29 Zn +
66
30 e
0 –1
C
14
6 N +
14
7 e
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Other nuclei are unstable because they
have too few neutrons relative to the
number of protons.
• These nuclei increase their stability by converting a proton to a neutron.
– An electron is captured by the nucleus during this process, which is called electron capture.
Co
59 27
Ni + e
59 28 0 –1 Cl 37 17
Ar + e
37 18
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
A
positron
is a particle with the mass of an
electron but a positive charge.
• Its symbol is e.
• During positron emission, a proton changes to a neutron, just as in electron capture.
0 +1
B
8
5 Be +
8 4 e 0 +1 O 15
8 N +
15
7 e
0 +1
– When a proton is converted to a neutron, the
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Nuclei that have an atomic number greater
than 83 are radioactive.
• These nuclei have both too many neutrons and too many protons to be stable.
– Therefore, they undergo radioactive decay.
– Alpha emission increases the neutron-to-proton ratio, which tends to increase the stability of the nucleus.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
In alpha emission, the mass number
decreases by four and the atomic number
decreases by two.
Ra
226
88 Rn + He
222 86
4 2
Th
232
90 Ra + He
228 88
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Nuclear Stability and DecayNuclear Stability and Decay
Recall that conservation of mass is an
important property of chemical reactions.
• In contrast, mass is not conserved during nuclear reactions.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
During nuclear decay, if the atomic
number decreases by one but the mass
number is unchanged, the radiation
emitted is
A.
a positron.
B.
an alpha particle.
C.
a beta particle.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
During nuclear decay, if the atomic
number decreases by one but the mass
number is unchanged, the radiation
emitted is
A. a positron.
B.
an alpha particle.
C.
a beta particle.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Half-Life
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
1 2
A
half-life
(t ) is the time required for
one-half of the nuclei in a radioisotope sample
to decay to products.
Interpret Graphs
Interpret Graphs
After each half-life, half of the original
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Half-lives can be as short as a second or as long as billions of years.
Half-Lives of Some Naturally Occurring Radioisotopes
Isotope Half-life Radiation emitted
Carbon-14 5.73 × 103 years
Potassium-40 1.25 × 109 years
Radon-222 3.8 days Radium-226 1.6 × 103 years
Thorium-234 24.1 days
Uranium-235 7.0 × 108 years
Uranium-238 4.5 × 109 years
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
• Scientists use half-lives of some long-term
radioisotopes to determine the age of ancient objects.
• Many artificially produced radioisotopes have short half-lives, which makes them useful in nuclear medicine.
– Short-lived isotopes are not a long-term radiation hazard for patients.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Comparing Half-Lives
• The age of
uranium-containing minerals can be estimated by measuring the ratio of uranium-238 to
lead-206.
• Because the half-life of uranium-238 is 4.5 × 109 years, it is possible to use its half-life to date rocks as old as the solar system.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Uranium compounds are found in
rocks and in soils that form from these
rocks. How can these uranium
compounds lead to a buildup of radon
in homes and other buildings?
CHEMISTRY & YOU
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Uranium compounds are found in
rocks and in soils that form from these
rocks. How can these uranium
compounds lead to a buildup of radon
in homes and other buildings?
CHEMISTRY & YOU
CHEMISTRY & YOU
Radon gas is a product of the decay of
uranium. As the uranium compounds in
the soil beneath homes and buildings
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Radiocarbon Dating
Plants use carbon dioxide to produce
carbon compounds, such as glucose.
• The ratio of carbon-14 to other carbon isotopes is constant during an organism’s life.
• When an organism dies, it stops exchanging carbon with the environment and its radioactive C atoms decay without being replaced.
• Archaeologists can use this data to estimate when an organism died.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Exponential Decay Function
• A stands for the amount remaining.
• A0 stands for the initial amount.
• n stands for the number of half-lives.
You can use the following equation to
calculate how much of an isotope will
remain after a given number of half-lives.
A
=
A
0
1
2
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
• The exponent n indicates how many times A0
must be multiplied by to determine 12 A.
A
=
A
0
1
2
n
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Half-LifeHalf-Life
Decay of Initial Amount (A0) of Radioisotope
Half-Life Amount Remaining
0 A0 × ( )0 = A 0
1 A0 × ( )1 = A
0 ×
2 A0 × ( )2 = A
0 × ×
This table shows examples in which
n
= 1 and
n
= 2.
Exponential Decay Function
1 2 1 2 1 2 1 2 1
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Using Half-Lives in Calculations
Sample Problem 25.1
Sample Problem 25.1
Carbon-14 emits beta radiation and decays with a half-life (t ) of 5730 years. Assume that you start
with a mass of 2.00 × 10–12 g of carbon-14.
1 2
a. How long is three half-lives?
b. How many grams of the
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
KNOWNS UNKNOWNS
3 half-lives = ? years
mass remaining = ? g
Analyze List the knowns and the unknowns.
1
Sample Problem 25.1
Sample Problem 25.1
• To calculate the length of three half-lives, multiply the half-life by three.
• To find the mass of the radioisotope
remaining, multiply the original mass by for each half-life that has elapsed.
1 2
t = 5730 years
initial mass (A0) = 2.00 × 10–12 g
number of half-lives (n) = 3
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
a. Multiply the half-life of carbon-14 by
the total number of half-lives.
Calculate Solve for the unknowns.
2
Sample Problem 25.1
Sample Problem 25.1
t × 1 n = 5730 years × 3 = 17,190 years
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Calculate Solve for the unknowns.
2
Sample Problem 25.1
Sample Problem 25.1
b. The initial mass of carbon-14 is
reduced by one-half for each half-life. So, multiply by three times.1
2
Remaining mass = 2.00 × 10–12 g × × ×1
2 12 12
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Calculate Solve for the unknowns.
2
Sample Problem 25.1
Sample Problem 25.1
b. You can get the same answer by
using the equation for an exponential decay function.
= (2.00 × 10–12 g)
= 0.250 × 10–12 g
= 2.50 × 10–13 g
A = A0
( )
1 = (2.00 × 10–12 g)2
n
( )
1 23
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Evaluate
Do the results make sense?3
Sample Problem 25.1
Sample Problem 25.1
• The mass of carbon-14 after three half-lives should be one-eighth of the original mass.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
The half-life of phosphorus-32 is
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
The half-life of phosphorus-32 is
14.3 days. How many milligrams of
phosphorus-32 remain after 100.1
days if you begin with 2.5 mg of the
radioisotope?
n = 100.1 days × = 7 half-lives 1 half-life14.3 days
= (2.5 mg) = 2.0 × 10–2 mg
A = A0
( )
12 = (2.5 mg) n( )
12 7( )
125.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Transmutation Reactions
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
For thousands of years, alchemists tried to
change lead into gold.
• What they wanted to achieve is
transmutation, or the conversion of an atom of one element into an atom of another
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Transmutation can occur by radioactive
decay, or when particles bombard the
nucleus of an atom.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Ernst Rutherford performed the earliest
artificial transmutation in 1919.
• He bombarded nitrogen gas with alpha particles.
• The unstable fluorine atoms quickly decay to form a stable isotope of oxygen and a proton.
O +
17 8 p 1 1 F 18 9 Proton Oxygen-17 Fluorine-18
N +
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Rutherford’s experiment eventually led to
the discovery of the proton.
• He and other scientists noticed a pattern as they did different transmutation experiments. Hydrogen nuclei were emitted.
• Scientists realized that these hydrogen nuclei (protons) must have a fundamental role in atomic structure.
He Alpha particle N Nitrogen atom F Unstable fluorine atom O Oxygen P Proton 4
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
James Chadwick’s discovery of the neutron
in 1932 also involved a transmutation
experiment.
• Neutrons were produced when beryllium-9 was bombarded with alpha particles.
C +
12 6 n 1 0 Neutron Carbon-12
Be +
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Elements with atomic numbers above 92,
the atomic number of uranium, are called
transuranium elements
.
• None of these elements occurs in nature. • All of them are radioactive.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Transuranium elements are synthesized in nuclear reactors and nuclear accelerators.
• Reactors produce beams of low-energy particles.
• Accelerators are used to increase the speed of bombarding
particles to very high speeds.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
• When uranium-238 is bombarded with the relatively slow neutrons from a nuclear reactor, some uranium nuclei capture these neutrons. The product is uranium-239.
• Uranium-239 is radioactive and emits a beta particle. The other product is an isotope of the artificial
radioactive element neptunium (atomic number 93).
• Neptunium is unstable and decays, emitting a beta particle and a second artificial element, plutonium (atomic number 94).
Np +
239 93 e 0 –1 U 239 92
U +
238 92 n 1 0 U 239 92
Pu +
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Transmutation ReactionsTransmutation Reactions
Scientists in Berkeley, California,
synthesized the first two artificial elements
in 1940.
• Since that time, more than 20 additional
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Which of the following always changes
when transmutation occurs?
A.
The number of electrons
B.
The mass number
C.
The atomic number
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Which of the following always changes
when transmutation occurs?
A.
The number of electrons
B.
The mass number
C. The atomic number
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Key ConceptsKey Concepts
The neutron-to-proton ratio in a
radioisotope determines the type of decay that occurs.
After each half-life, half of the original
radioactive atoms have decayed into atoms of a new element.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Key EquationKey Equation
A
=
A
0
1
2
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Glossary TermsGlossary Terms
• nuclear force: an attractive force that acts
between all nuclear particles that are
extremely close together, like protons and
neutrons in a nucleus
• band of stability: the location of stable nuclei on a neutron-vs.-proton plot
25.2 Nuclear Transformations >
25.2 Nuclear Transformations > Glossary TermsGlossary Terms
• half-life: the time required for one-half of the nuclei of a radioisotope sample to decay to products
• transmutation: the conversion of an atom of
one element to an atom of another element
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >
Electrons and the Structure of Atoms
• Unstable atomic nuclei decay by emitting alpha or beta particles.
• Often gamma rays are emitted.
25.2 Nuclear Transformations >
25.2 Nuclear Transformations >