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Page 1: Nuclear Chemistry - Suffolk County Community College · Nuclear Chemistry Chapter 19 ... Tro: Chemistry: A Molecular Approach 2 . 3 A X Z ... 23 Nuclear Transmutation 14N + 4a 17O

1

Nuclear Chemistry

Chapter 19

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

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2

Chemical Processes vs.

Nuclear Processes

• Chemical reactions involve changes in the

electronic structure of the atom

– atoms gain, lose, or share electrons

– no change in the nuclei occurs

• Nuclear reactions involve changes in the

structure of the nucleus

– when the number of protons in the nucleus

changes, the atom becomes a different element

2 Tro: Chemistry: A Molecular Approach

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X A Z

Mass Number

Atomic Number Element Symbol

Atomic number (Z) = number of protons in nucleus

Mass number (A) = number of protons + number of neutrons

= atomic number (Z) + number of neutrons

A

Z

1p 1

1H 1 or

proton 1n 0

neutron 0e

-1 0b

-1 or

electron 0e

+1 0b

+1 or

positron 4He 2

4a 2 or

a particle

1

1

1

0

0

-1

0

+1

4

2

Review

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Important Atomic Symbols

4 Tro: Chemistry: A Molecular Approach

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Balancing Nuclear Equations

1. Conserve mass number (A).

The sum of protons plus neutrons in the products must equal

the sum of protons plus neutrons in the reactants.

1n 0 U 235

92 + Cs 138 55 Rb 96

37 1n 0 + + 2

235 + 1 = 138 + 96 + 2x1

2. Conserve atomic number (Z) or nuclear charge.

The sum of nuclear charges in the products must equal the

sum of nuclear charges in the reactants.

1n 0 U 235

92 + Cs 138 55 Rb 96

37 1n 0 + + 2

92 + 0 = 55 + 37 + 2x0

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212Po decays by alpha emission. Write the balanced nuclear

equation for the decay of 212Po.

4He 2

4a 2 or alpha particle -

212Po 4He + AX 84 2 Z

212 = 4 + A A = 208

84 = 2 + Z Z = 82

212Po 4He + 208Pb 84 2 82

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Page 8: Nuclear Chemistry - Suffolk County Community College · Nuclear Chemistry Chapter 19 ... Tro: Chemistry: A Molecular Approach 2 . 3 A X Z ... 23 Nuclear Transmutation 14N + 4a 17O

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Nuclear Stability and Radioactive Decay

Beta decay

14C 14N + 0b 6 7 -1

40K 40Ca + 0b 19 20 -1

1n 1p + 0b 0 1 -1

Decrease # of neutrons by 1

Increase # of protons by 1

Positron decay

11C 11B + 0b 6 5 +1

38K 38Ar + 0b 19 18 +1

1p 1n + 0b 1 0 +1

Increase # of neutrons by 1

Decrease # of protons by 1

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Electron capture decay

Increase number of neutrons by 1

Decrease number of protons by 1

Nuclear Stability and Radioactive Decay

37Ar + 0e 37Cl 18 17 -1

55Fe + 0e 55Mn 26 25 -1

1p + 0e 1n 1 0 -1

Alpha decay

Decrease number of neutrons by 2

Decrease number of protons by 2 212Po 4He + 208Pb 84 2 82

Spontaneous fission

252Cf 2125In + 21n 98 49 0

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Particle Changes

10 Tro: Chemistry: A Molecular Approach

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Chapter 23: The Nucleus: A Chemist’s View

1. Balance the following nuclear reactions:

1. 211Po 207Pb + ____

2. 61Ni (d, 2n) _____

3. 27Al + α 30P + _____

4. _____ 187Os + β

5. 235U + n 135Xe + _____ + 2 1n

6. 75As (α, ___) 78Br

7. 20Na _____ + +1β

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n/p too large

beta decay

X

n/p too small

positron decay or electron capture

Y

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Nuclear Stability

• Certain numbers of neutrons and protons are extra stable

− n or p = 2, 8, 20, 50, 82 and 126

− Like extra stable numbers of electrons in noble gases (e- = 2, 10, 18, 36, 54 and 86)

• Nuclei with even numbers of both protons and neutrons are more stable than those with odd numbers of neutron and protons

• All isotopes of the elements with atomic numbers higher than 83 are radioactive

• All isotopes of Tc and Pm are radioactive

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Nuclear binding energy is the energy required to break up a

nucleus into its component protons and neutrons.

Nuclear binding energy + 19F 91p + 101n 9 1 0

Dm = 9 x (p mass) + 10 x (n mass) – 19F mass

DE = (Dm)c2

Dm= 9 x 1.007825 + 10 x 1.008665 – 18.9984

Dm = 0.1587 amu

DE = 2.37 x 10-11J

DE = 0.1587 amu x (3.00 x 108 m/s)2 = -1.43 x 1016 amu m2/s2

Using conversion factors:

1 kg = 6.022 x 1026 amu 1 J = kg m2/s2

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= 2.37 x 10-11 J

19 nucleons

= 1.25 x 10-12 J/nucleon

binding energy per nucleon = binding energy

number of nucleons

DE = (2.37 x 10-11J) x (6.022 x 1023/mol)

DE = -1.43 x 1013J/mol

DE = -1.43 x 1010kJ/mol

Nuclear binding energy = 1.43 x 1010kJ/mol

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Nuclear binding energy per nucleon vs mass number

nuclear stability nuclear binding energy

nucleon

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Kinetics of Radioactive Decay

N daughter

rate = kN

N = the number of atoms at time t

N0 = the number of atoms at time t = 0

k is the decay rate constant

Nt ln N0

-kt =

= t½ k 0.693

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Half-Lives of Various Nuclides

Nuclide Half-Life Type of Decay

Th–232 1.4 x 1010 yr alpha

U–238 4.5 x 109 yr alpha

C–14 5730 yr beta

Rn–220 55.6 sec alpha

Th–219 1.05 x 10–6 sec alpha

19 Tro: Chemistry: A Molecular Approach

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2. The half-life of Co-60 is 5.30 years. How many grams of a

4.567 g sample of Co-60 is left after 16.7 years?

3. Given the following atomic mass units: n = 1.008665 and p =

1.007838. Calculate

a) The mass defect per C-12 atom

b) The binding energy per C-12 atom

c) The binding energy per nucleon for C-12 atom

d) The amount of energy released per mole of C-12

4. How much energy is lost or gained when one mole of Polonium-

211 decays by alpha emission? The atomic masses are:

Po-211: 210.98665

Pb-207: 206.97590

a: 4.0026036

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Page 22: Nuclear Chemistry - Suffolk County Community College · Nuclear Chemistry Chapter 19 ... Tro: Chemistry: A Molecular Approach 2 . 3 A X Z ... 23 Nuclear Transmutation 14N + 4a 17O

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Radiocarbon Dating

14N + 1n 14C + 1H 7 1 6 0

14C 14N + 0b + n 6 7 -1

t½ = 5730 years

Uranium-238 Dating

238U 206Pb + 8 4a + 6 0b 92 -1 82 2 t½ = 4.51 x 109 years

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Nuclear Transmutation

14N + 4a 17O + 1p 7 2 8 1

27Al + 4a 30P + 1n 13 2 15 0

14N + 1p 11C + 4a 7 1 6 2

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Nuclear Transmutation

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Nuclear Fission

235U + 1n 90Sr + 143Xe + 31n + Energy 92 54 38 0 0

Energy = [mass 235U + mass n – (mass 90Sr + mass 143Xe + 3 x mass n )] x c2

Energy = 3.3 x 10-11J per 235U

= 2.0 x 1013 J per mole 235U

Combustion of 1 ton of coal = 5 x 107 J

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Nuclear Fission

235U + 1n 90Sr + 143Xe + 31n + Energy 92 54 38 0 0

Representative fission reaction

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Nuclear Fission

Nuclear chain reaction is a self-sustaining sequence of

nuclear fission reactions.

The minimum mass of fissionable material required to

generate a self-sustaining nuclear chain reaction is the

critical mass.

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Schematic Diagram of a Nuclear Reactor

U3O8

refueling

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Chemistry In Action: Nature’s Own Fission Reactor

Natural Uranium

0.7202 % U-235 99.2798% U-238

Measured at Oklo

0.7171 % U-235

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Nuclear Fusion

2H + 2H 3H + 1H 1 1 1 1

Fusion Reaction Energy Released

2H + 3H 4He + 1n 1 1 2 0

6Li + 2H 2 4He 3 1 2

6.3 x 10-13 J

2.8 x 10-12 J

3.6 x 10-12 J

Tokamak magnetic

plasma

confinement

solar fusion

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Thyroid images

with 125I-labeled

compound

normal enlarged

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Radioisotopes in Medicine

98Mo + 1n 99Mo 42 0 42

235U + 1n 99Mo + other fission products 92 0 42

99mTc 99Tc + g-ray 43 43

99Mo 99mTc + 0b 42 43 -1

Research production of 99Mo

Commercial production of 99Mo

t½ = 66 hours

t½ = 6 hours

Bone Scan with 99mTc

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Geiger-Müller Counter

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Biological Effects of Radiation

Radiation absorbed dose (rad)

1 rad = 1 x 10-5 J/g of material

Roentgen equivalent for man (rem)

1 rem = 1 rad x Q Quality Factor

g-ray = 1

b = 1

a = 20

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Chemistry In Action: Food Irradiation