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Chapter 21: Nuclear Chemistry

39 problems · 1 figure

Example 21.1 §21.1 source ↗

Find the density of a neutron star with a mass of 1.97 solar masses and a diameter of 13 km, and compare it to the density of a hydrogen nucleus, which has a diameter of 1.75 fm (1 fm = 1 × 10–15 m).

Answer

The density of the neutron star is 3.4 × 1018 kg/m3. The density of a hydrogen nucleus is 6.0 × 1017 kg/m3. The neutron star is 5.7 times denser than the hydrogen nucleus.

Example 21.2 §21.1 source ↗

What is the binding energy for the nuclide 919F (atomic mass: 18.9984 amu) in MeV per nucleus?

Answer

148.4 MeV

Example 21.3 §21.1 source ↗

What is the binding energy per nucleon in 919F (atomic mass, 18.9984 amu)?

Answer

7.810 MeV/nucleon

Example 21.4 §21.2 source ↗

The nuclide 53125I combines with an electron and produces a new nucleus and no other massive particles. What is the equation for this reaction?

Answer

53125I+ −10e⟶ 52125Te

Example 21.5 §21.3 source ↗

Radon-222, 86222Rn , has a half-life of 3.823 days. How long will it take a sample of radon-222 with a mass of 0.750 g to decay into other elements, leaving only 0.100 g of radon-222?

Answer

11.1 days

Example 21.6 §21.3 source ↗

More accurate dates of the reigns of ancient Egyptian pharaohs have been determined recently using plants that were preserved in their tombs. Samples of seeds and plant matter from King Tutankhamun’s tomb have a C-14 decay rate of 9.07 disintegrations/min/g of C. How long ago did King Tut’s reign come to an end?

Answer

about 3350 years ago, or approximately 1340 BC

Example 21.7 §21.3 source ↗

A sample of rock contains 6.14 × 10–4 g of Rb-87 and 3.51 × 10–5 g of Sr-87. Calculate the age of the rock. (The half-life of the β decay of Rb-87 is 4.7 × 1010 y.)

Answer

3.7 × 109 y

Example 21.8 §21.6 source ↗

Tritium is a radioactive isotope of hydrogen (t1/2 = 12.32 y) that has several uses, including self-powered lighting, in which electrons emitted in tritium radioactive decay cause phosphorus to glow. Its nucleus contains one proton and two neutrons, and the atomic mass of tritium is 3.016 amu. What is the activity of a sample containing 1.00mg of tritium (a) in Bq and (b) in Ci?

Answer

(a) 3.56 × 1011 Bq; (b) 0.962 Ci

21-1 §21.1 source ↗

Write the following isotopes in hyphenated form (e.g., “carbon-14”)

(a) 1124Na

(b) 1329Al

(c) 3673Kr

(d) 77194Ir

Answer

(a) sodium-24; (b) aluminum-29; (c) krypton-73; (d) iridium-194

21-3 §21.1 source ↗

For the following isotopes that have missing information, fill in the missing information to complete the notation

(a) 1434X

(b) X36P

(c) X57Mn

(d) 56121X

Answer

(a) 1434Si; (b) 1536P; (c) 2557Mn; (d) 56121Ba

21-5 §21.1 source ↗

Write the nuclide notation, including charge if applicable, for atoms with the following characteristics:

(a) 25 protons, 20 neutrons, 24 electrons

(b) 45 protons, 24 neutrons, 43 electrons

(c) 53 protons, 89 neutrons, 54 electrons

(d) 97 protons, 146 neutrons, 97 electrons

Answer

(a) 2545Mn+1; (b) 4569Rh+2; (c) 53142I−1; (d) 97243Bk

21-7 §21.1 source ↗

What are the two principal differences between nuclear reactions and ordinary chemical changes?

Answer

Nuclear reactions usually change one type of nucleus into another; chemical changes rearrange atoms. Nuclear reactions involve much larger energies than chemical reactions and have measureable mass changes.

21-9 §21.1 source ↗

Which of the following nuclei lie within the band of stability shown in Figure 21.2?

(a) chlorine-37

(b) calcium-40

(c) 204Bi

(d) 56Fe

(e) 206Pb

(f) 211Pb

(g) 222Rn

(h) carbon-14

Figure 21.2 in the book ↗
This plot shows the nuclides that are known to exist and those that are stable. The stable nuclides are indicated in blue, and the unstable nuclides are indicated in green. Note that all isotopes of elements with atomic numbers greater than 83 are unstable. The solid line is the line where n = Z.

Answer

(a), (b), (c), (d), and (e)

21-11 §21.2 source ↗

Write a brief description or definition of each of the following:

(a) nucleon

(b) α particle

(c) β particle

(d) positron

(e) γ ray

(f) nuclide

(g) mass number

(h) atomic number

Answer

(a) A nucleon is any particle contained in the nucleus of the atom, so it can refer to protons and neutrons. (b) An α particle is one product of natural radioactivity and is the nucleus of a helium atom. (c) A β particle is a product of natural radioactivity and is a high-speed electron. (d) A positron is a particle with the same mass as an electron but with a positive charge. (e) Gamma rays compose electromagnetic radiation of high energy and short wavelength. (f) Nuclide is a term used when referring to a single type of nucleus. (g) The mass number is the sum of the number of protons and the number of neutrons in an element. (h) The atomic number is the number of protons in the nucleus of an element.

21-13 §21.2 source ↗

Complete each of the following equations by adding the missing species:

(a) 1327Al+ 24He⟶ ?+ 01n

(b) 94239Pu+ ?⟶ 96 242Cm+ 01n

(c) 714N+ 24He⟶ ?+ 11H

(d) 92235U⟶ ?+ 55135Cs+ 401n

Answer

(a) 1327Al+ 24He⟶ 1530P+ 01n; (b) 94239Pu+ 24He⟶ 96242Cm+ 01n; (c) 714N+ 24He⟶ 817O+ 11H; (d) 92235U⟶ 3796Rb+ 55135Cs+ 401n

21-15 §21.2 source ↗

Write a balanced equation for each of the following nuclear reactions:

(a) the production of 17O from 14N by α particle bombardment

(b) the production of 14C from 14N by neutron bombardment

(c) the production of 233Th from 232Th by neutron bombardment

(d) the production of 239U from 238U by 12H bombardment

Answer

(a) 714N+ 24He⟶ 817O+ 11H; (b) 714C+ 01n⟶ 614C+ 11H; (c) 90232Th+ 01n⟶ 90233Th; (d) 192238U+ 12H⟶ 92239U+ 11H

21-17 §21.2 source ↗

The mass of the atom 919F is 18.99840 amu.

(a) Calculate its binding energy per atom in millions of electron volts.

(b) Calculate its binding energy per nucleon.

Answer

(a) 148.8 MeV per atom; (b) 7.808 MeV/nucleon

21-19 §21.3 source ↗

What are the types of radiation emitted by the nuclei of radioactive elements?

Answer

α (helium nuclei), β (electrons), β+ (positrons), and η (neutrons) may be emitted from a radioactive element, all of which are particles; γ rays also may be emitted.

21-21 §21.3 source ↗

What is the change in the nucleus that results from the following decay scenarios?

(a) emission of a β particle

(b) emission of a β+ particle

(c) capture of an electron

Answer

(a) conversion of a neutron to a proton: 01n⟶ 11p+ +10e; (b) conversion of a proton to a neutron; the positron has the same mass as an electron and the same magnitude of positive charge as the electron has negative charge; when the n:p ratio of a nucleus is too low, a proton is converted into a neutron with the emission of a positron: 11p⟶ 01n+ +10e; (c) In a proton-rich nucleus, an inner atomic electron can be absorbed. In simplest form, this changes a proton into a neutron: 11p+ -10e⟶ 01p

21-23 §21.3 source ↗

Why is electron capture accompanied by the emission of an X-ray?

Answer

The electron pulled into the nucleus was most likely found in the 1s orbital. As an electron falls from a higher energy level to replace it, the difference in the energy of the replacement electron in its two energy levels is given off as an X-ray.

21-25 §21.3 source ↗

Which of the following nuclei is most likely to decay by positron emission? Explain your choice.

(a) chromium-53

(b) manganese-51

(c) iron-59

Answer

Manganese-51 is most likely to decay by positron emission. The n:p ratio for Cr-53 is 2924 = 1.21; for Mn-51, it is 2625 = 1.04; for Fe-59, it is 3326 = 1.27. Positron decay occurs when the n:p ratio is low. Mn-51 has the lowest n:p ratio and therefore is most likely to decay by positron emission. Besides, 2453Cr is a stable isotope, and 2659Fe decays by beta emission.

21-27 §21.3 source ↗

The following nuclei do not lie in the band of stability. How would they be expected to decay?

(a) 1528P

(b) 92235U

(c) 2037Ca

(d) 39L i

(e) 96245Cm

Answer

(a) positron emission; (b) α decay; (c) positron emission; (d) β decay; (e) α decay

21-29 §21.3 source ↗

Write a nuclear reaction for each step in the formation of 84218Po from 92238U , which proceeds by a series of decay reactions involving the step-wise emission of α, β, β, α, α, α, α particles, in that order.

Answer

92238U⟶ 90234Th+ 24He; 90234Th⟶ 91234Pa+ -10e; 91234Pa⟶ 92234U+ -10e; 92234U⟶ 90230Th+ 24He 90230Th⟶ 88226Ra+ 24He 88226Ra⟶ 86222Rn+ 24He; 86222Rn⟶ 84218Po+ 24He

21-31 §21.3 source ↗

Define the term half-life and illustrate it with an example.

Answer

Half-life is the time required for half the atoms in a sample to decay. Example (answers may vary): For C-14, the half-life is 5770 years. A 10-g sample of C-14 would contain 5 g of C-14 after 5770 years; a 0.20-g sample of C-14 would contain 0.10 g after 5770 years.

21-33 §21.3 source ↗

239Pu is a nuclear waste byproduct with a half-life of 24,000 y. What fraction of the 239Pu present today will be present in 1000 y?

Answer

(12)0.04= 0.973 or 97.3%

21-35 §21.3 source ↗

If 1.000 g of 88226Ra produces 0.0001 mL of the gas 86222Rn at STP (standard temperature and pressure) in 24 h, what is the half-life of 226Ra in years?

Answer

2 × 103 y

21-37 §21.3 source ↗

Technetium-99 is often used for assessing heart, liver, and lung damage because certain technetium compounds are absorbed by damaged tissues. It has a half-life of 6.0 h. Calculate the rate constant for the decay of 4399Tc .

Answer

0.12 h–1

21-39 §21.3 source ↗

A sample of rock was found to contain 8.23 mg of rubidium-87 and 0.47 mg of strontium-87.

(a) Calculate the age of the rock if the half-life of the decay of rubidium by β emission is 4.7 × 1010 y.

(b) If some 3887Sr was initially present in the rock, would the rock be younger, older, or the same age as the age calculated in (a)? Explain your answer.

Answer

(a) 3.8 billion years; (b) The rock would be younger than the age calculated in part (a). If Sr was originally in the rock, the amount produced by radioactive decay would equal the present amount minus the initial amount. As this amount would be smaller than the amount used to calculate the age of the rock and the age is proportional to the amount of Sr, the rock would be younger.

21-41 §21.3 source ↗

Plutonium was detected in trace amounts in natural uranium deposits by Glenn Seaborg and his associates in 1941. They proposed that the source of this 239Pu was the capture of neutrons by 238U nuclei. Why is this plutonium not likely to have been trapped at the time the solar system formed 4.7 × 109 years ago?

Answer

c = 0; This shows that no Pu-239 could remain since the formation of the earth. Consequently, the plutonium now present could not have been formed with the uranium.

21-43 §21.3 source ↗

A 58B atom (mass = 8.0246 amu) decays into a 48Be atom (mass = 8.0053 amu) by loss of a β+ particle (mass = 0.00055 amu) or by electron capture. How much energy (in millions of electron volts) is produced by this reaction?

Answer

17.5 MeV

21-45 §21.3 source ↗

Write a balanced equation for each of the following nuclear reactions:

(a) bismuth-212 decays into polonium-212

(b) beryllium-8 and a positron are produced by the decay of an unstable nucleus

(c) neptunium-239 forms from the reaction of uranium-238 with a neutron and then spontaneously converts into plutonium-239

(d) strontium-90 decays into yttrium-90

Answer

(a) 83212Bi⟶ 84212Po+ -10e; (b) 58B⟶ 48Be+ -10e; (c) 92238U+ 01n⟶ 93239Np+ -10Np, 93239Np⟶ 94239Pu+ -10e; (d) 3890Sr⟶ 3990Y+ -10e

21-47 §21.4 source ↗

Write the balanced nuclear equation for the production of the following transuranium elements:

(a) berkelium-244, made by the reaction of Am-241 and He-4

(b) fermium-254, made by the reaction of Pu-239 with a large number of neutrons

(c) lawrencium-257, made by the reaction of Cf-250 and B-11

(d) dubnium-260, made by the reaction of Cf-249 and N-15

Answer

(a) 95241Am+ 24He⟶ 97244Bk+ 01n; (b) 94239Pu+ 1501n⟶ 100254Fm+ 6−10e; (c) 98250Cf+ 511B⟶ 103257Lr+ 401n; (d) 98249Cf+ 715N⟶ 105260Db+ 401n

21-49 §21.4 source ↗

Both fusion and fission are nuclear reactions. Why is a very high temperature required for fusion, but not for fission?

Answer

Two nuclei must collide for fusion to occur. High temperatures are required to give the nuclei enough kinetic energy to overcome the very strong repulsion resulting from their positive charges.

21-51 §21.4 source ↗

Describe the components of a nuclear reactor.

Answer

A nuclear reactor consists of the following:

1. A nuclear fuel. A fissionable isotope must be present in large enough quantities to sustain a controlled chain reaction. The radioactive isotope is contained in tubes called fuel rods.

2. A moderator. A moderator slows neutrons produced by nuclear reactions so that they can be absorbed by the fuel and cause additional nuclear reactions.

3. A coolant. The coolant carries heat from the fission reaction to an external boiler and turbine where it is transformed into electricity.

4. A control system. The control system consists of control rods placed between fuel rods to absorb neutrons and is used to adjust the number of neutrons and keep the rate of the chain reaction at a safe level.

5. A shield and containment system. The function of this component is to protect workers from radiation produced by the nuclear reactions and to withstand the high pressures resulting from high-temperature reactions.

21-53 §21.4 source ↗

Describe how the potential energy of uranium is converted into electrical energy in a nuclear power plant.

Answer

The fission of uranium generates heat, which is carried to an external steam generator (boiler). The resulting steam turns a turbine that powers an electrical generator.

21-55 §21.5 source ↗

How can a radioactive nuclide be used to show that the equilibrium:
AgCl(s)⇌ Ag+(aq)+ Cl−(aq)
is a dynamic equilibrium?

Answer

Introduction of either radioactive Ag+ or radioactive Cl– into the solution containing the stated reaction, with subsequent time given for equilibration, will produce a radioactive precipitate that was originally devoid of radiation.

21-57 §21.5 source ↗

Iodine that enters the body is stored in the thyroid gland from which it is released to control growth and metabolism. The thyroid can be imaged if iodine-131 is injected into the body. In larger doses, I-133 is also used as a means of treating cancer of the thyroid. I-131 has a half-life of 8.70 days and decays by β− emission.

(a) Write an equation for the decay.

(b) How long will it take for 95.0% of a dose of I-131 to decay?

Answer

(a) 53133I⟶ 54133Xe+ −10e; (b) 37.6 days

21-59 §21.6 source ↗

Based on what is known about Radon-222’s primary decay method, why is inhalation so dangerous?

Answer

Alpha particles can be stopped by very thin shielding but have much stronger ionizing potential than beta particles, X-rays, and γ-rays. When inhaled, there is no protective skin covering the cells of the lungs, making it possible to damage the DNA in those cells and cause cancer.

21-61 §21.6 source ↗

A scientist is studying a 2.234 g sample of thorium-229 (t1/2 = 7340 y) in a laboratory.

(a) What is its activity in Bq?

(b) What is its activity in Ci?

Answer

(a) 7.64 × 109 Bq; (b) 2.06 × 10−2 Ci

End of the book.

Problems and answers are adapted from Chemistry 2e by Paul Flowers, Klaus Theopold, Richard Langley and William R. Robinson, OpenStax, and are used under the CC BY-NC-SA 4.0 licence. Access for free at https://openstax.org/books/chemistry-2e/pages/1-introduction. Illustrations: Copyright Rice University, OpenStax, under CC BY-NC-SA 4.0 license. This adaptation is released under the same licence, is non-commercial, and is neither affiliated with nor endorsed by OpenStax or Rice University.