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3.1: Nuclear Chemistry and Radioactive Decay (Problems)

  • Page ID
    98692
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    PROBLEM \(\PageIndex{1}\)

    Write the following isotopes in nuclide notation (e.g., " \(\ce{^{14}_6C}\) ")

    1. oxygen-14
    2. copper-70
    3. tantalum-175
    4. francium-217
    Answer a

    \(\ce{^{14}_8O}\)

    Answer b

    \(\ce{^{70}_29Cu}\)

    Answer c

    \(\ce{^{175}_73Ta}\)

    Answer d

    \(\ce{^{217}_87Fr}\)

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    PROBLEM \(\PageIndex{2}\)

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

    1. \(\ce{^{34}_{14}X}\)
    2. \(\ce{^{36}_P}\)
    3. \(\ce{^{57}_{X}Mn}\)
    4. \(\ce{^{121}_{56}X}\)
    Answer a

    \(\ce{^{34}_{14}Si}\)

    Answer b

    \(\ce{^{36}_{15}P}\)

    Answer c

    \(\ce{^{57}_{25}Mn}\)

    Answer d

    \(\ce{^{121}_{56}Ba}\)

    PROBLEM \(\PageIndex{3}\)

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

    1. 25 protons, 20 neutrons, 24 electrons
    2. 45 protons, 24 neutrons, 43 electrons
    3. 53 protons, 89 neutrons, 54 electrons
    4. 97 protons, 146 neutrons, 97 electrons
    Answer a

    \(\ce{^{45}_{25}Mn^{+1}}\)

    Answer b

    \(\ce{^{69}_{45}Rh^{+2}}\)

    Answer c

    \(\ce{^{142}_{53}I^{−1}}\)

    Answer d

    \(\ce{^{243}_{97}Bk}\)

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    PROBLEM \(\PageIndex{4}\)

    Which of the following nuclei lie within the band of stability?CNX_Chem_21_01_BandStable.jpg

    1. chlorine-37
    2. calcium-40
    3. 204Bi
    4. 56Fe
    5. 206Pb
    6. 211Pb
    7. 222Rn
    8. carbon-14
    Answer

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

    PROBLEM \(\PageIndex{5}\)

    Which of the following nuclei lie within the band of stability?CNX_Chem_21_01_BandStable.jpg

    1. argon-40
    2. oxygen-16
    3. 122Ba
    4. 58Ni
    5. 205Tl
    6. 210Tl
    7. 226Ra
    8. magnesium-24
    Answer

    (b), (e - very close), and (h)

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    PROBLEM \(\PageIndex{6}\)

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

    1. nucleon
    2. α particle
    3. β particle
    4. positron
    5. γ ray
    6. nuclide
    7. mass number
    8. atomic number
    Answer a

    collective term for protons and neutrons in a nucleus

    Answer b

    (α or \(\ce{^4_2He}\) or \(\ce{^4_2α}\)) high-energy helium nucleus; a helium atom that has lost two electrons and contains two protons and two neutrons

    Answer c

    ( \(β\) or \(\ce{^0_{-1}e}\) or \(\ce{^0_{-1}β}\)) high-energy electron

    Answer d

    antiparticle to the electron; it has identical properties to an electron, except for having the opposite (positive) charge

    Answer e

    (γ or \(\ce{^0_0γ}\)) short wavelength, high-energy electromagnetic radiation that exhibits wave-particle duality

    Answer f

    nucleus of a particular isotope

    Answer g

    sum of the numbers of neutrons and protons in the nucleus of an atom

    Answer h

    number of protons in the nucleus of an atom

    PROBLEM \(\PageIndex{7}\)

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

    1. \(\ce{^{27}_{13}Al + ^4_2He⟶\:? + ^1_0n}\)
    2. \(\ce{^{239}_{94}Pu +\, ? ⟶ ^{242}_{96}Cm + ^1_0n}\)
    3. \(\ce{^{14}_7N + ^4_2He⟶\:? + ^1_1H}\)
    4. \(\ce{^{235}_{92}U⟶\:? + ^{135}_{55}Cs + 4^1_0n}\)
    Answer a

    \(\ce{^{27}_{13}Al + ^4_2He⟶ ^{30}_{15}P + ^1_0n}\)

    Answer b

    \(\ce{^{239}_{94}Pu + ^4_2He ⟶ ^{242}_{96}Cm + ^1_0n}\)

    Answer c

    \(\ce{^{14}_7N + ^4_2He⟶ ^{17}_8O + ^1_1H}\)

    Answer d

    \(\ce{^{235}_{92}U⟶ ^{96}_{37}Rb + ^{135}_{55}Cs + 4^1_0n}\)

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    PROBLEM \(\PageIndex{8}\)

    Complete each of the following equations:

    1. \(\ce{^7_3Li +\, ?⟶2^4_2He}\)
    2. \(\ce{^{14}_6C⟶ ^{14}_7N +\, ?}\)
    3. \(\ce{^{27}_{13}Al + ^4_2He⟶\,? + ^1_0n}\)
    4. \(\ce{^{250}_{96}Cm ⟶\, ? + ^{98}_{38}Sr + 4^1_0n}\)
    Answer a

    \(\ce{^7_3Li +^1_1H ⟶2^4_2He}\)

    Answer b

    \(\ce{^{14}_6C⟶ ^{14}_7N +^0_{-1}e}\)

    Answer c

    \(\ce{^{27}_{13}Al + ^4_2He⟶^30_15P + ^1_0n}\)

    Answer d

    \(\ce{^{250}_{96}Cm ⟶^148_{58}Ce + ^{98}_{38}Sr + 4^1_0n}\)

     

    PROBLEM \(\PageIndex{9}\)

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

    1. the production of 17O from 14N by α particle bombardment
    2. the production of 14C from 14N by neutron bombardment
    3. the production of 233Th from 232Th by neutron bombardment
    4. the production of 239U from 238U by \(\ce{^2_1H}\) bombardment
    Answer a

    \(\ce{^{14}_7N + He^2 ⟶ ^{17}_8O + ^1_1H}\)

    Answer b

    \(\ce{^{14}_7N + ^1_0n⟶ ^{14}_6N + ^1_1H}\)

    Answer c

    \(\ce{^{232}_{90}Th + ^1_0n⟶ ^{233}_{90}Th}\)

    Answer d

    \(\ce{^{238}_{92}U + ^2_1H⟶ ^{239}_{92}U + ^1_1H}\)

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    PROBLEM \(\PageIndex{10}\)

    Technetium-99 is prepared from 98Mo. Molybdenum-98 combines with a neutron to give molybdenum-99, an unstable isotope that emits a β particle to yield an excited form of technetium-99, represented as 99Tc*. This excited nucleus relaxes to the ground state, represented as 99Tc, by emitting a γ ray. The ground state of 99Tc then emits a β particle. Write the equations for each of these nuclear reactions.

    Answer

    \(\ce{^{98}_{42}Mo + ^1_0n \rightarrow ^{99}_{42}Mo}\)

    \(\ce{^{99}_{42}Mo} \rightarrow ^0_{-1}e + ^{99}_{43}Tc^*\)

    \(\ce{^{99}_{43}Tc}^* \rightarrow ^0_{0}\gamma + ^{99}_{43}Tc\)

    \(\ce{^{99}_{43}Tc \rightarrow ^0_{-1}e + ^{99}_{44}Ru}\)

     

    PROBLEM \(\PageIndex{11}\)

    What changes occur to the atomic number and mass of a nucleus during each of the following decay scenarios?

    1. an α particle is emitted
    2. a β particle is emitted
    3. γ radiation is emitted
    4. a positron is emitted
    5. an electron is captured
    Answer a

    Since an α particle is the same as a \(\ce{^4_2He}\) nucleus, the mass number will decrease by 4 and the atomic number will decrease by 2.

    Answer b

    Since a β particle is the same as \(\ce{^0_{-1}e}\), the mass number will not change but the atomic number will increase by 1.

    Answer c

    Since a γ ray has no mass (it is energy) the mass number and atomic number do not change.

    Answer d

    A positron is the opposite of a β particle, it is \(\ce{^0_{+1}e}\), the mass number will not change but the atomic number will decrease by 1

    Answer e

    Electron capture has the same effect on the nucleus as positron emission: The atomic number is decreased by one and the mass number does not change.

    PROBLEM \(\PageIndex{12}\)

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

    1. emission of a β particle
    2. emission of a β+ particle
    3. capture of an electron
    Answer a

    conversion of a neutron to a proton: \(\ce{^1_0n ⟶ ^1_1p + ^0_{+1}e}\)

    Answer 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: \(\ce{^1_1p ⟶ ^1_0n + ^0_{+1}e}\)

    Answer c

    In a proton-rich nucleus, an inner atomic electron can be absorbed. In simplest form, this changes a proton into a neutron: \(\ce{^1_1p + ^0_{-1}e ⟶ ^1_0p}\)

    PROBLEM \(\PageIndex{13}\)

    CNX_Chem_21_01_BandStable.jpgExplain how unstable heavy nuclides (atomic number > 83) may decompose to form nuclides of greater stability if

    (a) they are below the band of stability and

    (b) they are above the band of stability

     

     

     

     

     

     
     
     
    Answer

    Nuclei below the band of stability will undergo positron decay, while those above the band of stability will undergo beta decay. Heavy nuclei past the band of stability will undergo alpha decay

    PROBLEM \(\PageIndex{14}\)

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

    1. chromium-53
    2. manganese-51
    3. iron-59
    Answer

    Manganese-51 is most likely to decay by positron emission. The n:p ratio for Cr-53 is \(\dfrac{29}{24}\) = 1.21; for Mn-51, it is \(\dfrac{26}{25}\) = 1.04; for Fe-59, it is \(\dfrac{33}{26}\) = 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, \(\ce{^{53}_{24}Cr}\) is a stable isotope, and \(\ce{^{59}_{26}Fe}\) decays by beta emission.

    PROBLEM \(\PageIndex{15}\)

    CNX_Chem_21_01_BandStable.jpgThe following nuclei do not lie in the band of stability. How would they be expected to decay? Explain your answer.

    1. \(\ce{^{34}_{15}P}\)
    2. \(\ce{^{239}_{92}U}\)
    3. \(\ce{^{38}_{20}Ca}\)
    4. \(\ce{^3_1H}\)
    5. \(\ce{^{245}_{94}Pu}\)

     

     

     

     
    Answer a

    Above the band of stability, beta decay is expected

    Answer b

    Beyond the band of stability, heavy nuclei undergo alpha decay

    Answer c

    Below the band of stability, positron decay is expected

    Answer d

    Above the band of stability, beta decay is expected

    Answer e

    Beyond the band of stability, heavy nuclei undergo alpha decay

    PROBLEM \(\PageIndex{16}\)

    Write a nuclear reaction for each step in the formation of \(\ce{^{218}_{84}Po}\) from \(\ce{^{238}_{92}U}\) , 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

    \(\ce{^{238}_{92}U⟶ ^{234}_{90}Th + ^4_2He}\)

    \(\ce{^{234}_{90}Th⟶ ^{234}_{91}Pa + ^0_{-1}e}\)

    \(\ce{^{234}_{91}Pa⟶^{234}_{92}U + ^0_{-1}e}\)

    \(\ce{^{234}_{92}U⟶ ^{230}_{90}Th + ^4_2He}\)

    \(\ce{^{230}_{90}Th⟶ ^{226}_{88}Ra + ^4_2He } \)

    \( \ce {^{226}_{88}Ra⟶^{222}_{86}Rn + ^4_2He}\)

    \(\ce{^{222}_{86}Rn⟶^{218}_{84}Po + ^4_2He}\)

    PROBLEM \(\PageIndex{17}\)

    Write a nuclear reaction for each step in the formation of \(\ce{^{208}_{82}Pb}\) from \(\ce{^{228}_{90}Th}\), which proceeds by a series of decay reactions involving the step-wise emission of α, α, α, α, β, β, α particles, in that order.

    Answer

    \(\ce{^{228}_{90}Th \rightarrow ^4_2He + ^{224}_{88}Ra}\)

    \(\ce{^{224}_{88}Ra \rightarrow ^4_2He + ^{220}_{86}Rn}\)

    \(\ce{^{220}_{86}Th \rightarrow ^4_2He + ^{216}_{84}Po}\)

    \(\ce{^{216}_{84}Po \rightarrow ^4_2He + ^{212}_{82}Pb}\)

    \(\ce{^{212}_{82}Pb \rightarrow ^0_{-1}e + ^{212}_{83}Bi}\)

    \(\ce{^{212}_{83}Bi \rightarrow ^0_{-1}e + ^{212}_{84}Po}\)

    \(\ce{^{212}_{84}Po \rightarrow ^4_2He + ^{208}_{82}Pb}\)

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    3.1: Nuclear Chemistry and Radioactive Decay (Problems) is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by LibreTexts.

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