Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Complete the following nuclear equations, and identify \(\mathrm{X}\) in each case: (a) \({ }_{12}^{26} \mathrm{Mg}+{ }_{1}^{1} \mathrm{p} \longrightarrow \alpha+\mathrm{X}\) (b) \({ }_{27}^{59} \mathrm{Co}+{ }_{1}^{2} \mathrm{H} \longrightarrow{ }_{27}^{60} \mathrm{Co}+\mathrm{X}\) (c) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{36}^{94} \mathrm{Kr}+{ }_{56}^{139} \mathrm{Ba}+3 \mathrm{X}\) (d) \(\frac{53}{24} \mathrm{Cr}+{ }_{2}^{4} \alpha \longrightarrow{ }_{0}^{1} \mathrm{n}+\mathrm{X}\) \((\mathrm{e}){ }_{8}^{20} \mathrm{O} \longrightarrow{ }_{9}^{20} \mathrm{~F}+\mathrm{X}\)

Short Answer

Expert verified
(a) \( _{11}^{23} \mathrm{Na} \), (b) \( _{1}^{1} \mathrm{H} \), (c) \( _{0}^{1} \mathrm{n} \), (d) \( _{26}^{56} \mathrm{Fe} \), (e) \( _{-1}^{0} \beta \).

Step by step solution

01

Analyze Reaction (a)

The nuclear equation is: \[ {}_{12}^{26} \mathrm{Mg} + {}_{1}^{1} \mathrm{p} \rightarrow \alpha + \mathrm{X} \]We know that an alpha particle (\(\alpha\)) is \( _{2}^{4} \mathrm{He} \).Conserve both atomic and mass numbers to find \(\mathrm{X}\).
02

Solve for X in Reaction (a)

Equation for mass numbers: \[ 26 + 1 = 4 + A \] Thus, \( A = 23 \). Equation for atomic numbers: \[ 12 + 1 = 2 + Z \] Thus, \( Z = 11 \). Therefore, \(\mathrm{X}\) is \( _{11}^{23} \mathrm{Na} \) (sodium).
03

Analyze Reaction (b)

The nuclear equation is: \[ {}_{27}^{59} \mathrm{Co} + {}_{1}^{2} \mathrm{H} \rightarrow {}_{27}^{60} \mathrm{Co} + \mathrm{X} \]Conserve both atomic and mass numbers to find \(\mathrm{X}\).
04

Solve for X in Reaction (b)

Equation for mass numbers: \[ 59 + 2 = 60 + A \] Thus, \( A = 1 \).Equation for atomic numbers: \[ 27 + 1 = 27 + Z \] Thus, \( Z = 1 \). Therefore, \(\mathrm{X}\) is \( _{1}^{1} \mathrm{H} \) (a proton).
05

Analyze Reaction (c)

The nuclear equation is:\[ {}_{92}^{235} \mathrm{U} + {}_{0}^{1} \mathrm{n} \rightarrow {}_{36}^{94} \mathrm{Kr} + {}_{56}^{139} \mathrm{Ba} + 3\mathrm{X} \]Conserve both atomic and mass numbers to find \(\mathrm{X}\).
06

Solve for X in Reaction (c)

Equation for mass numbers: \[ 235 + 1 = 94 + 139 + 3A \] Thus, \( 3A = 3 \) and \( A = 1 \).Equation for atomic numbers: \[ 92 + 0 = 36 + 56 + 3Z \] Thus, \( 3Z = 0 \) and \( Z = 0 \). Therefore, \(\mathrm{X}\) is \( _{0}^{1} \mathrm{n} \) (a neutron).
07

Analyze Reaction (d)

The nuclear equation is:\[ \frac{53}{24} \mathrm{Cr} + {}_{2}^{4} \alpha \rightarrow {}_{0}^{1} \mathrm{n} + \mathrm{X} \]Conserve both atomic and mass numbers to find \(\mathrm{X}\).
08

Solve for X in Reaction (d)

Equation for mass numbers: \[ 53 + 4 = 1 + A \] Thus, \( A = 56 \).Equation for atomic numbers: \[ 24 + 2 = 0 + Z \] Thus, \( Z = 26 \). Therefore, \(\mathrm{X}\) is \( _{26}^{56} \mathrm{Fe} \) (iron).
09

Analyze Reaction (e)

The nuclear equation is:\[ {}_{8}^{20} \mathrm{O} \rightarrow {}_{9}^{20} \mathrm{~F} + \mathrm{X} \]Conserve both atomic and mass numbers to find \(\mathrm{X}\).
10

Solve for X in Reaction (e)

Equation for mass numbers: \[ 20 = 20 + A \] Thus, \( A = 0 \).Equation for atomic numbers: \[ 8 = 9 + Z \] Thus, \( Z = -1 \). Therefore, \(\mathrm{X}\) is \( _{-1}^{0} \beta \) (a beta particle, \( \beta^+ \)).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Conservation of Mass Number
In nuclear equations, the conservation of mass number plays a vital role in ensuring that the total number of nucleons (protons and neutrons) remains constant throughout the reaction. This principle states that the sum of mass numbers, which are the superscripts in the element symbol, must be equal on both sides of a nuclear reaction.
When solving nuclear equations, you can think of it like balancing a scale: each side of the reaction must weigh the same in terms of nucleons. For example, if you begin with a mass number of 26 in magnesium and 1 in a proton, the products must collectively have the same mass number total.
This not only helps in identifying missing elements but also ensures the stability and correctness of nuclear reactions.
Conservation of Atomic Number
The conservation of atomic number is another critical principle in nuclear reactions. It ensures that the net charge remains constant from reactants to products, meaning the sum of atomic numbers, which are the subscripts in the element symbol, must be identical on both sides of the equation.
This conservation is pivotal when determining unknown products in nuclear equations. For instance, when a process starts with an atomic number of 12 for magnesium and 1 for a proton, the resulting components' atomic numbers should add up to 13.
This balance not only aids in finding the identity of unknown elements but also maintains the chemical identity throughout the nuclear process. It ensures that the charge and elemental identity are preserved.
Alpha Particle
An alpha particle is a type of nuclear radiation consisting of two protons and two neutrons, just like a helium nucleus but without any electrons. It's symbolically represented as \(_{2}^{4}\mathrm{He}\).
Alpha particles are commonly released in radioactive decay processes where an unstable nucleus expels these helium nuclei to become more stable.
Due to their significant mass and double positive charge, alpha particles have low penetration power and can be stopped by a sheet of paper or skin. However, they can cause significant damage when they interact with living tissues directly, thus necessitating careful handling.
Alpha decay's mathematics involves reducing the atomic number by 2 and the mass number by 4 of the original nucleus, helping us balance the reaction and identify missing products.
Beta Particle
A beta particle is a high-speed electron or positron released from a nucleus during radioactive decay. It is represented typically as \(_{-1}^{0}\beta\).
There are two types of beta decay: beta-minus (\(\beta^-\)) and beta-plus (\(\beta^+\)). In beta-minus decay, a neutron transforms into a proton, and an electron (\(\beta^-\)) is emitted, while in beta-plus decay, a proton becomes a neutron, releasing a positron (\(\beta^+\)).
Beta particles have greater penetration power compared to alpha particles, often passing through paper but stopped by denser materials like aluminum.
In nuclear equations, beta decay plays a significant role in converting one element to another, with changes in the atomic number without altering the mass number, thus enabling complex transmutations in nuclear chemistry.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Define nuclear binding energy, mass defect, and nucleon.

The constituents of wine contain, among others, carbon, hydrogen, and oxygen atoms. A bottle of wine was sealed about 6 years ago. To confirm its age, which of the isotopes would you choose in a radioactive dating study? The half-lives of the isotopes are: \({ }^{14} \mathrm{C}: 5715\) years; \({ }^{15} \mathrm{O}: 124 \mathrm{~s} ;{ }^{3} \mathrm{H}: 12.5\) years. Assume that the activities of the isotopes were known at the time the bottle was sealed.

Nuclear waste disposal is one of the major concerns of the nuclear industry. In choosing a safe and stable environment to store nuclear wastes, consideration must be given to the heat released during nuclear decay. As an example, consider the \(\beta\) decay of \({ }^{90} \mathrm{Sr}(89.907738 \mathrm{amu})\) : $$ { }_{38}^{90} \mathrm{Sr} \longrightarrow{ }_{39}^{90} \mathrm{Y}+{ }_{-1}^{0} \beta \quad t_{1 / 2}=28.1 \mathrm{yr} $$ The \({ }^{90} \mathrm{Y}(89.907152 \mathrm{amu})\) further decays as follows: \({ }_{39}^{90} \mathrm{Y} \longrightarrow{ }_{40}^{90} \mathrm{Zr}+{ }_{-1}^{0} \beta \quad t_{1 / 2}=64 \mathrm{~h}\) Zirconium- \(90(89.904703 \mathrm{amu})\) is a stable isotope. (a) Use the mass defect to calculate the energy released (in joules) in each of the preceding two decays. (The mass of the electron is \(5.4857 \times 10^{-4}\) amu.) (b) Starting with 1 mole of \({ }^{90} \mathrm{Sr}\), calculate the number of moles of \({ }^{90} \mathrm{Sr}\) that will decay in a year. (c) Calculate the amount of heat released (in kJ) corresponding to the number of moles of \({ }^{90} \mathrm{Sr}\) decayed to \({ }^{90} \mathrm{Zr}\) in part \((\mathrm{b}).\)

Why is it preferable to use nuclear binding energy per nucleon for a comparison of the stabilities of different nuclei?

The following equations are for nuclear reactions that are known to occur in the explosion of an atomic bomb. Identify X. (a) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{56}^{140} \mathrm{Ba}+3{ }_{0}^{1} \mathrm{n}+\mathrm{X}\) (b) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{55}^{144} \mathrm{Cs}+{ }_{37}^{90} \mathrm{Rb}+2 \mathrm{X}\) (c) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{35}^{87} \mathrm{Br}+3{ }_{0}^{1} \mathrm{n}+\mathrm{X}\) (d) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{6}^{160} \mathrm{Sm}+{ }_{30}^{72} \mathrm{Zn}+4 \mathrm{X}\)

See all solutions

Recommended explanations on Chemistry Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free