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

Write balanced nuclear equations for the following processes: (a) rubidium-90 undergoes beta decay; (b) selenium-72 undergoes electron capture; (c) krypton-76 undergoes positron emission; (d) radium-226 emits alpha radiation.

Short Answer

Expert verified
a) \(^{90}_{37}\text{Rb} \rightarrow ^{90}_{38}\text{Sr} + ^0_{-1}\beta\) b) \(^{72}_{34}\text{Se} + ^0_{-1}e \rightarrow ^{72}_{33}\text{As}\) c) \(^{76}_{36}\text{Kr} \rightarrow ^{76}_{35}\text{Br} + ^0_{+1}\beta\) d) \(^{226}_{88}\text{Ra} \rightarrow ^{222}_{86}\text{Rn} + ^4_2\alpha\)

Step by step solution

01

a) Beta Decay of Rubidium-90

Beta decay occurs when a neutron in a nucleus is transformed into a proton, and an electron (called a beta particle) is emitted. The initial element changes into another element as the atomic number increases by one. In the beta decay of rubidium-90 (\(^{90}_{37}\text{Rb}\)), the resulting element will have an atomic number of 37 + 1 = 38, which is strontium (Sr). The balanced nuclear equation can be written as: \[^{90}_{37}\text{Rb} \rightarrow ^{90}_{38}\text{Sr} + ^0_{-1}\beta\]
02

b) Electron Capture of Selenium-72

Electron capture occurs when a proton in a nucleus captures an inner shell electron, converting into a neutron. This process reduces the atomic number by one, transmuting the initial element into another element. In the electron capture of selenium-72 (\(^{72}_{34}\text{Se}\)), the resulting element will have an atomic number of 34 - 1 = 33, which is arsenic (As). The balanced nuclear equation can be written as: \[^{72}_{34}\text{Se} + ^0_{-1}e \rightarrow ^{72}_{33}\text{As}\]
03

c) Positron Emission of Krypton-76

Positron emission happens when a proton in a nucleus is transformed into a neutron, emitting a positron in the process. The initial element changes into another element with an atomic number reduced by one. In the positron emission of krypton-76 (\(^{76}_{36}\text{Kr}\)), the resulting element will have an atomic number of 36 - 1 = 35, which is bromine (Br). The balanced nuclear equation can be written as: \[^{76}_{36}\text{Kr} \rightarrow ^{76}_{35}\text{Br} + ^0_{+1}\beta\]
04

d) Alpha Radiation Emission of Radium-226

Alpha radiation is the emission of alpha particles, which are essentially helium-4 nuclei containing two protons and two neutrons. As a result, the initial element's atomic number and mass number both decrease: atomic number decreases by two, and the mass number decreases by four. In the alpha radiation emission of radium-226 (\(^{226}_{88}\text{Ra}\)), the resulting element will have an atomic number of 88 - 2 = 86, which is radon (Rn), and a mass number of 226 - 4 = 222. The balanced nuclear equation can be written as: \[^{226}_{88}\text{Ra} \rightarrow ^{222}_{86}\text{Rn} + ^4_2\alpha\]

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!

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

When a positron is annihilated by combination with an electron, two photons of equal energy result. What is the wavelength of these photons? Are they gamma ray photons?

Complete and balance the following nuclear equations by supplying the missing particle: (a) \(_{16}^{32} \mathrm{~S}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{1}^{1} \mathrm{p}+?\) (b) \({ }_{4}^{7} \mathrm{Be}+{ }_{-\mathrm{j}}^{0}\) (orbital electron) \(\longrightarrow\) ? (c) \(? \longrightarrow{ }_{76}^{187} \mathrm{Os}+{ }_{-1}^{0} \mathrm{e}\) (d) \({ }_{2}^{98} \mathrm{Mo}+{ }_{1}^{2} \mathrm{H} \longrightarrow{ }_{0}^{1} \mathrm{n}+?\) (e) \({ }_{92}^{235} \mathrm{U}+{ }_{0}^{1} \mathrm{n} \longrightarrow{ }_{54}^{135} \mathrm{Xe}+2{ }_{0}^{1} \mathrm{n}+?\)

It has been suggested that strontium-90 (generated by nuclear testing) deposited in the hot desert will undergo radioactive decay more rapidly because it will be exposed to much higher average temperatures. (a) Is this a reasonable suggestion? (b) Does the process of radioactive decay have an activation energy, like the Arrhenius behavior of many chemical reactions \({ }^{\infty} 0\) (Section \(\left.14.5\right) ?\) Discuss.

A portion of the Sun's energy comes from the reaction $$ 4{ }_{1}^{1} \mathrm{H} \longrightarrow{ }_{2}^{4} \mathrm{He}+2 \stackrel{0}{1} $$ This reaction requires a temperature of about \(10^{6}\) to \(10^{7} \mathrm{~K}\). (a) Why is such a high temperature required? (b) Is the Sun solid?

The half-life for the process \({ }^{238} \mathrm{U} \longrightarrow{ }^{206} \mathrm{~Pb}\) is \(4.5 \times 10^{9}\) yr. A mineral sample contains \(75.0 \mathrm{mg}\) of \({ }^{238} \mathrm{U}\) and \(18.0 \mathrm{mg}\) of \({ }^{206} \mathrm{~Pb}\). What is the age of the mineral?

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