A \({}^{{\rm{60}}}{\rm{Co}}\) source is labelled \(4.00\,{\rm{mCi}}\), but its present activity is found to be \(1.85 \times {10^7}\,{\rm{Bq}}\). (a) What is the present activity in \({\rm{mCi}}\)? (b) How long ago did it actually have a \({\rm{4}}{\rm{.00mCi}}\) activity?

Short Answer

Expert verified

(a) The source's current activity is \(0.500\,{\rm{mCi}}\).

(b) The activity was \(4.00\,{\rm{mCi}}\),\(15.8\,{\rm{y}}\)ago.

Step by step solution

01

Define radioactivity

Radioactivity is a phenomenon in which a few substances spontaneously release energy and subatomic particles. The nuclear instability of an atom causes radioactivity.

02

Explanation

(a) As \(1\,{\rm{mCi}}\) equals \(3.70 \times {10^7}\,{\rm{Bq}}\), the source's current activity is,

\(\begin{array}{c}{R_f} = 1.85 \times {10^7}\,{\rm{Bq}}\\ = \frac{{(1.85 \times {{10}^7}\,{\rm{Bq}})}}{{(3.70 \times {{10}^7}\,{\rm{Bq/mCi}})}}\\ = 0.500\,{\rm{mCi}}\end{array}\)

Therefore, the source's current activity is\(0.500\,{\rm{mCi}}\).

03

Explanation

(b) A radioactive substance's activity is determined by,

\(R = \frac{{In(2)N}}{{{t_{1/2}}}}\)

As a result, the first activity is,

\(\begin{array}{c}{R_i} & = \frac{{In(2){N_i}}}{{{t_{1/2}}}}\\ & = 4.0\,{\rm{mCi}}\end{array}\)

the last activity is,

\(\begin{array}{c}{R_f} & = \frac{{In(2){N_f}}}{{{t_{1/2}}}}\\ & = 0.500\,{\rm{mCi}}\end{array}\)

To get the answer, divide equations,

\(\begin{array}{c}\frac{{{R_f}}}{{{R_i}}} & = \frac{{{N_f}}}{{{N_i}}}\\ & = \frac{{0.500\,{\rm{mCi}}}}{{4.0\,{\rm{mCi}}}}\\ & = \frac{1}{8}\\ & = {\left( {\frac{1}{2}} \right)^3}\end{array}\)

As a result, the time spent is,

\(t = 3{t_{1/2}}\)

Now that\({}^{{\rm{60}}}{\rm{Co}}\)has a half-life of\({t_{1/2}} = 5.27\,{\rm{y}}\), we may say that time is,

\(\begin{array}{c}t &= 3\left( {5.27\,{\rm{y}}} \right)\\ & = 15.8\,{\rm{y}}\end{array}\)

Therefore, the activity was \(4.00\,{\rm{mCi}}\),\(15.8\,{\rm{y}}\) ago.

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

Consider the generation of electricity by a radioactive isotope in a space probe, such as described in exercise. Construct a problem in which you calculate the mass of a radioactive isotope you need in order to supply power for a long space flight. Among the things to consider are the isotope chosen, its half-life and decay energy, the power needs of the probe and the length of the flight.

Construct Your Own Problem

Consider the decay of radioactive substances in the Earth's interior. The energy emitted is converted to thermal energy that reaches the earth's surface and is radiated away into cold dark space. Construct a problem in which you estimate the activity in a cubic meter of earth rock? And then calculate the power generated. Calculate how much power must cross each square meter of the Earth's surface if the power is dissipated at the same rate as it is generated. Among the things to consider are the activity per cubic meter, the energy per decay, and the size of the Earth.

If a \(1.50\,{\rm{cm}}\)-thick piece of lead can absorb \({\rm{90}}{\rm{.0 \% }}\) of the \({\rm{\gamma }}\) rays from a radioactive source, how many centimeters of lead are needed to absorb all but \({\rm{0}}{\rm{.100 \% }}\) of the \({\rm{\gamma }}\) rays?

Spontaneous radioactive decay occurs only when the decay products have less mass than the parent, and it tends to produce a daughter that is more stable than the parent. Explain how this is related to the fact that more tightly bound nuclei are more stable. (Consider the binding energy per nucleon.)

Neutrinos are experimentally determined to have an extremely small mass. Huge numbers of neutrinos are created in a supernova at the same time as massive amounts of light are first produced. When the 1987A supernova occurred in the Large Magellanic Cloud, visible primarily in the Southern Hemisphere and some 100,000 light-years away from Earth, neutrinos from the explosion were observed at about the same time as the light from the blast. How could the relative arrival times of neutrinos and light be used to place limits on the mass of neutrinos?

See all solutions

Recommended explanations on Physics 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