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

How much time is required for a \(6.25\) -mg sample of \({ }^{51} \mathrm{Cr}\) to decay to \(0.75 \mathrm{mg}\) if it has a half-life of \(27.8\) days?

Short Answer

Expert verified
It will take approximately \(77.6\) days for the \(6.25\) mg sample of \({ }^{51} \mathrm{Cr}\) to decay to \(0.75\) mg.

Step by step solution

01

Understand the radioactive decay formula

The formula for radioactive decay is given by \(A(t) = A_0 e^{-\lambda t}\), where \(A(t)\) is the amount of the substance remaining after time \(t\), \(A_0\) is the initial amount, \(\lambda\) is the decay constant, and \(e\) is the base of natural logarithm.
02

Calculate the decay constant using the half-life

To calculate the decay constant, we'll use the formula: \(\lambda = \frac{\ln{2}}{T_{1/2}}\), where \(T_{1/2}\) is the half-life. For \({ }^{51} \mathrm{Cr}\), the half-life is \)27.8$ days, so the decay constant will be: \(\lambda = \frac{\ln{2}}{27.8} \)
03

Plug in the initial and final amounts into the radioactive decay formula

We know that the initial amount \(A_0\) is \(6.25\) mg, and the final amount \(A(t)\) is \(0.75\) mg. Plugging in these values into the radioactive decay formula, we get: \(0.75 = 6.25 e^{-\frac{\ln{2}}{27.8}t}\)
04

Solve for time \(t\)

To solve for \(t\), we'll first divide both sides by \(6.25\) mg: \[\frac{0.75}{6.25} = e^{-\frac{\ln{2}}{27.8}t}\] Next, we'll take the natural logarithm of both sides: \[\ln{\left(\frac{0.75}{6.25}\right)} = -\frac{\ln{2}}{27.8}t\] Finally, isolate \(t\) by dividing both sides by \(-\frac{\ln{2}}{27.8}\): \[t = \frac{\ln{\left(\frac{0.75}{6.25}\right)}}{-\frac{\ln{2}}{27.8}}\]
05

Calculate the time

Now, we'll use a calculator to find \(t\): \[t = \frac{\ln{\left(\frac{3}{25}\right)}}{-\frac{\ln{2}}{27.8}} \approx 77.6 \ \text{days}\] It will take approximately \(77.6\) days for the \(6.25\) mg sample of \({ }^{51} \mathrm{Cr}\) to decay to \(0.75\) mg.

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.

Half-Life
Understanding half-life is key to grasping how radioactive substances decay over time. Simply put, half-life is the amount of time it takes for half of a radioactive substance to lose its radioactivity. This concept reveals the rate at which unstable atoms undergo decay, turning them into more stable forms.

To illustrate, if a sample has a half-life of 10 years, it means that after 10 years, only half of the original amount of the radioactive material will remain; the other half will have decayed. With another 10 years, half of the remaining material will decay, leaving a quarter of the original amount. This process continues exponentially, following a predictable pattern that helps scientists determine the age of materials and predict the decay of radioactive substances.

Half-life is an essential concept when dealing with radioactive materials, as it determines their longevity and potential impact on the environment or human health. It is also a fundamental concept in archeological dating methods like radiocarbon dating.
Decay Constant
The decay constant, often represented by the symbol \(\lambda\), is a probability measure of the likelihood of decay of a radioactive isotope. It is inversely related to half-life—essentially, the decay constant tells us how quickly a radioactive material will decay. For any radioisotope, the decay constant is a fixed value and remains unaffected by external conditions such as temperature or pressure.

To calculate the decay constant when the half-life is known, the following formula is used: \(\lambda = \frac{\ln{2}}{T_{1/2}}\), where \(T_{1/2}\) represents the half-life of the substance. \(\ln{2}\) is used here because it is the natural logarithm of 2, which correlates with the fact that half-life is the time taken for half of the substance to decay. It's a direct window into the atomic nature of matter, demonstrating how atoms deteriorate at a predictable rate that can be modeled mathematically.
Natural Logarithm
The natural logarithm, often denoted as \(\ln\), is a logarithmic function with the base \(e\) (Euler's number, approximately equal to 2.71828). This special logarithm is widely used in science and engineering because of its natural appearance in growth and decay problems, including radioactive decay calculations.

When dealing with exponential decay equations, taking the natural logarithm of both sides of an equation is a common step to solve for an unknown variable. This is because the natural logarithm is the inverse operation of exponentiation with base \(e\). Therefore, it allows us to move from the exponential form to a linear one, which is much easier to manipulate algebraically. This quality makes it indispensable for solving time-related decay problems, as seen in the example of radioactive decay in this exercise.
Exponential Decay
Exponential decay describes the process by which a quantity decreases at a rate proportional to its current value. This pattern is commonly observed in nature and is especially relevant to radioactive decay. The formula \(A(t) = A_0 e^{-\lambda t}\) succinctly captures the essence of exponential decay; it shows that the amount of a radioactive substance \(A(t)\) at any given time \(t\) reduces from its original amount \(A_0\) by a factor depending on the decay constant \(\lambda\) and the base of natural logarithms \(e\).

The 'exponential' aspect refers to the presence of the term \(e^{-\lambda t}\) in the decay equation, indicating that the decrease is not linear but rather diminishes more rapidly at first and then slows down as time goes on. Such behavior is typical with radioactive substances where the rate of decay is fastest initially and gradually reduces as fewer radioactive atoms are left to decay. Thus, understanding exponential decay is fundamental to interpreting how radioactive materials change over time.

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

Give the symbol for (a) a proton, (b) a beta particle, (c) a positron.

The Sun radiates energy into space at the rate of \(3.9 \times 10^{26} \mathrm{~J} / \mathrm{s} .(\mathrm{a})\) Calculate the rate of mass loss from the Sun in \(\mathrm{kg} / \mathrm{s}\). (b) How does this mass loss arise? (c) It is estimated that the Sun contains \(9 \times 10^{56}\) free protons. How many protons per second are consumed in nuclear reactions in the Sun?

Complete and balance the following nuclear equations by supplying the missing particle: (a) \({ }^{25}{ }_{8}^{2} \mathrm{Cf}+{ }_{5}^{10} \mathrm{~B} \longrightarrow 3_{0}^{1} \mathrm{n}+?\) (b) \({ }_{1}^{2} \mathrm{H}+{ }_{2}^{3} \mathrm{He} \longrightarrow{ }_{2}^{4} \mathrm{He}+?\)

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.

The energy from solar radiation falling on Earth is \(1.07 \times 10^{16} \mathrm{~kJ} / \mathrm{min}\). (a) How much loss of mass from the Sun occurs in one day from just the energy falling on Earth? (b) If the energy released in the reaction $$ { }^{235} \mathrm{U}+{ }_{0^{n}}{ }_{\mathbf{n}} \longrightarrow{ }^{141} \mathrm{Ba}+{ }_{36}^{92} \mathrm{Kr}+3{ }_{0}^{1} \mathrm{n} $$ \(\left({ }^{235} \mathrm{U}\right.\) nuclear mass, \(234.9935 \mathrm{amu} ;{ }^{141}\) Ba nuclear mass, \(140.8833 \mathrm{amu} ;{ }^{92} \mathrm{Kr}\) nuclear mass, \(91.9021 \mathrm{amu}\) ) is taken as typical of that occurring in a nuclear reactor, what mass of uranium- 235 is required to equal \(0.10 \%\) of the solar energy that falls on Earth in \(1.0\) day?

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