A bone sample containing strontium-90 \(\left(t_{1 / 2}=29 \mathrm{yr}\right)\) emits \(7.0 \times 10^{4} \beta^{-}\) particles per month. How long will it take for the emission to decrease to \(1.0 \times 10^{4}\) particles per month?

Short Answer

Expert verified
It will take approximately 81.4 years.

Step by step solution

01

- Understand the Half-life

The half-life \(\t_{1/2}\) is the time it takes for half of a radioactive substance to decay. For strontium-90, \(\t_{1/2} = 29 \text{ years}\).
02

- Determine the Initial and Final Activity

Initial activity (\text{A_0}\text{) = } \(7.0 \times 10^4 \text{ particles/month}\). Final activity (\text{A}\text{) = } \(1.0 \times 10^4 \text{ particles/month}\).
03

- Set Up the Decay Formula

Radioactive decay can be described using the formula \(\text{A} = \text{A_0} \times (\frac{1}{2})^{\frac{t}{t_{1/2}}}\).
04

- Solve for Time (t)

Plug in the values into the decay formula: \(1.0 \times 10^4 = 7.0 \times 10^4 \times (\frac{1}{2})^{\frac{t}{29}}\).\Divide both sides by \(7.0 \times 10^4\) to get: \( \frac{1.0 \times 10^4}{7.0 \times 10^4} = (\frac{1}{2})^{\frac{t}{29}}\).
05

- Simplify the Equation

Simplify the fraction on the left: \( \frac{1}{7} = (\frac{1}{2})^{\frac{t}{29}}\).
06

- Apply Logarithms

Take the logarithm of both sides to solve for \(t\): \(\text{ln}(\frac{1}{7}) = \text{ln}((\frac{1}{2})^{\frac{t}{29}})\).\This simplifies to: \(\text{ln}(\frac{1}{7}) = \frac{t}{29} \times \text{ln}(\frac{1}{2})\).
07

- Isolate the Variable t

Solve for \(t\): \(\text{t} = \frac{29 \times \text{ln}(\frac{1}{7})}{\text{ln}(\frac{1}{2})}\).
08

- Calculate the Time

Compute the value: \(\text{t} = \frac{29 \times \text{ln}(0.142857)}{\text{ln}(0.5)}\). Using a calculator: \(\text{t} \approx \frac{29 \times (-1.945910)}{-0.693147} \approx 81.4 \text{ years}\).

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Key Concepts

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

half-life calculation
Understanding the concept of half-life is crucial in solving any radioactive decay problem. A half-life \(\t_{1/2}\) is the time required for half of the radioactive substance to decay. For instance, if you start with 100 particles, after one half-life, only 50 of those particles will remain. The half-life of strontium-90, as given in this problem, is 29 years. Knowing the half-life helps you determine how the substance decreases over time. This calculation informs us how long it would take for the initial amount to reduce by half. In this exercise, you will note that the problem implicitly requires us to keep dividing the sample's emissions by two until we reach the final value.
decay formula application
The radioactive decay formula is an essential mathematical tool for such problems. The decay formula is: \[ A = A_0 \times \left( \frac{1}{2} \right)^{\frac{t}{t_{1/2}}} \]. Here, \(A\) is the final activity, \(A_0\) is the initial activity, \(t\) is the time, and \(t_{1/2}\) is the half-life. The formula shows how the initial activity decreases over time based on the half-life. To apply this formula, you input the initial activity and the desired final activity, then solve for the time \(t\), which tells you how long it will take to decay from the initial to the final activity level. Remember to keep units consistent for meaningful results.
logarithmic functions in decay problems
Logarithmic functions are vital when solving for time \(t\) in decay problems. After using the decay formula, you'll often end up with an expression where the unknown variable is in an exponent, such as: \[ (\frac{1}{2})^{\frac{t}{29}} = \frac{1}{7} \]. To solve for \(t\), you can take the natural logarithm (ln) of both sides. This process simplifies the equation, allowing you to isolate the variable. The logarithmic technique transforms exponential decay problems into linear ones. The process is as follows: \[ \text{ln}((\frac{1}{2})^{\frac{t}{29}}) = \text{ln}(\frac{1}{7}) \], which simplifies to \[ \frac{t}{29} \times \text{ln}(\frac{1}{2}) = \text{ln}(\frac{1}{7}) \]. This approach helps solve for \(t\) efficiently.
initial and final activity in radioactivity
Initial and final activities are key to understanding decay problems. Initial activity \(A_0\) represents the rate of decay at the start. In our problem, it’s given as \(7.0 \times 10^4\) particles/month. This initial activity helps set up your decay formula. Final activity \(A\) is the decay rate you want to find out when it reaches a certain value, here \(1.0 \times 10^4\) particles/month. Knowing these values lets you directly apply them to the decay formula: \[ 1.0 \times 10^4 = 7.0 \times 10^4 \times \left(\frac{1}{2}\right)^{\frac{t}{29}} \]. By solving this equation, you can determine the time frame for the activity to decrease to the desired level. Initial and final activities provide the essential boundary conditions for your calculations.

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Most popular questions from this chapter

Write balanced nuclear equations for the following: (a) Alpha decay of \({ }^{234} \mathrm{U}\) (b) Electron capture by neptunium- 232 (c) Positron emission by \({ }_{7}^{12} \mathrm{~N}\)

In the 1950 s, radioactive material was spread over the land from aboveground nuclear tests. A woman drinks some contaminated milk and ingests \(0.0500 \mathrm{~g}\) of \({ }^{90} \mathrm{Sr}\), which is taken up by bones and teeth and not eliminated. (a) How much \({ }^{90} \mathrm{Sr}\left(t_{1 / 2}=\right.\) \(29 \mathrm{yr}\) ) is present in her body after \(10 \mathrm{yr} ?\) (b) How long will it take for \(99.9 \%\) of the \({ }^{90} \mathrm{Sr}\) that she ingested to decay?

Uranium- 233 decays to thorium- 229 by \(\alpha\) decay, but the emissions have different energies and products: \(83 \%\) emit an \(\alpha\) particle with an energy of \(4.816 \mathrm{MeV}\) and give \({ }^{229} \mathrm{Th}\) in its ground state; \(15 \%\) emit an \(\alpha\) particle of \(4.773 \mathrm{MeV}\) and give \({ }^{229} \mathrm{Th}\) in excited state I; and \(2 \%\) emit a lower energy \(\alpha\) particle and give \({ }^{229} \mathrm{Th}\) in the higher excited state II. Excited state II emits a \(\gamma\) ray of \(0.060 \mathrm{MeV}\) to reach excited state I. (a) Find the \(\gamma\) -ray energy and wavelength that would convert excited state I to the ground state. (b) Find the energy of the \(\alpha\) particle that would raise \({ }^{233} \mathrm{U}\) to excited state II.

Seaborgium- 263 (Sg), the first isotope of element 106 synthesized, was produced, along with four neutrons, by bombarding californium- 249 with oxygen-18. The \({ }^{263} \mathrm{Sg}\) then underwent a series of decays starting with three \(\alpha\) emissions. Write balanced equations for the synthesis and the three \(\alpha\) emissions of \({ }^{263} \mathrm{Sg}\).

Nuclear disarmament could be accomplished if weapons were not "replenished." The tritium in warheads decays to helium with a half-life of 12.26 yr and must be replaced or the weapon is useless. What fraction of the tritium is lost in 5.50 yr?

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