Problem 29
Question
A radioactive isotope of mercury, \({ }^{197} \mathrm{Hg}\), decays to gold, \({ }^{197} \mathrm{Au},\) with a disintegration constant of \(0.0108 \mathrm{~h}^{-1} .\) (a) Calculate the half-life of the \({ }^{197} \mathrm{Hg}\). What fraction of a sample will remain at the end of (b) three half-lives and (c) 10.0 days?
Step-by-Step Solution
Verified Answer
(a) 64.17 hours; (b) 1/8 (12.5%) remains; (c) 7.4% remains.
1Step 1: Calculate the Half-life
The half-life of a radioactive isotope is calculated using the formula: \[ t_{1/2} = \frac{\ln(2)}{k} \]where \( t_{1/2} \) is the half-life and \( k \) is the disintegration constant. Here, \( k = 0.0108 \, \text{h}^{-1} \). First, compute the natural logarithm of 2: \( \ln(2) \approx 0.693 \). Substitute the values into the formula:\[ t_{1/2} = \frac{0.693}{0.0108} \approx 64.17 \, \text{hours} \]
2Step 2: Determine Remaining Fraction After Three Half-lives
After each half-life, the remaining fraction of the substance is halved. After one half-life, \( \frac{1}{2} \) of the substance remains; after two half-lives, \( \left(\frac{1}{2}\right)^2 \); and after three half-lives, \( \left(\frac{1}{2}\right)^3 \). Calculate this:\[ \left(\frac{1}{2}\right)^3 = \frac{1}{8} \]Thus, \( \frac{1}{8} \) or 12.5% of the original sample remains after three half-lives.
3Step 3: Calculate Fraction Remaining After 10 Days
First, convert 10 days to hours: \( 10 \, \text{days} \times 24 \, \frac{\text{hours}}{\text{day}} = 240 \, \text{hours} \). The decay formula is:\[ N(t) = N_0 e^{-kt} \]where \( N(t) \) is the amount remaining after time \( t \), \( N_0 \) is the initial amount, and \( k \) is the decay constant. Substitute the values:\[ N(t) = N_0 e^{-0.0108 \times 240} \]\[ N(t) = N_0 e^{-2.592} \]Compute the exponential value: \( e^{-2.592} \approx 0.074 \). Therefore, 7.4% of the original sample remains after 10 days.
Key Concepts
Half-life calculationDisintegration constantExponential decay formula
Half-life calculation
The concept of half-life is fundamental to understanding radioactive decay. It is the amount of time required for half of the radioactive nuclei in a sample to decay. This doesn't mean that after one half-life, the radioactive material completely disappears; rather, only half of it transforms, leaving the other half still radioactive. In the calculation of half-life, we use the formula:\[ t_{1/2} = \frac{\ln(2)}{k} \]where:
- \( t_{1/2} \) is the half-life, typically measured in units of time.
- \( \ln(2) \) is the natural logarithm of 2, approximately 0.693.
- \( k \) is the disintegration constant, which indicates the rate of decay.
Disintegration constant
The disintegration constant, noted as \( k \), is a crucial component in understanding how quickly a radioactive substance decays. It quantifies the probability of decay of a single nucleus per unit time and is usually expressed with units that match the time of decay, such as per hour or per second.Intuitively, a larger disintegration constant means the substance decays more quickly, while a smaller value indicates a slower rate of decay. It is directly used in calculating both the half-life and in the exponential decay formula that predicts how much of a substance remains after a certain period.Revisiting the example of radioactive mercury, the given disintegration constant \( k = 0.0108 \, \text{h}^{-1} \) conveys how rapidly this isotope decays each hour. This constant is fundamental for computing how much of a substance remains as it decays over time, using various calculations.
Exponential decay formula
Exponential decay describes how the quantity of a radioactive isotope decreases over time. This decay process follows a specific mathematical pattern, known as the exponential decay formula:\[ N(t) = N_0 e^{-kt} \]where:
- \( N(t) \) is the quantity remaining after time \( t \).
- \( N_0 \) is the initial quantity of the substance.
- \( e \) is the base of the natural logarithms, approximately equal to 2.718.
- \( k \) is the disintegration constant.
- \( t \) is the time elapsed.
Other exercises in this chapter
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