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It takes \(4 \mathrm{~h} \mathrm{} 39 \mathrm{~min}\) for a \(2.00\)-mg sample of radium-230 to decay to \(0.25 \mathrm{mg}\). What is the half-life of radium-230?

Short Answer

Expert verified
The half-life of radium-230 is approximately \(1.56\,\text{hours}\).

Step by step solution

01

Calculate the decay rate

First, let's rewrite the decay formula in terms of the decay constant k: \(k = \frac{\ln(N_0 / N(t))}{t}\) Now, plug in the given values: - \(N_0 = 2\,\text{mg}\) - \(N(t) = 0.25\,\text{mg}\) - \(t = 4\,\text{h} \,\mathrm{39}\, \mathrm{min} = 4.65\,\text{h}\) Calculate the decay constant k: \(k = \frac{\ln(2 / 0.25)}{4.65} = 0.44533 \, \mathrm{h}^{-1}\)
02

Calculate the half-life

Now, we can use the half-life formula and plug in the decay constant k: \[T_{1/2} = \frac{\ln 2}{k}\] Calculate the half-life: \(T_{1/2} = \frac{\ln 2}{0.44533} \approx 1.56\,\text{h}\) The half-life of radium-230 is approximately \(1.56\,\text{hours}\).

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Key Concepts

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

Radioactive Decay
Radioactive decay is the process by which an unstable atomic nucleus loses energy by emitting radiation. This fundamental process occurs in nature, allowing physicists and chemists to determine the age of ancient objects and understand the behavior of nuclear materials. Imagine you have a large pile of marbles, each representing an atom of a radioactive element. Over time, some of these marbles will change color, representing the atoms that have decayed into a different element or a different isotope.

For instance, in our exercise, radium-230 decays over time, changing into other elements. The speed at which this decay occurs gives us valuable information about the half-life of radium-230, helping us predict how long it will remain radioactive.
Decay Constant
The decay constant, represented by the symbol 'k', is a probability rate at which a particular nuclear species will decay per unit time. It is specific to each radioactive isotope. To grasp this better, think of your daily routine. Certain tasks might be constant like having breakfast or brushing your teeth. Similarly, the decay constant reflects the constant probability that a radium-230 atom will decay in any given hour.

In the exercise solution, the decay constant is calculated using the natural logarithm of the ratio between the initial amount of substance and the amount remaining after a period, divided by the time elapsed. This gives a precise rate of decay for radium-230, which is crucial in determining the half-life of the substance.
Exponential Decay
Exponential decay is the decrease in a quantity according to the law \(N(t) = N_0e^{-kt}\) where \(N_0\) is the initial quantity, \(N(t)\) is the quantity at time \(t\), and \(k\) is the decay constant. Imagine a balloon slowly deflating over time—the air inside it reduces at an exponential rate. Similarly, in the context of radioactive decay, the number of radioactive atoms decreases exponentially over time.

This mechanism is crucial to understanding our exercise as it explains why the amount of radium-230 decreases from 2.00 mg to 0.25 mg in 4 hours and 39 minutes. The half-life calculation is deeply rooted in this concept because it represents the time required for half the atoms in a radioactive sample to decay, which is a direct application of exponential decay behavior.

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Most popular questions from this chapter

In 2010, a team of scientists from Russia and the U.S. reported creation of the first atom of element 117 , which is not yet named and is denoted [117]. The synthesis involved the collision of a target of \({ }^{249}\) Bk with accelerated ions of an isotope which we will denote \(Q\). The product atom, which we will call \({ }_{97}^{249} \mathrm{Bk}+\mathrm{Q} \longrightarrow \mathrm{Z} \longrightarrow{ }_{117}^{294}[117]+3{ }_{0}^{1} \mathrm{n}\)

How much energy must be supplied to break a single \({ }^{21} \mathrm{Ne}\) nucleus into separated protons and neutrons if the nucleus has a mass of \(20.98846\) amu? What is the nuclear binding energy for \(1 \mathrm{~mol}\) of \({ }^{21} \mathrm{Ne}\) ?

Methyl acetate \(\left(\mathrm{CH}_{3} \mathrm{COOCH}_{3}\right)\) is formed by the reaction of acetic acid with methyl alcohol. If the methyl alcohol is labcled with oxygen-18, the oxygen-18 ends up in the methyl acetate: CC(=O)CCCCCC(=O)O (a) Do the \(\mathrm{C}-\mathrm{OH}\) bond of the acid and the \(\mathrm{O}-\mathrm{H}\) bond of the alcohol break in the reaction, or do the \(\mathrm{O}-\mathrm{H}\) bond of the acid and the \(\mathrm{C}-\mathrm{OH}\) bond of the alcohol break? (b) Imagine a similar experiment using the radioisotope \({ }^{3} \mathrm{H}\), which is called tritium and is usually denoted \(\mathrm{T}\). Would the reaction between \(\mathrm{CH}_{3} \mathrm{COOH}\) and \(\mathrm{TOCH}_{3}\) provide the same information about which bond is broken as does the above experiment with \(\mathrm{H}^{18} \mathrm{OCH}_{3}\) ?

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

Calculations Involving Radioactive Decay and Time If we start with \(1.000 \mathrm{~g}\) of strontium- \(90,0.953 \mathrm{~g}\) will remain after \(2.00 \mathrm{yr}\). (a) What is the half-life of strontium- 90 ? (b) How much strontium- 90 will remain after \(5.00 \mathrm{yr}\) ? (c) What is the initial activity of the sample in becquerels and curies? SOLUTION (a) Analyze We are asked to calculate a half-life, \(t_{1 / 2}\) based on data that tell us how much of a radioactive nucleus has decayed in a time interval \(t=2.00 \mathrm{yr}\) and the information \(N_{0}=1.000 \mathrm{~g}, N_{t}=0.953 \mathrm{~g}\). Plan We first calculate the rate constant for the decay, \(k\), and then use that to compute \(t_{1 / 2}\). Solve Equation \(21.19\) is solved for the decay constant, \(k\), and then Equation \(21.20\) is used to calculate half-life, \(t_{1 / 2}\) : $$ \begin{aligned} k &=-\frac{1}{t} \ln \frac{N_{\mathrm{f}}}{N_{0}}=-\frac{1}{2.00 \mathrm{yr}} \ln \frac{0.953 \mathrm{~g}}{1.000 \mathrm{~g}} \\ &=-\frac{1}{2.00 \mathrm{yr}}(-0.0481)=0.0241 \mathrm{yr}^{-1} \\ t_{1 / 2} &=\frac{0.693}{k}=\frac{0.693}{0.0241 \mathrm{yr}^{-1}}=28.8 \mathrm{yr} \end{aligned} $$ (b) Analyze We are asked to calculate the amount of a radionuclide remaining after a given period of time. Plan We need to calculate \(N_{b}\) the amount of strontium present at time \(t\), using the initial quantity, \(N_{0}\), and the rate constant for decay, \(k\), calculated in part (a). Solve Again using Equation \(21.19\), with \(k=0.0241 \mathrm{yr}^{-1}\), we have $$ \ln \frac{N_{t}}{N_{0}}=-k t=-\left(0.0241 \mathrm{yr}^{-1}\right)(5.00 \mathrm{yr})=-0.120 $$ \(N_{t} / N_{0}\) is calculated from \(\ln \left(N_{t} / N_{0}\right)=-0.120\) using the \(e^{x}\) or INV LN function of a calculator: $$ \frac{N_{t}}{N_{0}}=e^{-1.120}=0.887 $$ Because \(N_{0}=1.000 \mathrm{~g}\), we have $$ N_{t}=(0.887) N_{0}=(0.887)(1.000 \mathrm{~g})=0.887 \mathrm{~g} $$ (c) Analyze We are asked to calculate the activity of the sample in becquerels and curies. Plan We must calculate the number of disintegrations per atom per second and then multiply by the number of atoms in the sample. Solve The number of disintegrations per atom per second is given by the decay constant, \(k\) : $$ k=\left(\frac{0.0241}{\mathrm{yr}}\right)\left(\frac{1 \mathrm{yr}}{365 \text { days }}\right)\left(\frac{1 \text { day }}{24 \mathrm{~h}}\right)\left(\frac{\mathrm{lh}}{3600 \mathrm{~s}}\right)=7.64 \times 10^{-10} \mathrm{~s}^{-1} $$ To obtain the total number of disintegrations per second, we calculate the number of atoms in the sample. We multiply this quantity by \(k\), where we express \(k\) as the number of disintegrations per atom per second, to obtain the number of disintegrations per second: $$ \begin{aligned} \left(1.000 \mathrm{~g}^{90} \mathrm{Sr}\right)\left(\frac{1 \mathrm{~mol}^{90} \mathrm{Sr}}{90 \mathrm{~g}^{90} \mathrm{Sr}}\right)\left(\frac{6.022 \times 10^{23} \mathrm{atoms} \mathrm{Sr}}{1 \mathrm{~mol}^{90} \mathrm{Sr}}\right)=6.7 \times 10^{21} \text { atoms }^{90} \mathrm{Sr} \\ \text { Total disintegrations/s } &=\left(\frac{7.64 \times 10^{-10} \text { disintegrations }}{\text { atom }{ }^{2} \mathrm{~s}}\right)\left(6.7 \times 10^{21} \text { atoms }\right) \\ &=5.1 \times 10^{12} \text { disintegrations/s } \end{aligned} $$ Because \(1 \mathrm{~Bq}\) is one disintegration per second, the activity is \(5.1 \times 10^{12} \mathrm{~Bq}\). The activity in curies is given by $$ \left(5.1 \times 10^{12} \text { disintegrations/s }\right)\left(\frac{1 \mathrm{Ci}}{3.7 \times 10^{10} \text { disintegrations/s }}\right)=1.4 \times 10^{2} \mathrm{Ci} $$ We have used only two significant figures in products of these calculations because we do not know the atomic weight of \({ }^{90} \mathrm{Sr}\) to more than two significant figures without looking it up in a special source.

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