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Rubidium- 87 decays by \(\beta\) -particle production to strontium- 87 with a half-life of \(4.7 \times 10^{10}\) years. What is the age of a rock sample that contains \(109.7 \mu \mathrm{g}\) of \({ }^{87} \mathrm{Rb}\) and \(3.1 \mu \mathrm{g}\) of \({ }^{87} \mathrm{Sr}\) ? Assume that no \({ }^{87} \mathrm{Sr}\) was present when the rock was formed. The atomic masses for \({ }^{87} \mathrm{Rb}\) and \({ }^{87} \mathrm{Sr}\) are \(86.90919 \mathrm{u}\) and \(86.90888\) u, respectively.

Short Answer

Expert verified
The age of the rock sample is approximately \(1.69 \times 10^{10}\) years.

Step by step solution

01

Calculate the initial amount of Rubidium-87

Initially, all the Strontium-87 present in the sample would have been Rubidium-87 as it's assumed that no Strontium-87 was present when the rock was formed. So, we can add the current amounts of Rubidium-87 and Strontium-87 in the rock to find the initial amount of Rubidium-87. Initial Rubidium-87 = Current Rubidium-87 + Current Strontium-87 Initial Rubidium-87 = \(109.7\;\mu𝑔\) + \(3.1\;\mu𝑔\) Initial Rubidium-87 = \(112.8\;\mu𝑔\)
02

Calculate the decay constant (λ)

The decay constant (λ) can be calculated using the half-life formula: Half-life (t) = \(\frac{0.693}{\lambda}\) Rearranging to solve for λ: \(\lambda = \frac{0.693}{t}\) Using the given half-life of Rubidium-87, \(4.7 \times 10^{10}\) years: \(\lambda = \frac{0.693}{4.7 \times 10^{10}}\) \(\lambda \approx 1.474\times 10^{-11}\) years\(^{-1}\)
03

Calculate the age of the rock

Now we can use the decay rate formula to calculate the age of the rock: \(N_t = N_0e^{-\lambda t}\) Rearranging to solve for t: \(t = \frac{-\ln(\frac{N_t}{N_0})}{\lambda}\) Where \(N_0\) is the initial amount of Rubidium-87, \(N_t\) is the current amount of Rubidium-87, and \(\lambda\) is the decay constant. Plugging in the values: \(t = \frac{-\ln(\frac{109.7}{112.8})}{1.474\times 10^{-11}}\) \(t \approx 1.690 \times 10^{10}\) years So the age of the rock sample is approximately \(1.69 \times 10^{10}\) years.

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Key Concepts

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

Rubidium-87 Decay
Rubidium-87 is a naturally occurring isotope that undergoes radioactive decay through a process known as beta-particle production. In this process, a neutron in the nucleus of a Rubidium-87 atom is transformed into a proton while emitting a beta particle (an electron) and an antineutrino. This transformation results in the creation of a new element: Strontium-87. Over time, traces of Rubidium-87 in minerals convert steadily to Strontium-87, which can be measured to determine the age of geological samples, such as rocks.
To understand how much Rubidium-87 has decayed, it is important to consider the starting and current amounts in the sample. The original amount of Rubidium can be calculated by summing the present amounts of Rubidium-87 and the Strontium-87 decay product, assuming no Strontium-87 was initially present in the rock:
\[\text{Initial Rb-87} = \text{Current Rb-87} + \text{Current Sr-87}\]This equation is crucial in radiometric dating as it establishes a basis for subsequent age calculations.
Half-life Calculation
Half-life is the time required for half of a radioactive substance to decay into its daughter product. For Rubidium-87, the half-life is particularly long, about \(4.7 \times 10^{10}\) years. This prolonged half-life makes Rubidium-87 an excellent candidate for dating ancient geological events, as it allows for the determination of ages of rocks on a grand scale of billions of years.

The half-life can be mathematically connected to the decay constant using the formula:
\[ t_{1/2} = \frac{0.693}{\lambda} \]
The decay constant \(\lambda\) is a measure of the probability of decay per unit time. Rearranging the expression, we can solve for \(\lambda\) using Rubidium-87's known half-life:
  • \(\lambda = \frac{0.693}{4.7 \times 10^{10}}\)
  • This results in a decay constant approximately equal to \(1.474 \times 10^{-11} \text{ years}^{-1}\).
This relationship is pivotal for transforming the physical half-life into a numerical rate which can then be applied widely in age calculations.
Decay Constant
The decay constant \(\lambda\) is a fundamental part of the radioactive decay equation. It indicates how quickly a particular isotope will decay. For Rubidium-87, with a decay constant around \(1.474 \times 10^{-11} \text{ years}^{-1}\), this value dictates the rate at which it slowly converts to Strontium-87 over time.
The decay constant is used in the exponential decay formula:
  • \(N_t = N_0 e^{-\lambda t}\)
Here, \(N_t\) represents the amount of the radionuclide present after time \(t\), \(N_0\) is the initial quantity, and \(e\) is the base of natural logarithms. By rearranging this formula, researchers can solve for \(t\), the age of the sample.
The derived formula, \(t = \frac{-\ln(\frac{N_t}{N_0})}{\lambda}\), allows scientists to calculate the time elapsed since the formation of the sample. This method is critical in determining geological time scales, effectively turning Rubidium-87 decay into a precise natural clock.

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Most popular questions from this chapter

Fresh rainwater or surface water contains enough tritium \(\left({ }_{1}^{3} \mathrm{H}\right)\) to show \(5.5\) decay events per minute per \(100 . \mathrm{g}\) water. Tritium has a half-life of \(12.3\) years. You are asked to check a vintage wine that is claimed to have been produced in \(1946 .\) How many decay events per minute should you expect to observe in \(100 . \mathrm{g}\) of that wine?

Many transuranium elements, such as plutonium-232, have very short half-lives. (For \({ }^{232} \mathrm{Pu}\), the half-life is 36 minutes.) However, some, like protactinium-231 (half-life \(=3.34 \times\) \(10^{4}\) years), have relatively long half-lives. Use the masses given in the following table to calculate the change in energy when 1 mole of \({ }^{232}\) Pu nuclei and 1 mole of \({ }^{231}\) Pa nuclei are each formed from their respective number of protons and neutrons.

In addition to the process described in the text, a second process called the carbon-nitrogen cycle occurs in the sun: $$ \begin{aligned} { }_{1}^{1} \mathrm{H}+{ }_{6}^{12} \mathrm{C} \longrightarrow{ }_{7}^{13} \mathrm{~N}+{ }_{0}^{0} \gamma \\ { }_{7}^{13} \mathrm{~N} & \longrightarrow{ }_{6}^{13} \mathrm{C}+{ }_{+1}^{0} \mathrm{e} \\ { }_{1}^{1} \mathrm{H}+{ }_{6}^{13} \mathrm{C} &{ }_{7}^{14} \mathrm{~N}+{ }_{0}^{0} \gamma \\ { }_{1}^{1} \mathrm{H}+{ }_{7}^{14} \mathrm{~N} \longrightarrow &{ }_{8}^{15} \mathrm{O}+{ }_{0}^{0} \gamma \\ { }_{8}^{15} \mathrm{O} \longrightarrow{ }_{7}^{15} \mathrm{~N}+{ }_{+1}^{0} \mathrm{e} \\ { }_{1}^{1} \mathrm{H}+{ }_{7}^{15} \mathrm{~N} \longrightarrow{ }_{6}^{12} \mathrm{C}+{ }_{2}^{4} \mathrm{He}+{ }_{0}^{0} \gamma \\ \hline \end{aligned} $$ reaction: \(\quad 4{ }_{1}^{1} \mathrm{H} \longrightarrow{ }_{2}^{4} \mathrm{He}+2{ }_{+1}^{0} \mathrm{e}\) a. What is the catalyst in this process? b. What nucleons are intermediates? c. How much energy is released per mole of hydrogen nuclei in the overall reaction? (The atomic masses of \({ }_{1} \mathrm{H}\) and \({ }_{2}^{4} \mathrm{He}\) are \(1.00782 \mathrm{u}\) and \(4.00260 \mathrm{u}\), respectively. \()\)

Radioactive copper-64 decays with a half-life of \(12.8\) days. a. What is the value of \(k\) in \(\mathrm{s}^{-1}\) ? b. A sample contains \(28.0 \mathrm{mg}^{64} \mathrm{Cu}\). How many decay events will be produced in the first second? Assume the atomic mass of \({ }^{64} \mathrm{Cu}\) is \(64.0 \mathrm{u}\). c. A chemist obtains a fresh sample of \({ }^{64} \mathrm{Cu}\) and measures its radioactivity. She then determines that to do an experiment, the radioactivity cannot fall below \(25 \%\) of the initial measured value. How long does she have to do the experiment?

Scientists have estimated that the earth's crust was formed \(4.3\) billion years ago. The radioactive nuclide \({ }^{176} \mathrm{Lu}\), which decays to \({ }^{176} \mathrm{Hf}\), was used to estimate this age. The half- life of \({ }^{176} \mathrm{Lu}\) is 37 billion years. How are ratios of \({ }^{176} \mathrm{Lu}\) to \({ }^{176} \mathrm{Hf}\) utilized to date very old rocks?

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