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Fresh rainwater or surface water contains enough tritium \(\left({ }^{3} \mathrm{H}\right)\) 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?

Short Answer

Expert verified
You should expect to observe about 0.0596 decay events per minute in 100g of the vintage wine claimed to have been produced in 1946.

Step by step solution

01

Calculate the number of half-lives

First, we have to find out how many half-lives have passed since 1946. We can accomplish this by dividing the time elapsed (from 1946 to now) by the half-life of tritium. Let's assume it is the year 2022. The elapsed time will be: Elapsed time = Current year - Vintage year Elapsed time = 2022 - 1946 = 76 years Now, divide the elapsed time by the half-life of tritium to find the number of half-lives: Number of half-lives = Elapsed time / Half-life of tritium Number of half-lives = 76 years / 12.3 years
02

Calculate the decay events per minute in the wine

Now that we know the number of half-lives, we can use this information to determine the decay events per minute in 100g of the wine. We can use the half-life formula, with the initial decay events per minute in rainwater or surface water, and the number of half-lives: Decay events per minute = Initial decay events per minute x (1 / 2) ^ Number of half-lives Decay events per minute = 5.5 events per minute x (1 / 2) ^ (76 years / 12.3 years)
03

Calculate the final answer

Now, we will simplify the expression to find the decay events per minute in the wine: Decay events per minute ≈ 5.5 events per minute x (1 / 2) ^ (6.178861788619) Decay events per minute ≈ 5.5 events per minute x 0.0108422274 Decay events per minute ≈ 0.05963225 events per minute Therefore, you should expect to observe about 0.0596 decay events per minute in 100g of the vintage wine claimed to have been produced in 1946.

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Key Concepts

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

Half-Life of Radioactive Isotopes
Understanding the half-life of radioactive isotopes is crucial in various fields, from archaeology to medicine. Half-life is the time required for half the atoms in a sample of a radioactive isotope to decay.

For instance, if we start with 100 unstable atoms with a half-life of one year, we'd expect to have 50 left after one year, 25 after two years, and so on. In our example with tritium \( ^3H \), which has a half-life of 12.3 years, it takes that amount of time for half of the tritium atoms in the sample to transform into another element through the process of radioactive decay.

When examining vintage wine for authentication, knowing the half-life allows us to calculate the decrease in radioactivity over time. This calculation is based on the assumption that the initial amount of tritium was known and that its decrease follows a predictable pattern described by the half-life.
Nuclear Chemistry
Nuclear chemistry deals with the reactions and processes that occur within atomic nuclei. Radioactive decay, a spontaneous process by which an unstable atomic nucleus loses energy, is a key concept in this field.

Tritium decay—where the tritium nucleus \( ^3H \) decomposes into a stable helium isotope \( ^3He \)—is a prime example of beta decay, one type of radioactive decay.

Why is tritium decay significant?

Its presence in organic matter like wine allows us to date its production. This is due to the predictability of nuclear processes, which can be described using mathematical models. Thus, nuclear chemistry not only elucidates how these decays occur but also provides tools to measure time and verify historical claims, as is the goal in testing the vintage wine.
Scientific Problem-Solving
Scientific problem-solving involves using a systematic approach to understand and resolve complex issues. Here's how we applied it:

Firstly, we identified our primary objective: to determine the number of decay events per minute in the vintage wine. Secondly, we gathered necessary data, such as the half-life of tritium and the initial decay events in contemporary water samples.

Then, using a mathematical formula that incorporates the concept of half-life, we calculated the expected decay events. To achieve a clearer and more reliable outcome, we meticulously implemented each step, ensuring careful consideration of each variable. This approach exemplifies how precision and methodical procedures are essential to scientific inquiry and finding solutions to intricate problems like determining the age of a vintage wine based on radioactive isotope decay.

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Most popular questions from this chapter

A \(0.10-\mathrm{cm}^{3}\) sample of a solution containing a radioactive nuclide \(\left(5.0 \times 10^{3}\right.\) counts per minute per milliliter) is injected into a rat. Several minutes later \(1.0 \mathrm{~cm}^{3}\) blood is removed. The blood shows 48 counts per minute of radioactivity. Calculate the volume of blood in the rat. What assumptions must be made in performing this calculation?

Photosynthesis in plants can be represented by the following overall reaction: $$6 \mathrm{CO}_{2}(g)+6 \mathrm{H}_{2} \mathrm{O}(l) \stackrel{\text { Light }}{\longrightarrow} \mathrm{C}_{6} \mathrm{H}_{12} \mathrm{O}_{6}(s)+6 \mathrm{O}_{2}(g)$$ Algae grown in water containing some \({ }^{18} \mathrm{O}\) (in \(\mathrm{H}_{2}{ }^{18} \mathrm{O}\) ) evolve oxygen gas with the same isotopic composition as the oxygen in the water. When algae growing in water containing only \({ }^{16} \mathrm{O}\) were furnished carbon dioxide containing \({ }^{18} \mathrm{O}\), no \({ }^{18} \mathrm{O}\) was found to be evolved from the oxygen gas produced. What conclusions about photosynthesis can be drawn from these experiments?

Breeder reactors are used to convert the nonfissionable nuclide \({ }_{92}^{238} \mathrm{U}\) to a fissionable product. Neutron capture of the \({ }_{92}^{238} \mathrm{U}\) is followed by two successive beta decays. What is the final fissionable product?

The most stable nucleus in terms of binding energy per nucleon is \({ }^{56} \mathrm{Fe}\). If the atomic mass of \({ }^{56} \mathrm{Fe}\) is \(55.9349 \mathrm{amu}\), calculate the binding energy per nucleon for \({ }^{56} \mathrm{Fe}\).

Write an equation describing the radioactive decay of each of the following nuclides. (The particle produced is shown in parentheses, except for electron capture, where an electron is a reactant.) a. \({ }^{68} \mathrm{Ga}\) (electron capture) c. \({ }^{212} \mathrm{Fr}(\alpha)\) b. \(^{62} \mathrm{Cu}\) (positron) d. \({ }^{129} \mathrm{Sb}(\beta)\)

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