If a radioactive element has a half-life of 10,000 years, what fraction of it is left in a rock after 40,000 years? a. \(1 / 2\) b. \(1 / 4\) c. \(1 / 8\) d. \(1 / 16\) e. \(1 / 32\)

Short Answer

Expert verified
The fraction of the radioactive element left after 40,000 years is \[\frac{1}{16}\].

Step by step solution

01

Understanding the half-life

The half-life of a substance is the time it takes for half of the material to decay. Here, the half-life is 10,000 years.
02

Calculate the number of half-lives elapsed

To find how many half-lives have passed, divide the total time by the half-life. So, \[\text{Number of half-lives} = \frac{40,000 \text{ years}}{10,000 \text{ years/half-life}} = 4 \text{ half-lives}\]
03

Determine the remaining fraction after each half-life

With each half-life, half of the remaining material decays. After 1 half-life, \[\frac{1}{2} \text{ is left}\] After 2 half-lives, \[\frac{1}{4} \text{ is left}\] After 3 half-lives, \[\frac{1}{8} \text{ is left}\] After 4 half-lives, \[\frac{1}{16} \text{ is left}\]
04

Conclude the fraction remaining after 40,000 years

Since 4 half-lives have elapsed, the fraction of the radioactive element left is \[\frac{1}{16}\]

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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 a process where unstable atomic nuclei lose energy by emitting radiation. This can happen in the form of alpha, beta, or gamma radiation. The rate at which a radioactive substance decays is constant and unique to each element. This rate is often described in terms of half-life. Understanding radioactive decay is crucial in fields like nuclear medicine, archaeology, and geology. The decay is spontaneous and cannot be influenced by external conditions like temperature or pressure. As the substance decays, it transforms into a different element or a different isotope of the same element.
Half-life
The term 'half-life' refers to the time it takes for half of the radioactive atoms in a sample to decay. It is denoted by the symbol \(\tau_{1/2}\). For instance, if a substance has a half-life of 10,000 years, this means that after 10,000 years, only half of the original radioactive atoms will remain. After another 10,000 years, half of the remaining atoms will decay, leaving only a quarter (\(\frac{1}{4}\)) of the original number of atoms. This pattern continues with each successive half-life. To calculate the fraction left after a certain number of half-lives, you can use the formula: \[ \text{Remaining fraction} = \frac{1}{2^n} \] where \( n \) is the number of half-lives that have elapsed.
Exponential decay
Exponential decay describes any process that decreases at a rate proportional to its current value. In the context of radioactivity, the number of undecayed radioactive atoms decreases exponentially over time. This means that the decay is rapid at first but slows down as time passes. The general formula for exponential decay is given by: \[ N(t) = N_0 e^{-\frac{t}{\tau}} \] where \( N(t) \) is the quantity of substance at time \( t \), \( N_0 \) is the initial quantity, \( e \) is the base of natural logarithms, and \( \tau \) is the mean lifetime of the substance. Although this formula is robust, the half-life formula is often used because it is simpler to understand and apply in real-world scenarios.

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Most popular questions from this chapter

Different radioisotopes have different half-lives. For example, the half-life of carbon-14 is 5,700 years, the half-life of uranium- 235 is 704 million years, the half-life of potassium- 40 is 1.3 billion years, and the half-life of rubidium-87 is 49 billion years. a. Why wouldn't you use an isotope with a half-life similar to that of carbon-14 to determine the age of the Solar System? b. The age of the universe is approximately 14 billion years. Does that mean that no rubidium- 87 has decayed yet?

Video: Watch one of the available documentaries about the Apollo missions to the Moon (for example, In the Shadow of the Moon, 2008 ). Why did the United States decide to send astronauts to the Moon? Why did the Apollo program end? Are there current plans to send people to the Moon? b. The first science fiction film was the short Voyage to the Moon (Georges Méliès, 1902 ). A version with an English narration can be viewed at https://archive.org/details/ Levoyagedanslalune. A restored digitized and colorized version was released in 2011 and can be found at http: \(/ /\) vimeo.com/39275260. Where do the "Selenians" live on the Moon? In this first cinematic depiction of contact with life from outside of Earth, what do the human astronomers do to the Selenians? Contrast what the astronomers in the film find on the Moon with what the \(A\) pollo astronauts actually saw.

Explain how scientists know that rock layers at the bottom of the Grand Canyon are older than those found on the rim.

Earth has fewer craters than Venus. Why? a. Earth's atmosphere protects better than Venus's. b. Earth is a smaller target than Venus. c. Earth is closer to the asteroid belt. d. Earth's surface experiences more erosion.

Citizen science: a. Go to the website for "Moon Zoo" (http://moonzoo.org), a project that lets everyone participate in the analysis of images from NASA's Lunar Reconnaissance Orbiter. Read through the FAQ, then click on "Tutorials" and select "How to Take Part." (You will need to create an account if you haven't already done so for another Zooniverse project.) In this project you count craters on the Moon, noting where there are boulders, classifying some of these features, and looking for hardware left over from exploration missions. b. Go to the website for cosmoquest (http://cosmoquest.org) and click on "Mercury Mappers." You will need to create an account for the cosmoquest projects. Click on the circled question mark under the blue check box, and read the FAQ and watch the tutorial. What is the goal of this project? Where did the data come from? Classify some images. c. Go to the website for cosmoquest (http://cosmoquest.org) and click on "Moon Mappers." As in part (b), you will need an account. Click on the circled question mark under the blue check box and read the FAQ and watch the four tutorials. What are some of the basic features? How does the angle of the sunlight and the direction of illumination affect what you see? Now classify a few craters.

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