One recent estimate concludes that nearly 800 meteorites with mass greater than 100 grams (massive enough to cause personal injury strike the surface of Earth each day. Assuming you present a target of 0.25 square meter \(\left(\mathrm{m}^{2}\right)\) to a falling meteorite, what is the probability that you will be struck by a meteorite during your 100-year lifetime? (Note that the surface area of Earth is approximately \(5 \times 10^{14} \mathrm{m}^{2}\).)

Short Answer

Expert verified
The probability of being struck by a meteorite in 100 years is approximately 1.46 x 10^-6%.

Step by step solution

01

- Find the Daily Probability per Square Meter

Start with the given data: there are 800 meteorites falling each day on Earth's surface, which is approximately \(5 \times 10^{14} \text { m}^2\). The probability of one meteorite hitting any given square meter each day is: \[ \frac{800}{5 \times 10^{14}} \text{ per } \text{m}^2 \text{ per day}. \]
02

- Calculate the Daily Probability for a 0.25 \text { square meter target}

Multiply the probability by the area you present (0.25 square meters): \[ \text{Probability per day per 0.25 m}^2 = 0.25 \times \frac{800}{5 \times 10^{14}}. \] Result: \[ \text{Daily Probability} = \frac{200}{5 \times 10^{14}} = \frac{2}{5 \times 10^{12}}. \]
03

- Calculate the Yearly Probability

There are 365 days in a year, so your yearly probability of being hit by a meteorite is: \[ \text{Yearly Probability} = 365 \times \frac{2}{5 \times 10^{12}} = \frac{730}{5 \times 10^{12}} = 1.46 \times 10^{-10}. \]
04

- Calculate the Lifetime Probability

Assuming a 100-year lifetime, multiply the yearly probability by 100: \[ \text{Lifetime Probability} = 100 \times 1.46 \times 10^{-10} = 1.46 \times 10^{-8}. \]
05

- Convert Probability to a Percentage

To convert this into a percentage chance: \[ \text{Lifetime Probability (\text{%})} = 1.46 \times 10^{-8} \times 100 = 1.46 \times 10^{-6} \text{%}. \]

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Key Concepts

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

Probability Calculations
Probability calculations help us determine the likelihood of events happening. In this exercise, we calculated the probability of being hit by a meteorite using several steps. We started with the total number of meteorites that fall on Earth each day and divided it by the Earth's surface area to find the daily probability of a meteorite striking any specific square meter.
To refine this probability for a 0.25 square meter area, we multiplied by the target area. Then, by considering multiple days, we scaled this up from daily to yearly probability, and finally to a lifetime probability. The result gives us a clear understanding of the chances over different time frames.
By converting the final value into a percentage, we can more intuitively understand the extremely low likelihood of such an event.
Surface Area
Understanding surface area is crucial in our problem. Earth's surface area is approximately \[ 5 \times 10^{14} \text{ m}^2 \].
Surface area is basically the measure of how much exposed area an object has. To put it into perspective, it’s like calculating the amount of wrapping paper needed to cover Earth entirely. For meteorite impacts, the larger the surface area, the more spread out the impacts will be.
When calculating probabilities, knowing the exact area being considered (both Earth's overall surface and your specific target area of 0.25 square meters) directly affects result. Larger areas present larger targets and hence higher probabilities of being struck.
Meteorite Impact
Meteorite impacts are rare but fascinating phenomena. Each day, Earth gets hit by about 800 meteorites with a mass greater than 100 grams—enough to cause personal injury. These space rocks come in various sizes and shapes.
The chances of a meteorite hitting an individual are incredibly slim because they are spread over Earth’s vast surface. However, when they do strike, they can cause significant damage. Understanding the rare probability of encountering a meteorite impact firsthand can underscore the sheer size of Earth and how sparse these events are.
Such insights also highlight the importance of large-scale studies to comprehend cosmic events' probability, further emphasizing our tiny existence in the vast universe.
Mathematical Estimation
Mathematical estimation involves approximating values to make calculations more manageable, which is what we did in this exercise. We estimated the significant figures and utilized these approximations to perform the probability calculations.
We began with simplified values, such as Earth’s surface area (\[5 \times 10^{14} \] square meters), and daily meteorite impacts (800 per day). These approximations allowed us to understand and calculate the overall probability without dealing with excessively precise numbers that would complicate our computations.
By efficiently estimating each step, we turned a complex real-world problem into a more comprehendible and solvable one.

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Most popular questions from this chapter

Comet Halley has a mass of approximately \(2.2 \times 10^{14} \mathrm{kg} .\) It loses about \(3 \times 10^{11} \mathrm{kg}\) each time it passes the Sun. a. The first confirmed observation of the comet was made in 240 BCE. Assuming a constant period of 76.4 years, how many times has it reappeared since that early sighting? b. How much mass has the comet lost since 240 BCE? c. What percentage of the comet's total mass today does this amount represent?

The estimated amount of zodiacal dust in the Solar System remains constant at approximately \(10^{16}\) kg. Yet zodiacal dust is constantly being swept up by planets or removed by the pressure of sunlight. a. If all the dust disappeared (at a constant rate) over a span of 30,000 years, what would the average production rate, in kilograms per second, have to be to maintain the current content? b. Is this an example of static or dynamic equilibrium? Explain your answer.

Dwarf planets: a. Go to planetary astronomer Mike Brown's website of dwarf planets (http://gps.caltech.edu/-mbrown/dps.html). How many dwarf planets does he think are in the Solar System? Why is it difficult officially to certify an object as a dwarf planet? b. Go to the website for the New Horizons mission (http://pluto .jhuapl.edu), which reached Pluto in 2015 and is scheduled to visit Kuiper Belt objects afterward. Click on "Where Is New Horizons?" What is the spacecraft's current location? How far is it from Earth, and how far from Pluto? How long would it take to send a radio signal to the spacecraft? Click on "News Center." What has been learned from this mission?

Ceres has a diameter of \(975 \mathrm{km}\) and a period of about 9 hours. What is the rotational speed of a point on the surface of this dwarf planet?

By what criteria did Pluto fail to be considered a planet under the new IAU definition? Explain how this decision demonstrates the self-correcting nature of science.

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