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The speed at which certain animals run is a power function of their stride length, and the power is \(k=1.7\). (See Figure 5.39.) If one animal has a stride length three times as long as another, how much faster does it run?

Short Answer

Expert verified
The second animal runs approximately 6.961 times faster than the first.

Step by step solution

01

Identify the Given Information

We are given that the speed, \( v \), of an animal is a power function of its stride length, \( l \). The equation can be expressed as \( v = C \times l^k \), where \( C \) is a constant and \( k = 1.7 \). We are also told that the stride length of one animal is three times that of another, i.e., \( l_2 = 3l_1 \).
02

Set Up the Equation for Each Animal

For the first animal with stride length \( l_1 \), the speed is \( v_1 = C \times l_1^{1.7} \). For the second animal with stride length \( l_2 = 3l_1 \), the speed is \( v_2 = C \times (3l_1)^{1.7} \).
03

Simplify the Equation for the Second Animal

Substitute \( l_2 = 3l_1 \) into the speed equation for the second animal: \[ v_2 = C \times (3l_1)^{1.7} = C \times 3^{1.7} \times l_1^{1.7} \]
04

Divide the Speeds to Find the Ratio

To find out how much faster the second animal runs compared to the first, calculate the ratio \( \frac{v_2}{v_1} \):\[ \frac{v_2}{v_1} = \frac{C \times 3^{1.7} \times l_1^{1.7}}{C \times l_1^{1.7}} = 3^{1.7} \]
05

Calculate \( 3^{1.7} \)

Compute \( 3^{1.7} \) using a calculator. This yields approximately 6.961. Therefore, the second animal runs about 6.961 times faster than the first.

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Key Concepts

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

Stride Length
Stride length is a crucial element in understanding the movement of animals, particularly in relation to their speed. It refers to the distance covered in one complete step of an animal's movement cycle. In simpler terms, it's the distance between two consecutive points where the same foot touches the ground. This measurement can vary greatly among different species and is influenced by factors such as limb length and body size. In this context, stride length is particularly important because it scales with speed according to a power function.

When thinking about stride length, consider its impact on how an animal moves. Imagine two animals moving side by side, one with a stride length thrice that of the other. You would expect the animal with the longer stride to cover more ground with each step.

This concept is practical and easily observable. For instance, if you watch a horse galloping, it has long, powerful strides which enable it to achieve high speeds. Contrast this with a smaller animal like a rabbit, which has shorter strides but compensates with rapid, consecutive leaps. Understanding stride length helps in predicting the speed potential of various animals based on their physical characteristics.
Speed and Velocity
Speed and velocity might seem like they’re the same, but they have distinct meanings in physics. Speed is a scalar quantity that only considers magnitude—how fast something is moving. On the other hand, velocity is a vector quantity, meaning it considers both magnitude and direction.

Imagine you’re running around a track. Your speed is how fast you're running, for example, 10 meters per second. Your velocity, however, also takes into account that you’re running in a circular path, not just linearly in one direction.

In the context of our problem, the speed of an animal is influenced by its stride length through a power function. This power function tells us that as the stride length increases, speed increases by a factor determined by the exponent. Here, with an exponent of 1.7, the relationship isn’t linear, and that’s why a threefold increase in stride length results in more than just a threefold increase in speed. It gives us a measure of how effectively animals can convert stride length to speed.

Keeping these distinctions clear helps in understanding the deeper mechanics of motion described through mathematical modeling.
Algebraic Modeling
Algebraic modeling is a powerful technique used to represent real-world problems with mathematical equations. In this problem, we model the relationship between stride length and speed with a power function. This type of function is represented like this:
  • Speed, \( v \), is proportional to stride length, \( l \), raised to the power of \( k \).
  • This can be expressed as \( v = C \times l^k \), where \( C \) is some constant derived from factors like biology or environment, and \( k \) is the discovered power from empirical data, here 1.7.
Creating models like this helps simplify and quantify complex relationships so we can predict outcomes, such as speed from stride length.

In the given exercise, when the stride of one animal is three times another’s, we substitute this relation into the model’s equation. It shows using basic algebra how this stride difference leads to a significant speed difference, quantified by calculating \( 3^{1.7} \).

Algebraic models enable us to manipulate and explore how changes in one variable might affect another, providing valuable insights into the fundamental characteristics of diverse phenomena.

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Most popular questions from this chapter

A biologist has discovered that the weight of a certain fish is a power function of its length. He also knows that when the length of the fish is doubled, its weight increases by a factor of 8 . What is the power \(k\) ?

The following formula \({ }^{71}\) can be used to approximate the average transit speed \(S\) of a public transportation vehicle: $$ S=\frac{C D}{C T+D+C^{2}\left(\frac{1}{2 a}+\frac{1}{2 d}\right)} $$ Here \(C\) is the cruising speed in miles per hour, \(D\) is the average distance between stations in miles, \(T\) is the stop time at stations in hours, \(a\) is the rate of acceleration in miles per hour per hour, and \(d\) is the rate of deceleration in miles per hour per hour. For a certain subway the average distance between stations is 3 miles, the stop time is 3 minutes \((0.05\) hour), and rate of acceleration and deceleration are both \(3.5\) miles per hour per second (12,600 miles per hour per hour). a. Using the information provided, express \(S\) as a rational function of \(C\). b. As a rule of thumb, we might use the cruising speed as an estimate of transit speed. Discuss the merits of such a rule of thumb. How does increasing cruising speed affect such an estimate? (Suggestion: Compare the graph of the given rational function with that of the graph of \(S=C\).) c. What cruising speed will yield a transit speed of 30 miles per hour?

This is a continuation of Exercise 5. Table \(5.4\) gives the length \(L\), in inches, of a swimming animal and its maximum speed \(S\), in feet per second, when it swims. a. Find a formula for the regression line of \(\ln S\) against \(\ln L\). (Round the slope to one decimal place.) b. Find a formula that models \(S\) as a power function of \(L\). On the basis of the power you found, what special type of power function is this? $$ \begin{array}{|l|c|c|} \hline \text { Animal } & \text { Length } L & \begin{array}{c} \text { Swimming } \\ \text { speed } S \end{array} \\ \hline \text { Bacillus } & 9.8 \times 10^{-5} & 4.9 \times 10^{-5} \\ \hline \text { Paramecium } & 0.0087 & 0.0033 \\ \hline \text { Water mite } & 0.051 & 0.013 \\ \hline \text { Flatfish larva } & 0.37 & 0.38 \\ \hline \text { Goldfish } & 2.8 & 2.5 \\ \hline \text { Dace } & 5.9 & 5.7 \\ \hline \text { Adélie penguin } & 30 & 12.5 \\ \hline \text { Dolphin } & 87 & 33.8 \\ \hline \end{array} $$ c. Add the graph of \(S\) against \(L\) to the graph of \(F\) that you drew in Exercise \(5 .\) d. Is flying a significant improvement over swimming if an animal is 1 foot long (the approximate length of a flying fish)? e. Would flying be a significant improvement over swimming for an animal 20 feet long? f. A blue whale is about 85 feet long, and its maximum speed swimming is about 34 feet per second. Judging on the basis of these facts, do you think the trend you found in part b continues indefinitely as the length increases?

Poiseuillé's law describes the velocities of fluids flowing in a tube-for example, the flow of blood in a vein. (See Figure 5.104.) This law applies when the velocities are not too large-more specifically, when the flow has no turbulence. In this case the flow is laminar, which means that the paths of the flow are all parallel to the tube walls. The law states that $$ v=k\left(R^{2}-r^{2}\right), $$ where \(v\) is the velocity, \(k\) is a constant (which depends on the fluid, the tube, and the units used for measurement), \(R\) is the radius of the tube, and \(r\) is the distance from the centerline of the tube. Since \(k\) and \(R\) are fixed for any application, \(v\) is a function of \(r\) alone, and the formula gives the velocity at a point of distance \(r\) from the centerline of the tube. a. What is \(r\) for a point along the walls of the tube? What is the velocity of the fluid along the walls of the tube? b. Where in the tube does the fluid flow most rapidly? c. Choose numbers for \(k\) and \(R\) and make a graph of \(v\) as a function of \(r\). Be sure that the horizontal span for \(r\) goes from 0 to \(R\). d. Describe your graph from part c. e. Explain why you needed to use a horizontal span from 0 to \(R\) in order to describe the flow throughout the tube.

Binary stars are pairs of stars that orbit each other. The period \(p\) of such a pair is the time, in years, required for a single orbit. The separation \(s\) between such a pair is measured in seconds of arc. The parallax angle \(a\) (also in seconds of arc) for any stellar object is the angle of its apparent movement as the Earth moves through one half of its orbit around the sun. Astronomers can calculate the total mass \(M\) of a binary system using $$ M=s^{3} a^{-3} p^{-2} . $$ Here \(M\) is the number of solar masses. a. Alpha Centauri, the nearest star to the sun, is in fact a binary star. The separation of the pair is \(s=17.6\) seconds of arc, its parallax angle is \(a=0.76\) second of arc, and the period of the pair is \(80.1\) years. What is the mass of the Alpha Centauri pair? b. How would the mass change if the separation angle were doubled but parallax and period remained the same as for the Alpha Centauri system? c. How would the mass change if the parallax angle were doubled but separation and period remained the same? d. How would the mass change if the period doubled but parallax angle and separation remained the same?

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