In the previous section we saw that inverse variation can be expressed as a power function by using negative exponents. We can also use exponents to denote square roots and other radicals.
Subsection6.2.1\(n^\text{th}\) Roots
Recall that \(s\) is a square root of \(b\) if \(s^2 = b\text{,}\) and \(s\) is a cube root of \(b\) if \(s^3 = b\text{.}\) In a similar way, we can define the fourth, fifth, or sixth root of a number. For instance, the fourth root of \(b\) is a number \(s\) whose fourth power is \(b\text{.}\)
\(n\)th Roots.
\(s\) is called an \(n\)th root of \(b\) if \(\blert{s^n = b}\text{.}\)
We use the symbol \(\sqrt[n]{b}\) to denote the \(n\)th root of \(b\text{.}\) An expression of the form \(\sqrt[n]{b}\) is called a radical, \(b\) is called the radicand, and \(n\) is called the index of the radical.
A convenient notation for radicals uses fractional exponents. Consider the expression \(9^{1/2}\text{.}\) What meaning can we attach to an exponent that is a fraction? The third law of exponents says that when we raise a power to a power, we multiply the exponents together:
What about \(n\)th roots such as \(\sqrt{23}\) and \(5^{1/3}\) that cannot be evaluated easily? These are examples of irrational numbers. An irrational number is one that cannot be expressed as a quotient of two integers.
It is not possible to write down an exact decimal equivalent for an irrational number, but we can find an approximation to as many decimal places as we like. We can use a calculator to obtain decimal approximations for irrational numbers. For example, you can verify that
The following keying sequence for evaluating the irrational number \(7^{1/5}\) is incorrect:
7 ^ 1 ÷ 5 ENTER
You can check that this sequence calculates \(\dfrac{7^1}{5}\text{,}\) instead of \(7^{1/5}\text{.}\) Recall that according to the order of operations, powers are computed before multiplications or divisions. We must enclose the exponent \(1/5\) in parentheses and enter
7 ^ ( 1 ÷ 5 ) ENTER
Or, because \(\dfrac{1}{5}= 0.2\text{,}\) we can enter
7 ^ 0.2 ENTER
Subsection6.2.4Working with Fractional Exponents
Fractional exponents simplify many calculations involving radicals. You should learn to convert easily between exponential and radical notation.
In Example 6.2.16d, note that the exponent \(-1/4\) applies only to \(a\text{,}\) not to \(8a\text{.}\) Compare with \((8a)^{-1/4} = \dfrac{1}{\sqrt[4]{8a}}\)
Subsection6.2.5Using Fractional Exponents to Solve Equations
We know that raising to powers and taking roots are inverse operations, that is, each operation undoes the effects of the other. This relationship is especially easy to see when the root is denoted by a fractional exponent. For example, to solve the equation
\begin{equation*}
x^5 = 250
\end{equation*}
we would take the fifth root of each side. But instead of using radical notation, we can raise both sides of the equation to the power \(\dfrac{1}{5}\text{:}\)
\begin{align*}
\left(x^5\right)^{1/5} \amp= 250^{1/5}\\
x \amp \approx 3.017
\end{align*}
The third law of exponents tells us that \(\left(x^a\right)^b = x^{ab}\text{,}\) so
Thus, to solve an equation involving a power function \(x^n\text{,}\) we first isolate the power, then raise both sides to the exponent \(\dfrac{1}{n}\text{.}\)
For astronomers, the mass of a star is its most important property, but it is also the most difficult to measure directly. For many stars, their luminosity, or brightness, varies roughly as the fourth power of the mass.
Our Sun has luminosity \(4 \times 10^{26}\) watts and mass \(2 \times 10^{30}\) kilograms. Because the numbers involved are so large, astronomers often use these solar constants as units of measure: The luminosity of the Sun is \(1\) solar luminosity, and its mass is \(1\) solar mass. Write a power function for the luminosity, \(L\text{,}\) of a star in terms of its mass, \(M\text{,}\) using units of solar mass and solar luminosity.
The star Sirius is 23 times brighter than the Sun, so its luminosity is 23 solar luminosities. Estimate the mass of Sirius in units of solar mass.
The size of a diamond is usually given by its weight \(w\) in carats. The diameter, \(D\text{,}\) of a diamond cut in a traditional round style is then a power function of its weight, given by
A diamond weighing one-quarter carat has diameter about 4.05 millimeters. Find the constant of proportionality, \(k\text{,}\) and write a formula for \(D\) as a function of \(w\text{.}\)
Complete the table with the diameters of diamonds of various weights.
\(w~\) (carats)
\(0\)
\(0.5\)
\(0.75\)
\(1.0\)
\(1.25\)
\(1.5\)
\(2.0\)
\(2.5\)
\(3.0\)
\(D~\) (mm)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
\(~~~\)
Sketch a graph of the function \(D=f(w)\text{.}\)
What is the diameter of the Hope Diamond, which weighs 45.52 carats and is worth $300 million?
According to our formula, the Hope Diamond is about 22.85 millimeters in diameter.
Of course, power functions can be expressed using any of the notations we have discussed. For example, the function in the Example above can be written as
A radical equation is one in which the variable appears under a square root or other radical. The radical may be denoted by a fractional exponent. For example, the equation
\begin{equation*}
5x^{1/3} = 32
\end{equation*}
is a radical equation because \(x^{1/3} = \sqrt[3]{x}\text{.}\) To solve the equation, we first isolate the power to get
\begin{equation*}
x^{1/3} = 6.4
\end{equation*}
Then we raise both sides of the equation to the reciprocal of \(\dfrac{1}{3}\text{,}\) or \(3\text{.}\)
\begin{align*}
\left(x^{1/3}\right)^3 \amp = 6.4^3\\
x \amp = 262.144
\end{align*}
When a car brakes suddenly, its speed can be estimated from the length of the skid marks it leaves on the pavement. A formula for the car’s speed, in miles per hour, is
\begin{equation*}
v = f(d) = (24d)^{1/2}
\end{equation*}
where the length of the skid marks, \(d\text{,}\) is given in feet.
If a car leaves skid marks 80 feet long, how fast was the car traveling when the driver applied the brakes?
How far will a car skid if its driver applies the brakes while traveling 80 miles per hour?
The car was traveling at approximately 44 miles per hour.
We would like to find the value of \(d\) when the value of \(v\) is known. We substitute \(v = \alert{80}\) into the formula and solve the equation
\begin{equation*}
\alert{80} = (24d)^{1/2} ~~ \blert{\text{ Solve for }d.}
\end{equation*}
Because \(d\) appears to the power \(\frac{1}{2}\text{,}\) we first square both sides of the equation to get
\begin{align*}
80^2 \amp = \left((24d)^{1/2}\right)^2 \amp\amp \blert{\text{Square both sides.}}\\
6400 \amp = 24d \amp\amp \blert{\text{Divide by }24.}\\
266.\overline{6} \amp = d
\end{align*}
You can check that this value for \(d\) works in the original equation. Thus, the car will skid approximately 267 feet. A graph of the function \(v = (24d)^{1/2}\) is shown below, along with the points corresponding to the values in parts (a) and (b).
Note6.2.25.
Thus, we can solve an equation where one side is an \(n\)th root of \(x\) by raising both sides of the equation to the \(n\)th power. We must be careful when raising both sides of an equation to an even power, since extraneous solutions may be introduced. However, because most applications of power functions deal with positive numbers only, they do not usually involve extraneous solutions.
You already know that \(\sqrt{-9}\) is not a real number, because there is no real number whose square is \(-9\text{.}\) Similarly, \(\sqrt[4]{-16}\) is not a real number, because there is no real number \(r\) for which \(r^4 = -16\text{.}\) (Both of these radicals represent complex numbers.) In general, we cannot find an even root (square root, fourth root, and so on) of a negative number.
On the other hand, every positive number has two even roots that are real numbers. For example, both \(3\) and \(-3\) are square roots of \(9\text{.}\) The symbol \(\sqrt{9}\) refers only to the positive, or principal root, of \(9\text{.}\) If we want to refer to the negative square root of \(9\text{,}\) we must write \(-\sqrt{9} = -3\text{.}\) Similarly, both \(2\) and \(-2\) are fourth roots of \(16\text{,}\) because \(2^4 = 16\) and \((-2)^4 = 16\text{.}\) However, the symbol \(\sqrt[4]{16}\) refers to the principal, or positive, fourth root only. Thus,
Things are simpler for odd roots (cube roots, fifth roots, and so on). Every real number, whether positive, negative, or zero, has exactly one real-valued odd root. For example,
When a ship moves through the water, it creates waves that hinder its own progress. Because of this resistance, there is an upper limit to the speed at which a ship can travel, given in knots by
where \(L\) is the length of the vessel in feet. (Source: Gilner, 1972)
Complete the table of values for \(v_{\text{max}}\) as a function of \(L\text{.}\)
\(L\) (feet)
\(200\)
\(400\)
\(600\)
\(800\)
\(1000\)
\(v_{\text{max}}\) (knots)
\(\)
\(\)
\(\)
\(\)
\(\)
Graph maximum speed against vessel length.
The largest ship ever built, the oil tanker Seawise Giant, was 1,504 feet long. What was its top speed?
As a ship approaches its maximum speed, the power required increases sharply. Therefore, most merchant ships are designed to cruise at speeds no higher than
If you walk in the normal way, your speed, \(v\text{,}\) in meters per second, is limited by the length of your legs, \(r\text{,}\) according to the formula
\begin{equation*}
v \le \sqrt{gr}
\end{equation*}
where \(g\) is the acceleration due to gravity. (Source: Alexander, 1992)
Complete the table of values for \(v\) as a function of \(r\text{.}\) The constant, \(g\text{,}\) is approximately 10.
\(r\) (meters)
\(0.2\)
\(0.4\)
\(0.6\)
\(0.8\)
\(1.0\)
\(v\) (meters/sec)
\(\)
\(\)
\(\)
\(\)
\(\)
A typical adult man has legs about 0.9 meter long. How fast can he walk?
A typical four-year-old has legs 0.5 meter long. How fast can she walk?
Graph maximum walking speed against leg length.
Race-walkers can walk as fast as 4.4 meters per second by rotating their hips so that the effective length of their legs is increased. What is that effective length?
On the moon the value of \(g\) is 1.6. How fast can a typical adult man walk on the moon?
33.
The period of a pendulum is the time it takes for the pendulum to complete one entire swing, from left to right and back again. The greater the length, \(L\text{,}\) of the pendulum, the longer its period, \(T\text{.}\) In fact, if \(L\) is measured in feet, then the period is given in seconds by
The rate, \(r\text{,}\) in feet per second, at which water flows from a fire hose varies directly with the square root of the water pressure, \(P\text{,}\) in psi (pounds per square inch). What is the rate of water flow at a typical water pressure of 60 psi?
\(P\) (psi)
\(10\)
\(20\)
\(30\)
\(40\)
\(r\) (ft/sec)
\(38.3\)
\(54.1\)
\(66.3\)
\(76.5\)
Find the value of \(k\) and write a power function relating the variables.
What is the rate of water flow at a typical water pressure of 60 psi?
Graph your function and verify your answer to part (b) on the graph.
35.
Thanks to improvements in technology, the annual electricity cost of running most major appliances has decreased steadily since 1970. The average annual cost of running a refrigerator is given, in dollars, by the function
How much did it cost to run a refrigerator in 1980? In 1990?
When was the cost of running a refrigerator half of the cost in 1970? If the cost continues to decline according to the given function, when will it cost $50 per year to run a refrigerator?
Graph the function \(C(t)\text{.}\) Do you think that the cost will continue to decline indefinitely according to the given function? Why or why not?
When the Concorde lands at Heathrow airport in London, the width \(w\) of the sonic boom felt on the ground is given in kilometers by the following formula:
where \(T\) stands for the temperature on the ground in kelvins, \(h\) is the altitude of the Concorde when it breaks the sound barrier, and \(m\) is the drop in temperature for each gain in altitude of 1 kilometer. Find the width of the sonic boom if the ground temperature is 293 kelvins, the altitude of the Concorde is 15 kilometers, and the temperature drop is 4 kelvin per kilometer of altitude.
where \(L=3.9 \times 10^{33}\) is the total luminosity of the Sun, \(R=9.96 \times 10^{10}\) centimeters is the radius of the Sun, and \(s=5.7 \times 10^{-5}\) is a constant governing radiation. Calculate the temperature of the Sun.
39.
Graph the functions \(~~f (x) = 4 \sqrt[3]{x - 9}~~\) and \(~~g(x) = 12~~\) in the window