2.1 Limits, Rates of Change, and Tangent Lines

Rates of change play a role whenever we study the relationship between two changing quantities. Velocity is a familiar example (the rate of change of position with respect to time), but there are many others, such as

Figure 2.2: Gottfried Wilhem Leibniz (1646-1716). Painting by Francke, Herzog Anton-Ulrich Museum, Braunschweig, Germany.

Roughly speaking, if y and x are related quantities, the rate of change should tell us how much y changes in response to a unit change in x. For example, if an automobile travels at a velocity of 80 km/hr, then its position changes by 80 km for each unit change in time (the unit being 1 hour). If the trip lasts only half an hour, its position changes by 40 km, and in general, the change in position is 80t km, where t is the change in time (that is, the time elapsed in hours). In other words,

However, this simple formula is not valid or even meaningful if the velocity is not constant. After all, if the automobile is accelerating or decelerating, which velocity would we use in the formula?

The problem of extending this formula to account for changing velocity lies at the heart of calculus. As we will learn, differential calculus uses the limit concept to define instantaneous velocity, and integral calculus enables us to compute the change in position in terms of instantaneous velocity. But these ideas are very general. They apply to all rates of change, making calculus an indispensable tool for modeling an amazing range of real-world phenomena.

In this section, we discuss velocity and other rates of change, emphasizing their graphical interpretation in terms of tangent lines. Although at this stage, we cannot define precisely what a tangent line is—this will have to wait until Chapter 3—you can think of a tangent line as a line that skims a curve at a point, as in Figures (A) and (B) but not (C).

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Figure 2.3: The line is tangent in (A) and (B), but not in (C).

2.1.1 Velocity

When we speak of velocity, we usually mean instantaneous velocity, which indicates the speed and direction of an object at a particular moment. The idea of instantaneous velocity makes intuitive sense, but care is required to define it precisely.

In linear motion, velocity may be positive or negative (indicating the direction of motion). Speed, by definition, is the absolute value of velocity and is always non-negative.

Consider an object traveling in a straight line (linear motion). The average velocity over a given time interval has a straightforward definition as the ratio

For example, if an automobile travels 200 km in 4 hours, then its average velocity during this 4-hour period is . At any given moment the automobile may be going faster or slower than the average.

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Question 2.1 Average Rate of Change Progress Check

ZfHNpgQ7IvyPM3iof0wUmdhtw7n5rEkHRJ1IGPVvtgftm0T+oEKNAFBFrM1+cmV4iTKJtv/5c7YnVGERmyXCZ1chpCb4IKLY1DaLdsmwpbyMakgxZHBfyCEmNnyKswYFZ3qsYJ+y69pJ8lfPksLyqxZQmS4PQYS0A6zbP+HxQ81G+qpd+Yi+17g7mHDr+HGM8cUzG+j+V2yhggXvqFriBYPxB8uiX9Xx
2
Correct.
Try again. Remember that 20 minutes is 1/3 hour.
Incorrect.

We cannot define instantaneous velocity as a ratio in the same way because we would have to divide by the length of the time interval (which is zero). However, we should be able to estimate instantaneous velocity by computing average velocity over successively smaller time intervals. The guiding principle is: Average velocity over a very small time interval is very close to instantaneous velocity. To explore this idea further, we introduce some notation.

The Greek letter Δ (Delta) is commonly used to denote the change in a function or variable. If s(t) is the position of an object (distance from the origin) at time t and [t0, t1] is a time interval, we set

The change in position Δs is also called the displacement, or net change in position. For ,

One motion we will study is the motion of an object falling to earth under the influence of gravity (assuming no air resistance). Galileo discovered that if the object is released at time t = 0 from a state of rest (Figure 2), then the distance traveled after t seconds is given by the formula

s(t) = 4.9t2 m

Figure 2.4: Distance traveled by a falling object after t seconds is s(t) = 4.9t2 meters.

Example 1 A stone, released from a state of rest, falls to earth. Estimate the instantaneous velocity at t = 0.8 s.

Solution We use Galileo’s formula s(t) = 4.9t2 to compute the average velocity over the five short time intervals listed in Table 1. Consider the first interval [t0, t1] = [0.8, 0.81]:

Time intervals Average velocity (m/s)
[0.8, 0.81] 7.889
[0.8, 0.805] 7.8645
[0.8, 0.8001] 7.8405
[0.8, 0.80005] 7.84024
[0.8, 0.800001] 7.840005

The average velocity over [0.8, 0.81] is the ratio

The table above shows the results of similar calculations for intervals of successively shorter lengths. It looks like these average velocities are getting closer to 7.84 m/s as the length of the time interval shrinks:

7.889, 7.8645, 7.8405, 7.84024, 7.840005

There is nothing special about the particular time intervals in the table above. We are looking for a trend, and we could have chosen any intervals [0.8, t] for values of t approaching 0.8. We could also have chosen intervals [t, 0.8] for t < 0.8.

This suggests that 7.84 m/s is a good candidate for the instantaneous velocity at t = 0.8 s.

We express our conclusion in the previous example by saying that average velocity converges to instantaneous velocity or that instantaneous velocity is the limiting value of average velocity as the length of the time interval shrinks to zero.

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2.1.2 Graphical Interpretation of Velocity

The idea that average velocity converges to instantaneous velocity as we shorten the time interval has a vivid interpretation in terms of secant lines. The term secant line refers to a line through two points on a curve.

Consider the graph of position s(t) for an object traveling in a straight line (Figure 3). The ratio defining average velocity over [t0, t1] is nothing more than the slope of the secant line through the points (t0, s(t0)) and (t1, s(t1)). For t1t0,

Figure 2.5: The average velocity over [t0, t1] is equal to the slope of the secant line.

By interpreting average velocity as a slope, we can visualize what happens as the time interval gets smaller. Figure 4 shows the graph of position for the falling stone of Example 1, where s(t) = 4.9t2. As the time interval shrinks, the secant lines get closer to—and seem to rotate toward—the tangent line at t = 0.8.

Figure 2.6: Move the slider to see how the secant lines seem to "rotate" toward the tangent line.

And since the secant lines approach the tangent line, the slopes of the secant lines get closer and closer to the slope of the tangent line. In other words, the statement

As the time interval shrinks to zero, the average velocity approaches the instantaneous velocity.

has the graphical interpretation

As the time interval shrinks to zero, the slope of the secant line approaches the slope of the tangent line.

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We conclude that instantaneous velocity is equal to the slope of the tangent line to the graph of position as a function of time. This conclusion and its generalization to other rates of change are of fundamental importance in differential calculus.

2.1.3 Other Rates of Change

Velocity is only one of many examples of a rate of change. Our reasoning applies to any quantity y that depends on a variable x—say, y = f(x). For any interval [x0, x1], we set

For x1x0, the average rate of change of y with respect to x over [x0, x1] is the ratio

Sometimes, we write Δy and Δyx instead of Δf and Δfx.

The instantaneous rate of change at x = x0 is the limiting value of the average rates of change. We estimate it by computing the average rate over smaller and smaller intervals.

The word “instantaneous” is often dropped. When we use the term “rate of change,” it is understood that the instantaneous rate is intended.

In Example 1 above, we considered only right-hand intervals [x0, x1]. In the next example, we compute the average rate of change for intervals lying to both the left and the right of x0.

Example 2: Speed of Sound in Air

The formula provides a good approximation to the speed of sound υ in dry air (in m/s) as a function of air temperature T (in kelvins). Estimate the instantaneous rate of change of υ with respect to T when T = 273 K. What are the units of this rate?

Solution To estimate the instantaneous rate of change at T = 273, we compute the average rate for several intervals lying to the left and right of T = 273. For example, the average rate of change over [272.5, 273] is

The tables below suggest that the instantaneous rate is approximately 0.605. This is the rate of increase in speed per degree increase in temperature, so it has units of m/s-K, or meters per second per kelvin. The secant lines corresponding to the values in the tables are shown in Figures 5 and 6.

Temperature intervals Average rate of change
[272.5, 273] 0.60550
[272.8, 273] 0.60534
[272.9, 273] 0.60528
[272.99, 273] 0.60523
Table 2.2: Intervals lying to the left of T = 273.
Temperature intervals Average rate of change
[273, 273.5] 0.60495
[273, 273.2] 0.60512
[273, 273.1] 0.60517
[273, 273.01] 0.60522
Table 2.3: Intervals lying to the right of T = 273.
Figure 2.7: Secant lines for intervals lying to the left of T = 273.
Figure 2.8: Secant lines for intervals lying to the right of T = 273.

The applet below is designed to give you the opportunity to investigate the average rate of change for a variety of functions.

Figure 2.9: An interactive applet allowing you to investigate average rate of change.

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To conclude this section, we discuss the case of a simple but important class of functions: For any linear function f(x) = mx + b, the average rate of change over every interval is equal to the slope m (Figure 7). We verify as follows:

Figure 2.10: For a linear function f(x) = mx + b, the ratio Δfx is equal to the slope m for every interval.

The instantaneous rate of change at x = x0, which is the limiting value of these average rates, is also equal to m. This makes sense graphically because all secant lines and all tangent lines to the graph of f(x) coincide with the graph itself.

2.1.4 Summary