Calculating Projectile Motion: Hot Rock Projectile

Kilauea in Hawaii is the world’s most continuously active volcano. Very active volcanoes characteristically eject red-hot rocks and lava rather than smoke and ash. Suppose a large rock is ejected from the volcano with a speed of 25.0 m/s and at an angle 35.0º above the horizontal, as shown in the figure below.

This example further illustrates projectile motion.

Example: Calculating Projectile Motion: Hot Rock Projectile

Kilauea in Hawaii is the world’s most continuously active volcano. Very active volcanoes characteristically eject red-hot rocks and lava rather than smoke and ash. Suppose a large rock is ejected from the volcano with a speed of 25.0 m/s and at an angle \(\text{35.0º}\) above the horizontal, as shown in the figure below. The rock strikes the side of the volcano at an altitude 20.0 m lower than its starting point. (a) Calculate the time it takes the rock to follow this path. (b) What are the magnitude and direction of the rock’s velocity at impact?

The trajectory of a rock ejected from a volcano is shown. The initial velocity of rock v zero is equal to twenty five meters per second and it makes an angle of thirty five degrees with the horizontal x axis. The figure shows rock falling down a height of twenty meters below the volcano level. The velocity at this point is v which makes an angle of theta with horizontal x axis. The direction of v is south east.

The trajectory of a rock ejected from the Kilauea volcano.

Strategy

Again, resolving this two-dimensional motion into two independent one-dimensional motions will allow us to solve for the desired quantities. The time a projectile is in the air is governed by its vertical motion alone. We will solve for \(t\) first. While the rock is rising and falling vertically, the horizontal motion continues at a constant velocity. This example asks for the final velocity. Thus, the vertical and horizontal results will be recombined to obtain \(v\) and \({\theta }_{v}\) at the final time \(t\) determined in the first part of the example.

Solution for (a)

While the rock is in the air, it rises and then falls to a final position 20.0 m lower than its starting altitude. We can find the time for this by using

\(y={y}_{0}+{v}_{0y}t-\frac{1}{2}{\text{gt}}^{2}\text{.}\)

If we take the initial position \({y}_{0}\) to be zero, then the final position is \(y=-\text{20}\text{.0 m}\text{.}\) Now the initial vertical velocity is the vertical component of the initial velocity, found from \({v}_{0y}={v}_{0}\phantom{\rule{0.25em}{0ex}}\text{sin}\phantom{\rule{0.25em}{0ex}}{\theta }_{0}\) = (\(\text{25}\text{.}\text{0 m/s}\))(\(\text{sin 35.0º}\)) = \(\text{14}\text{.}\text{3 m/s}\). Substituting known values yields

\(-\text{20}\text{.}0\text{ m}=\left(\text{14}\text{.}3\text{ m/s}\right)t-\left(4\text{.}\text{90 m/s}{\text{}}^{2}\right){t}^{2}\text{.}\)

Rearranging terms gives a quadratic equation in \(t\):

\(\left(4\text{.}\text{90 m/s}{\text{}}^{2}\right){t}^{2}-\left(\text{14}\text{.}\text{3 m/s}\right)t-\left(\text{20.0 m}\right)=0.\)

This expression is a quadratic equation of the form \({\mathrm{at}}^{2}+\mathrm{bt}+c=0\), where the constants are \(a=4.90\), \(b=–14.3\), and \(c=–20.0.\) Its solutions are given by the quadratic formula:

\(t=\cfrac{-b±\sqrt{{b}^{2}-4\text{ac}}}{\text{2}\text{a}}\text{.}\)

This equation yields two solutions: \(t=3.96\) and \(t=–1.03\). (It is left as an exercise for the reader to verify these solutions.) The time is \(t=3.96\phantom{\rule{0.25em}{0ex}}\text{s}\) or \(–1.03\phantom{\rule{0.25em}{0ex}}\text{s}\). The negative value of time implies an event before the start of motion, and so we discard it. Thus,

\(t=3\text{.}\text{96 s}\text{.}\)

Discussion for (a)

The time for projectile motion is completely determined by the vertical motion. So any projectile that has an initial vertical velocity of 14.3 m/s and lands 20.0 m below its starting altitude will spend 3.96 s in the air.

Solution for (b)

From the information now in hand, we can find the final horizontal and vertical velocities \({v}_{x}\) and \({v}_{y}\) and combine them to find the total velocity \(v\) and the angle \({\theta }_{0}\) it makes with the horizontal. Of course, \({v}_{x}\) is constant so we can solve for it at any horizontal location. In this case, we chose the starting point since we know both the initial velocity and initial angle. Therefore:

\({v}_{x}={v}_{0}\phantom{\rule{0.25em}{0ex}}\text{cos}\phantom{\rule{0.25em}{0ex}}{\theta }_{0}=\left(\text{25}\text{.}0\text{ m/s}\right)\left(\text{cos 35º}\right)=\text{20}\text{.}5\text{ m/s.}\)

The final vertical velocity is given by the following equation:

\({v}_{y}={v}_{0y}-\text{gt,}\)

where \({v}_{0y}\) was found in part (a) to be \(\text{14}\text{.}\text{3 m/s}\). Thus,

\({v}_{y}=\text{14}\text{.}3\text{ m/s}-\left(9\text{.}\text{80 m/s}{\text{}}^{2}\right)\left(3\text{.}\text{96 s}\text{}\right)\)

so that

\({v}_{y}=-\text{24}\text{.}5\text{ m/s.}\)

To find the magnitude of the final velocity \(v\) we combine its perpendicular components, using the following equation:

\(v=\sqrt{v_x^2+v_y^2}=\sqrt{(\text{20.5 m/s})^2+(-\text{24.5 m/s})^2},\)

which gives

\(v=\text{31}\text{.}9\text{ m/s.}\)

The direction \({\theta }_{v}\) is found from the equation:

\({\theta }_{v}={\text{tan}}^{-1}\left({v}_{y}/{v}_{x}\right)\)

so that

\({\theta }_{v}={\text{tan}}^{-1}\left(-\text{24}\text{.}5/\text{20}\text{.}5\right)={\text{tan}}^{-1}\left(-1\text{.}\text{19}\right)\text{.}\)

Thus,

\({\theta }_{v}=-\text{50}\text{.}1º\text{.}\)

Discussion for (b)

The negative angle means that the velocity is \(\text{50}\text{.}1º\) below the horizontal. This result is consistent with the fact that the final vertical velocity is negative and hence downward—as you would expect because the final altitude is 20.0 m lower than the initial altitude. (See the figure above.)

One of the most important things illustrated by projectile motion is that vertical and horizontal motions are independent of each other. Galileo was the first person to fully comprehend this characteristic. He used it to predict the range of a projectile.

On level ground, we define range to be the horizontal distance \(R\) traveled by a projectile. Galileo and many others were interested in the range of projectiles primarily for military purposes—such as aiming cannons. However, investigating the range of projectiles can shed light on other interesting phenomena, such as the orbits of satellites around the Earth. Let us consider projectile range further.

Part a of the figure shows three different trajectories of projectiles on level ground. In each case the projectiles makes an angle of forty five degrees with the horizontal axis. The first projectile of initial velocity thirty meters per second travels a horizontal distance of R equal to ninety one point eight meters. The second projectile of initial velocity forty meters per second travels a horizontal distance of R equal to one hundred sixty three meters. The third projectile of initial velocity fifty meters per second travels a horizontal distance of R equal to two hundred fifty five meters.

Trajectories of projectiles on level ground. (a) The greater the initial speed \({v}_{0}\), the greater the range for a given initial angle. (b) The effect of initial angle \({\theta }_{0}\) on the range of a projectile with a given initial speed. Note that the range is the same for \(\text{15º}\) and \(\text{75º}\), although the maximum heights of those paths are different.

How does the initial velocity of a projectile affect its range? Obviously, the greater the initial speed \({v}_{0}\), the greater the range, as shown in the (a) part of the figure above. The initial angle \({\theta }_{0}\) also has a dramatic effect on the range, as illustrated in the (b) part of the figure above.

For a fixed initial speed, such as might be produced by a cannon, the maximum range is obtained with \({\theta }_{0}=\text{45º}\). This is true only for conditions neglecting air resistance. If air resistance is considered, the maximum angle is approximately \(\text{38º}\).

Interestingly, for every initial angle except \(\text{45º}\), there are two angles that give the same range—the sum of those angles is \(\text{90º}\). The range also depends on the value of the acceleration of gravity \(g\). The lunar astronaut Alan Shepherd was able to drive a golf ball a great distance on the Moon because gravity is weaker there. The range \(R\) of a projectile on level ground for which air resistance is negligible is given by

\(R=\cfrac{{v}_{0}^{2}\phantom{\rule{0.25em}{0ex}}\text{sin}\phantom{\rule{0.25em}{0ex}}{2\theta }_{0}}{g}\text{,}\)

where \({v}_{0}\) is the initial speed and \({\theta }_{0}\) is the initial angle relative to the horizontal. The proof of this equation is left as an end-of-tutorial problem (hints are given), but it does fit the major features of projectile range as described.

When we speak of the range of a projectile on level ground, we assume that \(R\) is very small compared with the circumference of the Earth. If, however, the range is large, the Earth curves away below the projectile and acceleration of gravity changes direction along the path. The range is larger than predicted by the range equation given above because the projectile has farther to fall than it would on level ground. (See the figure below.)

If the initial speed is great enough, the projectile goes into orbit. This possibility was recognized centuries before it could be accomplished. When an object is in orbit, the Earth curves away from underneath the object at the same rate as it falls. The object thus falls continuously but never hits the surface. These and other aspects of orbital motion, such as the rotation of the Earth, will be covered analytically and in greater depth later in this text.

Once again we see that thinking about one topic, such as the range of a projectile, can lead us to others, such as the Earth orbits. In the next topic, we will examine the addition of velocities, which is another important aspect of two-dimensional kinematics and will also yield insights beyond the immediate topic.

A figure of the Earth is shown and on top of it a very high tower is placed. A projectile satellite is launched from this very high tower with initial velocity of v zero in the horizontal direction. Several trajectories are shown with increasing range. A circular trajectory is shown indicating the satellite achieved its orbit and it is revolving around the Earth.

Projectile to satellite. In each case shown here, a projectile is launched from a very high tower to avoid air resistance. With increasing initial speed, the range increases and becomes longer than it would be on level ground because the Earth curves away underneath its path. With a large enough initial speed, orbit is achieved.

This lesson is part of:

Two-Dimensional Kinematics

View Full Tutorial

Track Your Learning Progress

Sign in to unlock unlimited practice exams, tutorial practice quizzes, personalized weak area practice, AI study assistance with Lexi, and detailed performance analytics.