Centripetal Acceleration

Read this text, which presents more explanation on the topic of centripetal acceleration. Pay attention to Figure 6.8 which shows an example of centripetal acceleration. In this example, a disk is rotating at a constant speed. As the disk rotates, the velocity vector at any given point on the disk changes because the direction changes. As shown in the free-body diagram at the top of the figure, the velocity vectors add to make a net velocity vector toward the center of the disk. This leads to centripetal acceleration because there is a net change in acceleration toward the disk.

Centripetal forces assume the equation  F_c=m\dfrac{v^2}{r} . Therefore, whatever equation characterized the classical forces in Unit 4 can also be related to a situation by its centripetal force equation just given.

We know from kinematics that acceleration is a change in velocity, either in its magnitude or in its direction, or both. In uniform circular motion, the direction of the velocity changes constantly, so there is always an associated acceleration, even though the magnitude of the velocity might be constant. You experience this acceleration yourself when you turn a corner in your car. (If you hold the wheel steady during a turn and move at constant speed, you are in uniform circular motion). What you notice is a sideways acceleration because you and the car are changing direction. The sharper the curve and the greater your speed, the more noticeable this acceleration will become. In this section we examine the direction and magnitude of that acceleration.

Figure 6.8 shows an object moving in a circular path at constant speed. The direction of the instantaneous velocity is shown at two points along the path. Acceleration is in the direction of the change in velocity, which points directly toward the center of rotation (the center of the circular path). This pointing is shown with the vector diagram in the figure. We call the acceleration of an object moving in uniform circular motion (resulting from a net external force) the centripetal acceleration(a_{c}); centripetal means "toward the center" or "center seeking".

The given figure shows a circle, with a triangle having vertices A B C made from the center to the boundry. A is at the center and B and C points are at the circle path. Lines A B and A C act as radii and B C is a chord. Delta theta is shown inside the triangle, and the arc length delta s and the chord length delta r are also given. At point B, velocity of object is shown as v one and at point C, velocity of object is shown as v two. Along the circle an equation is shown as delta v equals v sub 2 minus v sub 1.

Figure 6.8 The directions of the velocity of an object at two different points are shown, and the change in velocity \Delta \mathbf{v} is seen to point directly toward the center of curvature. (See small inset.) Because \mathbf{a}_{\mathrm{c}}=\Delta \mathbf{v} / \Delta t, the acceleration is also toward the center; \mathbf{a}_{c} is called centripetal acceleration. (Because \Delta \theta is very small, the arc length \Delta s is equal to the chord length \Delta r for small time differences.)

The direction of centripetal acceleration is toward the center of curvature, but what is its magnitude? Note that the triangle formed by the velocity vectors and the one formed by the radii r and \Delta s are similar. Both the triangles ABC and PQR are isosceles triangles (two equal sides). The two equal sides of the velocity vector triangle are the speeds v_{1}=v_{2}=v . Using the properties of two similar triangles, we obtain

\dfrac{\Delta v}{v}=\dfrac{\Delta s}{r} 

Acceleration is \Delta v / \Delta t, and so we first solve this expression for \Delta v :

\Delta v=\dfrac{v}{r} \Delta s

Then we divide this by \Delta t, yielding

\dfrac{\Delta v}{\Delta t}=\dfrac{v}{r} \times \dfrac{\Delta s}{\Delta t}

Finally, noting that \Delta v / \Delta t=a_{\mathrm{c}} and that \Delta s / \Delta t=v, the linear or tangential speed, we see that the magnitude of the centripetal acceleration is 


which is the acceleration of an object in a circle of radius r at a speed v . So, centripetal acceleration is greater at high speeds and in sharp curves (smaller radius), as you have noticed when driving a car. But it is a bit surprising that a_{\mathrm{c}} is proportional to speed squared, implying, for example, that it is four times as hard to take a curve at 100 km/h than at 50 km/h. A sharp corner has a small radius, so that a_{\mathrm{c}} is greater for tighter turns, as you have probably noticed.

It is also useful to express a_{\mathrm{c}} in terms of angular velocity. Substituting v=r \omega into the above expression, we find a_{\mathrm{c}}=(r \omega)^{2} / r=r \omega^{2} . We can express the magnitude of centripetal acceleration using either of two equations:

a_{\mathrm{c}}=\dfrac{v^{2}}{r} ; a_{\mathrm{c}}=r \omega^{2}.

Recall that the direction of a_{\mathrm{c}} is toward the center. You may use whichever expression is more convenient, as illustrated in examples below.

A centrifuge (see Figure 6.9b) is a rotating device used to separate specimens of different densities. High centripetal acceleration significantly decreases the time it takes for separation to occur, and makes separation possible with small samples. Centrifuges are used in a variety of applications in science and medicine, including the separation of single cell suspensions such as bacteria, viruses, and blood cells from a liquid medium and the separation of macromolecules, such as DNA and protein, from a solution. Centrifuges are often rated in terms of their centripetal acceleration relative to acceleration due to gravity (g); maximum centripetal acceleration of several hundred thousand g  is possible in a vacuum. Human centrifuges, extremely large centrifuges, have been used to test the tolerance of astronauts to the effects of accelerations larger than that of Earth's gravity.

Example 6.2 How Does the Centripetal Acceleration of a Car Around a Curve Compare with That Due to Gravity?

What is the magnitude of the centripetal acceleration of a car following a curve of radius 500 \mathrm{~m} at a speed of 25.0 \mathrm{~m} / \mathrm{s} (about 90 km/h? Compare the acceleration with that due to gravity for this fairly gentle curve taken at highway speed. See Figure 6.9(a).


Because v and r are given, the first expression in a_{\mathrm{c}}=\dfrac{v^{2}}{r} ; a_{\mathrm{c}}=r \omega^{2} is the most convenient to use.


Entering the given values of v=25.0 \mathrm{~m} / \mathrm{s} and r=500 \mathrm{~m} into the first expression for a_{\mathrm{c}} gives

a_{\mathrm{c}}=\dfrac{v^{2}}{r}=\dfrac{(25.0 \mathrm{~m} / \mathrm{s})^{2}}{500 \mathrm{~m}}=1.25 \mathrm{~m} / \mathrm{s}^{2}


To compare this with the acceleration due to gravity \left(g=9.80 \mathrm{~m} / \mathrm{s}^{2}\right), we take the ratio of a_{\mathrm{c}} / g=\left(1.25 \mathrm{~m} / \mathrm{s}^{2}\right) /\left(9.80 \mathrm{~m} / \mathrm{s}^{2}\right)=0.128. Thus, a_{\mathrm{c}}=0.128 \mathrm{~g} and is noticeable especially if you were not wearing a seat belt.

In figure a, a car shown from top is running on a circular road around a circular path. The center of the park is termed as the center of this circle and the distance from this point to the car is taken as radius r. The linear velocity is shown in perpendicular direction toward the front of the car, shown as v the centripetal acceleration is shown with an arrow pointed towards the center of rotation. In figure b, a centrifuge is shown an object of mass m is rotating in it at a constant speed. The object is at the distance equal to the radius, r, of the centrifuge. The centripetal acceleration is shown towards the center of rotation, and the velocity, v is shown perpendicular to the object in the clockwise direction.

Figure 6.9 (a) The car following a circular path at constant speed is accelerated perpendicular to its velocity, as shown. The magnitude of this centripetal acceleration is found in Example 6.2. (b) A particle of mass in a centrifuge is rotating at constant angular velocity. It must be accelerated perpendicular to its velocity or it would continue in a straight line. The magnitude of the necessary acceleration is found in Example 6.3.

Example 6.3 How Big Is the Centripetal Acceleration in an Ultracentrifuge?

Calculate the centripetal acceleration of a point 7.50 cm from the axis of an ultracentrifuge spinning at 7.5 \times 10^{4} \mathrm{rev} / \mathrm{min} . Determine the ratio of this acceleration to that due to gravity. See Figure 6.9(\mathrm{~b})


The term rev/min stands for revolutions per minute. By converting this to radians per second, we obtain the angular velocity \omega. Because r is given, we can use the second expression in the equation a_{\mathbf{c}}=\dfrac{v^{2}}{r} ; a_{\mathbf{c}}=r
    \omega^{2} to calculate the centripetal acceleration.


To convert 7.50 \times 10^{4} rev / min to radians per second, we use the facts that one revolution is 2 \pi rad and one minute is 60.0 \mathrm{~s}. Thus,

\omega=7.50 \times 10^{4} \dfrac{\text { rev }}{\min } \times \dfrac{2 \pi \text { rad }}{1 \, \mathrm{rev}} \times \dfrac{1 \mathrm{~min}}{60.0 \mathrm{~s}}=7854 \, \mathrm{rad} / \mathrm{s}

Now the centripetal acceleration is given by the second expression in a_{\mathrm{c}}=\dfrac{v^{2}}{r} ; a_{\mathrm{c}}=r \omega^{2} as

a_{\mathrm{c}}=r \omega^{2}

Converting 7.50 \mathrm{~cm} to meters and substituting known values gives

a_{\mathrm{c}}=(0.0750 \mathrm{~m})(7854 \, \mathrm{rad} / \mathrm{s})^{2}=4.63 \times 10^{6} \mathrm{~m} / \mathrm{s}^{2}

Note that the unitless radians are discarded in order to get the correct units for centripetal acceleration. Taking the ratio of a_{\mathrm{c}} to g yields

\dfrac{a_{\mathrm{c}}}{g}=\dfrac{4.63 \times 10^{6}}{9.80}=4.72 \times 10^{5}


This last result means that the centripetal acceleration is 472,000 times as strong as g. It is no wonder that such high ω centrifuges are called ultracentrifuges. The extremely large accelerations involved greatly decrease the time needed to cause the sedimentation of blood cells or other materials.

Of course, a net external force is needed to cause any acceleration, just as Newton proposed in his second law of motion. So a net external force is needed to cause a centripetal acceleration. In Centripetal Force, we will consider the forces involved in circular motion.

Source: Rice University, https://openstax.org/books/college-physics/pages/6-2-centripetal-acceleration#import-auto-id3033074
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Last modified: Monday, October 25, 2021, 10:31 AM