# Centrifugal force

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Centrifugal force (from Latin centrum "center" and fugere "to flee") refers to an outward force experienced by a body on a curved path and is directed away from the center of curvature. Such a force is experienced in a reference frame attached to the body, which (because the body is not in a uniform straight-line motion) is an accelerating reference frame, not an inertial reference frame. Such a body also may experience another force if it accelerates along the direction of its path, namely the Euler force.

Of course, the body experiencing the centrifugal force is unaware that its path is curved; the observation of a curved path is made from an inertial frame of reference.

## Reference frames

Newton's laws of motion and those of special relativity are expressed for observations made in an inertial frame of reference, that is, in any frame of reference that is in straight-line motion at constant speed relative to the "fixed stars", an historical reference taken today to refer to the entire universe. However, everyday experience does not take place in such a reference frame. For example, we live upon planet Earth, which rotates about its axis (an accelerated motion), orbits the Sun (another accelerated motion), and moves with the Milky Way (still another accelerated motion). These motions are slight, although they do affect matters such as aiming artillery pieces and plotting transoceanic air flights. More visceral examples of everyday experience of non-inertial frames are roller coaster rides and simply turning a sharp corner in a car. In these last examples we are immediately aware of forces upon us due to our motion, and we interpret these motions from our own viewpoint, not that of an imperturbable observer attached to the universe.

The question then arises as to how to connect these experiences in accelerating frames with laws of motion that are not formulated for such situations. The answer lies in the introduction of inertial forces, which are forces observed in the accelerating reference frame, due to its motion, but are not forces recognized in an inertial frame. These inertial forces are included in Newton's laws of motion, and with their inclusion Newton's laws work just as they would in an inertial frame. Centrifugal force is one of these inertial forces, the other two being the Coriolis force and the Euler force.

The way centrifugal forces work is illustrated below by a few examples. The treatment is non-relativistic.

## Rotating spheres

(PD) Image: John R. Brews
Exploded view of rotating spheres in an inertial frame of reference showing the centripetal forces on the spheres provided by the tension in a rope tying them together.
(PD) Image: John R. Brews
Rotating spheres subject to centrifugal (outward) force in a co-rotating frame in addition to the (inward) tension from the rope.

Consider two identical balls isolated in space, but connected by a rope. We ignore any effects of gravity. We observe the tension in the rope, for example, by placing a spring in the center of the rope and measuring its stretch when the rope is under tension. We sit at the center of the rope and inquire whether the two balls are rotating about us.

This thought experiment was devised by Newton, who wanted to explore the question of whether we could discover that the balls were rotating even though we had no point of reference from which to infer that rotation was underway. He concluded that an observed tension in the rope would allow us to infer that the balls are rotating: [1] [2]

 ‘ Yet the thing is not altogether desperate; for we have some arguments to guide us, partly from the apparent motions, which are the differences of the true motions; partly from the forces, which are the causes and effects of the true motions. For instance, if two globes kept at a given distance one from the other, by means of a cord that connects them, were revolved about their common center of gravity; we might, from the tension of the cord, discover the endeavor of the globes to recede from the axis of their motion, and from thence we might compute the quantity of their circular motions. ... And thus we might find both the quantity and the determination of this circular motion, even in an immense vacuum, where there was nothing external or sensible with which the globes could be compared. ’ —Isaac Newton, Principia: Book 1: Definitions – Scholium; 1729 Andrew Motte translation

It is clear that the tension in the rope, as indicated by the stretch of the spring, is an incontrovertible observation that any observer would see, regardless of whether they were stationary or rotating with the balls. (As an aside, relativists like Ernst Mach would point out that this thought experiment takes place in our universe, and so may not be indicative of what would happen in a different universe that contained only these two spheres.[3] The relativists claim that it is rotation with respect to the universe and all its contents that leads to the tension in the rope. Neither this view, nor its contrary, appears to be open to experimental test.)

Let us now look at this tension from the viewpoint of the inertial observers: they see the balls rotating with an angular rate of (say) ω radians/s. That means the balls have a speed of v = ωR where 2R is the separation of the centers of the balls. Their circular motion means that each ball is subject to an inward centripetal force provided by the tension in the rope, of magnitude FT = mv2/R = mRω2, and the measured stretch of the spring reflects exactly this force.

Next, let's look at things from the viewpoint of the rotating observers sitting at the center of the rope. They see the balls as stationary, because they are rotating with them. Because they rotate at the same rate as the spheres, they are said to be in a co-rotating frame. Although the observers cannot see their rotation, they can see the stretched spring. Despite the tension from the stretched string, the balls do not move, indicating they actually are subject to zero net force, which suggests the presence of a balancing force. The rotating observers succeed in using Newton's laws to explain the tension despite no motion, and to explain no motion despite the tension because, in their rotating frame, they experience a centrifugal force, an outward force radiating from their center position that affects all bodies they observe (including themselves if they move off-center). This centrifugal radially outward force on objects at distance R is of magnitude mRω2, but of course, these rotating observers simply see the tension in the spring, and they cannot calculate its magnitude from scratch because they cannot measure the rotational rate ω.

However, if they are quite sophisticated, the rotating observers will notice that the centrifugal force they observe on every object they measure has some peculiar properties not shared by forces such as gravitational, electrical, or nuclear forces. In particular, it has no observable source such as a mass, a charge or an atomic nucleus, like other physical forces, and appears to become larger the further you go from its radiating center, instead of weakening with distance like other forces. So they might conclude that this is an inertial force and try to explain their observations based upon their frame seen as a rotating frame, and calculate their rate of rotation using the measured tension and the formula FT = mRω2. If they did that, then their calculations would be mapped into an inertial frame, and they would analyze the situation the same way as an inertial observer. They then would use centripetal force instead of centrifugal force in their calculations, and their inferred rate of rotation ω.[4]

But as they move about in their rotating frame, their immediate visceral experience of the centrifugal force is a real part of everyday life, whatever the frame they use for theoretical calculations. In particular, the centrifugal force leads to real tension in the rope, despite the fact that nothing is moving. Likewise, when you corner a car, centrifugal force rams you into the door, a real effect from your perspective in your very own wildly accelerating frame of reference, even though the imperturbable inertial observer explains this occurrence as your need for a push from the car to keep you turning with the car instead of continuing on a straight path. If you drop your cell phone while cornering, it will fly away from you, because centrifugal force grabs it.

## Whirling table

(PD) Image: John R. Brews
The "whirling table". The rod is made to rotate about the axis and (from the bead's viewpoint) the centrifugal force acting on the sliding bead is balanced by the weight attached by a cord over two pulleys.

An apparatus called a "whirling table" consists of a rod that can be whirled about an axis, causing a bead to slide on the rod under the influence of centrifugal force.[5] A cord ties a weight to the sliding bead, and pulleys are used to make the consequent force upon the bead horizontal in direction.

In a frame co-rotating with the rod, equilibrium is achieved when the inward force on the bead due to the weight exactly counterbalances the outward centrifugal force upon the bead. By observing changes in the equilibrium balancing distance for a given weight, or the variation of the weight at a fixed distance, the centrifugal force can be measured under changing conditions and used to deduce any change in the rate of rotation, which is not observable directly in a co-rotating frame.

From the viewpoint of an inertial (non-rotating) frame of reference, equilibrium results when the bead is positioned in the particular circular orbit for which the weight provides the correct centripetal force. By observing how the equilibrium balancing distance varies with the weight and the speed of rotation, the centripetal force can be measured as a function of the rate of rotation and the distance of the bead from the center of rotation.

## Skywriter

(PD) Image: NASA
Image from NASA ASRS Callback Number 343, July 2008

What is the viewpoint of an airplane pilot engaged in skywriting? The plane's path is the smoky trail left behind, and progress can be registered as the distance s from the start of the trail to the plane's present position. The speed of the plane is v = ds / dt and the curvature of the path is measured by the osculating circle of radius ρ that is tangent to the path. For the inertial observer watching from the ground, the plane at any instant is executing circular motion about its (instantaneous) center of curvature, and so is subject to a centripetal force v2 / ρ acting radially inward toward this center of curvature.[6] To maintain trajectory, this centripetal force is provided by banking the airplane, generating a lift that provides this centripetal force. According to the pilot, however, the plane is stationary. Banking the airplane subjects him to a centrifugal force, while the plane remains in an equilibrium motionless position.[7] The pilot knows the direction and the magnitude of this centrifugal force by direct observation. If the pilot knew his speed and that he was on a curved path, he also could calculate this force as outward from the instantaneous center of curvature with a magnitude v2 / ρ.[8]

## Figure of the Earth

(PD) Image: John R. Brews
An ellipsoid showing its axes

If we did not know the Earth rotates about its axis, we could infer this rotation from the centrifugal force needed to account for the bulging observed at its equator.[9][10]

In his Principia, Newton proposed the shape of the rotating Earth was that of a homogeneous ellipsoid formed by an equilibrium between the gravitational force holding it together and the centrifugal force pulling it apart. This centrifugal force is greater at the equator than at the pole because the material at the equator is further from the axis of rotation. Hence, the planet bulges at the equator. The Earth's surface is an equipotential, that is, no work is done moving upon the Earth's surface, either against gravity or against centrifugal force. Based upon this equilibrium, Newton determined a flattening expressed by the ratio of diameters: 230 to 229.[11] A modern measurement of the Earth's oblateness leads to an equatorial radius of 6378.14 km and a polar radius of 6356.77 km,[12] about 1/10% less oblate than Newton's estimate.[13] A theoretical determination of the precise extent of oblateness in response to a centrifugal force requires an understanding of the make-up of the planet, not only today but during its formation.[14][15]

This effect is more easily seen with the planet Saturn which has a radius 8.5 to 9.5 times that of Earth but has a rotational period of only 10.57 hours. The ratios of Saturn's diameters is approximately 11 to 10.

(PD) Image: John R. Brews
Rotating shaft unbalanced by two identical attached weights.

## Centrifugal couple

The balancing of automobile tires or rotating shafts involves an example of centrifugal force referred to as a centrifugal couple.[16] The figure shows a rotating shaft unbalanced by two identical attached weights causing a counterclockwise centrifugal couple Cd that must be resisted by a clockwise couple Fℓ = Cd exerted by the bearings. The figure is drawn from the viewpoint of a frame rotating with the shaft, hence the centrifugal forces. To avoid the stress upon the bearings caused by the centrifugal couple, counterbalancing weights must be added.

The unbalancing weights are an idealization, of course. For example, suppose the rod is interpreted as the axle of an automobile tire, and the two weights represent asymmetry in the weight distribution of the of the tire. That is an idealization of the real imbalance that is due to imperfections of manufacture that make the tire composition inhomogeneous.

## Rotating liquid

(PD) Image: John R. Brews
Force diagram for an element of water surface in co-rotating frame. Top: Radial section and selected point on water surface; the water, the co-rotating frame, and the radial section share a constant angular rate of rotation given by the vector Ω. Bottom: Force diagram at selected point on surface. The slope of the surface adjusts to make all three forces sum to zero.

The shape of the surface of a rotating liquid in a bucket can be determined using Newton's laws for the various forces on an element of the surface. This example was used by Newton in the Principia as a means for an observer to detect whether they were rotating.[17]

The figure sets up the analysis in the co-rotating frame where the water appears stationary. The height of the water h = h(r) is a function of the radial distance r from the axis of rotation Ω, and the aim is to determine this function. An element of water volume on the surface is shown to be subject to three forces: the vertical force due to gravity Fg, the horizontal, radially outward centrifugal force FCfgl, and the force normal to the surface of the water Fn due to the rest of the water surrounding the selected element of surface. The force due to surrounding water is known to be normal to the surface of the water because a liquid in equilibrium cannot support shear stresses.[18] To quote Anthony and Brackett:[19]

 ‘ The surface of a fluid of uniform density…, if at rest, is everywhere perpendicular to the lines of force; for if this were not so, the force at a point on the surface could be resolved into two components, one perpendicular and the other tangent to the surface. But from the nature of a fluid, the tangential force would set up a motion of the fluid, which is contrary to the statement that the fluid is at rest. ’ —William Arnold Anthony & Cyrus Fogg Brackett: Elementary Text-book of Physics, p. 127

Moreover, because the element of water does not move, the sum of all three forces must be zero. To sum to zero, the force of the water must point oppositely to the sum of the centrifugal and gravity forces, which means the surface of the water must adjust so its normal points in this direction. (A very similar problem is the design of a banked turn, where the slope of the turn is set so a car will not slide off the road. The analogy in the case of rotating bucket is that the element of water surface will "slide" up or down the surface unless the normal to the surface aligns with the vector resultant formed by the vector addition Fg + FCfgl.)

As r increases, the centrifugal force increases according to the relation (the equations are written per unit mass):

${\displaystyle F_{\mathrm {Cfgl} }=m{\mathit {\Omega }}^{2}r\ ,}$

where Ω is the constant rate of rotation of the water. (In the co-rotating frame, the rate of rotation Ω cannot be measured directly because there is no rotation; but the centrifugal force can be seen to increase with r, and Ω is taken as an empirical proportionality factor.) The gravitational force is unchanged at

${\displaystyle F_{\mathrm {g} }=mg\ ,}$

where g is the acceleration due to gravity. These two forces add to make a resultant at an angle φ from the vertical given by

${\displaystyle \tan \varphi ={\frac {F_{\mathrm {Cfgl} }}{F_{\mathrm {g} }}}={\frac {{\mathit {\Omega }}^{2}r}{g}}\ ,}$

which clearly becomes larger as r increases. To insure that this resultant is normal to the surface of the water, and therefore can be effectively nulled by the force of the water beneath, the normal to the surface must have the same angle, that is,

${\displaystyle \tan \varphi ={\frac {dh}{dr}}\ ,}$

leading to the ordinary differential equation for the shape of the surface:

${\displaystyle {\frac {dh}{dr}}={\frac {{\mathit {\Omega }}^{2}r}{g}}\ ,}$

or, integrating:

${\displaystyle h(r)=h(0)+{\frac {1}{2g}}\left({\mathit {\Omega }}r\right)^{2}\ ,}$

where h(0) is the height of the water at r = 0. In words, the surface of the water is parabolic in its dependence upon the radius.

Of course, it is not possible for the observers in the co-rotating frame to measure directly the angular rate Ω. However, they can observe the parabolic surface, and if they adopt the view that the centrifugal force is due to rotation, they can determine their rate of rotation by measuring the curvature of the water's surface.

## Notes

1. An English translation is found at Sir Isaac Newton (1934). Philosophiae naturalis principia mathematica, Andrew Motte translation of 1729, revised by Florian Cajori. University of California Press, p. 12.
2. Max Born (1962). Einstein's Theory of Relativity. Courier Dover Publications, p. 80. ISBN 0486607690.
3. Ernst Mach (1915). The science of mechanics: a critical and historical account of its development. Supplement, 3rd ed. The Open Court Publishing Company, p. 33. “Try to fix Newton's bucket and rotate the heaven of fixed stars and then prove the absence of centrifugal forces”
4. In trying to determine whether the universe is rotating, this methodology is the procedure followed. Namely, it is assumed that the universe rotates with a hypothetical rate ω, and this parameter is determined by a "best-fit" to astronomical observations. The result is that to within experimental error, the universe is not rotating. The estimate is that the universe has rotated "less than one ten-thousandth of a turn in the last ten billion years". See GF Smoot (1991). “Cosmic background explorer (COBE) observations: new sky maps of the early universe”, Brigitte Rocca-Volmerange, Jean-Michel Deharveng, J. M. Deharveng, eds: The early observable universe from diffuse backgrounds, Proceedings of the XXVIth Rencontre de Moriond, XIth Moriond Astrophysics Meetings, Les Arcs, Savoie, France. Atlantica Séguier Frontières, p. 242. ISBN 2863321072.
5. Dionysius Lardner (1877). Mechanics. Oxford University Press, p. 150.
6. Donald A. Danielson (2003). Vectors and Tensors in Engineering and Physics. Westview Press, p.86. ISBN 0813340802.
7. As seen by the inertial observer, the plane also may exhibit angular acceleration about the center of curvature. For the pilot this acceleration introduces another fictitious force: the Euler force.
8. Denison Olmsted & Ebenezer Strong Snell (1861). An Introduction to Natural Philosophy. Collins & Brother, p. 133.
9. Archibald Tucker Ritchie (1850). The Dynamical Theory of the Formation of the Earth. Longman, Brown, Green and Longmans, p. 529.
10. John Clayton Taylor (2001). Hidden unity in nature's laws. Cambridge University Press, p. 26. ISBN 0521659388.
11. Sir Isaac Newton (1934). “Book III Proposition XIX Problem III: To find the proportion of the axis of a planet to the diameters perpendicular thereto”, Philosophiae naturalis principia mathematica (1687), Andrew Motte translation of 1729, revised by Florian Cajori. University of California Press, p. 424.
12. Charles D Brown (1998). Spacecraft mission design, 2nd ed. American Institute of Aeronautics & Astronomy, p. 58. ISBN 1563472627.
13. This error is the difference in the estimated ratio of diameters. However, a more demanding measure of oblateness is the flattening, defined as f = (a−b)/a where a and b are the semimajor and semiminor axes. Using the cited numbers, the flattening of Newton's prediction differs by 23% from that of modern estimates.
14. Hugh Murray (1837). “Figure and constitution of the Earth deduced from the theory of gravitation”, The Encyclopædia of Geography. Carey, Lea & Blanchard, pp. 124 ff.
15. Alexander Winchell (1888). World-life; Or, Comparative Geology. SC Griggs & Co., p. 425.
16. Gaetano Lanza (2009). Dynamics of Machinery, Reprint of 1911. BiblioBazaar, p. 112. ISBN 1103197215.
17. See page 10 in the Andrew Motte translation for this discussion, found here. For a full analysis see, for example, Jens M. Knudsen, Poul G. Hjorth (2000). Elements of Newtonian Mechanics, 3rd ed. Springer, p. 143. ISBN 354067652X.  This approach to determining whether one is rotating is called "Newton's bucket argument", because he referred to the surface of water in a rotating bucket.
18. Lawrence S. Lerner (1997). Physics for Scientists and Engineers. Jones & Bartlett, p. 404. ISBN 0867204796.
19. William Arnold Anthony & Cyrus Fogg Brackett (1884). Elementary Text-book of Physics. Wiley, p. 127.