# Learning Objectives

### Learning Objectives

By the end of this section, you will be able to do the following:

• Define normal and tension forces
• Apply Newton's laws of motion to solve problems involving a variety of forces
• Use trigonometric identities to resolve weight into components

The information presented in this section supports the following AP® learning objectives and science practices:

• 2.B.1.1 The student is able to apply $F=mgF=mg$ to calculate the gravitational force on an object with mass m in a gravitational field of strength g in the context of the effects of a net force on objects and systems. (S.P. 2.2, 7.2)
• 3.A.2.1 The student is able to represent forces in diagrams or mathematically using appropriately labeled vectors with magnitude, direction, and units during the analysis of a situation. (S.P. 1.1)
• 3.A.3.1 The student is able to analyze a scenario and make claims—develop arguments, justify assertions—about the forces exerted on an object by other objects for different types of forces or components of forces. (S.P. 6.4, 7.2)
• 3.A.3.3 The student is able to describe a force as an interaction between two objects and identify both objects for any force. (S.P. 1.4)
• 3.A.4.1 The student is able to construct explanations of physical situations involving the interaction of bodies using Newton's third law and the representation of action-reaction pairs of forces. (S.P. 1.4, 6.2)
• 3.A.4.2 The student is able to use Newton's third law to make claims and predictions about the action-reaction pairs of forces when two objects interact. (S.P. 6.4, 7.2)
• 3.A.4.3 The student is able to analyze situations involving interactions among several objects by using free-body diagrams that include the application of Newton's third law to identify forces. (S.P. 1.4)
• 3.B.1.3 The student is able to re-express a free-body diagram representation into a mathematical representation and solve the mathematical representation for the acceleration of the object. (S.P. 1.5, 2.2)
• 3.B.2.1 The student is able to create and use free-body diagrams to analyze physical situations to solve problems with motion qualitatively and quantitatively. (S.P. 1.1, 1.4, 2.2)

Forces are given many names, such as push, pull, thrust, lift, weight, friction, and tension. Traditionally, forces have been grouped into several categories and given names relating to their source, how they are transmitted, or their effects. The most important of these categories are discussed in this section, together with some interesting applications. Further examples of forces are discussed later in this text.

# Normal Force

### Normal Force

Weight also called force of gravity is a pervasive force that acts at all times and must be counteracted to keep an object from falling. You definitely notice that you must support the weight of a heavy object by pushing up on it when you hold it stationary, as illustrated in Figure 4.12(a). But how do inanimate objects like a table support the weight of a mass placed on them, such as shown in Figure 4.12(b)? When the bag of dog food is placed on the table, the table actually sags slightly under the load. This would be noticeable if the load were placed on a card table, but even rigid objects deform when a force is applied to them. Unless the object is deformed beyond its limit, it will exert a restoring force much like a deformed spring or trampoline or diving board. The greater the deformation, the greater the restoring force. So when the load is placed on the table, the table sags until the restoring force becomes as large as the weight of the load. At this point the net external force on the load is zero. That is the situation when the load is stationary on the table. The table sags quickly, and the sag is slight so we do not notice it. But it is similar to the sagging of a trampoline when you climb onto it.

Figure 4.12 (a) The person holding the bag of dog food must supply an upward force $FhandFhand size 12{F rSub { size 8{"hand"} } } {}$ equal in magnitude and opposite in direction to the weight of the food $ww size 12{w} {}$. (b) The card table sags when the dog food is placed on it, much like a stiff trampoline. Elastic restoring forces in the table grow as it sags until they supply a force $NN size 12{N} {}$ equal in magnitude and opposite in direction to the weight of the load.

We must conclude that whatever supports a load, be it animate or not, must supply an upward force equal to the weight of the load, as we assumed in a few of the previous examples. If the force supporting a load is perpendicular to the surface of contact between the load and its support, this force is defined to be a normal force, and here is given the symbol $NN size 12{N} {}$. This is not the unit for force N. The word normal means perpendicular to a surface. The normal force can be less than the object’s weight if the object is on an incline, as you will see in the next example.

### Common Misconception: Normal Force (N) vs. Newton (N)

In this section, we have introduced the quantity normal force, which is represented by the variable $NN size 12{N} {}$. This should not be confused with the symbol for the newton, which is also represented by the letter N. These symbols are particularly important to distinguish because the units of a normal force ($NN size 12{N} {}$) happen to be newtons (N). For example, the normal force $NN size 12{N} {}$ that the floor exerts on a chair might be $N=100 NN=100 N size 12{N="100"" N"} {}$. One important difference is that normal force is a vector, while the newton is simply a unit. Be careful not to confuse these letters in your calculations! You will encounter more similarities among variables and units as you proceed in physics. Another example of this is the quantity work ($WW size 12{W} {}$) and the unit watts (W).

### Example 4.5Weight on an Incline, a Two-Dimensional Problem

Consider the skier on a slope shown in Figure 4.13. Her mass including equipment is 60.0 kg. (a) What is her acceleration if friction is negligible? (b) What is her acceleration if friction is known to be 45.0 N?

Figure 4.13 Since motion and friction are parallel to the slope, it is most convenient to project all forces onto a coordinate system where one axis is parallel to the slope and the other is perpendicular (axes shown to left of skier). $NN size 12{N} {}$ is perpendicular to the slope and f is parallel to the slope, but $ww size 12{w} {}$ has components along both axes, namely $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$ and $w∥ w∥$. $NN size 12{N} {}$ is equal in magnitude to $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$, so that there is no motion perpendicular to the slope, but $ff size 12{f} {}$ is less than $w∥ w∥ size 12{w rSub { size 8{ \lline \lline } } } {}$, so that there is a downslope acceleration along the parallel axis.

Strategy

This is a two-dimensional problem, since the forces on the skier—the system of interest—are not parallel. The approach we have used in two-dimensional kinematics also works very well here. Choose a convenient coordinate system and project the vectors onto its axes, creating two connected one-dimensional problems to solve. The most convenient coordinate system for motion on an incline is one that has one coordinate parallel to the slope and one perpendicular to the slope. Remember that motions along mutually perpendicular axes are independent. We use the symbols $⊥⊥ size 12{ ortho } {}$ and $∥ ∥ size 12{ \lline \lline } {}$ to represent perpendicular and parallel, respectively. This choice of axes simplifies this type of problem, because there is no motion perpendicular to the slope and because friction is always parallel to the surface between two objects. The only external forces acting on the system are the skier’s weight, friction, and the support of the slope, respectively labeled $ww size 12{w} {}$, $ff size 12{f} {}$, and $NN size 12{N} {}$ in Figure 4.13. $NN size 12{N} {}$ is always perpendicular to the slope, and $ff size 12{f} {}$ is parallel to it. But $ww size 12{w} {}$ is not in the direction of either axis, and so the first step we take is to project it into components along the chosen axes, defining $w∥ w∥ size 12{w rSub { size 8{ \lline \lline } } } {}$ to be the component of weight parallel to the slope and $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$ to be the component of weight perpendicular to the slope. Once this is done, we can consider the two separate problems of forces parallel to the slope and forces perpendicular to the slope.

Solution

The magnitude of the component of the weight parallel to the slope is $w∥ =wsin(25º)=mgsin(25º)w∥ =wsin(25º)=mgsin(25º) size 12{w rSub { size 8{ \lline \lline } } =w"sin" $$"25"°$$ = ital "mg""sin" $$"25"°$$ } {}$, and the magnitude of the component of the weight perpendicular to the slope is $w⊥=wcos(25º)=mgcos(25º)w⊥=wcos(25º)=mgcos(25º) size 12{w rSub { size 8{ ortho } } =w"cos" $$"25"°$$ = ital "mg""cos" $$"25"°$$ } {}$.

(a) Neglecting friction. Since the acceleration is parallel to the slope, we need only consider forces parallel to the slope. Forces perpendicular to the slope add to zero, since there is no acceleration in that direction. The forces parallel to the slope are the amount of the skier’s weight parallel to the slope $w∥ w∥ size 12{w rSub { size 8{ \lline \lline } } } {}$ and friction $ff size 12{f} {}$. Using Newton’s second law, with subscripts to denote quantities parallel to the slope,

4.30 $a∥ =Fnet ∥ ma∥ =Fnet ∥ m$

where $Fnet ∥ =w∥ =mgsin(25º)Fnet ∥ =w∥ =mgsin(25º) size 12{F rSub { size 8{"net " \lline \lline } } =w rSub { size 8{ \lline \lline } } = ital "mg""sin" $$"25"°$$ } {}$, assuming no friction for this part, so that

4.31 $a∥ =Fnet ∥ m=mgsin(25º)m=gsin(25º)a∥ =Fnet ∥ m=mgsin(25º)m=gsin(25º)$
4.32 $(9.80 m/s2)(0.4226)=4.14m/s2(9.80 m/s2)(0.4226)=4.14m/s2$

is the acceleration.

(b) Including friction. We now have a given value for friction, and we know its direction is parallel to the slope and it opposes motion between surfaces in contact. So the net external force is now

4.33 $Fnet ∥ =w∥ −f,Fnet ∥ =w∥ −f size 12{F rSub { size 8{"net " \lline \lline } } =w rSub { size 8{ \lline \lline } } - f} {},$

and substituting this into Newton’s second law, $a∥ =Fnet ∥ ma∥ =Fnet ∥ m size 12{a rSub { size 8{ \lline \lline } } = { {F rSub { size 8{"net " \lline \lline } } } over {m} } } {}$, gives

4.34 $a∥ =Fnet ∣∣m=w∥ −fm=mgsin(25º)−fm.a∥ =Fnet ∣∣m=w∥ −fm=mgsin(25º)−fm size 12{a rSub { size 8{ \lline \lline } } = { {F rSub { size 8{"net " \lline \lline } } } over {m} } = { {w rSub { size 8{ \lline \lline } } - f} over {m} } = { { ital "mg""sin" $$"25"°$$ - f} over {m} } } {}.$

We substitute known values to obtain

4.35 $a∥ =(60.0 kg)(9.80 m/s2)(0.4226)−45.0 N60.0 kg,a∥ =(60.0 kg)(9.80 m/s2)(0.4226)−45.0 N60.0 kg size 12{a rSub { size 8{ \lline \lline } } = { { $$"60" "." "0 kg"$$ $$9 "." "80 m/s" rSup { size 8{2} }$$ $$0 "." "4226"$$ - "45" "." "0 N"} over {"60" "." "0 kg"} } } {},$

which yields

4.36 $a∥ =3.39 m/s2,a∥ =3.39 m/s2 size 12{a rSub { size 8{ \lline \lline } } =3 "." "39 m/s" rSup { size 8{2} } } {},$

which is the acceleration parallel to the incline when there is 45.0 N of opposing friction.

Discussion

Since friction always opposes motion between surfaces, the acceleration is smaller when there is friction than when there is none. In fact, it is a general result that if friction on an incline is negligible, then the acceleration down the incline is $a=gsinθa=gsinθ size 12{a=g"sin"θ} {}$, regardless of mass. This is related to the previously discussed fact that all objects fall with the same acceleration in the absence of air resistance. Similarly, all objects, regardless of mass, slide down a frictionless incline with the same acceleration if the angle is the same.

### Resolving Weight into Components

Figure 4.14 An object rests on an incline that makes an angle θ with the horizontal.

When an object rests on an incline that makes an angle $θθ size 12{θ} {}$ with the horizontal, the force of gravity acting on the object is divided into two components: a force acting perpendicular to the plane, $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$, and a force acting parallel to the plane, $w∥ w∥ size 12{w rSub { size 8{ \lline \lline } } } {}$. The perpendicular force of weight, $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$, is typically equal in magnitude and opposite in direction to the normal force, $NN size 12{N} {}$. The force acting parallel to the plane, $w∥ w∥ size 12{w rSub { size 8{ \lline \lline } } } {}$, causes the object to accelerate down the incline. The force of friction, $ff size 12{f} {}$, opposes the motion of the object, so it acts upward along the plane.

It is important to be careful when resolving the weight of the object into components. If the angle of the incline is at an angle $θθ size 12{θ} {}$ to the horizontal, then the magnitudes of the weight components are

4.37 $w∥ =wsin(θ)=mgsin(θ)w∥ =wsin(θ)=mgsin(θ) size 12{w rSub { size 8{ \lline \lline } } =w"sin" $$θ$$ = ital "mg""sin" $$θ$$ " "} {}$

and

4.38 $w⊥=wcos(θ)=mgcos(θ).w⊥=wcos(θ)=mgcos(θ) size 12{w rSub { size 8{ ortho } } =w"cos" $$θ$$ = ital "mg""cos" $$θ$$ } {}.$

Instead of memorizing these equations, it is helpful to be able to determine them from reason. To do this, draw the right triangle formed by the three weight vectors. Notice that the angle $θθ size 12{θ} {}$ of the incline is the same as the angle formed between $ww size 12{w} {}$ and $w⊥w⊥ size 12{w rSub { size 8{ ortho } } } {}$. Knowing this property, you can use trigonometry to determine the magnitude of the weight components

4.39 cos(θ)=w⊥ww⊥=wcos(θ)=mgcos(θ)cos(θ)=w⊥ww⊥=wcos(θ)=mgcos(θ)alignl { stack { size 12{"cos" $$θ$$ = { {w rSub { size 8{ ortho } } } over {w} } } {} # w rSub { size 8{ ortho } } =w"cos" $$θ$$ = ital "mg""cos" $$θ$$ {} } } {}
4.40 sin(θ)=w∥ ww∥ =wsin(θ)=mgsin(θ).sin(θ)=w∥ ww∥ =wsin(θ)=mgsin(θ).alignl { stack { size 12{"sin" $$θ$$ = { {w rSub { size 8{ \lline \lline } } } over {w} } } {} # w rSub { size 8{ \lline \lline } } =w"sin" $$θ$$ = ital "mg""sin" $$θ$$ {} } } {}

### Take-Home Experiment: Force Parallel

To investigate how a force parallel to an inclined plane changes, find a rubber band, some objects to hang from the end of the rubber band, and a board you can position at different angles. How much does the rubber band stretch when you hang the object from the end of the board? Now place the board at an angle so that the object slides off when placed on the board. How much does the rubber band extend if it is lined up parallel to the board and used to hold the object stationary on the board? Try two more angles. What does this show?

# Tension

### Tension

A tension is a force along the length of a medium, especially a force carried by a flexible medium, such as a rope or cable. The word tension comes from a Latin word meaning to stretch. Not coincidentally, the flexible cords that carry muscle forces to other parts of the body are called tendons. Any flexible connector, such as a string, rope, chain, wire, or cable, can exert pulls only parallel to its length; thus, a force carried by a flexible connector is a tension with direction parallel to the connector. It is important to understand that tension is a pull in a connector. In contrast, consider the phrase: “You can’t push a rope.” The tension force pulls outward along the two ends of a rope.

Consider a person holding a mass on a rope as shown in Figure 4.15.

Figure 4.15 When a perfectly flexible connector—one requiring no force to bend it—such as this rope transmits a force $TT size 12{T} {}$, that force must be parallel to the length of the rope, as shown. The pull such a flexible connector exerts is a tension. Note that the rope pulls with equal force but in opposite directions on the hand and the supported mass, neglecting the weight of the rope. This is an example of Newton’s third law. The rope is the medium that carries the equal and opposite forces between the two objects. The tension anywhere in the rope between the hand and the mass is equal. Once you have determined the tension in one location, you have determined the tension at all locations along the rope.

Tension in the rope must equal the weight of the supported mass, as we can prove using Newton’s second law. If the 5.00-kg mass in the figure is stationary, then its acceleration is zero, and thus $Fnet=0Fnet=0 size 12{F rSub { size 8{"net"} } =0} {}$. The only external forces acting on the mass are its weight $ww size 12{w} {}$ and the tension $TT size 12{T} {}$ supplied by the rope. Thus,

4.41 $Fnet=T−w=0,Fnet=T−w=0 size 12{F rSub { size 8{"net"} } =T - w=0} {},$

where $TT size 12{T} {}$ and $ww size 12{w} {}$ are the magnitudes of the tension and weight and their signs indicate direction, with up being positive here. Thus, just as you would expect, the tension equals the weight of the supported mass.

4.42 $T=w=mg.T=w=mg. size 12{T=w= ital "mg"} {}$

For a 5.00-kg mass, and neglecting the mass of the rope then we see that

4.43 $T=mg=(5.00 kg)(9.80 m/s2)=49.0 N.T=mg=(5.00 kg)(9.80 m/s2)=49.0 N size 12{T= ital "mg"= $$5 "." "00"" kg"$$ $$9 "." "80 m/s" rSup { size 8{2} }$$ ="49" "." 0" N"} {}.$

If we cut the rope and insert a spring, the spring would extend a length corresponding to a force of 49.0 N, providing a direct observation and measure of the tension force in the rope.

Flexible connectors are often used to transmit forces around corners, such as in a hospital traction system, a finger joint, or a bicycle brake cable. If there is no friction, the tension is transmitted undiminished. Only its direction changes, and it is always parallel to the flexible connector. This is illustrated in Figure 4.16(a) and (b).

Figure 4.16 (a) Tendons in the finger carry force $TT size 12{T} {}$ from the muscles to other parts of the finger, usually changing the force’s direction, but not its magnitude—the tendons are relatively friction free. (b) The brake cable on a bicycle carries the tension $TT size 12{T} {}$ from the handlebars to the brake mechanism. Again, the direction but not the magnitude of $TT size 12{T} {}$ is changed.

### Example 4.6What Is the Tension in a Tightrope?

Calculate the tension in the wire supporting the 70.0-kg tightrope walker shown in Figure 4.17.

Figure 4.17 The weight of a tightrope walker causes a wire to sag by 5.0 degrees. The system of interest here is the point in the wire at which the tightrope walker is standing.

Strategy

As you can see in the figure, the wire is not perfectly horizontal, but is bent under the person’s weight. Thus, the tension on either side of the person has an upward component that can support his weight. As usual, forces are vectors represented pictorially by arrows having the same directions as the forces and lengths proportional to their magnitudes. The system is the tightrope walker, and the only external forces acting on him are his weight $ww size 12{w} {}$ and the two tensions $TLTL size 12{T rSub { size 8{L} } } {}$ (left tension) and $TRTR size 12{T rSub { size 8{R} } } {}$ (right tension), as illustrated. It is reasonable to neglect the weight of the wire itself. The net external force is zero since the system is stationary. A little trigonometry can now be used to find the tensions. One conclusion is possible at the outset—we can see from part (b) of the figure that the magnitudes of the tensions $TLTL size 12{T rSub { size 8{L} } } {}$ and $TRTR size 12{T rSub { size 8{R} } } {}$ must be equal. This is because there is no horizontal acceleration in the rope, and the only forces acting to the left and right are $TLTL size 12{T rSub { size 8{L} } } {}$ and $TRTR size 12{T rSub { size 8{R} } } {}$. Thus, the magnitude of those forces must be equal so that they cancel each other out.

Whenever we have two-dimensional vector problems in which no two vectors are parallel, the easiest method of solution is to pick a convenient coordinate system and project the vectors onto its axes. In this case the best coordinate system has one axis horizontal and the other vertical. We call the horizontal the $xx size 12{x} {}$-axis and the vertical the $yy size 12{y} {}$-axis.

Solution

First, we need to resolve the tension vectors into their horizontal and vertical components. It helps to draw a new free-body diagram showing all of the horizontal and vertical components of each force acting on the system.

Figure 4.18 When the vectors are projected onto vertical and horizontal axes, their components along those axes must add to zero, since the tightrope walker is stationary. The small angle results in $TT size 12{T} {}$ being much greater than $ww size 12{w} {}$.

Consider the horizontal components of the forces (denoted with a subscript $xx size 12{x} {}$).

4.44 $Fnet x=TLx−TRx.Fnet x=TLx−TRx size 12{F rSub { size 8{"net x"} } = T rSub { size 8{"Lx"} } - T rSub { size 8{"Rx"} } } {}.$

The net external horizontal force $Fnet x=0Fnet x=0 size 12{F rSub { size 8{"net x"} } = 0} {}$, since the person is stationary. Thus,

4.45 Fnet x=0=TLx−TRxTLx=TRx.Fnet x=0=TLx−TRxTLx=TRx.alignl { stack { size 12{F rSub { size 8{"net x"} } =0=T rSub { size 8{"LX"} } - T rSub { size 8{"Rx"} } } {} # T rSub { size 8{"Lx"} } = T rSub { size 8{"Rx"} } {} } } {}

Now, observe Figure 4.18. You can use trigonometry to determine the magnitude of $TLTL size 12{T rSub { size 8{L} } } {}$ and $TRTR size 12{T rSub { size 8{R} } } {}$. Notice that

4.46 cos(5.0º)=TLxTLTLx=TLcos(5.0º)cos(5.0º)=TRxTRTRx=TRcos(5.0º).cos(5.0º)=TLxTLTLx=TLcos(5.0º)cos(5.0º)=TRxTRTRx=TRcos(5.0º).alignl { stack { size 12{"cos" $$5 "." 0°$$ = { {T rSub { size 8{"Lx"} } } over {T rSub { size 8{L} } } } } {} # T rSub { size 8{"Lx"} } =T rSub { size 8{L} } "cos" $$5 "." 0°$$ {} # "cos" $$5 "." 0°$$ = { {T rSub { size 8{"RX"} } } over {T rSub { size 8{R} } } } {} # T rSub { size 8{"Rx"} } =T rSub { size 8{R} } "cos" $$5 "." 0°$$ {} } } {}

Equating $TLxTLx size 12{T rSub { size 8{"Lx"} } } {}$ and $TRxTRx size 12{T rSub { size 8{"Rx"} } } {}$

4.47 $TLcos(5.0º)=TRcos(5.0º).TLcos(5.0º)=TRcos(5.0º) size 12{T rSub { size 8{L} } "cos" $$5 "." 0°$$ =T rSub { size 8{R} } "cos" $$5 "." 0°$$ } {}.$

Thus,

4.48 $TL=TR=T,TL=TR=T size 12{T rSub { size 8{L} } =T rSub { size 8{R} } =T} {},$

as predicted. Now, considering the vertical components (denoted by a subscript $yy size 12{y} {}$), we can solve for $TT size 12{T} {}$. Again, since the person is stationary, Newton’s second law implies that net $Fy=0Fy=0 size 12{F rSub { size 8{y} } =0} {}$. Thus, as illustrated in the free-body diagram in Figure 4.18,

4.49 $Fnet y=TLy+TRy−w=0.Fnet y=TLy+TRy−w=0 size 12{F rSub { size 8{"net "} rSub { size 8{y} } } =T rSub { size 8{L} rSub { size 8{y} } } +T rSub { size 8{R} rSub { size 8{y} } } - w=0} {}.$

Observing Figure 4.18, we can use trigonometry to determine the relationship between $TLyTLy size 12{T rSub { size 8{L} rSub { size 8{y} } } } {}$, $TRyTRy size 12{T rSub { size 8{R} rSub { size 8{y} } } } {}$, and $TT size 12{T} {}$. As we determined from the analysis in the horizontal direction, $TL=TR=TTL=TR=T size 12{T rSub { size 8{L} } =T rSub { size 8{R} } =T} {}$

4.50 sin(5.0º)=TLyTLTLy=TLsin(5.0º)=Tsin(5.0º)sin(5.0º)=TRyTRTRy=TRsin(5.0º)=Tsin(5.0º).sin(5.0º)=TLyTLTLy=TLsin(5.0º)=Tsin(5.0º)sin(5.0º)=TRyTRTRy=TRsin(5.0º)=Tsin(5.0º).alignl { stack { size 12{"sin" $$5 "." 0°$$ = { {T rSub { size 8{L} rSub { size 8{y} } } } over {T rSub { size 8{L} } } } } {} # T rSub { size 8{L} rSub { size 8{y} } } =T rSub { size 8{L} } "sin" $$5 "." 0°$$ =T"sin" $$5 "." 0°$$ {} # "sin" $$5 "." 0°$$ = { {T rSub { size 8{R} rSub { size 8{y} } } } over {T rSub { size 8{R} } } } {} # T rSub { size 8{R} rSub { size 8{y} } } =T rSub { size 8{R} } "sin" $$5 "." 0°$$ =T"sin" $$5 "." 0°$$ {} } } {}

Now, we can substitute the values for $TLyTLy size 12{T rSub { size 8{L} rSub { size 8{y} } } } {}$ and $TRyTRy size 12{T rSub { size 8{R} rSub { size 8{y} } } } {}$, into the net force equation in the vertical direction

4.51 Fnet y=TLy+TRy−w=0Fnet y=Tsin(5.0º)+Tsin(5.0º)−w=02Tsin(5.0º)−w=02Tsin(5.0º)=wFnet y=TLy+TRy−w=0Fnet y=Tsin(5.0º)+Tsin(5.0º)−w=02Tsin(5.0º)−w=02Tsin(5.0º)=walignl { stack { size 12{F rSub { size 8{"net "} rSub { size 8{y} } } =T rSub { size 8{L} rSub { size 8{y} } } +T rSub { size 8{R} rSub { size 8{y} } } - w=0} {} # F rSub { size 8{"net "} rSub { size 8{y} } } =T"sin" $$5 "." 0°$$ +T"sin" $$5 "." 0°$$ - w=0 {} # 2T"sin" $$5 "." 0°$$ - w=0 {} # 2T"sin" $$5 "." 0°$$ =w {} } } {}

and

4.52 $T=w2sin(5.0º)=mg2sin(5.0º),T=w2sin(5.0º)=mg2sin(5.0º) size 12{T= { {w} over {2"sin" $$5 "." 0°$$ } } = { { ital "mg"} over {2"sin" $$5 "." 0°$$ } } } {},$

so that

4.53 $T=(70.0 kg)(9.80 m/s2)2(0.0872),T=(70.0 kg)(9.80 m/s2)2(0.0872) size 12{T= { { $$"70" "." "0 kg"$$ $$9 "." "80 m/s" rSup { size 8{2} }$$ } over {2 $$0 "." "0872"$$ } } = { {"686 N"} over {0 "." "174"} } } {},$

and the tension is

4.54 $T=3,900 N.T=3,900 N size 12{T="3900"" N"} {}.$

Discussion

Note that the vertical tension in the wire acts as a normal force that supports the weight of the tightrope walker. The tension is almost six times the 686-N weight of the tightrope walker. Since the wire is nearly horizontal, the vertical component of its tension is only a small fraction of the tension in the wire. The large horizontal components are in opposite directions and cancel, and so most of the tension in the wire is not used to support the weight of the tightrope walker.

If we wish to create a very large tension, all we have to do is exert a force perpendicular to a flexible connector, as illustrated in Figure 4.19. As we saw in the last example, the weight of the tightrope walker acted as a force perpendicular to the rope. We saw that the tension in the roped related to the weight of the tightrope walker in the following way

4.55 $T=w2sin(θ).T=w2sin(θ) size 12{T= { {w} over {2"sin" $$θ$$ } } } {}.$

We can extend this expression to describe the tension $TT size 12{T} {}$ created when a perpendicular force ($F⊥F⊥ size 12{F rSub { size 8{ ortho } } } {}$) is exerted at the middle of a flexible connector.

4.56 $T=F⊥2sin(θ).T=F⊥2sin(θ). size 12{T= { {F rSub { size 8{ ortho } } } over {2"sin" $$θ$$ } } } {}$

Note that $θθ size 12{θ} {}$ is the angle between the horizontal and the bent connector. In this case, $TT size 12{T} {}$ becomes very large as $θθ size 12{θ} {}$ approaches zero. Even the relatively small weight of any flexible connector will cause it to sag, since an infinite tension would result if it were horizontal, that is, $θ=0θ=0$ and $sinθ=0sinθ=0 size 12{"sin"θ=0} {}$ (see Figure 4.19).

Figure 4.19 We can create a very large tension in the chain by pushing on it perpendicular to its length, as shown. Suppose we wish to pull a car out of the mud when no tow truck is available. Each time the car moves forward, the chain is tightened to keep it as nearly straight as possible. The tension in the chain is given by $T=F⊥2sin(θ)T=F⊥2sin(θ) size 12{T= { {F rSub { size 8{ ortho } } } over {2"sin" $$θ$$ } } } {}$ ; since $θθ size 12{θ} {}$ is small, $TT size 12{T} {}$ is very large. This situation is analogous to the tightrope walker shown in Figure 4.17, except that the tensions shown here are those transmitted to the car and the tree rather than those acting at the point where $F⊥F⊥ size 12{F rSub { size 8{ ortho } } } {}$ is applied.
Figure 4.20 Unless an infinite tension is exerted, any flexible connector—such as the chain at the bottom of the picture—will sag under its own weight, giving a characteristic curve when the weight is evenly distributed along the length. Suspension bridges—such as the Golden Gate Bridge shown in this image—are essentially very heavy flexible connectors. The weight of the bridge is evenly distributed along the length of flexible connectors, usually cables, which take on the characteristic shape. (Credit: Leaflet, Wikimedia Commons)

# Extended Topic: Real Forces and Inertial Frames

### Extended Topic: Real Forces and Inertial Frames

There is another distinction among forces in addition to the types already mentioned. Some forces are real, whereas others are not. Real forces are those that have some physical origin, such as the gravitational pull. Contrastingly, fictitious forces are those that arise simply because an observer is in an accelerating frame of reference, such as one that rotates (like a merry-go-round) or undergoes linear acceleration (like a car slowing down). For example, if a satellite is heading due north above Earth’s northern hemisphere, then to an observer on Earth it will appear to experience a force to the west that has no physical origin. Of course, what is happening here is that Earth is rotating toward the east and moves east under the satellite. In Earth’s frame, this looks like a westward force on the satellite, or it can be interpreted as a violation of Newton’s first law (the law of inertia). An inertial frame of reference is one in which all forces are real and, equivalently, one in which Newton’s laws have the simple forms given in this chapter.

Earth’s rotation is slow enough that Earth is nearly an inertial frame. You ordinarily must perform precise experiments to observe fictitious forces and the slight departures from Newton’s laws, such as the effect just described. On the large scale, such as for the rotation of weather systems and ocean currents, the effects can be easily observed.

The crucial factor in determining whether a frame of reference is inertial is whether it accelerates or rotates relative to a known inertial frame. Unless stated otherwise, all phenomena discussed in this text are considered in inertial frames.

All the forces discussed in this section are real forces, but there are a number of other real forces, such as lift and thrust, that are not discussed in this section. They are more specialized, and it is not necessary to discuss every type of force. It is natural, however, to ask where the basic simplicity we seek to find in physics is in the long list of forces. Are some more basic than others? Are some different manifestations of the same underlying force? The answer to both questions is yes, as will be seen in the next (extended) section and in the treatment of modern physics later in the text.

### PhET Explorations: Forces in 1 Dimension

Explore the forces at work when you try to push a filing cabinet. Create an applied force and see the resulting friction force and total force acting on the cabinet. Charts show the forces, position, velocity, and acceleration vs. time. View a free-body diagram of all the forces including gravitational and normal forces.