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Opus in profectus

# Centripetal Force

## Practice

### practice problem 1

A 250 kg motorcycle is driven around a 12 meter tall vertical circular track at a constant speed of 11 m/s.
1. Determine the normal and friction forces at the four points labeled in the diagram below.
1. at the bottom (and rising)
2. halfway to the top
3. at the top
4. 45° past the top
2. Determine the minimum coefficient of static friction needed to complete the stunt as planned.
(The mass of the motorcycle includes the mass of the rider. Assume that aerodynamic drag and rolling resistance are negligible.) #### solution

1. The only forces present in this problem are weight (which always points down), normal (which always points toward the center of the loop), and friction (which is always tangential to the loop). The weight of the motorcycle never changes. The normal varies from a maximum at the bottom of the loop to a minimum at the top. As the motorcycle drives up the loop, the friction force acts along the direction of motion to keep gravity from slowing it down. As the motorcycle drives down the loop, the friction force acts opposite the direction of motion to keep gravity from speeding it up. The bike isn't speeding up or slowing down, but it is changing direction. This means the net force always points toward the center of motion.

1. Weight points down and normal points up, so the net force is their difference. The normal force points toward the center, so it should be given the positive value. The net force is the centripetal force.

 ∑F = ma Ni − mg = mv2 r
 Ni = m ⎛⎜⎝ v2 + g ⎞⎟⎠ r
 Ni = 250 kg ⎛⎜⎝ (11 m/s)2 + (9.8 m/s2) ⎞⎟⎠ (6 m)
 Ni = 7490 N

Friction isn't necessary since the motorcycle isn't accelerating horizontally.

fi = 0 N

2. The normal force points horizontally, toward the center of the loop. There isn't anything to balance this force at this position. This is our net force — our centripetal force.

 ∑F = ma
 Nii = mv2 r
 Nii = (250 kg)(11 m/s)2 (6 m)
 Nii = 5040 N

Weight points down and normal points inward (toward the center of the loop). They aren't opposite anymore, so they can't cancel. The motorcycle isn't accelerating vertically at this moment, so there must be something to balance the weight. That's where friction steps in. Friction and weight are equal.

 fii = W = mgfii = (250 kg)(9.8 m/s2)fii = 2450 N
3. Both weight and normal point down, so the net force is their sum.

 ∑F = ma Niii + mg = mv2 r
 Niii = m ⎛⎜⎝ v2 − g ⎞⎟⎠ r
 Niii = 250 kg ⎛⎜⎝ (11 m/s)2 − (9.8 m/s2) ⎞⎟⎠ (6 m)
 Niii = 2590 N

Once again, friction isn't necessary since the motorcycle isn't accelerating horizontally.

fiii = 0 N

4. The normal and friction forces are at right angles to each other. This makes them "good" vectors. Normal points toward the center and contributes to the centripetal force. Friction is tangential to the circle and contributes nothing to the centripetal force. Weight is the "bad" vector. It needs to be broken up into components. The component pointing toward the center contributes to the centripetal force.

 ∑F = ma
 Niv + mg cos θ = mv2 r
 Niv = m ⎛⎜⎝ v2 − g cos θ ⎞⎟⎠ r
 Niv = 250 kg ⎛⎜⎝ (11 m/s)2 − (9.8 m/s2)(cos 45°) ⎞⎟⎠ (6 m)
 Niv = 3310 N

The component of the weight tangent to the track is balanced by the friction (so that the speed stays constant).

 fiv = W sin θ = mg sin θfiv = (250 kg)(9.8 m/s2)(sin 45°)fiv = 1730 N

As I was solving this problem, I realized there is a conceptually easier way to solve it. What stays constant in this problem? Weight and centripetal force. What changes? Direction. Compute weight and centripetal force once, then combine them as appropriate to the location.

 W = mgW = (250 kg)(9.8 m/s2)W = 2450 N
 Fc = mv2 r
 Fc = (250 kg)(11 m/s)2 (6 m)
 Fc = 5040 N
1. Weight points down and normal points up. The net force (their difference) is the centripetal force.

 ∑F = maNi − W = FcNi = Fc + WNi = 5040 N + 2450 NNi = 7490 N

Friction isn't necessary since the motorcycle isn't accelerating horizontally.

fi = 0 N

2. Normal points toward the center, which makes it the centripetal force.

 ∑F = maNii = FcNii = 5040 N

Friction counteracts weight to keep the motorcycle moving with constant speed around the loop.

 fii = Wfii = 2450 N
3. Both weight and normal point down toward the center of the loop. The net force (their sum) is the centripetal force.

 ∑F = maNiii + W = FcNiii = Fc − WNiii = 5040 N − 2450 NNiii = 2590 N

Again, friction isn't necessary since the motorcycle isn't accelerating horizontally.

fiii = 0 N

4. The position for this part of the problem was rigged so the two components would have the same magnitude and there'd be fewer things to calculate.

 W∥ = W⊥ = mg sin θ = mg cos θW∥ = W⊥ = (250 kg)(9.8 m/s2)/√2W∥ = W⊥ = 1730 N

The normal force and a component of the weight point toward the center of the loop (the component perpendicular to the loop), so they get to be the centripetal force.

 Niv + W⊥ = FcNiv = Fc − W⊥Niv = 5040 N − 1730 NNiv = 3310 N

The other component of the weight (the component parallel to the loop) is balanced by friction so the net force tangential to the loop is zero and the speed does not change.

 fiv = W∥fiv = 1730 N
2. Static friction needs to be greatest when the motorcycle is vertical. The tires need to grip the loop to balance out the weight and keep the bike from accelerating tangential to the loop. At these two points (one where the bike is going up and the other where the bike is going down) friction equals weight and normal provides the centripetal force. I'll solve this both ways — once using the fancy, formal method…

 μmin = f = mg = gr N mv2/r v2 μmin = (9.8 m/s2)(6 m) (11 m/s)2 μmin = 0.486

and again using the conceptually easier method…

 μmin = f = W N Fc μmin = 2450 N 5040 N μmin = 0.486

### practice problem 2

Ringworld (paid link) is the title of a classic science fiction novel written by Larry Niven in 1970. Set in the year 2850, it is the story of four adventurers (two human and two alien) who are chosen to explore an engineered world encircling a sun-like star. The Ringworld is an enormous cylindrical band with a radius roughly equal to that of the Earth's orbit and a width about the same as the diameter of the Sun. It was constructed by some unspecified form of matter transmutation using the planets and minor bodies that once orbited the Ringworld's sun as raw material. The flat, inner surface is covered with a natural-looking, Earth-like terrain and it spins at a speed fast enough to provide its inhabitants with the sensation of Earth-like gravity. Thousand mile high walls along the edges keep the Ringworld's atmosphere from spilling out into space. The Ringworld is the home of hundreds of hominid species, but they are mostly non-technological. The advanced civilization that engineered the Ringworld collapsed centuries ago and the adventurers find only its remains.

Magnify

How fast does Ringworld spin to provide its inhabitants with the sensation of normal Earth gravity? State your answer in…
1. meters per second
2. Earth days per rotation
3. rotations per Earth year

#### solution

1. Use the centripetal acceleration equation and solve for speed. Substitute values for the acceleration due to gravity on Earth and the radius of the Earth's orbit (also known as an astronomical unit).

 ac = v2 ⇒ v = √acr r
 v = √ [(9.81 m/s2)(1.50 × 1011 m)] v = 1.21 × 106 m/s

Sounds fast, but the speed of things in space tends to be fast anyway. How does this compare to the yearly motion of the Earth around the Sun? That's the goal of the next parts of the question.

2. We'll solve this practice problem two ways. First we'll use the definition of speed and substitute the value calculated above and the distance traveled in one rotation (the circumference).

 v = ∆s = 2πr ∆t T
 T = 2πr v
 T = 2π(1.50 × 1011 m) 1.21 × 106 m/s
 T = 780,000 s ≈ 9 days

The fancier way is to start from the centripetal acceleration equation, replace speed with circumference over period, and simplify. This gives us an equation that some people like so much they memorize it.

 ac = v2 = (2πr/T)2 = 4π2r r r T2

Solve for period and substitute.

 T = 2π√ r ac
 T = 2π√ 1.50 × 1011 m 9.81 m/s2
 T = 780,000 s ≈ 9 days

That's a quick "year" — if we use the astronomical definition of the year as the period of one trip around the Sun. How does it compare to a regular calendar year?

3. This problem is best solved by dimensional analysis.

 n = 365 days/year 9 days/rotation
 n = 40.5 rotations/year

### practice problem 3

The following passage outlines the design specifications of a proposed maglev train system (the Transrapid).

The curve radii of modern high-speed systems result in dependence on the speed and the maximum possible superelevation of the guideway to compensate for the centrifugal forces occurring. The Transrapid's guideway can have a maximum superelevation of 12 degree (up to 16 degree in special cases) which allows smaller radii at higher speeds than in the case of conventional wheel-on-rail systems.

• 200 km/h:0705 m
• 400 km/h: 2825 m
• 500 km/h: 4415 m

ThyssenKrupp Transrapid GmbH, 2002

Determine…

1. the maximum centripetal acceleration (in m/s2 and g) implied by these specifications
2. the speed limit (in m/s and km/h) on a curved section of track with the minimal radius

#### solution

Once you get past reading the awkward translation from German to English, this is a conceptually easy question. Set up a table like the one below and complete the missing parts. Use a graphing calculator as it eliminates the drudgery of repeated calculation.

(km/h) (m/s) (m) (m/s2) (g)
0350
200 0705
400 2825
500 4415
mean centripetal acceleration →

Start by converting the maximum speeds from km/h to m/s.

 ⎡⎢⎣ m = km 1000 m 1 h ⎤⎥⎦ s h 1 km 3600 s

Then apply the equation for centripetal acceleration.

 ac = v2 r

The resulting values will be in m/s2. To convert to g, divide by the standard value for the acceleration due to gravity.

ac[g] = ac[m/s2] ÷ 9.80665 m/s2

This procedure gives a set of numbers that are reasonably close to one another: three values in m/s2 and three in g. Find the mean of both of these triplets. A partially completed table is provided below.

(km/h) (m/s) (m) (m/s2) (g)
0350
200 056 0705 4.38 0.446
400 111 2825 4.37 0.446
500 139 4415 4.37 0.446
mean centripetal acceleration → 4.37 0.446

For the second part of this question, follow the logic of the first part in reverse order. Assume that the maximum permissible centripetal acceleration is the same for all curves, regardless of size. Use the mean value we just calculated to determine the speed limit on a curve with a 350 m radius.

 v = √acr ⇐ ac = v2 r
v = √(4.372 m/s2)(350 m)

v = 39.1 m/s

Then convert from m/s to km/h.

 39.1 m 1 km 3600 s = 140 km/h 1 s 1000 m 1 h

Add these results to the table.

(km/h) (m/s) (m) (m/s2) (g)
140 039 0350 4.37 0.446
200 056 0705 4.38 0.446
400 111 0825 4.37 0.446
500 139 4415 4.36 0.446
mean centripetal acceleration → 4.37 0.446

A more advanced technique is to solve the problem graphically. Starting from the equation for centripetal acceleration.

 ac = v2 r

Makev2 the subject and compare to the equation for a straight line.

 v2 = acr ⇔ y = mx + b

The equation is telling us we should put speed squared on they axis and radius on thex axis.

 y = v2 x = r

This makes the centripetal acceleration equal the slope of the line of best fit.

 m = slope = ac ac = 4.37 m/s2 ac = 0.445 g
 b = intercept b = 7.28 m2/s2 b ≈ 0

The intercept value of 7.28 m2/s2 is effectively equal to zero. Since the speed squared values are all on the order of several thousand, an intercept that's less than ten is "small" in comparison.

Use the coefficients from the line of best fit to find the speed limit on the minimum radius curve. Finish by converting the speed back to km/h from m/s.

 y = mx + b v2 = acr + 0 v2 = (4.37 m/s2)(350 m) v = 39 m/s = 140 km/h

### practice problem 4

Complete the following table.
1. Complete the first two columns using astronomical data from a reliable source. Be sure to specify the units used for each entry.
2. Complete the last two columns using a calculator. Be sure to state your answers in SI units.
Orbital parameters
Moon
Mercury
Earth
Pluto
Sun

#### solution

The data for the moon and planets came from a page in this book. The data for the Sun came from a page in The Physics Factbook. The distance from the Earth to the Sun is called an astronomical unit (au). I plan on discussing the au in the section of this book on miscellaneous units (1 au = 149.6 × 106 km). I know you know the period of Earth's orbit. You may just have to pause and think for a second. The first two columns of the table are done.

Orbital parameters
Moon 384,400 km 27.32 days
Mercury 57.91 × 106 km 87.97 days
Earth 1 au 1 year
Pluto 5,906 × 106 km 90,465 days
Sun 30,000 light years 225 million years

Speed is the rate of change of distance with time, which in circular motion means circumference divided by period.

 v = 2πr T

We are going to use this equation over and over again. Please watch those units. Convert to meters and seconds as appropriate.

Moon
 v = 2π(3.844 × 108 m) (27.32 × 24 × 60 × 60 s) v = 1,023 m/s
Mercury
 v = 2π(5.791 × 1010 m) (87.97 × 24 × 60 × 60 s) v = 47,900 m/s
Earth
 v = 2π(1.496 × 1011 m) (365.25 × 24 × 60 × 60 s) v = 29,800 m/s
Pluto
 v = 2π(5.906 × 1012 m) (90,465 × 24 × 60 × 60 s) v = 4,750 m/s
Sun
 v = 2π(30,000 years)(3.00 × 108 m/s) (2.25 × 108 year) v = 251,000 m/s

Now that we have all the speeds, we can compute the centripetal accelerations.

 ac = v2 r

Again we'll do it over and over again…

Moon
 ac = (1,023 m/s)2 (3.844 × 108 m) ac = 0.00272 m/s2
Mercury
 ac = (47,900 m/s)2 (5.791 × 1010 m) ac = 0.03958 m/s2
Earth
 ac = (29,800 m/s)2 (1.496 × 1011 m) ac = 0.00593 m/s2
Pluto
 ac = (4,750 m/s)2 (5.906 × 1012 m) ac = 3.82 × 10−6 m/s2
Sun
 ac = (251,000 m/s)2 (30,000 years)(3.00 × 108 m/s)(365.25 × 24 × 60 × 60 s) ac = 2.22 × 10−10 m/s2

The table is now ready for completion.

Orbital parameters