PHYS 101 Introductory Physics, Mechanics • McGill University, Montreal

Corrected exercises: friction, circular motion and gravitation (PHYS 101)

This is the corrected exercise set for the friction, circular motion and gravitation chapter of PHYS 101, Introductory Physics, Mechanics, the algebra-based first mechanics course at McGill University. It is written for the course as it is actually taught: no derivative, no integral, nothing but algebra, proportions and right-angle trigonometry. Almost every free solution you will find online for this chapter is written for a calculus-based course, and a solution that begins by differentiating is not a PHYS 101 solution even when its final number is right.

The thread running through all ten exercises: the centripetal force is not a force to add to your diagram, it is a NAME given to the resultant of the forces already on it. The routine never changes, draw the real forces, point an axis at the centre of the circle, and write that their sum along that axis is mv2/rmv^{2}/r. The same reversal governs friction: static friction has no value of its own, it takes whatever value prevents the sliding, and μsN\mu_{s}N is only the ceiling it may not pass.

The traps named explicitly in the solutions: writing fs=μsNf_{s} = \mu_{s}N for a block that is merely at rest, using N=mgcosθN = mg\cos\theta on a banked curve where the acceleration is horizontal, reading ac=v2/ra_{c} = v^{2}/r as though a larger radius always meant a smaller acceleration, feeding an altitude into rr in the law of gravitation instead of a distance from the centre, taking a square root where Kepler's law calls for a cube root, and explaining a centrifuge or a bucket of water with a centrifugal force that no object exerts.

10 corrected exercises • 100 points • 150 minutes

Course recap

  • Static friction is an INEQUALITY: fsμsNf_{s} \le \mu_{s}N. Its actual value balances the other forces along the surface; μsN\mu_{s}N is only the ceiling.
  • Kinetic friction is fixed: fk=μkNf_{k} = \mu_{k}N, directed against the motion, and μk<μs\mu_{k} < \mu_{s} for the same pair of surfaces.
  • On an incline at angle θ\theta, the axes follow the surface: N=mgcosθN = mg\cos\theta across it and mgsinθmg\sin\theta along it. A block lets go at tanθs=μs\tan\theta_{s} = \mu_{s}.
  • Uniform circular motion: ac=v2r=4π2rT2a_{c} = \frac{v^{2}}{r} = \frac{4\pi^{2}r}{T^{2}}, always directed at the centre. The speed is constant, the velocity is not.
  • Centripetal force is not a new force. It is the RESULTANT along the radius of the real forces, and it equals mv2/rmv^{2}/r.
  • Flat curve: friction alone turns the car, so vmax=μsgrv_{\max} = \sqrt{\mu_{s}gr}. Banked curve with no friction: tanθ=v2rg\tan\theta = \frac{v^{2}}{rg}, and N=mgcosθN = \frac{mg}{\cos\theta}, LARGER than mgmg.
  • Vertical circle at the top: tension and weight both point inward, T+mg=mv2rT + mg = \frac{mv^{2}}{r}, so the rope goes slack below vmin=grv_{\min} = \sqrt{gr}. At the bottom, Tmg=mv2rT - mg = \frac{mv^{2}}{r}.
  • Universal gravitation: F=Gm1m2r2F = G\frac{m_{1}m_{2}}{r^{2}} with rr measured CENTRE to centre, and g=GMR2g = \frac{GM}{R^{2}} at the surface of a body of mass MM and radius RR.
  • Circular orbit: v=GMrv = \sqrt{\frac{GM}{r}} and T2=4π2GMr3T^{2} = \frac{4\pi^{2}}{GM}r^{3}. The mass of the satellite cancels out of both.
  • Apparent weight is the NORMAL force, not mgmg: N=m(g±v2r)N = m\left(g \pm \frac{v^{2}}{r}\right), plus at the bottom of a dip, minus at the top of a crest. Weightlessness in orbit is N=0N = 0, never g=0g = 0.

Part A: the basics (/50)

Exercise 1: The force that has no value of its own

A crate of mass m=25m = 25 kg sits on a level concrete floor. The coefficient of static friction between crate and floor is μs=0.45\mu_{s} = 0.45, the coefficient of kinetic friction is μk=0.32\mu_{k} = 0.32. Take g=9.8g = 9.8 m/s2^2.

A worker pushes horizontally. The figure shows the situation and the free-body diagram of the crate: four forces, and not one of them is called a friction formula until you know whether the crate is sliding.

F25 kgNmgFf
  • a) The worker pushes with F=60F = 60 N. Give the normal force, the friction force and the acceleration.
  • b) He pushes harder, F=110F = 110 N, and the crate still has not moved. Give the friction force now.
  • c) He pushes with F=130F = 130 N. Give the friction force and the acceleration.
  • d) Sketch the friction force as a function of the applied force, from F=0F = 0 to F=160F = 160 N, and explain the jump.
Show the solution

Answers

  • a) N=245N = 245 N, f=60f = 60 N, a=0a = 0
  • b) f=110f = 110 N (the ceiling is 110.25110.25 N, not yet reached)
  • c) f=fk=78.4f = f_{k} = 78.4 N and a=2.06a = 2.06 m/s2^2
  • d) A straight line f=Ff = F up to 110.25110.25 N, then a drop to 78.478.4 N, then a horizontal line at 78.478.4 N

The normal force first, because both coefficients multiply it. The floor is level and the push is horizontal, so nothing has a vertical component except NN and the weight: N=mg=25×9.8=245N = mg = 25 \times 9.8 = 245 N. Write this line once, use it three times. The ceiling on static friction is fs,max=μsN=0.45×245=110.25f_{s,\max} = \mu_{s} N = 0.45 \times 245 = 110.25 N and the sliding value is fk=μkN=0.32×245=78.4f_{k} = \mu_{k} N = 0.32 \times 245 = 78.4 N. Both numbers exist before you know what the crate does.

a) Compare F=60F = 60 N with the ceiling 110.25110.25 N. The push is below it, so the crate does not move, and if it does not move its acceleration is zero. Newton's first law along the floor then says the horizontal forces cancel: f=F=60f = F = 60 N. Notice what was NOT done here: μsN\mu_{s} N was not used as the answer. Static friction is not a formula, it is whatever number balances the push, and μsN\mu_{s} N is only the largest number it is allowed to take.

b) Same reasoning, F=110F = 110 N, and 110<110.25110 < 110.25: still stuck, so f=110f = 110 N and a=0a = 0. The crate is 0.250.25 N away from moving and the friction force is 110110 N, not 110.25110.25 N. Writing f=110.25f = 110.25 N here is the single most common error of the chapter and it costs the whole question, because it puts a net force of 0.25-0.25 N on a crate that is standing still.

c) Now 130>110.25130 > 110.25: the crate breaks loose and slides. The moment it slides, friction stops adjusting and locks at fk=78.4f_{k} = 78.4 N. Newton's second law along the direction of motion: a=Ffkm=13078.425=51.625=2.06a = \frac{F - f_{k}}{m} = \frac{130 - 78.4}{25} = \frac{51.6}{25} = 2.06 m/s2^2. Sanity check: the answer must be positive and small, a few m/s2^2 for a shove on a heavy crate, and it is.

d) The graph is a straight line of slope 11 from the origin to the point (110.25; 110.25)(110.25;\ 110.25), then a vertical drop to 78.478.4 N, then a horizontal line. The drop is the physical content of the chapter: at the instant the crate starts to slide, friction falls from 110.25110.25 N to 78.478.4 N, so the net force jumps from 00 to 110.2578.4=31.85110.25 - 78.4 = 31.85 N and the crate leaps forward at a=31.85/25=1.27a = 31.85/25 = 1.27 m/s2^2 with no extra push. That is why a heavy box you are straining against suddenly shoots away.

The trap, and what it costs. Two symbols, μsN\mu_{s} N and fsf_{s}, are not the same object: the first is a ceiling, the second is the actual force, and fsμsNf_{s} \le \mu_{s} N is an INEQUALITY. Every friction question begins with the comparison test, FF against μsN\mu_{s} N, and only then chooses between f=Ff = F and f=μkNf = \mu_{k} N. Skipping the test is worth 3 to 4 points on a midterm because every later number inherits the wrong friction.

2040608010012014016020406080100120140f = Fpeak 110.25 Nthen 78.4 NF applied (N)friction f (N)

Exercise 2: The incline that carries friction, and the angle where it lets go

A block of mass m=4.0m = 4.0 kg is placed on a plank. The plank is slowly tilted. The coefficients between block and plank are μs=0.60\mu_{s} = 0.60 and μk=0.45\mu_{k} = 0.45. Take g=9.8g = 9.8 m/s2^2.

The figure shows the three real forces acting on the block at a general angle θ\theta: the weight, the normal force and friction. There is no fourth arrow, and in particular nothing pushing the block along the plank.

Nmgfθ
  • a) At θ=25\theta = 25^{\circ} the block has not moved. Give the friction force on it.
  • b) Find the angle θs\theta_{s} at which the block is on the point of sliding.
  • c) Show that θs\theta_{s} does not depend on the mass of the block.
  • d) The plank is held at θ=35\theta = 35^{\circ}. Find the acceleration of the sliding block.
Show the solution

Answers

  • a) f=mgsin25=16.6f = mg\sin 25^{\circ} = 16.6 N (well under the ceiling of 21.321.3 N)
  • b) θs=arctan(0.60)=31.0\theta_{s} = \arctan(0.60) = 31.0^{\circ}
  • c) mm cancels: tanθs=μs\tan\theta_{s} = \mu_{s} contains no mass
  • d) a=g(sin35μkcos35)=2.01a = g(\sin 35^{\circ} - \mu_{k}\cos 35^{\circ}) = 2.01 m/s2^2 down the plank

Axes along and across the plank, as in chapter 4, and only the weight needs splitting. Across the plank: N=mgcosθN = mg\cos\theta. Along the plank, taking down-slope as positive: mgsinθfmg\sin\theta - f. Nothing here is new except that ff is no longer zero.

a) At θ=25\theta = 25^{\circ} the block is at rest, so the along-plank forces cancel: f=mgsin25=4.0×9.8×0.4226=16.6f = mg\sin 25^{\circ} = 4.0 \times 9.8 \times 0.4226 = 16.6 N, directed UP the plank. Then check that this is allowed: the ceiling is μsmgcos25=0.60×4.0×9.8×0.9063=21.3\mu_{s} mg\cos 25^{\circ} = 0.60 \times 4.0 \times 9.8 \times 0.9063 = 21.3 N, and 16.6<21.316.6 < 21.3, so the block can indeed hold. Answering 21.321.3 N here is the same error as in exercise 1 in a new costume, and it is worth 2 points.

b) The block is on the point of sliding when the demand meets the ceiling: mgsinθs=μsmgcosθsmg\sin\theta_{s} = \mu_{s}\, mg\cos\theta_{s}, hence tanθs=μs=0.60\tan\theta_{s} = \mu_{s} = 0.60 and θs=arctan(0.60)=31.0\theta_{s} = \arctan(0.60) = 31.0^{\circ}. Check it against part a: 25<31.025^{\circ} < 31.0^{\circ}, so the block was indeed still holding, and the two answers agree.

c) Both sides of mgsinθs=μsmgcosθsmg\sin\theta_{s} = \mu_{s} mg\cos\theta_{s} carry the factor mgmg, which cancels. The tipping angle depends on the two surfaces and on nothing else: a 44 kg block and a 400400 kg block let go at the same 31.031.0^{\circ}. This is the standard laboratory measurement of μs\mu_{s}, and it is why you never need a balance to perform it.

d) At θ=35>θs\theta = 35^{\circ} > \theta_{s} the block slides, so friction locks at fk=μkmgcosθf_{k} = \mu_{k} mg\cos\theta and points UP the plank, against the motion. Newton's second law along the plank: ma=mgsinθμkmgcosθma = mg\sin\theta - \mu_{k} mg\cos\theta, so a=g(sinθμkcosθ)=9.8×(0.57360.45×0.8192)=9.8×0.2050=2.01a = g(\sin\theta - \mu_{k}\cos\theta) = 9.8 \times (0.5736 - 0.45 \times 0.8192) = 9.8 \times 0.2050 = 2.01 m/s2^2 down the plank. The mass has cancelled again, which is the check to run before reaching for the calculator.

What the numbers must obey. The answer to d has to sit between 00 and gsin35=5.62g\sin 35^{\circ} = 5.62 m/s2^2, the frictionless value of chapter 4: friction can only slow a slide, never reverse it or speed it up. Getting aa larger than 5.625.62 m/s2^2 means a sign error on ff; getting aa negative at an angle above θs\theta_{s} means μk\mu_{k} was used where μs\mu_{s} belonged. And the block never accelerates UP the plank: at rest above θs\theta_{s} it starts down, at rest below it stays put.

Exercise 3: Accelerating without going any faster

A coin lies on a turntable at a distance r=0.12r = 0.12 m from the axis. The turntable spins at 4545 revolutions per minute and the coin turns with it, without sliding. Take g=9.8g = 9.8 m/s2^2.

The figure is the view from above: the dashed circle is the path of the coin, and the two arrows are its velocity and its acceleration at one instant.

var = 0.12 m45 rpm
  • a) Find the period of one revolution and the speed of the coin.
  • b) Find the magnitude of the centripetal acceleration, by two different routes.
  • c) Name the force that produces this acceleration, and find the smallest coefficient of static friction that keeps the coin in place.
  • d) The coin is moved to r=0.24r = 0.24 m, the turntable still at 4545 rpm. Does the required coefficient double, halve or stay the same?
Show the solution

Answers

  • a) T=1.33T = 1.33 s and v=0.565v = 0.565 m/s
  • b) ac=2.66a_{c} = 2.66 m/s2^2, by v2/rv^{2}/r and by 4π2r/T24\pi^{2}r/T^{2}
  • c) Static friction from the turntable surface, pointing at the axis; μs0.272\mu_{s} \ge 0.272
  • d) It doubles, to 0.5440.544: at fixed TT, aca_{c} is proportional to rr

a) 4545 revolutions per minute is 45/60=0.7545/60 = 0.75 revolution per second, so one revolution takes T=1/0.75=1.33T = 1/0.75 = 1.33 s. In one period the coin travels one circumference: v=2πrT=2π×0.121.3333=0.565v = \frac{2\pi r}{T} = \frac{2\pi \times 0.12}{1.3333} = 0.565 m/s. Slow, which is what you expect from a record player.

b) Two routes, and they must agree. ac=v2r=0.56520.12=0.31980.12=2.66a_{c} = \frac{v^{2}}{r} = \frac{0.565^{2}}{0.12} = \frac{0.3198}{0.12} = 2.66 m/s2^2. Or, skipping the speed entirely, ac=4π2rT2=4π2×0.121.33332=4.7381.778=2.66a_{c} = \frac{4\pi^{2} r}{T^{2}} = \frac{4\pi^{2} \times 0.12}{1.3333^{2}} = \frac{4.738}{1.778} = 2.66 m/s2^2. The second form is the one to use whenever the data are a period or a rotation rate, because it never asks you to compute vv first. Both say the same thing: the speed of the coin never changes, and it is accelerating all the same, because the DIRECTION of its velocity turns through a full circle every 1.331.33 s.

c) There is no string, no hand, nothing pushing the coin sideways except the surface it rests on: the centripetal force is supplied by STATIC friction, pointing from the coin toward the axis. Note that static friction is what holds the coin, not kinetic: the coin does not slide on the turntable, it rides with it. Newton's second law along the radius, positive toward the centre: fs=macf_{s} = m a_{c}, and the ceiling is fsμsN=μsmgf_{s} \le \mu_{s} N = \mu_{s} mg. So macμsmgm a_{c} \le \mu_{s} mg, the mass cancels, and μsacg=2.66489.8=0.272\mu_{s} \ge \frac{a_{c}}{g} = \frac{2.6648}{9.8} = 0.272. A copper coin on felt clears this easily, which is why the coin stays.

d) The trap is to read ac=v2/ra_{c} = v^{2}/r and conclude that a bigger radius means a smaller acceleration. It would, at fixed SPEED. Here the turntable rate is fixed, so TT is fixed and vv doubles along with rr: use ac=4π2r/T2a_{c} = 4\pi^{2}r/T^{2}, which is proportional to rr. The acceleration doubles to 5.335.33 m/s2^2 and the required coefficient doubles to 0.5440.544. Check by the other route: v=2π(0.24)/1.3333=1.131v = 2\pi(0.24)/1.3333 = 1.131 m/s and v2/r=1.279/0.24=5.33v^{2}/r = 1.279/0.24 = 5.33 m/s2^2. Same number.

The lesson worth carrying. The two formulas for aca_{c} are the same formula, but they hold different things fixed in your head, and choosing the wrong one produces an answer that is wrong by a factor of four. Ask what the problem keeps constant, the speed or the rotation rate, before choosing. On the turntable, the outer coins fly off first, exactly the opposite of what v2/rv^{2}/r suggests to a careless reader.

Exercise 4: Universal gravitation and the surface of a planet

Newton's law of universal gravitation gives the attraction between two masses a distance rr apart, measured centre to centre: F=Gm1m2r2F = G\frac{m_{1}m_{2}}{r^{2}} with G=6.67×1011G = 6.67 \times 10^{-11} N m2^2/kg2^2.

Mars has mass M=6.42×1023M = 6.42 \times 10^{23} kg and radius R=3.39×106R = 3.39 \times 10^{6} m. Take g=9.8g = 9.8 m/s2^2 on Earth.

  • a) Find gg at the surface of Mars.
  • b) An astronaut with a mass of 7070 kg stands on Mars. Give her mass and her weight there, and her weight on Earth.
  • c) Find the altitude above the Martian surface at which gg has fallen to half its surface value.
  • d) A classmate says that at an altitude equal to one Martian radius, gg is half. Correct him with a number.
Show the solution

Answers

  • a) gM=3.73g_{M} = 3.73 m/s2^2
  • b) Mass 7070 kg on both; weight 261261 N on Mars, 686686 N on Earth
  • c) h=R(21)=1.40×106h = R(\sqrt{2} - 1) = 1.40 \times 10^{6} m, about 14001400 km
  • d) At r=2Rr = 2R, gg is a QUARTER: 0.9320.932 m/s2^2

a) An object of mass mm on the surface feels F=GMmR2F = G\frac{Mm}{R^{2}}, and by definition that same force is mgMmg_{M}. The mm cancels, which is the whole reason a surface gravity exists at all: gM=GMR2=6.67×1011×6.42×1023(3.39×106)2=4.282×10131.149×1013=3.73g_{M} = \frac{GM}{R^{2}} = \frac{6.67\times 10^{-11} \times 6.42\times 10^{23}}{(3.39\times 10^{6})^{2}} = \frac{4.282\times 10^{13}}{1.149\times 10^{13}} = 3.73 m/s2^2. Order of magnitude check: Mars is about a tenth of Earth's mass and about half its radius, so gg should be roughly 0.1/0.25=0.40.1/0.25 = 0.4 of Earth's, and 3.73/9.8=0.383.73/9.8 = 0.38.

b) Mass is the amount of matter and it travels unchanged: 7070 kg on Mars, 7070 kg on Earth, 7070 kg in orbit. Weight is a FORCE, w=mgw = mg, and it changes with the planet: wM=70×3.726=261w_{M} = 70 \times 3.726 = 261 N, against wE=70×9.8=686w_{E} = 70 \times 9.8 = 686 N. Writing the Martian weight in kilograms is worth a point on any exam, and writing that her mass is smaller on Mars is worth the whole part.

c) g(r)=GMr2g(r) = \frac{GM}{r^{2}}, and we want g(r)=12gMg(r) = \frac{1}{2}g_{M}, so GMr2=12GMR2\frac{GM}{r^{2}} = \frac{1}{2}\frac{GM}{R^{2}}. Everything cancels except the radii: r2=2R2r^{2} = 2R^{2}, so r=R2=4.79×106r = R\sqrt{2} = 4.79\times 10^{6} m. That is the distance from the CENTRE. The altitude is h=rR=4.794×1063.39×106=1.40×106h = r - R = 4.794\times 10^{6} - 3.39\times 10^{6} = 1.40\times 10^{6} m, about 14001400 km. Forgetting the last subtraction turns an altitude into a radius and is the most frequent loss of the question.

d) At an altitude of one radius, the distance from the centre is r=2Rr = 2R, and an inverse SQUARE divides by 22=42^{2} = 4, not by 22: g(2R)=3.7264=0.932g(2R) = \frac{3.726}{4} = 0.932 m/s2^2. To halve gg you go out by a factor 21.41\sqrt{2} \approx 1.41, which is part c. The mental rule worth keeping: distance times 22 means force divided by 44, distance times 33 means force divided by 99.

Where the rr is measured, and why it matters. In F=GMm/r2F = GMm/r^{2}, rr is the separation of the CENTRES, never the height above the ground. For anything on or near a planet that distinction is the whole problem: at 400400 km above Earth, rr is 67706770 km and not 400400 km, so gg is still about 8989 per cent of its surface value. A solution that feeds an altitude into rr produces gravitational fields thousands of times too strong and should be caught by the order-of-magnitude check before it is handed in.

Exercise 5: A circular orbit, its period, and Kepler's third law

A satellite of mass mm moves in a circular orbit of radius rr around the Earth, M=5.97×1024M = 5.97\times 10^{24} kg, RE=6.37×106R_{E} = 6.37\times 10^{6} m, G=6.67×1011G = 6.67\times 10^{-11} N m2^2/kg2^2. Use GM=3.982×1014GM = 3.982\times 10^{14} in SI units.

Nothing is pushing the satellite forward. One single force acts on it, and it points at the centre of the Earth.

  • a) Starting from Newton's second law along the radius, show that v=GM/rv = \sqrt{GM/r} and that T2=4π2GMr3T^{2} = \frac{4\pi^{2}}{GM}r^{3}.
  • b) The International Space Station orbits at an altitude of 400400 km. Find its speed and its period in minutes.
  • c) A geostationary satellite has a period of 2424 h. Find its orbital radius and its altitude.
  • d) Check your two results against each other using Kepler's third law alone, without recomputing anything.
Show the solution

Answers

  • a) GMm/r2=mv2/rGMm/r^{2} = mv^{2}/r gives v=GM/rv = \sqrt{GM/r}, then T=2πr/vT = 2\pi r/v gives T2=4π2r3/(GM)T^{2} = 4\pi^{2}r^{3}/(GM)
  • b) v=7.67v = 7.67 km/s and T=5546T = 5546 s, about 92.492.4 min
  • c) r=4.22×107r = 4.22\times 10^{7} m, altitude 3.59×1073.59\times 10^{7} m, about 3590035\,900 km
  • d) (r2/r1)3/2=15.6(r_{2}/r_{1})^{3/2} = 15.6 and 92.4×15.6=144092.4 \times 15.6 = 1440 min =24= 24 h

a) The satellite travels a circle at constant speed, so its acceleration is v2/rv^{2}/r toward the centre. The only force on it is gravity, also toward the centre. Newton's second law along the radius therefore reads GMmr2=mv2rG\frac{Mm}{r^{2}} = m\frac{v^{2}}{r}. The mass of the SATELLITE cancels, which is the headline result: the orbit does not care whether you send up a bolt or a space station. Simplify one power of rr: v2=GMrv^{2} = \frac{GM}{r}, so v=GM/rv = \sqrt{GM/r}. For the period, one lap is one circumference at that speed, T=2πrv=2πrrGMT = \frac{2\pi r}{v} = 2\pi r\sqrt{\frac{r}{GM}}, and squaring gives T2=4π2GMr3T^{2} = \frac{4\pi^{2}}{GM}r^{3}, which is Kepler's third law with the constant made explicit.

b) The radius is measured from the CENTRE of the Earth: r=6.37×106+4.00×105=6.77×106r = 6.37\times 10^{6} + 4.00\times 10^{5} = 6.77\times 10^{6} m. Then v=3.982×10146.77×106=5.882×107=7.67×103v = \sqrt{\frac{3.982\times 10^{14}}{6.77\times 10^{6}}} = \sqrt{5.882\times 10^{7}} = 7.67\times 10^{3} m/s, about 7.677.67 km/s or 2760027\,600 km/h. Period: T=2π×6.77×1067669=5546T = \frac{2\pi \times 6.77\times 10^{6}}{7669} = 5546 s =92.4= 92.4 min. The astronauts see a sunrise roughly every hour and a half, which is the check everybody can remember.

c) Here the period is the datum, so invert the law: r3=GMT24π2r^{3} = \frac{GM\,T^{2}}{4\pi^{2}} with T=24×3600=86400T = 24 \times 3600 = 86\,400 s. Then r3=3.982×1014×7.465×10939.478=7.530×1022r^{3} = \frac{3.982\times 10^{14} \times 7.465\times 10^{9}}{39.478} = 7.530\times 10^{22} m3^3, and the cube root is r=4.22×107r = 4.22\times 10^{7} m. Altitude: 4.22×1076.37×106=3.59×1074.22\times 10^{7} - 6.37\times 10^{6} = 3.59\times 10^{7} m, about 3590035\,900 km, the number quoted for every television satellite. Taking the square root instead of the cube root is the classic slip, and it gives 2.7×10112.7\times 10^{11} m, well past the Moon: the order of magnitude catches it instantly.

d) Kepler's third law says T2/r3T^{2}/r^{3} is the same for every satellite of the same planet, so T2T1=(r2r1)3/2\frac{T_{2}}{T_{1}} = \left(\frac{r_{2}}{r_{1}}\right)^{3/2}. Here r2r1=4.222×1076.77×106=6.236\frac{r_{2}}{r_{1}} = \frac{4.222\times 10^{7}}{6.77\times 10^{6}} = 6.236 and 6.2363/2=15.586.236^{3/2} = 15.58. So T2=92.4×15.58=1440T_{2} = 92.4 \times 15.58 = 1440 min =24= 24 h. The two independent calculations agree, which is what the ratio form is for: it needs no constants and no calculator memory, only the two radii.

Two things to keep. Orbital speed goes DOWN as you climb, v1/rv \propto 1/\sqrt{r}, which surprises everyone: the geostationary satellite moves at 3.073.07 km/s, less than half the ISS. And the mass of the satellite is absent from every result on this page, so any answer of yours in which it survives contains an algebra error, not a physical effect.

Part B: problems and reasoning (/50)

Exercise 6: The banked curve and the conical pendulum are the same problem

A highway exit is banked at θ=12\theta = 12^{\circ} and follows a circle of radius r=85r = 85 m. The figure is a cross-section: the centre of the turn is off to the left, and the acceleration of the car is HORIZONTAL, pointing at that centre.

In the second half of the question, a ball of mass 0.500.50 kg hangs from a string of length L=1.20L = 1.20 m and is swung so that the string traces a cone, making a constant angle of 2525^{\circ} with the vertical. Take g=9.8g = 9.8 m/s2^2.

Nmgcentre12°
  • a) Find the speed at which a car rounds the banked curve with no help from friction, in m/s and in km/h.
  • b) For a car of mass 12001200 kg at that speed, find the normal force, and compare it with the weight.
  • c) For the conical pendulum, find the radius of the circle, the speed of the ball and the time for one revolution.
  • d) Write the one pair of equations that solves both situations, and say what plays the part of the string in the car problem.
Show the solution

Answers

  • a) v=rgtanθ=13.3v = \sqrt{rg\tan\theta} = 13.3 m/s, about 47.947.9 km/h
  • b) N=mg/cosθ=1.20×104N = mg/\cos\theta = 1.20\times 10^{4} N, larger than mg=1.18×104mg = 1.18\times 10^{4} N
  • c) r=0.507r = 0.507 m, v=1.52v = 1.52 m/s, one revolution in 2.092.09 s
  • d) Vertical: Xcosθ=mgX\cos\theta = mg. Horizontal: Xsinθ=mv2/rX\sin\theta = mv^{2}/r. The normal force plays the part of the tension

Set the axes horizontal and vertical, not along the slope. This is the single decision the question turns on, and it is the opposite of exercise 2. On an incline a block accelerates ALONG the surface, so axes follow the surface. On a banked curve the car has no vertical acceleration at all and its acceleration is horizontal, toward the centre. Use horizontal and vertical axes and split the NORMAL force instead of the weight.

a) Two real forces on a frictionless banked car, NN perpendicular to the road and mgmg down. Vertical, no acceleration: Ncosθ=mgN\cos\theta = mg. Horizontal, toward the centre: Nsinθ=mv2rN\sin\theta = \frac{mv^{2}}{r}. Divide the second by the first and both NN and mm vanish: tanθ=v2rg\tan\theta = \frac{v^{2}}{rg}, so v=rgtanθ=85×9.8×0.2126=177.1=13.3v = \sqrt{rg\tan\theta} = \sqrt{85 \times 9.8 \times 0.2126} = \sqrt{177.1} = 13.3 m/s, that is 47.947.9 km/h. A gentle 1212^{\circ} bank is designed for a slow ramp, which is what an exit is.

b) From the vertical equation, N=mgcosθ=1200×9.8cos12=117600.9781=1.20×104N = \frac{mg}{\cos\theta} = \frac{1200 \times 9.8}{\cos 12^{\circ}} = \frac{11\,760}{0.9781} = 1.20\times 10^{4} N. That is LARGER than the weight 1176011\,760 N, by about 22 per cent, and it must be: the road has to hold the car up and push it round the bend at the same time. Writing N=mgcosθN = mg\cos\theta here, the formula from the incline, gives 1150011\,500 N, smaller than the weight, and the sign of the error is visible without any calculation. That confusion is the most expensive single line of the chapter.

c) The ball moves in a HORIZONTAL circle whose radius is not the length of the string: r=Lsin25=1.20×0.4226=0.507r = L\sin 25^{\circ} = 1.20 \times 0.4226 = 0.507 m. Two real forces, tension XX along the string and weight mgmg down. Vertical: Xcos25=mgX\cos 25^{\circ} = mg. Horizontal: Xsin25=mv2/rX\sin 25^{\circ} = mv^{2}/r. Dividing again, tan25=v2rg\tan 25^{\circ} = \frac{v^{2}}{rg}, so v=0.5071×9.8×0.4663=2.318=1.52v = \sqrt{0.5071 \times 9.8 \times 0.4663} = \sqrt{2.318} = 1.52 m/s. One revolution: T=2πrv=3.1861.522=2.09T = \frac{2\pi r}{v} = \frac{3.186}{1.522} = 2.09 s. As a check, the tension is X=mgcos25=4.90.9063=5.41X = \frac{mg}{\cos 25^{\circ}} = \frac{4.9}{0.9063} = 5.41 N, again larger than the weight 4.94.9 N.

d) Both problems are the same two lines: Xcosθ=mgX\cos\theta = mg vertically and Xsinθ=mv2rX\sin\theta = \frac{mv^{2}}{r} horizontally, where XX is the one tilted force, the tension for the pendulum and the normal force for the car. Dividing kills XX and mm together and leaves tanθ=v2/(rg)\tan\theta = v^{2}/(rg) in both cases. In neither problem is there a force pushing outward. What an outward arrow would represent is the seat pressing on your back, an interaction between you and the car, and it has no place in the diagram of the CAR.

How to read tanθ=v2/(rg)\tan\theta = v^{2}/(rg). It contains no mass, so a loaded truck and a motorcycle have the same design speed on the same ramp. It rises with v2v^{2}, so doubling the design speed demands tanθ\tan\theta four times larger. And it is a DESIGN speed, not a limit: below it the car tends to slide down the bank and friction must point up the slope, above it friction must point down. Chapter 6 will not change any of this, because none of it is about energy.

Exercise 7: The bucket at the top of the circle

A bucket holding water, total mass 3.03.0 kg, is swung in a vertical circle at the end of a rope of length L=1.10L = 1.10 m, as in the figure. The rope is attached at OO.

The speed is not the same all the way round, so each part below gives you the speed at the point it asks about. Take g=9.8g = 9.8 m/s2^2.

L = 1.10 mtopbottomO
  • a) Draw the forces on the bucket at the TOP of the circle and write Newton's second law along the radius there.
  • b) Find the smallest speed at the top for which the rope stays taut.
  • c) At the top the bucket is moving at 4.54.5 m/s. Find the tension in the rope.
  • d) At the bottom it is moving at 6.06.0 m/s. Find the tension, and compare it with the weight.
Show the solution

Answers

  • a) Tension and weight BOTH point downward, toward the centre: T+mg=mv2/LT + mg = mv^{2}/L
  • b) vmin=gL=3.28v_{\min} = \sqrt{gL} = 3.28 m/s
  • c) T=m(v2/Lg)=25.8T = m(v^{2}/L - g) = 25.8 N
  • d) T=m(v2/L+g)=128T = m(v^{2}/L + g) = 128 N, about 4.34.3 times the weight 29.429.4 N

a) At the top of the circle the centre is BELOW the bucket, so the inward direction is downward. Two real forces act: the rope pulls the bucket toward OO, that is downward, and the weight also acts downward. Both arrows point the same way, which is the feature of this position and the reason it is examined. Taking downward as positive because that is toward the centre: T+mg=mv2LT + mg = \frac{mv^{2}}{L}. There is no third arrow. Nothing holds the bucket up at the top, and the water does not need holding up.

b) The rope can pull but never push, so T0T \ge 0. The limiting case is T=0T = 0, where gravity alone bends the path: mg=mvmin2Lmg = \frac{mv_{\min}^{2}}{L}, the mass cancels, and vmin=gL=9.8×1.10=10.78=3.28v_{\min} = \sqrt{gL} = \sqrt{9.8 \times 1.10} = \sqrt{10.78} = 3.28 m/s. Below that speed the circle of radius 1.101.10 m would demand less centripetal force than gravity already supplies, so the bucket falls inside the circle and the rope goes slack. Note what vminv_{\min} does not contain: the mass. A bucket of water and an empty bucket let go at the same speed.

c) T=m(v2Lg)=3.0×(4.521.109.8)=3.0×(18.419.80)=25.8T = m\left(\frac{v^{2}}{L} - g\right) = 3.0 \times \left(\frac{4.5^{2}}{1.10} - 9.8\right) = 3.0 \times (18.41 - 9.80) = 25.8 N. The bracket is positive because 4.5>3.284.5 > 3.28, as it must be. A negative tension is not a physical answer, it is the signal that the speed given is below vminv_{\min} and that the object has already left the circular path.

d) At the bottom the centre is ABOVE, so inward is upward, and the two forces now oppose each other: Tmg=mv2LT - mg = \frac{mv^{2}}{L}, giving T=m(v2L+g)=3.0×(361.10+9.8)=3.0×42.53=128T = m\left(\frac{v^{2}}{L} + g\right) = 3.0 \times \left(\frac{36}{1.10} + 9.8\right) = 3.0 \times 42.53 = 128 N. Compare with the weight, 3.0×9.8=29.43.0 \times 9.8 = 29.4 N: the rope carries about 4.34.3 times the weight at the bottom and only 25.825.8 N at the top. The rope breaks at the bottom of the swing, never at the top, and that is what the two signs are telling you.

Why the water does not fall out, said properly. Not because something throws it outward. At the top the bucket's bottom is above the water and can only PUSH the water downward, toward the centre. That push plus the water's own weight is exactly the centripetal force the circle demands. At vminv_{\min} the bucket pushes with zero force and gravity does the whole job; below vminv_{\min} gravity is more than the circle needs, so the water falls inside the circle, which from the ground looks like it landing on your head. An answer built on a centrifugal force gets the right feeling and the wrong physics, and examiners mark the reasoning.

Tmgacentre

Exercise 8: Five statements to correct

For each statement, say whether it is true or false. If it is false, rewrite it so that it becomes true, and give the number that settles it.

Full marks require the correction, not the verdict alone.

  • a) The force of kinetic friction on a sliding block is, to a good approximation, independent of the area of contact and of the speed.
  • b) The force of static friction on a block at rest equals μsN\mu_{s}N.
  • c) An object moving in a circle has, on top of the forces acting on it, a centripetal force that must be added to its free-body diagram.
  • d) Astronauts float inside the International Space Station because there is no gravity 400400 km above the ground.
  • e) A loaded truck needs a larger coefficient of static friction than a small car to take the same flat curve at the same speed.
Show the solution

Answers

  • a) TRUE, and it is the useful part of the model fk=μkNf_{k} = \mu_{k}N
  • b) FALSE: fsμsNf_{s} \le \mu_{s}N, with equality only on the point of slipping
  • c) FALSE: the centripetal force is the NAME of the resultant of the forces already drawn
  • d) FALSE: gg is still 8.698.69 m/s2^2 there, 8989 per cent of its ground value; they are in free fall
  • e) FALSE: μsv2/(rg)\mu_{s} \ge v^{2}/(rg) contains no mass, so both need the same coefficient

a) TRUE. The model fk=μkNf_{k} = \mu_{k} N says friction depends on how hard the surfaces are pressed together and on the pair of materials, and on nothing else. Doubling the contact area halves the pressure at every point and leaves the total force unchanged, which is why a brick slides the same way on its face and on its edge. It is an approximation, and it fails at very high speeds and for tyres near their limit, but on this course it is exact. Be careful not to over-correct a true statement: rewriting a true line costs marks as surely as missing a false one.

b) FALSE. μsN\mu_{s}N is a CEILING, not a value: fsμsNf_{s} \le \mu_{s}N. The actual static friction takes whatever value is needed to keep the block still, and it equals μsN\mu_{s}N in exactly one situation, on the point of slipping. Correct version: the force of static friction on a block at rest is whatever is needed to balance the other forces along the surface, and it cannot exceed μsN\mu_{s}N. The number from exercise 1: with N=245N = 245 N and μs=0.45\mu_{s} = 0.45 the ceiling is 110.25110.25 N, but under a push of 6060 N the friction force is 6060 N.

c) FALSE. The forces on an object are the ones other objects exert on it: gravity, a normal force, tension, friction. Circular motion adds none. The phrase centripetal force names the RESULTANT of those real forces, taken along the direction of the centre, and its value is mv2/rmv^{2}/r. Correct version: for an object in uniform circular motion, the resultant of the real forces points at the centre and has magnitude mv2/rmv^{2}/r. Adding an extra arrow labelled FcF_{c} counts the same force twice and makes the resultant zero, so the object should travel in a straight line, which it plainly does not.

d) FALSE, and doubly so. The figure shows gg against altitude: at 400400 km, g=GMr2=3.982×1014(6.77×106)2=8.69g = \frac{GM}{r^{2}} = \frac{3.982\times 10^{14}}{(6.77\times 10^{6})^{2}} = 8.69 m/s2^2, that is 8989 per cent of the 9.819.81 m/s2^2 at the ground. Gravity is what holds the station in orbit at all, as exercise 5 shows. Correct version: astronauts float because the station and everything in it are in free fall together, accelerating toward the Earth at 8.698.69 m/s2^2, so nothing presses on the floor. What is zero is the apparent weight, that is the normal force, never gg.

e) FALSE. On a flat curve the friction force supplies the whole centripetal force: fs=mv2rf_{s} = \frac{mv^{2}}{r} with fsμsmgf_{s} \le \mu_{s}mg. The mass cancels and leaves μsv2rg\mu_{s} \ge \frac{v^{2}}{rg}. For r=85r = 85 m at 13.313.3 m/s that is μs0.213\mu_{s} \ge 0.213, whatever the vehicle weighs. Correct version: the required coefficient of static friction depends only on the speed and the radius, so both vehicles need the same value. The truck does need a larger friction FORCE, since fs=mv2/rf_{s} = mv^{2}/r grows with its mass, but its normal force grows in the same proportion, and the two effects cancel exactly.

50010001500200025003000350040001234567891011ground: 9.81ISS 400 km: 8.69altitude above the ground (km)g (m/s²)

Exercise 9: The laboratory centrifuge

A benchtop centrifuge spins samples at 1200012\,000 revolutions per minute. A tube sits so that the material at its far end is r=8.5r = 8.5 cm from the axis of rotation. Take g=9.8g = 9.8 m/s2^2.

Catalogues quote centrifuges by their relative centrifugal field, the ratio of the centripetal acceleration to gg, written as a number followed by the symbol gg.

  • a) Find the period of one revolution and the centripetal acceleration at the far end of the tube.
  • b) Express that acceleration as a relative centrifugal field, and find the speed of the sample.
  • c) A protocol asks for twice the field. By what factor must the rotation rate be raised, and what rate is that?
  • d) A red blood cell is denser than the plasma around it. Explain, with forces only, why it ends up at the far end of the tube.
Show the solution

Answers

  • a) T=5.0T = 5.0 ms and ac=1.34×105a_{c} = 1.34\times 10^{5} m/s2^2
  • b) About 1.37×1041.37\times 10^{4} times gg; v=107v = 107 m/s
  • c) Rate multiplied by 2=1.41\sqrt{2} = 1.41, that is about 1700017\,000 rpm
  • d) The plasma cannot supply the cell the macma_{c} its circle demands, so the cell falls behind the circle and drifts outward

a) 1200012\,000 revolutions per minute is 200200 revolutions per second, so T=1200=5.0×103T = \frac{1}{200} = 5.0\times 10^{-3} s. With a period in hand, use the period form and never compute the speed first: ac=4π2rT2=4π2×0.085(5.0×103)2=3.3562.5×105=1.34×105a_{c} = \frac{4\pi^{2}r}{T^{2}} = \frac{4\pi^{2} \times 0.085}{(5.0\times 10^{-3})^{2}} = \frac{3.356}{2.5\times 10^{-5}} = 1.34\times 10^{5} m/s2^2. Watch the two unit conversions that decide the answer: 8.58.5 cm is 0.0850.085 m, and rpm is not a frequency in hertz until it is divided by 6060. A factor of 6060 in a squared quantity is a factor of 36003600 in the result.

b) Relative centrifugal field: acg=1342279.8=1.37×104\frac{a_{c}}{g} = \frac{134\,227}{9.8} = 1.37\times 10^{4}, quoted as about 1370013\,700 times gg, which is in the ordinary range of a benchtop machine. The speed at the far end is v=2πrT=2π×0.0855.0×103=107v = \frac{2\pi r}{T} = \frac{2\pi \times 0.085}{5.0\times 10^{-3}} = 107 m/s, roughly 385385 km/h, and this is why a rotor that comes loose destroys the instrument.

c) At fixed radius, ac=4π2rf2a_{c} = 4\pi^{2}rf^{2} with ff the rotation rate, so the field goes as the SQUARE of the rate. Doubling the field needs the rate multiplied by 2=1.414\sqrt{2} = 1.414: 12000×1.414=1697012\,000 \times 1.414 = 16\,970 rpm, call it 1700017\,000. Doubling the rpm, the instinctive answer, would multiply the field by four and can exceed the rated maximum of the rotor, which is a safety matter and not only an arithmetic one. The same square law is why a protocol is always quoted in times gg and not in rpm: the rpm figure means nothing without the radius of the rotor.

d) Everything inside the tube is being carried around a circle, so everything needs an inward resultant of macm a_{c}. For the liquid this comes from the pressure of the liquid behind it, higher near the wall, lower near the axis, exactly as the water in a bucket. A cell denser than the plasma has MORE mass in the same volume, so it needs more inward force than the plasma pressure around it supplies. The shortfall means its inward acceleration is smaller than the circle requires, so it cannot keep to its circle and drifts outward, toward the bottom of the tube, until it reaches the wall. Nothing threw it outward: it simply was not pulled inward hard enough.

The same reversal as the whole chapter. Sedimentation is usually explained by a centrifugal force pushing the heavy particles out, which predicts the right destination for the wrong reason and fails as soon as you ask what object exerts that force. Written with real forces only, the account also explains why a cell LESS dense than the medium, a fat globule in milk, moves INWARD: it needs less inward force than the surrounding pressure supplies, so it is pushed toward the axis, and the cream rises to the middle.

Exercise 10: Pulling out of a dive, and the limits of a pilot

A pilot pulls out of a dive along a circular arc of radius r=650r = 650 m at a constant speed of 180180 m/s. At the lowest point of the arc, the seat pushes up on her.

The apparent weight is the force the seat exerts, and flight medicine quotes it as a multiple of the true weight: above about 55 times, blood no longer reaches the retina and the pilot greys out. Take g=9.8g = 9.8 m/s2^2.

  • a) Find the centripetal acceleration on the arc.
  • b) Find the force of the seat on a pilot of mass 6565 kg at the lowest point, and express it as a multiple of her weight.
  • c) Find the largest speed on this arc for which the apparent weight stays at 55 times the true weight.
  • d) The same aircraft flies over the crest of a hill on an arc of the same radius. Find the speed at which the pilot feels weightless.
Show the solution

Answers

  • a) ac=v2/r=49.8a_{c} = v^{2}/r = 49.8 m/s2^2
  • b) N=3878N = 3878 N, about 6.096.09 times her weight of 637637 N
  • c) v=4gr=160v = \sqrt{4gr} = 160 m/s, about 575575 km/h
  • d) v=gr=79.8v = \sqrt{gr} = 79.8 m/s, about 287287 km/h

a) On a circular arc at constant speed the acceleration is centripetal: ac=v2r=1802650=32400650=49.8a_{c} = \frac{v^{2}}{r} = \frac{180^{2}}{650} = \frac{32\,400}{650} = 49.8 m/s2^2. Already about five times gg, and no force has been named yet. Reading this number before touching the forces is the fastest way to see where the problem is going.

b) At the bottom of the arc the centre of the circle is ABOVE the pilot, so inward is upward. Two real forces on her: the seat pushing up with NN, and her weight mgmg down. Newton's second law along the radius, upward positive: Nmg=mv2rN - mg = \frac{mv^{2}}{r}, so N=m(g+v2r)=65×(9.8+49.85)=65×59.65=3878N = m\left(g + \frac{v^{2}}{r}\right) = 65 \times (9.8 + 49.85) = 65 \times 59.65 = 3878 N. Her true weight is 65×9.8=63765 \times 9.8 = 637 N, so the ratio is 3878637=6.09\frac{3878}{637} = 6.09. Above the greyout threshold: without a pressure suit this manoeuvre is on the edge of consciousness.

c) Notice that the ratio never needed the mass: Nmg=1+v2rg\frac{N}{mg} = 1 + \frac{v^{2}}{rg}. Setting that to 55 gives v2rg=4\frac{v^{2}}{rg} = 4, so v=4gr=4×9.8×650=25480=160v = \sqrt{4gr} = \sqrt{4 \times 9.8 \times 650} = \sqrt{25\,480} = 160 m/s, about 575575 km/h. Check against part b: 160<180160 < 180, and a slower pass through the same arc must be gentler, so the inequality points the right way. Alternatively the pilot could keep 180180 m/s and open the arc out to a larger radius, r=v24g=827r = \frac{v^{2}}{4g} = 827 m, which is exactly what a pilot does in practice.

d) Over a crest the centre of the circle is BELOW, so inward is downward and the two forces swap roles: mgN=mv2rmg - N = \frac{mv^{2}}{r}, giving N=m(gv2r)N = m\left(g - \frac{v^{2}}{r}\right). Apparent weightlessness is N=0N = 0, which needs v2r=g\frac{v^{2}}{r} = g, that is v=gr=9.8×650=79.8v = \sqrt{gr} = \sqrt{9.8 \times 650} = 79.8 m/s, about 287287 km/h. This is the same condition as the bucket at the top of its circle in exercise 7, v=grv = \sqrt{gr}, and for the same reason: gravity alone bends the path, so nothing else needs to touch the object.

One equation, two signs, three sensations. Write N=m(g±v2r)N = m\left(g \pm \frac{v^{2}}{r}\right) and let the position choose the sign: plus at the bottom of a valley, minus at the top of a hill, and the answers to the whole chapter of apparent weight follow. The pilot is heavy at the bottom and light at the top, an astronaut in orbit is permanently at the N=0N = 0 case, and in none of these does gg change by a measurable amount. What changes is the force of the seat, which is the only thing your body can actually feel.

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