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Forces and Motion

Newton's Laws of Motion

First Law (Law of Inertia)

An object remains at rest or continues to move with uniform velocity unless acted upon by a net external force.

F=0    v=constant\sum \vec{F} = \vec{0} \implies \vec{v} = \mathrm{constant}

Inertia is the resistance of an object to changes in its state of motion. It is quantified by the object's mass: a larger mass implies greater inertia.

Second Law

The net force acting on an object equals the rate of change of its momentum:

Fnet=dpdt=d(mv)dt\vec{F}_{\mathrm{net}} = \frac{d\vec{p}}{dt} = \frac{d(m\vec{v})}{dt}

For constant mass this reduces to:

Fnet=ma\vec{F}_{\mathrm{net}} = m\vec{a}

The SI unit of force is the newton (N), where 1N=1kgm/s21 \mathrm{ N} = 1 \mathrm{ kg}\cdot\mathrm{m/s}^2.

Third Law

If body A exerts a force on body B, then body B exerts an equal and opposite force on body A:

FAB=FBA\vec{F}_{AB} = -\vec{F}_{BA}

Action-reaction pairs always act on different bodies. They are equal in magnitude, opposite in direction, and of the same type (both gravitational, both contact, etc.).

Worked Example 1

A block of mass 8kg8 \mathrm{ kg} is pushed across a rough horizontal surface by a horizontal force of 50N50 \mathrm{ N}. The coefficient of kinetic friction is 0.30.3. Find the acceleration.

Solution

Normal reaction: N=mg=8×9.81=78.48NN = mg = 8 \times 9.81 = 78.48 \mathrm{ N}

Friction: fk=μkN=0.3×78.48=23.54Nf_k = \mu_k N = 0.3 \times 78.48 = 23.54 \mathrm{ N}

a=Fnetm=5023.548=26.468=3.31m/s2a = \frac{F_{\mathrm{net}}}{m} = \frac{50 - 23.54}{8} = \frac{26.46}{8} = 3.31 \mathrm{ m/s}^2

Worked Example 2

Two blocks, m1=3kgm_1 = 3 \mathrm{ kg} and m2=5kgm_2 = 5 \mathrm{ kg}, are placed on a smooth horizontal table and connected by a light inextensible string. A horizontal force of 24N24 \mathrm{ N} is applied to m2m_2, pulling the system to the right. Find the acceleration and the tension in the string.

Solution

The two blocks move together with the same acceleration:

a=Fm1+m2=243+5=248=3.0m/s2a = \frac{F}{m_1 + m_2} = \frac{24}{3 + 5} = \frac{24}{8} = 3.0 \mathrm{ m/s}^2

For block m1m_1 alone, the only horizontal force is the tension TT:

T=m1a=3×3.0=9.0NT = m_1 a = 3 \times 3.0 = 9.0 \mathrm{ N}

Worked Example 3

A lift (elevator) of mass 800kg800 \mathrm{ kg} carries 3 passengers of total mass 210kg210 \mathrm{ kg}. The lift accelerates upward at 1.5m/s21.5 \mathrm{ m/s}^2 for the first 3 seconds. Find the tension in the cable during this acceleration and the distance travelled.

Solution

Total mass: m=800+210=1010kgm = 800 + 210 = 1010 \mathrm{ kg}

Applying Newton's second law upward: Tmg=maT - mg = ma

T=m(g+a)=1010(9.81+1.5)=1010×11.31=11423NT = m(g + a) = 1010(9.81 + 1.5) = 1010 \times 11.31 = 11423 \mathrm{ N}

Distance: s=ut+12at2=0+12(1.5)(9)=6.75ms = ut + \frac{1}{2}at^2 = 0 + \frac{1}{2}(1.5)(9) = 6.75 \mathrm{ m}


Friction

Static and Kinetic Friction

TypeSymbolConditionMagnitude
Staticfsf_sNo relative motion0fsμsN0 \leqslant f_s \leqslant \mu_s N
Kineticfkf_kSurfaces slidingfk=μkNf_k = \mu_k N

The coefficient of static friction μs\mu_s is always greater than or equal to the coefficient of kinetic friction μk\mu_k:

μsμk\mu_s \geqslant \mu_k

Static friction adjusts its magnitude to match the applied force, up to a maximum of μsN\mu_s N. Once the applied force exceeds this maximum, the object begins to slide, and kinetic friction takes over.

Inclined Planes

For an object on an inclined plane at angle θ\theta to the horizontal:

  • Component of weight parallel to the plane: mgsinθmg\sin\theta
  • Component of weight perpendicular to the plane: mgcosθmg\cos\theta
  • Normal reaction: N=mgcosθN = mg\cos\theta
  • Friction (if sliding): f=μmgcosθf = \mu mg\cos\theta

The object slides down the plane when mgsinθ>μsmgcosθmg\sin\theta \gt \mu_s mg\cos\theta, i.e.:

tanθ>μs\tan\theta \gt \mu_s

Worked Example 3

A 5kg5 \mathrm{ kg} block rests on a rough plane inclined at 3535^\circ. The block is on the verge of sliding. Find the coefficient of static friction.

Solution

At the point of sliding, mgsinθ=μsmgcosθmg\sin\theta = \mu_s mg\cos\theta:

μs=tan35=0.700\mu_s = \tan 35^\circ = 0.700

Worked Example 4

A 10kg10 \mathrm{ kg} block sits on a rough horizontal surface with μs=0.4\mu_s = 0.4 and μk=0.3\mu_k = 0.3. A force of 30N30 \mathrm{ N} is applied at 3030^\circ above the horizontal. Does the block move? If so, find its acceleration.

Solution

Resolve the applied force:

Fx=30cos30=25.98N,Fy=30sin30=15.0NF_x = 30\cos 30^\circ = 25.98 \mathrm{ N}, \quad F_y = 30\sin 30^\circ = 15.0 \mathrm{ N}

Normal reaction: N=mgFy=10×9.8115.0=98.115.0=83.1NN = mg - F_y = 10 \times 9.81 - 15.0 = 98.1 - 15.0 = 83.1 \mathrm{ N}

Maximum static friction: fs,max=μsN=0.4×83.1=33.2Nf_{s,\max} = \mu_s N = 0.4 \times 83.1 = 33.2 \mathrm{ N}

Since Fx=25.98N<33.2NF_x = 25.98 \mathrm{ N} \lt 33.2 \mathrm{ N}, the block does not move.


Momentum and Impulse

Linear Momentum

p=mv\vec{p} = m\vec{v}

Momentum is a vector quantity with SI unit kgm/s\mathrm{ kg\, m/s}.

Conservation of Momentum

For a system of objects with no external net force:

pinitial=pfinal\sum \vec{p}_{\mathrm{initial}} = \sum \vec{p}_{\mathrm{final}}

m1u1+m2u2=m1v1+m2v2m_1 \vec{u}_1 + m_2 \vec{u}_2 = m_1 \vec{v}_1 + m_2 \vec{v}_2

Impulse

J=FΔt=Δp\vec{J} = \vec{F}\,\Delta t = \Delta \vec{p}

Impulse equals the change in momentum. It is also the area under a force-time graph. The SI unit is Ns\mathrm{ N\, s}.

Collisions

TypeMomentumKinetic Energy
ElasticConservedConserved
InelasticConservedNot conserved
Perfectly inelasticConservedMaximum loss (objects stick)

Worked Example 5

A 0.2kg0.2 \mathrm{ kg} ball travelling at 15m/s15 \mathrm{ m/s} strikes a wall and rebounds at 10m/s10 \mathrm{ m/s} along the same line. Contact time is 0.02s0.02 \mathrm{ s}. Find the average force.

Solution

Taking the initial direction as positive:

Δp=m(vu)=0.2(1015)=0.2(25)=5.0kgm/s\Delta p = m(v - u) = 0.2(-10 - 15) = 0.2(-25) = -5.0 \mathrm{ kg\, m/s}

F=ΔpΔt=5.00.02=250NF = \frac{\Delta p}{\Delta t} = \frac{-5.0}{0.02} = -250 \mathrm{ N}

The magnitude of the average force is 250N250 \mathrm{ N}, directed away from the wall.

Worked Example 6

A 3kg3 \mathrm{ kg} trolley moving at 4m/s4 \mathrm{ m/s} collides with a stationary 5kg5 \mathrm{ kg} trolley and they stick together. Find the velocity after the collision and the kinetic energy lost.

Solution

By conservation of momentum:

m1u1+m2u2=(m1+m2)vm_1 u_1 + m_2 u_2 = (m_1 + m_2)v

3×4+5×0=(3+5)v    12=8v    v=1.5m/s3 \times 4 + 5 \times 0 = (3 + 5)v \implies 12 = 8v \implies v = 1.5 \mathrm{ m/s}

Initial KE: Ek,i=12(3)(42)=24.0JE_{k,i} = \frac{1}{2}(3)(4^2) = 24.0 \mathrm{ J}

Final KE: Ek,f=12(8)(1.52)=9.0JE_{k,f} = \frac{1}{2}(8)(1.5^2) = 9.0 \mathrm{ J}

Energy lost: ΔEk=24.09.0=15.0J\Delta E_k = 24.0 - 9.0 = 15.0 \mathrm{ J}

Worked Example 7

A 0.05kg0.05 \mathrm{ kg} bullet travelling at 400m/s400 \mathrm{ m/s} embeds itself in a 2kg2 \mathrm{ kg} wooden block at rest on a smooth surface. Find the velocity of the block immediately after impact.

Solution

By conservation of momentum (perfectly inelastic collision):

m1u1+m2u2=(m1+m2)vm_1 u_1 + m_2 u_2 = (m_1 + m_2)v

0.05×400+2×0=(0.05+2)v0.05 \times 400 + 2 \times 0 = (0.05 + 2)v

20=2.05v    v=9.76m/s20 = 2.05v \implies v = 9.76 \mathrm{ m/s}


Projectile Motion

Analysis by Components

For a projectile launched with speed uu at angle θ\theta above the horizontal:

QuantityHorizontalVertical
Acceleration00g-g
Velocityux=ucosθu_x = u\cos\theta (constant)uy=usinθgtu_y = u\sin\theta - gt
Displacementx=ucosθtx = u\cos\theta\cdot ty=usinθt12gt2y = u\sin\theta\cdot t - \frac{1}{2}gt^2

Key Results

Time of flight (landing at same height):

T=2usinθgT = \frac{2u\sin\theta}{g}

Maximum height:

H=u2sin2θ2gH = \frac{u^2\sin^2\theta}{2g}

Horizontal range:

R=u2sin2θgR = \frac{u^2\sin 2\theta}{g}

Maximum range occurs at θ=45\theta = 45^\circ, giving Rmax=u2/gR_{\max} = u^2/g.

Complementary angles (θ\theta and 90θ90^\circ - \theta) produce the same range.

Projectile Motion

Explore how launch angle and initial speed affect the trajectory.

Worked Example 7

A ball is thrown from ground level with speed 20m/s20 \mathrm{ m/s} at 5050^\circ above the horizontal. Find the range and maximum height.

Solution

R=202sin1009.81=400×0.98489.81=40.2mR = \frac{20^2 \sin 100^\circ}{9.81} = \frac{400 \times 0.9848}{9.81} = 40.2 \mathrm{ m}

H=202sin2502×9.81=400×0.586819.62=11.97mH = \frac{20^2 \sin^2 50^\circ}{2 \times 9.81} = \frac{400 \times 0.5868}{19.62} = 11.97 \mathrm{ m}


Circular Motion

Angular Quantities

QuantitySymbolSI UnitRelation
Angular displacementθ\thetaradθ=s/r\theta = s/r
Angular velocityω\omegarad/sω=dθ/dt\omega = d\theta/dt
PeriodTTsT=2π/ωT = 2\pi/\omega
FrequencyffHzf=1/T=ω/(2π)f = 1/T = \omega/(2\pi)

Linear-angular relation: v=rωv = r\omega, a=rαa = r\alpha

Centripetal Acceleration and Force

An object moving at constant speed vv in a circle of radius rr has centripetal acceleration:

ac=v2r=ω2r=4π2rT2a_c = \frac{v^2}{r} = \omega^2 r = \frac{4\pi^2 r}{T^2}

directed towards the centre of the circle. The required centripetal force is:

Fc=mv2r=mω2rF_c = \frac{mv^2}{r} = m\omega^2 r

Vertical Circular Motion

For an object on a string in vertical circular motion, speed varies because gravity does work. At the top of the circle:

T+mg=mvtop2rT + mg = \frac{mv_{\mathrm{top}}^2}{r}

At the bottom:

Tmg=mvbottom2rT - mg = \frac{mv_{\mathrm{bottom}}^2}{r}

For the object to complete the full circle, the string must remain taut at the top (T0T \geqslant 0):

vtopgrv_{\mathrm{top}} \geqslant \sqrt{gr}

Worked Example 8

A car of mass 1200kg1200 \mathrm{ kg} travels around a flat curve of radius 60m60 \mathrm{ m} at 15m/s15 \mathrm{ m/s}. Find the minimum coefficient of friction required.

Solution

Fc=mv2r=1200×15260=1200×22560=4500NF_c = \frac{mv^2}{r} = \frac{1200 \times 15^2}{60} = \frac{1200 \times 225}{60} = 4500 \mathrm{ N}

The centripetal force is provided by friction: Fc=μsmgF_c = \mu_s mg

μs=Fcmg=45001200×9.81=450011772=0.382\mu_s = \frac{F_c}{mg} = \frac{4500}{1200 \times 9.81} = \frac{4500}{11772} = 0.382

Worked Example 9

A 0.5kg0.5 \mathrm{ kg} ball is attached to a string of length 0.8m0.8 \mathrm{ m} and whirled in a vertical circle. Find the minimum speed at the lowest point for the ball to complete the full circle.

Solution

For the ball to complete the full circle, the speed at the top must satisfy vtopgrv_{\mathrm{top}} \geqslant \sqrt{gr}.

Using energy conservation between the bottom and top:

12mvbottom2=12mvtop2+mg(2r)\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

Setting vtop=grv_{\mathrm{top}} = \sqrt{gr}:

12mvbottom2=12m(gr)+2mgr=52mgr\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}m(gr) + 2mgr = \frac{5}{2}mgr

vbottom=5gr=5×9.81×0.8=39.24=6.26m/sv_{\mathrm{bottom}} = \sqrt{5gr} = \sqrt{5 \times 9.81 \times 0.8} = \sqrt{39.24} = 6.26 \mathrm{ m/s}


Gravitation

Newton's Law of Universal Gravitation

F=Gm1m2r2F = \frac{Gm_1 m_2}{r^2}

where G=6.67×1011Nm2kg2G = 6.67 \times 10^{-11} \mathrm{ N\, m}^2\,\mathrm{ kg}^{-2}.

Gravitational Field Strength

g=Fm=GMr2g = \frac{F}{m} = \frac{GM}{r^2}

Near the Earth's surface, g9.81N/kgg \approx 9.81 \mathrm{ N/kg} (equivalent to m/s2\mathrm{ m/s}^2).

Gravitational Potential Energy

For two masses separated by distance rr:

Ep=GMmrE_p = -\frac{GMm}{r}

The negative sign reflects the convention that Ep=0E_p = 0 at infinite separation. Work must be done against gravity to increase the separation.

Orbital Motion

For a satellite of mass mm orbiting a central body of mass MM at radius rr:

GMmr2=mv2r    v=GMr\frac{GMm}{r^2} = \frac{mv^2}{r} \implies v = \sqrt{\frac{GM}{r}}

T=2πrv=2πr3GMT = \frac{2\pi r}{v} = 2\pi\sqrt{\frac{r^3}{GM}}

This is Kepler's third law: T2r3T^2 \propto r^3.

Gravity and Orbits

Visualise how orbital speed and period depend on the distance from the central body.

Worked Example 10

Find the orbital speed of a satellite orbiting the Earth at a height of 400km400 \mathrm{ km}. (Earth radius RE=6.37×106mR_E = 6.37 \times 10^6 \mathrm{ m}, Earth mass ME=5.97×1024kgM_E = 5.97 \times 10^{24} \mathrm{ kg})

Solution

r=RE+400×103=6.77×106mr = R_E + 400 \times 10^3 = 6.77 \times 10^6 \mathrm{ m}

v=GMEr=6.67×1011×5.97×10246.77×106=5.88×107=7668m/sv = \sqrt{\frac{GM_E}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.77 \times 10^6}} = \sqrt{5.88 \times 10^7} = 7668 \mathrm{ m/s}


Common Pitfalls

  • Confusing action-reaction pairs with balanced forces. Newton's third law pairs act on different objects; balanced forces act on the same object.
  • Forgetting that friction opposes relative motion, not necessarily the direction of the applied force.
  • Using μsN\mu_s N for kinetic friction or μkN\mu_k N for static friction. They are different.
  • In projectile motion, treating horizontal and vertical components as coupled. They share only the common variable tt.
  • Adding centripetal force as an extra force on a free body diagram. Centripetal force is the name given to the net inward force, not an additional force.

Summary Table

TopicKey FormulaKey Concept
Newton's Second LawF=maF = maNet force causes acceleration
Static frictionfsμsNf_s \leqslant \mu_s NAdjusts to match applied force
Kinetic frictionfk=μkNf_k = \mu_k NConstant during sliding
Momentump=mvp = mvVector quantity
ImpulseJ=FΔt=ΔpJ = F\Delta t = \Delta pArea under F-t graph
Projectile rangeR=u2sin2θ/gR = u^2\sin 2\theta/gMaximum at 4545^\circ
Centripetal forceFc=mv2/rF_c = mv^2/rNet force towards centre
GravitationF=Gm1m2/r2F = Gm_1 m_2/r^2Inverse square law
Orbital speedv=GM/rv = \sqrt{GM/r}Balances gravity

Problem Set

Problem 1. A 6kg6 \mathrm{ kg} block on a smooth horizontal table is connected by a light inextensible string over a smooth pulley to a 4kg4 \mathrm{ kg} block hanging freely. Find the acceleration of the system and the tension in the string.

Solution

For the 4kg4 \mathrm{ kg} block (taking downward as positive): 4gT=4a4g - T = 4a

For the 6kg6 \mathrm{ kg} block: T=6aT = 6a

Adding: 4g=10a    a=4×9.8110=3.92m/s24g = 10a \implies a = \frac{4 \times 9.81}{10} = 3.92 \mathrm{ m/s}^2

T=6×3.92=23.5NT = 6 \times 3.92 = 23.5 \mathrm{ N}

If you get this wrong, revise: Newton's Laws of Motion / Second Law

Problem 2. A 3kg3 \mathrm{ kg} block is placed on a rough inclined plane at 3030^\circ. The coefficient of static friction is 0.350.35. Does the block slide? If it does, find the acceleration (μk=0.25\mu_k = 0.25).

Solution

Check: tan30=0.577>μs=0.35\tan 30^\circ = 0.577 \gt \mu_s = 0.35, so the block slides.

a=g(sinθμkcosθ)=9.81(0.50.25×0.866)=9.81(0.50.217)=9.81×0.283=2.78m/s2a = g(\sin\theta - \mu_k\cos\theta) = 9.81(0.5 - 0.25 \times 0.866) = 9.81(0.5 - 0.217) = 9.81 \times 0.283 = 2.78 \mathrm{ m/s}^2

If you get this wrong, revise: Friction / Inclined Planes

Problem 3. A 2kg2 \mathrm{ kg} object moving at 6m/s6 \mathrm{ m/s} collides elastically with a 4kg4 \mathrm{ kg} object at rest. Find the velocities after collision.

Solution

Conservation of momentum: 2(6)+4(0)=2v1+4v2    12=2v1+4v2(1)2(6) + 4(0) = 2v_1 + 4v_2 \implies 12 = 2v_1 + 4v_2 \quad (1)

Conservation of KE: 12(2)(36)=12(2)v12+12(4)v22    36=v12+2v22(2)\frac{1}{2}(2)(36) = \frac{1}{2}(2)v_1^2 + \frac{1}{2}(4)v_2^2 \implies 36 = v_1^2 + 2v_2^2 \quad (2)

From (1): v1=62v2v_1 = 6 - 2v_2. Substituting into (2):

36=(62v2)2+2v22=3624v2+4v22+2v22=3624v2+6v2236 = (6 - 2v_2)^2 + 2v_2^2 = 36 - 24v_2 + 4v_2^2 + 2v_2^2 = 36 - 24v_2 + 6v_2^2

6v2224v2=0    6v2(v24)=06v_2^2 - 24v_2 = 0 \implies 6v_2(v_2 - 4) = 0

v2=0v_2 = 0 (original) or v2=4m/sv_2 = 4 \mathrm{ m/s}. Therefore v1=68=2m/sv_1 = 6 - 8 = -2 \mathrm{ m/s}.

The 2kg2 \mathrm{ kg} object rebounds at 2m/s2 \mathrm{ m/s}; the 4kg4 \mathrm{ kg} object moves forward at 4m/s4 \mathrm{ m/s}.

If you get this wrong, revise: Momentum and Impulse / Collisions

Problem 4. A 150g150 \mathrm{ g} cricket ball is hit by a bat. The force-time graph is a triangle with peak force 600N600 \mathrm{ N} and contact time 0.005s0.005 \mathrm{ s}. Find the impulse and the speed of the ball after impact (initially at rest).

Solution

Impulse = area under F-t graph =12×600×0.005=1.5Ns= \frac{1}{2} \times 600 \times 0.005 = 1.5 \mathrm{ N\, s}

J=Δp=mv    v=Jm=1.50.150=10.0m/sJ = \Delta p = mv \implies v = \frac{J}{m} = \frac{1.5}{0.150} = 10.0 \mathrm{ m/s}

If you get this wrong, revise: Momentum and Impulse / Impulse

Problem 5. A projectile is launched at 25m/s25 \mathrm{ m/s} from the edge of a cliff 80m80 \mathrm{ m} high at 4040^\circ above the horizontal. Find the horizontal distance from the cliff edge where it lands.

Solution

Vertical: y=uyt+12at2y = u_y t + \frac{1}{2}at^2, where uy=25sin40=16.07m/su_y = 25\sin 40^\circ = 16.07 \mathrm{ m/s}

80=16.07t4.905t2    4.905t216.07t80=0-80 = 16.07t - 4.905t^2 \implies 4.905t^2 - 16.07t - 80 = 0

t=16.07±258.2+1569.69.81=16.07±1827.89.81=16.07+42.769.81=5.99st = \frac{16.07 \pm \sqrt{258.2 + 1569.6}}{9.81} = \frac{16.07 \pm \sqrt{1827.8}}{9.81} = \frac{16.07 + 42.76}{9.81} = 5.99 \mathrm{ s}

Horizontal distance: d=uxt=25cos40×5.99=19.15×5.99=114.7md = u_x t = 25\cos 40^\circ \times 5.99 = 19.15 \times 5.99 = 114.7 \mathrm{ m}

If you get this wrong, revise: Projectile Motion / Analysis by Components

Problem 6. A stone is tied to a string of length 1.2m1.2 \mathrm{ m} and whirled in a horizontal circle. The string breaks when the tension reaches 50N50 \mathrm{ N}. The stone has mass 0.4kg0.4 \mathrm{ kg}. Find the maximum speed before the string breaks.

Solution

The tension provides the centripetal force: T=mv2rT = \frac{mv^2}{r}

v=Trm=50×1.20.4=150=12.2m/sv = \sqrt{\frac{Tr}{m}} = \sqrt{\frac{50 \times 1.2}{0.4}} = \sqrt{150} = 12.2 \mathrm{ m/s}

If you get this wrong, revise: Circular Motion / Centripetal Acceleration and Force

Problem 7. A satellite orbits the Earth at a height of 600km600 \mathrm{ km}. Find the orbital period and the gravitational field strength at that altitude.

Solution

r=6.37×106+600×103=6.97×106mr = 6.37 \times 10^6 + 600 \times 10^3 = 6.97 \times 10^6 \mathrm{ m}

g=GMEr2=6.67×1011×5.97×1024(6.97×106)2=3.98×10144.86×1013=8.19N/kgg = \frac{GM_E}{r^2} = \frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{(6.97 \times 10^6)^2} = \frac{3.98 \times 10^{14}}{4.86 \times 10^{13}} = 8.19 \mathrm{ N/kg}

T=2πr3GME=2π(6.97×106)36.67×1011×5.97×1024=2π3.385×10203.982×1014=2π850300=2π×922.1=5794s=96.6minutesT = 2\pi\sqrt{\frac{r^3}{GM_E}} = 2\pi\sqrt{\frac{(6.97 \times 10^6)^3}{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}} = 2\pi\sqrt{\frac{3.385 \times 10^{20}}{3.982 \times 10^{14}}} = 2\pi\sqrt{850300} = 2\pi \times 922.1 = 5794 \mathrm{ s} = 96.6 \mathrm{ minutes}

If you get this wrong, revise: Gravitation / Orbital Motion

Problem 8. A 4kg4 \mathrm{ kg} block slides down a rough incline of length 6m6 \mathrm{ m} at 3030^\circ to the horizontal. The coefficient of kinetic friction is 0.250.25. Find the speed at the bottom if the block starts from rest.

Solution

Net force down the plane: F=mgsin30μkmgcos30F = mg\sin 30^\circ - \mu_k mg\cos 30^\circ

F=4×9.81×0.50.25×4×9.81×0.866=19.628.50=11.12NF = 4 \times 9.81 \times 0.5 - 0.25 \times 4 \times 9.81 \times 0.866 = 19.62 - 8.50 = 11.12 \mathrm{ N}

a=Fm=11.124=2.78m/s2a = \frac{F}{m} = \frac{11.12}{4} = 2.78 \mathrm{ m/s}^2

v=2as=2×2.78×6=33.36=5.78m/sv = \sqrt{2as} = \sqrt{2 \times 2.78 \times 6} = \sqrt{33.36} = 5.78 \mathrm{ m/s}

If you get this wrong, revise: Friction / Inclined Planes and Newton's Second Law

Problem 9. A 1.5kg1.5 \mathrm{ kg} ball on a string of length 0.5m0.5 \mathrm{ m} is swung in a vertical circle. At the lowest point, the tension is 45N45 \mathrm{ N}. Find the speed at the lowest point and the speed at the highest point.

Solution

At the lowest point: Tmg=mv2rT - mg = \frac{mv^2}{r}

451.5×9.81=1.5vbottom20.5    4514.7=3vbottom245 - 1.5 \times 9.81 = \frac{1.5 v_{\mathrm{bottom}}^2}{0.5} \implies 45 - 14.7 = 3 v_{\mathrm{bottom}}^2

vbottom2=30.33=10.1    vbottom=3.18m/sv_{\mathrm{bottom}}^2 = \frac{30.3}{3} = 10.1 \implies v_{\mathrm{bottom}} = 3.18 \mathrm{ m/s}

Energy conservation between bottom and top:

12mvbottom2=12mvtop2+mg(2r)\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

10.1=vtop2+2×9.81×1.0=vtop2+19.6210.1 = v_{\mathrm{top}}^2 + 2 \times 9.81 \times 1.0 = v_{\mathrm{top}}^2 + 19.62

vtop2=9.52v_{\mathrm{top}}^2 = -9.52

The result is negative, meaning the ball does not reach the top of the circle. The speed is insufficient.

If you get this wrong, revise: Circular Motion / Vertical Circular Motion

Problem 10. Two astronauts of masses 80kg80 \mathrm{ kg} and 60kg60 \mathrm{ kg} are initially at rest in deep space, connected by a light rope. They push off each other and the 80kg80 \mathrm{ kg} astronaut moves away at 0.5m/s0.5 \mathrm{ m/s}. Find the velocity of the 60kg60 \mathrm{ kg} astronaut and the distance between them after 5 seconds.

Solution

By conservation of momentum (initially at rest, total momentum = 0):

80×0.5+60×v2=0    v2=4060=0.667m/s80 \times 0.5 + 60 \times v_2 = 0 \implies v_2 = -\frac{40}{60} = -0.667 \mathrm{ m/s}

The 60kg60 \mathrm{ kg} astronaut moves at 0.667m/s0.667 \mathrm{ m/s} in the opposite direction.

Relative speed =0.5+0.667=1.167m/s= 0.5 + 0.667 = 1.167 \mathrm{ m/s}

Distance after 5 s=1.167×5=5.83m\mathrm{Distance\ after\ 5\ s} = 1.167 \times 5 = 5.83 \mathrm{ m}

If you get this wrong, revise: Momentum and Impulse / Conservation of Momentum

For the A-Level treatment of this topic, see Dynamics.


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Derivations

Derivation: Centripetal Acceleration

Consider an object moving at constant speed vv in a circle of radius rr. In a small time Δt\Delta t, it moves from point A to point B, subtending a small angle Δθ\Delta\theta at the centre.

The change in velocity is directed towards the centre (radially inward). For small angles:

ΔvvΔθ=vvΔtr=v2Δtr\Delta v \approx v \cdot \Delta\theta = v \cdot \frac{v\Delta t}{r} = \frac{v^2 \Delta t}{r}

The centripetal acceleration is:

ac=ΔvΔt=v2ra_c = \frac{\Delta v}{\Delta t} = \frac{v^2}{r}

In terms of angular velocity (v=rωv = r\omega):

ac=(rω)2r=rω2=4π2rT2a_c = \frac{(r\omega)^2}{r} = r\omega^2 = \frac{4\pi^2 r}{T^2}

This acceleration is always directed towards the centre of the circle and is perpendicular to the velocity (which is tangential). Since the force is perpendicular to the velocity, the magnetic force does no work and the speed remains constant.

Derivation: Escape Velocity

For an object to escape from the surface of a planet of mass MM and radius RR, its total energy (kinetic + gravitational potential) at infinity must be at least zero.

At the surface: Etotal=12mve2GMmRE_{\mathrm{total}} = \frac{1}{2}mv_e^2 - \frac{GMm}{R}

At infinity: Etotal=0E_{\mathrm{total}} = 0 (just barely escaping)

12mve2=GMmR\frac{1}{2}mv_e^2 = \frac{GMm}{R}

ve=2GMRv_e = \sqrt{\frac{2GM}{R}}

Derivation: Orbital Speed and Period

For a satellite in circular orbit at radius rr around a central body of mass MM, the gravitational force provides the centripetal force:

GMmr2=mv2r\frac{GMm}{r^2} = \frac{mv^2}{r}

v=GMrv = \sqrt{\frac{GM}{r}}

The orbital period is:

T=2πrv=2πrGM/r=2πr3GMT = \frac{2\pi r}{v} = \frac{2\pi r}{\sqrt{GM/r}} = 2\pi\sqrt{\frac{r^3}{GM}}

Squaring both sides: T2=4π2GMr3T^2 = \frac{4\pi^2}{GM}r^3, which is Kepler's third law (T2r3T^2 \propto r^3).

Derivation: Range of a Projectile

For a projectile launched from ground level with speed uu at angle θ\theta:

Horizontal: x=ucosθtx = u\cos\theta \cdot t

Vertical at landing (y=0y = 0): 0=usinθt12gt2    t=2usinθg0 = u\sin\theta \cdot t - \frac{1}{2}gt^2 \implies t = \frac{2u\sin\theta}{g}

Substituting: R=ucosθ2usinθg=u22sinθcosθg=u2sin2θgR = u\cos\theta \cdot \frac{2u\sin\theta}{g} = \frac{u^2 \cdot 2\sin\theta\cos\theta}{g} = \frac{u^2\sin 2\theta}{g}

Maximum range when sin2θ=1\sin 2\theta = 1, i.e., θ=45\theta = 45^\circ: Rmax=u2/gR_{\max} = u^2/g.


Experimental Methods

Determining Acceleration Due to Gravity Using a Free-Fall Apparatus

Apparatus: An electromagnetic release mechanism, a metal ball, a trapdoor, an electronic timer, and a metre rule.

Procedure:

  1. Measure the height hh from the bottom of the ball to the trapdoor.
  2. Release the ball electromagnetically; the timer starts.
  3. The ball hits the trapdoor, stopping the timer. Record the time tt.
  4. Repeat for several heights.
  5. Plot hh (y-axis) versus t2t^2 (x-axis).
  6. From h=12gt2h = \frac{1}{2}gt^2: gradient =g/2= g/2, so g=2×gradientg = 2 \times \mathrm{gradient}.

Sources of error:

  • Reaction time of the timer mechanism (minimised by using electronic timing).
  • Air resistance on the ball (use a dense, small ball to minimise).
  • Measurement of height hh (measure from the bottom of the ball, not the centre).

Improvements: Repeat each measurement multiple times and average. Use a heavier ball to reduce air resistance effects.

Verifying Newton's Second Law Using a Trolley on a Ramp

Apparatus: A trolley on a horizontal track, light gates, a set of slotted masses, a string over a pulley, and a data logger.

Procedure:

  1. Attach a string to the trolley, passing over a pulley at the edge of the track, with a hanging mass mm providing the accelerating force.
  2. Measure the acceleration aa of the trolley using the light gates for different values of the total mass (m+Mm + M, where MM is the trolley mass) while keeping the accelerating force mgmg constant.
  3. Plot aa (y-axis) versus 1/(m+M)1/(m + M) (x-axis). A straight line through the origin confirms a1/(total mass)a \propto 1/(\mathrm{total\ mass}).
  4. Alternatively, keep the total mass constant and vary the hanging mass. Plot aa versus F=mgF = mg. A straight line through the origin confirms aFa \propto F.

Precautions:

  • Compensate for friction by tilting the track slightly so the trolley moves at constant speed with no hanging mass.
  • Ensure the string is parallel to the track.
  • Use a light string and low-friction pulley.

Measuring the Coefficient of Friction on an Inclined Plane

Apparatus: An inclined plane, a block, a protractor, and a set of masses.

Procedure:

  1. Place the block on the inclined plane and gradually increase the angle.
  2. Record the angle θc\theta_c at which the block just begins to slide.
  3. At this critical angle: tanθc=μs\tan\theta_c = \mu_s.
  4. Repeat several times and average.
  5. For the coefficient of kinetic friction, measure the acceleration aa of the block sliding down the plane: a=g(sinθμkcosθ)a = g(\sin\theta - \mu_k\cos\theta), so μk=tanθa/(gcosθ)\mu_k = \tan\theta - a/(g\cos\theta).

Data Analysis and Uncertainty

Uncertainty in Acceleration Calculations

When determining gg from h=12gt2h = \frac{1}{2}gt^2:

g=2ht2g = \frac{2h}{t^2}

Δgg=(Δhh)2+(2Δtt)2\frac{\Delta g}{g} = \sqrt{\left(\frac{\Delta h}{h}\right)^2 + \left(2\frac{\Delta t}{t}\right)^2}

The time measurement typically dominates the uncertainty due to the factor of 2.

Example: h=(1.00±0.01)mh = (1.00 \pm 0.01) \mathrm{ m}, t=(0.450±0.005)st = (0.450 \pm 0.005) \mathrm{ s}:

g=2×1.00(0.450)2=2.000.2025=9.88m/s2g = \frac{2 \times 1.00}{(0.450)^2} = \frac{2.00}{0.2025} = 9.88 \mathrm{ m/s}^2

Δgg=(0.01)2+(2×0.0111)2=0.0001+0.000493=0.000593=0.0244=2.4%\frac{\Delta g}{g} = \sqrt{(0.01)^2 + (2 \times 0.0111)^2} = \sqrt{0.0001 + 0.000493} = \sqrt{0.000593} = 0.0244 = 2.4\%

Δg=0.024×9.88=0.24m/s2\Delta g = 0.024 \times 9.88 = 0.24 \mathrm{ m/s}^2

g=(9.9±0.2)m/s2g = (9.9 \pm 0.2) \mathrm{ m/s}^2

Linearising Projectile Motion Data

To verify R=u2sin2θ/gR = u^2\sin 2\theta / g at constant launch speed:

  • Plot RR (y-axis) versus sin2θ\sin 2\theta (x-axis).
  • A straight line through the origin confirms the relationship.
  • The gradient equals u2/gu^2/g.

Additional Worked Examples

Worked Example 11

A 3.0kg3.0 \mathrm{ kg} block is pushed against a spring of spring constant 300N/m300 \mathrm{ N/m}, compressing it by 0.10m0.10 \mathrm{ m}. The block is released and moves across a rough horizontal surface with μk=0.2\mu_k = 0.2. How far does the block travel before coming to rest?

Solution

Energy stored in spring: Ep=12(300)(0.10)2=1.5JE_p = \frac{1}{2}(300)(0.10)^2 = 1.5 \mathrm{ J}

This energy is dissipated by friction: Ep=fk×d=μkmg×dE_p = f_k \times d = \mu_k mg \times d

1.5=0.2×3.0×9.81×d=5.886d1.5 = 0.2 \times 3.0 \times 9.81 \times d = 5.886d

d=1.55.886=0.255md = \frac{1.5}{5.886} = 0.255 \mathrm{ m}

Worked Example 12

A ball is thrown from the top of a building 45m45 \mathrm{ m} high with initial velocity 20m/s20 \mathrm{ m/s} at 3030^\circ above the horizontal. Find: (a) the time taken to reach the ground, (b) the horizontal distance from the base of the building where it lands, (c) the speed and direction of the ball just before impact.

Solution

ux=20cos30=17.32m/su_x = 20\cos 30^\circ = 17.32 \mathrm{ m/s}, uy=20sin30=10.0m/su_y = 20\sin 30^\circ = 10.0 \mathrm{ m/s}

(a) Vertical motion (taking upward as positive, h=45mh = -45 \mathrm{ m}):

45=10.0t12(9.81)t2    4.905t210.0t45=0-45 = 10.0t - \frac{1}{2}(9.81)t^2 \implies 4.905t^2 - 10.0t - 45 = 0

t=10.0±100+882.99.81=10.0±982.99.81=10.0+31.359.81=4.21st = \frac{10.0 \pm \sqrt{100 + 882.9}}{9.81} = \frac{10.0 \pm \sqrt{982.9}}{9.81} = \frac{10.0 + 31.35}{9.81} = 4.21 \mathrm{ s}

(b) Horizontal distance: d=uxt=17.32×4.21=72.9md = u_x t = 17.32 \times 4.21 = 72.9 \mathrm{ m}

(c) Vertical velocity at impact: vy=uygt=10.09.81×4.21=10.041.3=31.3m/sv_y = u_y - gt = 10.0 - 9.81 \times 4.21 = 10.0 - 41.3 = -31.3 \mathrm{ m/s}

Horizontal velocity at impact: vx=17.32m/sv_x = 17.32 \mathrm{ m/s} (constant)

v=vx2+vy2=17.322+31.32=300+980=1280=35.8m/sv = \sqrt{v_x^2 + v_y^2} = \sqrt{17.32^2 + 31.3^2} = \sqrt{300 + 980} = \sqrt{1280} = 35.8 \mathrm{ m/s}

Angle below horizontal: α=tan1(31.317.32)=tan1(1.807)=61.0\alpha = \tan^{-1}\left(\frac{31.3}{17.32}\right) = \tan^{-1}(1.807) = 61.0^\circ below horizontal

Worked Example 13

A satellite of mass 500kg500 \mathrm{ kg} is in a circular orbit 300km300 \mathrm{ km} above the Earth's surface. Calculate: (a) the orbital speed, (b) the orbital period, (c) the gravitational potential energy, (d) the kinetic energy, (e) the total energy.

(Earth mass =5.97×1024kg= 5.97 \times 10^{24} \mathrm{ kg}, Earth radius =6.37×106m= 6.37 \times 10^6 \mathrm{ m})

Solution

r=6.37×106+300×103=6.67×106mr = 6.37 \times 10^6 + 300 \times 10^3 = 6.67 \times 10^6 \mathrm{ m}

(a) v=GMr=6.67×1011×5.97×10246.67×106=5.97×107=7727m/sv = \sqrt{\frac{GM}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.67 \times 10^6}} = \sqrt{5.97 \times 10^7} = 7727 \mathrm{ m/s}

(b) T=2πrv=2π×6.67×1067727=4.19×1077727=5421s=90.4minutesT = \frac{2\pi r}{v} = \frac{2\pi \times 6.67 \times 10^6}{7727} = \frac{4.19 \times 10^7}{7727} = 5421 \mathrm{ s} = 90.4 \mathrm{ minutes}

(c) Ep=GMmr=6.67×1011×5.97×1024×5006.67×106=1.99×10176.67×106=2.98×1010JE_p = -\frac{GMm}{r} = -\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 500}{6.67 \times 10^6} = -\frac{1.99 \times 10^{17}}{6.67 \times 10^6} = -2.98 \times 10^{10} \mathrm{ J}

(d) Ek=12mv2=12(500)(7727)2=250×5.97×107=1.49×1010JE_k = \frac{1}{2}mv^2 = \frac{1}{2}(500)(7727)^2 = 250 \times 5.97 \times 10^7 = 1.49 \times 10^{10} \mathrm{ J}

(e) Etotal=Ek+Ep=1.49×1010+(2.98×1010)=1.49×1010JE_{\mathrm{total}} = E_k + E_p = 1.49 \times 10^{10} + (-2.98 \times 10^{10}) = -1.49 \times 10^{10} \mathrm{ J}

Note: For a circular orbit, Etotal=Ek=12EpE_{\mathrm{total}} = -E_k = \frac{1}{2}E_p.


Exam-Style Questions

Question 1 (DSE Structured)

A student investigates the motion of a trolley down an inclined plane. The plane is inclined at 2020^\circ to the horizontal. The trolley is released from rest and its acceleration is measured using light gates at different distances from the starting point.

Distance from start (m)Speed (m/s)
0.201.10
0.401.58
0.601.95
0.802.25
1.002.52

(a) Plot a graph of v2v^2 (y-axis) against distance ss (x-axis). Determine the acceleration from the gradient.

(b) Calculate the theoretical acceleration for a frictionless incline and compare it with the experimental value. Hence determine the coefficient of kinetic friction.

(c) Explain why the student plots v2v^2 against ss rather than vv against ss.

(d) Suggest two improvements to this experiment to reduce random errors.

Solution

(a)

ss (m)v2v^2 (m2^2/s2^2)
0.201.102=1.211.10^2 = 1.21
0.401.582=2.501.58^2 = 2.50
0.601.952=3.801.95^2 = 3.80
0.802.252=5.062.25^2 = 5.06
1.002.522=6.352.52^2 = 6.35

From v2=u2+2asv^2 = u^2 + 2as with u=0u = 0: v2=2asv^2 = 2as.

Gradient =Δv2/Δs(6.351.21)/(1.000.20)=5.14/0.80=6.42m/s2= \Delta v^2 / \Delta s \approx (6.35 - 1.21)/(1.00 - 0.20) = 5.14/0.80 = 6.42 \mathrm{ m/s}^2

Since gradient =2a= 2a: a=6.42/2=3.21m/s2a = 6.42/2 = 3.21 \mathrm{ m/s}^2

(b) Theoretical (frictionless): a=gsin20=9.81×0.342=3.36m/s2a = g\sin 20^\circ = 9.81 \times 0.342 = 3.36 \mathrm{ m/s}^2

Experimental: a=3.21m/s2a = 3.21 \mathrm{ m/s}^2

The difference is due to friction: aexp=gsinθμkgcosθa_{\mathrm{exp}} = g\sin\theta - \mu_k g\cos\theta

3.21=3.36μk×9.81×cos20=3.369.22μk3.21 = 3.36 - \mu_k \times 9.81 \times \cos 20^\circ = 3.36 - 9.22\mu_k

μk=3.363.219.22=0.159.22=0.016\mu_k = \frac{3.36 - 3.21}{9.22} = \frac{0.15}{9.22} = 0.016

(c) From the kinematic equation v2=u2+2asv^2 = u^2 + 2as, plotting v2v^2 against ss (with u=0u = 0) gives a straight line through the origin with gradient 2a2a. A plot of vv against ss would be a curve (v=2asv = \sqrt{2as}), which is harder to analyse.

(d) Two improvements:

  1. Repeat each measurement several times and use the average to reduce random errors.
  2. Use a data logger with higher time resolution (smaller uncertainty in timing).

Question 2 (DSE Structured)

Two objects, A (2.0kg2.0 \mathrm{ kg}) and B (3.0kg3.0 \mathrm{ kg}), are connected by a light inextensible string over a smooth pulley. Object A rests on a rough horizontal table (μk=0.3\mu_k = 0.3) and object B hangs freely.

(a) Draw free body diagrams for both objects.

(b) Calculate the acceleration of the system and the tension in the string.

(c) Object B starts from rest. Find the speed of the system after B has fallen 0.80m0.80 \mathrm{ m}.

(d) If the string is cut just as B reaches the floor (having fallen 0.80m0.80 \mathrm{ m}), how far does A slide before stopping?

Solution

(a) Object A: Weight 2g2g down, normal reaction NN up, tension TT right, friction ff left. Object B: Weight 3g3g down, tension TT up.

(b) For B (taking down as positive): 3gT=3a(1)3g - T = 3a \quad (1)

For A (taking right as positive): Tf=2aT - f = 2a, where f=μkN=μk×2g=0.3×2g=0.6gf = \mu_k N = \mu_k \times 2g = 0.3 \times 2g = 0.6g

T0.6g=2a(2)T - 0.6g = 2a \quad (2)

Adding (1) and (2): 3g0.6g=5a    2.4g=5a3g - 0.6g = 5a \implies 2.4g = 5a

a=2.4×9.815=23.545=4.71m/s2a = \frac{2.4 \times 9.81}{5} = \frac{23.54}{5} = 4.71 \mathrm{ m/s}^2

From (2): T=2a+0.6g=2(4.71)+0.6(9.81)=9.42+5.89=15.3NT = 2a + 0.6g = 2(4.71) + 0.6(9.81) = 9.42 + 5.89 = 15.3 \mathrm{ N}

(c) v2=u2+2as=0+2(4.71)(0.80)=7.54v^2 = u^2 + 2as = 0 + 2(4.71)(0.80) = 7.54

v=7.54=2.75m/sv = \sqrt{7.54} = 2.75 \mathrm{ m/s}

(d) After the string is cut, A slides with initial speed 2.75m/s2.75 \mathrm{ m/s} and decelerates due to friction only:

a=fm=μkmgm=μkg=0.3×9.81=2.94m/s2a = -\frac{f}{m} = -\frac{\mu_k mg}{m} = -\mu_k g = -0.3 \times 9.81 = -2.94 \mathrm{ m/s}^2

v2=u2+2as    0=(2.75)2+2(2.94)sv^2 = u^2 + 2as \implies 0 = (2.75)^2 + 2(-2.94)s

s=7.565.89=1.28ms = \frac{7.56}{5.89} = 1.28 \mathrm{ m}

A slides 1.28m1.28 \mathrm{ m} before stopping.

Question 3 (DSE Structured)

(a) State the conditions for an object to be in equilibrium.

(b) A uniform beam of weight 80N80 \mathrm{ N} and length 4.0m4.0 \mathrm{ m} is hinged at one end (point P) and supported by a cable attached to the other end (point Q). The cable makes an angle of 3030^\circ with the beam. A 150N150 \mathrm{ N} weight hangs from a point 1.5m1.5 \mathrm{ m} from P.

(i) Calculate the tension in the cable. (ii) Calculate the magnitude and direction of the force exerted by the hinge on the beam.

Solution

(a) For an object to be in equilibrium:

  1. The net force on the object must be zero (F=0\sum \vec{F} = 0).
  2. The net moment (torque) about any point must be zero (τ=0\sum \tau = 0).

(b) (i) Take moments about P (eliminates the hinge force):

Clockwise moments = 80×2.0+150×1.5=160+225=385Nm80 \times 2.0 + 150 \times 1.5 = 160 + 225 = 385 \mathrm{ N\, m}

(Weight of beam acts at centre, 2.0m2.0 \mathrm{ m} from P.)

Anticlockwise moment = Tsin30×4.0=T×0.5×4.0=2.0TT\sin 30^\circ \times 4.0 = T \times 0.5 \times 4.0 = 2.0T

2.0T=385    T=192.5N2.0T = 385 \implies T = 192.5 \mathrm{ N}

(ii) Resolving forces on the beam:

Vertical: Hy+Tsin30=80+150H_y + T\sin 30^\circ = 80 + 150

Hy+192.5×0.5=230    Hy+96.25=230    Hy=133.75NH_y + 192.5 \times 0.5 = 230 \implies H_y + 96.25 = 230 \implies H_y = 133.75 \mathrm{ N} (upward)

Horizontal: Hx=Tcos30=192.5×0.866=166.7NH_x = T\cos 30^\circ = 192.5 \times 0.866 = 166.7 \mathrm{ N} (away from the wall)

H=Hx2+Hy2=166.72+133.752=27789+17889=45678=213.7NH = \sqrt{H_x^2 + H_y^2} = \sqrt{166.7^2 + 133.75^2} = \sqrt{27789 + 17889} = \sqrt{45678} = 213.7 \mathrm{ N}

Angle above horizontal: α=tan1(133.75/166.7)=tan1(0.803)=38.7\alpha = \tan^{-1}(133.75/166.7) = \tan^{-1}(0.803) = 38.7^\circ

Question 4 (DSE Structured)

A 500g500 \mathrm{ g} ball is attached to a string of length 0.80m0.80 \mathrm{ m} and swung in a vertical circle.

(a) The ball has speed 6.0m/s6.0 \mathrm{ m/s} at the lowest point. Calculate the tension in the string at this point.

(b) Calculate the speed of the ball at the highest point.

(c) Calculate the tension in the string at the highest point.

(d) Calculate the minimum speed at the lowest point for the ball to complete the full circle.

(e) Explain why the ball cannot complete the full circle if the string is replaced by a light rod (consider what happens at the top).

Solution

(a) At the lowest point: Tbottommg=mvbottom2rT_{\mathrm{bottom}} - mg = \frac{mv_{\mathrm{bottom}}^2}{r}

Tbottom=mg+mvbottom2r=0.5×9.81+0.5×360.80=4.905+22.5=27.4NT_{\mathrm{bottom}} = mg + \frac{mv_{\mathrm{bottom}}^2}{r} = 0.5 \times 9.81 + \frac{0.5 \times 36}{0.80} = 4.905 + 22.5 = 27.4 \mathrm{ N}

(b) Energy conservation between lowest and highest points (height difference =2r=1.6m= 2r = 1.6 \mathrm{ m}):

12mvbottom2=12mvtop2+mg(2r)\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

12(0.5)(36)=12(0.5)vtop2+0.5×9.81×1.6\frac{1}{2}(0.5)(36) = \frac{1}{2}(0.5)v_{\mathrm{top}}^2 + 0.5 \times 9.81 \times 1.6

9.0=0.25vtop2+7.859.0 = 0.25v_{\mathrm{top}}^2 + 7.85

vtop2=9.07.850.25=1.150.25=4.6v_{\mathrm{top}}^2 = \frac{9.0 - 7.85}{0.25} = \frac{1.15}{0.25} = 4.6

vtop=4.6=2.14m/sv_{\mathrm{top}} = \sqrt{4.6} = 2.14 \mathrm{ m/s}

(c) At the highest point: Ttop+mg=mvtop2rT_{\mathrm{top}} + mg = \frac{mv_{\mathrm{top}}^2}{r}

Ttop=mvtop2rmg=0.5×4.60.804.905=2.8754.905=2.03NT_{\mathrm{top}} = \frac{mv_{\mathrm{top}}^2}{r} - mg = \frac{0.5 \times 4.6}{0.80} - 4.905 = 2.875 - 4.905 = -2.03 \mathrm{ N}

Since the tension is negative, the string goes slack before the ball reaches the top. The ball does not complete the full circle.

(d) For the ball to just complete the circle: Ttop=0T_{\mathrm{top}} = 0 at the top, so vtop=gr=9.81×0.80=7.848=2.80m/sv_{\mathrm{top}} = \sqrt{gr} = \sqrt{9.81 \times 0.80} = \sqrt{7.848} = 2.80 \mathrm{ m/s}

12mvbottom2=12m(gr)+mg(2r)=12mgr+2mgr=52mgr\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}m(gr) + mg(2r) = \frac{1}{2}mgr + 2mgr = \frac{5}{2}mgr

vbottom=5gr=5×9.81×0.80=39.24=6.26m/sv_{\mathrm{bottom}} = \sqrt{5gr} = \sqrt{5 \times 9.81 \times 0.80} = \sqrt{39.24} = 6.26 \mathrm{ m/s}

(e) With a light rod, the rod can push as well as pull. At the top, even if vtop<grv_{\mathrm{top}} < \sqrt{gr}, the rod can exert a push (compression) to provide the additional centripetal force. The ball will still complete the circle as long as it reaches the top with any speed (the rod supports it).

With a string, the string can only pull (tension 0\geq 0). If the speed at the top is too low, the string goes slack and the ball falls.

Question 5 (DSE Structured)

A spacecraft of mass 1000kg1000 \mathrm{ kg} is travelling towards the Moon. The Moon has mass 7.35×1022kg7.35 \times 10^{22} \mathrm{ kg} and radius 1.74×106m1.74 \times 10^6 \mathrm{ m}.

(a) Calculate the gravitational field strength on the surface of the Moon.

(b) The spacecraft is at a height of 500km500 \mathrm{ km} above the Moon's surface. Calculate the gravitational force on the spacecraft.

(c) Calculate the escape velocity from the Moon's surface.

(d) Explain why the Moon has no atmosphere, referring to escape velocity and molecular speeds.

Solution

(a) gMoon=GMR2=6.67×1011×7.35×1022(1.74×106)2g_{\mathrm{Moon}} = \frac{GM}{R^2} = \frac{6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{(1.74 \times 10^6)^2}

gMoon=4.90×10123.03×1012=1.62N/kgg_{\mathrm{Moon}} = \frac{4.90 \times 10^{12}}{3.03 \times 10^{12}} = 1.62 \mathrm{ N/kg}

(b) r=1.74×106+500×103=2.24×106mr = 1.74 \times 10^6 + 500 \times 10^3 = 2.24 \times 10^6 \mathrm{ m}

F=GMmr2=6.67×1011×7.35×1022×1000(2.24×106)2=4.90×10155.02×1012=976NF = \frac{GMm}{r^2} = \frac{6.67 \times 10^{-11} \times 7.35 \times 10^{22} \times 1000}{(2.24 \times 10^6)^2} = \frac{4.90 \times 10^{15}}{5.02 \times 10^{12}} = 976 \mathrm{ N}

(c) ve=2GMR=2×6.67×1011×7.35×10221.74×106=9.80×10121.74×106=5.63×106=2370m/sv_e = \sqrt{\frac{2GM}{R}} = \sqrt{\frac{2 \times 6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{1.74 \times 10^6}} = \sqrt{\frac{9.80 \times 10^{12}}{1.74 \times 10^6}} = \sqrt{5.63 \times 10^6} = 2370 \mathrm{ m/s}

(d) The Moon's escape velocity (2370m/s2370 \mathrm{ m/s}) is relatively low. Gas molecules in the upper atmosphere have a range of speeds described by the Maxwell-Boltzmann distribution. A significant fraction of molecules (especially lighter ones like hydrogen and helium) have speeds exceeding the escape velocity. Over geological time, these molecules escape into space, and the Moon cannot retain an atmosphere. The Earth's much higher escape velocity (11200m/s11200 \mathrm{ m/s}) means very few molecules have sufficient speed to escape.


Extended Problems

Extended Problem 1: Banked Curve with Friction

A road curve of radius 80m80 \mathrm{ m} is banked at 1515^\circ. The coefficient of static friction between tyres and road is 0.400.40.

(a) Calculate the maximum speed at which a car can negotiate the curve without sliding up the bank.

(b) Calculate the minimum speed at which the car can negotiate the curve without sliding down the bank.

Solution

(a) At maximum speed, friction acts down the bank. Taking components:

Horizontally: Nsinθ+fcosθ=mvmax2rN\sin\theta + f\cos\theta = \frac{mv_{\max}^2}{r}

Vertically: Ncosθfsinθ=mgN\cos\theta - f\sin\theta = mg

Dividing the horizontal by the vertical equation:

sinθ+μscosθcosθμssinθ=vmax2rg\frac{\sin\theta + \mu_s\cos\theta}{\cos\theta - \mu_s\sin\theta} = \frac{v_{\max}^2}{rg}

vmax2=rgsin15+0.40cos15cos150.40sin15=80×9.81×0.259+0.3860.9660.104=784.8×0.6450.862=587v_{\max}^2 = rg\frac{\sin 15^\circ + 0.40\cos 15^\circ}{\cos 15^\circ - 0.40\sin 15^\circ} = 80 \times 9.81 \times \frac{0.259 + 0.386}{0.966 - 0.104} = 784.8 \times \frac{0.645}{0.862} = 587

vmax=587=24.2m/sv_{\max} = \sqrt{587} = 24.2 \mathrm{ m/s}

(b) At minimum speed, friction acts up the bank:

vmin2=rgsinθμscosθcosθ+μssinθ=80×9.81×0.2590.3860.966+0.104=784.8×0.1271.070v_{\min}^2 = rg\frac{\sin\theta - \mu_s\cos\theta}{\cos\theta + \mu_s\sin\theta} = 80 \times 9.81 \times \frac{0.259 - 0.386}{0.966 + 0.104} = 784.8 \times \frac{-0.127}{1.070}

Since the numerator is negative, vmin2<0v_{\min}^2 < 0, meaning the car will not slide down the bank at any speed (the banking alone provides enough centripetal force for stationary or very slow speeds). The minimum speed is effectively 00.

Extended Problem 2: Satellite Orbit Transfer

A satellite of mass 500kg500 \mathrm{ kg} is in a circular orbit of radius 7.0×106m7.0 \times 10^6 \mathrm{ m} around the Earth. The satellite needs to transfer to a higher circular orbit of radius 7.5×106m7.5 \times 10^6 \mathrm{ m}.

(a) Calculate the orbital speed in the lower orbit.

(b) Calculate the orbital speed in the higher orbit.

(c) Calculate the total energy required for the transfer (ignoring the mass of fuel burned).

(Earth mass =5.97×1024kg= 5.97 \times 10^{24} \mathrm{ kg})

Solution

(a) v1=GMr1=6.67×1011×5.97×10247.0×106=5.69×107=7544m/sv_1 = \sqrt{\frac{GM}{r_1}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{7.0 \times 10^6}} = \sqrt{5.69 \times 10^7} = 7544 \mathrm{ m/s}

(b) v2=GMr2=6.67×1011×5.97×10247.5×106=5.31×107=7287m/sv_2 = \sqrt{\frac{GM}{r_2}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{7.5 \times 10^6}} = \sqrt{5.31 \times 10^7} = 7287 \mathrm{ m/s}

(c) The energy in a circular orbit: E=GMm2rE = -\frac{GMm}{2r}

E1=6.67×1011×5.97×1024×5002×7.0×106=1.99×10171.4×107=1.42×1010JE_1 = -\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 500}{2 \times 7.0 \times 10^6} = -\frac{1.99 \times 10^{17}}{1.4 \times 10^7} = -1.42 \times 10^{10} \mathrm{ J}

E2=1.99×10171.5×107=1.33×1010JE_2 = -\frac{1.99 \times 10^{17}}{1.5 \times 10^7} = -1.33 \times 10^{10} \mathrm{ J}

Energy required: ΔE=E2E1=1.33×1010(1.42×1010)=9.0×108J\Delta E = E_2 - E_1 = -1.33 \times 10^{10} - (-1.42 \times 10^{10}) = 9.0 \times 10^8 \mathrm{ J}