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Physics - Mechanics

Intuition

Kinematics is the language of motion: Before you can understand why things move (forces, energy), you need to describe how they move (displacement, velocity, acceleration). Kinematics gives you the vocabulary and equations to describe any motion, from a ball rolling down a ramp to a satellite orbiting Earth.

Why it matters: Kinematics is the foundation of all mechanics. Every physics problem involving motion, from projectile motion to circular motion to oscillations, starts with kinematic descriptions. It’s also essential for engineering, robotics, and computer graphics.

The key insight: Velocity is the derivative of displacement, and acceleration is the derivative of velocity. This means acceleration tells you how velocity changes, which tells you how position changes. In the opposite direction, integration accumulates: the area under a velocity-time graph is displacement, and the area under an acceleration-time graph is velocity.

Kinematics

Kinematics is the study of motion without considering the forces that cause it. It describes the Motion of objects using displacement, velocity, and acceleration.

Displacement, Velocity, and Acceleration

QuantitySymbolSI UnitDefinition
DisplacementssmDistance moved in a specified direction
Velocityvvm/sRate of change of displacement
Accelerationaam/s2^2Rate of change of velocity

Displacement is a vector quantity; it has both magnitude and direction. Speed is the scalar Counterpart of velocity.

v=ΔsΔtv = \frac{\Delta s}{\Delta t} a=ΔvΔta = \frac{\Delta v}{\Delta t}

Equations of Uniformly Accelerated Motion (SUVAT Equations)

For motion with constant acceleration, the following equations apply:

v=u+atv = u + at s=ut+12at2s = ut + \frac{1}{2}at^2 v2=u2+2asv^2 = u^2 + 2as s=12(u+v)ts = \frac{1}{2}(u + v)t

Where:

  • uu = initial velocity
  • vv = final velocity
  • aa = constant acceleration
  • ss = displacement
  • tt = time

Worked Example 1

A car starts from rest and accelerates uniformly at 3m/s23 \mathrm{ m/s}^2 for 55 seconds. Find the Distance travelled.

Solution

Using s=ut+12at2s = ut + \frac{1}{2}at^2:

s=0+12(3)(5)2=12(3)(25)=37.5ms = 0 + \frac{1}{2}(3)(5)^2 = \frac{1}{2}(3)(25) = 37.5 \mathrm{ m}

Worked Example 1b

A cyclist travelling at 8m/s8 \mathrm{ m/s} applies the brakes and decelerates uniformly at 2m/s22 \mathrm{ m/s}^2. Find the time taken to stop and the distance travelled during braking.

Solution

Using v=u+atv = u + at with v=0v = 0:

0=8+(−2)t0 = 8 + (-2)t t=4st = 4 \mathrm{ s}

Using v2=u2+2asv^2 = u^2 + 2as:

0=82+2(−2)s0 = 8^2 + 2(-2)s s=644=16ms = \frac{64}{4} = 16 \mathrm{ m}

The cyclist takes 4s4 \mathrm{ s} to stop and travels 16m16 \mathrm{ m} during braking.

Worked Example 2

A ball is thrown vertically upwards with initial velocity 20m/s20 \mathrm{ m/s}. Find the maximum Height reached and the time taken to reach it.

Solution

At maximum height, v=0v = 0:

v2=u2+2asv^2 = u^2 + 2as 0=202+2(−9.81)s0 = 20^2 + 2(-9.81)s s=40019.62=20.39ms = \frac{400}{19.62} = 20.39 \mathrm{ m}

Time to reach maximum height:

v=u+atv = u + at 0=20−9.81t0 = 20 - 9.81t t=209.81=2.04st = \frac{20}{9.81} = 2.04 \mathrm{ s}

Displacement-Time and Velocity-Time Graphs

For a displacement-time graph:

  • Slope = instantaneous velocity
  • A straight line indicates constant velocity
  • A curved line indicates acceleration

For a velocity-time graph:

  • Slope = acceleration
  • Area under the graph = displacement
  • A straight line indicates uniform acceleration

Tip: Tip Squares or integration.

Free Fall

All objects in free fall near the Earth’s surface experience the same acceleration due to gravity, Denoted gg:

g≈9.81m/s2g \approx 9.81 \mathrm{ m/s}^2

The acceleration is downward regardless of whether the object is moving up or down.

Worked Example 3

An object is dropped from a height of 80m80 \mathrm{ m}. How long does it take to reach the ground?

Solutions=ut+12gt2s = ut + \frac{1}{2}gt^2 80=0+12(9.81)t280 = 0 + \frac{1}{2}(9.81)t^2 t2=1609.81t^2 = \frac{160}{9.81} t=16.31=4.04st = \sqrt{16.31} = 4.04 \mathrm{ s}

Projectile Motion

Projectile motion is the motion of an object launched into the air at an angle. It can be analysed by resolving the motion into horizontal and vertical components.

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

ux=ucos⁡θ(constant,nohorizontalacceleration)u_x = u\cos\theta \quad \mathrm{(constant, no horizontal acceleration)} uy=usin⁡θ(subjecttog)u_y = u\sin\theta \quad \mathrm{(subject to } g \mathrm{)}

The horizontal displacement (range) is:

R=u2sin⁡2θgR = \frac{u^2 \sin 2\theta}{g}

Maximum range occurs at θ=45∘\theta = 45^\circ.

The maximum height is:

H=u2sin⁡2θ2gH = \frac{u^2 \sin^2\theta}{2g}

Time of flight:

T=2usin⁡θgT = \frac{2u\sin\theta}{g}

Info: Info They share only the common variable tt (time).

Worked Example 4

A ball is thrown with initial velocity 15m/s15 \mathrm{ m/s} at 30∘30^\circ above the horizontal. Find the range and maximum height.

Solution

Horizontal component: ux=15cos⁡30∘=12.99m/su_x = 15\cos 30^\circ = 12.99 \mathrm{ m/s}

Vertical component: uy=15sin⁡30∘=7.5m/su_y = 15\sin 30^\circ = 7.5 \mathrm{ m/s}

Maximum height:

H=uy22g=7.522(9.81)=56.2519.62=2.87mH = \frac{u_y^2}{2g} = \frac{7.5^2}{2(9.81)} = \frac{56.25}{19.62} = 2.87 \mathrm{ m}

Time of flight:

T=2uyg=2(7.5)9.81=1.53sT = \frac{2u_y}{g} = \frac{2(7.5)}{9.81} = 1.53 \mathrm{ s}

Range:

R=ux×T=12.99×1.53=19.87mR = u_x \times T = 12.99 \times 1.53 = 19.87 \mathrm{ m}

Worked Example 4b

A stone is thrown horizontally from a cliff 60m60 \mathrm{ m} high with speed 15m/s15 \mathrm{ m/s}. Find the horizontal distance it travels before hitting the ground.

Solution

Vertical motion (to find time of flight):

s=ut+12gt2s = ut + \frac{1}{2}gt^2 60=0+12(9.81)t260 = 0 + \frac{1}{2}(9.81)t^2 t=1209.81=3.50st = \sqrt{\frac{120}{9.81}} = 3.50 \mathrm{ s}

Horizontal motion:

d=ux×t=15×3.50=52.5md = u_x \times t = 15 \times 3.50 = 52.5 \mathrm{ m}

Dynamics

Dynamics is the study of forces and their effects on motion. The central principle is Newton’s laws of 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 resultant external force.

Second Law: The resultant force acting on an object is equal to the rate of change of momentum Of the object:

F=ΔpΔt=d(mv)dtF = \frac{\Delta p}{\Delta t} = \frac{d(mv)}{dt}

For constant mass:

F=maF = ma

Third Law: If body A exerts a force on body B. Then body B exerts an equal and opposite Force on body A.

FAB=−FBAF_{AB} = -F_{BA}

Caution: Warning Together as they do not act on the same object.

Types of Forces

ForceSymbolDescription
WeightW=mgW = mgGravitational force on an object
Normal reactionNN or RRPerpendicular contact force from a surface
FrictionffOpposes relative motion between surfaces
TensionTTPulling force along a string or rope
Air resistanceFdF_dResistive force in a fluid, depends on speed

Free Body Diagrams

A free body diagram shows all the forces acting on a single object. Follow these steps:

  1. Isolate the object of interest
  2. Draw all external forces as arrows from the centre of the object
  3. Do not include forces that the object exerts on other objects

Worked Example 5

A block of mass 5kg5 \mathrm{ kg} is placed on a smooth inclined plane at 30∘30^\circ to the Horizontal. Find the acceleration down the plane.

Solution

Forces parallel to the plane: mgsin⁡θ=5(9.81)sin⁡30∘=24.525Nmg\sin\theta = 5(9.81)\sin 30^\circ = 24.525 \mathrm{ N}

Since the plane is smooth (no friction):

F=maF = ma 24.525=5a24.525 = 5a a=4.91m/s2a = 4.91 \mathrm{ m/s}^2

Worked Example 5b

Two objects of mass 3kg3 \mathrm{ kg} and 5kg5 \mathrm{ kg} are connected by a light inextensible String over a smooth pulley (Atwood machine). Find the acceleration and the tension in the string.

Solution

For the 3kg3 \mathrm{ kg} mass (let upward be positive):

T−3g=3a⋯(1)T - 3g = 3a \quad \cdots (1)

For the 5kg5 \mathrm{ kg} mass (let downward be positive):

5g−T=5a⋯(2)5g - T = 5a \quad \cdots (2)

Adding (1) and (2):

2g=8a2g = 8a a=2g8=19.628=2.45m/s2a = \frac{2g}{8} = \frac{19.62}{8} = 2.45 \mathrm{ m/s}^2

Substituting into (1):

T=3(9.81+2.45)=3×12.26=36.79NT = 3(9.81 + 2.45) = 3 \times 12.26 = 36.79 \mathrm{ N}

Friction

Friction opposes relative motion between two surfaces in contact.

  • Static friction (fsf_s): prevents motion from starting; varies up to a maximum value
  • Kinetic friction (fkf_k): opposes motion when surfaces are sliding; approximately constant
fs⩽μsNf_s \leqslant \mu_s N fk=μkNf_k = \mu_k N

Where μ\mu is the coefficient of friction and NN is the normal reaction force.

Tip: Tip

Worked Example 6

A 10kg10 \mathrm{ kg} block rests on a rough horizontal surface with μ=0.3\mu = 0.3. A horizontal force of 40N40 \mathrm{ N} is applied. Does the block move?

Solution

Normal reaction: N=mg=10×9.81=98.1NN = mg = 10 \times 9.81 = 98.1 \mathrm{ N}

Maximum static friction: fs=0.3×98.1=29.43Nf_s = 0.3 \times 98.1 = 29.43 \mathrm{ N}

Applied force =40N>29.43N= 40 \mathrm{ N} \gt 29.43 \mathrm{ N} So the block moves.

Acceleration: a=F−fkm=40−29.4310=1.057m/s2a = \frac{F - f_k}{m} = \frac{40 - 29.43}{10} = 1.057 \mathrm{ m/s}^2


Work, Energy, and Power

Work Done

Work is done when a force causes displacement in the direction of the force.

W=Fscos⁡θW = Fs\cos\theta

Where θ\theta is the angle between the force and the displacement.

  • If θ=0∘\theta = 0^\circ: W=FsW = Fs (maximum work)
  • If θ=90∘\theta = 90^\circ: W=0W = 0 (no work done)
  • If θ>90∘\theta \gt 90^\circ: W<0W \lt 0 (force opposes motion)

The SI unit of work is the joule (J), where 1J=1N⋅m1 \mathrm{ J} = 1 \mathrm{ N}\cdot\mathrm m.

Work Done by a Varying Force

When force varies with displacement, work is found from the area under a force-displacement graph:

W=∫s1s2F dsW = \int_{s_1}^{s_2} F \, ds

Work Done Against Gravity

W=mghW = mgh

This is the work required to raise an object of mass mm through a vertical height hh.

Work Done Stretching a Spring (Hooke’s Law)

For a spring obeying Hooke’s law, F=kxF = kx:

W=12kx2W = \frac{1}{2}kx^2

Where kk is the spring constant and xx is the extension.

Kinetic Energy

Ek=12mv2E_k = \frac{1}{2}mv^2

The kinetic energy of an object depends on its mass and the square of its speed.

Potential Energy

Gravitational potential energy:

Ep=mghE_p = mgh

Elastic potential energy (spring):

Ep=12kx2E_p = \frac{1}{2}kx^2

Principle of Conservation of Energy

Energy cannot be created or destroyed, only transformed from one form to another.

Totalenergyatstart=Totalenergyatend\mathrm{Total energy at start} = \mathrm{Total energy at end}

In the presence of friction:

Ek+Ep+Wfriction=constantE_k + E_p + W_{\mathrm{friction}} = \mathrm{constant}

Or equivalently:

Ek1+Ep1=Ek2+Ep2+WlosttofrictionE_{k1} + E_{p1} = E_{k2} + E_{p2} + W_{\mathrm{lost to friction}}

Info: Info The motion.

Worked Example 7

A roller coaster car of mass 500kg500 \mathrm{ kg} starts from rest at point A20m20 \mathrm{ m} Above the ground. It descends to point B5m5 \mathrm{ m} above the ground. Find its speed at B Neglecting friction.

Solution

At A: Ek=0E_k = 0, Ep=500×9.81×20=98100JE_p = 500 \times 9.81 \times 20 = 98100 \mathrm{ J}

At B: Ek=12(500)v2E_k = \frac{1}{2}(500)v^2, Ep=500×9.81×5=24525JE_p = 500 \times 9.81 \times 5 = 24525 \mathrm{ J}

By conservation of energy:

98100=12(500)v2+2452598100 = \frac{1}{2}(500)v^2 + 24525 12(500)v2=73575\frac{1}{2}(500)v^2 = 73575 v2=147150500=294.3v^2 = \frac{147150}{500} = 294.3 v=17.16m/sv = 17.16 \mathrm{ m/s}

Worked Example 7b

A 2kg2 \mathrm{ kg} block slides down a rough inclined plane of length 5m5 \mathrm{ m} at 30∘30^\circ to the horizontal. The coefficient of friction is 0.20.2. Find the speed at the bottom starting from Rest.

Solution

Force down the plane: mgsin⁡30∘=2(9.81)(0.5)=9.81Nmg\sin 30^\circ = 2(9.81)(0.5) = 9.81 \mathrm{ N}

Normal reaction: N=mgcos⁡30∘=2(9.81)(0.866)=16.99NN = mg\cos 30^\circ = 2(9.81)(0.866) = 16.99 \mathrm{ N}

Friction: f=μN=0.2×16.99=3.40Nf = \mu N = 0.2 \times 16.99 = 3.40 \mathrm{ N}

Net force: F=9.81−3.40=6.41NF = 9.81 - 3.40 = 6.41 \mathrm{ N}

a=Fm=6.412=3.205m/s2a = \frac{F}{m} = \frac{6.41}{2} = 3.205 \mathrm{ m/s}^2 v2=u2+2as=0+2(3.205)(5)=32.05v^2 = u^2 + 2as = 0 + 2(3.205)(5) = 32.05 v=5.66m/sv = 5.66 \mathrm{ m/s}

Power

Power is the rate of doing work:

P=WtP = \frac{W}{t} P=FvP = Fv

The SI unit of power is the watt (W), where 1W=1J/s1 \mathrm{ W} = 1 \mathrm{ J/s}.

Worked Example 8

A car of mass 1200kg1200 \mathrm{ kg} travels at a constant speed of 20m/s20 \mathrm{ m/s} up a slope of sin⁡−1(0.1)\sin^{-1}(0.1). The total resistive force is 300N300 \mathrm{ N}. Find the power output of the Engine.

Solution

Component of weight along the slope: mgsin⁡θ=1200×9.81×0.1=1177.2Nmg\sin\theta = 1200 \times 9.81 \times 0.1 = 1177.2 \mathrm{ N}

Total force the engine must overcome: F=1177.2+300=1477.2NF = 1177.2 + 300 = 1477.2 \mathrm{ N}

P=Fv=1477.2×20=29544W=29.5kWP = Fv = 1477.2 \times 20 = 29544 \mathrm{ W} = 29.5 \mathrm{ kW}

Momentum and Impulse

Linear Momentum

p=mvp = mv

Momentum is a vector quantity with SI unit kg m/s.

Principle of Conservation of Momentum

For a system of objects with no external resultant force:

∑pinitial=∑pfinal\sum p_{\mathrm{initial}} = \sum p_{\mathrm{final}} m1u1+m2u2=m1v1+m2v2m_1u_1 + m_2u_2 = m_1v_1 + m_2v_2

Newton’s Second Law in Terms of Momentum

F=ΔpΔtF = \frac{\Delta p}{\Delta t}

This is the most general form of Newton’s second law and is valid even when mass changes.

Impulse

Impulse=FΔt=Δp\mathrm{Impulse} = F\Delta t = \Delta p

Impulse equals the change in momentum. The SI unit is N s.

Tip: Impulse is the area under a force-time graph. For a variable force, use J=∫F dtJ = \int F \, dt.

Worked Example 9

A 0.15kg0.15 \mathrm{ kg} cricket ball travelling at 30m/s30 \mathrm{ m/s} is hit back along the same line at 20m/s20 \mathrm{ m/s}. If the bat is in contact with the ball for 0.005s0.005 \mathrm{ s} Find the Average force exerted.

Solution

Take the initial direction as positive.

Δp=m(v−u)=0.15(−20−30)=0.15(−50)=−7.5kgm/s\Delta p = m(v - u) = 0.15(-20 - 30) = 0.15(-50) = -7.5 \mathrm{ kg m/s} F=ΔpΔt=−7.50.005=−1500NF = \frac{\Delta p}{\Delta t} = \frac{-7.5}{0.005} = -1500 \mathrm{ N}

The negative sign indicates the force acts in the opposite direction to the initial motion. The Magnitude of the average force is 1500N1500 \mathrm{ N}.

Collisions

Elastic collision: Both momentum and kinetic energy are conserved.

Inelastic collision: Momentum is conserved but kinetic energy is not.

Perfectly inelastic collision: The objects stick together after collision (maximum kinetic Energy loss).

Worked Example 10

A 2kg2 \mathrm{ kg} object moving at 5m/s5 \mathrm{ m/s} collides head-on with a 3kg3 \mathrm{ kg} Object at rest. If the collision is perfectly inelastic, find the common velocity after collision.

Solution

By conservation of momentum:

m1u1+m2u2=(m1+m2)vm_1u_1 + m_2u_2 = (m_1 + m_2)v 2(5)+3(0)=(2+3)v2(5) + 3(0) = (2 + 3)v 10=5v10 = 5v v=2m/sv = 2 \mathrm{ m/s}

Worked Example 11 (Elastic Collision)

A 2kg2 \mathrm{ kg} object moving at 5m/s5 \mathrm{ m/s} collides elastically with a 3kg3 \mathrm{ kg} Object at rest. Find the velocities after collision.

Solution

Conservation of momentum:

2(5)+3(0)=2v1+3v22(5) + 3(0) = 2v_1 + 3v_2 10=2v1+3v2(1)10 = 2v_1 + 3v_2 \quad \mathrm{(1)}

Conservation of kinetic energy:

12(2)(52)=12(2)v12+12(3)v22\frac{1}{2}(2)(5^2) = \frac{1}{2}(2)v_1^2 + \frac{1}{2}(3)v_2^2 25=v12+1.5v22(2)25 = v_1^2 + 1.5v_2^2 \quad \mathrm{(2)}

From equation (1): v1=10−3v22v_1 = \frac{10 - 3v_2}{2}

Substituting into (2):

25=(10−3v22)2+1.5v2225 = \left(\frac{10 - 3v_2}{2}\right)^2 + 1.5v_2^2 25=100−60v2+9v224+1.5v2225 = \frac{100 - 60v_2 + 9v_2^2}{4} + 1.5v_2^2 100=100−60v2+9v22+6v22100 = 100 - 60v_2 + 9v_2^2 + 6v_2^2 15v22−60v2=015v_2^2 - 60v_2 = 0 15v2(v2−4)=015v_2(v_2 - 4) = 0

v2=0v_2 = 0 (original situation) or v2=4m/sv_2 = 4 \mathrm{ m/s}

Therefore v1=10−122=−1m/sv_1 = \frac{10 - 12}{2} = -1 \mathrm{ m/s}

The 2kg2 \mathrm{ kg} object rebounds at 1m/s1 \mathrm{ m/s} And the 3kg3 \mathrm{ kg} object moves Forward at 4m/s4 \mathrm{ m/s}.


Circular Motion

Angular Quantities

QuantitySymbolSI UnitRelation
Angular displacementθ\thetaradθ=sr\theta = \frac{s}{r}
Angular velocityω\omegarad/sω=dθdt\omega = \frac{d\theta}{dt}
Angular accelerationα\alpharad/s2^2α=dωdt\alpha = \frac{d\omega}{dt}

Relation to linear quantities:

v=rωv = r\omega a=rαa = r\alpha

Centripetal Acceleration and Force

An object moving in a circle at constant speed has a centripetal acceleration directed towards the Centre:

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

The centripetal force required is:

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

Worked Example 12

A car of mass 1000kg1000 \mathrm{ kg} travels around a roundabout of radius 25m25 \mathrm{ m} at 10m/s10 \mathrm{ m/s}. Find the centripetal force.

SolutionFc=mv2r=1000×10225=10000025=4000NF_c = \frac{mv^2}{r} = \frac{1000 \times 10^2}{25} = \frac{100000}{25} = 4000 \mathrm{ N}

This force is provided by friction between the tyres and the road.

Worked Example 13

A particle of mass 0.5kg0.5 \mathrm{ kg} is attached to a string of length 0.8m0.8 \mathrm{ m} and Whirled in a horizontal circle at 3rev/s3 \mathrm{ rev/s}. Find the tension in the string.

Solution

Angular velocity: ω=2π×3=6πrad/s\omega = 2\pi \times 3 = 6\pi \mathrm{ rad/s}

T=Fc=mω2r=0.5×(6π)2×0.8T = F_c = m\omega^2 r = 0.5 \times (6\pi)^2 \times 0.8 T=0.5×36π2×0.8=14.4π2=142.1NT = 0.5 \times 36\pi^2 \times 0.8 = 14.4\pi^2 = 142.1 \mathrm{ N}

Worked Example 13b

A car of mass 800kg800 \mathrm{ kg} travels at 15m/s15 \mathrm{ m/s} around a banked curve of radius 50m50 \mathrm{ m} and angle 20∘20^\circ. Find the normal reaction force and the frictional force Required if the car does not rely on friction alone.

Solution

Resolving vertically: Ncos⁡20∘=mgN\cos 20^\circ = mg

N=800×9.81cos⁡20∘=78480.9397=8352NN = \frac{800 \times 9.81}{\cos 20^\circ} = \frac{7848}{0.9397} = 8352 \mathrm{ N}

Resolving horizontally (centripetal direction):

Nsin⁡20∘+f=mv2rN\sin 20^\circ + f = \frac{mv^2}{r} 8352×0.342+f=800×225508352 \times 0.342 + f = \frac{800 \times 225}{50} 2856+f=36002856 + f = 3600 f=744Nf = 744 \mathrm{ N}

Vertical Circular Motion

For an object moving in a vertical circle, the speed is not constant because gravity does work on the object.

At the top of the circle:

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

At the bottom of the circle:

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

For the object to complete the full circle, the tension at the top must satisfy T⩾0T \geqslant 0 Giving:

vtop⩾grv_{\mathrm{top}} \geqslant \sqrt{gr}

Gravitation

Newton’s Law of Universal Gravitation

Every particle attracts every other particle with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them:

F=Gm1m2r2F = \frac{Gm_1m_2}{r^2}

Where G=6.67×10−11Nm2kg−2G = 6.67 \times 10^{-11} \mathrm{ N m}^2 \mathrm{ kg}^{-2} is the universal gravitational Constant.

Gravitational Field Strength

The gravitational field strength at a point is the force per unit mass placed at that point:

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

Near the Earth’s surface, g≈9.81N/kgg \approx 9.81 \mathrm{ N/kg}.

Gravitational Potential Energy

For two masses separated by distance rr:

Ep=−GMmrE_p = -\frac{GMm}{r}

The negative sign indicates that work must be done against gravity to separate the masses to Infinity (where Ep=0E_p = 0).

Orbital Motion

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

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

Orbital period:

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

Worked Example 14

Find the orbital speed of a satellite orbiting the Earth at a height of 300km300 \mathrm{ km} above the Surface. (Earth’s radius =6.37×106m= 6.37 \times 10^6 \mathrm{ m} Earth’s mass =5.97×1024kg= 5.97 \times 10^{24} \mathrm{ kg})

Solutionr=6.37×106+300×103=6.67×106mr = 6.37 \times 10^6 + 300 \times 10^3 = 6.67 \times 10^6 \mathrm{ m} v=GMr=6.67×10−11×5.97×10246.67×106v = \sqrt{\frac{GM}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.67 \times 10^6}} v=5.97×107=7727m/sv = \sqrt{5.97 \times 10^7} = 7727 \mathrm{ m/s}

Summary Table

TopicKey FormulaKey Concept
Kinematicsv2=u2+2asv^2 = u^2 + 2asSUVAT for constant acceleration
Projectile motionR=u2sin⁡2θgR = \frac{u^2\sin 2\theta}{g}Resolve into horizontal and vertical
Newton’s Second LawF=maF = maForce equals rate of change of momentum
WorkW=Fscos⁡θW = Fs\cos\thetaEnergy transfer by a force
Kinetic energyEk=12mv2E_k = \frac{1}{2}mv^2Energy of motion
Conservation of energyEk1+Ep1=Ek2+Ep2E_{k1} + E_{p1} = E_{k2} + E_{p2}Energy cannot be created or destroyed
Momentump=mvp = mvVector quantity
ImpulseJ=FΔt=ΔpJ = F\Delta t = \Delta pChange in momentum
Centripetal forceFc=mv2rF_c = \frac{mv^2}{r}Resultant force towards centre
GravitationF=Gm1m2r2F = \frac{Gm_1m_2}{r^2}Inverse square law

Exam Tips

  • Always draw a clear free body diagram before applying Newton’s second law.
  • Define a positive direction and stick to it throughout the calculation.
  • In projectile motion, treat horizontal and vertical components separately.
  • Check whether energy is conserved before applying conservation of energy equations.
  • In collision problems, momentum is always conserved; kinetic energy is only conserved in elastic collisions.
  • For circular motion, always identify what provides the centripetal force.
  • Remember that gg acts downward; use negative sign when taking upward as positive.
Exam-Style Practice Questions

Question 1: A stone is thrown horizontally from a cliff 60m60 \mathrm{ m} high with speed 15m/s15 \mathrm{ m/s}. Find the horizontal distance it travels before hitting the ground.

Details

Solution

Vertical motion: 60=12(9.81)t260 = \frac{1}{2}(9.81)t^2 So t=1209.81=3.50st = \sqrt{\frac{120}{9.81}} = 3.50 \mathrm{ s}

Horizontal distance: d=15×3.50=52.5md = 15 \times 3.50 = 52.5 \mathrm{ m}

Question 2: Two objects of mass 3kg3 \mathrm{ kg} and 5kg5 \mathrm{ kg} are connected by a light Inextensible string over a smooth pulley. Find the acceleration and the tension.

Solutiona=(m2−m1)gm1+m2=(5−3)(9.81)3+5=19.628=2.45m/s2a = \frac{(m_2 - m_1)g}{m_1 + m_2} = \frac{(5 - 3)(9.81)}{3 + 5} = \frac{19.62}{8} = 2.45 \mathrm{ m/s}^2 T=2m1m2gm1+m2=2(3)(5)(9.81)8=36.79NT = \frac{2m_1m_2g}{m_1 + m_2} = \frac{2(3)(5)(9.81)}{8} = 36.79 \mathrm{ N}

Question 3: A 0.5kg0.5 \mathrm{ kg} ball is dropped from a height of 2m2 \mathrm{ m} onto a hard Floor and rebounds to 1.5m1.5 \mathrm{ m}. Find the impulse exerted by the floor.

Solution

Velocity just before impact: v=2gh=2(9.81)(2)=6.26m/sv = \sqrt{2gh} = \sqrt{2(9.81)(2)} = 6.26 \mathrm{ m/s} (downward)

Velocity just after rebound: v=2(9.81)(1.5)=5.42m/sv = \sqrt{2(9.81)(1.5)} = 5.42 \mathrm{ m/s} (upward)

Taking upward as positive: Δp=0.5(5.42−(−6.26))=0.5(11.68)=5.84kgm/s\Delta p = 0.5(5.42 - (-6.26)) = 0.5(11.68) = 5.84 \mathrm{ kg m/s}

Impulse =5.84Ns= 5.84 \mathrm{ N s} (upward)

Question 4: A 3kg3 \mathrm{ kg} object slides down a rough inclined plane of length 5m5 \mathrm{ m} at 30∘30^\circ to the horizontal. The coefficient of friction is 0.20.2. Find the Speed at the bottom if the object starts from rest.

Solution

Force down the plane: mgsin⁡30∘=3(9.81)(0.5)=14.715Nmg\sin 30^\circ = 3(9.81)(0.5) = 14.715 \mathrm{ N}

Normal reaction: N=mgcos⁡30∘=3(9.81)(0.866)=25.49NN = mg\cos 30^\circ = 3(9.81)(0.866) = 25.49 \mathrm{ N}

Friction: f=μN=0.2×25.49=5.10Nf = \mu N = 0.2 \times 25.49 = 5.10 \mathrm{ N}

Net force down the plane: F=14.715−5.10=9.615NF = 14.715 - 5.10 = 9.615 \mathrm{ N}

a=Fm=9.6153=3.205m/s2a = \frac{F}{m} = \frac{9.615}{3} = 3.205 \mathrm{ m/s}^2 v2=u2+2as=0+2(3.205)(5)=32.05v^2 = u^2 + 2as = 0 + 2(3.205)(5) = 32.05 v=5.66m/sv = 5.66 \mathrm{ m/s}

Question 5: A satellite orbits the Earth at a height of 500km500 \mathrm{ km}. Given the Earth’s Mass is 5.97×1024kg5.97 \times 10^{24} \mathrm{ kg} and radius is 6.37×106m6.37 \times 10^6 \mathrm{ m} Find the Orbital period.

Solutionr=6.37×106+500×103=6.87×106mr = 6.37 \times 10^6 + 500 \times 10^3 = 6.87 \times 10^6 \mathrm{ m} v=GMr=6.67×10−11×5.97×10246.87×106=5.79×107=7611m/sv = \sqrt{\frac{GM}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{6.87 \times 10^6}} = \sqrt{5.79 \times 10^7} = 7611 \mathrm{ m/s} T=2πrv=2π×6.87×1067611=5671s=94.5minutesT = \frac{2\pi r}{v} = \frac{2\pi \times 6.87 \times 10^6}{7611} = 5671 \mathrm{ s} = 94.5 \mathrm{ minutes}

Simple Harmonic Motion

Definition

Simple harmonic motion (SHM) is a type of periodic motion where the restoring force is directly Proportional to the displacement from the equilibrium position and acts in the opposite direction.

F=−kxF = -kx a=−ω2xa = -\omega^2 x

Where:

  • FF = restoring force
  • kk = force constant (spring constant)
  • xx = displacement from equilibrium
  • ω\omega = angular frequency
  • aa = acceleration

Equations of SHM

Displacement:

x=Acos⁡(ωt)orx=Asin⁡(ωt)x = A\cos(\omega t) \quad \mathrm{or} \quad x = A\sin(\omega t)

Where AA is the amplitude (maximum displacement).

Velocity:

v=±ωA2−x2v = \pm\omega\sqrt{A^2 - x^2}

Maximum velocity occurs at equilibrium (x=0x = 0):

vmax⁡=ωAv_{\max} = \omega A

Acceleration:

a=−ω2xa = -\omega^2 x

Maximum acceleration occurs at maximum displacement (x=Ax = A):

amax⁡=ω2Aa_{\max} = \omega^2 A

Period:

For a mass-spring system: T=2πmkT = 2\pi\sqrt{\frac{m}{k}}

For a simple pendulum (small angle approximation): T=2πLgT = 2\pi\sqrt{\frac{L}{g}}

Worked Example 15

A mass of 0.5kg0.5 \mathrm{ kg} is attached to a spring with constant 200N/m200 \mathrm{ N/m} and displaced 0.05m0.05 \mathrm{ m} from equilibrium. Find the period, maximum velocity, and maximum acceleration.

SolutionT=2πmk=2π0.5200=2π0.0025=2π×0.05=0.314sT = 2\pi\sqrt{\frac{m}{k}} = 2\pi\sqrt{\frac{0.5}{200}} = 2\pi\sqrt{0.0025} = 2\pi \times 0.05 = 0.314 \mathrm{ s} ω=2πT=2π0.314=20.0rad/s\omega = \frac{2\pi}{T} = \frac{2\pi}{0.314} = 20.0 \mathrm{ rad/s} vmax⁡=ωA=20.0×0.05=1.00m/sv_{\max} = \omega A = 20.0 \times 0.05 = 1.00 \mathrm{ m/s} amax⁡=ω2A=400×0.05=20.0m/s2a_{\max} = \omega^2 A = 400 \times 0.05 = 20.0 \mathrm{ m/s}^2

Worked Example 16

A simple pendulum has a length of 1.0m1.0 \mathrm{ m}. Find its period.

SolutionT=2πLg=2π1.09.81=2π×0.319=2.01sT = 2\pi\sqrt{\frac{L}{g}} = 2\pi\sqrt{\frac{1.0}{9.81}} = 2\pi \times 0.319 = 2.01 \mathrm{ s}

Energy in SHM

In SHM, kinetic energy and potential energy continuously interchange, but the total energy remains Constant.

Ek=12mv2=12mω2(A2−x2)E_k = \frac{1}{2}mv^2 = \frac{1}{2}m\omega^2(A^2 - x^2) Ep=12kx2=12mω2x2E_p = \frac{1}{2}kx^2 = \frac{1}{2}m\omega^2 x^2 Etotal=12mω2A2=12kA2E_{\mathrm{total}} = \frac{1}{2}m\omega^2 A^2 = \frac{1}{2}kA^2

At equilibrium (x=0x = 0): all energy is kinetic (Ek=EtotalE_k = E_{\mathrm{total}})

At maximum displacement (x=Ax = A): all energy is potential (Ep=EtotalE_p = E_{\mathrm{total}})

Worked Example 17

A mass-spring system has mass 0.2kg0.2 \mathrm{ kg} Spring constant 80N/m80 \mathrm{ N/m} And amplitude 0.03m0.03 \mathrm{ m}. Find the total energy and the speed when the displacement is 0.02m0.02 \mathrm{ m}.

SolutionEtotal=12kA2=12(80)(0.03)2=12(80)(0.0009)=0.036JE_{\mathrm{total}} = \frac{1}{2}kA^2 = \frac{1}{2}(80)(0.03)^2 = \frac{1}{2}(80)(0.0009) = 0.036 \mathrm{ J}

At x=0.02mx = 0.02 \mathrm{ m}:

Ek=Etotal−Ep=0.036−12(80)(0.02)2=0.036−0.016=0.020JE_k = E_{\mathrm{total}} - E_p = 0.036 - \frac{1}{2}(80)(0.02)^2 = 0.036 - 0.016 = 0.020 \mathrm{ J} v=2Ekm=2×0.0200.2=0.20=0.447m/sv = \sqrt{\frac{2E_k}{m}} = \sqrt{\frac{2 \times 0.020}{0.2}} = \sqrt{0.20} = 0.447 \mathrm{ m/s}

Damping and Forced Oscillations

Damping

Damping is the reduction in amplitude of oscillations due to energy loss ( to friction or air Resistance).

  • Light damping: Amplitude decreases gradually; the period is nearly unchanged
  • Heavy damping: Amplitude decreases rapidly; period increases slightly
  • Critical damping: The system returns to equilibrium in the shortest time without oscillating
  • Overdamping: The system returns to equilibrium very slowly without oscillating

Resonance

When a system is driven at its natural frequency, the amplitude of oscillation reaches a maximum. This is called resonance.

  • At resonance, energy is transferred most efficiently from the driving force to the system
  • The amplitude at resonance depends on the degree of damping
  • Lightly damped systems show sharp resonance peaks
  • Heavily damped systems show broad, low resonance peaks

Examples of SHM and Resonance

ExampleType
Mass on a springSHM
Simple pendulumSHM (small angles)
Liquid in a U-tubeSHM
Vibrating tuning forkSHM
Bridge in windResonance (potentially destructive)
Microwave heatingResonance of water molecules
Musical instrumentsResonance of air columns and strings

Problem Set

Problem 1: SUVAT, Deceleration

A car travelling at 25m/s25 \mathrm{ m/s} decelerates uniformly to rest in 4s4 \mathrm{ s}. Find the Deceleration and the distance travelled.

Solutionv=u+at  ⟹  0=25+a(4)  ⟹  a=−6.25m/s2v = u + at \implies 0 = 25 + a(4) \implies a = -6.25 \mathrm{ m/s}^2 s=ut+12at2=25(4)+12(−6.25)(16)=100−50=50ms = ut + \frac{1}{2}at^2 = 25(4) + \frac{1}{2}(-6.25)(16) = 100 - 50 = 50 \mathrm{ m}

If you get this wrong, revise: SUVAT equations and the sign convention for deceleration.

Problem 2: Projectile, Maximum Height and Range

A ball is thrown with speed 20m/s20 \mathrm{ m/s} at 45∘45^\circ above the horizontal. Find the maximum Height and the horizontal range.

Solutionux=20cos⁡45∘=14.14m/su_x = 20\cos 45^\circ = 14.14 \mathrm{ m/s} uy=20sin⁡45∘=14.14m/su_y = 20\sin 45^\circ = 14.14 \mathrm{ m/s} H=uy22g=14.1422(9.81)=20019.62=10.19mH = \frac{u_y^2}{2g} = \frac{14.14^2}{2(9.81)} = \frac{200}{19.62} = 10.19 \mathrm{ m} R=u2sin⁡2θg=400×sin⁡90∘9.81=4009.81=40.77mR = \frac{u^2 \sin 2\theta}{g} = \frac{400 \times \sin 90^\circ}{9.81} = \frac{400}{9.81} = 40.77 \mathrm{ m}

If you get this wrong, revise: Projectile motion formulas for maximum height and range.

Problem 3: Newton’s Second Law, Inclined Plane

A 4kg4 \mathrm{ kg} block is placed on a rough inclined plane at 35∘35^\circ to the horizontal. The Coefficient of kinetic friction is 0.250.25. Find the acceleration of the block sliding down.

SolutionF∥=mgsin⁡35∘=4×9.81×0.5736=22.51NF_{\parallel} = mg\sin 35^\circ = 4 \times 9.81 \times 0.5736 = 22.51 \mathrm{ N} N=mgcos⁡35∘=4×9.81×0.8192=32.15NN = mg\cos 35^\circ = 4 \times 9.81 \times 0.8192 = 32.15 \mathrm{ N} fk=μkN=0.25×32.15=8.04Nf_k = \mu_k N = 0.25 \times 32.15 = 8.04 \mathrm{ N} Fnet=22.51−8.04=14.47NF_{\mathrm{net}} = 22.51 - 8.04 = 14.47 \mathrm{ N} a=14.474=3.62m/s2a = \frac{14.47}{4} = 3.62 \mathrm{ m/s}^2

If you get this wrong, revise: Forces on an inclined plane and kinetic friction.

Problem 4: Conservation of Energy with Friction

A 1.5kg1.5 \mathrm{ kg} block slides from rest down a curved frictionless ramp of height 3m3 \mathrm{ m} Onto a rough horizontal surface. The coefficient of friction on the horizontal surface is 0.30.3. How far does the block slide before stopping?

Solution

By conservation of energy, the kinetic energy at the bottom of the ramp equals the potential energy at the top:

Ek=mgh=1.5×9.81×3=44.15JE_k = mgh = 1.5 \times 9.81 \times 3 = 44.15 \mathrm{ J}

This energy is dissipated by friction on the horizontal surface:

Ek=fk×d=μmg×dE_k = f_k \times d = \mu mg \times d 44.15=0.3×1.5×9.81×d=4.41d44.15 = 0.3 \times 1.5 \times 9.81 \times d = 4.41d d=44.154.41=10.01md = \frac{44.15}{4.41} = 10.01 \mathrm{ m}

If you get this wrong, revise: Conservation of energy and work done against friction.

Problem 5: Elastic Collision, Equal Masses

A ball of mass 2kg2 \mathrm{ kg} moving at 6m/s6 \mathrm{ m/s} collides elastically with a stationary Ball of the same mass. Find the velocities after collision.

Solution

For an elastic collision between equal masses, the balls exchange velocities:

v1=0m/s,v2=6m/sv_1 = 0 \mathrm{ m/s}, \quad v_2 = 6 \mathrm{ m/s}

Verification:

Conservation of momentum: 2(6)+2(0)=2(0)+2(6)=122(6) + 2(0) = 2(0) + 2(6) = 12 ✓

Conservation of KE: 12(2)(36)=36=12(2)(0)+12(2)(36)=36\frac{1}{2}(2)(36) = 36 = \frac{1}{2}(2)(0) + \frac{1}{2}(2)(36) = 36 ✓

If you get this wrong, revise: Elastic collisions between equal masses and conservation laws.

Problem 6: Impulse from Force-Time Graph

A force-time graph shows a constant force of 50N50 \mathrm{ N} acting for 0.1s0.1 \mathrm{ s} Followed by a linearly decreasing force from 50N50 \mathrm{ N} to 0N0 \mathrm{ N} over the next 0.2s0.2 \mathrm{ s}. Find the impulse and the change in velocity of a 5kg5 \mathrm{ kg} object.

Solution

Impulse = area under the F-t graph:

First part: 50×0.1=5.0Ns50 \times 0.1 = 5.0 \mathrm{ N s}

Second part: 12×50×0.2=5.0Ns\frac{1}{2} \times 50 \times 0.2 = 5.0 \mathrm{ N s}

Total impulse: J=5.0+5.0=10.0NsJ = 5.0 + 5.0 = 10.0 \mathrm{ N s}

Δv=Jm=10.05=2.0m/s\Delta v = \frac{J}{m} = \frac{10.0}{5} = 2.0 \mathrm{ m/s}

If you get this wrong, revise: Impulse as the area under a force-time graph and the impulse-momentum Theorem.

Problem 7: Centripetal Force, Conical Pendulum

A conical pendulum consists of a 0.5kg0.5 \mathrm{ kg} mass on a string of length 1.0m1.0 \mathrm{ m} Swinging in a horizontal circle of radius 0.8m0.8 \mathrm{ m}. Find the tension and the speed of the Mass.

Solution

The string makes an angle with the vertical. The vertical component of tension balances weight:

Tcos⁡θ=mgT\cos\theta = mg

The horizontal component provides centripetal force:

Tsin⁡θ=mv2rT\sin\theta = \frac{mv^2}{r}

The string length is L=1.0mL = 1.0 \mathrm{ m} and the radius is r=0.8mr = 0.8 \mathrm{ m} So:

sin⁡θ=rL=0.8,cos⁡θ=0.6\sin\theta = \frac{r}{L} = 0.8, \quad \cos\theta = 0.6 T=mgcos⁡θ=0.5×9.810.6=8.175NT = \frac{mg}{\cos\theta} = \frac{0.5 \times 9.81}{0.6} = 8.175 \mathrm{ N} Tsin⁡θ=mv2r  ⟹  8.175×0.8=0.5v20.8T\sin\theta = \frac{mv^2}{r} \implies 8.175 \times 0.8 = \frac{0.5v^2}{0.8} v2=8.175×0.8×0.80.5=10.46v^2 = \frac{8.175 \times 0.8 \times 0.8}{0.5} = 10.46 v=3.23m/sv = 3.23 \mathrm{ m/s}

If you get this wrong, revise: Circular motion in a vertical plane and resolving forces for conical Pendulums.

Problem 8: Gravitational Field Strength, Above Surface

Find the gravitational field strength at a height of 300km300 \mathrm{ km} above the Earth’s surface. (Earth’s radius =6.37×106m= 6.37 \times 10^6 \mathrm{ m} Earth’s mass =5.97×1024kg= 5.97 \times 10^{24} \mathrm{ kg})

Solutionr=6.37×106+3.0×105=6.67×106mr = 6.37 \times 10^6 + 3.0 \times 10^5 = 6.67 \times 10^6 \mathrm{ m} g=GMr2=6.67×10−11×5.97×1024(6.67×106)2g = \frac{GM}{r^2} = \frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{(6.67 \times 10^6)^2} g=3.982×10144.449×1013=8.95N/kgg = \frac{3.982 \times 10^{14}}{4.449 \times 10^{13}} = 8.95 \mathrm{ N/kg}

This is less than 9.81N/kg9.81 \mathrm{ N/kg} at the surface, as expected.

If you get this wrong, revise: Newton’s law of gravitation and gravitational field strength at a Distance from a spherical body.

Problem 9: SHM, Finding Velocity at a Given Displacement

A mass-spring system has mass 0.3kg0.3 \mathrm{ kg} Spring constant 120N/m120 \mathrm{ N/m} And amplitude 0.04m0.04 \mathrm{ m}. Find the velocity when the displacement is 0.02m0.02 \mathrm{ m}.

Solutionω=km=1200.3=400=20rad/s\omega = \sqrt{\frac{k}{m}} = \sqrt{\frac{120}{0.3}} = \sqrt{400} = 20 \mathrm{ rad/s} v=±ωA2−x2=200.042−0.022=200.0016−0.0004=200.0012v = \pm\omega\sqrt{A^2 - x^2} = 20\sqrt{0.04^2 - 0.02^2} = 20\sqrt{0.0016 - 0.0004} = 20\sqrt{0.0012} v=20×0.0346=0.693m/sv = 20 \times 0.0346 = 0.693 \mathrm{ m/s}

If you get this wrong, revise: SHM velocity equation and the relationship between velocity and Displacement.

Problem 10: Simple Pendulum, Finding Length

A simple pendulum has a period of 2.5s2.5 \mathrm{ s}. Find its length.

SolutionT=2πLgT = 2\pi\sqrt{\frac{L}{g}} T2π=Lg\frac{T}{2\pi} = \sqrt{\frac{L}{g}} Lg=(T2π)2=(2.52π)2=(0.3979)2=0.1583\frac{L}{g} = \left(\frac{T}{2\pi}\right)^2 = \left(\frac{2.5}{2\pi}\right)^2 = (0.3979)^2 = 0.1583 L=0.1583×9.81=1.55mL = 0.1583 \times 9.81 = 1.55 \mathrm{ m}

If you get this wrong, revise: Simple pendulum period formula and rearranging it to find LL.

Problem 11: Work Done by a Spring

A spring with constant 500N/m500 \mathrm{ N/m} is stretched 0.08m0.08 \mathrm{ m} from its natural length. Find the work done and the elastic potential energy stored.

SolutionW=12kx2=12(500)(0.08)2=12(500)(0.0064)=1.6JW = \frac{1}{2}kx^2 = \frac{1}{2}(500)(0.08)^2 = \frac{1}{2}(500)(0.0064) = 1.6 \mathrm{ J}

The work done equals the elastic potential energy stored: Ep=1.6JE_p = 1.6 \mathrm{ J}.

If you get this wrong, revise: Hooke’s law and work done in stretching a spring.

Problem 12: Power on an Incline

A 60kg60 \mathrm{ kg} person runs up a flight of stairs of vertical height 5m5 \mathrm{ m} in 8s8 \mathrm{ s}. Find the average power developed.

SolutionW=mgh=60×9.81×5=2943JW = mgh = 60 \times 9.81 \times 5 = 2943 \mathrm{ J} P=Wt=29438=367.9WP = \frac{W}{t} = \frac{2943}{8} = 367.9 \mathrm{ W}

If you get this wrong, revise: Work done against gravity and the definition of power.

Problem 13: Vertical Circular Motion, Minimum Speed

A bucket of water of mass 0.8kg0.8 \mathrm{ kg} is whirled in a vertical circle of radius 0.6m0.6 \mathrm{ m}. Find the minimum speed at the top of the circle for the water to remain in the bucket.

Solution

At the top of the circle, the minimum condition is when the normal reaction (or tension) is zero:

mg=mvtop2rmg = \frac{mv_{\mathrm{top}}^2}{r} vtop=gr=9.81×0.6=5.886=2.43m/sv_{\mathrm{top}} = \sqrt{gr} = \sqrt{9.81 \times 0.6} = \sqrt{5.886} = 2.43 \mathrm{ m/s}

If you get this wrong, revise: Vertical circular motion and the minimum speed condition at the top of The circle.

Problem 14: Geostationary Orbit

A geostationary satellite orbits at a distance of 4.23×107m4.23 \times 10^7 \mathrm{ m} from the centre of the Earth. Find its orbital speed and verify that the orbital period is approximately 24 hours. (Earth’s mass =5.97×1024kg= 5.97 \times 10^{24} \mathrm{ kg})

Solutionv=GMr=6.67×10−11×5.97×10244.23×107v = \sqrt{\frac{GM}{r}} = \sqrt{\frac{6.67 \times 10^{-11} \times 5.97 \times 10^{24}}{4.23 \times 10^7}} v=9.41×106=3068m/sv = \sqrt{9.41 \times 10^6} = 3068 \mathrm{ m/s} T=2πrv=2π×4.23×1073068=86600s=24.06hoursT = \frac{2\pi r}{v} = \frac{2\pi \times 4.23 \times 10^7}{3068} = 86600 \mathrm{ s} = 24.06 \mathrm{ hours}

This confirms the geostationary orbit period is approximately 24 hours.

If you get this wrong, revise: Orbital motion, orbital speed, and orbital period formulas.

Problem 15: Energy in SHM, Fraction of KE

A mass-spring system oscillates with amplitude AA. At what displacement is the kinetic energy equal to half the total energy?

SolutionEk=12EtotalE_k = \frac{1}{2}E_{\mathrm{total}} 12mω2(A2−x2)=12×12mω2A2\frac{1}{2}m\omega^2(A^2 - x^2) = \frac{1}{2} \times \frac{1}{2}m\omega^2 A^2 A2−x2=A22A^2 - x^2 = \frac{A^2}{2} x2=A22x^2 = \frac{A^2}{2} x=±A2=±0.707Ax = \pm\frac{A}{\sqrt{2}} = \pm 0.707A

The KE equals half the total energy at x=±0.707Ax = \pm 0.707A from equilibrium.

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

If you get this wrong, revise: Energy exchange in SHM and the expressions for EkE_k and EpE_p as Functions of displacement.