Convert units: nm, mm and cm to m, and check whether angles are measured from the normal.
Check signs and plausibility: a virtual image has dᵢ < 0, an approaching source sounds higher, a closed pipe has only odd harmonics.
2Practice problems
1.KinematicsMedium
A car driving at 90 km/h brakes with a constant deceleration of 5.5 m/s² until it stops. How long does braking take? Find t.
v₀ = 90 km/ha = −5.5 m/s²v = 0
t = s
2.KinematicsHard
A model rocket is launched straight up from rest. Its engine gives it a constant upward acceleration of 20 m/s² for 1.5 s, after which the engine stops and the rocket moves freely. Ignore air resistance and use g = 9.81 m/s². How long after launch does it hit the ground? Find t.
a = 20 m/s²t1 = 1.5 sg = 9.81 m/s²
t = s
3.Newton’s lawsMedium
A 6 kg block slides down a frictionless slope at 45° to the horizontal. Use g = 9.81 m/s². Find the acceleration a of the block along the slope.
m = 6 kgθ = 45°μ = 0g = 9.81 m/s²
a = m/s²
4.Newton’s lawsHard
A 5.5 kg block on a horizontal table is connected by a light string over a frictionless pulley to a hanging 4 kg mass. The coefficient of kinetic friction between block and table is 0.1. Use g = 9.81 m/s². Find the acceleration a of the system.
m1 = 5.5 kgm2 = 4 kgμ = 0.1g = 9.81 m/s²
a = m/s²
5.Projectile motionMedium
A ball is launched at 60° above horizontal from level ground. Ignore air resistance. Find the time of flight t until the ball hits the ground.
v0 = 38 m/sθ = 60°g = 9.81 m/s²
t = s
6.Projectile motionHard
A ball is launched at 60° above horizontal from the top of a 60 m cliff. Ignore air resistance. Find the time of flight t until the ball hits the ground.
v0 = 19 m/sθ = 60°h = 60 mg = 9.81 m/s²
t = s
7.Work & energyMedium
A block slides from rest down a slope at 35° to the horizontal. The coefficient of kinetic friction is 0.2. Find its speed v after it has slid 17 m along the slope.
θ = 35°μ = 0.2d = 17 mg = 9.81 m/s²
v = m/s
8.Work & energyHard
A 15 kg block starts from rest at the bottom of a 35° slope and is pulled up the slope by a constant force of 185 N parallel to the slope. The coefficient of kinetic friction is 0.25. Find the speed v of the block after it has moved 3 m up the slope.
A 1900 kg car moving at 6 m/s runs into a stationary 1800 kg car and the two lock together. How much kinetic energy ΔK is lost in the collision?
m1 = 1900 kgv1 = 6 m/sm2 = 1800 kgv2 = 0
ΔK = J
10.Momentum & collisionsHard
A 1600 kg car runs into a parked 1700 kg car. The wrecks lock together and skid 8 m before stopping. The coefficient of kinetic friction between tyres and road is 0.8. Use g = 9.81 m/s². Find the speed v1 of the first car just before the collision.
A vertical rectangular gate 1.5 m wide sits in the wall of a tank of water, with its top edge 1.5 m below the surface. Find the resultant hydrostatic force F on the gate.
A vertical rectangular gate 3 m wide sits in the wall of a tank of glycerin, with its top edge 2.5 m below the surface. Find the resultant hydrostatic force F on the gate.
Water flows through a horizontal venturi meter with an inlet diameter of 200 mm and a throat diameter of 100 mm. The pressure at the inlet is 58 kPa higher than at the throat. Ignoring losses, find the flow rate Q.
Water flows up through a pipe that narrows from 100 mm to 75 mm while rising 6 m. At section 1 the pressure is 370 kPa and the velocity is 1.75 m/s. Ignoring losses, find the pressure p2 at section 2.
A heat engine receives heat from a source at 850 °C and rejects heat to the surroundings at 25 °C. Its actual thermal efficiency is 44%. Find its second-law efficiency ηII, the ratio of the actual efficiency to the Carnot efficiency.
TH = 850 °CTL = 25 °Cη = 44%
ηII = %
18.Heat engines & refrigeratorsHard
A heat pump keeps a house at 20 °C while it is 2 °C outside, delivering 11 kW of heat to the house. Find the minimum power input Ẇmin.
TH = 20 °CTL = 2 °CQ̇H = 11 kW
Ẇmin = kW
19.Waves, sound & opticsMedium
An object stands 40 cm in front of a thin converging lens with a focal length of 10 cm. Find the image distance di. Use the sign convention 1/f = 1/do + 1/di (f < 0 for a diverging lens, di < 0 for a virtual image).
do = 40 cmf = 10 cm
di = cm
20.Waves, sound & opticsHard
Two thin lenses share an axis, 20 cm apart: lens 1 with f₁ = 20 cm and lens 2 with f₂ = 5 cm. An object stands 12 cm in front of lens 1. Find the position di2 of the final image measured from lens 2 (positive beyond lens 2, real-is-positive convention).
f1 = 20 cmf2 = 5 cms = 20 cmdo = 12 cm
di2 = cm
3Solutions
1.Kinematics
Answer: t = 4.545 s
Motion with constant acceleration: v = v₀ + a·t, s = v₀·t + ½·a·t² and v² = v₀² + 2·a·s. Pick the equation that contains the three things you know and the one you want, and keep the signs consistent with one positive direction.
Units
v₀ = 90/3.6 = 25 m/s
Braking time
0 = v₀ − a·t → t = v₀/a = 25/5.5 = 4.545 s
Answer
t = 4.545 s
2.Kinematics
Answer: t = 8.292 s
Motion with constant acceleration: v = v₀ + a·t, s = v₀·t + ½·a·t² and v² = v₀² + 2·a·s. Pick the equation that contains the three things you know and the one you want, and keep the signs consistent with one positive direction.
Powered phase
v₁ = 20·1.5 = 30 m/s
h₁ = ½·20·1.5² = 22.5 m
Free flight to the ground
Solve −h₁ = v₁·t₂ − ½·g·t₂² for the positive root.
t₂ = (30 + √(30² + 2·9.81·22.5))/9.81 = 6.792 s
t = 1.5 + 6.792 = 8.292 s
Answer
t = 8.292 s
3.Newton’s laws
Answer: a = 6.937 m/s²
Newton’s second law: the net force on a body equals its mass times its acceleration, ΣF = m·a. Draw a free-body diagram, choose a positive direction along the motion, and add every force in that direction: applied forces, friction μ·N against the motion, and the components of gravity.
Newton’s second law: the net force on a body equals its mass times its acceleration, ΣF = m·a. Draw a free-body diagram, choose a positive direction along the motion, and add every force in that direction: applied forces, friction μ·N against the motion, and the components of gravity.
Projectile motion: with no air resistance, x = vxt and y = h + vyt − ½gt². The two directions are independent except that they share the same time.
Split the launch velocity
Horizontal velocity stays constant; vertical motion has a constant acceleration g = 9.81 m/s² downward.
vx = v0·cos θ = 38·cos 60° = 19 m/s
vy = v0·sin θ = 38·sin 60° = 32.91 m/s
Time in the air
Starting and landing at the same height: t = 2vy/g.
t = 2·32.91/9.81 = 6.709 s
Answer
t = 6.709 s
6.Projectile motion
Answer: t = 5.556 s
Projectile motion: with no air resistance, x = vxt and y = h + vyt − ½gt². The two directions are independent except that they share the same time.
Split the launch velocity
Horizontal velocity stays constant; vertical motion has a constant acceleration g = 9.81 m/s² downward.
vx = v0·cos θ = 19·cos 60° = 9.5 m/s
vy = v0·sin θ = 19·sin 60° = 16.45 m/s
Time in the air
Solve y(t) = h + vy·t − ½gt² = 0 for the positive root.
0 = 60 + 16.45·t − 4.905·t²
t = (vy + √(vy² + 2gh))/g = (16.45 + √(270.8 + 1177))/9.81 = 5.556 s
Answer
t = 5.556 s
7.Work & energy
Answer: v = 11.69 m/s
Work–energy principle: the change in kinetic energy equals the work done by all forces. Writing gravity and springs as potential energy (mgh and ½kx²) turns this into a balance: initial energy = final energy + energy lost to friction (μN·d).
Energy balance along the slope
The block drops a height d·sin θ while friction removes μmg·cos θ·d. The mass cancels.
½v² = g·d·(sin θ − μ·cos θ)
v = √(2·9.81·17·(0.5736 − 0.2·0.8192)) = 11.69 m/s
Answer
v = 11.69 m/s
8.Work & energy
Answer: v = 5.309 m/s
Work–energy principle: the change in kinetic energy equals the work done by all forces. Writing gravity and springs as potential energy (mgh and ½kx²) turns this into a balance: initial energy = final energy + energy lost to friction (μN·d).
Forces along the slope
m·g = 15·9.81 = 147.2 N
mg·sin θ = 84.4 N
μ·mg·cos θ = 30.13 N
Work–energy
½mv² = (185 − 114.5)·3 = 211.4 J
v = √(2·211.4/15) = 5.309 m/s
Answer
v = 5.309 m/s
9.Momentum & collisions
Answer: ΔK = 16638 J
Conservation of momentum: when no external force acts during a collision, the total momentum Σm·v before equals the total after. Velocities have a direction, so pick a positive direction and give velocities the other way a minus sign. In an elastic collision kinetic energy is conserved too; in a perfectly inelastic one the bodies stick together.
Common velocity
v′ = m1·v1/(m1 + m2) = 1900·6/3700 = 3.081 m/s
Kinetic energy before and after
Kbefore = ½·1900·6² = 34200 J
Kafter = ½·3700·3.081² = 17562 J
Energy lost
ΔK = 34200 − 17562 = 16638 J
Answer
ΔK = 16638 J
The lost energy goes into deformation, heat and sound.
10.Momentum & collisions
Answer: v1 = 23.11 m/s
Conservation of momentum: when no external force acts during a collision, the total momentum Σm·v before equals the total after. Velocities have a direction, so pick a positive direction and give velocities the other way a minus sign. In an elastic collision kinetic energy is conserved too; in a perfectly inelastic one the bodies stick together.
Hydrostatic force on a plane surface: F = ρ·g·yc·A. It acts at the centre of pressure, ycp = yc + Ic/(ycA), which always lies below the centroid.
Centroid depth and area
yc = d + H/2 = 1.5 + 1.5/2 = 2.25 m
A = H·b = 1.5·1.5 = 2.25 m²
Resultant force
F = ρ·g·yc·A = 1000·9.81·2.25·2.25 = 49.66 kN
Answer
F = 49.66 kN
12.Hydrostatic force
Answer: F = 347.6 kN
Hydrostatic force on a plane surface: F = ρ·g·yc·A. It acts at the centre of pressure, ycp = yc + Ic/(ycA), which always lies below the centroid.
Centroid depth and area
yc = d + H/2 = 2.5 + 2.5/2 = 3.75 m
A = H·b = 2.5·3 = 7.5 m²
Resultant force
F = ρ·g·yc·A = 1260·9.81·3.75·7.5 = 347.6 kN
Answer
F = 347.6 kN
13.Continuity & Bernoulli
Answer: Q = 87.36 L/s
Continuity and Bernoulli: for an incompressible fluid the flow rate is the same at every section, Q = A₁v₁ = A₂v₂. Along a streamline without losses, p + ½ρv² + ρgz is constant, so where the fluid is faster or higher its pressure is lower.
Continuity
v1 = v2·(100/200)² = 0.25·v2
Bernoulli between inlet and throat
The pipe is horizontal, so only pressure and velocity change.
Continuity and Bernoulli: for an incompressible fluid the flow rate is the same at every section, Q = A₁v₁ = A₂v₂. Along a streamline without losses, p + ½ρv² + ρgz is constant, so where the fluid is faster or higher its pressure is lower.
Second-law limits: no cycle working between reservoirs at absolute temperatures TH and TL can beat the reversible (Carnot) cycle: ηmax = 1 − TL/TH, COPR,max = TL/(TH − TL) and COPHP,max = TH/(TH − TL). Energy is always conserved: QH = W + QL.
Absolute temperatures
TH = 850 + 273.15 = 1123 K
TL = 25 + 273.15 = 298.1 K
Carnot efficiency
ηCarnot = 1 − 298.1/1123 = 73.45 %
Second-law efficiency
ηII = η/ηCarnot = 44/73.45 = 59.9 %
Answer
ηII = 59.9 %
18.Heat engines & refrigerators
Answer: Ẇmin = 0.6754 kW
Second-law limits: no cycle working between reservoirs at absolute temperatures TH and TL can beat the reversible (Carnot) cycle: ηmax = 1 − TL/TH, COPR,max = TL/(TH − TL) and COPHP,max = TH/(TH − TL). Energy is always conserved: QH = W + QL.
The least work is needed by a reversible machine, which has the highest COP.
Ẇmin = Q̇H/COP = 11/16.29 = 0.6754 kW
Answer
Ẇmin = 0.6754 kW
19.Waves, sound & optics
Answer: di = 13.33 cm
Geometric optics: at a boundary, n₁·sin θ₁ = n₂·sin θ₂ (Snell's law), with angles measured from the normal and n = c/v. Going into a slower medium the ray bends towards the normal. From a denser medium (n₁ > n₂) beyond the critical angle θc = arcsin(n₂/n₁) all light is reflected: total internal reflection. Thin lenses and spherical mirrors obey 1/f = 1/do + 1/di with the magnification m = −di/do. Sign convention: f > 0 for a converging lens and a concave mirror (f = R/2), f < 0 for a diverging lens and a convex mirror; di > 0 for a real image, di < 0 for a virtual one, and m < 0 for an inverted image.
Thin-lens equation
1/di = 1/f − 1/do = 1/10 − 1/40
di = 13.33 cm
Ray diagram
real, on the far side of the lens
Answer
di = 13.33 cm
20.Waves, sound & optics
Answer: di2 = 5.556 cm
Geometric optics: at a boundary, n₁·sin θ₁ = n₂·sin θ₂ (Snell's law), with angles measured from the normal and n = c/v. Going into a slower medium the ray bends towards the normal. From a denser medium (n₁ > n₂) beyond the critical angle θc = arcsin(n₂/n₁) all light is reflected: total internal reflection. Thin lenses and spherical mirrors obey 1/f = 1/do + 1/di with the magnification m = −di/do. Sign convention: f > 0 for a converging lens and a concave mirror (f = R/2), f < 0 for a diverging lens and a convex mirror; di > 0 for a real image, di < 0 for a virtual one, and m < 0 for an inverted image.