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Momentum

Momentum

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Board Coverage AQA Paper 1 | Edexcel CP2 | OCR (A) Paper 1 | CIE P2

Collision Lab

Explore the simulation above to develop intuition for this topic.

1. Linear Momentum

Definition. The linear momentum of a body of mass mm moving with velocity v\mathbf{v} is:

p=mv\boxed{\mathbf{p} = m\mathbf{v}}

Momentum is a vector quantity with SI units kg m s1^{-1}.

2. Conservation of Momentum

Principle of Conservation of Linear Momentum. In the absence of an external net force, the total momentum of a system is conserved:

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

Proof from Newton's Laws

Consider two bodies AA and BB that interact with each other but with no external forces.

By Newton's third law: FAB=FBA\mathbf{F}_{AB} = -\mathbf{F}_{BA}.

By Newton's second law: FAB=LBdpARB◆◆LBdtRB\mathbf{F}_{AB} = \frac◆LB◆d\mathbf{p}_A◆RB◆◆LB◆dt◆RB◆ and FBA=LBdpBRB◆◆LBdtRB\mathbf{F}_{BA} = \frac◆LB◆d\mathbf{p}_B◆RB◆◆LB◆dt◆RB◆.

Therefore:

LBdpARB◆◆LBdtRB=LBdpBRB◆◆LBdtRB    LBdpARB◆◆LBdtRB+LBdpBRB◆◆LBdtRB=0    ddt(pA+pB)=0\frac◆LB◆d\mathbf{p}_A◆RB◆◆LB◆dt◆RB◆ = -\frac◆LB◆d\mathbf{p}_B◆RB◆◆LB◆dt◆RB◆ \implies \frac◆LB◆d\mathbf{p}_A◆RB◆◆LB◆dt◆RB◆ + \frac◆LB◆d\mathbf{p}_B◆RB◆◆LB◆dt◆RB◆ = 0 \implies \frac{d}{dt}(\mathbf{p}_A + \mathbf{p}_B) = 0

Hence pA+pB=constant\mathbf{p}_A + \mathbf{p}_B = \mathrm{constant}. \square

Intuition. Momentum conservation is more fundamental than energy conservation in collisions because it holds for all types of collisions — elastic, inelastic, and explosive. Kinetic energy is only conserved in elastic collisions.

3. Impulse

Definition. The impulse JJ delivered by a force F\mathbf{F} acting over a time interval Δt\Delta t is:

J=FΔt=Δp\boxed{\mathbf{J} = \mathbf{F}\Delta t = \Delta\mathbf{p}}

For a variable force:

J=t1t2F(t)dt\mathbf{J} = \int_{t_1}^{t_2} \mathbf{F}(t)\,dt

Derivation from Newton's second law.

F=LBdpRB◆◆LBdtRB    Fdt=dp    Fdt=dp=Δp\mathbf{F} = \frac◆LB◆d\mathbf{p}◆RB◆◆LB◆dt◆RB◆ \implies \mathbf{F}\,dt = d\mathbf{p} \implies \int \mathbf{F}\,dt = \int d\mathbf{p} = \Delta\mathbf{p}

\square

Units. Impulse has units N s, which are equivalent to kg m s1^{-1} (the same as momentum).

Intuition. Impulse explains why airbags save lives. The change in momentum Δp\Delta p is fixed (car stops, so pp goes from mvmv to 0). The airbag increases Δt\Delta t, so the force F=Δp/ΔtF = \Delta p / \Delta t is reduced.

4. Collisions

Coefficient of Restitution

Definition. The coefficient of restitution ee measures the elasticity of a collision:

e=v1v2u1u2\boxed{e = -\frac{v_1 - v_2}{u_1 - u_2}}

where u1,u2u_1, u_2 are the velocities before collision and v1,v2v_1, v_2 are the velocities after collision, measured along the line of impact.

Derivation. For a collision between two bodies, Newton's experimental law of restitution states that the relative speed of separation equals ee times the relative speed of approach. Since the bodies separate after collision (v2>v1v_2 > v_1 if body 2 was struck), and approached before (u1>u2u_1 > u_2), the minus sign ensures e>0e > 0.

  • Perfectly elastic collision: e=1e = 1 (kinetic energy is conserved)
  • Perfectly inelastic collision: e=0e = 0 (bodies coalesce — maximum KE loss)
  • Inelastic collision: 0<e<10 < e < 1

1D Elastic Collision: Final Velocities

For two bodies of masses m1m_1 and m2m_2 with initial velocities u1u_1 and u2u_2:

Conservation of momentum:

m1u1+m2u2=m1v1+m2v2...(i)m_1 u_1 + m_2 u_2 = m_1 v_1 + m_2 v_2 \quad \mathrm{...(i)}

Conservation of kinetic energy (elastic, e=1e = 1):

12m1u12+12m2u22=12m1v12+12m2v22...(ii)\frac{1}{2}m_1 u_1^2 + \frac{1}{2}m_2 u_2^2 = \frac{1}{2}m_1 v_1^2 + \frac{1}{2}m_2 v_2^2 \quad \mathrm{...(ii)}

From (i): m1(u1v1)=m2(v2u2)m_1(u_1 - v_1) = m_2(v_2 - u_2) ... (iii)

From (ii): m1(u12v12)=m2(v22u22)m_1(u_1^2 - v_1^2) = m_2(v_2^2 - u_2^2) ... (iv)

Dividing (iv) by (iii):

u1+v1=u2+v2    v1v2=(u1u2)(Newtonsrestitutionwithe=1)u_1 + v_1 = u_2 + v_2 \implies v_1 - v_2 = -(u_1 - u_2) \quad \mathrm{(Newton's restitution with } e = 1\mathrm{)}

From v1=u2+v2u1v_1 = u_2 + v_2 - u_1, substituting into (i):

m1u1+m2u2=m1(u2+v2u1)+m2v2m_1 u_1 + m_2 u_2 = m_1(u_2 + v_2 - u_1) + m_2 v_2

m1u1+m2u2=m1u2+m1v2m1u1+m2v2m_1 u_1 + m_2 u_2 = m_1 u_2 + m_1 v_2 - m_1 u_1 + m_2 v_2

2m1u1+(m2m1)u2=(m1+m2)v22m_1 u_1 + (m_2 - m_1)u_2 = (m_1 + m_2)v_2

v2=(m2m1)u2+2m1u1m1+m2\boxed{v_2 = \frac{(m_2 - m_1)u_2 + 2m_1 u_1}{m_1 + m_2}}

By symmetry:

v1=(m1m2)u1+2m2u2m1+m2\boxed{v_1 = \frac{(m_1 - m_2)u_1 + 2m_2 u_2}{m_1 + m_2}}

Special Cases

Equal masses (m1=m2m_1 = m_2): v1=u2v_1 = u_2 and v2=u1v_2 = u_1. The bodies exchange velocities.

Stationary target (u2=0u_2 = 0):

v1=(m1m2)u1m1+m2,v2=2m1u1m1+m2v_1 = \frac{(m_1 - m_2)u_1}{m_1 + m_2}, \qquad v_2 = \frac{2m_1 u_1}{m_1 + m_2}

Heavy stationary target (m2m1m_2 \gg m_1): v1u1v_1 \approx -u_1 (light body rebounds), v20v_2 \approx 0 (heavy body barely moves).

Light stationary target (m2m1m_2 \ll m_1): v1u1v_1 \approx u_1 (heavy body continues), v22u1v_2 \approx 2u_1 (light body moves at twice the speed).

Inelastic Collision

For a perfectly inelastic collision (e=0e = 0), the bodies coalesce. Let the common final velocity be vv:

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

v=m1u1+m2u2m1+m2\boxed{v = \frac{m_1 u_1 + m_2 u_2}{m_1 + m_2}}

Kinetic energy lost:

ΔEk=12m1u12+12m2u2212(m1+m2)v2\Delta E_k = \frac{1}{2}m_1 u_1^2 + \frac{1}{2}m_2 u_2^2 - \frac{1}{2}(m_1 + m_2)v^2

=m1m22(m1+m2)(u1u2)2= \frac{m_1 m_2}{2(m_1 + m_2)}(u_1 - u_2)^2

Note that the energy loss depends on the relative velocity — a faster approach means more energy is dissipated.

5. 2D Collisions

In two dimensions, momentum conservation applies separately in each direction:

pxbefore=pxafter,pybefore=pyafter\sum p_x^{\mathrm{before}} = \sum p_x^{\mathrm{after}}, \qquad \sum p_y^{\mathrm{before}} = \sum p_y^{\mathrm{after}}

For an elastic collision, we also conserve kinetic energy. The coefficient of restitution applies along the line of centres.

Details

Example: 2D Collision A particle of mass 2m2m moving with speed uu collides with a stationary particle of mass mm. After the collision, the 2m2m particle moves at 6060^\circ to its original direction. Find the final speeds (elastic collision).

Answer. Let the original direction be the xx-axis.

Momentum conservation (xx): 2mu=2mv1cos60°+mv2cosθ2mu = 2mv_1\cos 60° + mv_2\cos\theta, i.e., 2u=v1+v2cosθ2u = v_1 + v_2\cos\theta.

Momentum conservation (yy): 0=2mv1sin60°mv2sinθ0 = 2mv_1\sin 60° - mv_2\sin\theta, i.e., v2sinθ=v13v_2\sin\theta = v_1\sqrt{3}.

KE conservation: 2mu2=2mv12+mv222mu^2 = 2mv_1^2 + mv_2^2, i.e., 2u2=2v12+v222u^2 = 2v_1^2 + v_2^2.

From the xx-momentum: v2cosθ=2uv1v_2\cos\theta = 2u - v_1. Squaring and adding the yy-equation: v22=(2uv1)2+3v12=4u24uv1+4v12v_2^2 = (2u - v_1)^2 + 3v_1^2 = 4u^2 - 4uv_1 + 4v_1^2.

Substituting into KE: 2u2=2v12+4u24uv1+4v122u^2 = 2v_1^2 + 4u^2 - 4uv_1 + 4v_1^2, i.e., 6v124uv1+2u2=06v_1^2 - 4uv_1 + 2u^2 = 0, i.e., 3v122uv1+u2=03v_1^2 - 2uv_1 + u^2 = 0, i.e., (v1u)(3v1u)=0(v_1 - u)(3v_1 - u) = 0.

Since v1uv_1 \neq u (the particle deflects), v1=u/3v_1 = u/3. Then v22=4u24u2/3+4u2/9=3612+49u2=289u2v_2^2 = 4u^2 - 4u^2/3 + 4u^2/9 = \frac{36 - 12 + 4}{9}u^2 = \frac{28}{9}u^2, so v2=LB27RB◆◆LB3RBuv_2 = \frac◆LB◆2\sqrt{7}◆RB◆◆LB◆3◆RB◆u.

6. Force-Time Graphs

The area under a force-time graph equals the impulse, which equals the change in momentum.

For a collision, the force typically rises rapidly, peaks, and falls. A larger maximum force corresponds to a shorter collision time (for the same impulse).

Problem Set

Details

Problem 1 A 15001500 kg car travelling at 2020 m s1^{-1} collides head-on with a 10001000 kg car travelling at 1515 m s1^{-1} in the opposite direction. If they stick together, find the common velocity and the kinetic energy lost.

Answer. Taking the direction of the first car as positive: pi=1500(20)+1000(15)=3000015000=15000p_i = 1500(20) + 1000(-15) = 30000 - 15000 = 15000 kg m s1^{-1}.

v=150002500=6.0v = \frac{15000}{2500} = 6.0 m s1^{-1} (in the original direction of the first car).

KE lost: ΔEk=m1m22(m1+m2)(u1u2)2=LB1500×1000RB◆◆LB2×2500RB(20(35))2=300×1225=367500\Delta E_k = \frac{m_1 m_2}{2(m_1+m_2)}(u_1 - u_2)^2 = \frac◆LB◆1500 \times 1000◆RB◆◆LB◆2 \times 2500◆RB◆(20-(-35))^2 = 300 \times 1225 = 367\,500 J.

If you get this wrong, revise: Inelastic Collision

Details

Problem 2 A ball of mass 0.150.15 kg hits a wall normally at 1212 m s1^{-1} and rebounds at 8.08.0 m s1^{-1}. Calculate: (a) the impulse, (b) the average force if contact lasts 0.0400.040 s.

Answer. (a) Taking away from the wall as positive: J=Δp=m(vu)=0.15(8(12))=0.15×20=3.0J = \Delta p = m(v - u) = 0.15(8 - (-12)) = 0.15 \times 20 = 3.0 N s (away from wall).

(b) F=J/Δt=3.0/0.040=75F = J/\Delta t = 3.0/0.040 = 75 N.

If you get this wrong, revise: Impulse

Details

Problem 3 In a nuclear reactor, a neutron of mass mm travelling at vv collides elastically with a stationary carbon nucleus of mass 12m12m. What fraction of the neutron's kinetic energy is transferred to the carbon nucleus?

Answer. v2=2m1u1m1+m2=LB2mvRB◆◆LBm+12mRB=2v13v_2 = \frac{2m_1 u_1}{m_1 + m_2} = \frac◆LB◆2m \cdot v◆RB◆◆LB◆m + 12m◆RB◆ = \frac{2v}{13}.

KE of carbon = 12(12m)(2v13)2=12(12m)4v2169=48mv2338\frac{1}{2}(12m)\left(\frac{2v}{13}\right)^2 = \frac{1}{2}(12m)\frac{4v^2}{169} = \frac{48mv^2}{338}.

Initial KE = 12mv2\frac{1}{2}mv^2. Fraction transferred = 48/3381/2=48169=48169=0.284=28.4%\frac{48/338}{1/2} = \frac{48}{169} = \frac{48}{169} = 0.284 = 28.4\%.

If you get this wrong, revise: 1D Elastic Collision: Final Velocities

Details

Problem 4 A cricket ball of mass 0.160.16 kg is bowled at 3535 m s1^{-1} and hit straight back at 4040 m s1^{-1}. Contact time is 0.0010.001 s. Find the average force exerted by the bat.

Answer. Taking the direction of the hit as positive: J=0.16(40(35))=0.16×75=12J = 0.16(40 - (-35)) = 0.16 \times 75 = 12 N s. F=12/0.001=12000F = 12/0.001 = 12\,000 N =12= 12 kN.

If you get this wrong, revise: Impulse

Details

Problem 5 Two identical particles collide. One is at rest and the other has velocity u\mathbf{u}. After an elastic collision, the first particle moves at 3030^\circ to u\mathbf{u}. Find the direction of the second particle and the final speeds.

Answer. By conservation of momentum (equal masses in elastic collision), the particles move at right angles to each other after collision. So the second particle moves at 6060^\circ to u\mathbf{u}.

By symmetry and KE conservation: both have speed ucos60°=u/2u\cos 60° = u/2... No, let me be more careful.

Momentum (xx): mu=mv1cos30°+mv2cos60mu = mv_1\cos 30° + mv_2\cos 60^\circ, i.e., u=LB3RB◆◆LB2RBv1+12v2u = \frac◆LB◆\sqrt{3}◆RB◆◆LB◆2◆RB◆v_1 + \frac{1}{2}v_2.

Momentum (yy): 0=mv1sin30°mv2sin600 = mv_1\sin 30° - mv_2\sin 60^\circ, i.e., v1=3v2v_1 = \sqrt{3}\,v_2.

Substituting: u=LB3RB◆◆LB2RB(3v2)+v22=3v22+v22=2v2u = \frac◆LB◆\sqrt{3}◆RB◆◆LB◆2◆RB◆(\sqrt{3}v_2) + \frac{v_2}{2} = \frac{3v_2}{2} + \frac{v_2}{2} = 2v_2. So v2=u/2v_2 = u/2 and v1=3u/2v_1 = \sqrt{3}u/2.

If you get this wrong, revise: 2D Collisions

Details

Problem 6 Prove that kinetic energy is not conserved in a perfectly inelastic collision between two bodies, using the general result for energy loss.

Answer. For e=0e = 0, the common velocity is v=(m1u1+m2u2)/(m1+m2)v = (m_1 u_1 + m_2 u_2)/(m_1 + m_2). The KE loss is ΔEk=m1m22(m1+m2)(u1u2)2\Delta E_k = \frac{m_1 m_2}{2(m_1+m_2)}(u_1 - u_2)^2. This is zero only if u1=u2u_1 = u_2 (no collision). For any actual collision (u1u2u_1 \neq u_2), ΔEk>0\Delta E_k > 0, so KE is not conserved. \square

If you get this wrong, revise: Inelastic Collision

Details

Problem 7 A 6060 kg astronaut floating in space throws a 2.02.0 kg tool at 8.08.0 m s1^{-1}. What is the astronaut's recoil velocity?

Answer. By conservation of momentum: 0=mava+mtvt0 = m_a v_a + m_t v_t. va=mtvtma=LB2.0×8.0RB◆◆LB60RB=0.267v_a = -\frac{m_t v_t}{m_a} = -\frac◆LB◆2.0 \times 8.0◆RB◆◆LB◆60◆RB◆ = -0.267 m s1^{-1} (opposite to the throw).

If you get this wrong, revise: Conservation of Momentum

Details

Problem 8 A 0.500.50 kg ball falls vertically from height 5.05.0 m onto a concrete floor and rebounds to height 3.23.2 m. Find the coefficient of restitution between the ball and the floor.

Answer. Speed just before impact: v1=LB2g×5.0RB=98.1=9.90v_1 = \sqrt◆LB◆2g \times 5.0◆RB◆ = \sqrt{98.1} = 9.90 m s1^{-1} (downward, so u1=9.90u_1 = -9.90).

Speed just after impact: v2=LB2g×3.2RB=62.78=7.92v_2 = \sqrt◆LB◆2g \times 3.2◆RB◆ = \sqrt{62.78} = 7.92 m s1^{-1} (upward).

The floor has infinite mass, so e=LBvseparationRB◆◆LBvapproachRB=7.929.90=0.80e = \frac◆LB◆v_{\mathrm{separation}}◆RB◆◆LB◆v_{\mathrm{approach}}◆RB◆ = \frac{7.92}{9.90} = 0.80.

If you get this wrong, revise: Coefficient of Restitution

Details

Problem 9 A 3.03.0 kg body moving at 4.04.0 m s1^{-1} collides with a 5.05.0 kg body moving at 2.02.0 m s1^{-1} in the same direction. The coefficient of restitution is 0.60.6. Find the velocities after the collision.

Answer. Momentum: 3(4)+5(2)=3v1+5v23(4) + 5(2) = 3v_1 + 5v_2, i.e., 22=3v1+5v222 = 3v_1 + 5v_2 ... (i).

Restitution: 0.6=v1v242=v1v220.6 = -\frac{v_1 - v_2}{4 - 2} = -\frac{v_1 - v_2}{2}, so v1v2=1.2v_1 - v_2 = -1.2 ... (ii).

From (ii): v1=v21.2v_1 = v_2 - 1.2. Substituting into (i): 22=3(v21.2)+5v2=8v23.622 = 3(v_2 - 1.2) + 5v_2 = 8v_2 - 3.6. v2=25.6/8=3.2v_2 = 25.6/8 = 3.2 m s1^{-1}. v1=3.21.2=2.0v_1 = 3.2 - 1.2 = 2.0 m s1^{-1}.

If you get this wrong, revise: Coefficient of Restitution

Details

Problem 10 Two trolleys approach each other on a frictionless track. Trolley A (2.02.0 kg) moves at 3.03.0 m s1^{-1} to the right, trolley B (3.03.0 kg) moves at 2.02.0 m s1^{-1} to the left. They collide elastically. Find their final velocities.

Answer. Taking right as positive: u1=3.0u_1 = 3.0, u2=2.0u_2 = -2.0.

v1=(23)(3)+2(3)(2)2+3=3125=3.0v_1 = \frac{(2-3)(3) + 2(3)(-2)}{2+3} = \frac{-3 - 12}{5} = -3.0 m s1^{-1}.

v2=(32)(2)+2(2)(3)5=2+125=2.0v_2 = \frac{(3-2)(-2) + 2(2)(3)}{5} = \frac{-2 + 12}{5} = 2.0 m s1^{-1}.

The bodies exchange their original speeds (approximately — this is because the masses are close).

If you get this wrong, revise: 1D Elastic Collision: Final Velocities

Details

Problem 11 Explain, using momentum conservation, why a gun recoils when fired, and calculate the recoil velocity of a 2.02.0 kg rifle that fires a 1010 g bullet at 400400 m s1^{-1}.

Answer. Before firing, total momentum is zero (both at rest). After firing, the bullet moves forward with momentum pb=0.010×400=4.0p_b = 0.010 \times 400 = 4.0 kg m s1^{-1}. By conservation: prifle=4.0p_{\mathrm{rifle}} = -4.0 kg m s1^{-1}, so vr=4.0/2.0=2.0v_r = -4.0/2.0 = -2.0 m s1^{-1}.

If you get this wrong, revise: Conservation of Momentum

7. Impulse in 2D

Definition. In two dimensions, impulse is a vector quantity:

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

Resolving into components:

Jx=Δpx=FxΔt,Jy=Δpy=FyΔtJ_x = \Delta p_x = F_x\,\Delta t, \qquad J_y = \Delta p_y = F_y\,\Delta t

J=Jx2+Jy2|\mathbf{J}| = \sqrt{J_x^2 + J_y^2}

When a ball strikes a smooth wall, only the component of momentum perpendicular to the wall changes. The parallel component is unchanged because the wall exerts no force parallel to its surface.

tip

Exam Technique For a ball hitting a smooth wall at angle α\alpha to the normal with speed uu and rebounding with the normal component reduced by factor ee: the impulse is J=m(1+e)ucosαJ = m(1+e)u\cos\alpha perpendicular to the wall, and the rebound angle β\beta satisfies tanβ=LBusinαRB◆◆LBeucosαRB=LBtanαRB◆◆LBeRB\tan\beta = \frac◆LB◆u\sin\alpha◆RB◆◆LB◆eu\cos\alpha◆RB◆ = \frac◆LB◆\tan\alpha◆RB◆◆LB◆e◆RB◆, which is greater than α\alpha when e<1e \lt 1.

Details

Example: Ball Hitting a Wall at an Angle A ball of mass 0.200.20 kg hits a smooth vertical wall at 3030^\circ to the normal with speed 8.08.0 m s1^{-1}. The coefficient of restitution is 0.750.75. Find: (a) the impulse exerted by the wall, (b) the speed and direction of the ball after impact.

Answer. Take the xx-axis perpendicular to the wall (positive away from wall) and the yy-axis parallel to the wall.

Before impact: ux=8.0cos30°=6.93u_x = -8.0\cos 30° = -6.93 m s1^{-1} (towards wall) uy=8.0sin30°=4.00u_y = 8.0\sin 30° = 4.00 m s1^{-1} (parallel to wall)

After impact (smooth wall, so uyu_y unchanged; normal component reverses with restitution): vx=+0.75×6.93=+5.20v_x = +0.75 \times 6.93 = +5.20 m s1^{-1} (away from wall) vy=4.00v_y = 4.00 m s1^{-1} (unchanged)

(a) Jx=m(vxux)=0.20(5.20(6.93))=0.20×12.13=2.43J_x = m(v_x - u_x) = 0.20(5.20 - (-6.93)) = 0.20 \times 12.13 = 2.43 N s. Jy=0J_y = 0 (smooth wall).

The impulse is 2.432.43 N s perpendicular to the wall, directed away from the wall.

(b) Speed: v=vx2+vy2=5.202+4.002=27.04+16.00=43.04=6.56v = \sqrt{v_x^2 + v_y^2} = \sqrt{5.20^2 + 4.00^2} = \sqrt{27.04 + 16.00} = \sqrt{43.04} = 6.56 m s1^{-1}.

Angle to normal: tanβ=vy/vx=4.00/5.20=0.769\tan\beta = v_y/v_x = 4.00/5.20 = 0.769, so β=37.6\beta = 37.6^\circ.

The rebound angle (37.637.6^\circ) is greater than the approach angle (3030^\circ), as expected when e<1e \lt 1.

8. Coefficient of Restitution -- Relative Velocity Form

Definition. The coefficient of restitution can be expressed in terms of relative velocities:

e=LBrelativespeedofseparationRB◆◆LBrelativespeedofapproachRB\boxed{e = \frac◆LB◆|\mathrm{relative speed of separation}|◆RB◆◆LB◆|\mathrm{relative speed of approach}|◆RB◆}

Derivation for a 1D Collision

Consider two bodies with masses m1m_1 and m2m_2. Before collision they move with velocities u1u_1 and u2u_2; after collision their velocities are v1v_1 and v2v_2.

Relative speed of approach. The speed at which the bodies approach each other is u1u2|u_1 - u_2|.

Relative speed of separation. The speed at which the bodies move apart after collision is v2v1|v_2 - v_1|.

Newton's law of restitution states:

e=LBv2v1RB◆◆LBu1u2RBe = \frac◆LB◆|v_2 - v_1|◆RB◆◆LB◆|u_1 - u_2|◆RB◆

If body 1 catches up to body 2 (u1>u2u_1 \gt u_2) and they separate after collision (v2>v1v_2 \gt v_1), then:

e=v2v1u1u2e = \frac{v_2 - v_1}{u_1 - u_2}

This is algebraically equivalent to the form e=v1v2u1u2e = -\dfrac{v_1 - v_2}{u_1 - u_2} given in Section 4. \square

Intuition. The relative velocity form shows that ee is a property of the collision itself (the materials involved), not of the individual bodies. For a perfectly elastic collision (e=1e = 1), the relative speed is unchanged -- the bodies bounce off each other just as fast as they approached.

warning

warning line joining the centres of the two bodies at the moment of impact). In oblique collisions, only the components along this line are used in the restitution equation. The perpendicular components are governed by the smoothness of the surfaces.

9. Bouncing Ball: Proof that e=h/he = \sqrt{h'/h}

Theorem. For a ball dropped from height hh onto a hard floor, rebounding to height hh', the coefficient of restitution satisfies e=h/he = \sqrt{h'/h}.

Proof (energy method). The ball falls from height hh under gravity. By conservation of energy:

mgh=12mu2    u=2ghmgh = \tfrac{1}{2}mu^2 \implies u = \sqrt{2gh}

where uu is the speed just before impact (downward).

After impact, the ball rises to height hh'. By conservation of energy:

12mv2=mgh    v=2gh\tfrac{1}{2}mv^2 = mgh' \implies v = \sqrt{2gh'}

where vv is the speed just after impact (upward).

The floor has effectively infinite mass and does not move, so the relative speed of approach is uu and the relative speed of separation is vv:

e=vu=LB2ghRB◆◆LB2ghRB=LBhhRBe = \frac{v}{u} = \frac◆LB◆\sqrt{2gh'}◆RB◆◆LB◆\sqrt{2gh}◆RB◆ = \sqrt◆LB◆\frac{h'}{h}◆RB◆

\square

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Exam Technique This result provides a quick experimental method to determine ee: drop a ball from a known height, measure the rebound height, and compute e=h/he = \sqrt{h'/h}. This is often tested in practical exams. For successive bounces, the heights form a geometric sequence: h, e2h, e4h, h,\ e^2h,\ e^4h,\ \ldots

10. Explosions and Rocket Propulsion

Explosions

Intuition. In an explosion, a body at rest (or moving) breaks into fragments due to internal forces. Since internal forces come in equal and opposite pairs (Newton's third law), the total external force on the system is zero and momentum is conserved.

If a body of mass MM at rest explodes into two fragments of masses m1m_1 and m2m_2:

0=m1v1+m2v20 = m_1\mathbf{v}_1 + m_2\mathbf{v}_2

The fragments move in opposite directions with speeds inversely proportional to their masses:

LBv1RB◆◆LBv2RB=m2m1\frac◆LB◆|\mathbf{v}_1|◆RB◆◆LB◆|\mathbf{v}_2|◆RB◆ = \frac{m_2}{m_1}

Kinetic energy in an explosion. KE increases as chemical (or nuclear) energy is converted to KE of fragments:

ΔEk=12m1v12+12m2v220\Delta E_k = \tfrac{1}{2}m_1v_1^2 + \tfrac{1}{2}m_2v_2^2 - 0

Since m1v1=m2v2=pm_1v_1 = m_2v_2 = p (momentum conservation):

ΔEk=p22m1+p22m2=Mp22m1m2\Delta E_k = \frac{p^2}{2m_1} + \frac{p^2}{2m_2} = \frac{M\,p^2}{2m_1 m_2}

Rocket Propulsion

Intuition. A rocket moves forward by ejecting exhaust gases backward. The rocket does not "push against" the air or the ground -- it works in vacuum by momentum conservation.

Consider a rocket of mass mm moving at velocity vv. In time dtdt, it ejects fuel of mass dmdm at exhaust velocity uu relative to the rocket. The absolute velocity of the exhaust is vuv - u.

Momentum conservation (no external forces):

mv=(mdm)(v+dv)+dm(vu)m\,v = (m - dm)(v + dv) + dm\,(v - u)

Expanding and neglecting dmdvdm\,dv:

mv=mv+mdvvdmdmdv+vdmudmmv = mv + m\,dv - v\,dm - dm\,dv + v\,dm - u\,dm

0=mdvudm0 = m\,dv - u\,dm

mdv=udm\boxed{m\,dv = -u\,dm}

This is the rocket equation (Tsiolkovsky equation in differential form). Since dm<0dm \lt 0 (the rocket loses mass), dv>0dv \gt 0 (the rocket accelerates).

Integrating from initial mass m0m_0 to final mass mfm_f:

0Δvdv=um0mfdmm\int_0^{\Delta v} dv = -u\int_{m_0}^{m_f}\frac{dm}{m}

Δv=uln(m0mf)\Delta v = u\ln\left(\frac{m_0}{m_f}\right)

Intuition. The rocket equation shows that Δv\Delta v depends on exhaust velocity uu and mass ratio m0/mfm_0/m_f. This is why multi-stage rockets are used -- dropping empty stages reduces mfm_f without reducing m0m_0.

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Board Coverage AQA: Momentum conservation in explosions is required; the rocket equation is extension material. Edexcel CP2: Explosions appear in the momentum topic; the rocket equation is not explicitly required but may appear in context. OCR (A): Explosions are core; rocket propulsion is stretch material. CIE P2: Explosions are required; the rocket equation occasionally appears as a challenging problem.

Further Problems

Details

Problem 12 A 5.05.0 kg object at rest explodes into three fragments. Fragment A (2.02.0 kg) moves at 1212 m s1^{-1} due north, and fragment B (1.51.5 kg) moves at 8.08.0 m s1^{-1} due east. Find the velocity of fragment C.

Answer. By conservation of momentum, the total momentum before the explosion is zero, so the vector sum of the momenta after must also be zero.

pA=2.0×12=24p_A = 2.0 \times 12 = 24 kg m s1^{-1} (north) pB=1.5×8.0=12p_B = 1.5 \times 8.0 = 12 kg m s1^{-1} (east)

pC=(pA+pB)p_C = -(p_A + p_B). Resolving into components (taking east as +x+x, north as +y+y):

pCx=12p_{Cx} = -12 kg m s1^{-1} (west), pCy=24p_{Cy} = -24 kg m s1^{-1} (south).

mC=5.02.01.5=1.5m_C = 5.0 - 2.0 - 1.5 = 1.5 kg.

vC=(12/1.5)2+(24/1.5)2=64+256=320=17.9v_C = \sqrt{(-12/1.5)^2 + (-24/1.5)^2} = \sqrt{64 + 256} = \sqrt{320} = 17.9 m s1^{-1}.

Direction: tanθ=24/12=2.0\tan\theta = 24/12 = 2.0, so θ=63.4\theta = 63.4^\circ south of west.

If you get this wrong, revise: Explosions and Rocket Propulsion

Details

Problem 13 A ball of mass 0.100.10 kg is projected at 2020^\circ to the vertical towards a smooth vertical wall with speed 1010 m s1^{-1}. The coefficient of restitution between the ball and the wall is 0.600.60. Find the impulse exerted by the wall and the speed of the ball after impact.

Answer. Let the xx-axis be perpendicular to the wall (positive away from wall). The angle to the normal is 2020^\circ.

Before: ux=10cos20°=9.40u_x = -10\cos 20° = -9.40 m s1^{-1}, uy=10sin20°=3.42u_y = 10\sin 20° = 3.42 m s1^{-1}.

After (smooth wall): vx=+0.60×9.40=+5.64v_x = +0.60 \times 9.40 = +5.64 m s1^{-1}, vy=3.42v_y = 3.42 m s1^{-1}.

Impulse: Jx=0.10(5.64(9.40))=0.10×15.04=1.50J_x = 0.10(5.64 - (-9.40)) = 0.10 \times 15.04 = 1.50 N s away from the wall. Jy=0J_y = 0.

Speed after: v=5.642+3.422=31.8+11.7=43.5=6.60v = \sqrt{5.64^2 + 3.42^2} = \sqrt{31.8 + 11.7} = \sqrt{43.5} = 6.60 m s1^{-1}.

If you get this wrong, revise: Impulse in 2D

Details

Problem 14 A particle falls from height HH and bounces on a hard floor with coefficient of restitution ee. Show that the total vertical distance travelled before the particle comes to rest is 1+e21e2H\dfrac{1+e^2}{1-e^2}\,H.

Answer. The particle falls HH, rises to e2He^2H, falls e2He^2H, rises to e4He^4H, and so on.

Total distance d=H+2e2H+2e4H+2e6H+d = H + 2e^2H + 2e^4H + 2e^6H + \cdots

d=H+2e2H(1+e2+e4+)d = H + 2e^2H(1 + e^2 + e^4 + \cdots)

The bracketed series converges to 11e2\frac{1}{1-e^2} for 0e<10 \leq e \lt 1:

d=H+2e2H1e2=H(1e2)+2e2H1e2=H(1+e2)1e2d = H + \frac{2e^2H}{1-e^2} = \frac{H(1-e^2) + 2e^2H}{1-e^2} = \frac{H(1+e^2)}{1-e^2}

\square

If you get this wrong, revise: Bouncing Ball: Proof that e=h/he = \sqrt{h'/h}

Details

Problem 15 Two bodies of masses 3.03.0 kg and 5.05.0 kg collide. Before the collision, the 3.03.0 kg body moves at 6.06.0 m s1^{-1} and the 5.05.0 kg body moves at 2.02.0 m s1^{-1} in the opposite direction. After the collision, the 3.03.0 kg body moves at 1.01.0 m s1^{-1} in its original direction. Find: (a) the velocity of the 5.05.0 kg body after the collision, (b) the coefficient of restitution, (c) the kinetic energy lost.

Answer. Taking the direction of the 3.03.0 kg body as positive.

(a) Momentum conservation: 3.0(6.0)+5.0(2.0)=3.0(1.0)+5.0v23.0(6.0) + 5.0(-2.0) = 3.0(1.0) + 5.0v_2.

1810=3+5v218 - 10 = 3 + 5v_2, so 5v2=55v_2 = 5, giving v2=1.0v_2 = 1.0 m s1^{-1} (in the original direction of the 3.03.0 kg body).

(b) e=v2v1u1u2=1.01.06.0(2.0)=08.0=0e = \frac{v_2 - v_1}{u_1 - u_2} = \frac{1.0 - 1.0}{6.0 - (-2.0)} = \frac{0}{8.0} = 0.

The collision is perfectly inelastic (but the bodies do not coalesce -- they happen to have the same final velocity).

(c) Initial KE =12(3)(36)+12(5)(4)=54+10=64= \tfrac{1}{2}(3)(36) + \tfrac{1}{2}(5)(4) = 54 + 10 = 64 J.

Final KE =12(3)(1)+12(5)(1)=1.5+2.5=4.0= \tfrac{1}{2}(3)(1) + \tfrac{1}{2}(5)(1) = 1.5 + 2.5 = 4.0 J.

KE lost =644=60= 64 - 4 = 60 J.

If you get this wrong, revise: Coefficient of Restitution -- Relative Velocity Form

Details

Problem 16 A rocket of initial mass 10001000 kg (including 800800 kg of fuel) burns fuel at a constant rate, ejecting exhaust at 20002000 m s1^{-1} relative to the rocket. Find the rocket's velocity when all the fuel is exhausted, neglecting gravity and air resistance.

Answer. m0=1000m_0 = 1000 kg, mf=1000800=200m_f = 1000 - 800 = 200 kg, u=2000u = 2000 m s1^{-1}.

Δv=uln(m0/mf)=2000ln(1000/200)=2000ln5=2000×1.609=3219\Delta v = u\ln(m_0/m_f) = 2000\ln(1000/200) = 2000\ln 5 = 2000 \times 1.609 = 3219 m s1^{-1}.

If you get this wrong, revise: Rocket Propulsion


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Diagnostic Test Ready to test your understanding of Momentum? The diagnostic test contains the hardest questions within the A-Level specification for this topic, each with a full worked solution.

Unit tests probe edge cases and common misconceptions. Integration tests combine Momentum with other physics topics to test synthesis under exam conditions.

See Diagnostic Guide for instructions on self-marking and building a personal test matrix.

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Common Pitfalls

  • Confusing momentum and kinetic energy in collisions: Momentum is always conserved in a collision (if no external forces). Kinetic energy is only conserved in PERFECTLY ELASTIC collisions. In inelastic collisions, kinetic energy is lost (converted to heat, sound, deformation) but momentum is still conserved. Never assume a collision is elastic unless told so.

  • Forgetting that momentum is a vector: When solving 2D collision problems, momentum must be conserved separately in each direction (x and y). A common error is to add momentum magnitudes without considering direction. Two objects of equal mass moving at equal speeds in opposite directions have a total momentum of ZERO.

  • Assuming impulse only changes the faster object's momentum: In a collision, both objects experience equal and opposite impulses (Newton's third law). The change in momentum of object A is equal in magnitude and opposite in direction to the change in momentum of object B, regardless of their relative masses or speeds.

  • Misapplying the coefficient of restitution: The coefficient of restitution e relates the RELATIVE speed of separation to the RELATIVE speed of approach: e = (v2 - v1) / (u1 - u2). Note the order of subtraction -- the sign matters. For a perfectly elastic collision e = 1, for perfectly inelastic e = 0.