Level 3 — ProductionMomentum & Collisions

Momentum & Collisions

45 minutes60 marksprintable — key stays hidden on paper

Level 3: Production Paper (From-Scratch Derivations & Explain-Out-Loud)

Time limit: 45 minutes Total marks: 60

Instructions: Derivations must start from stated first principles. Show every step. Where "explain out loud" is asked, write your reasoning in complete prose.


Question 1 — Impulse–momentum & conservation from first principles (10 marks)

(a) Starting from Newton's second law in the form F=dpdt\vec{F} = \dfrac{d\vec{p}}{dt}, derive the impulse–momentum theorem J=Δp\vec{J} = \Delta\vec{p}. Define impulse. (3)

(b) Using Newton's third law, derive the conservation of total linear momentum for an isolated two-particle system. (4)

(c) Explain out loud: precisely which condition on external forces must hold for total momentum to be conserved for a many-particle system, and why internal forces never change total momentum. (3)


Question 2 — 1D elastic collision, solved from scratch (12 marks)

Two particles collide head-on elastically. Mass m1m_1 has initial velocity u1u_1; mass m2m_2 has u2u_2.

(a) Write the two conservation laws (momentum, kinetic energy). (2)

(b) Derive the final velocities v1,v2v_1, v_2 from scratch, showing the algebra (hint: form the relative-velocity relation). (6)

(c) A 2.0 kg2.0\text{ kg} ball at 6.0 m/s6.0\text{ m/s} strikes a stationary 4.0 kg4.0\text{ kg} ball elastically. Compute v1v_1 and v2v_2. (4)


Question 3 — Coefficient of restitution & inelastic KE loss (10 marks)

(a) Define the coefficient of restitution ee for a 1D collision, and state its values for perfectly elastic and perfectly inelastic cases. (2)

(b) Derive the fraction of kinetic energy lost in a perfectly inelastic head-on collision when m2m_2 is initially at rest (u2=0u_2 = 0). Express the answer in terms of m1,m2m_1, m_2. (5)

(c) A 3.0 kg3.0\text{ kg} lump (8.0 m/s8.0\text{ m/s}) hits a stationary 1.0 kg1.0\text{ kg} lump and they stick. Find the common velocity and the fractional KE lost. (3)


Question 4 — Centre of mass derivation (10 marks)

(a) State the definition of the centre of mass for a system of discrete particles. (2)

(b) From scratch, derive the position of the centre of mass of a uniform semicircular arc (thin wire) of radius RR, measured from the centre. Set up the integral and evaluate. (6)

(c) State (no derivation) the CM distance from centre for a uniform semicircular lamina (disc). (2)


Question 5 — Motion of CM & 2D elastic angles (10 marks)

(a) Derive that Fext=MaCM\vec{F}_{\text{ext}} = M\vec{a}_{\text{CM}} for a system of particles, starting from the definition of CM. (4)

(b) Prove that when a moving particle elastically collides with an identical stationary particle in 2D (glancing collision), the two outgoing velocities are perpendicular. (6)


Question 6 — Rocket equation (code-from-memory) (8 marks)

(a) Derive the rocket equation (Tsiolkovsky) Δv=vexln ⁣m0mf\Delta v = v_{\text{ex}}\ln\!\dfrac{m_0}{m_f} from momentum conservation of ejected mass, in gravity-free space. (5)

(b) Write, from memory, a short Python function delta_v(m0, mf, vex) returning the achieved Δv\Delta v. Then state Δv\Delta v for m0=1000m_0=1000, mf=400m_f=400, vex=2500 m/sv_{\text{ex}}=2500\text{ m/s}. (3)


Answer keyMark scheme & solutions

Question 1 (10)

(a) From F=dp/dt\vec F = d\vec p/dt, integrate over collision time: t1t2Fdt=dp=p2p1=Δp.\int_{t_1}^{t_2}\vec F\,dt = \int d\vec p = \vec p_2 - \vec p_1 = \Delta\vec p. Define impulse Jt1t2Fdt\vec J \equiv \int_{t_1}^{t_2}\vec F\,dt. Hence J=Δp\vec J = \Delta\vec p. (1 integral setup, 1 evaluation, 1 definition)

(b) Particles 1, 2 exert forces on each other. By Newton's III: F12=F21\vec F_{12} = -\vec F_{21}. For each: F21=dp1/dt\vec F_{21} = d\vec p_1/dt, F12=dp2/dt\vec F_{12} = d\vec p_2/dt (only internal forces). Add: d(p1+p2)dt=F21+F12=0.\dfrac{d(\vec p_1+\vec p_2)}{dt} = \vec F_{21}+\vec F_{12} = 0. Therefore p1+p2=\vec p_1 + \vec p_2 = constant. (1 III law, 1 each eqn, 1 conclusion)

(c) Momentum is conserved iff the net external force = 0 (vector sum). Internal forces occur in Newton-III pairs that cancel pairwise in the total sum Fij=0\sum \vec F_{ij}=0, so they cannot alter total p\vec p; only external forces can. (1 condition, 1 pairing, 1 why)


Question 2 (12)

(a) Momentum: m1u1+m2u2=m1v1+m2v2m_1u_1+m_2u_2 = m_1v_1+m_2v_2. KE: 12m1u12+12m2u22=12m1v12+12m2v22\tfrac12 m_1u_1^2+\tfrac12 m_2u_2^2 = \tfrac12 m_1v_1^2+\tfrac12 m_2v_2^2. (2)

(b) Rearrange: m1(u1v1)=m2(v2u2)m_1(u_1-v_1)=m_2(v_2-u_2) …(i) m1(u12v12)=m2(v22u22)m_1(u_1^2-v_1^2)=m_2(v_2^2-u_2^2) …(ii) Divide (ii) by (i): u1+v1=v2+u2u1u2=v2v1u_1+v_1 = v_2+u_2 \Rightarrow u_1-u_2 = v_2-v_1 (relative velocity reverses). (3) Solve with (i): v1=(m1m2)u1+2m2u2m1+m2,v2=(m2m1)u2+2m1u1m1+m2.v_1=\frac{(m_1-m_2)u_1+2m_2u_2}{m_1+m_2},\quad v_2=\frac{(m_2-m_1)u_2+2m_1u_1}{m_1+m_2}. (3)

(c) m1=2,m2=4,u1=6,u2=0m_1=2,m_2=4,u_1=6,u_2=0: v1=(24)66=126=2.0 m/sv_1=\dfrac{(2-4)6}{6}=\dfrac{-12}{6}=-2.0\text{ m/s}. v2=2266=246=4.0 m/sv_2=\dfrac{2\cdot2\cdot6}{6}=\dfrac{24}{6}=4.0\text{ m/s}. (2+2)


Question 3 (10)

(a) e=v2v1u1u2e = \dfrac{v_2-v_1}{u_1-u_2} = (relative speed of separation)/(relative speed of approach). Elastic e=1e=1; perfectly inelastic e=0e=0. (2)

(b) Common velocity v=m1u1m1+m2v=\dfrac{m_1u_1}{m_1+m_2}. Initial KE =12m1u12=\tfrac12 m_1u_1^2. Final =12(m1+m2)v2=12m12u12m1+m2=\tfrac12(m_1+m_2)v^2 = \tfrac12\dfrac{m_1^2u_1^2}{m_1+m_2}. ΔKEKEi=1m1m1+m2=m2m1+m2.\frac{\Delta KE}{KE_i}=1-\frac{m_1}{m_1+m_2}=\frac{m_2}{m_1+m_2}. (2 velocity, 2 energies, 1 fraction)

(c) v=384=6.0 m/sv=\dfrac{3\cdot8}{4}=6.0\text{ m/s}. Fractional loss =m2m1+m2=14=0.25=\dfrac{m_2}{m_1+m_2}=\dfrac{1}{4}=0.25 (25%). (2+1)


Question 4 (10)

(a) rCM=mirimi\vec r_{\text{CM}} = \dfrac{\sum m_i \vec r_i}{\sum m_i} (or 1Mrdm\dfrac1M\int \vec r\,dm). (2)

(b) Semicircular arc, radius RR, linear density λ=M/(πR)\lambda = M/(\pi R). Symmetry ⇒ CM on the axis (call yy). Element at angle θ\theta: dm=λRdθdm=\lambda R\,d\theta, y=Rsinθy=R\sin\theta, θ[0,π]\theta\in[0,\pi]. yCM=1M0πRsinθλRdθ=λR2M0πsinθdθ=λR2M[cosθ]0π=λR2M(2).y_{\text{CM}}=\frac{1}{M}\int_0^\pi R\sin\theta\,\lambda R\,d\theta=\frac{\lambda R^2}{M}\int_0^\pi\sin\theta\,d\theta=\frac{\lambda R^2}{M}\,[{-\cos\theta}]_0^\pi=\frac{\lambda R^2}{M}(2). With λR=M/π\lambda R = M/\pi: yCM=2Rπy_{\text{CM}} = \dfrac{2R}{\pi}. (2 setup, 2 integral, 2 result)

(c) Semicircular lamina: yCM=4R3πy_{\text{CM}} = \dfrac{4R}{3\pi}. (2)


Question 5 (10)

(a) MrCM=miriM\vec r_{\text{CM}}=\sum m_i\vec r_i. Differentiate twice: MaCM=miai=FiM\vec a_{\text{CM}}=\sum m_i\vec a_i=\sum \vec F_i. Internal forces cancel (III law) ⇒ Fi=Fext\sum\vec F_i = \vec F_{\text{ext}}. Hence Fext=MaCM\vec F_{\text{ext}}=M\vec a_{\text{CM}}. (1+1+1+1)

(b) Equal masses mm. Momentum: u=v1+v2\vec u = \vec v_1+\vec v_2. KE (÷12m\tfrac12 m): u2=v12+v22u^2 = v_1^2+v_2^2. Square the vector eqn: u2=uu=(v1+v2)2=v12+v22+2v1v2u^2=\vec u\cdot\vec u=(\vec v_1+\vec v_2)^2=v_1^2+v_2^2+2\vec v_1\cdot\vec v_2. Comparing: 2v1v2=0v1v22\vec v_1\cdot\vec v_2 = 0 \Rightarrow \vec v_1\perp\vec v_2 (provided both nonzero). (2 momentum, 2 energy, 2 dot-product conclusion)


Question 6 (8)

(a) In dt, mass dm-dm (i.e. dm<0dm<0) ejected at exhaust speed vexv_{\text{ex}} relative to rocket. Momentum conservation (no external force): mdv=vexdm.m\,dv = -v_{\text{ex}}\,dm. 0Δvdv=vexm0mfdmmΔv=vexlnm0mf.\int_0^{\Delta v}dv = -v_{\text{ex}}\int_{m_0}^{m_f}\frac{dm}{m}\Rightarrow \Delta v = v_{\text{ex}}\ln\frac{m_0}{m_f}. (2 momentum eqn, 2 integrate, 1 result)

(b)

import math
def delta_v(m0, mf, vex):
    return vex * math.log(m0/mf)

Δv=2500ln(1000/400)=2500ln(2.5)=2500(0.9163)=2290.7 m/s\Delta v = 2500\ln(1000/400)=2500\ln(2.5)=2500(0.9163)=2290.7\text{ m/s}. (2 code, 1 value)


[
{"claim":"Elastic collision v1 = -2 m/s for m1=2,m2=4,u1=6,u2=0","code":"m1,m2,u1,u2=2,4,6,0\nv1=((m1-m2)*u1+2*m2*u2)/(m1+m2)\nresult = v1==-2"},
{"claim":"Elastic collision v2 = 4 m/s","code":"m1,m2,u1,u2=2,4,6,0\nv2=((m2-m1)*u2+2*m1*u1)/(m1+m2)\nresult = v2==4"},
{"claim":"Inelastic common velocity 6 m/s and fractional KE loss 0.25","code":"m1,m2,u1=3,1,8\nv=m1*u1/(m1+m2)\nfrac=m2/(m1+m2)\nresult = (v==6) and (frac==Rational(1,4))"},
{"claim":"Semicircular arc CM = 2R/pi","code":"R,th=symbols('R theta',positive=True)\ny=integrate(R*sin(th)*R,(th,0,pi))/(pi*R)\nresult = simplify(y-2*R/pi)==0"},
{"claim":"Rocket delta_v ~2290.7 m/s","code":"dv=2500*log(Rational(1000,400))\nresult = abs(float(dv)-2290.73)<0.5"}
]