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Dynamics covers kinematics and kinetics of particles and rigid bodies: motion in various coordinate systems, Newton's second law, work-energy, impulse-momentum, and rotating bodies. Exams chain several concepts into one problem — pick the wrong method and you run out of time. Practicing full problems with step-by-step solutions teaches you which approach each setup calls for.

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Topics typically tested

  • Rectilinear & curvilinear kinematics
  • Normal-tangential & polar coordinates
  • Newton's second law problems
  • Work-energy methods
  • Impulse, momentum & impact
  • Rigid-body rotation & relative motion

Sample Dynamics exam questions

Three original questions in the style of a real Dynamics exam, each with a worked solution. Your own practice exam can be built from your course's notes and syllabus.

Question 1Multiple choiceNormal-tangential & polar coordinates

A car travels along a horizontal circular track of radius 200 m. Starting from a speed of 10 m/s, the driver increases the speed at a constant rate (constant tangential acceleration) so that the car reaches 20 m/s after travelling 75 m along the track. What is the magnitude of the car's total acceleration at the instant its speed is 15 m/s?

  1. A.

    1.13 m/s²

  2. B.

    2.00 m/s²

  3. C.

    2.29 m/s²

  4. D.

    3.13 m/s²

Worked solution
Answer:C

Use normal–tangential components. The tangential acceleration is constant, so the constant-acceleration relation v2=v02+2atsv^2 = v_0^2 + 2a_t s applies along the path:

at=v2−v022s=202−1022(75)=300150=2.00 m/s2a_t = \frac{v^2 - v_0^2}{2s} = \frac{20^2 - 10^2}{2(75)} = \frac{300}{150} = 2.00\,\text{m/s}^2

The normal (centripetal) component depends only on the instantaneous speed and the radius of curvature:

an=v2ρ=152200=1.125 m/s2a_n = \frac{v^2}{\rho} = \frac{15^2}{200} = 1.125\,\text{m/s}^2

The two components are perpendicular, so the magnitude is their vector sum:

a=at2+an2=2.002+1.1252=5.266=2.29 m/s2a = \sqrt{a_t^2 + a_n^2} = \sqrt{2.00^2 + 1.125^2} = \sqrt{5.266} = 2.29\,\text{m/s}^2

The acceleration vector points tan⁡−1(1.125/2.00)=29.4∘\tan^{-1}(1.125/2.00) = 29.4^\circ inward from the tangent.

The tempting answer 3.13 m/s² adds the two components as scalars; they are at right angles, so they must be combined with Pythagoras. 2.00 m/s² ignores the normal component, which exists whenever the path curves, and 1.13 m/s² ignores the speed-up.

a=2.29 m/s2a = 2.29\,\text{m/s}^2

Question 2Short answerWork-energy methods

A 5.0 kg block is released from rest at the top of a plane inclined at 30∘30^\circ to the horizontal. The coefficient of kinetic friction between the block and the plane is μk=0.20\mu_k = 0.20. Take g=9.81 m/s2g = 9.81\,\text{m/s}^2. Using the principle of work and energy, find the speed of the block after it has slid 4.0 m down the incline.

Worked solution
Answer:

5.06 m/s

Apply the principle of work and energy between the release point (1) and the point 4.0 m down the slope (2): T1+∑U1→2=T2T_1 + \sum U_{1\to 2} = T_2, with T1=0T_1 = 0 because the block starts from rest.

Forces on the block: weight W=5.0(9.81)=49.05W = 5.0(9.81) = 49.05 N, the normal force N=Wcos⁡30∘=42.48N = W\cos 30^\circ = 42.48 N (there is no acceleration perpendicular to the plane), and kinetic friction Ff=μkN=0.20(42.48)=8.496F_f = \mu_k N = 0.20(42.48) = 8.496 N acting up the slope. The normal force does no work because it is perpendicular to the motion.

Work of gravity (positive, since the block drops 4.0sin⁡30∘=2.04.0\sin 30^\circ = 2.0 m):

Ug=W ssin⁡30∘=49.05(4.0)(0.5)=98.1 JU_g = W\,s\sin 30^\circ = 49.05(4.0)(0.5) = 98.1\,\text{J}

Work of friction (negative, since it opposes the motion):

Uf=−Ff s=−8.496(4.0)=−33.98 JU_f = -F_f\,s = -8.496(4.0) = -33.98\,\text{J}

Work–energy:

0+98.1−33.98=12(5.0)v22  ⇒  v22=2(64.12)5.0=25.650 + 98.1 - 33.98 = \tfrac{1}{2}(5.0)v_2^2 \;\Rightarrow\; v_2^2 = \frac{2(64.12)}{5.0} = 25.65 v2=5.06 m/sv_2 = 5.06\,\text{m/s}

Without friction the speed would be 2(9.81)(2.0)=6.26\sqrt{2(9.81)(2.0)} = 6.26 m/s; friction removes about a third of the kinetic energy, which is consistent with a friction force that is about a third of the down-slope weight component.

v=5.06 m/sv = 5.06\,\text{m/s}

Question 3Worked problemImpulse, momentum & impact

Two smooth spheres move along the same straight line on a frictionless horizontal surface. Sphere A (mass 3.0 kg) moves to the right at 6.0 m/s and sphere B (mass 5.0 kg) moves to the left at 2.0 m/s. They undergo a direct central impact with coefficient of restitution e=0.60e = 0.60. Take rightward as positive. Find (a) the velocity of each sphere immediately after the impact and (b) the kinetic energy lost in the collision.

Worked solution
Answer:

(a) A: 2.0 m/s to the left; B: 2.8 m/s to the right. (b) 38.4 J lost

Take rightward as positive, so (vA)1=+6.0(v_A)_1 = +6.0 m/s and (vB)1=−2.0(v_B)_1 = -2.0 m/s.

Conservation of linear momentum for the two-sphere system (no external impulse acts along the line of impact):

3.0(6.0)+5.0(−2.0)=3.0 vA+5.0 vB  ⇒  3vA+5vB=8.03.0(6.0) + 5.0(-2.0) = 3.0\,v_A + 5.0\,v_B \;\Rightarrow\; 3v_A + 5v_B = 8.0

Coefficient of restitution, written as separation velocity over approach velocity so that the signs take care of themselves:

e=vB−vA(vA)1−(vB)1  ⇒  vB−vA=0.60 [6.0−(−2.0)]=4.8e = \frac{v_B - v_A}{(v_A)_1 - (v_B)_1} \;\Rightarrow\; v_B - v_A = 0.60\,[6.0 - (-2.0)] = 4.8

Substitute vB=vA+4.8v_B = v_A + 4.8 into the momentum equation:

3vA+5(vA+4.8)=8.0  ⇒  8vA=−16  ⇒  vA=−2.0 m/s,vB=2.8 m/s3v_A + 5(v_A + 4.8) = 8.0 \;\Rightarrow\; 8v_A = -16 \;\Rightarrow\; v_A = -2.0\,\text{m/s},\quad v_B = 2.8\,\text{m/s}

Sphere A rebounds to the left at 2.0 m/s and sphere B moves to the right at 2.8 m/s. The spheres separate (vB>vAv_B > v_A), as they must after an impact.

Kinetic energy before and after:

T1=12(3.0)(6.0)2+12(5.0)(2.0)2=54+10=64 JT_1 = \tfrac{1}{2}(3.0)(6.0)^2 + \tfrac{1}{2}(5.0)(2.0)^2 = 54 + 10 = 64\,\text{J} T2=12(3.0)(2.0)2+12(5.0)(2.8)2=6.0+19.6=25.6 JT_2 = \tfrac{1}{2}(3.0)(2.0)^2 + \tfrac{1}{2}(5.0)(2.8)^2 = 6.0 + 19.6 = 25.6\,\text{J}

The loss T1−T2=38.4T_1 - T_2 = 38.4 J is dissipated as heat, sound and permanent deformation. A loss is expected whenever e<1e < 1; it is large here (60% of the initial energy) because the spheres approach each other quickly while their centre of mass moves at only 8.0/8.0=1.08.0/8.0 = 1.0 m/s.

(a) vA=2.0v_A = 2.0 m/s to the left, vB=2.8v_B = 2.8 m/s to the right; (b) 38.4 J of kinetic energy is lost

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