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Physics · Ch 5 — Work, Energy and Power

Collisions

5.11

Collisions

Collisions

In physics, we study motion — change in position. But at the same time, we try to discover physical quantities that do not change during a physical process. The laws of conservation of momentum and conservation of energy are the most powerful examples of such unchanging quantities. In this section, we apply these conservation laws to a very common phenomenon: collisions.

Games like billiards, marbles, and carrom are full of collisions. We will study the collision of two masses in an idealised form. Consider two masses m1m_1 and m2m_2. The particle m1m_1 is moving with an initial speed v1iv_{1i} (the subscript ii stands for "initial"). We can take m2m_2 to be at rest without any loss of generality — any collision where both masses are moving can be turned into this situation by shifting to the centre-of-mass frame. So the mass m1m_1 collides with the stationary mass m2m_2. …

Figure 5.10Collision of mass m1 with a stationary mass m2.
Fig. 5.10 — Collision of mass m1 with a stationary mass m2.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your textbook's own diagram.

The figure is a two-panel sketch on an xx–yy coordinate grid. The origin marks the point of collision. Before the collision, a blue sphere of mass m1m_1 moves horizontally from the left along the xx-axis with velocity v⃗1i\vec{v}_{1i}. A grey sphere of mass m2m_2 sits stationary at the origin. After the collision, the blue sphere moves up and to the right at an angle θ1\theta_1 above the xx-axis, with final velocity v⃗1f\vec{v}_{1f}. The grey sphere moves down and to the right at an angle θ2\theta_2 below the xx-axis, with final velocity v⃗2f\vec{v}_{2f}. The arrows representing v⃗1f\vec{v}_{1f} and v⃗2f\vec{v}_{2f} are drawn from the origin, showing the two outgoing paths.

The physical idea is a two-dimensional elastic collision between a moving projectile and a stationary target. The figure makes clear that the motion is confined to a plane — the incoming momentum is entirely along xx, but after the collision the momentum is shared between both bodies in both xx and yy directions. The angles θ1\theta_1 and θ2\theta_2 are measured from the original line of motion (the xx-axis), and they are not independent: conservation of momentum in the yy-direction forces a relation between them.

The textbook develops the two fundamental conservation laws from this figure. For an elastic collision, kinetic energy is also conserved. The key equations are:

m1v1i=m1v1fcos⁡θ1+m2v2fcos⁡θ2m_1 v_{1i} = m_1 v_{1f} \cos\theta_1 + m_2 v_{2f} \cos\theta_2

0=m1v1fsin⁡θ1−m2v2fsin⁡θ20 = m_1 v_{1f} \sin\theta_1 - m_2 v_{2f} \sin\theta_2

12m1v1i2=12m1v1f2+12m2v2f2\frac{1}{2} m_1 v_{1i}^2 = \frac{1}{2} m_1 v_{1f}^2 + \frac{1}{2} m_2 v_{2f}^2

The first equation is conservation of momentum along the xx-axis: the initial momentum m1v1im_1 v_{1i} equals the sum of the xx-components of the final momenta. The second equation is conservation of momentum along the yy-axis: the initial yy-momentum is zero, so the upward yy-component of m1m_1's final momentum must equal the downward yy-component of m2m_2's final momentum (the minus sign accounts for opposite directions). The third equation is conservation of kinetic energy, which holds only for an elastic collision.

Watch out

The angles θ1\theta_1 and θ2\theta_2 are not arbitrary. For a given m1m_1, m2m_2, and v1iv_{1i}, these three equations determine the four unknowns v1fv_{1f}, v2fv_{2f}, θ1\theta_1, and θ2\theta_2 only if one additional condition is given — for example, the impact parameter or the fact that the collision is elastic. In many textbook problems, one of the angles or final speeds is provided. …