Collisions in Two Dimensions
Last Updated :
30 Jun, 2021
A Collision occurs when a powerful force strikes on two or more bodies in a relatively short period of time. Collision is a one-time occurrence. As a result of the collision, the involved particles' energy and momentum change. The collision may occur as a result of actual physical contact between the participating bodies, such as a collision between two billiard balls or a ball and bat. There may be collisions where there is no direct physical touch, such as an alpha particle colliding with a nucleus.
Any collision is led by three different definable stages, namely before, during, and after the impact. Because the particles are independent before the collision, the interaction forces between them are zero. Furthermore, following the impact, the force returns to zero. Because the particles come into touch with each other during the collision, the force of interaction becomes extremely strong. The dominant forces direct the movement of the bodies. Because the amount of the interacting force is unknown in most practical circumstances, Newton's second law of motion cannot be used in such cases. The initial and final velocities can be computed using the law of conservation of momentum.
For instance, consider two bodies with masses m1 and m2, moving with velocities u1 and u2. They undergo a collision due to the application of an external force Fext for a small interval of time, and then the final velocities become v1 and v2.

Two Dimensional Elastic Collisions
The following cases may arise in case of elastic collision between two bodies :
(1) Two-dimensional Elastic Collision in Laboratory Reference Frame
Let us consider a system of two particles without the existence of any external forces. The first particle of mass m1 moving with an initial velocity of \vec{v}_{1,i} and the second particle of mass m2 which is initially at rest position. The interacting particles undergo a collision where the first particle moves with velocity \vec{v}_{1,f} and the second particle with velocity \vec{v}_{2,f} . The reference frame with one particle at rest can be termed as the target, the laboratory reference frame.
The angles θ1,f and θ2,f made by the particles along with the positive forward direction of the first particle are called the laboratory scattering angles.
The problem statement is to determine the magnitudes and directions of each of the final velocity vectors, v_{1,f},v_{2,f},θ_{1,f}\ and\ θ_{2,f} . The total kinetic energy and momentum are conserved in the whole system.
The components of the total momentum are obtained by,
\vec{P}^{sys}_i=m_i\vec{v}_{1,i}+m_2\vec{v}_{2,i}\ \ \ \ \ \ \ ..eq(1)\\ P^{sys}_{x,i}=m_1v_{1,i}\ \ \ \ \ \ \ \ ..eq (2)\\ P^{sys}_{y,i}=0
\vec{P}^{sys}_f=m_1\vec{v}_{1,f}+m_2\vec{v}_{2,f}\ \ \ \ \ \ \ \ ..eq (3)
The components of momentum in the final state are obtained by,
P^{sys}_{x,f}=m_1v_{1,f}cos\theta_{1,f}+m_2v_{2,f}cos\theta_{2,f}\\ P^{sys}_{y,f}=m_1v_{1,f}sin\theta_{1,f}+m_2v_{2,f}sin\theta_{2,f}\ \ \ \ \ \ \ ..eq (4)
Since, the total momentum is conserved, we get,
P^{sys}_{x,i}=P^{sys}_{x,f}\ \ \ \ \ \ \ \ .......Equation (5)\\ P^{sys}_{y,i}=P^{sys}_{y,f}\ \ \ \ \ \ \ \ ..eq (6)
Further from above equations, we obtain,
m_1v_{1,i}=m_1v_{1,f}cos\theta_{1,f}+m_2v_{2,f}cos\theta_{2,f}\ \ \ \ \ \ \ ..eq (7)\\ 0=m_1v_{1,f}sin\theta_{1,f}-m_2v_{2,f}sin\theta{2,f}\ \ \ \ \ \ \ \ ..eq(8)
Since, the kinetic energy is preserved during an elastic collision,
K^{sys}_i=K^{sys}_f ..eq(9)
Computing eq(7),
\frac{1}{2}m_1v^2_{1,i}=\frac{1}{2}m_1v^2_{1,f}+\frac{1}{2}m_2v^2_{2,f} ..eq (10)
Rewriting eq(5) and eq (6) as,
m_2v_{2,f}cos\theta_{2,f}=m_1(v_{1,i}-v_{1,f}cos\theta_{1,f})\ \ \ \ \ \ \ ..eq (11)\\ m_2v_{2,f}sin\theta_{2,f}=m_1v_{1,f}sin\theta_{1,f}\ \ \ \ \ \ \ ..eq (12)
Squaring and adding each of the expressions in eq (9) and eq(10),
cos^2\theta+sin^2\theta=1\ \ \ \ \ \ ..eq(13) \\ v^2_{2,f}=\frac{m^2_1}{m^2_2}(v^2_{1,i}-2v_{1,i}v_{1,f}cos\theta_{1,f}+v^2_{1,f})\ \ \ \ \ \ \ \ ..eq (14)
Substituting the eq (11) into eq (8), we obtain,
\frac{1}{2}m_{1,i}=\frac{1}{2}m_1v_{1,f}+\frac{1}{2}\frac{m^2_1}{m_2}(v^2_{1,i}-2_{1,i}v_{1,f}cos\theta_{1,f}+v^2_{1,f})\ \ \ \ \ ..eq (15)
Simplifying eq (12), we get,
0=\left(1+\frac{m_1}{m_2}\right)v^2_{1,f}-\frac{m_1}{m_2}2v_{1,i}v_{1,f}cos\theta-\left(1-\frac{m_1}{m_2}\right)v^2_{1,i}\ \ \ \ \ \ \ ..eq (16)
Let ∝ = \frac{m_1}{m_2}
Rewriting eq (13) ,
0=(1+\alpha)v^2_{1,f}-2\alpha v_{1,f}v_{1,f}cos\theta_{1,f}-(1-\alpha)v^2_{1,i}\ \ \ \ \ \ \ ..eq (17)
Finding solution of quadratic equation, we can obtain the following results,
v_{1,f}=\frac{\alpha v_{1,i}cos\theta _{1,f}\pm(\alpha^2v^2_{1,f}+(1-\alpha)v^2_{1,i})^{\frac{1}{2}}}{(1+\alpha)}\ \ \ \ \ ..eq\ (18)
Computing for eq (9),
\frac{v_{2,fsin\theta_{2,f}}}{v_{2,f}cos\theta_{,f}}=\frac{v_{1,f}sin\theta_{1,f}}{v_{1,i}-v_{1,f}cos\theta_{1,f}}\ \ \ \ \ \ \ ..eq (19)
Simplifying eq (16), we get,
tan\theta_{2,f}=\frac{v_{1,f}sin\theta_{1,f}}{v_{1,i}-v_{1,f}cos\theta_{1,f}}\ \ \ \ \ \ \ \ ..eq\ (20)
We can conclude that the relationship between the scattering angles is independent of the masses of the colliding particles.
Therefore,
the scattering angle for the second particle can be computed by,
\theta_{2,f}=tan^{-1}\left(\frac{v_{1,f}sin\theta_{1,f}}{v_{1,i}-v_{1,f}cos\theta_{1,f}}\right)\ \ \ \ \ \ \ ..eq\ (21)
Using eq (10), in order to compute the final velocity of the first particle,
v_{2,f}=\frac{v_{1,f}sin\theta_{1,f}}{\alpha sin\theta_{2,f}}\ \ \ \ \ \ ..eq\ (22)
(2) Elastic collision with infinite masses in two dimensions
Let us assume a body to be of mass m1colliding with an infinite mass at rest. Let us assume its velocity be un along the normal before collision and in the tangential direction to be ut
Since the momentum is conserved in the tangential direction,
m1ut = mv1,t
v1,t = ut
Since the momentum is conserved in the normal direction,
m1un = m1v1,n + m2v2n
In case of elastic collision between bodies, the velocity of approach equals the velocity of separation, therefore,
v2,n - v1,n = un
Simplifying, we obtain,
v_{1,n}=\frac{m_1-m_2}{m_1+m_2}u_n\\ v_{2,n}=\frac{2m_1}{m_1+m_2}u_n
On approximating, we use, m2 >> m1
v1,n = -u1,n
v2,n = 0
(3) Elastic collision of equal masses in two dimensions
Let us assume a body to be of mass m. The second body holds the same mass m and is initially at rest. The two interacting particles undergo collision. Let us assume the velocity to be un along the normal before collision and ut along the tangent.
Since the momentum is conserved in the tangential direction,
mut = mv1,t
v1,t = ut
Since the momentum is conserved in the normal direction,
mun = mv1,n + mv2,n
In case of elastic collision between bodies, the velocity of approach equals the velocity of separation, therefore,
v2,n - v1,n = un
The equation can be further solved to obtain,
v_{1,n}=\frac{m_1-m_2}{m_1+m_2}u_n\\ v_{2,n}=\frac{2m_1}{m_1+m_2}u_n
Since, the masses are equal , we get, m2 = m1
v1,n = 0
that is,
v2,n = un
(4) Inelastic Collision in Two Dimension
For a completely inelastic collision, let us assume a system consisting of two particles m1 with velocity v1 and m2 with velocity v2 at an angle of θ1 with respect to each other. After the inelastic collision, both the masses form a single mass M and move with a final velocity vf.
The law of conservation of energy is not applicable in an inelastic collision. The equations of momentum can be generated for masses in both the x and y directions, by shifting the orientation of the object with mass m1 in the x-axis direction.
Now, we obtain,
x component: m1v1 + Mvfcosθ2
y component: m2v2sinθ1 Mvfsinθ2
The final result leaves us with two-equation and two variables, vf, and θ2. Thus, any completely inelastic collision in two dimensions is easily solvable in comparison to the completely elastic collision.
Deflection of a moving particle by a particle at rest
Let us assume a system of two masses, m1 moving with a velocity u1 and the second body of mass m2 to be at rest. After the collision, the first mass object starts moving with a velocity of v1 and gets deflected by the angle θ1 in the incident direction. Similarly, the second mass object starts moving with a velocity of v2 and gets deflected by the angle θ2 in the incident direction.
Now, we have,
According to the law of conservation of linear momentum ,
For components along the x-axis, we have,
m1u1 = m1v1cosθ1 +m2v2cosθ2 .. eq(1)
For components along y-axis, we have,
0=m1v1sinθ1 -m2v2sinθ2 ..eq(2)
Since, the system reduces to the availability of three equations and four unknown variables, solving the system with only these values becomes impossible.
Sample Problems
Problem 1: A mass of 10 kg is traveling with a velocity of 30 m/s in the positive y-axis. The mass undergoes a collision with another object of mass 40 g moving along the negative y-axis at a speed of 50 m/s. Calculate the final velocity.
Solution:
According to the law of conservation of momentum, therefore,
Momentum before impact = Momentum After Impact
Equating the values, we get,
10 × 30 + (.04) × (-50) = 10.04 v
Since, the 40g particle is moving in negative direction, we have,
v = 29.68 m/s
Problem 2: There is an isolated system containing three masses, m1 = m2 = 2 m and m3 = 3 m. All the masses travel in direction, but with the same initial velocity equivalent to v0. The bodies collide and undergo an elastic collision. Compute the maximal possible final speed of each of the three bodies.
Solution:
Total initial kinetic energy in the system =
\frac{1}{2}m_1v_0^2 + \frac{1}{2}m_2v_0^2 + \frac{1}{3}m_3v_0^2=3mv_0^2
The maximum speed is attained when the speeds of other particles is reduced to zero.
Therefore,
\frac{1}{2}m_1(v_{1max})^2 = 3mv_0^2
Substituting the values of the masses,
We get,
v1max = 2.45v0
v2max = 1.73v0
v3max = 1.41v0
Problem 3: A sphere moving with a velocity vector strikes a vertical wall. The wall is parallel to the velocity vector. The coefficient of restitution between the sphere and wall is e. What is the velocity vector of the sphere on hitting the ball?
Solution:
Computing the value,
vy = 2 m/s
vx = -e × 2 = -1 m/s
\vec{v}=v_x\hat{i}+v_y\hat{j}=(-\hat{i}+2\hat{j})unit
Problem 4: Consider a body of mass m kg moving with a speed u. The ball hits the floor elastically with an angle of incidence, in such a way, that the velocity before and after the collision remains the same. Also, the angle of rebound equals the angle of incidence. Let us assume the velocity towards the floor to be negative. What will be the change in momentum taken parallel to the surface?
Solution:
Since, we know, that the force acting on the body of mass 'm' is the normal reaction force of the surface. The change in momentum taken parallel to the surface will be equivalent to 0, since no parallel force acts on the ball.
Problem 5: Explain the aftermath repercussions when two unequal masses collide.
Solution:
When two bodies of unequal mass collide, the force acting on both objects is not equal and opposite in nature. Both the interacting particles experience unequal accelerations during the collision because of the contact forces.
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Acceleration due to Gravity
Acceleration due to gravity (or acceleration of gravity) or gravity acceleration is the acceleration caused by the gravitational force of attraction of large bodies. As we know that the term acceleration is defined as the rate of change of velocity with respect to a given time. Scientists like Sir I
8 min read
What is the Acceleration due to Gravity on Earth ?
Take something in your hand and toss it down. Its speed is zero when you free it from your grip. Its pace rises as it descends. It flies faster the longer it goes. This sounds like acceleration. Acceleration, on the other hand, implies more than just rising speed. Pick up the same object and throw i
11 min read
Gravitational Potential Energy
The energy possessed by objects due to changes in their position in a gravitational field is called Gravitational Potential Energy. It is the energy of the object due to the gravitational forces. The work done per unit mass to bring the body from infinity to a location inside the gravitational field
13 min read
Escape Velocity
Escape velocity as the name suggests, is the velocity required by an object to escape from the gravitational barrier of any celestial object. "What happens when you throw a stone upward in the air?" The stone comes back to the Earth's surface. If we throw the stone with a much higher force still it
7 min read
Artificial Satellites
When looked at the night sky many heavenly bodies like stars, moon, satellites, etc are observed in the sky. Satellites are small objects revolving or orbiting around a planet or on object larger than it. The most commonly observed and known satellite is the moon, the moon is the satellite of Earth,
8 min read
Binding Energy of Satellites
Humans learn early in life that all material items have a natural tendency to gravitate towards the earth. Anything thrown up falls to the ground, traveling uphill is much more exhausting than walking downhill, Rains from the clouds above fall to the ground, and there are several additional examples
10 min read
Chapter 8 - Mechanical Properties of Solids
Stress and Strain
Stress and Strain are the two terms in Physics that describe the forces causing the deformation of objects. Deformation is known as the change of the shape of an object by applications of force. The object experiences it due to external forces; for example, the forces might be like squeezing, squash
12 min read
Hooke's Law
Hooke's law provides a relation between the stress applied to any material and the strain observed by the material. This law was proposed by English scientist Robert Hooke. Let's learn about Hooke's law, its application, and others, in detail in this article. What is Hookeâs Law?According to Hooke's
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Stress-Strain Curve
Stress-Strain Curve is a very crucial concept in the study of material science and engineering. It describes the relationship between stress and the strain applied on an object. We know that stress is the applied force on the material, and strain, is the resulting change (deformation or elongation)
11 min read
Modulus of Elasticity
Modulus of Elasticity or Elastic Modulus is the measurement of resistance offered by a material against the deformation force acting on it. Modulus of Elasticity is also called Young's Modulus. It is given as the ratio of Stress to Strain. The unit of elastic modulus is megapascal or gigapascal Modu
12 min read
Elastic Behavior of Materials
Solids are made up of atoms based on their atomic elasticity (or molecules). They are surrounded by other atoms of the same kind, which are maintained in equilibrium by interatomic forces. When an external force is applied, these particles are displaced, causing the solid to deform. When the deformi
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Chapter 9 - Mechanical Properties of Fluids