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Question: A projectile is fired with a speed of u at an angle \(\theta \) above the horizontal field. The coef...

A projectile is fired with a speed of u at an angle θ\theta above the horizontal field. The coefficient of restitution of collision between the projectile and the field is e. How far from the starting point, does the projectile make its second collision with the field?

Explanation

Solution

Firstly, calculate the time of flight for the projectile then find the distances from the starting point when the projectile will land at its first collision and second collision. After, adding both the positions we can calculate the final answer.
Formula used: t=2×usinθgt = \dfrac{{2 \times u\sin \theta }}{g}

Complete answer:
Given that: initial velocity of the projectile = u and the angle of projection of the projectile with respect to ground = θ\theta .
When the projectile hits the ground for the first time, the velocity remains the same i.e. u. the component of the velocity parallel to ground, ucosθu\cos \theta should remain constant. However, the vertical component of the projectile undergoes a change after the collision.

If the coefficient of restitution of the collision between the projectile and the field is e. using the formula of time of flight we know that t=2usinθgt = \dfrac{{2u\sin \theta }}{g}
Where ‘u’ is the initial velocity, ‘g’ is the acceleration due to gravity and ‘θ’ is the angle of projection. For first collision
t1=2usinθg{t_1} = \dfrac{{2u\sin \theta }}{g}
Now position will be given by,
\eqalign{ & {R_1} = \dfrac{{2u\sin \theta }}{g} \times u\cos \theta \cr & \Rightarrow {R_1} = \dfrac{{{u^2}\sin 2\theta }}{g}.......\left( 1 \right) \cr}
As we know, 2sinθcosθ=sin2θ2\sin \theta \cos \theta = \sin 2\theta
R1{R_1}Is the position of the projectile after the first collision, which is u2sin2θg\dfrac{{{u^2}\sin 2\theta }}{g}
Now, for the second collision
t2=2eusinθg{t_2} = \dfrac{{2eu\sin \theta }}{g}
We know that position after second collision is given by
\eqalign{ & {R_2} = \dfrac{{2eu\sin \theta }}{g} \times u\cos \theta \cr & \Rightarrow {R_2} = \dfrac{{e{u^2}\sin 2\theta }}{g}........(2) \cr}
Now, the position of the projectile from the starting point to its final point is given by
R=R1+R2R = {R_1} + {R_2}
From (1) and (2) we get
\eqalign{ & R = \dfrac{{{u^2}\sin 2\theta }}{g} + \dfrac{{e{u^2}\sin 2\theta }}{g} \cr & \therefore R = \dfrac{{{u^2}\sin 2\theta }}{g}\left( {1 + e} \right) \cr}
This is the final answer.

Note:
The component of velocity parallel to ground, that is ucosθu\cos \theta should remain constant. But, usinθu\sin \theta which is the vertical component will change after the collision. As we know the time taken by an object to travel distance is known as time of flight.