If \( V_1 \) is the velocity of a body projected from point A and \( V_2 \) is the velocity of a body projected from point B, which is vertically below the highest point C, and if both the bodies collide, then:
Show Hint
For projectile motion:
- Velocity is affected by gravitational potential energy changes.
- Use energy conservation or kinematic equations to compare speeds.
- Symmetry of projectile paths helps in velocity comparison.
To analyze the motion of the two bodies and determine their velocity relationship at the point of collision, we apply the kinematic equations for projectile motion. Step 1: Understanding the Given Motion
- The body at point \( A \) is projected with velocity \( V_1 \) at an angle \( \theta \).
- The body at point \( B \) is projected vertically with velocity \( V_2 \).
- The highest point \( C \) represents the peak of the trajectory of the first body.
- Both bodies collide at a certain point, meaning they must meet at the same height and at the same time. Step 2: Motion of the Body from \( A \)
- The body projected from \( A \) reaches the highest point \( C \) with a vertical velocity component of zero.
- The initial vertical velocity of the body from \( A \) is:
\[
u_{Ay} = V_1 \sin \theta
\]
- The time taken to reach the highest point \( C \) is given by:
\[
t_C = \frac{u_{Ay}}{g} = \frac{V_1 \sin \theta}{g}
\]
- The total height of \( C \), using the equation of motion \( v^2 = u^2 + 2as \), is:
\[
h = \frac{(V_1 \sin \theta)^2}{2g}
\]
Step 3: Motion of the Body from \( B \)
- The second body at \( B \) is projected vertically upwards with velocity \( V_2 \).
- Let the time taken by the second body to reach the point of collision be \( t \).
- The equation of motion for vertical displacement is:
\[
h' = V_2 t - \frac{1}{2} g t^2
\]
Since both bodies collide at the same height and time, setting \( h = h' \), we equate the expressions:
\[
\frac{(V_1 \sin \theta)^2}{2g} = V_2 t - \frac{1}{2} g t^2
\]
Substituting \( t = \frac{V_1 \sin \theta}{g} \), we get:
\[
\frac{(V_1 \sin \theta)^2}{2g} = V_2 \times \frac{V_1 \sin \theta}{g} - \frac{1}{2} g \left(\frac{V_1 \sin \theta}{g}\right)^2
\]
Simplifying,
\[
\frac{(V_1 \sin \theta)^2}{2g} = \frac{V_1 V_2 \sin \theta}{g} - \frac{(V_1 \sin \theta)^2}{2g}
\]
Rearranging for \( V_2 \),
\[
V_2 = \frac{1}{2} V_1
\]
Thus, the correct answer is:
\[
{V_2 = \frac{1}{2} V_1}
\]