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NEET PHYSICSMedium

A projectile is fired from the surface of the earth with a velocity of 5 m/s5 \text{ m/s} and angle θ\theta with the horizontal. Another projectile fired from another planet with a velocity of 3 m/s3 \text{ m/s} at the same angle follows a trajectory, which is identical to the trajectory of the projectile fired from the earth. The value of the acceleration due to gravity on the planet (in m/s2\text{m/s}^2) is: [Given, g=9.8 m/s2g = 9.8 \text{ m/s}^2]

A

3.5

B

5.9

C

16.3

D

110.8

Step-by-Step Solution

  1. Equation of Trajectory: The path of a projectile is given by the equation: y=xtanθgx22v2cos2θy = x \tan \theta - \frac{g x^2}{2 v^2 \cos^2 \theta} where yy and xx are coordinates, vv is the initial velocity, θ\theta is the angle of projection, and gg is the acceleration due to gravity .
  2. Condition for Identical Trajectory: For two projectiles to follow the same trajectory (identical path y(x)y(x)), the coefficients of xx and x2x^2 in the equation must be identical.
  • The term tanθ\tan \theta is already the same since the angle θ\theta is given as equal.
  • The term g2v2cos2θ\frac{g}{2 v^2 \cos^2 \theta} must also be equal for both cases.
  1. Derivation: Since θ\theta is constant, cos2θ\cos^2 \theta is constant. Therefore, the ratio gv2\frac{g}{v^2} must be constant: gearthvearth2=gplanetvplanet2\frac{g_{earth}}{v_{earth}^2} = \frac{g_{planet}}{v_{planet}^2}
  2. Calculation:
  • Earth: ge=9.8 m/s2g_e = 9.8 \text{ m/s}^2, ve=5 m/sv_e = 5 \text{ m/s}
  • Planet: gp=?g_p = ?, vp=3 m/sv_p = 3 \text{ m/s} gp=ge(vpve)2g_p = g_e \left( \frac{v_p}{v_e} \right)^2 gp=9.8×(35)2=9.8×925=9.8×0.36g_p = 9.8 \times \left( \frac{3}{5} \right)^2 = 9.8 \times \frac{9}{25} = 9.8 \times 0.36 gp=3.5283.5 m/s2g_p = 3.528 \approx 3.5 \text{ m/s}^2
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