Alessandro C. answered 09/29/24
3+ years tutoring Ph.D. in Theoretical Astrophysics
The equation for a body that moves with constant acceleration is d(t) = d0 + v0 t + 1/2 a t^2 where d0 is the initial position of the body, v0 is the initial velocity and a is the acceleration.
For a ball under the acceleration of gravity g, the height of the body at a time t is given by Y(t) = Y0 + v0 t - 1/2 g t^2 where the minus sign in front of g is because we are assuming the positive direction of the y coordinate to be up (and negative down).
For the third problem, we put into practice everything we learned so far.
In this case, we have Y(t*) = 0 m since the ball touches the ground at the final instant, Y0 = 90 m, v0 = 0 m/s since the ball is left to fall and the gravity acceleration g is directed towards down. In this case we have: Y(t*) = Y0 + v0 t* -1/2 g t*^2 -> Y0 = 1/2g t*^2 -> t* = √(2Y0/g) = 4.28s.
Finally, the final velocity of the ball v(t*) at the final time t* is given by the equation v(t*) = v0 - g t* = -g t*-> v(t*) = - 42.02 m/s which means the velocity is directed towards the ground as we expect