So say you have a vertical mast of height $32$m, and then say a particle P is projected horizontally from the top of the mast at $18$ m/s. Then say that a particle Q is projected at $30$ m/s from the bottom of the mast at an angle x above the horizontal. Given that the particles collide and that $\cos(x) = \frac35$. Is there a way to find the time taken for the collision from the moment they were projected?
Finding the time elapsed between the instant when two particles are projected and the instant they collide
383 Views Asked by Bumbble Comm https://math.techqa.club/user/bumbble-comm/detail AtThere are 2 best solutions below
On
I suppose the idea is that both particles follow parabolic trajectories, that is, we assume the "standard" gravitational acceleration, no air resistance, use the flat-non-rotating-Earth approximation, etc.
The thing about gravity is that it affects both particles identically. That is, if one particle is deflected downward $1$ meter at time $t,$ then the other particle also is deflected downward $1$ meter. So with respect to whether the particles collide, and how long it takes, the effects of gravity cancel out (unless they cause some other event to occur before the particles can collide, such as one particle collides with the ground).
So first solve the problem assuming no forces apply at all after the instant when the particles are projected. So, aside from all the other simplifying assumptions, assume there is no gravity. (You can think of this as solving the problem in an accelerating frame of reference that happens to be in free fall.)
Compute $\sin(x)$ from the given value of $\cos(x).$ From this you get the vertical velocity of the second particle, and you get the time $t_1$ that it takes the second particle to reach the height $32$ meters.
As a sanity check, compute the horizontal positions of both particles at time $t_1.$ If they are not the same, there is an error either in your calculations or in the problem statement.
As another sanity check, you can take the solution for $t_1$ and find where the particles are at that time if you have "standard" gravitational acceleration.
The laws of motion are \begin{align} x_1(t)&=v_1^0t\\ y_1(t)&=h-\frac{1}{2}gt^2\\ x_2(t)&=v_2^0\cos(x)t\\ y_2(t)&=v_2^0\sin(x)t-\frac{1}{2}gt^2\\ \end{align} We can see that $x_1(t) = x_2(t)$ is an identity.
Equating $$ y_1(t)=y_2(t) $$ we get $$ t=\frac{h}{v_2^0\sin(x)}=\frac{32m}{30m/s\sqrt{1-\left(\frac{3}{5}\right)^2}}=1.33s $$ A graphic representation