Bandersnatch said:
Because you are told in the problem that the collision with DART is at 90 degrees to the velocity of the asteroid. So any velocity the asteroid may have gained (##\Delta V##) will be in the same direction as DART was moving along. Otherwise, the asteroid would have gained some momentum 'sideways', even though nothing ever hit it sideways. That would run afoul of conservation of momentum, so it's disallowed.Yes. Along the direction of collision would mean 'like b', since that's the direction DART hits the asteroid towards. That's the direction of the push, of the impulse.
It is, by the way, the same picture as the last one you made. The velocity vector c in the former is the one you labelled 'x' in the latter. The x is the sum of the other two.
There is a potential false intuition that might creep in here and confuse you, to the effect of: since x is longer than initial velocity, the body must have accelerated sideways as a result of the collision. But in reality, it is only longer in the way they hypotenuse in a right triangle is longer than its base. All the extra length is gained at the right angle.
I understand this.
PeroK said:
It says in the question to assume that the collision is at ##90## degrees to the direction of the asteroid's velocity. Conservation of momentum (in all directions) tell you the rest.
I have written the conservation of momentum in all directions but I can't see from the equation that the change in velocity of asteroid will be 90 degree to its initial direction of motion.
Let asteroid moving to the right collides with DART moving upwards, where:
m
a = mass of asteroid
m
d = mass of DART
u
a = initial velocity of asteroid
u
d = initial velocity of DART
v = final velocity of asteroid and DART
θ = angle between v and horizontal
From conservation of momentum in x - direction:
m
a . u
a = (m
a + m
d) . v cos θ ... (1)
From conservation of momentum in y - direction:
m
d . u
d = (m
a + m
d) . v sin θ ... (2)
Dividing (2) by (1): tan θ = (m
d . u
d) / (m
a . u
a) ... (3)
Change in velocity of asteroid in x - direction: Δv
x = v cos θ - u
a
Change in velocity of asteroid in y - direction: Δv
y = v sin θ
Change in velocity of asteroid:
$$\Delta v = \sqrt{(\Delta v_x)^2 + (\Delta v_y)^2}$$
$$=\sqrt{v^2-2v u_a \cos \theta +u_a^2} ~... (4)$$
From all of those equations, how can I know the change in velocity of the asteroid will have a direction of vertically upwards? I expect Δv
x to be zero so v cos θ = u
a but how to get this relation?
Thanks