A ball with mass m is thrown from the origin at speed V 0 toward the right on an exotic planet where the strength of gravity is g ′ = 1 0 g = 1 m / s 2 .
Let α be the largest possible angle such that, for all θ < α , the distance between the ball and its launch point will be strictly increasing for t > 0 .
What is tan 2 α , to two decimal places?
Details and Assumptions:
Bonus: Generalize this angle for arbitrary values of V 0 , m , and g ′ .
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I really like the use of vectors! Its much less complicated than what I did with the differential equation, finding derivatives, etc.
(I +1'd this morning on my phone. Waited to get to a computer to type this up)
Relevant wiki: Problem solving 2D
This doesn't need to be framed as a 3D problem. 2D kinematics works fine. Write down the x and y expressions. I will simply call the downward acceleration g because that is a familiar convention.
x = V 0 cos ( θ ) t y = V 0 sin ( θ ) t − 2 1 g t 2
Distance from launch point (origin):
D 2 = x 2 + y 2 = V 0 2 cos 2 ( θ ) t 2 + V 0 2 sin 2 ( θ ) t 2 − V 0 g sin ( θ ) t 3 + 4 1 g 2 t 4 = V 0 2 t 2 − V 0 g sin ( θ ) t 3 + 4 1 g 2 t 4
Rate of change of squared distance must be greater than zero for all values of t :
d t d ( D 2 ) = 2 V 0 2 t − 3 V 0 g sin ( θ ) t 2 + g 2 t 3 > 0 ⟹ 2 V 0 2 − 3 V 0 g sin ( θ ) t + g 2 t 2 > 0
Plugging in numbers gives:
2 0 0 0 0 − 3 0 0 sin ( θ ) t + t 2 > 0 c + b t + a t 2 > 0
We know that this will be satisfied if there are no real-valued solutions for the quadratic:
2 0 0 0 0 − 3 0 0 sin ( θ ) t + t 2 = 0
Determine the critical value of θ which makes ( b 2 = 4 a c ) :
9 0 0 0 0 sin 2 ( θ ) = 8 0 0 0 0 sin 2 ( θ ) = 9 8 tan 2 ( θ ) = 1 − sin 2 ( θ ) sin 2 ( θ ) = 1 − 9 8 9 8 = 8
I have a little problem, doesn't it will be b 2 − 4 a c < 0 at the last stage? Because problem states that "the distance will be strictly increasing" so it means no stationary.
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I made it an equality condition, because I'm looking for a single critical value of theta.
Relevant wiki: Problem solving 2D
The motion is parabolic:
y = a x 2 + b x
where b = tan θ . Just combine the horizontal equation of motion x = V 0 t cos θ with the vertical one y = − g ′ t 2 / 2 + V 0 t sin θ in order to obtain that.
Now the distance from the origin:
d 2 = x 2 + y 2 = x 2 [ 1 + ( a x + b ) 2 ]
Derive it with respect to x (which I use here instead of time as independent variable because x ( t ) is a monotonic function of time):
2 d d ′ = 2 x ( 2 a 2 x 2 + 3 a b x + 1 + b 2 )
The prime denotes derivation with respect to x . Now, d and x are always positive, so d ′ > 0 if the discriminant of the second order polynomial between parenthesis is non-positive:
Δ 2 = 9 a 2 b 2 − 8 a 2 ( 1 + b 2 ) ≤ 0
From which we get:
b 2 ≤ 8
Therefore:
tan 2 α = 8
The result is already independent of mass, g ′ and V 0 .
Define x ^ to be the unit vector parallel to the projection of V 0 onto the plane, and y ^ to be the unit vector which points upwards normal to the plane.
Let r ( t ) = x ( t ) x ^ + y ( t ) y ^ be the ball's position vector and let C be the circle whose center is the origin and circumference passes through r ( t ) . The distance between the origin and r ( t ) is increasing if and only if the ball's velocity points outside of the circle. Hence;
d x d y ∣ ∣ ∣ ∣ r ( t ) > d x d y ∣ ∣ ∣ ∣ C
Since d x d y along any circle centered at the origin is y − x , we get that x ′ y ′ + y x > 0 or y y ′ + x x ′ > 0 .
Since this is a kinematic problem, it is true that y ( t ) = A t + B t 2 and x ( t ) = C t (the only acceleration is in the y-direction)
We get:
[ A t + B t 2 ] [ A + 2 B t ] + C 2 t > 0 ⇒ ( A 2 + C 2 ) + 3 A B t + 2 B 2 t 2 > 0
Note: we can divide through by t since we only care about when t > 0 .
For the above to be true for t > 0 , we must have no positive roots in t . In other words, either the discriminant is negative, or both roots are negative. Based on our knowledge of kinematics, we know that B corresponds with the y acceleration, which is negative. We also know A corresponds with the initial y velocity, which is positive. Hence, 4 B 2 − 3 A B , the t value which corresponds to the axis of symmetry of the parabola, is positive. Thus, we must have the discriminant be negative.
We get 9 A 2 B 2 − 8 B 2 ( A 2 + C 2 ) < 0 ⇒ C 2 A 2 < 8
We know A = V 0 sin ( θ ) and C = V 0 cos ( θ ) , so we get that t a n 2 ( θ ) < 8 . Since tan ( θ ) is increasing over our interval, we get that tan 2 ( α ) = 8 satisfies our conditions on α . This is true regardless of our chosen values for V 0 , m , and g .
Lets call the coordinates of the ball ( r ( t ) = x ( t ) , z ( t ) )
From the picture we can see that the equation of motion is
r ( t ) = ( v 0 cos ( θ ) t , v 0 sin ( θ ) t − 2 1 g t 2 )
Thus the distance of the ball from the axis origin is
∣ r ( t ) ∣ 2 = v 0 2 cos 2 ( θ ) t 2 + v 0 2 sin 2 ( θ ) t 2 − v 0 sin ( θ ) g t 3 + 4 1 g 2 t 4 = A t 2 + B t 3 + C t 4
with A = v 0 2 , B = − v 0 sin ( θ ) g and C = 4 1 g 2 . We want ∣ r ( t ) ∣ to be constantly increasing and so the ∣ r ( t ) ∣ 2 to be constantly increasing. That means we demand that
d t d ( A t 2 + B t 3 + C t 4 ) > 0 ⇒ 2 A t + 3 B t 2 + 4 C t 3 > 0
and because time is positive we devide with it
2 A + 3 B t + 4 C t 2 > 0
So for this to be satisfied the distinctive Δ = 9 B 2 − 8 A C must be negative! Thus we get
9 v 0 2 sin 2 ( θ ) g 2 − 8 v 0 2 g 2 < 0 ⇒ sin 2 ( θ ) < 9 8
In the liminiting case where θ = α , sin 2 ( α ) = 8 / 9 and so
tan 2 α = 1 − sin 2 α sin 2 α = 1 / 9 8 / 9 = 8
We see from the solution that the result is independent of the gravitational consant g (the planet we do the projectile) the initial velocity v 0 and the mass m of the object!
I "cheated": I graphed the distance from the origin in Excel, and varied the angle until I found the extremal value. I stopped refining when it became clear that the answer is 8. See the 3 figures below
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Relevant wiki: Projectile motion - Medium
The answer is independent of the values given.
The shortest distance is attained when the velocity vector v is perpendicular to the segment from the starting point d . It is well-known that { d x = v x 0 t d y = v y 0 t − 2 1 g t 2 { v x = v x 0 v y = v y 0 − g t They are perpendicular when their dot product is zero, i.e. 0 = d x v x + d y v y = v x 0 2 t + v y 0 2 t − 2 3 v y 0 g t 2 + 2 1 g 2 t 3 . We wish to find ratios of v y 0 and v x 0 for which this equation does not have solutions.
Divide the equation by t ; then ( v 0 x 2 + v 0 y 2 ) − 2 3 v 0 y ( g t ) + 2 1 ( g t ) 2 = C + B ( g t ) + A ( g t ) 2 = 0 . This is a quadratic equation; it has no solutions iff the discriminant is negative: D = B 2 − 4 A C = ( 2 3 v 0 y ) 2 − 2 v 0 x 2 − 2 v 0 y 2 < 0 . 4 1 v 0 y 2 < 2 v 0 x 2 . tan 2 θ = v 0 x 2 v 0 y 2 < 1 / 4 2 = 8 .
To illustrate this, I have plotted the graphs of d ( t ) for various angles.
The blue graph is for an angle of 6 5 ∘ , less than our critical angle. The black graph is for an angle of 7 5 ∘ . The red graph shows the angle we calculated, of approx. 7 0 . 5 ∘ . It has a horizontal inflection point toward the end of the motion. If the launch angle is made any greater, this inflection point will bifurcate into a local minimum and a local maximum.
We can also find the location of the projectile at this bifurcation point. If D = 0 , the solution of the quadratic above is given by g t = 2 A − B = 2 3 v 0 y . The velocity at that time will be ( v x , v y ) = ( v 0 x , − 2 1 v 0 y ) , and the direction of d is perpendicular; so that d x d y = − v y v x = 2 v 0 y v 0 x = tan θ 2 , so that the direction angle of d at that moment is equal to ϕ d = inv tan 2 1 ≈ 3 5 . 3 ∘ , again independent of the values of v 0 and g .
In fact, this direction angle ϕ d is exactly half of the launch angle: tan 2 ϕ d = 1 − ( tan ϕ d ) 2 2 tan ϕ d = 1 − 2 1 2 = 2 2 = 8 = tan θ .