Ascending a Sinusoidal Wire

A massive bead is attached to a wire in 3 D 3D space with the following parametrization: P = ( P x , P y , P z ) = α u 1 + 2 sin ( α ) u 2 . \vec{P} = (P_x, P_y, P_z) = \alpha \, \vec{u_1} + 2 \, \sin(\alpha) \, \vec{u_2}. In the above expression, P \vec{P} is a point on the wire, α \alpha is a spatial parameter, u 1 \vec{u_1} is a unit-vector in the direction of ( 1 , 2 , 3 ) (1,2,3) , and u 2 \vec{u_2} is a unit-vector in the direction of ( 1 , 5 , 3 ) (-1,5,-3) . Distances are in meters.

There is an ambient gravitational acceleration of 10 m/s 2 10 \text{ m/s}^2 in the z -z direction. The bead moves without losses over the wire.

Starting at the origin, the bead has an initial speed of v = 14 m/s , v = 14 \text{ m/s}, and is directed so that the z z -coordinate of the bead generally increases.

When the bead eventually stops moving and starts sliding back down again, how far is the bead from the origin (in meters)?

If the answer is D D , enter the result as 1000 D \lfloor 1000 \, D \rfloor .


The answer is 11139.

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1 solution

Nicola Mignoni
Feb 28, 2018

Due to the fact that the gravitational field is a conservative field, the Δ E \Delta E of energy does not depend on a particular walk of the point. So, we can write, for the 'Law of conservation of Energy', that

Δ E f , i = 0 \displaystyle \Delta E_{f,i}=0

Where E i E_i is the energy of the point at the origin, while E f E_f is the energy when it stops. Let's fix at z = 0 z=0 the potential energy E p = 0 E_p=0 . So at the beginning, the material point has just cinetic energy

E i = 1 2 m v i 2 \displaystyle E_i=\frac{1}{2}m v_{i}^2

At the end, when v f = 0 v_f=0 , it has just the amount of potential energy

E f = m g z f \displaystyle E_f=mgz_f

So

m g z f 1 2 m v i 2 = 0 , z f = 9.8 m \displaystyle mgz_f-\frac{1}{2}mv_{i}^2=0 \text{,} \quad z_f=9.8 m

We have to find the parametrization of P \vec{P} . Vectors u 1 = ( 1 , 2 , 3 ) \vec{u_1}=(1,2,3) and u 2 = ( 1 , 5 , 3 ) \vec{u_2}=(-1,5,-3) give us directions, but we need versors. So let's multiply each vector by the opposite of its module.

u 1 1 = 1 14 , u 2 1 = 1 35 \displaystyle ||\vec{u_1}||^{-1}=\frac{1}{\sqrt{14}} \text{,} \quad ||\vec{u_2}||^{-1}=\frac{1}{\sqrt{35}}

u 1 = ( 1 14 , 2 14 , 3 14 ) , u 2 = ( 1 14 , 5 14 , 3 14 ) \displaystyle \vec{u_1}=(\frac{1}{\sqrt{14}},\frac{2}{\sqrt{14}},\frac{3}{\sqrt{14}}) \text{,} \quad \vec{u_2}=(-\frac{1}{\sqrt{14}},\frac{5}{\sqrt{14}},-\frac{3}{\sqrt{14}})

And so P \vec{P} becomes

P ( α ) = ( α 14 2 sin α 35 , 2 α 14 + 10 sin α 35 , 3 α 14 6 sin α 35 ) \displaystyle \vec{P}(\alpha)=\left(\frac{\alpha}{\sqrt{14}}-\frac{2\sin{\alpha}}{\sqrt{35}},\frac{2\alpha}{\sqrt{14}}+\frac{10\sin{\alpha}}{\sqrt{35}},\frac{3\alpha}{\sqrt{14}}-\frac{6\sin{\alpha}}{\sqrt{35}}\right)

Since we previously calculated z f z_f , we know the z z -coordinate of the ending point. So

9.8 = 3 α 14 6 sin α 35 , α = 10.958 \displaystyle 9.8=\frac{3\alpha}{\sqrt{14}}-\frac{6\sin{\alpha}}{\sqrt{35}} \text{,} \quad \alpha=10.958

Eventually

P f = P ( α = 10.958 ) = ( 3.266 , 4.168 , 9.8 ) \displaystyle \vec{P_f}=\vec{P}(\alpha=10.958)=(3.266,4.168,9.8)

The distance of P f \vec{P_f} from the origin is

P f = 11.139 m \displaystyle ||\vec{P_f} ||=11.139m

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