Orbital Trajectory

A uniform solid sphere of mass 1 0 11 kg 10^{11} \, \text{kg} and radius 1 m 1 \, \text{m} is situated at the origin. A massive particle is launched from the sphere's surface at ( x , y , z ) = ( 1 , 0 , 0 ) m (x,y,z) = (1,0,0) \, \text{m} with velocity ( v x , v y , v z ) = ( 1.5 , 1.5 , 1.5 ) m/s (v_x,v_y,v_z) = (1.5,1.5,1.5) \, \text{m/s} .

When the particle lands again on the sphere, what is its x x -coordinate (in meters)?

Details and Assumptions:
- Universal gravitational constant G = 6.67 × 1 0 11 [ SI units ] G = 6.67 \times 10^{-11} \, [\text{SI units}]
- The particle mass is much smaller than that of the sphere
- Ignore any effects of General Relativity
- The only gravity is due to the sphere


The answer is -0.3651.

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1 solution

Mark Hennings
May 14, 2018

Introduce vectors i = ( 1 0 0 ) j = 1 2 ( 0 1 1 ) k = 1 2 ( 0 1 1 ) \mathbf{i} \; = \; \left(\begin{array}{c} 1 \\ 0 \\ 0 \end{array}\right) \hspace{1cm} \mathbf{j} \; = \; \tfrac{1}{\sqrt{2}}\left(\begin{array}{c} 0 \\ 1 \\ 1 \end{array}\right) \hspace{1cm} \mathbf{k} \; = \; \tfrac{1}{\sqrt{2}}\left(\begin{array}{c} 0 \\ -1 \\ 1 \end{array}\right) Then i , j , k \mathbf{i},\mathbf{j},\mathbf{k} are a right-handed orthonormal triad such that the initial displacement and velocity of the particle are i \mathbf{i} and 3 2 i + 3 2 j \tfrac32\mathbf{i}+\tfrac{3}{\sqrt{2}}\mathbf{j} . The equation of motion of the particle is r ¨ = G M r 3 r \ddot{\mathbf{r}} \; = \; -\tfrac{GM}{r^3}\mathbf{r} so that d d t ( r r ˙ ) = r r ¨ = 0 \tfrac{d}{dt}(\mathbf{r} \wedge \dot{\mathbf{r}}) = \mathbf{r} \wedge \ddot{\mathbf{r}} = \mathbf{0} , so that r r ˙ = 3 2 k \mathbf{r} \wedge \dot{\mathbf{r}} = \tfrac{3}{\sqrt{2}}\mathbf{k} is constant. The motion of the particle is in the i , j \mathbf{i},\mathbf{j} plane.

If we introduce θ \theta so that r = r cos θ i + r sin θ j \mathbf{r} \; = \; r\cos\theta\mathbf{i} + r\sin\theta\mathbf{j} then the equation of motion tells us that r 2 θ ˙ = 3 2 r ¨ r θ ˙ 2 = G M r 2 r^2\dot{\theta} \; = \; \tfrac{3}{\sqrt{2}} \hspace{2cm} \ddot{r} - r\dot{\theta}^2 \; = \; -GMr^{-2} If we define u = r 1 u = r^{-1} then d 2 u d θ 2 + u = 2 9 G M \frac{d^2u}{d\theta^2} + u \; = \; \tfrac29GM so that u = 2 9 G M + A cos θ + B sin θ u = \tfrac29GM + A\cos\theta + B\sin\theta for some A , B A,B . Initially r = 1 r=1 and r ˙ = 3 2 \dot{r} = \tfrac32 , and hence we have that u = 1 u = 1 and d u d θ = 1 2 \tfrac{du}{d\theta} = -\tfrac{1}{\sqrt{2}} initially, and hence u = 2 9 G M + ( 1 2 9 G M ) cos θ 1 2 sin θ u \; = \; \tfrac29GM + \big(1 - \tfrac29GM\big)\cos\theta - \tfrac{1}{\sqrt{2}}\sin\theta The particle strikes the sphere when u = 1 u=1 , which means either sin 1 2 θ = 0 \sin\tfrac12\theta = 0 (the launch point) or tan 1 2 θ = 9 2 ( 2 G M 9 ) \tan\tfrac12\theta \; = \; \frac{9}{\sqrt{2}(2GM - 9)} Since the position vector of the particle at the point of impact is cos θ i + sin θ j \cos\theta \mathbf{i} + \sin\theta\mathbf{j} , we deduce that the x x -coordinate ot the point of impact is cos θ \cos\theta , where θ = 2 tan 1 ( 9 2 ( 2 G M 9 ) ) \theta \; = \; 2\tan^{-1}\left(\frac{9}{\sqrt{2}(2GM-9)}\right) For the given values of G G and M M , this makes the answer 0.365116... \boxed{-0.365116...}

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