Satellites In Orbit

Two identical rockets are in circular trajectories around Earth under the control of their engines. Rocket A is twice as far from the center of Earth as rocket B, yet they have the same centripetal acceleration. What is the ratio of the velocity of rocket B to that of rocket A, v B v A ? \dfrac{v_B}{v_A}?


The answer is 0.707.

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6 solutions

Michael Tang
Dec 14, 2013

Let r r be the distance from B to the center C of the Earth. Then, 2 r 2r is the distance from A to C. Thus, the acceleration of rocket B is v B 2 r , \dfrac{v_B^2}{r}, and the acceleration of rocket A is v A 2 2 r . \dfrac{v_A^2}{2r}. Therefore v B 2 r = v A 2 2 r v B 2 = v A 2 2 v B 2 v A 2 = 1 2 \begin{aligned} \dfrac{v_B^2}{r} &= \dfrac{v_A^2}{2r} \\ v_B^2 &= \dfrac{v_A^2}{2} \\ \dfrac{v_B^2}{v_A^2} &= \dfrac{1}{2} \end{aligned} so v B v A = 1 2 0.707 . \dfrac{v_B}{v_A} = \sqrt{\dfrac{1}{2}} \approx \boxed{0.707}.

oops.. i forgot the rario.. took it V1/v2 .. so got 1.414

Shakthi Janardhanan - 7 years, 4 months ago

Did the same way! Nice sol.n +1!!

Rishabh Tiwari - 5 years ago
Daniel Chiu
Nov 3, 2013

The centripedal acceleration is v 2 r \dfrac{v^2}{r} Let the radii of the orbits of the satellites be r A r_A and r B r_B . Then, r A = 2 r B r B r A = 1 2 r_A=2r_B\implies\dfrac{r_B}{r_A}=\dfrac{1}{2} v A 2 r A = v B 2 r B v B 2 v A 2 = r B r A v B v A = r B r A = 1 2 0.707 \dfrac{{v_A}^2}{r_A}=\dfrac{{v_B}^2}{r_B}\implies\dfrac{{v_B}^2}{{v_A}^2}=\dfrac{r_B}{r_A}\implies \dfrac{v_B}{v_A}=\sqrt{\dfrac{r_B}{r_A}}=\sqrt{\dfrac{1}{2}}\approx\boxed{0.707}

Oliver Welsh
Nov 4, 2013

We can use the formula a c = v 2 r a_c = \frac{v^2}{r} where a c a_c , v v and r r are the centripetal acceleration, velocity and radius respectively. Let v A v_A and v B v_B be the velocities of sattellite A and B respectively. Since they both have the same centripetal acceleration, it can be written that v A 2 2 r = v B 2 r \frac{v_A^2}{2r} = \frac{v_B^2}{r} v A 2 2 = v B 2 \frac{v_A^2}{2} = v_B^2 1 2 = v B 2 v A 2 \frac{1}{2} =\frac{v_B^2}{v_A^2} v B v A = 1 2 0.707 \frac{v_B}{v_A} = \frac{1}{\sqrt{2}} \approx \fbox{0.707}

Using the formula for the orbital velocity of any satellite: v = g R v= \sqrt{gR} , were g is gravitational acceleration and R is distance from Earth's centre.
Given that
R A = 2 R B R_{A} = 2R_{B}
Now, for the first rocket:
v A = g R A v_{A} = \sqrt{gR_{A}}
or v A = 2 g R B v_{A} = \sqrt{2gR_{B}} .................(1)
and for the second rocket:
v B = g R B v_{B} = \sqrt{gR_{B}} .....................(2)
So, by dividing eq2 by eq1,
v B v A = g R B 2 g R B \frac{v_{B}}{v_{A}} = \sqrt\frac{gR_{B}}{2gR_{B}}
v B v A = 1 2 \frac{v_{B}}{v_{A}} = \frac{1}{\sqrt{2}}
Therefore, v B v A = 0.707 \frac{v_{B}}{v_{A}} = \boxed{0.707}





Please note that the formula is derived by taking into account that the centripetal acceleration is supplied by gravitational acceleration which means that if both of the rockets have same centripetal acceleration then both have the same gravitational acceleration too and the factor "g" can be cancelled out.

Noor Muhammad Malik - 7 years, 7 months ago

I too did in the same way.

Adhiraj Dutta - 1 year, 5 months ago

a B = a A a_{B} = a_{A}

v B 2 / R B = v A 2 / R A v_{B}^{2} / R_{B} = v_{A}^{2} / R_{A}

we'll have :

v B / v A = ( R B / R A ) 1 / 2 v_{B}/v_{A} = (R_{B} / R_{A})^{1/2} which R A = 2 R B R_{A} = 2 R_{B}

finally we'll have :

v B / v A = 1 / 2 = 0.707 v_{B}/v_{A} = 1/ √2 = 0.707

a B = a A a_{B}=a_{A} ( v B ) 2 r B = ( v A ) 2 r A \frac{(v_{B})^{2}}{r_B}=\frac{(v_{A})^{2}}{r_A} ( v B ) 2 ( v A ) 2 = r B r A \frac{(v_{B})^{2}}{(v_{A})^{2}}=\frac{r_B}{r_A} in the problem it says that rocket A is twice as far from the center of the Earth as rocket B, so our equation will be ( v B ) 2 ( v A ) 2 = r B 2 ( r B ) \frac{(v_{B})^{2}}{(v_{A})^{2}}=\frac{r_B}{2(r_B)} v B v A = 1 2 \frac{v_{B}}{v_{A}}=\sqrt{\frac{1}{2}} v B v A = 0.707... \frac{v_{B}}{v_{A}}=0.707...

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