A satellite is in a circular orbit around an unknown planet. The satellite has a speed of 1.48 x 10^4 m/s, and the radius of the orbit is 2.26 x 10^6 m. A second satellite also has a circular orbit around this same planet. The orbit of this second satellite has a radius of 9.14 x 10^6 m. What is the orbital speed of the second satellite? (7360 m/s) How to get anwser?
\[\left( \frac{ t1 }{ t2 } \right)^2=\left( \frac{ r1 }{ r2 } \right)^3\] rememeber this equation?
^ its the Kepler's third law equation. T stands for the period
I don't have that equation on my forumla sheet, is there another explanation?
do you want me to explain how i get that equation
this is how you get the equation sorry if it is too big
im not getting the right anwser ,i got 8000, the answer is supposed to be 7360
\[r_1 = 2.26 * 10^6\]\[r_2 = 9.14 * 10^6\]\[C_1=2\pi r_1 =2\pi*2.26*10^6\]\[C_2=2\pi r_2=2\pi*9.14*10^6\]\[v_1=1.48 * 10^4\]\[T_1 = \frac{C_1}{v_1}\]\[T_2=\frac{C_2}{v_2}\]\[v_2=\frac{C_2}{T_2}\]\[(\frac{T_1}{T_2})^2 = (\frac{r_1}{r_2})^3\]\[\frac{\frac{C_1 } {v_1 } } {\frac{C_2 } {v_2 } }=(\frac{r_1}{r_2} )^{3/2}\]\[\frac{C_1 v_2}{C_2 v_1} = (\frac{r_1}{r_2} )^{3/2}\]\[v_2 = (\frac{r_1}{r_2} )^{3/2} \frac{C_2 v_1}{C_1}\] Plug in the numbers. If you don't make any mistakes, I think you will be happy with the result.
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