Answer:
[tex]v = 4.1 \times 10^4 m/s[/tex]
Explanation:
Here we know that for every satellite we have net force on it given as centripetal force
So it is given as
[tex]F_c = \frac{mv^2}{r}[/tex]
[tex]\frac{GMm}{r^2} = \frac{mv^2}{r}[/tex]
now we will have
[tex]v^2 = \frac{GM}{r}[/tex]
here we know that
r = distance from the center of the planet
[tex]r = 7.14 \times 10^7 + 4.40 \times 10^6[/tex]
[tex]r = 7.58 \times 10^7 m[/tex]
now we will have
[tex]v^2 = \frac{6.67 \times 10^{-11}(1.90 \times 10^{27})}{7.58 \times 10^7}[/tex]
[tex]v^2 = 1.67 \times 10^9 [/tex]
[tex]v = 4.1 \times 10^4 m/s[/tex]