Respuesta :
Answer:
r = 4.24x10⁴ km.
Explanation:
To find the radius of such an orbit we need to use Kepler's third law:
[tex] \frac{T_{1}^{2}}{T_{2}^{2}} = \frac{r_{1}^{3}}{r_{2}^{3}} [/tex]
where T₁: is the orbital period of the geosynchronous Earth satellite = 1 d, T₂: is the orbital period of the moon = 0.07481 y, r₁: is the radius of such an orbit and r₂: is the orbital radius of the moon = 3.84x10⁵ km.
From equation (1), r₁ is:
[tex] r_{1} = r_{2} \sqrt[3] {(\frac{T_{1}}{T_{2}})^{2}} [/tex]
[tex] r_{1} = 3.84\cdot 10^{5} km \sqrt[3] {(\frac{1 d}{0.07481 y \cdot \frac{365 d}{1 y}})^{2}} [/tex]
[tex] r_{1} = 4.24 \cdot 10^{4} km [/tex]
Therefore, the radius of such an orbit is 4.24x10⁴ km.
I hope it helps you!
The radius of orbit of Earth based on the data for the moon is [tex]4.24 \times 10^{4} \;\rm km[/tex].
Given data:
The orbital period of Earth Satellite is, T = 1 day.
We can use the Kepler's law to find the radius of orbit. Then applying the mathematical formula of Kepler's Law as,
[tex]\dfrac{T^{2}}{T'^{2}}=\dfrac{r^{2}}{r'^{2}}[/tex]
Here,
T' is the orbital period of moon. (T' = 0.07481 y)
r is the radius of Earth orbit.
r' is the radius of moon.
Solve for r as,
[tex]r = r' \sqrt{\dfrac{T^{2}}{T'^{2}}}\\\\r = 3.85 \times 10^{5} \times \sqrt{\dfrac{1^{2}}{({0.07481 \times 365)^{2}}}} \\\\\\r = 4.24 \times 10^{4} \;\rm km[/tex]
Thus, we can conclude that the radius of orbit of Earth based on the data for the moon is [tex]4.24 \times 10^{4} \;\rm km[/tex].
Learn more about the Kepler's law here:
https://brainly.com/question/1086445