Kepler's law is still confusing me even with all the info I've gathered, I attached an example question that I've been stuck on for a bit to work on.

Given
Mass is
[tex]m=5.98\times10^{24}kg[/tex]Distance is
[tex]d=1.92\times10^8m[/tex]To find
The orbital period.
Explanation
The orbital speed is given by
[tex]v=\sqrt[]{\frac{Gm}{d}}[/tex]where G is the gravitational constant
Putting the values,
[tex]\begin{gathered} v=\sqrt[]{6.67\times10^{-11}\times5.98\times\frac{10^{24}}{1.92\times10^8}} \\ \Rightarrow v=1441.33\text{ m/s} \end{gathered}[/tex]The orbital period is
[tex]\begin{gathered} T=\frac{2\pi\text{ d}}{v} \\ \Rightarrow T=\frac{2\pi\times1.92\times10^8}{1441.33} \\ \Rightarrow T=836985s\text{ =9.7 days} \end{gathered}[/tex]Conclusion
The orbital period is 9.7 days