Step 1: Identifying the dependencies and dimensions
We are given that the time period \( T \) depends on the radius of orbit \( R \), the mass of the earth \( M \), and the gravitational constant \( G \). Mathematically, we assume:
\[
T \propto R^a M^b G^c.
\]
Writing dimensions:
\[
[T] = T, \quad [R] = L, \quad [M] = M, \quad [G] = M^{-1}L^3T^{-2}.
\]
Step 2: Equating dimensions
Since,
\[
T = K R^a M^b G^c,
\]
taking dimensions on both sides:
\[
[T] = [L]^a [M]^b [M^{-1} L^3 T^{-2}]^c.
\]
Expanding:
\[
T = L^a M^b M^{-c} L^{3c} T^{-2c}.
\]
\[
= L^{a + 3c} M^{b - c} T^{-2c}.
\]
Step 3: Solving for exponents
Comparing powers of \( T \):
\[
-2c = 1 \quad \Rightarrow \quad c = -\frac{1}{2}.
\]
Comparing powers of \( M \):
\[
b - c = 0 \quad \Rightarrow \quad b = c = -\frac{1}{2}.
\]
Comparing powers of \( L \):
\[
a + 3c = 0 \quad \Rightarrow \quad a = -3c = \frac{3}{2}.
\]
Step 4: Final expression
Thus, the expression for \( T \) is:
\[
T = K \sqrt{\frac{R^3}{GM}}.
\]
Step 5: Conclusion
Thus, the correct answer is:
\[
K \sqrt{\frac{R^3}{GM}}.
\]