Step 1: Understanding the Concept:
The acceleration due to gravity decreases both above the surface and below the surface, but at different rates. For small heights compared with the Earth's radius \(R\), the first order formulas hold.
Step 2: Key Formula or Approach:
1. Height \(h\): \(g_h = g\left(1 - \dfrac{2h}{R}\right)\).
2. Depth \(d\): \(g_d = g\left(1 - \dfrac dR\right)\).
Step 3: Detailed Explanation:
Set the two values equal, with \(d = 90\) km:
\[ \frac{2h}{R} = \frac dR \Rightarrow 2h = d \Rightarrow h = \frac{d}{2} = \frac{90}{2} = 45 \text{ km} \]
The height does not depend on the value of \(R\) here, because \(R\) cancels. Since \(g\) falls twice as fast with height as with depth, we need only half the distance above the surface. Options (A) 180 km would need a depth of 360 km, and option (C) 90 km would give a larger drop than the depth does.
Final Answer:
The height is 45 km, option (D).
\[ \boxed{45 \text{ km (D)}} \]