To find the distances above and below Earth's surface where an object's weight is constant, we analyze gravitational force variations.
Gravitational force at a distance \( x \) from Earth's center (where \( R \) is Earth's radius) is:
1. Above the surface (at height \( h \)):
\(F_{\text{above}} = \frac{GMm}{(R+h)^2}\)
2. Below the surface (at depth \( d \)):
\(F_{\text{below}} = \frac{GMm}{R^2} \cdot \left(1 - \frac{d}{R}\right)\)
Setting these forces equal:
\(\frac{GMm}{(R+h)^2} = \frac{GMm}{R^2} \cdot \left(1 - \frac{d}{R}\right)\)
Canceling \( GMm \) and solving for \( h \) in terms of \( d \):
\(\frac{1}{(R+h)^2} = \frac{1}{R^2} \left(1 - \frac{d}{R}\right)\)
Further simplification yields:
\(R^2 = (R+h)^2 \left(1 - \frac{d}{R}\right)\)
For symmetric weight, \( d = h \). Substituting this:
\((R+h)^2 \left(1 - \frac{h}{R}\right) = R^2\)
Solving this quadratic equation for \( h \):
\(h = (\sqrt5 - 1)\frac{R}{2}\)
Thus, an object has the same weight at a distance of \( (\sqrt5 - 1)\frac{R}{2} \) above and below Earth's surface.
This confirms \( (\sqrt5 - 1)\frac{R}{2} \) as the correct distance.