Explanation
While Copernicus rightly observed that the planets revolve around the Sun, it was Johannes Kepler who correctly defined their orbits.
Gravitational force on the earth surface,
$$F_{G_s}= \dfrac{GMm}{R^{2}}$$
Gravitational force at a height 'h' above,
$$F_{G_{h}}= \dfrac{GMm}{(R+h)^{2}}$$
G.T. $$F_{G_{h}}= \dfrac{90}{100}(F_{G_{S}})$$
$$\Rightarrow \dfrac{GMm}{(R+h)^{2}}=\dfrac{9}{10}(\dfrac{GMm}{R^{2}})$$
$$\Rightarrow R+h=\sqrt{\dfrac{10}{9}}(R)$$
$$\Rightarrow 6370+h= \dfrac{3.162}{3} (6370)$$
$$\Rightarrow h=\dfrac{0.162 \times 6370}{3}=344$$ km
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