Its weight would be one-quarter its weight on Earth when it is twice as far from the center of the Earth.
According to Newton's law of universal gravitation, when the astronomy textbook is on the earth, its weight, W equals the force of attraction of the earth on it, F.
So, W = F = GMm/R² where
Now, when the astronomy textbook is shot into space at a distance twice its initial distance, that is R' = 2R, its new weight, W' is
W' = GMm/R'²
Substituting the value of R' into the equation, we have
W' = GMm/(2R)²
W' = GMm/4R²
W' = W/4 (since W = GMm/R²)
So, its weight would be one-quarter its weight on Earth when it is twice as far from the center of the Earth.
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