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Answer» Me = 4/3 π Re³ * d, where Re = Radius of Earth Me = Mass of EArth d = density of Earth (we assume it is uniform)
Let us find the gravity at a distance r from the center of Earth. Mass of Earth enclosed inside the radius r is :
M = 4/3 π r³ d = 4/3 π r³ (3Me /Re³ 4π) = Me r³/ Re³
Gravity at a location r distance AWAY from center of Earth is = G (Me r³/Re³) / r² THUS g' = G Me r / Re³ = g r /Re , where g = acceleration DUE to gravity at the surface of Earth. Thus if r = 0, g' = 0.
In other words, M varies as cube of R and in the denominator, we have a square of R. Thus g is proportional to R inside the Earth's surface.
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