Gravitational intensity below the Earth's surface
Field inside the Earth
Consider a point inside the Earth at distance r from the centre (r< R). Let the field strength at that point be g. Therefore:
g = GM'/2
where M' is the mass of the Earth within radius r. But M' = r3M/R3. Therefore mg = GmMr/R and so:
Gravitational intensity (g) at radius r = go[r/R]
This means that theoretically the gravitational field intensity decreases linearly inside the Earth; however, this is only true if we assume that the Earth has a uniform density.
In fact the density increases with depth, the density of the Earth's crust being about 2.8x10
3 kg m
-3 while that of the surface of the core is 9.7x10
3 kg m
-3 .
This actually results in an increase in g for a short distance below the surface. The theoretical and actual variations are shown above. If R — r = h, then the theoretical reduction in gravitational intensity at a depth h below the surface is given by:
go – g = hgo/R
Gravitational intensity above the Earth's surface
Consider a point a distance r from the centre of the Earth where r > R.
g = GM/r
2 but g
o = GM/R
2.
Therefore:
g = go[R2/r2]
For a height h above the Earth's surface, r = R + h. Using the result above, and assuming that h is small compared with the radius of the Earth R, we can say that:
go – g = [2h/R]go
Thus the value of g at a depth h below the Earth's surface is greater than that at the same distance above the surface.
Example problem
Find the gravitational intensity at a point 1000 m above mean sea level.
Take R = 6400 km and go = 9.81 ms-2.
go – g = [2x103go]/6.4x106 = 0.31x10-3go = 0.003 ms-2
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