By considering the equilibrium of a small volume element, show that in a fluid
in equilibrium under pressure and gravitational forces, \(\nabla p=\rho
\boldsymbol{g}\), where \(\rho\) is the density and \(p\) the pressure (the
equation of hydrostatic equilibrium). Deduce that, for an incompressible fluid
of uniform density \(\rho, p+\rho \Phi\) is a constant. Use this result to
obtain a rough estimate of the pressure at the centre of the Earth. (Mean
density of Earth \(=5.5 \times 10^{3} \mathrm{~kg} \mathrm{~m}^{-3}\). Note that
the pressure at the surface is essentially zero. The actual pressure at the
centre is more than this estimate - in fact about \(3.6 \times 10^{11}
\mathrm{~Pa}\) - because of the non-uniformity of \(\rho .\) It should be noted
that - as indicated in Problem 12 - even very small departures from
hydrostatic equilibrium would result in collapse on a short time scale, only
checked by an increase in internal pressure via other processes.)