Two small identical uniform spheres of density \(\rho\) and radius \(r\) are
orbiting the Earth in a circular orbit of radius \(a\). Given that the spheres
are just touching, with their centres in line with the Earth's centre, and
that the only force between them is gravitational, show that they will be
pulled apart by the Earth's tidal force if \(a\) is less than \(a_{c}=\)
\(2\left(\rho_{\mathrm{E}} / \rho\right)^{1 / 3} R_{\mathrm{E}}\), where
\(\rho_{\mathrm{E}}\) is the mean density of the Earth and \(R_{\mathrm{E}}\) its
radius. (This is an illustration of the existence of the Roche limit, within
which small planetoids would be torn apart by tidal forces. The actual limit
is larger than the one found here, because the spheres themselves would be
distorted by the tidal force, thus enhancing the effect. It is
\(a_{\mathrm{c}}=2.45\left(\rho_{\mathrm{E}} / \rho\right)^{1 / 3}
R_{\mathrm{E}} .\) For the mean density of the Moon, for example, \(\rho=3.34
\times 10^{3} \mathrm{~kg} \mathrm{~m}^{-3}\), this gives
\(\left.a_{\mathrm{c}}=2.89 R_{\mathrm{E}} \cdot\right)\)