Consider a small, spherical particle of radius \(r\) located in space a distance
\(R\) from the Sun. (a) Show that the ratio \(F_{\mathrm{rad}} /
F_{\mathrm{grav}}\) is proportional to \(1 / r,\) where \(F_{\mathrm{rad}}\) is the
force exerted by solar radiation and \(F_{\mathrm{grav}}\) is the force of
gravitational attraction. (b) The result of part
(a) means that, for a sufficiently small value of \(r,\) the force exerted on
the particle by solar radiation exceeds the force of gravitational attraction.
Calculate the value of \(r\) for which the particle is in equilibrium under the
two forces. (Assume that the particle has a perfectly absorbing surface and a
mass density of \(1.50 \mathrm{g} / \mathrm{cm}^{3} .\) Let the particle be
located \(3.75 \times 10^{11} \mathrm{m}\) from the Sun, and use \(214 \mathrm{W}
/ \mathrm{m}^{2}\) as the value of the solar intensity at that point.)