Consider a planet covered in
water ice with a uniform albedo of 0.75. The planet is tide-locked
(that is, the same face always points to the Sun, while the other
side is in perpetual night). (a) Compute the solar constant needed
to begin to melt some of this ice. (You can assume that there is no
atmosphere, so that each bit of the planet’s surface is in
equilibrium with the solar radiation it absorbs.)