The equation d2u / dx2 + d2u / dy2 + d2u / dz2 = 0, transformed to polar coordinates by putting x = r sin θ cos ϕ , y = r sin θ sin ϕ , z = r cos θ , becomes, as is well known, d2u / dθ2 + cot θdu / dθ + 1/(sin θ ) 2d2u / dϕ2 + r2d2u / dr2 + 2 rdu / dr = 0, which may be written in the form {(sin θd / dθ ) 2 + ( d / dϕ ) 2 + (sin θ ) 2rd / dr ( rd/dr + 1)} u = 0; . . . . (1.) and if it be assumed that u = u0 + u1r + u2r2 + . . . . ., then by substituting this value of u in either of the two equations last written, that u n is a function of θ and ϕ satisfying the equation {(sin θd / dθ ) 2 + ( d / dϕ ) 2 + n ( n + 1)(sin θ ) 2 } u n =0, . . . . . (2.) which, under a slightly different form, is commonly called the Equation of Laplace’s Functions .