Using the Gibbs description of an interphase, the necessary conditions
for equilibrium bf a closed, two-phase fluid system in the presence o
f gravity are the Laplace and Young equations and a condition on the c
hemical potentials. The last condition has been neglected in all previ
ous examinations of contact angles in a gravitational field. After int
roducing explicit expressions for the chemical potentials, we find tha
t the condition on the chemical potentials can be used to determine th
e pressure profile within the system. In a ''two-interface'' system in
which a liquid phase is both above and below a vapor phase and the va
por phase forms a solid-vapor interphase in one region, the pressure p
rofile in the liquid phases is the same as it would;have been if the v
apor phase were not there; thus in a gravitational field, the pressure
is smaller in the liquid phase above the vapor phase than it is in th
e liquid phase below the vapor phase. This results in the contact angl
e at the upper three-phase line necessarily being smaller than that at
the lower three-phase line. This difference in contact angles is conv
entionally referred teas contact angle hysteresis; however, we show th
at it is simply an equilibrium property of a capillary system in a gra
vitational held. The contact angle difference predicted to exist in th
e presence of gravity does not violate the Young equation, but the You
ng equation does impose a restriction on the equilibrium adsorption is
otherms at the solid-vapor and solid-liquid interfaces. (C) 1998 Ameri
can Institute of Physics.