The study of a classical ideal gas column of finite height H in a unif
orm gravitational field g is made by the microcanonical ensemble at en
ergy E. The primary functions of this ensemble, the phase volume and t
he density of states, are derived. Related statistical quantities, suc
h as the entropy, the temperature and the heat capacity, are also repo
rted. The equivalence in the thermodynamic limit between the calculate
d microcanonical expressions and those obtained from the canonical ens
emble is shown numerically. The expression for the temperature is used
to analyze the temperature change when the gas is permitted to expand
into an evacuated region increasing the height of the column from H-1
to H-2. The microcanonical single-particle momentum and height distri
butions are also reported.