In a sealed blackbody cavity with gas, pressure gradients commonly tak
e three forms: (a) statistical fluctuations, (b) transients associated
with the system relaxing toward equilibrium, and (c) equilibrium pres
sure gradients associated with potential gradients (such as with gravi
ty). In this paper, it is shown that in the low-density (collisionless
) regime, a fourth type of pressure gradient may arise, this due to st
eady-state differential thermal desorption of surface species from che
mically active surfaces. This gas phase is inherently nonequilibrium i
n character. Numerical simulations using realistic physical parameters
support the possibility of this gas phase and indicate that these nov
el pressure gradients might be observable in the laboratory; candidate
chemical systems are suggested.