Earlier studies have failed to establish a consensus on the amount of
mercury vapour released from dental amalgam restorations. The purpose
of this study was to accurately and quantitatively measure the equilib
rium mercury vapour pressure from dental amalgam. The vapour pressure
was measured using a quartz crystal microbalance as a function of the
load from 0-5.4 MPa. Auger spectra were collected of the as-formed and
argon ion sputter cleaned dental amalgam surface. For the as-formed s
urface the mercury vapour density is zero with no load and increases t
o 0.6 mu g m(-3) at 5.4 MPa. Following cleaning the mercury, vapour de
nsity increased to a maximum value of 15 mu g m(-3). The Auger spectra
of the as-formed surfaces were dominated by features associated with
carbon and oxygen. These spectral results in concert with the mercury
vapour density measurements indicate that the oxide film on the as-for
med surfaces inhibited the release of mercury vapour. The results of t
his experiment provide an upper limit for the amount of mercury vapour
released by dental amalgams. Under conditions simulating the oral cav
ity this value would be reduced by oxides that form on the surface of
dental amalgam restorations. (C) 1998 Elsevier Science Ltd. All rights
reserved