The properties of metallic hydrogen-nonmetallic helium mixtures are of cons
iderable interest for planetary modelling. In the light of the unfavourable
outlook for reliable measurements under the extraordinarily high temperatu
res and pressures prevailing in the planet's interiors it becomes interesti
ng to study the phases of fluid mercury-helium mixtures which might serve a
s a model for the hydrogen-helium-system. At sufficiently high density, non
metallic expanded mercury experiences a transition to a conducting state no
t unlike that recently observed in hydrogen. The experimental results for m
ercury-helium, which extend to pressures of 4000 bar and temperatures to 18
00 K, show that two distinct fluid phases exist at supercritical temperatur
es and high pressures. (C) 1999 Elsevier Science B.V. All rights reserved.