Radiometric observations of Pluto and its moon, Charon, by the Infrared Ast
ronomical Satellite (IRAS) in 1983 marked the first detection of the system
at thermal wavelengths. Reexamination of the IRAS observations prove that
Pluto-Charon was detected several times during the all-sky survey in additi
on to the pointed observations that targeted the system. Pluto-Charon exhib
its thermal lightcurve variations that can be explained by the known variat
ion in hemispherically averaged geometric albedo with sub-Earth longitude.
Changes in albedo, however, are not sufficient to explain the lower than ex
pected fluxes observed at microwave wavelengths. (C) 1999 Academic Press.