Previous work by K. A. Tryka et al. (Science 261, 751-754, 1993) has s
hown that the profile of the 2.148-mu m band of solid nitrogen can be
used as a ''thermometer'' and determined the temperature of nitrogen i
ce on Triton to be 38(-1)(+2) K. Here we reevaluate that data and refi
ne the temperature value to 38 +/- 1 K. Applying the same technique to
Pluto we determine that the temperature of the N-2 ice on that body i
s 40 +/- 2 K. Using this result we have created a nonisothermal flux m
odel of the Pluto-Charon system, The model treats Pluto as a body with
symmetric N-2 polar caps and an equatorial region devoid of N-2. Comp
arison with the infrared and millimeter flux measurements shows that t
he published fluxes are consistent with models incorporating extensive
N-2 polar caps (down to +/-15 degrees or 20 degrees latitude) and an
equatorial region with a bolometric albedo less than or equal to 0.2.
(C) 1994 Academic Press, Inc.