  In this letter we explore the environment of Pluto and Charon in the far
infrared with the main aim to identify the signs of any possible dust ring,
should it exist in the system. Our study is based on observations performed at
70 um with the PACS instrument onboard the Herschel Space Observatory at 9
epochs between March 14 and 19, 2012. The far-infrared images of the
Pluto-Charon system are compared to those of the point spread function (PSF)
reference quasar 3C454.3. The deviation between the observed Pluto-Charon and
reference PSFs are less then 1 sigma indicating that clear evidence for an
extended dust ring around the system was not found. Our method is capable of
detecting a hypothetical ring with a total flux of ~3.3 mJy at a distance of
~153 000 km (~8.2 Pluto-Charon distances) from the system barycentre. We place
upper limits on the total disk mass and on the column density in a reasonable
disk configuration and analyse the hazard during the flyby of NASAs New
Horizons in July 2015. This realistic model configuration predicts a column
density of 8.7x10^(-10) gcm^(-2) along the path of the probe and an impactor
mass of 8.7x10^(-5) g.
