We report the discovery of widespread water vapour absorption in the 2
(12)-1(01) 179.5 mu m transition toward the SgrB2 molecular cloud. The
data were obtained with the Long Wavelength Spectrometer (LWS) on boa
rd the ISO satellite. A raster map centered on SgrB2 made with the LWS
grating clearly shows the 179.5 mu m H2O line in absorption against t
he far-infrared continuum at all observed positions with a line absorp
tion depth of similar to 15%. The grating data are complemented with F
abry-Perot observations of the H2O 179.5 and 174.6 mu m lines, and the
(H2O)-O-18 181.05 mu m. The transitions connecting the ground level s
how a broad absorption profile between -150 and 100 kms(-1) proving th
at water vapour is present in the molecular gas along the line of sigh
t toward SgrB2. The H2O absorption lines probably arise in the tenuous
and extended envelope of SgrB2 where collisional excitation is neglig
ible and the excitation is mainly due to absorption of photons emitted
by the dust. We derive a lower limit to the H2O abundance in SgrB2 of
10(-5).