We have mapped the dwarf galaxy NGC 1569 at 1.2 mm with the MPIfR bolometer
at the IRAM 30m telescope. The total flux density allows us, together with
the IRAS fluxes densities at 12, 25, 60 and 100 mum, to draw conclusions a
bout the dust properties and to estimate the total dust mass. We find stron
g evidence for a significant enhancement of very small grains and a depleti
on of PAHs.