Small solid particles represent an important and ubiquitous component
of our and other galaxies and determine their overall spectral appeara
nce, Although they constitute only a minor ingredient by mass, they co
ntrol the thermal, dynamical, chemical, and ionization state of the co
ol and dense-phases of the interstellar medium, The grains are produce
d in the massive outflows of evolved stars, modified by shocks and rad
iative processing in the diffuse interstellar medium, and grow by accr
etion of ice mantles and coagulation in the dense cores of molecular c
louds, The last step in their lifecycle is consumption by forming star
s or their incorporation into planets, Cosmic dust particles are an ex
tremely exciting system if one is interested in the formation routes f
rom gas phase molecules to solids, the optical behaviour of small part
icles, and surface chemistry. Astronomical spectroscopy, together with
dedicated laboratory studies, has led to the identification of carbon
aceous solids, silicates, and different forms of ices in the Milky Way
.