Dust particles are agglomerations of billions of atoms. They are
thought to be either silicate material or graphite material sometimes
with a coating or water ice. Because they are composed of the
trace elements of the Universe, they are exceedingly rare compared
to hydrogen
and helium in the interstellar medium. There is roughly 1 hydrogen
atom per sugar cube (per cubic centimeter) in the ISM while
there is roughly 1 dust particle (grain) per cubic footbal
field in the ISM.
They are the principal
absorbers and scatterers of radiation, however.
Hydrogen atoms can only absorb very specific energies of radiation. They
are transparent to the bulk of the radiation produced by stars and so
they do not dim distant stars very much. Dust absorbs radiation
over large wavelength regions very efficiently.
Dust only lets us
see out to a few kiloparsecs (less than 5 - 10,000 light years into the
Milky Way
galaxy in optical light -- 1 parsec = 3.3 light years). This means that
Dust makes distant stars appear fainter than simply their distances
would imply ===> we overestimate the distances to stars and we cannot
see extremely distant stars.