The dark regions in the starry night sky are not pockets in the universe
that are devoid of stars as had long been thought. Rather, they are dark
because of interstellar dust that hides the stars behind it. Although its
visual effect is so pronounced, dust is only a minor constituent of the
material, extremely low in density, that lies between the stars. Dust accounts
for about one percent of the total mass of interstellar matter. The rest is
hydrogen and helium gas, with small amounts of other elements. The interstellar
material, rather like terrestrial clouds, comes in all shapes and sizes. The
average density of interstellar material in the vicinity of our Sun is 1,000 to
10,000 times less than the best terrestrial laboratory vacuum. It is only
because of the enormous interstellar distances that so little material per unit
of volume becomes so significant. Optical astronomy is most directly affected,
for although interstellar gas is perfectly transparent, the dust is not.
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