Dark nebula
In astronomy, the dust of interstellar medium seems to be concentrated in large clouds which appears as star-poor regions called dark nebulae.
Molecular Cloud Barnard 68 is a dark nebula, not a hole in space. No stars are visible in the center which indicates that Barnard 68 is relatively nearby, with measurements placing it about 500 light-years away and half a light-year across. These clouds are likely places for new stars to form.
Dark nebulae can be seen if they obscure part of a emission or reflection nebula (eg. the Horsehead nebula) or if they block out background stars (eg. the Coalsack).
The form of such dark clouds is very irregular: they have no clearly defined outer boundaries and sometimes take on convoluted serpentine shapes. The largest dark nebulae are visible to the naked eye, appearing as dark patches against the brighter background of the Milky Way.
The hydrogen of these opaque dark clouds exists in the form of molecular hydrogen. The largest nebulae of this type, the so-called giant molecular clouds (GMC), are more than a million times as massive as the Sun. They contain much of the mass of the interstellar medium, are some 150 light-years across, and have an average density of 100 to 300 molecules per cubic centimetre and an internal temperature of only 7 to 15 K. Molecular clouds consist mainly of gas and dust but contain many stars as well. The cloud cores are completely hidden from view and would be undetectable except for the microwave emissions from their constituent molecules. This radiation is not absorbed by dust and readily escapes the cloud. The material within the clouds is clumped together in all sizes, with some clouds ranging down to the masses of individual stars, small clumps may extend about one light-year across. The clouds have an internal magnetic field that provides support against their own gravity.
GMCs play an important role in the Galaxy dynamics: when a star passes near a GMC, the considerable gravity pull will perturb the star's orbit by a not-insignificant amount. After repeated near encounters, a middle-aged star will have significant velocity components in all directions, instead of an almost circular orbit like a newborn star (this is because the newborn star inherits the circular orbit of the GMC where it was born). This gives the astronomer another tool to estimate star ages, and contributes to explain the thinkness of the galactic disk.
In the inner regions of dark nebulae important events take place: the formation of stars.
