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> Emission Nebula
> Reflection Nebula
> Dark Nebula
> Planetary Nebula
> Supernova Remnant
> Crab Nebula
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Nebula, a localized
mass of the gases and finely divided dust particles that are spread
throughout interstellar space. Before the invention of the telescope, the
term nebula (Latin, “cloud”) was applied to all celestial objects of a
diffuse appearance. As a result, many objects now known to be star
clusters or galaxies were called nebulae.
Nebulae exist within other galaxies as well as in our own, the
Milky Way.
They are classified as planetary nebulae, supernova remnants, and diffuse
nebulae, including reflecting, emission, and dark nebulae. Small, very
bright nebulae known as Herbig-Haro objects are found in dense
interstellar clouds, and are probably the products of gas jets expelled by
new stars in the process of formation.
Planetary nebulae, or planetaries, are so called because many of them
superficially resemble planets through telescopes. They are actually
shells of material that an old star of average mass sheds during a late,
red giant stage in its evolution, before becoming a white dwarf. The Ring
Nebula in the constellation Lyra, a typical planetary, has a rotational
period of 132,900 years and a mass calculated to be about 14 times that of
the Earth's sun. Several thousand planetaries have been discovered in the
Milky Way. More spectacular but fewer in number are nebulae that are the
fragments of supernova explosions, perhaps the most famous of which is the
Crab Nebula in Taurus, now fading at the rate of about 0.4 per cent per
year. Nebulae of this kind are strong emitters of radio waves, as a result
of the explosions that formed them and the probable pulsar remnants of the
original star.
Diffuse nebulae are extremely large, often many light years wide, with no
definite outline and a tenuous, cloud-like appearance. They are either
luminous or dark. The former shine as a result of the light of
neighbouring stars. They include some of the most striking objects in the
sky, such as the Great Nebula in Orion (the middle “star” in the Sword).
The tremendous streams of matter in the diffuse nebulae are intermingled
in violent, chaotic currents. Many thousands of luminous nebulae are
known. Spectral studies show that light emanating from them consists of
reflected starlight and also, in so-called emission nebulae, of stimulated
radiation coming from ionized gases and dust in the nebulae.
Dark, diffuse nebulae are observed as nonluminous or faintly luminous
clouds, obscuring portions of the Milky Way. They are too distant from the
stimulation of neighbouring stars to reflect or emit much light of their
own. One of the most famous dark nebulae is the Horsehead Nebula in Orion,
so named after the shape of the dark mass silhouetted in front of a more
luminous nebular region. The longest dark rift observed on photographic
plates of the star clouds of the Milky Way is a succession of dark
nebulae. Both dark and luminous nebulae are considered likely sites for
the processes of dust-cloud condensation that lead to the formation of new
stars.
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