M16 The Eagle Nebula
The Eagle Nebula is a cloud of gas and dust in the constellation Serpens, mainly molecular hydrogen, some 7,000 light years away from us and 50 to 70 light years wide. It contains several stellar nurseries and is about 5.5
Goran Petrov
Nebulae are gigantic volumes of cosmic dust and/or gas, such as, and most of all, hydrogen and helium (the two most abundant atoms in the Universe). A cloud of this material can, when the conditions are ripe, collapse under its own gravity to create a new star or stars. Therefore, nebulae (or nebulas) are often stellar nurseries. In contrast, nebulae can also be created by an explosion of a dying star at the end of its main sequence.
Historically, all observed fuzzy objects (as opposed to pinpoint stars) were marked as nebulae, including galaxies – before they were understood to be galaxies in the early 20th century, and other deep space objects, such as globular clusters.
Nebulae are classified into: emission (such as M42), reflection (such as NGC 7023), dark (such as Barnard 33) or planetary nebulae (such as M57), or supernova remnants (such as M1).
The Eagle Nebula is a cloud of gas and dust in the constellation Serpens, mainly molecular hydrogen, some 7,000 light years away from us and 50 to 70 light years wide. It contains several stellar nurseries and is about 5.5
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