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Encyclopedia > Diffuse nebula
The Orion Nebula, a famous emission nebula.
The Orion Nebula, a famous emission nebula.

In astronomy, diffuse nebulae is the general term for illuminated nebulae. The three types of diffuse nebulae are reflection nebulae, emission nebulae and supernova remnants. They are diffuse as opposed to the non-diffuse dark nebulae, i.e. the particles have spread out. Download high resolution version (950x656, 108 KB) Objekt: M42 Orionnebel Datum: 10. ... Download high resolution version (950x656, 108 KB) Objekt: M42 Orionnebel Datum: 10. ... The Orion Nebula (also known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated south of Orions Belt. ... A giant Hubble mosaic of the Crab Nebula, a supernova remnant Astronomy (also frequently referred to as astrophysics) is the scientific study of celestial objects (such as stars, planets, comets, and galaxies) and phenomena that originate outside the Earths atmosphere (such as the cosmic background radiation). ... The Triangulum Emission Nebula NGC 604 The Pillars of Creation from the Eagle Nebula For other uses, see Nebula (disambiguation). ... The Witch Head reflection nebula (IC2118), about 1000 light years from earth, is associated with the bright star Rigel in the constellation Orion. ... An emission nebula is a cloud of ionized gas ( a plasma) emitting light of various colors. ... The Crab Nebula is an expanding cloud of gas created by the 1054 supernova. ... Dark Nebula Dark Nebula (Dark Zero in the original Japanese version) is a fictional character in the Kirby series of video games for Nintendo. ...


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Diffuse Nebulae (547 words)
Diffuse nebulae, sometimes inacurately referred to as gaseous nebulae, are clouds of interstellar matter, namely thin but widespread agglomerations of gas and dust.
The first diffuse nebula discovered was the Orion Nebula, M42, observed telescopically in 1610 by N.
Diffuse nebulae were longly be considered as distant, unresolved star clusters or star clouds, until in the 1860s spectroscopy revealed their gaseous nature by showing line spectra, in particular due to the pioneering research of William Huggins.
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