Explanation: By starlight this eerie visage shines in the dark, a crooked profile evoking its popular name, the Witch Head Nebula. In fact, this entrancing telescopic portrait gives the impression that the witch has fixed her gaze on Orion's bright supergiant star Rigel. More formally known as IC 2118, the Witch Head Nebula spans about 50 light-years and is composed of interstellar dust grains reflecting Rigel's starlight. The blue color of the Witch Head Nebula and of the dust surrounding Rigel is caused not only by Rigel's intense blue starlight but because the dust grains scatter blue light more efficiently than red. The same physical process causes Earth's daytime sky to appear blue, although the scatterers in Earth's atmosphere are molecules of nitrogen and oxygen. Rigel, the Witch Head Nebula, and gas and dust that surrounds them lie about 800 light-years away.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Rigel - Witch Head Nebula - Rigel' - tumannost' Golova Ved'my Publikacii so slovami: Rigel - Witch Head Nebula - Rigel' - tumannost' Golova Ved'my
Sm. takzhe: Rigel' i tumannost' Golova Ved'my IC 2118: tumannost' Golova Ved'my Rigel' v shirokom pole Upyr' v IC 2118 Tumannost' Golova Ved'my Pylayushii bolid mezhdu Tumannost'yu Oriona i Rigelem Vesennii Orion Vse publikacii na tu zhe temu >>