Explanation: Unspeakable beauty and unimaginable bedlam can be found together in the Trifid Nebula. Also known as M20, this photogenic nebula is visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. The red-glowing gas results from high-energy starlight striking interstellar hydrogen gas. The dark dust filaments that lace M20 were created in the atmospheres of cool giant stars and in the debris from supernovae explosions. Which bright young stars light up the blue reflection nebula is still being investigated. The light from M20 we see today left perhaps 3000 years ago, although the exact distance remains unknown. Light takes about 50 years to cross M20.

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

Publikacii s klyuchevymi slovami: M 20 - dust - Trehrazdel'naya tumannost' Publikacii so slovami: M 20 - dust - Trehrazdel'naya tumannost'
Sm. takzhe: Sem' Sester v pyli Temnyi Morskoi konek v Cefee Svet, temnota i pyl' v Trehrazdel'noi tumannosti NGC 7023: tumannost' Iris Triplet v Strel'ce Prekrasnaya Trehrazdel'naya tumannost' Pleyady: Sem' Sester v pyli Vse publikacii na tu zhe temu >>