Explanation: The Trifid nebula (M20) is a bright star forming region in Sagittarius, 5000 light years from Earth. In visible light, the interstellar gas cloud is crossed by dark, obscuring dust lanes which roughly divide the glowing emission nebula into three major parts. But the Trifid nebula's well known appearance is dramatically reversed in this infrared view. At longer infrared wavelengths the dust lanes are brighter, radiating more energy than the gas. This image was recorded by the liquid helium cooled Infrared Space Observatory (ISO).

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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: infrared - Trehrazdel'naya tumannost' - Mezhzvezdnaya pyl' - emissionnaya tumannost' - infrakrasnoe izluchenie Publikacii so slovami: infrared - Trehrazdel'naya tumannost' - Mezhzvezdnaya pyl' - emissionnaya tumannost' - infrakrasnoe izluchenie
Sm. takzhe: Slonovii hobot v Cefee Prizraki v Kassiopee Melott 15 v tumannosti Serdce Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Svet, temnota i pyl' v Trehrazdel'noi tumannosti Triplet v Strel'ce Prekrasnaya Trehrazdel'naya tumannost' Vse publikacii na tu zhe temu >>