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)
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: 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: Prekrasnaya Trehrazdel'naya tumannost' NGC 6188: drakony v Zhertvennike Ou4: tumannost' Gigantskii Kal'mar RCW 85 Sh2-132: tumannost' Lev M78 ot kosmicheskogo teleskopa "Evklid" IC 1795: tumannost' Ryb'ya golova Vse publikacii na tu zhe temu >>