Explanation: The Trifid Nebula, also known as Messier 20, is easy to find with a small telescope, a well known stop in the nebula rich constellation Sagittarius. But where visible light pictures show the nebula divided into three parts by dark, obscuring dust lanes, this penetrating infrared image reveals filaments of glowing dust clouds and newborn stars. The spectacular false-color view is courtesy of the Spitzer Space Telescope. Astronomers have used the Spitzer infrared image data to count newborn and embryonic stars which otherwise can lie hidden in the natal dust and gas clouds of this intriguing stellar nursery. As seen here, the Trifid is about 30 light-years across and lies only 5,500 light-years away.

News: Leap second to be added to 2016.

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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: M 20 - Trifid nebula - infrared - star formation - Trehrazdel'naya tumannost' - infrakrasnoe izluchenie Publikacii so slovami: M 20 - Trifid nebula - infrared - star formation - Trehrazdel'naya tumannost' - infrakrasnoe izluchenie
Sm. takzhe: NGC 1893 i Golovastiki v IC 410 Zvezdnaya fabrika Mess'e 17 Zvezdoobrazovanie v tumannosti Pakman Galaktika Sombrero v infrakrasnom svete Zvezdy, pyl' i tumannost' v NGC 6559 V centre Trehrazdel'noi tumannosti NGC 1333: zvezdnye yasli v Persee Vse publikacii na tu zhe temu >>