Explanation: The Pelican Nebula is slowly being transformed. IC 5070, the official designation, is divided from the larger North America Nebula by a molecular cloud filled with dark dust. The Pelican, however, receives much study because it is a particularly active mix of star formation and evolving gas clouds. The above picture was produced in two specific colors to better understand these interactions. Here, hot hydrogen gas glows in red, while cooler Sulfur glows blue-green. The light from young energetic stars is slowly transforming the cold gas to hot gas, with the advancing boundary between the two known as an ionization front. Particularly dense filaments of cold gas are seen to still remain. Millions of years from now this nebula might no longer be known as the Pelican, as the balance and placement of stars and gas will leave something that appears completely different.

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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: nebula - ionization - Pelican Nebula - ionization front - Pelican Publikacii so slovami: nebula - ionization - Pelican Nebula - ionization front - Pelican
Sm. takzhe: Raznocvetnye oblaka i zvezdy okolo ρ Zmeenosca Tumannosti: ot Chaiki do Kalifornii Gaz, pyl' i zvezdy tumannosti Pelikan Tumannost' Akula NGC 7380: tumannost' Koldun Galaktika pozadi zvezd, gaza i pyli Zvezdy, pyl', stolby i strui v tumannosti Pelikan Vse publikacii na tu zhe temu >>