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The Pelican Nebula in Gas Dust and Stars
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The Pelican Nebula in Gas Dust and Stars
Credit & Copyright: Roberto Colombari
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 featured picture was produced in three specific colors -- light emitted by sulfur, hydrogen, and oxygen -- that can help us to better understand these interactions. 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, visible in bright orange on the right. Particularly dense tentacles of cold gas 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 surely leave something that appears completely different.

Yearly Astronomy Review: APOD editor to speak in January in Philadelphia and New York City

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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.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: Pelican Nebula - ionization - Tumannost' Pelikan - Mezhzvezdnyi gaz - pyl' - zvezdoobrazovanie
Publikacii so slovami: Pelican Nebula - ionization - Tumannost' Pelikan - Mezhzvezdnyi gaz - pyl' - zvezdoobrazovanie
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