Explanation: Newborn stars are forming in the Eagle Nebula. This image, taken with the Hubble Space Telescope in 1995, shows evaporating gaseous globules (EGGs) emerging from pillars of molecular hydrogen gas and dust. The giant pillars are light years in length and are so dense that interior gas contracts gravitationally to form stars. At each pillars' end, the intense radiation of bright young stars causes low density material to boil away, leaving stellar nurseries of dense EGGs exposed. The Eagle Nebula, associated with the open star cluster M16, lies about 7000 light years away.

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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 16 - Eagle Nebula - Tumannost' Orla Publikacii so slovami: M 16 - Eagle Nebula - Tumannost' Orla
Sm. takzhe: M16: stolpy sozidaniya Tumannost' Orla i goryachie rentgenovskie zvezdy M16: tumannost' Orla v glubokom pole M16: kolonna zvezdoobrazovaniya ot teleskopa "Dzheims Vebb" Stolpy sozidaniya Formiruyushaya zvezdy tumannost' Orla bez zvezd Feya tumannosti Orla Vse publikacii na tu zhe temu >>