Explanation: How do stars form? This stunning picture taken recently by the Hubble Space Telescope gives us a first hand glimpse. Here evaporating gaseous globules (EGGs) are captured emerging from pillars of molecular hydrogen and dust in the Eagle Nebula (M16). These pillars, dubbed "elephant trunks," are light years in length and are so dense that interior gas gravitationally contracts to form stars. At each pillars' end, the intense radiation of bright young stars causes low density gas to boil away, leaving stellar nurseries of dense EGGs exposed.

Tomorrow's picture: Eagle EGGs in M16

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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 - globuly - zvezdoobrazovanie - Molekulyarnye oblaka Publikacii so slovami: M 16 - globuly - zvezdoobrazovanie - Molekulyarnye oblaka
Sm. takzhe: NGC 7714: vspyshka zvezdoobrazovaniya posle stolknoveniya galaktik NGC 2170: abstraktnaya kartina s tumannost'yu Angel Tumannost' Konus ot teleskopa imeni Habbla NGC 1893 i Golovastiki v IC 410 Vdol' molekulyarnogo oblaka v Tel'ce Zvezdoobrazovanie v tumannosti Pakman Tumannost' Orla i goryachie rentgenovskie zvezdy Vse publikacii na tu zhe temu >>