Explanation: Stars are sometimes born in the midst of chaos. About 3 million years ago in the nearby galaxy M33, a large cloud of gas spawned dense internal knots which gravitationally collapsed to form stars. NGC 604 was so large, however, it could form enough stars to make a globular cluster. Many young stars from this cloud are visible in the above image from the Hubble Space Telescope, along with what is left of the initial gas cloud. Some stars were so massive they have already evolved and exploded in a supernova. The brightest stars that are left emit light so energetic that they create one of the largest cloud of ionized hydrogen gas known, comparable to the Tarantula Nebula in our Milky Way's close neighbor, the Large Magellanic Cloud.

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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: NGC 604 - stellar nursery - Oblasti zvezdoobrazovaniya Publikacii so slovami: NGC 604 - stellar nursery - Oblasti zvezdoobrazovaniya
Sm. takzhe: IC 1795: tumannost' Ryb'ya golova NGC 604: gigantskie zvezdnye yasli Zvezdnaya fabrika Mess'e 17 Shirokoe pole s ρ Zmeenosca Tumannost' Rozetka v liniyah vodoroda i kisloroda Na krayu NGC 2174 Zvezdnye potoki v M83 Vse publikacii na tu zhe temu >>