Explanation: Near the outskirts of the Small Magellanic Cloud, a satellite galaxy some 200 thousand light-years distant, lies 5 million year young star cluster NGC 602. Surrounded by natal gas and dust, NGC 602 is just below center in this telescopic field of view with the angular size of the Full Moon on the sky. The cluster itself is about 200 light-years in diameter. Glowing interior ridges and swept back shapes strongly suggest that energetic radiation and shock waves from NGC 602's massive young stars have eroded the dusty material and triggered a progression of star formation moving away from the cluster's center. Of course, the more extended wings of emission in the region suggest a popular name for the complex cosmic environment, The Flying Lizard Nebula.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: star cluster - small Magellanic cloud - Maloe Magellanovo Oblako - zvezdnoe skoplenie Publikacii so slovami: star cluster - small Magellanic cloud - Maloe Magellanovo Oblako - zvezdnoe skoplenie
Sm. takzhe: NGC 602: zvezdy protiv stolbov Molodoe zvezdnoe skoplenie NGC 1333 NGC 602: zvezdnoe skoplenie Ustrica Zvezdnoe skoplenie IC 348 ot teleskopa "Dzheims Vebb" Bol'shoi Kovsh nad goroi Piramida Molodoe zvezdnoe skoplenie NGC 346 Molodye zvezdy v NGC 346 Vse publikacii na tu zhe temu >>