Explanation: The well known Pleiades star cluster is slowly destroying part of a passing cloud of gas and dust. The Pleiades is the brightest open cluster of stars on Earth's sky and can be seen from almost any northerly location with the unaided eye. The passing young dust cloud is thought to be part of Gould's belt, an unusual ring of young star formation surrounding the Sun in the local Milky Way Galaxy. Over the past 100,000 years, part Gould's belt is by chance moving right through the older Pleiades and is causing a strong reaction between stars and dust. Pressure from the star's light significantly repels the dust in the surrounding blue reflection nebula, with smaller dust particles being repelled more strongly. A short-term result is that parts of the dust cloud have become filamentary and stratified, as seen in the above deep-exposure image.

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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: pleiades - star cluster - dust - Pleyady - otrazhatel'nye tumannosti - pyl' Publikacii so slovami: pleiades - star cluster - dust - Pleyady - otrazhatel'nye tumannosti - pyl'
Sm. takzhe: Molodye zvezdy i temnye tumannosti Pleyady: zvezdnoe skoplenie Sem' sester Prizraki v Kassiopee Sem' Sester v pyli NGC 6727: tumannost' Buinyi Pavian Temnyi Morskoi konek v Cefee Molodoe zvezdnoe skoplenie NGC 1333 Vse publikacii na tu zhe temu >>