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M11: zvezdnoe skoplenie "Dikaya utka"
<< Vchera 21.01.2003 Zavtra >>
M11: zvezdnoe skoplenie "Dikaya utka"
Avtory i prava: Jean-Charles Cuillandre (CFHT), Hawaiian Starlight, CFHT
Poyasnenie: Mnogie zvezdy, podobnye nashemu Solncu, obrazovalis' v rasseyannyh zvezdnyh skopleniyah. Rasseyannoe skoplenie M11, privedennoe na risunke, soderzhit tysyachi zvezd i nahoditsya ot nas na rasstoyanii pyat' tysyach svetovyh let. Vse zvezdy etogo skopleniya obrazovalis' primerno 250 millionov let nazad. Yarkie molodye zvezdy v M11 vyglyadyat golubymi. Rasseyannye skopleniya, nazyvaemye takzhe galakticheskimi skopleniyami, soderzhat men'she zvezd i eti zvezdy bolee molodye, chem v sharovyh skopleniyah. Otlichie sharovyh skoplenii ot rasseyannyh skoplenii zaklyuchaetsya takzhe v tom, chto poslednie v osnovnom lezhat v ploskosti nashei Galaktiki. M11 mozhno uvidet' v binokl' v sozvezdii Shita.

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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.

English text
Po materialam Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: M 11 - open cluster - Rasseyannoe skoplenie
Publikacii so slovami: M 11 - open cluster - Rasseyannoe skoplenie
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