Explanation: Scattered within this cavernous nebula, cataloged as NGC 604, are over 200 newly formed hot, massive, stars. At 1,500 light-years across, this expansive cloud of interstellar gas and dust is effectively a giant stellar nursery located some three million light-years distant in the spiral galaxy, M33. The newborn stars irradiate the gas with energetic ultraviolet light stripping electrons from atoms and producing a characteristic nebular glow. The details of the nebula's structure hold clues to the mysteries of star formation and galaxy evolution.

<<  Aprel'  >> Pn Vt Sr Cht Pt Sb Vs     1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30       1995   1996   1997 1998   1999   2000 2001   2002   2003 2004   2005   2006 2007   2008   2009 2010   2011   2012 2013   2014   2015 2016   2017   2018 2019   2020   2021 2022   2023   2024

Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr'

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: stellar nursery - star formation - emission nebula - massivnye zvezdy - zvezdoobrazovanie - evolyuciya galaktik - Tumannosti mezhzvezdnye Publikacii so slovami: stellar nursery - star formation - emission nebula - massivnye zvezdy - zvezdoobrazovanie - evolyuciya galaktik - Tumannosti mezhzvezdnye
Sm. takzhe: IC 348 i Barnard 3 Prizraki v Kassiopee M16: stolpy sozidaniya Zvezdnaya fabrika Mess'e 17 Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 IC 5146: tumannost' Kokon Kometarnye globuly Vse publikacii na tu zhe temu >>