Explanation: Pictured above are clouds of young stars forming an arc in the nearby Large Magellanic Cloud, the nearest galaxy to the our Milky Way Galaxy. These stars are situated in a star forming region known as N 51. The stars are so young they shine mostly in blue and ultraviolet light, and so massive their lifetimes are only millions of years - much shorter than the billions of years of lower mass stars like our Sun. This picture was taken in ultraviolet light by NASA's Ultraviolet Imaging Telescope in March 1995. The reason the arc has the observed shape is currently unknown.

<<  Oktyabr'  >> 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 31           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: LMC - clouds - massivnye zvezdy - Oblasti zvezdoobrazovaniya - Bol'shoe Magellanovo Oblako Publikacii so slovami: LMC - clouds - massivnye zvezdy - Oblasti zvezdoobrazovaniya - Bol'shoe Magellanovo Oblako
Sm. takzhe: IC 1795: tumannost' Ryb'ya golova Zona Tarantula Zvezdnaya fabrika Mess'e 17 Bol'shoe Magellanovo Oblako Tri galaktiki i kometa Grozovoi vorotnik nad Viskonsinom Tumannost' Tarantul ot teleskopa SuperBIT Vse publikacii na tu zhe temu >>