Explanation: The dark nebula predominant at the lower left of the above photograph is known as the Pipe Nebula. The dark clouds, suggestively shaped like smoke rising from a pipe, are caused by absorption of background starlight by dust. These dust clouds can be traced all the way to the Rho Ophiuchi nebular clouds on the right. The brightest star in the field is Antares. Many types of nebula are highlighted here: the red are emission nebula, the blue are reflection nebula, and the dark are absorption nebula. This picture has been digitally enhanced.

<<  Mai  >> 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: nebula - dark nebula - Mezhzvezdnaya pyl' - emissionnaya tumannost' - otrazhatel'nye tumannosti - Pylevaya tumannost' Publikacii so slovami: nebula - dark nebula - Mezhzvezdnaya pyl' - emissionnaya tumannost' - otrazhatel'nye tumannosti - Pylevaya tumannost'
Sm. takzhe: Slonovii hobot v Cefee IC 348 i Barnard 3 LDN 43: tumannost' Kosmicheskaya Letuchaya Mysh' Prizraki v Kassiopee NGC 6727: tumannost' Buinyi Pavian Melott 15 v tumannosti Serdce Tumannost' Tyul'pan i chernaya dyra Lebed' X-1 Vse publikacii na tu zhe temu >>