Explanation: This interstellar beast is formed of cosmic dust and gas interacting with the energetic light and winds from hot young stars. The shape, visual texture, and color, combine to give the region the popular name Fox Fur Nebula. The characteristic blue glow on the left is dust reflecting light from the bright star S Mon, just beyond the left edge of the image. Mottled pink and brown areas are a combination of the cosmic dust and reddish emission from ionized hydrogen gas. S Mon is part of a young open cluster of stars, NGC 2264, located about 2,500 light years away toward the constellation of Monoceros, just north of the Cone Nebula.

digg_url = 'http://apod.nasa.gov/apod/ap080422.html'; digg_skin = 'compact';

<<  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: S Mon - NGC 2264 - tumannost' Lisii meh Publikacii so slovami: S Mon - NGC 2264 - tumannost' Lisii meh
Sm. takzhe: Lisii meh, Edinorog i Rozhdestvenskaya elka Lisii meh, Edinorog i rozhdestvenskaya elka v shirokom pole Kosmicheskie oblaka v Edinoroge Tumannost' Lisii Meh Orion s vyderzhkoi 212 chasov Lisii meh, Edinorog i Rozhdestvenskaya elka Vblizi tumannosti Konus Vse publikacii na tu zhe temu >>