Credit & Copyright: Paul C. Swift
Explanation:
In cosmic brush strokes
of glowing hydrogen gas, this beautiful
skyscape unfolds across the plane of our
Milky Way Galaxy and
the center of the northern constellation
Cygnus the Swan.
The featured image spans about six degrees.
Bright supergiant star Gamma
Cygni
(Sadr) to the upper left of the image
center lies in the foreground of the complex gas and dust clouds
and
crowded star fields.
Left of Gamma Cygni,
shaped like two luminous wings divided by
a long dark dust lane is IC 1318, whose popular name is understandably the
Butterfly
Nebula.
The more compact, bright nebula at the lower right is NGC 6888,
the Crescent Nebula.
Some distance estimates for Gamma Cygni place it at
around 750 light-years while estimates for IC 1318 and NGC 6888 range
from 2,000 to 5,000 light-years.
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' |
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:
Cygnus - Lebed' - Tumannosti mezhzvezdnye
Publikacii so slovami: Cygnus - Lebed' - Tumannosti mezhzvezdnye | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> |