Credit & Copyright: Jose Francisco Hernandez
(Altamira Observatory)
Explanation:
Supergiant star Gamma Cygni lies at the center
of the Northern Cross, a famous
asterism
in the constellation of the Swan
(Cygnus).
Known by the proper name Sadr,
the bright star also lies at the center of
this gorgeous skyscape, featuring a complex of
stars, dust clouds, and glowing nebulae along the
plane of our
Milky Way galaxy.
The field of view spans over 3 degrees
(six Full Moons) on
the sky and
includes emission nebula
IC 1318 and open star cluster NGC 6910.
Left of Gamma Cygni and shaped
like two glowing cosmic wings divided by a long dark
dust lane, IC 1318's popular name is understandably the
Butterfly Nebula.
Above and slightly left of
Gamma Cygni, are the young, still tightly
grouped
stars of NGC 6910.
Some distance estimates for
Gamma Cygni place it at around 750 light-years
while estimates for IC 1318 and
NGC 6910
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.
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