Credit & Copyright: Alex Lin
(Chilescope)
Explanation:
One of the most identifiable nebulas in the sky,
the Horsehead Nebula
in Orion, is part of a large, dark,
molecular cloud.
Also known as Barnard 33, the unusual shape was first
discovered on a
photographic plate in the late 1800s.
The red glow originates from
hydrogen
gas predominantly behind the nebula, ionized by the nearby bright star
Sigma Orionis.
The darkness of the
Horsehead is caused mostly by thick
dust,
although the lower part of the
Horsehead's neck casts a
shadow
to the left.
Streams of gas leaving
the nebula are funneled by a strong
magnetic field.
Bright spots in the
Horsehead Nebula's base are young stars just in the
process of forming.
Light takes about 1,500 years to reach us from the
Horsehead Nebula.
The featured image was taken from the
Chilescope Observatory in the
mountains of
Chile.
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:
tumannost' Konskaya Golova - Horsehead Nebula
Publikacii so slovami: tumannost' Konskaya Golova - Horsehead Nebula | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
