by APOD Robot » Wed Apr 27, 2011 4:08 am
The Dark Tower in Scorpius
Explanation: In silhouette against a crowded star field toward the constellation
Scorpius, this dusty cosmic cloud evokes for some the image of an
ominous dark tower. In fact, clumps of dust and molecular gas
collapsing to form stars may well lurk within the dark nebula, a structure that spans almost 40 light-years across this
gorgeous telescopic portrait. Known as a
cometary globule, the swept-back cloud, extending from the lower right to the head (top of the tower) left and above center, is shaped by intense ultraviolet radiation from the
OB association of very hot stars in
NGC 6231, off the upper edge of the scene. That energetic ultraviolet light also powers the globule's bordering reddish glow of
hydrogen gas. Hot stars embedded in the dust can be seen as bluish
reflection nebulae. This dark tower,
NGC 6231, and associated nebulae are about 5,000 light-years away.
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[url=http://apod.nasa.gov/apod/ap110427.html][img]http://apod.nasa.gov/apod/calendar/S_110427.jpg[/img] [size=150]The Dark Tower in Scorpius[/size][/url]
[b] Explanation: [/b] In silhouette against a crowded star field toward the constellation [url=http://hawastsoc.org/deepsky/sco/index.html]Scorpius[/url], this dusty cosmic cloud evokes for some the image of an [url=http://poetry.eserver.org/childe-roland.html]ominous dark tower[/url]. In fact, clumps of dust and molecular gas [url=http://archive.ncsa.uiuc.edu/Cyberia/Bima/StarForm.html]collapsing[/url] to form stars may well lurk within the dark nebula, a structure that spans almost 40 light-years across this [url=http://www.astrodonimaging.com/gallery/display.cfm?imgID=227]gorgeous telescopic portrait[/url]. Known as a [url=http://apod.nasa.gov/apod/ap070806.html]cometary globule[/url], the swept-back cloud, extending from the lower right to the head (top of the tower) left and above center, is shaped by intense ultraviolet radiation from the [url=http://en.wikipedia.org/wiki/Stellar_association#Types]OB association[/url] of very hot stars in [url=http://www.aao.gov.au/images/captions/aat072.html]NGC 6231[/url], off the upper edge of the scene. That energetic ultraviolet light also powers the globule's bordering reddish glow of [url=http://apod.nasa.gov/apod/ap051223.html]hydrogen gas[/url]. Hot stars embedded in the dust can be seen as bluish [url=http://apod.nasa.gov/apod/ap011228.html]reflection nebulae[/url]. This dark tower, [url=http://panther-observatory.com/gallery/deepsky/doc/NGC6231_wide.htm]NGC 6231[/url], and associated nebulae are about 5,000 light-years away.
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