by APOD Robot » Sun Nov 20, 2011 5:12 am
W5: Pillars of Star Formation
Explanation: How do stars form? A study of star forming region
W5 by the sun-orbiting
Spitzer Space Telescope provides clear clues by recording that massive stars near the center of empty cavities are older than stars near the edges. A likely reason for this is that the older stars in the center are actually
triggering the formation of the younger edge stars. The triggered
star formation occurs when hot outflowing gas compresses cooler gas into
knots dense enough to gravitationally contract into stars.
Spectacular pillars, left slowly evaporating from the hot outflowing gas, provide further
visual clues. In the
above scientifically-colored
infrared image, red indicates heated
dust, while white and green indicate particularly dense gas clouds.
W5 is also known as
IC 1848, and
together with IC 1805 form a complex region of star formation popularly dubbed the
Heart and
Soul Nebulas. The
above image highlights a part of W5 spanning about 2,000
light years that is rich in
star forming pillars. W5 lies about 6,500 light years away toward the
constellation of
Cassiopeia.
[/b]
[url=http://apod.nasa.gov/apod/ap111120.html][img]http://apod.nasa.gov/apod/calendar/S_111120.jpg[/img] [size=150]W5: Pillars of Star Formation[/size][/url]
[b] Explanation: [/b] How do stars form? A study of star forming region [url=http://www.nasa.gov/mission_pages/spitzer/news/spitzer-20080822.html]W5[/url] by the sun-orbiting [url=http://www.spitzer.caltech.edu/mission/32-The-Mission]Spitzer Space Telescope[/url] provides clear clues by recording that massive stars near the center of empty cavities are older than stars near the edges. A likely reason for this is that the older stars in the center are actually [url=http://www.youtube.com/watch?v=W13ZYepDBvo]triggering[/url] the formation of the younger edge stars. The triggered [url=http://en.wikipedia.org/wiki/Star_formation]star formation[/url] occurs when hot outflowing gas compresses cooler gas into [url=http://apod.nasa.gov/apod/ap080528.html]knots dense[/url] enough to gravitationally contract into stars. [url=http://apod.nasa.gov/apod/ap070218.html]Spectacular pillars[/url], left slowly evaporating from the hot outflowing gas, provide further [url=http://upload.wikimedia.org/wikipedia/en/a/a3/Escher%27s_Relativity.jpg]visual clues[/url]. In the [url=http://www.spitzer.caltech.edu/images/1953-ssc2008-15a1-W5-Star-Formation-Region]above[/url] scientifically-colored [url=http://missionscience.nasa.gov/ems/07_infraredwaves.html]infrared[/url] image, red indicates heated [url=http://apod.nasa.gov/apod/ap030706.html]dust[/url], while white and green indicate particularly dense gas clouds. [url=http://ads.ari.uni-heidelberg.de/abs/2008ApJ...688.1142K]W5[/url] is also known as [url=http://en.wikipedia.org/wiki/Soul_Nebula]IC 1848[/url], and [url=http://apod.nasa.gov/apod/ap080914.html]together with IC 1805[/url] form a complex region of star formation popularly dubbed the [url=http://www.youtube.com/watch?v=h45UrpBsCKI]Heart[/url] and [url=http://en.wikipedia.org/wiki/Soul_music]Soul[/url] Nebulas. The [url=http://www.spitzer.caltech.edu/images/1953-ssc2008-15a1-W5-Star-Formation-Region]above image[/url] highlights a part of W5 spanning about 2,000 [url=http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html]light years[/url] that is rich in [url=http://apod.nasa.gov/apod/ap070430.html]star forming pillar[/url]s. W5 lies about 6,500 light years away toward the [url=http://en.wikipedia.org/wiki/Constellation]constellation[/url] of [url=http://www.astro.wisc.edu/~dolan/constellations/constellations/Cassiopeia.html]Cassiopeia[/url].
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