by APOD Robot » Thu Apr 14, 2011 4:06 am
Young Stars in the Rho Ophiuchi Cloud
Explanation: Dust clouds and embedded newborn stars glow at
infrared wavelengths in this tantalizing false-color composition from WISE, the
Wide-field Infrared Survey Explorer. The
cosmic canvas features one of the closest star forming regions, part of the Rho Ophiuchi
cloud complex some 400 light-years distant near the southern edge of the
pronounceable constellation
Ophiuchus. After forming along a
large cloud of cold molecular hydrogen gas, young stars heat the surrounding dust to produce the infrared glow. Stars in the process of formation, called young stellar objects or
YSOs, are embedded in the compact pinkish nebulae seen here, but are otherwise hidden from the prying eyes of optical telescopes. An
exploration of the region in penetrating infrared light has detected emerging and newly formed stars whose average age is estimated to be a mere 300,000 years. That's extremely young compared to the
Sun's age of 5 billion years. The prominent reddish nebula at the lower right surrounding the star
Sigma Scorpii is a reflection nebula produced by dust scattering starlight. This view from WISE
spans almost 2 degrees and covers about 14 light-years at the estimated distance of the Rho Ophiuchi cloud.
[/b]
[url=http://apod.nasa.gov/apod/ap110414.html][img]http://apod.nasa.gov/apod/calendar/S_110414.jpg[/img] [size=150]Young Stars in the Rho Ophiuchi Cloud[/size][/url]
[b] Explanation: [/b] Dust clouds and embedded newborn stars glow at [url=http://coolcosmos.ipac.caltech.edu/cosmic_classroom/ir_tutorial/what_is_ir.html]infrared wavelengths[/url] in this tantalizing false-color composition from WISE, the [url=http://wise.ssl.berkeley.edu/index.html]Wide-field Infrared Survey Explorer[/url]. The [url=http://wise.ssl.berkeley.edu/gallery_rho_ophiuchi.html]cosmic canvas features[/url] one of the closest star forming regions, part of the Rho Ophiuchi [url=http://apod.nasa.gov/apod/ap070903.html]cloud complex[/url] some 400 light-years distant near the southern edge of the [url=http://www.astronomyclub.org/learn/Say_What.htm]pronounceable[/url] constellation [url=http://hawastsoc.org/deepsky/oph/index.html]Ophiuchus[/url]. After forming along a [url=http://archive.ncsa.uiuc.edu/Cyberia/Bima/StarForm.html]large cloud[/url] of cold molecular hydrogen gas, young stars heat the surrounding dust to produce the infrared glow. Stars in the process of formation, called young stellar objects or [url=http://en.wikipedia.org/wiki/Young_stellar_object]YSOs[/url], are embedded in the compact pinkish nebulae seen here, but are otherwise hidden from the prying eyes of optical telescopes. An [url=http://arxiv.org/abs/0709.3492]exploration[/url] of the region in penetrating infrared light has detected emerging and newly formed stars whose average age is estimated to be a mere 300,000 years. That's extremely young compared to the [url=http://en.wikipedia.org/wiki/Sun#Life_cycle]Sun's age[/url] of 5 billion years. The prominent reddish nebula at the lower right surrounding the star [url=http://stars.astro.illinois.edu/sow/alniyat-s.html]Sigma Scorpii[/url] is a reflection nebula produced by dust scattering starlight. This view from WISE [url=http://chandra.harvard.edu/photo/scale.html]spans[/url] almost 2 degrees and covers about 14 light-years at the estimated distance of the Rho Ophiuchi cloud.
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