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MEDIA INFORMATION

 
 
 
COLLECTION NAME:
NASA Spitzer Space Telescope Collection
mediaCollectionId
nasaNAS~12~12
NASA Spitzer Space Telescope Collection
Collection
true
Record 
Title:
Towering Infernos
title
Towering Infernos
Title
false
Description:
This majestic false-color image from NASA's Spitzer Space Telescope shows the "mountains" where stars are born. Dubbed "Mountains of Creation" by Spitzer scientists, these towering pillars of cool gas and dust are illuminated at their tips with light from warm, embryonic stars. The new infrared picture is reminiscent of Hubble's iconic visible-light image of the Eagle Nebula (inset), which also features a star-forming region, or nebula, that is being sculpted into pillars by radiation and winds from hot, massive stars. The pillars in the Spitzer image are part of a region called W5, in the Cassiopeia constellation 7,000 light-years away and 50 light-years across. They are more than 10 times in the size of those in the Eagle Nebula (shown to scale here). The Spitzer's view differs from Hubble's because infrared light penetrates dust, whereas visible light is blocked by it. In the Spitzer image, hundreds of forming stars (white/yellow) can seen for the first time inside the central pillar, and dozens inside the tall pillar to the left. Scientists believe these star clusters were triggered into existence by radiation and winds from an "initiator" star more than 10 times the mass of our Sun. This star is not pictured, but the finger-like pillars "point" toward its location above the image frame. The Spitzer picture also reveals stars (blue) a bit older than the ones in the pillar tips in the evacuated areas between the clouds. Scientists believe these stars were born around the same time as the massive initiator star not pictured. A third group of young stars occupies the bright area below the central pillar. It is not known whether these stars formed in a related or separate event. Some of the blue dots are foreground stars that are not members of this nebula. The red color in the Spitzer image represents organic molecules known as polycyclic aromatic hydrocarbons. These building blocks of life are often found in star-forming clouds of gas and dust. Like small dust grains, they are heated by the light from the young stars, then emit energy in infrared wavelengths. This image was taken by the Infrared Array Camera (IRAC) on Spitzer. It is a 4-color composite of infrared light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange), and 8.0 microns (red).
description
This majestic false-color image from NASA's Spitzer Space Telescope shows the "mountains" where stars are born. Dubbed "Mountains of Creation" by Spitzer scientists, these towering pillars of cool gas and dust are illuminated at their tips with light from warm, embryonic stars. The new infrared picture is reminiscent of Hubble's iconic visible-light image of the Eagle Nebula (inset), which also features a star-forming region, or nebula, that is being sculpted into pillars by radiation and winds from hot, massive stars. The pillars in the Spitzer image are part of a region called W5, in the Cassiopeia constellation 7,000 light-years away and 50 light-years across. They are more than 10 times in the size of those in the Eagle Nebula (shown to scale here). The Spitzer's view differs from Hubble's because infrared light penetrates dust, whereas visible light is blocked by it. In the Spitzer image, hundreds of forming stars (white/yellow) can seen for the first time inside the central pillar, and dozens inside the tall pillar to the left. Scientists believe these star clusters were triggered into existence by radiation and winds from an "initiator" star more than 10 times the mass of our Sun. This star is not pictured, but the finger-like pillars "point" toward its location above the image frame. The Spitzer picture also reveals stars (blue) a bit older than the ones in the pillar tips in the evacuated areas between the clouds. Scientists believe these stars were born around the same time as the massive initiator star not pictured. A third group of young stars occupies the bright area below the central pillar. It is not known whether these stars formed in a related or separate event. Some of the blue dots are foreground stars that are not members of this nebula. The red color in the Spitzer image represents organic molecules known as polycyclic aromatic hydrocarbons. These building blocks of life are often found in star-forming clouds of gas and dust. Like small dust grains, they are heated by the light from the young stars, then emit energy in infrared wavelengths. This image was taken by the Infrared Array Camera (IRAC) on Spitzer. It is a 4-color composite of infrared light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange), and 8.0 microns (red).
Description
false
Release Date:
2005/11/09
release_date
2005/11/09
Release Date
false
Press Release:
Spitzer Captures Cosmic Mountains of Creation [ http://www.spitzer.… ]
press_release
Spitzer Captures Cosmic Mountains of Creation [ http://www.spitzer.caltech.edu/Media/releases/ssc2005-23/release.shtml ]
Press Release
false
Release Credit:
NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
release_credit
NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
Release Credit
false
Image Credit:
NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
image_credit
NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian CfA)
Image Credit
false
Object type:
Star forming region
object_type
Star forming region
Object type
false
Position (J2000):
*RA: *03h01m56.00s *Dec: *60d35m50.00s
position__j2000_
*RA: *03h01m56.00s *Dec: *60d35m50.00s
Position (J2000)
false
Distance:
2000 pc; 7000 light-years
distance
2000 pc; 7000 light-years
Distance
false
Constellation:
Cassiopeia
constellation
Cassiopeia
Constellation
false
Wavelength:
3.6 (blue), 4.5 (green), 5.8 (orange), 8.0 (red) microns
wavelength
3.6 (blue), 4.5 (green), 5.8 (orange), 8.0 (red) microns
Wavelength
false
Image scale:
34 x 26 arcmin
image_scale
34 x 26 arcmin
Image scale
false
Observers:
Lori Allen (Harvard-Smithsonian CfA) Joseph Hora (Harvard-Smithsonian CfA) Luis Chavarria (Harvard-Smithsonian CfA) Lynne Deutsch (Harvard-Smithsonian CfA)
observers
Lori Allen (Harvard-Smithsonian CfA) Joseph Hora (Harvard-Smithsonian CfA) Luis Chavarria (Harvard-Smithsonian CfA) Lynne Deutsch (Harvard-Smithsonian CfA)
Observers
false
Instrument:
IRAC
instrument
IRAC
Instrument
false
Orientation:
North is 84 deg CCW from up
orientation
North is 84 deg CCW from up
Orientation
false
Related links:
Podcast Interview with Dr. Lori Allen [ http://www.spitzer.… ] Harvard-Smithsonian Center for Astrophysics press release [ http://www.cfa.harv… ]
related_links
Podcast Interview with Dr. Lori Allen [ http://www.spitzer.caltech.edu/features/podcasts/index.shtml#20051109 ] Harvard-Smithsonian Center for Astrophysics press release [ http://www.cfa.harvard.edu/press/pr0535.html ]
Related links
false
note:
*Hubble's* Screen-Resolution (456x450): JPEG [ http://ipac.jpl.nas… ssc2005-23b1_small.jpg ] High-Resolution (1518x1497): JPEG | Mac TIFF | PC TIFF Credit: NASA/ ESA/STScI/J. Hester & P. Scowen (Arizona State University)
note
*Hubble's* Screen-Resolution (456x450): JPEG [ http://ipac.jpl.nasa.gov/media_images/ ssc2005-23b1_small.jpg ] High-Resolution (1518x1497): JPEG | Mac TIFF | PC TIFF Credit: NASA/ ESA/STScI/J. Hester & P. Scowen (Arizona State University)
note
false
facet_what:
Cassiopeia
facet_what
Cassiopeia
facet_what
false
facet_where:
Arizona
facet_where
Arizona
facet_where
false
Image #:
ssc2005-23b
image__
ssc2005-23b
Image #
false
original url:
http://sscws1.ipac.…
original_url
http://sscws1.ipac.caltech.edu/Imagegallery/image.php?image_name=ssc2005-23b
original url
false
UID:
SPD-SPITZ-ssc2005-23b
uid
SPD-SPITZ-ssc2005-23b
UID
false
Annotations:  
Link To Source
Source