Frame Frame Frame Frame Frame
Frame Frame Frame Frame Frame
Frame Frame
NASA Spitzer Space Telescope • Jet Propulsion Laboratory
• California Institute of Technology
• Vision for Space Exploration
Frame Frame
Frame Frame Frame Frame Frame
Frame Frame Frame Frame Frame
Frame Frame Spitzer Newsroom Frame Frame
Frame Frame Frame Frame Frame
Frame Frame
 
Press Releases
 
— Chronological
 
— By Subject
 
— Outside Institutions
 
 
What's Happening Archive
 
 
Visuals
 
— Image Use Policy
 
 
Update Notifications
 
— Mailing List
 
— RSS Feed (XML)
 
 
References
 
— Fast Facts
 
— Press Kit (.pdf)
 
— Fact Sheet (.pdf)
 
— Field Guides
 
— Glossary
 
 
Media Contacts
 

Introduction Press Release Visuals Quick Facts

Video Preview
Credit: NASA/JPL-Caltech/R. Hurt (SSC-Caltech)

Trifid's Shifting Sides

This movie shifts from the well-known visible-light picture of the glowing Trifid Nebula to infrared views from NASA's Spitzer Space Telescope. The Trifid Nebula is a giant star-forming cloud of gas and dust located 5,400 light-years away in the constellation Sagittarius.

The false-color Spitzer images reveal a different side of the Trifid Nebula. Where dark lanes of dust are visible trisecting the nebula in the visible-light picture, bright regions of star-forming activity are seen in the Spitzer pictures. All together, Spitzer uncovered 30 massive embryonic stars and 120 smaller newborn stars throughout the Trifid Nebula, in both its dark lanes and luminous clouds. These stars are visible in all the Spitzer images, mainly as yellow or red spots. Embryonic stars are developing stars about to burst into existence.

Ten of the 30 massive embryos discovered by Spitzer were found in four dark cores, or stellar "incubators," where stars are born. Astronomers using data from the Institute of Radioastronomy millimeter telescope in Spain had previously identified these cores but thought they were not quite ripe for stars. Spitzer's highly sensitive infrared eyes were able to penetrate all four cores to reveal rapidly growing embryos.

The movie begins with a visible-light image from the National Optical Astronomy Observatory, Tucson, Ariz., then shifts to a Spitzer picture from its infrared array camera. The next image is a combination of data from Spitzer's infrared array camera and its multiband imaging photometer. The final still is made up of data from only the multiband imaging photometer.

The Spitzer infrared array camera image is a three-color composite of invisible light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 and 8.0 microns (red). The Spitzer mosaic image from the infrared array camera and multiband imaging photometer consists of light of 4.5 microns (blue), 8.0 microns (green) and 24 microns (red). The multiband imaging photometer image shows 24-micron emissions.

To view, choose your preferred resolution and file format below. For tape requests, our media contacts will be happy to assist you.

Slow Connections (160x120): Windows Media (84 KB) | QuickTime 4.0 (56 KB)
Fast Connections (320x240): Windows Media (472 KB) | QuickTime 4.0 (856 KB) | QuickTime 6.0 (860 KB) | MPEG 1 (1 MB) | MPEG 4 (624 KB)
Full-Size (640x480): Windows Media (488 KB) | QuickTime 6.0 (1.7 MB) | MPEG 4 (1.7 MB)

Introduction Press Release Visuals Quick Facts



The Spitzer Space Telescope is a NASA mission managed by the Jet Propulsion Laboratory. This website is maintained by the Spitzer Science Center, located on the campus of the California Institute of Technology and part of NASA's Infrared Processing and Analysis Center.

Frame Frame
Frame Frame Frame Frame Frame
Frame Frame Frame Frame Frame