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 Visuals Quick Facts

Graph showing disk detection
Credit: NASA/JPL-Caltech/S.Carey (Caltech)

'Galactic Ghoul' Rears Its Spooky Head

A "monster" lurking behind a blanket of cosmic dust is unveiled in this new Halloween image from NASA's Spitzer Space Telescope. Resembling a ghoul with two hollow eyes and a screaming mouth, this masked cloud of newborn stars was uncovered by Spitzer's heat-seeking infrared eyes.

The spooky cloud -- a nebula called "DR 6" residing in the plane of our Milky Way galaxy -- is home to a cluster of about 10 massive newborn stars, ranging in size from 10 to 20 times the mass of our Sun. The nebular "eyes" and "mouth" were carved out by intense heat and winds, which shoot outward from the stars (located in the central bar or "nose"). The green material remaining in the eyes and mouth is comprised of gas, while the red regions and tendrils beyond make up the dusty cloud that originally gave birth to the young stars.

Within the nebula's nose, a second generation of stars is in the process of forming. These stars, in turn, will sculpt their stellar nursery, and ultimately affect the birth of yet another generation of stars. Spitzer provides astronomers with an unprecedented combination of sensitivity and spatial resolution to study this cycle in detail.

DR 6 is located 3,900 light-years away in the constellation Cygnus. The distance from one end of its central bar to the other is the about 3.5 light-years, or about the same distance from our Sun to its nearest neighbor, Alpha Centauri.

This image composite was taken on Nov. 27, 2003, by Spitzer's infrared array camera. It is composed of images obtained at four wavelengths: 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red).

To download, choose your preferred resolution and file format below. "High-Resolution" files will always the highest resolution and widest crop available, intended for print. Other resolutions are provided for convenient on-screen viewing.

Screen-Resolution (360x450) JPEG (56 KB)
Medium-Resolution (720x900): JPEG (144 KB)
High-Resolution (1200x1500): JPEG (1 MB) | Mac TIFF (2.2 MB) | PC TIFF (2.2 MB)

About the Object Object Name: DR6
Object Type: Star Formation Region
Position (J2000): RA: 20h27m13.39s Dec: 39d26m33.1s
Constellation: Cygnus
About the Data Image Credit: NASA/JPL-Caltech/S. Carey
Instrument: IRAC
Wavelength: 3.6 (blue), 4.5 (green), 5.8-8.0 (red) microns
Exposure Date: 2003 November 2003
Exposure Time: 50 seconds per position
Image Scale: 9.8 x 13.8 arcmin
Orientation: North is 30.7 deg CCW from up
Release Date: October 28, 2004
Observers IRAC IST (SSC/Caltech), IRAC IT (SAO)

Introduction 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