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 More Info

Spectrum
Credit: NASA/JPL-Caltech/D. Watson (Univ. of Rochester)

Spitzer Sees Water Loud and Clear

This plot of infrared data, called a spectrum, shows the strong signature of water vapor deep within the core of an embryonic star system, called NGC 1333-IRAS 4B.

The data were captured by NASA's Spitzer Space Telescope using an instrument called a spectrograph. A spectrograph collects light and sorts it according to color, or wavelength. In this case, infrared light from NGC 1333-IRAS 4B was broken up into the wavelengths listed on the horizontal axis of the plot. The sharp spikes, called spectral lines, occur at wavelengths at which the stellar object is particularly bright. The signature of water vapor is revealed in the pattern of wavelengths at which the spikes appear.

By comparing the observed data to a model (lower curve), astronomers can also determine the physical and chemical details of the region. For example, astronomers say these data suggest that ice in a cocoon surrounding the forming star is falling inward. The ice then smacks supersonically into a dusty planet-forming disk surrounding the stellar embryo, heats up and vaporizes quickly, releasing the infrared light that Spitzer collected.

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 (450x360) JPEG (44 KB)
Medium-Resolution (900x720): JPEG (160 KB)
High-Resolution (3000x2400): JPEG (4.7 MB) | Mac TIFF (8.3 MB) | PC TIFF (8.3 MB) | AI (28.4 MB)

About the Object Object Name: NGC 1333-IRAS 4B
Object Type: protostar
Position (J2000): RA: 3 29 12 Dec: +31 13 08
Distance: 320 pc (1000 light-years)
Constellation: Pegasus
About the Data Image Credit: NASA/ JPL-Caltech/D. Watson (University of Rochester)
Instrument: Infrared Spectrograph (IRS)
Wavelength: 20 to 37 microns
Exposure Date: March 2006
Release Date: 2007-08-29
Observers Dan Watson (University of Rochester)
C.J Bohac (University of Rochester)
C. Hull (University of Rochester)
William J. Forrest (University of Rochester)
Ben Sargent (University of Rochester)
Joel Green (University of Rochester)
Kyoung Hee Kim (University of Rochester)
E. Furlan (University of California at Los Angeles)
Joan Najita (National Optical Astronomy Observatory)
Nuria Calvet (University of Michigan)
Lee Hartmann (University of Michigan)
Paola dÕAlessio (National Autonomous University of Mexico)
Jim Houck (Cornell University)

Introduction Press Release Visuals More Info



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. Privacy Policy

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