Spitzer Spectrum of Ices in a Protoplanetary Disc

Spitzer_ssc2004-20c_1024

spitzer_ssc2004-20c November 9th, 2004

Credit: NASA/JPL-Caltech/K. Pontoppidan (Leiden Observatory)

Astronomers have made the first clear detection of a variety of ices -- water, ammonium, and carbon dioxide -- in the inner planet-forming region near a young star about 120 light years away. Such an observation is only possible by combining the unique sensitivity of NASA's Spitzer Space Telescope with the fortunate alignment of this particular system.

Planet-forming discs are seen in a variety of orientations, ranging from edge-on (where the discs block the light of the star entirely) to face-on (where the disc is lost in the glare of the star). In this system, known to astronomers as CRBR 2422.8-3423, the disc lies at a unique angle. The light from the star just peeks out over the disc, like a distant sunrise, and contains clues about the disc material through which it has passed.

These observations use Spitzer's infrared spectrograph which acts much like a prism, spreading light out into its component parts, or spectrum. Astronomers study this infrared rainbow, measuring how much light from the star reaches us at different wavelengths. From this they can determine the composition of the disc.

Different ices in the disc each have their own unique infrared "colors" and will block the light in different parts of the star's spectrum. For example, the dip in the spectrum around 6 microns indicates the presence of water ice. The feature at 7 microns is caused by warmed ammonium ions and therefore must be close to the star, within the inner planet-forming region of the disc.

This result has given astronomers a new tool in probing the inner workings of planet-forming discs. By looking for other young stars with discs lined up at just the right angle, they can learn more about the stuff that formed our own solar system almost 5 billion years ago.

Provider: Spitzer Space Telescope

Image Source: http://www.spitzer.caltech.edu/images/1338-ssc2004-20c-Spitzer-Spectrum-of-Ices-in-a-Protoplanetary-Disc

Curator: Spitzer Space Telescope, Pasadena, CA, USA

Image Use Policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy

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Image Details Image Details

Image Type
Chart
Object Name
CRBR 2422.8-3423
Subject - Milky Way
Star > Circumstellar Material > Disk > Protoplanetary

Distance Details Distance

Universescale1
390 light years

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Spitzer (IRS) Infrared (Mid-Infrared) -
28 s (5-15 microns), 244s (10-20 microns), 484 s (19-37 microns)
Spitzer_ssc2004-20c_1280
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ID
ssc2004-20c
Subject Category
B.3.7.2.1.  
Subject Name
CRBR 2422.8-3423
Credits
NASA/JPL-Caltech/K. Pontoppidan (Leiden Observatory)
Type
Chart
Image Quality
Good
Distance Notes
Distance taken from Fast Facts.
Facility
Spitzer
Instrument
IRS
Color Assignment
Band
Infrared
Bandpass
Mid-Infrared
Central Wavelength
Start Time
Integration Time
Dataset ID
Notes
2
Coordinate Frame
Equinox
Reference Value
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
FITS Header
Notes
Creator (Curator)
Spitzer Space Telescope
URL
http://www.spitzer.caltech.edu
Name
Spitzer Space Telescope
Email
Telephone
Address
1200 E. California Blvd.
City
Pasadena
State/Province
CA
Postal Code
91125
Country
USA
Rights
http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
Publisher
Spitzer Science Center
Publisher ID
spitzer
Resource ID
ssc2004-20c.tif
Metadata Date
2012-03-26
Metadata Version
1.1
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Detailed color mapping information coming soon...

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Universescalefull
390 light years

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