Lump of Planetary Stuff

Spitzer_ssc2009-18a_1024

spitzer_ssc2009-18a September 23rd, 2009

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

This artist's conception shows a lump of material in a swirling, planet-forming disk. Astronomers using NASA's Spitzer Space Telescope found evidence that a companion to a star -- either another star or a planet -- could be pushing planetary material together, as illustrated here.

Planets are born out of spinning disks of gas and dust. They can carve out lanes or gaps in the disks as they grow bigger and bigger. Scientists used Spitzer's infrared vision to study the disk around a star called LRLL 31, located about 1,000 light-years away in the IC 348 region of the constellation Perseus. Spitzer's new infrared observations reveal that the disk has both an inner and outer gap.

What's more, the data show that infrared light from the disk is changing over as little time as one week -- a very unusual occurrence. In particular, light of different wavelengths seesawed back and forth, with short-wavelength light going up when long-wavelength light went down, and vice versa.

According to astronomers, this change could be caused by a companion to the star (illustrated as a planet in this picture). As the companion spins around, its gravity would cause the wall of the inner disk to squeeze into a lump. This lump would also spin around the star, shadowing part of the outer disk. When the bright side of the lump is on the far side of the star, and facing Earth, more infrared light at shorter wavelengths should be observed (hotter material closer to the star emits shorter wavelengths of infrared light). In addition, the shadow of the lump should cause longer-wavelength infrared light from the outer disk to decrease. The opposite would be true when the lump is in front of the star and its bright side is hidden (shorter-wavelength light would go down, and longer-wavelength light up). This is precisely what Spitzer observed.

The size of the lump and the planet have been exaggerated to better illustrate the dynamics of the system.

Provider: Spitzer Space Telescope

Image Source: http://www.spitzer.caltech.edu/images/2734-ssc2009-18a-Lump-of-Planetary-Stuff

Curator: Spitzer Space Telescope, Pasadena, CA, USA

Image Use Policy: Public Domain

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Image Details Image Details

Image Type
Artwork
Object Name
LRLL 31
Subject - Milky Way
Star > Circumstellar Material > Disk

Distance Details Distance

Universescale1
1,000 light years
Spitzer_ssc2009-18a_1280
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ID
ssc2009-18a
Subject Category
B.3.7.2.  
Subject Name
LRLL 31
Credits
NASA/JPL-Caltech/R. Hurt (SSC)
Release Date
2009-09-23
Lightyears
1,000
Redshift
1,000
Reference Url
http://www.spitzer.caltech.edu/images/2734-ssc2009-18a-Lump-of-Planetary-Stuff
Type
Artwork
Image Quality
Good
Distance Notes
Facility
Instrument
Color Assignment
Band
Bandpass
Central Wavelength
Start Time
Integration Time
Dataset ID
Notes
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
Email
Telephone
Address
1200 E. California Blvd.
City
Pasadena
State/Province
CA
Postal Code
91125
Country
USA
Rights
Public Domain
Publisher
Spitzer Science Center
Publisher ID
spitzer
Resource ID
ssc2009-18a.tif
Metadata Date
2011-09-01
Metadata Version
1.1
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Detailed color mapping information coming soon...

×
Universescalefull
1,000 light years

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