Planet Clumps and Crystals Around Brown Dwarfs

Spitzer_ssc2005-21a_1024

spitzer_ssc2005-21a October 20th, 2005

Credit: NASA/JPL-Caltech/D. Apai (University of Arizona)

This graph of data from NASA's Spitzer Space Telescope shows the spectra (middle four lines) of dusty disks around four brown dwarfs, or "failed stars," located 520 light-years away in the Chamaeleon constellation. The data suggest that the dust in these disks is crystallizing and clumping together in what may be the birth of planets.

Spectra are created by breaking light apart into its basic components, like a prism turning sunlight into a rainbow. Their bumps represent the "fingerprints" or signatures of different minerals.

Here, the light green vertical bands highlight the spectral fingerprints of crystals made up primarily of a green silicate mineral found on Earth called olivine. As the graph illustrates, three of the four brown dwarfs possess these microscopic gem-like particles. For comparison, the spectra of dust between stars (top) and the comet Hale-Bopp (bottom) are shown. The comet has the tiny crystals, whereas the interstellar dust does not.

The broadening of these spectral features or bumpsseen here as you move down the graphindicates silicate grains of increasing size.Another analysis of this same data shows that some of the brown dwarfs' dusty disks flare in their outer regions, while others are flattened. This flattening is correlated with increasing grain size, and probably occurs because the heavier dust grains are settling downward.

Together, these observationsof crystals, growing dust grains and flattened disksprovide strong evidence that the dust around these brown dwarfs is evolving into what might become planets. Prior to the findings, these first steps of planet formation were seen only in disks around stars, the brighter and bigger cousins to brown dwarfs.

Provider: Spitzer Space Telescope

Image Source: http://www.spitzer.caltech.edu/images/1497-ssc2005-21a-Planet-Clumps-and-Crystals-Around-Brown-Dwarfs

Curator: Spitzer Space Telescope, Pasadena, CA, USA

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

View Options View Options

Image Details Image Details

Image Type
Chart
Subject - Local Universe
Star > Type > Brown Dwarf
Star > Circumstellar Material > Disk > Debris

Distance Details Distance

Universescale1
520 light years

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Spitzer (IRS) Infrared 7.5 µm
Spitzer (IRS) Infrared 13.0 µm
Spectrum plotted from 7.5 to 13 microns
Spectrum_ir1
Spitzer_ssc2005-21a_1280
×
ID
ssc2005-21a
Subject Category
C.3.2.3.   C.3.7.2.3.  
Subject Name
Credits
NASA/JPL-Caltech/D. Apai (University of Arizona)
Release Date
2005-10-20
Lightyears
520
Redshift
520
Reference Url
http://www.spitzer.caltech.edu/images/1497-ssc2005-21a-Planet-Clumps-and-Crystals-Around-Brown-Dwarfs
Type
Chart
Image Quality
Good
Distance Notes
Distance from description
Facility
Spitzer, Spitzer
Instrument
IRS, IRS
Color Assignment
Band
Infrared, Infrared
Bandpass
Central Wavelength
7500, 13000
Start Time
Integration Time
Dataset ID
Notes
S
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
ssc2005-21a.tif
Metadata Date
2012-03-21
Metadata Version
1.1
×

 

Detailed color mapping information coming soon...

×
Universescalefull
520 light years

Providers | Sign In