Cracking the Code of Faraway Worlds: An Exoplanet Atmosphere

Spitzer_ssc2007-04c_1024

spitzer_ssc2007-04c February 21st, 2007

Credit: NASA/JPL-Caltech/C. Grillmair (SSC/Caltech)

This infrared data from NASA's Spitzer Space Telescope called a spectrum tells astronomers that a distant gas planet, a so-called "hot Jupiter" called HD 189733b, might be smothered with high clouds. It is one of the first spectra of an alien world.

A spectrum is created when an instrument called a spectrograph cracks light from an object open into a rainbow of different wavelengths. Patterns or ripples within the spectrum indicate the presence, or absence, of molecules making up the object.

Astronomers using Spitzer's spectrograph were able to obtain infrared spectra for two so-called "transiting" hot-Jupiter planets using the "secondary eclipse" technique. In this method, the spectrograph first collects the combined infrared light from the planet plus its star, then, as the planet is eclipsed by the star, the infrared light of just the star. Subtracting the latter from the former reveals the planet's own rainbow of infrared colors.

Astronomers were perplexed when they first saw the infrared spectrum above. It doesn't look anything like what theorists had predicted. Theorists thought the spectra of hot, Jupiter-like planets like this one would be filled with the signatures of molecules in the planets' atmospheres. But the spectrum doesn't show any molecules, and is instead what astronomers call "flat." For example, theorists thought there'd be a strong signature of water in the form of a big drop in the wavelength range between 7 and 10 microns. The fact that water is not detected may indicate that it is hidden underneath a thick blanket of high, dry clouds. The average brightness of the spectrum is also a bit lower than theoretical predictions, suggesting that very high winds are rapidly moving the terrific heat of the noonday sun from the day side of HD 189733b to the night side.

This spectrum was produced by Dr. Carl Grillmair of NASA's Spitzer Science Center at the California Institute of Technology in Pasadena, Calif., and his colleagues.

Provider: Spitzer Space Telescope

Image Source: http://www.spitzer.caltech.edu/images/1755-ssc2007-04c-Cracking-the-Code-of-Faraway-Worlds-An-Exoplanet-Atmosphere

Curator: Spitzer Space Telescope, Pasadena, CA, USA

Image Use Policy: Public Domain

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Image Details Image Details

Image Type
Chart
Object Name
HD 189733b
Subject - Milky Way
Planet > Type > Gas Giant
Planet > Feature > Atmosphere
Planet > Special Cases > Transiting
Planet > Special Cases > Hot Jupiter

Distance Details Distance

Universescale1
153 light years

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Spitzer (IRS) Infrared -
Spectrum plotted from 7.5 to 15 microns
Spitzer_ssc2007-04c_1280
×
ID
ssc2007-04c
Subject Category
B.1.1.2   B.1.2.2   B.1.3.1   B.1.3.2  
Subject Name
HD 189733b
Credits
NASA/JPL-Caltech/C. Grillmair (SSC/Caltech)
Type
Chart
Image Quality
Good
Distance Notes
Distance taken from Fast Facts.
Facility
Spitzer
Instrument
IRS
Color Assignment
Band
Infrared
Bandpass
Central Wavelength
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
Public Domain
Publisher
Spitzer Science Center
Publisher ID
spitzer
Resource ID
ssc2007-04c.tif
Metadata Date
2011-09-06
Metadata Version
1.1
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Detailed color mapping information coming soon...

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Universescalefull
153 light years

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