NASA Telescopes See Weather Patterns in Brown Dwarf

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Jan. 8, 2013

J.D. Harrington 
Headquarters, Washington                             
202-358-5241 
j.d.harrington@xxxxxxxx 

Whitney Clavin 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-4673 
whitney.clavin@xxxxxxxxxxxx 

RELEASE: 13-011

NASA TELESCOPES SEE WEATHER PATTERNS IN BROWN DWARF

WASHINGTON -- Astronomers using NASA's Spitzer and Hubble space 
telescopes have probed the stormy atmosphere of a brown dwarf, 
creating the most detailed "weather map" yet for this class of cool, 
star-like orbs. The forecast shows wind-driven, planet-sized clouds 
enshrouding these strange worlds. 

Brown dwarfs form out of condensing gas, as stars do, but lack the 
mass to fuse hydrogen atoms and produce energy. Instead, these 
objects, which some call failed stars, are more similar to gas 
planets with their complex, varied atmospheres. The new research is a 
stepping stone toward a better understanding not only of brown 
dwarfs, but also of the atmospheres of planets beyond our solar 
system. 

"With Hubble and Spitzer, we were able to look at different 
atmospheric layers of a brown dwarf, similar to the way doctors use 
medical imaging techniques to study the different tissues in your 
body," said Daniel Apai, the principal investigator of the research 
at the University of Arizona in Tucson, who presented the results at 
the American Astronomical Society meeting Tuesday in Long Beach, 
Calif. 

A study describing the results, led by Esther Buenzli, also of the 
University of Arizona, is published in the Astrophysical Journal 
Letters. 

The researchers turned Hubble and Spitzer simultaneously toward a 
brown dwarf with the long name of 2MASSJ22282889-431026. They found 
that its light varied in time, brightening and dimming about every 90 
minutes as the body rotated. But more surprising, the team also found 
the timing of this change in brightness depended on whether they 
looked using different wavelengths of infrared light. 

These variations are the result of different layers or patches of 
material swirling around the brown dwarf in windy storms as large as 
Earth itself. Spitzer and Hubble see different atmospheric layers 
because certain infrared wavelengths are blocked by vapors of water 
and methane high up, while other infrared wavelengths emerge from 
much deeper layers. 

"Unlike the water clouds of Earth or the ammonia clouds of Jupiter, 
clouds on brown dwarfs are composed of hot grains of sand, liquid 
drops of iron, and other exotic compounds," said Mark Marley, 
research scientist at NASA's Ames Research Center in Moffett Field, 
Calif., and co-author of the paper. "So this large atmospheric 
disturbance found by Spitzer and Hubble gives a new meaning to the 
concept of extreme weather." 

According to Buenzli, this is the first time researchers can probe 
variability at several different altitudes at the same time in the 
atmosphere of a brown dwarf. "Although brown dwarfs are cool relative 
to other stars, they are actually hot by earthly standards. This 
particular object is about 1,100 to 1,300 degrees Fahrenheit (600 to 
700 degrees Celsius)," Buenzli said. 

"What we see here is evidence for massive, organized cloud systems, 
perhaps akin to giant versions of the Great Red Spot on Jupiter," 
said Adam Showman, a theorist at the University of Arizona involved 
in the research. "These out-of-sync light variations provide a 
fingerprint of how the brown dwarf's weather systems stack up 
vertically. The data suggest regions on the brown dwarf where the 
weather is cloudy and rich in silicate vapor deep in the atmosphere 
coincide with balmier, drier conditions at higher altitudes -- and 
vice versa." 

Researchers plan to look at the atmospheres of dozens of additional 
nearby brown dwarfs using both Spitzer and Hubble. 

"From studies such as this we will learn much about this important 
class of objects, whose mass falls between that of stars and 
Jupiter-sized planets." said Glenn Wahlgren, Spitzer Program 
scientist at NASA Headquarters in Washington. "This technique will 
see extensive use when we are able to image individual exoplanets." 

For more information about Spitzer, visit: 

http://www.nasa.gov/spitzer 

For more information about Hubble, visit: 

http://www.nasa.gov/hubble 

	
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