Scientists Peer Into a Brown Dwarf, Find Stormy Atmosphere
This artist's conception illustrates the brown dwarf named 2MASSJ22282889-431026. NASA's Hubble and Spitzer space telescopes
observed the object to learn more about its turbulent atmosphere. Brown dwarfs are more massive and hotter than planets but
lack the mass required to become sizzling stars. Their atmospheres can be similar to the giant planet Jupiter's.
January 8, 2013
By Daniel Stolte/UANews and Whitney Clavin/JPL
Pointing the Spitzer and Hubble space telescopes simultaneously at a brown dwarf, a UA-led team of astronomers has obtained
detailed images of the stormy atmosphere that enshrouds these strange objects, which are not quite planets and not quite stars.
Their forecast shows planet-sized clouds and showers of sandy and iron rain.
A University of Arizona-led team of astronomers for the first time has used NASA's
Hubble space telescopes
simultaneously to peer into the stormy atmosphere of a brown dwarf, creating the most detailed “weather map” yet for this
class of strange, not-quite-star-and-not-quite-planet objects. The forecast shows wind-driven, planet-sized clouds enshrouding
these strange worlds.
Brown dwarfs form out of condensing gas like stars but fail to accrue enough mass to ignite the nuclear fusion process necessary
to turn them into a star. Instead, they pass their lives as dimly glowing, constantly cooling gas balls similar to gas planets with
their complex, varied atmospheres. The new research is a stepping stone toward better understanding not only brown dwarfs but also
the atmospheres of planets beyond our solar system.
This artist's illustration shows the atmosphere of a brown dwarf called 2MASSJ22282889-431026, which was observed
simultaneously by NASA's Spitzer and Hubble space telescopes. The results were unexpected, revealing offset layers of material
as indicated in the diagram. For example, the large, bright patch in the outer layer has shifted to the right in the inner
layer. The observations indicate this brown dwarf - a ball of gas that "failed" to become a star - is marked by wind-driven,
planet-size clouds. (Image: NASA/JPL-Caltech)
“With Hubble and Spitzer, we were able to look at the 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 from the UA,
who presented the results at the American Astronomical Society meeting in Long Beach, Calif. Apai is an assistant professor with
joint appointments in the UA’s departments of astronomy and planetary sciences.
A study describing the results, led by Esther Buenzli, a postdoctoral researcher in the UA’s department of astronomy,
published in the Astrophysical Journal Letters.
The researchers turned Hubble and Spitzer simultaneously toward a brown dwarf called 2MASSJ22282889-431026.
They found that its light varied in time, brightening and dimming as the body rotated around every 1.4 hours.
But more surprising, the team also found that the timing of this brightening changed depending on whether they looked
at it with Spitzer or Hubble using different wavelengths of infrared light (Hubble sees shorter-wavelength 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 atmosphere layers because certain infrared wavelengths are blocked by
vapors of water and methane high up, while other infrared wavelengths emerge from much deeper.
"What we see here is evidence for massive, organized cloud systems, perhaps akin to giant versions of the Great Red Spot on Jupiter
or large-scale storm systems on Earth,” said Adam Showman, a theorist with the UA’s Lunar and Planetary Laboratory who was
involved in the research.
“We were expecting the phases of the light variations to be in sync between the two telescopes, so we were really surprised
that they were offset,” said Buenzli. “This is the first time that we can probe variability at several different altitudes at
the same time in the atmosphere of a brown dwarf.”
“The deeper layers appear to lag behind the higher layers,” Apai explained. “This tells us that the same or similar cloud
distribution is present in the different layers, but the deeper you look, the later you will see the same clouds turning
“We were very surprised to see such a big lag. Our best guess is this has to do with the brown dwarf’s atmospheric circulation.
The bigger picture here is that we see a very large-scale atmospheric structure in this brown dwarf.”
“These out-of-sync light variations provide a fingerprint of how the brown dwarf’s weather systems stack up vertically,”
added Showman. “The data suggest that regions on the brown dwarf where the weather is moist and cloudy deep in the atmosphere
coincide with balmier, drier conditions at higher altitudes – and vice versa.”
Ranging in size between Jupiter and the smallest stars and commonly weighing in at 30-40 Jupiter masses, brown dwarfs are cool
relative to other stars but quite hot by our Earthly standards. This particular object is about 600 to 700 degrees Celsius
(1,100 to 1,300 degrees Fahrenheit). Being quite warm, they emit strongly in the infrared, wavelengths picked up by Spitzer and
At the cooler, outer layers of the star, gas condenses into smoke-sized particles, including sand and iron, which fall down into
the interior as a sandy and iron rain. Just like on Earth, the iron and sand “raindrops” heat up as they enter the deeper warmer
layer and eventually evaporate, triggering a rain cycle.
Apai said the atmospheric dynamics on brown dwarfs are very different from those here on Earth.
“On our planet, we have only one species of cloud - water,” he explained, “But on this brown dwarf,
there is such a wide temperature range that we have many different species of clouds.”
In three ongoing Spitzer programs, Apai and his co-investigators have successfully explored the properties of cloud covers in about
50 brown dwarfs.
“As different wavelengths probe different pressures and different rotational phases probe different latitudes we will be able to
explore the two or even three-dimensional structure of the atmospheres,” Apai said.
Buenzli said that theorists are excited to model the new data: a new era of weather reporting has begun.
“Eventually, we want to probe the atmospheres of exoplanets in a similar fashion,” she said.
“Currently, we can't get this type of data on exoplanets because their bright host stars blind our vision,” Apai said.
“Brown dwarfs are the perfect laboratories for studying the exotic science of worlds beyond our own.”
This graph shows the brightness variations of the brown dwarf named 2MASSJ22282889-431026 measured simultaneously by
both NASA’s Hubble and Spitzer space telescopes. As the object rotates every 1.4 hours, its emitted light periodically
brightens and dims. Surprisingly, the timing, or phase, of the variations in brightness changes when measured at different
wavelengths of infrared light. Spitzer and Hubble’s wavelengths probe different layers in the atmosphere of the brown dwarf.
The phase shifts indicate complex clouds or weather patterns that change with altitude.
(Image: NASA/JPL-Caltech/University of Arizona)
The findings are the first published from a set of Spitzer and Hubble space telescope programs led by Apai.
By mapping cloud systems in brown dwarfs, these studies are opening a new field, extrasolar atmospheric dynamics,
which bridges astronomy and planetary science.
Apai is the principal investigator of the project Extrasolar Storms, which uses the Spitzer and Hubble space telescope together
to follow the evolution of gigantic storms in the atmospheres of brown dwarfs over 1.5 years. Storms is one of the largest projects
ever approved for the Spitzer Space Telescope, equaling two months of continuous observations with this $1 billion telescope.
Launched in 2003, Spitzer has long exceeded its nominal lifetime. A group led by UA Regents' Professor George Rieke developed one
of Spitzer’s infrared detectors, the Multiband Imaging Photometer.
The Storms team includes 12 experts from the U.S., Canada and the UK, four of which are at the UA: In addition to Apai,
Buenzli and Showman, Davin Flateau, another graduate student of Apai’s is part of the team.
“Brown dwarfs are fascinating and diverse,” said Apai. “Now we've got a new technique to chase their gigantic and violent storms.”