"This first-of-its-kind measurement represents a significant advance in the field of extrasolar planetary science," said Jeremy Richardson, NASA Postdoctoral Fellow at NASA's Goddard Space Flight Center, Greenbelt, Md. Richardson and colleagues published their study in the Feb. 22 issue of Nature magazine.
One way in which scientists can study the properties of extrasolar planets is using spectroscopy, which refers to spreading light into its different colors (similar to a prism). For these observations, the team used NASA’s Spitzer Space Telescope, which operates in the infrared.
The team took advantage of the unique geometry of this particular planetary system. It is a so-called "transiting planet," meaning that the planet crosses in front of its star as seen from Earth. By measuring the spectrum of the planet and star together, then subtracting the spectrum of the star alone (when the planet is hidden behind the star), scientists can figure out the spectrum of the planet.
Richardson and his co-authors found that the extrasolar planet's spectrum revealed the "signature" of silicate (an element found on Earth) dust in clouds high in the planet's atmosphere.
Although the scientists saw "spectral signatures" or identifiers that were related to clouds, they were surprised that they didn't see any signatures that showed there was water vapor. On Earth, clouds are composed primarily of water vapor.
Richardson said that planets similar to this one, often called "hot Jupiter" type planets because they are gaseous like Jupiter but very close to their parent stars (even closer than Mercury is to the sun), must contain water vapor.
"Since oxygen and hydrogen are such abundant molecules in the cosmos it is virtually impossible for water (as vapor, or steam) to be absent from the planet, Richardson said. “So. the water vapor must be hidden, probably by the same cloud layer that we detect in the spectrum."
Once more powerful infrared telescopes like the James Webb Space Telescope, slated for launch in 2013, are launched, and as smaller planets are detected, this technique may hold promise for detecting the signatures of life on hot Earth-like planets.
In addition to Richardson's team, two other independent groups also captured spectra of extrasolar planets. See http://www.spitzer.caltech.edu/Media/releases/ssc2007-04/ for details.
Rob Gutro | EurekAlert!
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