NASA's Spitzer Sees the Light of Alien "Super Earth"

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May 8, 2012

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: 12-138

NASA'S SPITZER SEES THE LIGHT OF ALIEN "SUPER EARTH"

WASHINGTON -- NASA's Spitzer Space Telescope has detected light 
emanating from a "super-Earth" planet beyond our solar system for the 
first time. While the planet is not habitable, the detection is a 
historic step toward the eventual search for signs of life on other 
planets. 

"Spitzer has amazed us yet again," said Bill Danchi, Spitzer program 
scientist at NASA Headquarters in Washington. "The spacecraft is 
pioneering the study of atmospheres of distant planets and paving the 
way for NASA's upcoming James Webb Space Telescope to apply a similar 
technique on potentially habitable planets." 

The planet, called 55 Cancri e, falls into a class of planets termed 
super Earths, which are more massive than our home world but lighter 
than giant planets like Neptune. Fifty-five Cancri e is about twice 
as big and eight times as massive as Earth. The planet orbits a 
bright star, called 55 Cancri, in a mere 18 hours. 

Previously, Spitzer and other telescopes were able to study the planet 
by analyzing how the light from 55 Cancri changed as the planet 
passed in front of the star. In the new study, Spitzer measured how 
much infrared light comes from the planet itself. The results reveal 
the planet is likely dark and its sun-facing side is more than 2,000 
Kelvin (3,140 degrees Fahrenheit), hot enough to melt metal. 

The new information is consistent with a prior theory that 55 Cancri e 
is a water world: a rocky core surrounded by a layer of water in a 
"supercritical" state where it is both liquid and gas, and topped by 
a blanket of steam. 

"It could be very similar to Neptune, if you pulled Neptune in toward 
our sun and watched its atmosphere boil away," said Michaël Gillon of 
Université de Liège in Belgium, principal investigator of the 
research, which appears in the Astrophysical Journal. The lead author 
is Brice-Olivier Demory of the Massachusetts Institute of Technology 
in Cambridge. 

The 55 Cancri system is relatively close to Earth at 41 light-years 
away. It has five planets, with 55 Cancri e being the closest to the 
star and tidally locked, so one side always faces the star. Spitzer 
discovered the sun-facing side is extremely hot, indicating the 
planet probably does not have a substantial atmosphere to carry the 
sun's heat to the unlit side. 

NASA's James Webb Space Telescope, scheduled to launch in 2018, likely 
will be able to learn even more about the planet's composition. The 
telescope might be able to use a similar infrared method as Spitzer 
to search other potentially habitable planets for signs of molecules 
possibly related to life. 

"When we conceived of Spitzer more than 40 years ago, exoplanets 
hadn't even been discovered," said Michael Werner, Spitzer project 
scientist at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, 
Calif. "Because Spitzer was built very well, it's been able to adapt 
to this new field and make historic advances such as this." 

In 2005, Spitzer became the first telescope to detect light from a 
planet beyond our solar system. To the surprise of many, the 
observatory saw the infrared light of a "hot Jupiter," a gaseous 
planet much larger than the solid 55 Cancri e. Since then, other 
telescopes, including NASA's Hubble and Kepler space telescopes, have 
performed similar feats with gas giants using the same method. 

In this method, a telescope gazes at a star as a planet circles behind 
it. When the planet disappears from view, the light from the star 
system dips ever so slightly, but enough that astronomers can 
determine how much light came from the planet itself. This 
information reveals the temperature of a planet, and, in some cases, 
its atmospheric components. Most other current planet-hunting methods 
obtain indirect measurements of a planet by observing its effects on 
the star. 

During Spitzer's ongoing extended mission, steps were taken to enhance 
its unique ability to see exoplanets, including 55 Cancri e. Those 
steps, which included changing the cycling of a heater and using an 
instrument in a new way, led to improvements in how precisely the 
telescope points at targets. 

JPL manages the Spitzer Space Telescope mission for NASA's Science 
Mission Directorate in Washington. Science operations are conducted 
at the Spitzer Science Center at the California Institute of 
Technology (Caltech) in Pasadena. Data are archived at the Infrared 
Science Archive housed at the Infrared Processing and Analysis Center 
at Caltech. Caltech manages JPL for NASA. 

For more information about Spitzer, visit: 

http://www.nasa.gov/spitzer 

	
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