August 6, 2009

J D Harrington Headquarters, Washington
202-358-5241 j d harrington@nasa gov

Michael Mewhinney Ames Research Center, Moffett Field, Calif 650-604-3937 michael s mewhinney@nasa gov
RELEASE: 09-180

NASA'S KEPLER MISSION SPIES CHANGING PHASES IN A DISTANT WORLD

WASHINGTON -- NASA's new exoplanet-hunting Kepler space telescope has detected the atmosphere of a known giant gas planet, demonstrating the telescope's extraordinary scientific capabilities The discovery will be published Friday in the journal Science

The find is based on a relatively short 10 days of test data collected before the official start of science operations Kepler was launched March 6, 2009, from Cape Canaveral Air Force Station in Florida The observation demonstrates the extremely high precision of the measurements made by the telescope, even before its calibration and data analysis software were finished

"As NASA's first exoplanets mission, Kepler has made a dramatic entrance on the planet-hunting scene," said Jon Morse, director of the Science Mission Directorate's Astrophysics Division at NASA Headquarters in Washington "Detecting this planet's atmosphere in just the first 10 days of data is only a taste of things to come The planet hunt is on!"

Kepler team members say these new data indicate the mission is indeed capable of finding Earth-like planets, if they exist Kepler will spend the next three-and-a-half years searching for planets as small as Earth, including those that orbit stars in a warm zone where there could be water It will do this by looking for periodic dips in the brightness of stars, which occur when orbiting planets transit, or cross in front of, the stars

"When the light curves from tens of thousands of stars were shown to the Kepler science team, everyone was awed; no one had ever seen such exquisitely detailed measurements of the light variations of so many different types of stars," said William Borucki, the principal science investigator and lead author of the paper

The observations were collected from a planet called HAT-P-7, known to transit a star located about 1,000 light years from Earth The planet orbits the star in just 2 2 days and is 26 times closer than Earth is to the sun Its orbit, combined with a mass somewhat larger than the planet Jupiter, classifies this planet as a "hot Jupiter " It is so close to its star, the planet is as hot as the glowing red heating element on a stove

The Kepler measurements show the transit from the previously detected HAT-P-7 However, these new measurements are so precise, they also show a smooth rise and fall of the light between transits caused by the changing phases of the planet, similar to those of our moon This is a combination of both the light emitted from the planet and the light reflected off the planet The smooth rise and fall of light is also punctuated by a small drop in light, called an occultation, exactly halfway between each transit An occultation happens when a planet passes behind a star

The new Kepler data can be used to study this hot Jupiter in unprecedented detail The depth of the occultation and the shape and amplitude of the light curve show the planet has an atmosphere with a day-side temperature of about 4,310 degrees Fahrenheit Little of this heat is carried to the cool night side The occultation time compared to the main transit time shows the planet has a circular orbit The discovery of light from this planet confirms the predictions by researchers and theoretical models that the emission would be detectable by Kepler

This new discovery also demonstrates Kepler has the precision to find Earth-size planets The observed brightness variation is just one and a half times what is expected for a transit caused by an Earth-sized planet Although this is already the highest precision ever obtained for an observation of this star, Kepler will be even more precise after analysis software being developed for the mission is completed

"This early result shows the Kepler detection system is performing right on the mark," said David Koch, deputy principal investigator of NASA's Ames Research Center at Moffett Field, Calif "It bodes well for Kepler's prospects to be able to detect Earth-size planets "

Kepler is a NASA Discovery mission Ames is responsible for the ground system development, mission operations and science data analysis NASA's Jet Propulsion Laboratory in Pasadena, Calif , manages the Kepler mission development Ball Aerospace and Technologies Corp of Boulder, Colo , is responsible for developing the Kepler flight system and supporting mission operations

For images, animations and more information about the Kepler mission, visit:

http://www nasa gov/kepler

-end-

To subscribe to the list, send a message to: hqnews-subscribe@mediaservices nasa gov To remove your address from the list, send a message to: hqnews-unsubscribe@mediaservices nasa gov

The following information is a reminder of your current mailing list subscription:

You are subscribed to the following list: [list_name]

using the following email: example@example.com

You may automatically unsubscribe from this list at any time by visiting the following URL:

http://www aus-city com/cgi-bin/dada/mail cgi/u/[list]/

If the above URL is inoperable, make sure that you have copied the entire address Some mail readers will wrap a long URL and thus break this automatic unsubscribe mechanism

You may also change your subscription by visiting this list's main screen:

<[program_url]/list/[list]>

If you're still having trouble, please contact the list owner at:

<mailto:[list_owner_email]>

The following physical address is associated with this mailing list:

[physical_address]