NASA'S Kepler Mission Discovers 461 New Planet Candidates

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Jan. 07, 2013

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

Michele Johnson 
Ames Research Center, Moffett Field, Calif. 
650-604-4789 
michele.johnson@xxxxxxxx 


RELEASE: 13-008

NASA'S KEPLER MISSION DISCOVERS 461 NEW PLANET CANDIDATES

WASHINGTON -- NASA's Kepler mission Monday announced the discovery of 
461 new planet candidates. Four of the potential new planets are less 
than twice the size of Earth and orbit in their sun's "habitable 
zone," the region in the planetary system where liquid water might 
exist on the surface of a planet. 

Based on observations conducted from May 2009 to March 2011, the 
findings show a steady increase in the number of smaller-size planet 
candidates and the number of stars with more than one candidate. 

"There is no better way to kickoff the start of the Kepler extended 
mission than to discover more possible outposts on the frontier of 
potentially life bearing worlds," said Christopher Burke, Kepler 
scientist at the SETI Institute in Mountain View, Calif., who is 
leading the analysis. 

Since the last Kepler catalog was released in February 2012, the 
number of candidates discovered in the Kepler data has increased by 
20 percent and now totals 2,740 potential planets orbiting 2,036 
stars. The most dramatic increases are seen in the number of 
Earth-size and super Earth-size candidates discovered, which grew by 
43 and 21 percent respectively. 

The new data increases the number of stars discovered to have more 
than one planet candidate from 365 to 467. Today, 43 percent of 
Kepler's planet candidates are observed to have neighbor planets. 

"The large number of multi-candidate systems being found by Kepler 
implies that a substantial fraction of exoplanets reside in flat 
multi-planet systems," said Jack Lissauer, planetary scientist at 
NASA's Ames Research Center in Moffett Field, Calif. "This is 
consistent with what we know about our own planetary neighborhood." 

The Kepler space telescope identifies planet candidates by repeatedly 
measuring the change in brightness of more than 150,000 stars in 
search of planets that pass in front, or "transit," their host star. 
At least three transits are required to verify a signal as a 
potential planet. 

Scientists analyzed more than 13,000 transit-like signals to eliminate 
known spacecraft instrumentation and astrophysical false positives, 
phenomena that masquerade as planetary candidates, to identify the 
potential new planets. 

Candidates require additional follow-up observations and analyses to 
be confirmed as planets. At the beginning of 2012, 33 candidates in 
the Kepler data had been confirmed as planets. Today, there are 105. 

"The analysis of increasingly longer time periods of Kepler data 
uncovers smaller planets in longer period orbits-- orbital periods 
similar to Earth's," said Steve Howell, Kepler mission project 
scientist at Ames. "It is no longer a question of will we find a true 
Earth analogue, but a question of when." 

The complete list of Kepler planet candidates is available in an 
interactive table at the NASA Exoplanet Archive. The archive is 
funded by NASA's Exoplanet Exploration Program to collect and make 
public data to support the search for and characterization of 
exoplanets and their host stars. 

Ames manages Kepler's ground system development, mission operations 
and science data analysis. NASA's Jet Propulsion Laboratory (JPL) in 
Pasadena, Calif., managed Kepler mission development. Ball Aerospace 
and Technologies Corp. in Boulder, Colo., developed the Kepler flight 
system and supports mission operations with JPL at the Laboratory for 
Atmospheric and Space Physics at the University of Colorado in 
Boulder. 

The Space Telescope Science Institute in Baltimore archives, hosts and 
distributes the Kepler science data. Kepler is NASA's 10th Discovery 
Mission and is funded by NASA's Science Mission Directorate at the 
agency's headquarters in Washington. 

JPL manages NASA's Exoplanet Exploration Program. The NASA Exoplanet 
Archive is hosted at the Infrared Processing and Analysis Center at 
the California Institute of Technology. 

For information about the NASA Exoplanet Archive, visit: 

http://exoplanetarchive.ipac.caltech.edu/index.html 

For information about the Kepler Mission, visit: 

http://www.nasa.gov/kepler 

	
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