NASA'S Kepler Discovers its Smallest 'Habitable Zone' Planets to Date

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April 18, 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: 13-112

NASA'S KEPLER DISCOVERS ITS SMALLEST 'HABITABLE ZONE' PLANETS TO DATE

WASHINGTON -- NASA's Kepler mission has discovered two new planetary 
systems that include three super-Earth-size planets in the "habitable 
zone," the range of distance from a star where the surface 
temperature of an orbiting planet might be suitable for liquid water. 

The Kepler-62 system has five planets; 62b, 62c, 62d, 62e and 62f. The 
Kepler-69 system has two planets; 69b and 69c. Kepler-62e, 62f and 
69c are the super-Earth-sized planets. 

Two of the newly discovered planets orbit a star smaller and cooler 
than the sun. Kepler-62f is only 40 percent larger than Earth, making 
it the exoplanet closest to the size of our planet known in the 
habitable zone of another star. Kepler-62f is likely to have a rocky 
composition. Kepler-62e, orbits on the inner edge of the habitable 
zone and is roughly 60 percent larger than Earth. 

The third planet, Kepler-69c, is 70 percent larger than the size of 
Earth, and orbits in the habitable zone of a star similar to our sun. 
Astronomers are uncertain about the composition of Kepler-69c, but 
its orbit of 242 days around a sun-like star resembles that of our 
neighboring planet Venus. 

Scientists do not know whether life could exist on the newfound 
planets, but their discovery signals we are another step closer to 
finding a world similar to Earth around a star like our sun. 

"The Kepler spacecraft has certainly turned out to be a rock star of 
science," said John Grunsfeld, associate administrator of the Science 
Mission Directorate at NASA Headquarters in Washington. "The 
discovery of these rocky planets in the habitable zone brings us a 
bit closer to finding a place like home. It is only a matter of time 
before we know if the galaxy is home to a multitude of planets like 
Earth, or if we are a rarity." 

The Kepler space telescope, which simultaneously and continuously 
measures the brightness of more than 150,000 stars, is NASA's first 
mission capable of detecting Earth-size planets around stars like our 
sun. 

Orbiting its star every 122 days, Kepler-62e was the first of these 
habitable zone planets identified. Kepler-62f, with an orbital period 
of 267 days, was later found by Eric Agol, associate professor of 
astronomy at the University of Washington and co-author of a paper on 
the discoveries published in the journal Science. 

The size of Kepler-62f is now measured, but its mass and composition 
are not. However, based on previous studies of rocky exoplanets 
similar in size, scientists are able to estimate its mass by 
association. 

"The detection and confirmation of planets is an enormously 
collaborative effort of talent and resources, and requires expertise 
from across the scientific community to produce these tremendous 
results," said William Borucki, Kepler science principal investigator 
at NASA's Ames Research Center at Moffett Field, Calif., and lead 
author of the Kepler-62 system paper in Science. "Kepler has brought 
a resurgence of astronomical discoveries and we are making excellent 
progress toward determining if planets like ours are the exception or 
the rule." 

The two habitable zone worlds orbiting Kepler-62 have three companions 
in orbits closer to their star, two larger than the size of Earth and 
one about the size of Mars. Kepler-62b, Kepler-62c and Kepler-62d, 
orbit every five, 12, and 18 days, respectively, making them very hot 
and inhospitable for life as we know it. 

The five planets of the Kepler-62 system orbit a star classified as a 
K2 dwarf, measuring just two-thirds the size of the sun and only 
one-fifth as bright. At seven billion years old, the star is somewhat 
older than the sun. It is about 1,200 light-years from Earth in the 
constellation Lyra. 

A companion to Kepler 69c, known as Kepler 69b, is more than twice the 
size of Earth and whizzes around its star every 13 days. The 
Kepler-69 planets' host star belongs to the same class as our sun, 
called G-type. It is 93 percent the size of the sun and 80 percent as 
luminous and is located approximately 2,700 light-years from Earth in 
the constellation Cygnus. 

"We only know of one star that hosts a planet with life, the sun. 
Finding a planet in the habitable zone around a star like our sun is 
a significant milestone toward finding truly Earth-like planets," 
said Thomas Barclay, Kepler scientist at the Bay Area Environmental 
Research Institute in Sonoma, Calif., and lead author of the 
Kepler-69 system discovery published in the Astrophysical Journal. 

When a planet candidate transits, or passes in front of the star from 
the spacecraft's vantage point, a percentage of light from the star 
is blocked. The resulting dip in the brightness of the starlight 
reveals the transiting planet's size relative to its star. Using the 
transit method, Kepler has detected 2,740 candidates. Using various 
analysis techniques, ground telescopes and other space assets, 122 
planets have been confirmed. 

Early in the mission, the Kepler telescope primarily found large, 
gaseous giants in very close orbits of their stars. Known as "hot 
Jupiters," these are easier to detect due to their size and very 
short orbital periods. Earth would take three years to accomplish the 
three transits required to be accepted as a planet candidate. As 
Kepler continues to observe, transit signals of habitable zone 
planets the size of Earth orbiting stars like the sun will begin to 
emerge. 

Ames is responsible for Kepler's ground system development, mission 
operations, and science data analysis. NASA's Jet Propulsion 
Laboratory in Pasadena, Calif., managed Kepler mission development. 

Ball Aerospace & Technologies Corp. in Boulder, Colo., developed the 
Kepler flight system and supports mission operations with 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 Kepler science data. Kepler is NASA's 10th Discovery 
Mission and was funded by the agency's Science Mission Directorate. 

For more information about the Kepler mission, visit: 


http://www.nasa.gov/kepler 

	
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