NASA's Kepler Mission Finds Three Smallest Exoplanets

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Jan. 11, 2012

Trent J. Perrotto
Headquarters, Washington
202-358-0321
trent.j.perrotto@xxxxxxxx

Michele Johnson
Ames Research Center, Moffett Field, Calif. 
650-604-6982
michele.johnson@xxxxxxxx

Whitney Clavin
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-4673
whitney.clavin@xxxxxxxxxxxx

RELEASE: 12-013

NASA'S KEPLER MISSION FINDS THREE SMALLEST EXOPLANETS

WASHINGTON -- Astronomers using data from NASA's Kepler mission have 
discovered the three smallest planets yet detected orbiting a star 
beyond our sun. The planets orbit a single star, called KOI-961, and 
are 0.78, 0.73 and 0.57 times the radius of Earth. The smallest is 
about the size of Mars.

All three planets are thought to be rocky like Earth, but orbit close 
to their star. That makes them too hot to be in the habitable zone, 
which is the region where liquid water could exist. Of the more than 
700 planets confirmed to orbit other stars -- called exoplanets -- 
only a handful are known to be rocky. 

"Astronomers are just beginning to confirm thousands of planet 
candidates uncovered by Kepler so far," said Doug Hudgins, Kepler 
program scientist at NASA Headquarters in Washington. "Finding one as 
small as Mars is amazing, and hints that there may be a bounty of 
rocky planets all around us." 

Kepler searches for planets by continuously monitoring more than 
150,000 stars, looking for telltale dips in their brightness caused 
by crossing, or transiting, planets. At least three transits are 
required to verify a signal as a planet. Follow-up observations from 
ground-based telescopes also are needed to confirm the discoveries.

The latest discovery comes from a team led by astronomers at the 
California Institute of Technology in Pasadena. The team used data 
publicly released by the Kepler mission, along with follow-up 
observations from the Palomar Observatory, near San Diego, and the 
W.M. Keck Observatory atop Mauna Kea in Hawaii. Their measurements 
dramatically revised the sizes of the planets from what originally 
was estimated. 

The three planets are very close to their star, taking less than two 
days to orbit around it. The KOI-961 star is a red dwarf with a 
diameter one-sixth that of our sun, making it just 70 percent bigger 
than Jupiter.

"This is the tiniest solar system found so far," said John Johnson, 
the principal investigator of the research from NASA's Exoplanet 
Science Institute at the California Institute of Technology in 
Pasadena. "It's actually more similar to Jupiter and its moons in 
scale than any other planetary system. The discovery is further proof 
of the diversity of planetary systems in our galaxy." 

Red dwarfs are the most common kind of star in our Milky Way galaxy. 
The discovery of three rocky planets around one red dwarf suggests 
that the galaxy could be teeming with similar rocky planets. 

"These types of systems could be ubiquitous in the universe," said 
Phil Muirhead, lead author of the new study from Caltech. "This is a 
really exciting time for planet hunters."

The discovery follows a string of recent milestones for the Kepler 
mission. In December 2011, scientists announced the mission's first 
confirmed planet in the habitable zone of a sun-like star: a planet 
2.4 times the size of Earth called Kepler-22b. Later in the month, 
the team announced the discovery of the first Earth-size planets 
orbiting a sun-like star outside our solar system, called Kepler-20e 
and Kepler-20f. 

For the latest discovery, the team obtained the sizes of the three 
planets called KOI-961.01, KOI-961.02 and KOI-961.03 with the help of 
a well-studied twin star to KOI-961, or Barnard's Star. By better 
understanding the KOI-961 star, they then could determine how big the 
planets must be to have caused the observed dips in starlight. In 
addition to the Kepler observations and ground-based telescope 
measurements, the team used modeling techniques to confirm the planet 
discoveries. 

Prior to these confirmed planets, only six other planets had been 
confirmed using the Kepler public data.

NASA's Ames Research Center in Moffett Field, Calif., manages Kepler's 
ground system development, mission operations and science data 
analysis. NASA's Jet Propulsion Laboratory, Pasadena, Calif., managed 
the Kepler mission's development.

For information about the Kepler Mission, visit:

http://www.nasa.gov/kepler 

	
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