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Kepler spots exoplanets by noting the tiny brightness dips caused when they cross the face of their parent stars.
Kepler finds alien worlds by detecting the tiny brightness dips caused when they transit, or cross the face of, their stars from the instrument's perspective.
The $600 million Kepler observatory detects exoplanets by flagging the tiny brightness dips caused when they pass in front of their host stars from the instrument's perspective.
It was spotted by NASA's Kepler space telescope, which launched in March 2009 to hunt for transiting exoplanets by noting the tiny brightness dips caused when they cross in front of their stars.
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It looked for tiny dips in brightness caused when planets drift in front of their parent star.
Their existence is given away by a tiny drop in brightness caused when a planet transits in front of its parent star, as seen from Earth.
Kepler will take a different approach in its planetary scan, Dr. Seager said, searching not for stellar wobbles but for "tiny drops in brightness," possible signs of a planet transiting across the distant Sun's face.
On September 26th the group announced, in a paper posted to arXiv, an online database, that its participants had discovered two probable exoplanets, one a Jupiter-like gas giant, and the other, possibly, a smaller, rocky world about twice the diameter of Earth.Kepler works by monitoring the thousands of stars in its field of view for tiny changes in brightness.
And it orbits its parent star firmly inside the "habitable zone", in which temperatures are just right for liquid water.The planet was found by NASA's recently-defunct Kepler space telescope, which stared at hundreds of thousands of distant stars, looking for the tiny dip in brightness produced when a planet crosses in front of its star as seen from Earth.
Kepler, an orbiting telescope owned by NASA, America's space agency, looks for exoplanets by identifying the tiny dip in brightness caused when one of them passes in front of its host star, as seen from Earth a phenomenon known as "transiting".
As exciting as the plans for direct imaging are, most exoplanets are still found using indirect techniques – such as detecting a wobble in the position of the star that indicates it is being pulled slightly towards an orbiting planet, or a method called "transiting", in which planets are identified by the tiny dip in brightness caused when they pass in front of its star.
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