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Kepler’s 6 Years in Science and Counting

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NASA’s Kepler spacecraft began hunting for planets outside our solar system on May 12, 2009. From the trove of data collected, we have learned that planets are common, that most sun-like stars have at least one planet and that nature makes planets with unimaginable diversity. Kepler was launched on March 6, 2009. Its mission was to survey a portion of our galaxy to determine what fraction of stars might harbour potentially habitable, Earth-sized exoplanets, or planets that orbit other stars. Of particular interest are exoplanets orbiting in the habitable zone — the range of distance from a star in which the surface temperature of an orbiting planet might sustain liquid water. For life as we know it, liquid water is a necessary ingredient. Of the more than 1,000 confirmed planets found by Kepler, eight are less than twice the size of Earth and are in their stars’ habitable zone. All eight orbit stars cooler and smaller than our sun.  During its four-year prime mission, Kepler simultaneously and continuously measured the brightness of more than 150,000 stars, looking for the telltale dimming that would indicate the presence of an orbiting planet. From these dimmings, or transits, and information about the parent star, researchers can determine a planet’s size (radius), the time it takes to orbit its star and the amount of energy received from the host star.

Kepler’s exquisitely precise photometer, or light sensor, was designed to detect minute changes in brightness, in order to infer the presence of an Earth-sized planet. For a remote observer, Earth transiting the sun would dim its light by less than 1/100th of one percent, or the equivalent of the amount of light blocked by a gnat crawling across a car’s headlight viewed from several miles away.

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