File:Light Curve of a Planet Transiting Its Star.jpg

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English: Transit data are rich with information. By measuring the depth of the dip in brightness and knowing the size of the star, scientists can determine the size or radius of the planet. The orbital period of the planet can be determined by measuring the elapsed time between transits. Once the orbital period is known, Kepler's Third Law of Planetary Motion can be applied to determine the average distance of the planet from its stars.
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Source http://www.nasa.gov/mission_pages/kepler/multimedia/images/transit-light-curve.html
Author NASA Ames

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current19:02, 25 January 2013Thumbnail for version as of 19:02, 25 January 20132,126 × 905 (259 KB)Stas1995 (talk | contribs)User created page with UploadWizard

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