The most successful technique for finding planets beyond our solar system so far is transit photometry, which measures changes in a star’s brightness caused by a mini-eclipse. When a planet crosses in front of its star along our line of sight, it blocks some of the star’s light. If the dimming lasts for a set amount of time and occurs at regular intervals, it likely means an exoplanet is passing in front of, or transiting, the star once every orbital period.
NASA’s Kepler Space Telescope has used this technique to become the most successful planet-hunting spacecraft to date, with more than a thousand established discoveries and many more awaiting confirmation...
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