Modern techniques to discover exoplanet candidates - Radial velocity or Transit methods - have their own limitations. In order to confirm that a candidate is an exoplanet you should make 3 standalone, independent observations. Each of these observations should show disturbances of radial velocity or drops in starlight flux for at least for three times.
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Негізгі бет Ғылым және технология On the Universe and Tau Ceti
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