This issue reports a brief review about transit method of detecting extrasolar planet (exoplanet). When a exoplanet crosses (transits) in front of its host star's disk along the line of sight, then the observed visual brightness of the star drops by a small amount. The transit method is responsible for 23% of some important new discoveries of exoplanets. In this sense, we explain didactically the conceptual and calculational details of transit method. As a result of application of the transit method, we applied it to exoplanet COROT-1b.
CITATION STYLE
Santos, W. C., & Amorim, R. G. G. (2017). Transit method and discovery of exoplanet. Revista Brasileira de Ensino de Fisica, 39(2). https://doi.org/10.1590/1806-9126-RBEF-2016-0217
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