Transit depth refers to the fraction of a star's light that is blocked when a planet passes in front of it, measured during a transit event. This measurement is crucial because it provides insights into the size of the exoplanet relative to its host star, enabling scientists to infer the planet's radius and potential atmospheric characteristics. Understanding transit depth enhances the analysis of light curves generated by different observational methods, which can reveal vital information about exoplanets, their compositions, and their orbits.
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