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if an exoplanet is orbiting this star such that from our vantage point it goes in front of the star then that exoplanet will block out some star light and cause a dip in its Luminosity we can detect this and this is a common method of detecting exoplanets the trick now is that if the exoplanet has an atmosphere then some of the light from the Star will pass through that atmosphere the light that passes through the atmosphere because it interacts with the chemicals in it can give us a lot of information about that atmosphereamp;#39;s chemical composition so by analyzing the light coming from the Star and then subtracting the light that passed through the atmosphere we can get a signature of what was absorbed and match that with known chemicals
