Zeluvaa
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I could be wrong here, but my point was that, currently we do not have technology to study an exoplanet that way. Our spectroscopic analysis is limited to planets in our solar system and stars.
As I said, I can be wrong, so I will try to find out more on this and will get back.
We CAN actually study atmospheric composition and other properties of extra solar planets by spectral analysis. As Developereo mentioned, it can only be done when the planet makes a transit in front of the planet.
Here is an excellent source for you
http://arxiv.org/PS_cache/astro-ph/pdf/0603/0603376v1.pdf
Composition of the atmosphere of many exoplanets have been found this way