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  • The contrastbetween star and planet at these wavelengths becomes so advantageous that, for the nearest stars,hydrogen, helium, methane, water ammonia and other molecules can all be detected in low-resolutionspectra of the atmospheres of super-Earth planets in habitable zones.Alternatively, exoplanet atmospheres can be observed during transits in the optical and near-infrared.Ground- and space-base
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