= Solution
First, an Earth-like atmosphere produces signals of only order parts per million in transit and planet-star contrasts near $10^{-10}$ in reflected light, demanding extreme photon collection, calibration, and starlight suppression. Second, stellar spots, faculae, flares, and spectral variability can imitate or overwhelm atmospheric features, especially around active M dwarfs. Third, long orbital periods provide few transits, while clouds, hazes, refraction, and overlapping molecular bands make the resulting sparse spectra difficult to interpret uniquely.
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