Astronomers can determine a planet's materials by analyzing the light it reflects, but this process is particularly challenging for distant exoplanets due to interference from surrounding light sources. Spectroscopic data is primarily obtained from transit planets, where the planet's atmosphere absorbs specific wavelengths, creating a detectable dip in the spectrum. Direct imaging is feasible for larger planets in wide orbits, requiring advanced telescopes to isolate the target light. Recent advancements, such as Multi-Laser Ground Layer Adaptive Optics, enhance the ability to study exoplanet atmospheres. The discussion highlights the importance of technology in capturing and analyzing light from distant celestial bodies.