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Adaptive optics is a telescopic system designed to enhance image resolution by correcting distortions caused by atmospheric turbulence. This technology is crucial in astronomy because Earth's atmosphere can blur images from telescopes, limiting the detail observable.12

By rapidly adjusting the telescope's mirror surface, adaptive optics can counteract the effects of atmospheric turbulence, leading to clearer and more detailed astronomical images. This technique allows ground-based telescopes to achieve resolutions closer to their theoretical limits, overcoming a significant challenge in astronomical observation.21

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