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Ground-based imaging of extrasolar planets using adaptive optics

Abstract

The detection of extrasolar planets by direct imaging presents an extraordinary technical challenge. They must be identified against background light scattered from a star close by and about a billion times brighter. It has been supposed that a near-perfect space telescope would be required to avoid atmospheric blurring. But by using adaptive optics operating at fundamental performance limits, the new generation of large ground-based telescopes has the potential to detect planets orbiting nearby stars.

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Angel, J. Ground-based imaging of extrasolar planets using adaptive optics. Nature 368, 203–207 (1994). https://doi.org/10.1038/368203a0

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