Sharper than Hubble
from Arizona Science
How changing the shape of a mirror a thousand times per second results in high resolution imaging of low-mass stars, brown dwarfs, and extrasolar planets.
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What this episode covers
How changing the shape of a mirror a thousand times per second results in high resolution imaging of low-mass stars, brown dwarfs, and extrasolar planets. In this Episode: Laird Close Ph.D. Professor, Department of Astronomy and Steward Observatory at the University of Arizona; Tim Swindle, Ph.D, Director and Department Head of the University of Arizona's Lunar and Planetary Laboratory
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