Reflection, Refraction and Diffraction

Keck Telescope

The most powerful telescope on the summit on Mauna Kea is the twin Keck observatory, which has two 10 metre diameter mirrors. At the heart of each Keck Telescope is a revolutionary primary mirror made up of 36 hexagonal segments that effectively work as a single piece of reflective glass. By combining advanced optical and infrared detectors with sophisticated electronics that can combine collected light from both telescopes, the Keck observatory remains amongst the leading astronomical facilities in the world.

Very Large Telescope (VLT)

The Very Large Telescope (VLT) is located at the Paranal Observatory in Chile's Atacama desert, and is the world's most advanced optical telescope. It comprises four 8.2 metre reflecting telescopes and three auxiliary 1 metre telescopes that can move about.

The VLT produces extremely sharp images using a special technique called optical inferometry (i.e. combining the light from all telescopes) and can capture light from the faintest and most remote objects in the Universe.