Optical and infrared observations are the bread and butter of astronomy. For thousands of years the earliest scientists were inspired by the light coming from the sun and the night sky, the light they could see with the unaided eye. These observations have shaped our vision of the world throughout history. Using modern telescopes we can see far beyond the wavelengths visible to the naked eye, catching the photons from the most distant known objects in the Universe, from radio waves through to the most energetic gamma rays. But it’s optical and infrared images, like those produced by the Hubble Space Telescope, that still prove the most inspiring to many scientists and the public.
For the past 2 years I’ve been involved in the planning of the next generation of optical/IR observatories, the European Extremely Large Telescope or E-ELT. Specifically, I work on the design of a potential instrument for this mammoth of a telescope, whose 42-m primary mirror diameter will be four times larger than the largest optical telescopes in the world today. Previous generations of telescopes have always seen an approximate doubling of mirror size, and this new generation of observatories signal an important departure from this trend – a hugely ambitious endeavour by all accounts.


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