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How Does The Very Large Telescope Work?

18 May, 2012

MessageToEagle.com - The world's most advanced optical instrument, the Very Large Telescope (VTL) is located in the Atacama Desert, on Cerro Paranal, a mountain in Chile.

Operated by ESO the the Very Large Telescope Interferometer, allows astronomers to see details up to 25 times finer than with the individual telescopes.

Explore the state-of-the-art technology behind the Very Large telescope, which has provided astronomers with an unequalled view of the Universe.

To obtain the sharpest images of the sky, the VLT has to cope with two major effects that distort the images of celestial objects.

The first one is mirror deformations due to their large sizes.

This problem is corrected using a computer-controlled support system - active optics - that ensures that the mirrors keep their desired shapes under all circumstances.

The second effect is produced by Earth's atmosphere, which makes stars appear blurry, even with the largest telescopes.

Adaptive optics is a real-time correction of the distortions produced by the atmosphere using computer-controlled mirrors that deform hundreds of times per second to counteract the atmospheric effects.

As one demonstration of its power the VLT's sensitive infrared cameras, helped by adaptive optics, have been able to peer through the massive dust clouds that block our view to Milky Way's core.

The images, taken over many years, have allowed astronomers to actually watch stars orbiting around the monstrous black hole that lies in the center of our galaxy. It was even possible to detect energetic flares from gas clouds falling into the black hole.

The Very Large Telescope is without doubt impressing and keeps delivering surprises to astronomers.

MessagetoEagle.com

See also:
Beautiful Night Sky Timelapse Takes You On A Journey To Astronomer's Paradise

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