Showing posts with label Adaptive optics. Show all posts
Showing posts with label Adaptive optics. Show all posts

Laser Towards Milky Ways Centre

Laser Towards Milky Ways Centre


DescriptionEnglish: In mid-August 2010 ESO Photo Ambassador Yuri Beletsky snapped this photo at ESO’s Paranal Observatory, Chile. A group of astronomers were observing the centre of the Milky Way using the laser guide star facility at Yepun, one of the four Unit Telescopes of the Very Large Telescope (VLT).
Yepun’s laser beam crosses the southern sky and creates an artificial star at an altitude of 90 km high in the Earth's mesosphere. The Laser Guide Star (LGS) is part of the VLT’s adaptive optics system and is used as a reference to correct the blurring effect of the atmosphere on images. The colour of the laser is precisely tuned to energise a layer of sodium atoms found in one of the upper layers of the atmosphere — one can recognise the familiar colour of sodium street lamps in the colour of the laser. This layer of sodium atoms is thought to be a leftover from meteorites entering the Earth’s atmosphere. When excited by the light from the laser, the atoms start glowing, forming a small bright spot that can be used as an artificial reference star for the adaptive optics. Using this technique, astronomers can obtain sharper observations. For example, when looking towards the centre of our Milky Way, researchers can better monitor the galactic core, where a central supermassive black hole, surrounded by closely orbiting stars, is swallowing gas and dust.
Taken with a wide angle lens, this photo covers about 180° of the sky.
Date6 September 2010
Sourcehttp://commons.wikimedia.org/wiki/File:Laser_Towards_Milky_Ways_Centre.jpg
AuthorESO/Yuri Beletsky (ybialets at eso.org)
PermissionCreative Commons Attribution 4.0 International License
LicensingThis file is licensed under the Creative Commons Attribution 4.0 International license.


From Wikimedia Commons http://commons.wikimedia.org/