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Corning Reaches Milestone In Development Of Discovery Channel Telescope
Corning NY (SPX) Jun 23, 2005 Corning announced Wednesday that it has completed the sagging process of the 4.2-meter ULE(r) mirror blank that will serve as the primary mirror for Lowell Observatory's Discovery Channel Telescope. Corning's proprietary ULE(r) is a glass material which exhibits virtually no dimensional changes over extreme temperature variations. This material is generally considered to be one of best in the world for astronomical optics. The sagging process consisted of creating a form made of refractories that meet the concave-convex shape requirements of mirror designers. The ULE mirror blank was positioned over the form and heated to approximately 2700� Fahrenheit to attain the material's softening point. At this point, the blank began to sag around the refractories and conformed to the specifications of the mirror designers. Danny Henderson, division vice president and business director, Corning Specialty Materials said, "Corning is very proud to have been selected the material supplier for the DCT mirror. The successful completion of the sagging milestone can be attributed to Corning's wealth of experience in supplying astronomy ULE mirrors and the excellent performance of the team in Canton, N.Y. We are now proceeding to the next phase of the program, the net grinding of the mirror blank. Corning looks forward to working closely with Discovery Communications and Lowell Observatory through completion of the DCT mirror." The Discovery Channel Telescope (DCT) will be located at a new site being developed by Lowell Observatory on the Coconino National Forest in northern Arizona. The telescope will support research of Lowell Observatory astronomers and provide programming opportunities for Discovery Communications, the parent company of cable television's Discovery Channel. When completed, it will be the fifth largest telescope in the continental United States. The telescope will have a wide variety of uses including: the search for potentially threatening earth-approaching asteroids, exploration of the outer solar system, including the newly discovered Kuiper Belt, and investigations of distant stars and galaxies. The DCT has a unique optical configuration that allows it the ability to focus on a wide field or to be switched to a longer focal length. This attribute greatly exceeds the capabilities of today's existing telescopes of the same class. The DCT, in a single wide field exposure mode, will allow astronomers to survey an area of the sky equal to the size of 16 full moons. In the longer focal length mode, the DCT will allow astronomers to zoom in on selected objects for detailed observation and subsequent analysis. During a recent visit to Canton, N.Y. to view the progress of the mirror blank production, Robert L. Millis, director of Lowell Observatory said, "Corning has demonstrated unfailing professionalism, outstanding customer service, and impressive mastery of its state-of-the-art manufacturing processes during the fabrication of the ULE primary mirror blank for the Discovery Channel Telescope. We look forward to having this Corning product at the heart of our new telescope." Community Email This Article Comment On This Article Related Links Corning Semiconductor Optics Corning Incorporated SpaceDaily Search SpaceDaily Subscribe To SpaceDaily Express Space Telescope News and Technology at Skynightly.com
Large Binocular Telescope Successfully Achieves "First Light"
Tucson AZ (SPX) Oct 27, 2005The Large Binocular Telescope (LBT) partners in the U.S.A., Italy and Germany are pleased to announce that they chieved "First Light" on Oct. 12, 2005. These exceptional images were obtained with one of the telescope's two primary mirrors in place and were released Wednesday.
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