Printer Friendly
The Free Library
5,666,618 articles and books
Member login
User name  
Password 
 
Join us Forgot password?

MOLDING SUCCESSFUL MIRROR PROJECT : ARIZONA CAST TO FASHION 40,000 POUNDS OF GLASS TO USE IN TELESCOPE.


Byline: Arthur H. Rotstein Associated Press Associated Press: see news agency.
Associated Press (AP)

Cooperative news agency, the oldest and largest in the U.S. and long the largest in the world.
 

Beneath the University of Arizona's football stadium, a massive, spinning furnace is being tested, empty except for a giant mold inside.

The furnace is being heated nightly for the next few weeks to 1,180 degrees Celsius - more than 2,150 degrees Fahrenheit. Later this month, when cooled, it will be opened and the mold checked to make certain there are no cracks.

Workers will load it with nearly 20 tons of glass, and sometime in January it will be fired up for real.

The 40,000 pounds of glass will be cooked to make the first of twin 8.4-meter mirrors about 3-1/2 inches thick for the Large Binocular Telescope The Large Binocular Telescope (LBT, originally named the Columbus Project) is located on 10,700-foot Mount Graham in the Pinaleno Mountains of southeastern Arizona and is a part of the Mount Graham International Observatory. .

``It's the routine pre-fire act that we go through before every casting,'' says Roger Angel, head of the Steward Observatory The University of Arizona's Steward Observatory's main office is located on the University's campus and is closely tied to the Department of Astronomy. Established in 1916 by its first director, Andrew Ellicott Douglass, and a $60,000 bequest made by Lavinia Steward in memory of  Mirror Laboratory.

``Right now we're heating the mold empty . . . before we commit $700,000 of glass,'' adds John Hill, director of the $60 million telescope project and Steward's mirror-casting director.

The single-piece slabs of glass will be the key ingredients in the Large Binocular Telescope. Each will be polished to form a mirror more than 27 feet in diameter. Together, they will provide the telescope with viewing power to make it one of the world's most powerful optical instruments.

The project on 10,700-foot Mount Graham Mount Graham is a mountain in southeastern Arizona in the United States, in the Coronado National Forest. It is the highest mountain in the Pinaleño Mountains. The mountain reaches 10,720 feet (3,267 meters) in height, attaining the highest elevation in Graham County.  near Safford, 125 miles northeast of Tucson, finally is on track to completion after a decadelong dec·ade·long  
adj.
Lasting a decade: a decadelong national research effort. 
 court fight with an environmental coalition. Opponents said they feared building the telescope would lead to extinction of an endangered subspecies subspecies, also called race, a genetically distinct geographical subunit of a species. See also classification.  of red squirrel found nowhere else.

Angel came up with the idea about 15 years ago to revolutionize mirror-making by creating huge, relatively inexpensive, single-piece mirrors that are lightweight yet rigid.

The key was to melt borosilicate glass borosilicate glass
n.
A strong heat-resistant glass that contains a minimum of 5 percent boric oxide.
 in a spinning furnace to create a glass blank with hollow backing and a steep focal ratio Noun 1. focal ratio - the ratio of the focal length to the diameter of a (camera) lens system
f number, stop number, speed

ratio - the relative magnitudes of two quantities (usually expressed as a quotient)
. In other words Adv. 1. in other words - otherwise stated; "in other words, we are broke"
put differently
, part of the structure of the mirror is built the same way as a bee's honeycomb honeycomb

a mosaic of closely packed units with depressed centers giving a honeycomb appearance.


honeycomb ringworm
see favus.

honeycomb stomach
reticulum.
 - partly hollow but still strong and lightweight. The focal ratio is considered critical because it holds expenses down by reducing the height of the building needed to house the telescope.

No one has cast as large a blank of glass conventionally, Hill said. One of comparable thickness and focal ratio would weigh five times more - 100 tons.

When the furnace is turned on for real, he said, it will be kept at its maximum temperature for about 11 hours.

``That's the time for the glass to melt and fill the mold,'' Angel said. The furnace then will spin for three days to let the glass solidify, followed by up to four months of slow cooling so that it tempers and hardens without becoming brittle. That process is called annealing annealing (ənēl`ĭng), process in which glass, metals, and other materials are treated to render them less brittle and more workable. .

``It may be as slow as 5 degrees a day,'' said Angel, who received a five-year, $330,000 grant last spring from the John D. and Catherine T. MacArthur Foundation John D. and Catherine T. MacArthur Foundation, philanthropic institution founded 1978 by John D. MacArthur (1897–1978), owner of a prominent insurance company and other businesses, and his wife Catherine T.  in recognition of his creativity.

Two periods in the mirror production will be critical. The first is when the temperature is cranked all the way up, he said.

``The period of maximum danger, I would guess, is while the glass is liquid, because it exerts strong buoyant forces on the mold,'' Angel said.

``It's trying to lift up, and there are significant forces trying to tear the mold apart. We think we've made it strong enough. That's the acid test.''

The other will be at temperatures of about 500 degrees Celsius to about 450 degrees, during the annealing, Angel said.

The mirror lab has produced glass blanks 3.5 meters in diameter and two of 6.5 meters, and each time the size has increased, new things have been learned, Angel said.

Angel hopes there won't be too many new lessons this time.

``We try to fix everything we can anticipate,'' he said. ``So the new lesson will be things we didn't anticipate.''

After the glass is cast, it will take about two years to polish the first mirror by computer - once smaller ones already in queue are finished.

The cost for each big mirror, when cast and polished, will be about $12 million, Hill said.

``This probably won't go to the mountain until the fall of 2000 or something like that,'' Hill said.

CAPTION(S):

Photo

Photo: University of Arizona's Dean Ketelsen checks out a finished mirror before grinding and finishing in the mirror laboratory in Tucson, Ariz.

Associated Press
COPYRIGHT 1996 Daily News
No portion of this article can be reproduced without the express written permission from the copyright holder.
Copyright 1996, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

 Reader Opinion

Title:

Comment:



 

Article Details
Printer friendly Cite/link Email Feedback
Publication:Daily News (Los Angeles, CA)
Date:Dec 1, 1996
Words:745
Previous Article:NASA HOPES TO BEAT ODDS ON MARS ROVER.(NEWS)
Next Article:NOTED NEW MEXICO SHOEMAKER CAPTURES CLIENTS' SOLES.(NEWS)



Related Articles
Large telescopes, low prices; astronomers do it with mirrors - by leaving out most of the glass.
NNTT's next generation: harmonizing a quartet of large telescopes. (National New Technology Telescope)
Spinning a large telescope from glass.
New telescope for old. (Multiple Mirror Telescope to cast single mirror)
Big telescopes on a roll: the world has a number of projects for telescopes in a size range thought to be impossible not many years ago.
Small foam-mirror telescope built.
Rodents and telescopes: a squirrelly issue. (endangered squirrel on a planned observatory sight in Arizona)
Dawn of a big telescope: astronomers await the debut of Keck's tiled mirror. (W.M. Keck Observatory, Hawaii) (Cover Story)
Hubble's flaws: looking for the source. (Hubble Space Telescope)
Store fixture components. (Illustrated Product Guide).(Advertisement)

Terms of use | Copyright © 2009 Farlex, Inc. | Feedback | For webmasters | Submit articles