Inustry
News—A Whirlwind Visit to Potential Glass Suppliers
Gary
Sanders
A
project like TMT simply cannot take place without a strong industrial
component. This space in the Newscast, "Industry News," has
featured articles written by several of our current industrial
partners (M3 of Tucson, Hytec of Los Alamos, AMEC of Vancouver).
We also described a prospective primary
mirror glass supplier, Corning, in our first "Focus On" article.
In this installment I want to describe the next steps in acquiring
the hundreds and hundreds of finished primary segments that we
will need for TMT (which Jerry Nelson began
explaining last month,
and finishes up in an article on
polishing mirrors in this Newscast.)
Actually, this step was quite a bit of fun, though it involved
grueling travel and long, but productive, work days. We have to
buy glass. We must have the glass blanks polished to shape and
tested by optical means. The finished segments must meet our demanding
requirements and they must be as cheap as possible. The strategy
is to contract with the most capable companies in the world through
a competitive process. And so we have to come to know these companies
and their capabilities, methods and products.
TMT-quality
zero-expansion glass is currently supplied by Corning (Canton,
NY), LZOS (Lytkarino, Russia), Ohara (Sagamihara, Japan), and
Schott (Mainz, Germany). In our first "Focus On" article
in June, we are photographed standing next to a TMT-shaped sample
segment produced by Corning. But visits at a trade show do not
provide the kind of detailed exploration of requirements and products
that factory visits do. We must visit the four firms who may supply
the glass blanks for TMT. This is a key early step in setting up
a fair commercial competition. Unfortunately, these specialty glass
suppliers are located in far-flung locales.
Similarly, our prospective segment fabrication firms are few and
far and wide. We previously conducted a commercial bidding process
that selected three firms or consortia to engage in the first stage
of fabrication studies. The selected firms are ITT (Rochester,
NY) teamed with Tinsley (Richmond, CA); SAGEM (Paris, France);
and Zygo (Middlefield, CT). Each of these three partners has delivered
a design for TMT segment fabrication and several studies have been
initiated with glass prototypes. Visiting these firms is an essential
step in refining the remaining commercial selection process.
We decided to start with a marathon visit to three of the eight
firms listed above. So five senior members of TMT1 gathered one
recent weekend, on a warm sunny afternoon, to jet off to Moscow,
where the temperature hovered near freezing and light snow flurries
would remind us that we had departed California.
After a 12+ hour overnight flight and another long night of sleep,
we visited the very impressive Soviet-era factory of LZOS, crown
jewel of glass suppliers in Russia since 1939. Large boules of
zero-expansion Astrosital entertained us, as did precision grinding,
machining and polishing tools, and optical testing setups. Detailed
discussions of thermal expansion, stress birefringence, homogeneity,
and price filled a long day. The Southern African Large Telescope
(SALT), a 10-meter segmented mirror, is fashioned from this Russian
product. Clearly, LZOS has moved successfully from state ownership
to the capitalism of a Joint Stock Company.
After
a long day at LZOS, we spent our only evening in Moscow walking
around the Kremlin and St. Basil’s cathedral. High
above the ramparts of the venerable Kremlin, in the evening dusk,
two bright luminous red stars marked the scene. Yes, these are
the very glassy, illuminated
red stars that have hung over the
Kremlin through decades of the Cold War. And the red glass in those
stars was made by LZOS, a reminder of the famed factory that we
had visited hours before.
We traveled to Mainz, Germany the next day, where Schott paraded
their Zerodur glass, used in the Keck 10-meter mirrors and in many
other astronomy applications. Another long, but exciting, day spent
in technical and commercial discussions was rounded out by a tour
of the glass-processing facilities. There we saw a sample TMT segment
blank produced by Schott and processed in a preliminary manner
by SAGEM. The group gathered around this icon as it lay in an inspection
machine.
Another
dash by jet to Paris and another full day; this time at SAGEM
(formerly REOSC), also well known in the astronomy business.
The 8-meter Gemini and ESO VLT mirrors were made here, as were
the recent segments for the primary mirror of the 10-meter Gran
Telescopio Canarias (GTC) in the Canary Islands. Technical and
commercial discussions and tours of circular and planetary polishing
machines were capped by a first look at an experimental stressed
mirror polishing setup for TMT segments (read Jerry
Nelson’s
companion piece on polishing). SAGEM has been working under contract
to us for a year and its progress is visible in front of us.
After an evening in downtown Paris, a fine meal and a stroll about
the iconic Eiffel Tower, the tired team smiles back at the camera
in the photo. A vigorous week. Perhaps the smile is contemplation
of the long ride home in the morning.
Ohara and Corning and ITT and Tinsley and Zygo will be next.
1 Project Manager Gary Sanders, Business Manager David
Goodman, Project Scientist Jerry Nelson, Telescope Department Head
Larry Stepp, and Optics Group Leader Ben Platt made the trip. |