SUBARU Telescope 8.3m Primary Mirror Finished (Forwarded) 
Author Message
 SUBARU Telescope 8.3m Primary Mirror Finished (Forwarded)
Subaru Telescope
650 N. A'ohoku Place
Hilo, Hawaii 96720
U.S.A.

CONTACTS:

Subaru Telescope, Hilo, HAWAII:


Prof. Masahiko Hayashi,

Dr. Ian Shelton, Public

NAOJ, Mitaka, JAPAN:

Prof. H. Karoji, Subaru

FOR RELEASE: SATURDAY, AUGUST 29, 1998, 00:00 JST
(FRIDAY AUGUST 28, 1998, 11:00 EDT)

PRESS RELEASE NO.: ST-PR980829

SUBARU Telescope 8.3m Primary Mirror Finished

The largest monolithic mirror with the highest surface quality

Overview :

The National Astronomical Observatory of Japan (NAOJ) has announced the
completion of one of the world's largest monolithic optical-infrared
mirrors, with a physical diameter of 8.3 meters (27 feet). The mirror is
destined for the NAOJ Subaru Telescope under construction atop Mauna Kea,
Hawaii.

A team of opticians at Contraves Brashear Systems (CBS) led by Dr. S. Smith
completed the painstaking polishing of the huge primary mirror at the end of
July 1998 at the Wampum underground facility of CBS in the suburbs of
Pittsburgh, Pennsylvania. The engineering team of NAOJ, MELCO (Mitsubishi
Electric Corporation), and CBS carried out intensive measurements to verify
the surface figure of the primary mirror while it was mounted on its
computer controlled support system manufactured by MELCO. They confirmed
that the mean residual rms surface error can be reduced to as small as 12
nanometers* over an entire surface of 8.2 meters in diameter, making this
the most accurate mirror of such size ever produced.
(* 1 nanometer or "nm" = ~0.00000004 inches)

To help understand this achievement, imagine enlarging the 8.2m surface to
82 km (51 miles), which is about the size of the Big Island of Hawaii. The
mean residual error of 12 nm would then correspond to the task of smoothing
out the landscape to follow a precisely specified curve with no hills or
valleys (on average) taller or deeper than 0.12 mm (0.005"), the thickness
of an ordinary sheet of paper! This tremendous achievement is the outcome of
combining large mirror fabrication expertise found in the United States with
Japanese expertise in making sophisticated control systems.

The Subaru Telescope project has now successfully completed its most
difficult and important phase. The primary mirror will leave Wampum in
September and arrive at the summit of Mauna Kea by the end of October. At
the summit, the mirror will receive a thin coating of pure aluminum to make
it highly reflective and finally be attached to the telescope's mechanical
structure. Tests to evaluate the telescope's performance will follow. We are
planning to obtain our first scientifically important images (i.e. "First
Light") at the end of January next year.

Facts and Data:

1. Subaru Primary Mirror Size and Specifications

Constructed from Corning Ultra Low Expansion Glass (ULE) ...
     Thermal Expansion Coefficient ... less than 10 parts per billion
     per deg Celsius.

Physical Size ...
     Diameter: 8.3m (27'), with a central hole 1.2 m (4') in diameter
     Thickness: 20cm (8")
     Weight: 22.8 metric tons
     Effective Mirror Surface: 8.2m diameter
     Focal Length: 15 m (49')

Surface error (root mean square) ... 12 nm after 32 mode active correction
of residual deformation

Strehl Ratio* ... 0.916 at 500 nm wavelength
     * Strehl Ratio is a measure describing the deterioration due to the
     surface error. Ideal value is 1.0. The achieved value of 0.916 is
     outstanding for visual wavelengths.

The 80 % encircled energy** ... 0.04 arcsec at 500 nm wavelength
     ** This means that 80 % of visual photons collected by this primary
     mirror would fall onto a tiny spot that corresponds to 0.04 arcsec on
     the sky (about 0.00002 times the apparent diameter of the full Moon).

2. Comparison With Other Large Mirrors

European Southern Observatory (ESO) successfully started the test operation
of their first 8.1m telescope, VLT1 in Chile at the end of May this year and
has shown it can produce very sharp images. There will be three more 8m
telescopes, VLT2, 3, and 4 to be completed by ESO. In addition, the GEMINI
consortium is constructing twin 8m telescopes, one at Mauna Kea and the
other in Chile. Some of the primary mirrors of these 8m telescopes are
already completed. The Subaru primary mirror, however, is the largest and
appears to have the smallest surface error among these 8m mirrors.

Subaru Telescope, with this marvelous primary mirror will have an imaging
capability that rivals that of the Hubble Space Telescope (HST). The light
gathering power of the Subaru Telescope is more than 10 times larger than
that of the HST. Subaru Telescope, together with other 8m class telescopes
and the two 10 m Keck telescopes with segmented mirrors, will contribute
much to enhance our understanding on the structure and evolution of the
Universe.

3. Outline of the Subaru Project

The 9 year project to construct the 8.2m Subaru Telescope began in the
fiscal year 1991. The total budget of the project amounts to about 38
billion yen. It has the world's largest monolithic thin primary mirror,
supported by 261 computer controlled actuators to achieve the ideal surface
shape to collect light from distant faint objects. The enclosure of Subaru
Telescope has a capability to suppress thermal turbulence around the
telescope. Seven scientific instruments are under construction to allow
various modes of observation.

Subaru Telescope, together with VLT, GEMINI, Keck, and HST, is expected to
open up a new era for the exploration of the universe.

NAOJ established the Subaru Telescope Hawaii Facility in Hilo, Hawaii in
April 1997 to support the construction and operation of this telescope. This
is Japan's first governmental research institute built and operated in a
foreign country. A total of 24 staff members moved from Japan and about two
dozen local members are expected to be hired and work around the clock at
Subaru Telescope. The director of Subaru Telescope is professor Norio Kaifu.

4. The First Light Event

The "First Light" of Subaru Telescope is expected to take place at the end
of January 1999. Details of the schedule will be announced in October 1998.
NAOJ is planning to arrange another press release and have live broadcasting
of the First Light scene and initial images taken with Subaru Telescope via
Japanese TV, NHK, and some other media.

[NOTE: Images supporting this release are available at
http://www.***.com/ ]

---
Andrew Yee



Sun, 18 Feb 2001 03:00:00 GMT
 SUBARU Telescope 8.3m Primary Mirror Finished (Forwarded)

Quote:
>Subaru Telescope
>Physical Size ...
>     Diameter: 8.3m (27'), with a central hole 1.2 m (4') in diameter
>     Thickness: 20cm (8")
>     Weight: 22.8 metric tons
>     Effective Mirror Surface: 8.2m diameter
>     Focal Length: 15 m (49')

What is the central hole for?
--
Brenda Kalt



Wed, 21 Feb 2001 03:00:00 GMT
 SUBARU Telescope 8.3m Primary Mirror Finished (Forwarded)

Quote:


> >Subaru Telescope

> >Physical Size ...
> >     Diameter: 8.3m (27'), with a central hole 1.2 m (4') in diameter
> >     Thickness: 20cm (8")
> >     Weight: 22.8 metric tons
> >     Effective Mirror Surface: 8.2m diameter
> >     Focal Length: 15 m (49')

> What is the central hole for?

Take a look here: http://www.mania.com.au/~robo/astronom.html

It is to allow the light that is reflected off of the secondary
mirror to pass through the back of the 'scope.



Thu, 22 Feb 2001 03:00:00 GMT
 
 [ 3 post ] 

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