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Above
image shows the Rigid Conformal lap on a 8.4m Giant Magellan Telescope
off-axis segment.
Current
Projects
Hobby Eberly Telescope
Giant Magellan Telescope
Completed
Projects
Discovery Channel Telescope
The large optics shop polished the primary mirror for the Discovery Channel
Telescope (DCT) which is to be housed at Lowell Observatory. The F/1.9
mirror blank was approximately 4.3 meters.
Arizona Imaging Spectrometer (Starlight)
A 16" R-C telescope for a space shuttle experiment--This novel telescope's
optics and structure are made entirely of a metal matrix composite comprised
of aluminum and silicon carbide. This design provides an athermalized
telescope which is extremely rugged and achieves diffraction limited
performance over a 1 degree field.
Gravity Probe B Facetted Quartz Block
A two facetted quartz blocks for the Gravity Probe B spaceborne
experiment--These blocks have tenth wave requirements on surface figure and
one arcsecond perpendicularity tolerances between facets in two planes.
Far Infrared Space Telescope Technology Demonstrator Mold
A 2 meter diameter convex F/1 sphere for the FIRST program--This convex
sphere will be used as a mold for demonstrating replicating technology for
graphite-composite based optics.
James Webb Space Telescope Technology Demonstrator
An ultra-lightweight 2 meter diameter, 2 mm thick demonstrator mirror for
the JWSB program--The University of Arizona has developed a process to
fabricate thin shells which can be actively controlled for figure
correction. The shell will be attached to actuators which will be mounted on
a carbon fiber support structure.
DCATT Primary Mirror
A 1 meter diameter aluminum mirror for DCATT (Developmental Cryogenic Active
Telescope Testbed). The goal of the testbed is to represent in hardware an
optical system that incorporates all of the functional elements envisioned
in the NGST active optical system, and to investigate the viability and
efficiency of candidate wavefront sensing and wavefront control techniques
and algorithms. Arizona Daily Star story
Hughes 1.5 Meter Reference Sphere
A 1.5 meter reference sphere with a 10 meter radius of curvature. This
mirror will be used in a cryo chamber as part of a testbed for sensor
packages.
Greenbank Telescope Retroreflector
Designed and Fabricated a retroreflector design which achieves an acceptance
angle of 120━ compared to 24━ for a typical cornercube reflector. 18
retroreflectors will be positioned on the perimeter of the Greenbank
Telescope for measuring deflections induced by wind and gravity loading.
EUV Imager Mirrors
Nine F/0.5 primary mirrors to be used in a spaceborne EUV Imager. These
mirrors were figured to an accuracy of better than an eighth wave with a
surface roughness of better than three Angstroms rms.
SLOAN 2.5 Meter Primary
A hyperbolic F/2.2 2.5 meter primary mirror for the SLOAN digital sky
survey. This telescope will be used to perform a digital sky survey in
support of cosmology studies. The following article shows a detailed
description of the implemented telescope complete with optical prescription,
image analysis, and photographs: http://www.astro.princeton.edu/PBOOK/telescop/telescop.htm
Multiple Mirror Telescope Primary and Secondary Mirrors for the
Smithsonian Institute and Stewart Observatory
Fabricated seven 1.8 meter diameter primary mirrors and six secondary
mirrors. This telescope was based on new technology which utilized six
primary mirror segments to effectively act as one monolithic mirror.
Allegheny Observatory 30" Objective
Fabricated a 30" doublet objective which was achromatized for the red. This
telescope is used to search for planetary systems outside our solar system.
United States Naval Observatory Astrographic Lens System
Fabricated five lenses ranging in size from 8.5" to 10.5" which comprised
the Astrographic Lens System. This system is used to take distortion free
photographs of the sky in order to accurately track the movement of stars.
This is arguably the best lens of its kind in the world.
Developmental Ultra-lightweight Metal Foam Telescopes for the United
States Department of Defense
Fabricated several developmental telescopes which used metal foam primary
mirrors. The mirror sizes ranged from 8" to 16" in diameter.
Jet Propulsion Laboratory 1.5 Meter Off-Axis Parabola
Developed a new technology for fabricating large off-axis optics. Fabricated
a 1.5 meter optic for JPL and performed fabrication research on several
other optics involved in the SDI program.
Optical System for the Descent Imager/Spectral Radiometer
Fabricated the optics for a spaceborne optical system which is used for
geological studies. This work was performed by the following organizations:
Lunar and Planetary Laboratory, Jet Propulsion Laboratory, United States
Geological Survey, Dept de Recherche Spatiale (France), Max Planck Institut
fur Aeronomie (Germany), and Technesche Universitat Braunschweig (Germany).
NASA Fabrication Experiments
Developed and utilized fabrication methods to produce large antenna
reflector mold segments used for replicating optical surfaces. Fabricated
several convex off-axis paraboloid optics for the Solar Telescope Project.
Bok 2.3 Meter Telescope Primary mirror
Fabricated a 2.3 meter primary for a telescope located at Kitt Peak National
Observatory and operated by Steward Observatory.
2 Meter Aperture Collimator
Fabricated the optics for a three mirror collimator which produces a 2 meter
diameter beam for the United States Army Missle Command.
High Gravity Environment Infrared Source Collimators
Fabricated several two element collimator systems for the United States Air
Force which produced 6" diameter unobscured beams and can survive a 10G
load.
Test Optics for the 6.5 Meter MMT Conversion Primary Mirror
Fabricated the null lens optical elements used to test the MMT conversion
6.5 meter primary mirror.
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