Optical Surfaces to Produce Beam Compressor for MRO
Optical component manufacturer Optical Surfaces Ltd. has been selected by the Magdalena Ridge Observatory (MRO) to produce an ultrastable 7.5× off-axis beam compressor that will form a key beam transfer element in the facility’s optical interferometer.
When completed, the Magdalena Ridge Observatory Interferometer (MROI) will be a powerful optical-IR interferometer dedicated to high-resolution imaging of all types of astronomical objects. The MORI will help enable observation of many types of nearby stars, including direct observations of the radial pulsations of Cepheid variable stars, surface features on giant stars, and bright, active galactic nuclei. In its initial phase, the MROI will consist of three 1.4-m diameter telescopes.
“We are delighted to have been selected for this prestigious international astronomical project,” said Aris Kouris, sales director at Optical Surfaces. “Optical Surfaces beam compressors incorporate high-precision off-axis mirrors, which provide an unobstructed output and highly efficient transmission. Beam compressors are the optical tool of choice for decreasing the diameter of a collimated input beam to a smaller collimated output beam. The reflective design of our beam reducers is achromatic and with protected silver coatings can operate from the visible spectrum to far IR without adjustment. However, located at an elevation of 10,600 ft above sea level in the Magdalena Mountains, the MROI beam compressor will be subject to considerable variation in temperature. As a consequence, the design for our 7.5× beam compressor will incorporate invar element tie bars to provide thermal stabilization.”
The telescopes will be movable between sets of discrete foundations, allowing baselines between 7.5 and 347 m in length. The MROI is projected to be able to produce an angular resolution of 0.6 milli-arcsec at a 1-μm wavelength.
“To minimize diffraction effects from long-distance propagation, starlight is collimated into a 95-mm diameter beam at the telescope for propagation through most of the relay system,” said Robert Ligon, instrument scientist at MRO. “The beam compressor to be produced by Optical Surfaces is a key component of the system, allowing the 95-mm beam of starlight to be reduced in size for the final division among instruments. After installation of the first telescope and enclosure at the beginning of the summer, the arrival of the beam compressor will allow us to complete our first beam line and begin testing the interferometer beam train before the arrival of our second telescope.”
Optical Surfaces is a producer of optical components, reference flats, and beam expanders.
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