Magdalena Ridge extends optical interferometer capacity

 

Magdalena Ridge Observatory (MRO) has purchased a second generation off-axis beam compressor from Optical Surfaces that will expand the capabilities of the facility’s optical interferometer.

An interferometer is an investigative tool that merges two or more sources of light to create an interference pattern that can be measured and analysed. In astronomy, interferometers combine the light collected by more than one telescope allowing them to act together as one bigger 'virtual telescope'. The waves of light from each telescope are combined to make them brighter. Interferometry makes it possible to see fainter objects in more detail.

The Magdalena Ridge Observatory Interferometer (MROI) project’s mission is to develop a ten-element imaging interferometer that will operate at wavelengths between 0.6 and 2.4 microns with baselines from 7.8 to 340 meters. The technical and scientific goals of the interferometer are to produce model-independent images of faint and complex astronomical targets at resolutions over 100 times that of the Hubble Space Telescope.

Dr Michelle Creech Eakman, Professor of Physics at MRO commented “To minimise diffraction effects from long distance propagation, the original 7.5x off-axis beam compressor supplied by Optical Surfaces was designed to allow a 95-mm beam of starlight to be reduced in size for the final division among instruments on the telescope. Because of the excellent performance of this optical system, we decided to single source from Optical Surfaces for three second-generation beam compressors that offer a better field-of-view to aid interferometric alignment.  These beam compressors will be crucial components in the MROI as they will allow us to work in the smaller beam space (less than 20mm diameter) outside the vacuum system.  We are hoping to attain first fringes during the first half of 2024”.

Dr Aris Kouris, Sales Director at Optical Surfaces added “Located at 10,600 ft above sea level in the Magdalena Mountains, our beam compressors for the MROI are subject to considerable variation in temperature. This means that we needed to incorporate invar element tie bars into the beam compressor design to provide thermal stabilisation. Our 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”.

 

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