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Proceedings Paper

A segmented subreflector with electroformed nickel laminated panels for the Large Millimeter Telescope
Author(s): G. Valsecchi; R. Banham; G. Bianucci; J. Eder; R. Ghislanzoni; A. Ritucci; M. Terraneo; F. E. Zocchi; D. Smith; D. Gale; D. Hughes
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Paper Abstract

The Large Millimeter Telescope (LMT) Alfonso Serrano is a 50 m diameter single-dish radio telescope optimized for astronomical observations at wavelengths of about a millimeter. Built and operated by the Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE) in collaboration with the University of Massachusetts (UMASS), the telescope is located at the 4600 m summit of volcano Sierra Negra, Mexico. Anticipating the completion of the main reflector, currently operating over a 32 m subaperture, INAOE has contracted Media Lario for the design and manufacturing of a new 2.63 m subreflector that will enable higher efficiency astronomical observations with the entire main reflector surface. The new subreflector manufactured by Media Lario is segmented in 9 smaller panels, one central dome and eight identical petals, assembled and precisely aligned on a steel truss structure that will be connected to the hexapod mounted on the tetrapod head. Each panel was fabricated with Media Lario’s unique laminated technology consisting of front and rear Nickel skins, electroformed from precise molds and bonded to a lightweight Aluminum honeycomb core. The reflecting surface of each panel was given a thin galvanic Rhodium coating that ensures that the reflector survives the harsh environmental conditions at the summit of Sierra Negra during the 30 year lifetime of the telescope. Finally, the 2.63 m subreflector produced by Media Lario was qualified for typical cold night through hot day observation conditions with a maximum RMS error of 24.8 μm, which meets INAOE’s requirements.

Paper Details

Date Published: 22 July 2016
PDF: 11 pages
Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99123P (22 July 2016); doi: 10.1117/12.2232390
Show Author Affiliations
G. Valsecchi, Media Lario Technologies S.r.l. (Italy)
R. Banham, Media Lario Technologies S.r.l. (Italy)
G. Bianucci, Media Lario Technologies S.r.l. (Italy)
J. Eder, Media Lario Technologies S.r.l. (Italy)
R. Ghislanzoni, Media Lario Technologies S.r.l. (Italy)
A. Ritucci, Media Lario Technologies S.r.l. (Italy)
M. Terraneo, Media Lario Technologies S.r.l. (Italy)
F. E. Zocchi, Media Lario Technologies S.r.l. (Italy)
D. Smith, MERLAB, P.C. (United States)
D. Gale, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)
D. Hughes, Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico)


Published in SPIE Proceedings Vol. 9912:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II
Ramón Navarro; James H. Burge, Editor(s)

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