27 November 2017 The afocal telescope optical design and tolerance analysis for the ESA ARIEL mission
Author Affiliations +
Proceedings Volume 10590, International Optical Design Conference 2017; 105901P (2017) https://doi.org/10.1117/12.2292299
Event: International Optical Design Conference - IODC 2017, 2017, Denver, United States
Abstract
ARIEL (Atmospheric Remote-sensing Infrared Exoplanet Large-survey) is one of the three present candidates for the next ESA medium-class science mission (M4) to be launched in 2026. During its 3.5 years of scientific operations from L2 orbit, this mission will observe spectroscopically in the infrared (IR) a large population of known transiting planets in the neighbourhood of the Solar System. The aim is to enable a deep understanding of the physics and chemistry of these exoplanets. ARIEL is based on a 1-m class telescope ahead of a suite of instruments: two spectrometer channels covering the band 1.95 to 7.80 µm and four photometric channels (two wide and two narrow band) in the range 0.5 to 1.9 μm. The ARIEL optical design is conceived as a fore-module common afocal telescope that will feed the spectrometer and photometric channels. The telescope optical design is based on an eccentric pupil two-mirror classic Cassegrain configuration coupled to a tertiary paraboloidal mirror. An all-aluminum structure has been considered for the telescope layout, and a detailed tolerance analysis has been conducted to assess the telescope feasibility. This analysis has been done including the different parts of the realization and life of the instrument, from integration on-ground to in-flight stability during the scientific acquisitions. The primary mirror (M1) temperature will be monitored and finely tuned via an active thermal control system based on thermistors and heaters. The heaters will be switched on and off to maintain the M1 temperature within ±1K thanks to a proportional–integral–derivative (PID) controller.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Vania Da Deppo, Vania Da Deppo, Kevin Middleton, Kevin Middleton, Mauro Focardi, Mauro Focardi, Gianluca Morgante, Gianluca Morgante, Samuele Grella, Samuele Grella, Riccardo Claudi, Riccardo Claudi, Emanuele Pace, Emanuele Pace, Iacopo Ficai Veltroni, Iacopo Ficai Veltroni, Giuseppina Micela, Giuseppina Micela, } "The afocal telescope optical design and tolerance analysis for the ESA ARIEL mission", Proc. SPIE 10590, International Optical Design Conference 2017, 105901P (27 November 2017); doi: 10.1117/12.2292299; https://doi.org/10.1117/12.2292299
PROCEEDINGS
12 PAGES


SHARE
RELATED CONTENT

Ring field TMA for PRISMA theory, optical design, and...
Proceedings of SPIE (September 22 2015)
The afocal telescope of the ESA ARIEL mission analysis...
Proceedings of SPIE (September 04 2017)
Design of off-axis three-mirror system with Zernike surface
Proceedings of SPIE (December 30 2010)
Some Design Aspects Of A Multiple-Mirror Telescope
Proceedings of SPIE (August 31 1972)
Giant Magellan Telescope (GMT)
Proceedings of SPIE (July 06 2004)

Back to Top