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Aluminum based large telescopes: the ARIEL Mission case

  • P. Picchi*
  • , A. Tozzi
  • , A. Brucalassi
  • , Antonio J. Araiza
  • , E. Pace
  • , P. Chioetto
  • , P. Zuppella
  • , A. Scippa
  • , R. Lilli
  • , D. Gottini
  • , Javier P. Alvarez
  • , A. García
  • , Alejandro F. Soler
  • , F. D’Anca
  • , E. Guerriero
  • , C. Del Vecchio
  • , G. Falcini
  • , L. Carbonaro
  • , P. Eccleston
  • , A. Caldwell
  • D. Ferruzzi, G. Malaguti, G. Micela, E. Pascale, A. Bocchieri, G. Preti, R. Piazzolla, M. Salatti, D. Brienza, E. Tommasi, G. Tinetti, D. Vernani, G. Morgante
*Corresponding author for this work
  • University of Florence
  • Osservatorio Astrofisico Di Arcetri
  • University of Padua
  • INAF-Osservatorio Astronomico di Padova
  • CNR National Research Council Italy
  • Ciudad Universitaria
  • Osservatorio Astrofisico di Torino
  • RAL Space
  • INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
  • School of Medicine
  • Italian Space Agency
  • Department of Physics and Astronomy
  • UCL University College London
  • Media Lario S.r.l.
  • INAF-Osservatorio Astronomico di Bologna

Research output: Chapter in Book/Report/Conference proceedingConference paperpeer-review

1 Citation (Scopus)

Abstract

Ariel (Atmospheric Remote-Sensing Infrared Exoplanet Large Survey) is the adopted M4 mission of ESA “Cosmic Vision” program. Its purpose is to conduct a survey of the atmospheres of known exoplanets through transit spectroscopy. Launch is scheduled for 2029. Ariel scientific payload consists of an off-axis, unobscured Cassegrain telescope feeding a set of photometers and spectrometers in the waveband between 0.5 and 7.8 µm, and operating at cryogenic temperatures. The Ariel Telescope consists of a primary parabolic mirror with an elliptical aperture of 1.1 m of major axis, followed by a hyperbolic secondary, a parabolic recollimating tertiary and a flat folding mirror. The Primary mirror is a very innovative device made of lightened aluminum. Aluminum mirrors for cryogenic instruments and for space application are already in use, but never before now it has been attempted the creation of such a large mirror made entirely of aluminum: this means that the production process must be completely revised and fine-tuned, finding new solutions, studying the thermal processes and paying a great care to the quality check. By the way, the advantages are many: thermal stabilization is simpler than with mirrors made of other materials based on glass or composite materials, the cost of the material is negligeable, the shape may be free and the possibility of making all parts of the telescope, from optical surfaces to the structural parts, of the same material guarantees a perfect alignment at whichever temperature. The results and expectations for the flight model are discussed in this paper.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2024
Subtitle of host publicationOptical, Infrared, and Millimeter Wave
EditorsLaura E. Coyle, Shuji Matsuura, Marshall D. Perrin
PublisherSPIE
ISBN (Electronic)9781510675070
DOIs
Publication statusPublished - 2024
EventSpace Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave - Yokohama, Japan
Duration: 16 Jun 202422 Jun 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13092
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSpace Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave
Country/TerritoryJapan
CityYokohama
Period16/06/202422/06/2024

Keywords

  • ARIEL mission
  • cryogenic optics
  • IR Space telescopes
  • metal mirrors
  • NiP treatment

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