The Athena x-ray optics development and accommodation

  • Marcos Bavdaz
  • , Eric Wille
  • , Mark Ayre
  • , Ivo Ferreira
  • , Brian Shortt
  • , Sebastiaan Fransen
  • , Mark Millinger
  • , Maximilien J. Collon
  • , Giuseppe Vacanti
  • , Nicolas M. Barrière
  • , Boris Landgraf
  • , Mark Olde Riekerink
  • , Jeroen Haneveld
  • , Ronald Start
  • , Coen van Baren
  • , Desiree Della Monica Ferreira
  • , Sonny Massahi
  • , Sara Svendsen
  • , Finn Christensen
  • , Michael Krumrey
  • Evelyn Handick, Vadim Burwitz, Miranda Bradshaw, Giovanni Pareschi, Giuseppe Valsecchi, Dervis Vernani, Geeta Kailla, William Mundon, Gavin Phillips, Jakob Schneider, Tapio Korhonen, Alejandro Sanchez, Dominique Heinis, Massimiliano Tordi, Richard Willingale

    Research output: Chapter in Book/Report/Conference proceedingArticle in proceedingsResearchpeer-review

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    Abstract

    The ATHENA mission, under study and preparation by ESA as its second Large-class science mission, requires the largest X-ray optics ever flown, building on a novel optics technology based on mono crystalline silicon. Referred to as Silicon Pore Optics technology (SPO), the optics is highly modular and benefits from technology spin-in from the semiconductor industry. The telescope aperture of about 2.5 meters is populated by 600 mirror modules, accurately co -aligned to produce a common focus. The development of the SPO technology is a joint effort by European industrial and research entities, working together to address the challenges to demonstrate the imaging performance, robustness and efficient series production of the ATHENA optics. A technology development plan was established and is being regularly updated to reflect the latest developments, and is fully funded by the ESA technology development programmes. An industrial consortium was formed to ensure coherence of the individual technology development activities. The SPO technology uses precision machined mirror plates produced using thelatest generation top quality 12 inch silicon wafers, which are assembled into rugged stacks. The surfaces of the mirror plates and the integral support structure is such, that no glue is required to join the individual mirror plates. Once accurately aligned with respect to each other, the surfaces of the mirror plates merge in a physical bonding process. The resultant SPO mirror modules are therefore very accurate and stable and can sustain the harsh conditions encountered during launch and are able to tolerate the space environment expected during operations. The accommodation of the ATHENA telescope is also innovative, relying on a hexapod mechanismto align the optics to the selected detector instruments located in the focal plane. Systemstudies are complemented by dedicated technology development activities to demonstrate the capabilities before the adoption of the ATHENA mission.

    Original languageEnglish
    Title of host publicationProceedings of SPIE : International Conference on Space Optics — ICSO 2020
    EditorsStephen L. O'Dell, Jessica A. Gaskin, Giovanni Pareschi
    Number of pages15
    PublisherSPIE - International Society for Optical Engineering
    Publication date2021
    Article number1185220
    DOIs
    Publication statusPublished - 2021
    Event2020 International Conference on Space Optics - Virtual conference, Virtual, Online
    Duration: 30 Mar 20212 Apr 2021

    Conference

    Conference2020 International Conference on Space Optics
    LocationVirtual conference
    CityVirtual, Online
    Period30/03/202102/04/2021
    SeriesProceedings of SPIE - The International Society for Optical Engineering
    ISSN0277-786X

    Keywords

    • ATHENA
    • Silicon Pore Optics
    • Technology preparation
    • X-ray astronomy
    • X-ray optics
    • X-ray telescopes
    • X-ray testing

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