The Mid-Infrared Instrument for the James Webb Space Telescope, II: Design and Build

G. S. Wright, David Wright, G. B. Goodson, G. H. Rieke, Gabby Aitink-Kroes, J. Amiaux, Ana Aricha-Yanguas, Ruyman Azzollini, Kimberly Banks, N. C. Jessen, H. U. Nørgaard-Nielsen

    Research output: Contribution to journalJournal articleResearchpeer-review

    998 Downloads (Pure)


    The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28: 5 µm. MIRI has, within a single "package," four key scientific functions: photometric imaging, coronagraphy, single-source low-spectral resolving power (R similar to 100) spectroscopy, and medium-resolving power (R ∼ 1500 to 3500) integral field spectroscopy. An associated cooler system maintains MIRI at its operating temperature of <6.7 K. This paper describes the driving principles behind the design of MIRI, the primary design parameters, and their realization in terms of the "as-built" instrument. It also describes the test program that led to delivery of the tested and calibrated Flight Model to NASA in 2012, and the confirmation after delivery of the key interface requirements.
    Original languageEnglish
    JournalPublications of the Astronomical Society of the Pacific
    Issue number953
    Pages (from-to)595-611
    Publication statusPublished - 2015

    Bibliographical note

    For full list of authors, consult the publication


    • Space vehicles: instruments
    • instrumentation: photometers
    • instrumentation: spectrographs


    Dive into the research topics of 'The Mid-Infrared Instrument for the James Webb Space Telescope, II: Design and Build'. Together they form a unique fingerprint.

    Cite this