MIRI

E59345

MIRI is the Mid-Infrared Instrument on the James Webb Space Telescope, designed to capture detailed images and spectra of celestial objects in the mid-infrared range.

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Statements (47)

Predicate Object
instanceOf astronomical instrument
space telescope instrument
acronymFor Mid-Infrared Instrument
collaboration European Space Agency
surface form: ESA

European MIRI Consortium
NASA
coolingRequirement cryogenic
distinction only JWST instrument operating exclusively in the mid-infrared
enables high-contrast coronagraphic observations
high-sensitivity mid-infrared imaging
mid-infrared spectroscopy
fullName Mid-Infrared Instrument
function coronagraphy
imaging
spectroscopy
hasMode coronagraphic mode
imaging mode
low-resolution spectrometer mode
medium-resolution spectrometer mode
hostSpaceAgency European Space Agency
surface form: ESA

NASA
launchDate 2021-12-25 (via JWST)
launchVehicle Ariane 5 ECA
surface form: Ariane 5 (via JWST)
location JWST instrument module at Sun–Earth L2
observatory James Webb Space Telescope
surface form: JWST
observes exoplanets
galaxies
interstellar medium
protoplanetary disks
solar system objects
stars
operatingTemperature around 7 kelvin
partOf James Webb Space Telescope
requires dedicated cryocooler
scienceGoals characterize exoplanet atmospheres
observe protoplanetary and debris disks
study formation of stars and planetary systems
study high-redshift galaxies
study interstellar dust and gas
scientificRole capture detailed images of celestial objects in the mid-infrared
obtain spectra of celestial objects in the mid-infrared
spacecraft James Webb Space Telescope
surface form: JWST observatory
spectralCoverageEnd about 28 micrometers
spectralCoverageStart about 5 micrometers
telescope James Webb Space Telescope
usesDetectorType mid-infrared detector arrays
wavelengthRange mid-infrared

Referenced by (5)

Full triples — surface form annotated when it differs from this entity's canonical label.