Mid-Infrared Instrument (MIRI)

GPTKB entity

Statements (54)
Predicate Object
gptkbp:instance_of gptkb:scientific_instruments
gptkbp:average_temperature around 7 K
gptkbp:characteristic reflective telescope
gptkbp:collaborator gptkb:Canadian_Space_Agency
gptkb:University_of_Edinburgh
gptkb:University_of_Arizona
gptkb:Space_Telescope_Science_Institute
gptkb:NASA
gptkbp:data_type FITS
gptkbp:designed_by gptkb:NASA
gptkbp:designed_for gptkb:James_Webb_Space_Telescope
gptkbp:developed_by gptkb:NASA_and_ESA
gptkb:European_Space_Agency
gptkbp:frequency 5 to 28 micrometers
https://www.w3.org/2000/01/rdf-schema#label Mid-Infrared Instrument (MIRI)
gptkbp:impact contributes to the study of dark matter and dark energy
advances knowledge of star formation
aids in the search for organic molecules
contributes to cosmology research
enables studies of interstellar dust
enhances understanding of exoplanets
enhances understanding of the chemical universe
facilitates observations of solar system bodies
provides data for future astronomical missions
provides insights into galactic evolution
supports studies of the early universe
supports the search for life beyond Earth
gptkbp:includes a coronagraph
two cameras
a filter wheel
a spectrometer wheel
four spectrometers
gptkbp:launch_date December 25, 2021
gptkbp:lighting July 2022
gptkbp:operates_in mid-infrared spectrum
gptkbp:operational_status operational
gptkbp:powers approximately 200 watts
gptkbp:provides spectroscopy capabilities
imaging capabilities
gptkbp:resolution 0.1 arcseconds
gptkbp:scientific_goals observe distant galaxies
study formation of stars
study formation of planetary systems
analyze the chemical composition of celestial objects
gptkbp:sensitivity detect faint objects
5 to 28 microns
gptkbp:used_for imaging and spectroscopy in the mid-infrared spectrum
gptkbp:uses cryogenic cooling
detectors based on Hg Cd Te
microshutter arrays
gptkbp:view 10 arcminutes
gptkbp:weight approximately 300 kg
gptkbp:bfsParent gptkb:James_Webb_Space_Telescope
gptkbp:bfsLayer 4