Multiband Imaging Photometer for Spitzer

E238783

The Multiband Imaging Photometer for Spitzer (MIPS) is an instrument on the Spitzer Space Telescope designed to capture high-sensitivity images and photometric measurements in the mid- to far-infrared wavelengths, enabling detailed studies of cold dust, star formation, and distant galaxies.

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Multiband Imaging Photometer for Spitzer canonical 1

Statements (47)

Predicate Object
instanceOf Spitzer Space Telescope instrument
astronomical instrument
infrared photometer
space telescope instrument
abbreviation MIPS
coolingRequirement cryogenic operation
dataProduct infrared images
infrared photometric catalogs
designedFor high-sensitivity imaging
mid- to far-infrared observations
photometric measurements
enables detection of faint infrared sources
mapping of cold dust in galaxies
measurement of infrared spectral energy distributions
hasCapability imaging
mapping of extended emission
photometry
hostMission Spitzer Space Telescope
surface form: NASA Spitzer Space Telescope mission
locatedIn Spitzer Space Telescope cryogenic instrument chamber
observatory Spitzer Space Telescope
observes galaxies
molecular clouds
planetary debris disks
star-forming regions
thermal emission from dust
observingEnvironment space-based
operatedOn Spitzer Space Telescope
partOf Spitzer Space Telescope science payload
scientificPurpose study of circumstellar dust
study of cold dust
study of debris disks
study of distant galaxies
study of interstellar medium
study of star formation
spaceAgency NASA
spectralBand 160 micrometre band
24 micrometre band
70 micrometre band
telescope Spitzer Space Telescope
usedIn cosmology-related surveys
extragalactic astronomy
galactic astronomy
star formation studies
usesDetectorType Ge:Ga detector
Si:As detector
wavelengthRange far-infrared
mid-infrared

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Spitzer Space Telescope scienceInstruments Multiband Imaging Photometer for Spitzer