Spiral Galaxy IC 5332: Complex Structures Revealed | James Webb Space Telescope
MIRI is the only Webb instrument that is sensitive to the mid-infrared region of the electromagnetic spectrum (specifically in the 5 µm – 28 µm wavelength range); Webb’s other instruments all operate in the near-infrared. One of MIRI’s most remarkable features is that it operates 33 °C below the rest of the observatory at the frosty temperature of –266 °C. That means that MIRI operates in an environment only 7 °C warmer than absolute zero, which is the lowest possible temperature according to the laws of thermodynamics. MIRI requires this frigid environment in order for its highly specialized detectors to function correctly, and it has a dedicated active cooling system to ensure that its detectors are kept at the correct temperature.
It is worth noting just how challenging it is to obtain observations in the mid-infrared region of the electromagnetic spectrum. The mid-infrared is incredibly difficult to observe from Earth as much of it is absorbed by Earth’s atmosphere, and heat from Earth’s atmosphere further complicates things. Hubble could not observe the mid-infrared region as its mirrors were not cool enough, meaning that infrared radiation from the mirrors themselves would have dominated any attempted observations. The extra effort made to ensure that MIRI’s detectors had the freezing environment necessary to operate properly is evident in this stunning image.
MIRI was contributed by European Space Agency and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.
Credit: European Space Agency (ESA)/Webb, NASA & CSA, J. Lee and the PHANGS-JWST Team
Duration: 30 seconds
Release Date: September 27, 2022
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