NIRCam
Sign in to saveAlso known as Near-InfraRed Camera
thumb|NIRCam wrapped up in 2013 thumb|NIRCam being installed in 2014
Wikidata facts
- Image
- JWST Nircam1lwres.jpg
Show 5 more facts
- short name
- NIRCam
- Commons category
- Near-Infrared Camera (NIRCam)
- minimum wavelength of sensitivity
- 0.6
- maximum wavelength of sensitivity
- 5
- native label
- Near-InfraRed Camera
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10 sectionsContents
- Main
- Components
- Overview
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- Electronics
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- Labeled diagram
- See also
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- External links
thumb|NIRCam wrapped up in 2013 thumb|NIRCam being installed in 2014
NIRCam (Near-InfraRed Camera) is an instrument aboard the James Webb Space Telescope. It has two major tasks, as an imager from 0.6 to 5 μm wavelength, and as a wavefront sensor to keep the 18-section mirrors functioning as one. In other words, it is a camera and is also used to provide information to align the 18 segments of the primary mirror. It is an infrared camera with ten mercury-cadmium-telluride (HgCdTe) detector arrays, and each array has an array of 2048×2048 pixels. The camera has a field of view of 2.2×2.2 arcminutes with an angular resolution of 0.07 arcseconds at 2 μm. NIRCam is also equipped with coronagraphs, which helps to collect data on exoplanets near stars. It helps with imaging anything next to a much brighter object, because the coronagraph blocks that light.