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The JWST Science Instrument Payload: Mission Context and StatusThe James Webb Space Telescope (JWST) is the scientific successor to the Hubble Space Telescope. It is a cryogenic infrared space observatory with a 25 sq m aperture (6 m class) telescope that will achieve diffraction limited angular resolution at a wavelength of 2 microns. The science instrument payload includes four passively cooled near-infrared instruments providing broad- and narrow-band imagery, coronography, as well as multi-object and integral-field spectroscopy over the 0.6 < lambda < 5.0 microns spectrum. An actively cooled mid-infrared instrument provides broad-band imagery, coronography, and integral-field spectroscopy over the 5.0 < lambda < 29 microns spectrum. The JWST is being developed by NASA, in partnership with the European and Canadian Space Agencies, as a general user facility with science observations to be proposed by the international astronomical community in a manner similar to the Hubble Space Telescope. Technology development and mission design are complete. Construction, integration and verification testing is underway in all areas of the program. The JWST is on schedule for launch during 2018.
Document ID
20160013314
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Greenhouse, Matthew A.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
November 8, 2016
Publication Date
August 2, 2014
Publication Information
Publication: Proceedings of SPIE
Publisher: SPIE
Volume: 9143
Subject Category
Astronomy
Report/Patent Number
GSFC-E-DAA-TN32998
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Keywords
cryogenic infrared space observatory
broad-band imagery
The James Webb Space Telescope (JWST)

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