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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 micrometers. 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 is less than lambda is less than 5.0 micrometers spectrum. An actively cooled mid-infrared instrument provides broad-band imagery, coronography, and integral-field spectroscopy over the 5.0 is less than lambda is less than 29 micrometers 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 proposed by the international astronomical community in a manner similar to the Hubble Space Telescope. Technology development and mission design are complete. The science instrument payload is in the final stage of testing ahead of delivery for integration with the telescope during early 2016. The JWST is on schedule for launch during 2018.
Document ID
20160013309
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
September 4, 2015
Publication Information
Publication: Proceedings of SPIE 9602:UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts VII
Publisher: SPIE
Volume: 9602
Subject Category
Instrumentation And Photography
Report/Patent Number
GSFC-E-DAA-TN33000
Distribution Limits
Public
Copyright
Other
Keywords
narrow-band imagery
integral-field spectroscopy
The James Webb Space Telescope (JWST)

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