Full scale James Webb Space Telescope model at South by Southwest in Austin
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Names | Next Generation Space Telescope James Webb Space Telescope |
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Mission type | Astronomy | ||||||||||||
Operator | NASA / ESA / CSA / STScI | ||||||||||||
Website |
jwst sci asc-csa stsci |
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Mission duration | 5 years (design) 10 years (goal) |
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Spacecraft properties | |||||||||||||
Manufacturer |
Northrop Grumman Ball Aerospace |
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Launch mass | 6,500 kg (14,300 lb) | ||||||||||||
Dimensions | 20.197 m × 14.162 m (66.26 ft × 46.46 ft) (sunshield) | ||||||||||||
Power | 2,000 watts | ||||||||||||
Start of mission | |||||||||||||
Launch date | October 2018 | ||||||||||||
Rocket | Ariane 5 ECA | ||||||||||||
Launch site | Kourou ELA-3 | ||||||||||||
Contractor | Arianespace | ||||||||||||
Orbital parameters | |||||||||||||
Reference system | Sun–Earth L2 | ||||||||||||
Regime | Halo orbit | ||||||||||||
Periapsis | 374,000 km (232,000 mi) | ||||||||||||
Apoapsis | 1,500,000 km (930,000 mi) | ||||||||||||
Period | 6 months | ||||||||||||
Epoch | planned | ||||||||||||
Main | |||||||||||||
Type | Korsch telescope | ||||||||||||
Diameter | 6.5 m (21 ft) | ||||||||||||
Focal length | 131.4 m (431 ft) | ||||||||||||
Collecting area | 25 m2 (270 sq ft) | ||||||||||||
Wavelengths | from 0.6 µm (orange) to 28.5 µm (mid-infrared) |
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Transponders | |||||||||||||
Band |
S-band (TT&C support) Ka band (data acquisition) |
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Bandwidth | S-band up: 16 kbit/s S-band down: 40 kbit/s Ka band down: up to 28 Mbit/s |
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James Webb Space Telescope insignia |
Instruments | |
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NIRCam | Near IR Camera |
NIRSpec | Near-Infrared Spectrograph |
MIRI | Mid IR Instrument |
NIRISS | Near Infrared Imager and Slitless Spectrograph |
FGS |
Fine Guidance Sensor
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Fine Guidance Sensor
Elements:
The James Webb Space Telescope (JWST), previously known as Next Generation Space Telescope (NGST), is a part of NASA's ongoing Flagship program. It is under construction and scheduled to launch in October 2018. The JWST will offer unprecedented resolution and sensitivity from long-wavelength (orange-red) visible light, through near-infrared to the mid-infrared (0.6 to 27 micrometers). While Hubble has a 2.4-meter (7.9 ft) mirror, the JWST features a larger and segmented 6.5-meter-diameter (21 ft 4 in) primary mirror and will be located near the Earth–Sun L2 point. A large sunshield will keep its mirror and four science instruments below 50 K (−220 °C; −370 °F).
JWST's capabilities will enable a broad range of investigations across the fields of astronomy and cosmology. One particular goal involves observing some of the most distant events and objects in the Universe, such as the formation of the first galaxies. These types of targets are beyond the reach of current ground and space-based instruments. Another goal is understanding the formation of stars and planets. This will include direct imaging of exoplanets.
In gestation since 1996, the project represents an international collaboration of about 17 countries led by NASA, and with significant contributions from the European Space Agency and the Canadian Space Agency. It is named after James E. Webb, the second administrator of NASA, who played an integral role in the Apollo program.