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James Webb Space Telescope

James Webb Space Telescope
James Webb Space Telescope model
Full scale James Webb Space Telescope model at South by Southwest in Austin
Names Next Generation Space Telescope
James Webb Space Telescope
Mission type Astronomy
Operator NASA / ESA / CSA / STScI
Website jwst.nasa.gov
sci.esa.int/jwst
asc-csa.gc.ca
stsci.edu/jwst
Mission duration 5 years (design)
10 years (goal)
Spacecraft properties
Manufacturer Northrop Grumman
Ball Aerospace
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)
Transponders
Band S-band (TT&C support)
Ka band (data acquisition)
Bandwidth S-band up: 16 kbit/s
S-band down: 40 kbit/s
Ka band down: up to 28 Mbit/s
JWST logo
James Webb Space Telescope insignia

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.


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