James Webb Space Telescope
The James Webb Space Telescope (JWST) will have an 18-segment primary mirror 6.6 meters (22 feet) in diameter – over 2.5 times as large as the 2.4-m mirror of the Hubble Space Telescope. Each of the hexagonal mirror segments measures 1.3 m (4.3 ft.) in diameter and weighs just 20 kg (46 lb.). They are made of the lightweight metal beryllium. Although the completed primary mirror will be much larger than that of Hubble, it will weigh roughly half as much. JWST will be stationed much further from the Earth so that its equipment can remain cold and free from terrestrial infrared 'noise'. Three principal instruments will gather images of the Universe in the infrared region of the spectrum.
JWST is expected to provide a vast amount of new information on the structure of circumstellar disks around young stars, including high-resolution images showing details, such as gaps, which may indicate the presence of newly-formed planets. It will also be capable of detecting the presence of extrasolar planets directly due to their infrared emission. This is because planets are brighter relative to their central stars in the infrared part of the spectrum than they are at visible wavelengths. For example, Jupiter is 100 million times fainter than the Sun in the optical region, but only 10,000 times fainter in the infrared. JWST will also study the earliest galaxies and some of the first stars formed after the Big Bang. These early objects have a high redshift from our vantage-point, meaning that the best observations of them are available in the infrared.
JWST is scheduled for launch by an Ariane V rocket in 2014. It will operate from a Lissajous orbit about the L2 Earth-Sun Lagrangian point, some 1.5 million km from Earth.
Related entries infrared astronomy
infrared astronomy satellites
Related category SATELLITES AND SPACE PROBES
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