Canada will build a key component of the gigantic James Webb Space Telescope (JWST) to be launched by NASA in August 2011. The Canadian Space Agency (CSA) recently awarded a $5-million contract to Ottawa-based EMS Technologies' Space and Technology Group for the design of the fine guidance sensor, in partnership with COM DEV of Cambridge, Ontario. Northrup Grumman Space Technologies of Los Angeles, California, will build the JWST under NASA supervision at an estimated cost of US$1.5 billion.
About James Webb Space Telescope:
This major facility-class space observatory will be launched in 2011 and is a successor to the very successful 2.5-m Hubble Space Telescope. While Hubble makes observations mainly in the visible and ultraviolet wavebands, the James Webb Space Telescope (JWST) mission concept is for a large filled-aperture telescope (primary mirror diameter of approximately 6.5 m) located far from Earth at the L2 Lagrangian point, about 1.5 million kilometres from the Earth.
Shielded from the Sun and Earth by a large deployable sun-shade, the entire telescope assembly will be passively cooled to about 35K (35 degrees above absolute zero), giving Shielded from the Sun and Earth by a large deployable sun-shade, the entire telescope assembly will be passively cooled to about 35K (35 degrees above absolute zero), giving James Webb Space Telescope exceptional performance in the near-infrared and mid-infrared wavebands. The baseline wavelength range for the instrumentation is 0.6 to 28 microns, and the telescope will be diffraction-limited above 2 microns. The sensitivity of the telescope will be limited only by the natural zodiacal background, and should exceed that of ground-based and other space-based observatories by factors of 10 to 100,000, depending on the wavelength and type of observation. The JWST observatory will have a 5- to 10-year lifetime and will not be serviceable by astronauts (as is Hubble).
Like Hubble, the JWST will be used by a broad astronomical community to observe targets ranging from objects within our Solar System to the most remote galaxies seen during their formation in the early universe.
"This major new observatory will take over where Hubble, Spitzer, and other space telescopes leave off," said Dr. Virendra Jha, CSA Vice-President of Science, Technologies and Programs. "It is being designed by teams in Canada, the U.S., and Europe. JWST will open new windows on the first stars and quasars in the early universe, as well as star and planet formation in nearby galaxies. JWST is uniquely designed for these investigations."
"Our instrument, the fine guidance sensor, is critical to the success of the mission. It will measure the positions of very faint stars to extremely high accuracy. This is necessary for JWST to achieve the high quality of images required by the scientific objectives," added Mr. Alan Haase, Senior Vice-President and General Manager of EMS Technologies' Space and Technology Group. "We are also including a tunable filter camera that will provide unique scientific capabilities."
NRC's Herzberg Institute of Astrophysics (HIA) has played a key role in this scientific mission, working with CSA and its contractors to establish the Canadian contribution and helping with early design work. The Canadian project scientist, Dr. John Hutchings of HIA, also leads a team of scientists from across the country in planning the instrument function, calibrations and early science investigations. Canada has guaranteed science time on JWST as a partner in the project. Canadian scientists are also members of the U.S. and European teams producing two of the other instruments.
"When launched in 2011, JWST will peer into the past to greater distances than ever before," says Dr. Hutchings. "With it, we will be able to observe the formation of the first stars and galaxies in the universe, close to the beginning of time."
With an aperture diameter of 6.5 m, the surface area of JWST's main mirror will be seven times larger than Hubble's, and hundreds of times more sensitive than any other telescope. Its five-layer sunshield-almost as large as a tennis court-will keep the instruments at 37 degrees above absolute zero and will allow the telescope to detect faint, red-shifted signals from the early stages of the universe. The JWST will be stationed 1.5 million km from Earth at the Second Lagrangian Point (L2). This location lies beyond the Earth's orbit, thus the bright Earth is never seen by JWST; this reduces problems with stray light.
Source: Canadian Space Agency
Explore further: Computer model shows moon's core surrounded by liquid and it's caused by Earth's gravity