IRAS
Encyclopedia : I : IR : IRA : IRAS
The Infrared Astronomical Satellite (IRAS) was a space-based observatory that performed a survey of the entire sky at infrared wavelengths.
| |
| Organization | NASA, NIVR, SERC |
|---|---|
| Wavelength regime | infrared |
| Orbit | ("sun-synchronous") |
| Launch date | 25 Jan 1983 |
| Deorbit date | 21 Nov 1983 |
| Coolant | 720 L (77 kg) of superfluid He |
| Mass | (fill in) |
| Other names | none |
| Webpage | http://lambda.gsfc.nasa.gov/product/iras |
| Physical Characteristics | |
| Telescope Style | () |
| Diameter | 0.57 m |
| Collecting Area | ~1 m2 |
| Focal Length | 5.5 m, f/9.6 |
| Instruments | |
| (main survey instrument) | array of 65 detectors |
| Low Resolution Spectrometer (LRS) | 8–22 µm slitless spectrometer |
| Chopped Photometric Channel (CPC) | low-quality mapping |
Launched in January 25, 1983, its mission lasted ten months. It was a joint project of the United States (NASA), the Netherlands (NIVR), and the United Kingdom (SERC).
IRAS mapped 96% of the sky four times, at 12, 25, 60 and 100 micrometre wavelengths, with resolutions ranging from 0.5' at 12 micrometers to 2' at 100 micrometers. It discovered about 500,000 sources, many of which are still awaiting identification. About 75,000 of those are believed to be starburst galaxies, still enduring their star-formation stage. Many other sources are normal stars with disks of dust around them, possibly the early stage of a planetary system formation. New discoveries included a dust disk around Vega and the first images of the Milky Way Galaxy's core.
IRAS's life, like most of infrared satellites, was limited by its cooling system: to effectively work in the infrared domain, a satellite must be cooled to impressively low temperatures. In IRAS' case, 720 liters of superfluid helium kept the satellite at a temperature of 1.6 kelvins (about −272 °C). The fluid keeps the satellite cool by evaporation. When the fluid totally evaporated, the satellite temperature rose preventing further observations.
Today (2004), the Spitzer Space Telescope is the best infrared telescope, allowing astronomers to follow up many detections first made by IRAS.
See also: telescope, space telescope.
IRAS was designed to catalogue fixed sources so it scanned the same region of sky several times. John Davies and Simon Green (then at University of Leicester) searched the rejected sources for moving objects. This led to the discovery of three asteroids, including notably 3200 Phaethon (an Apollo asteroid and the parent body of the Geminid meteor shower), six comets and a huge dust trail associated with comet Tempel-2. . The comets included the periodic comets 126P/IRAS and 161P/Hartley-IRAS and comet IRAS-Araki-Alcock, which made a close approach to the Earth in 1983. See Nature 309 p315-319 for details.
| 3200 Phaethon | October 11 1983 |
| 3728 IRAS | August 23 1983 |
| (10714) 1983 QG | August 31 1983 |
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