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AKA: SA-200LL. Status: Operational 2004. First Launch: 2004-11-20. Last Launch: 2004-11-20. Number: 1 . Gross mass: 1,331 kg (2,934 lb). Its three instruments would work together to observe GRBs and afterglows in the gamma-ray, X-ray, ultraviolet, and optical wavebands. The main mission objectives for Swift were to:
During its nominal 2-year mission, Swift was expected to observe more than 200 bursts with a sensitivity ~3 times fainter than the BATSE detector aboard the Compton Gamma-Ray Observatory. Swift's Burst Alert Telescope would detect and acquire high-precision locations for gamma ray bursts and then relay a 1-4 arc-minute position estimate to the ground within 15 seconds. After the initial burst detection, the spacecraft would "swiftly" (approximately 20 to 75 seconds) and autonomously repoint itself to bring the burst location within the field of view of the sensitive narrow-field X-ray and UV/optical telescopes to observe afterglow. Swift would provide red shifts for the bursts and multi-wavelength light curves for the duration of the afterglow. Swift measurements would be of great interest to the astronomical community and all data products would be available to the public via the internet as soon as they were processed. The Swift mission would represent the most comprehensive study of GRB afterglow to date. Swift was part of NASA's medium explorer (MIDEX) program. The hardware was developed by an international team from the United States, the United Kingdom, and Italy, with additional scientific involvement in France, Japan, Germany, Denmark, Spain, and South Africa. Swift Baseline Capabilities:
The Swift telescope payload was comprised of three instruments which worked in tandem to provide rapid identification and multiwavelength follow-up of Gamma-ray bursts (GRBs) and their afterglows. Within 20 to 75 seconds of a detected GRB, the telescope would slew autonomously so that the fields-of-view of the pointed instruments overlap the location of the burst. The afterglows would be monitored over their durations, and the data rapidly disseminated to the public.
Burst Alert Telescope (BAT): 15 - 150 keV
X-ray Telescope (XRT): 0.3 - 10 keV
UV/Optical Telescope (UVOT): 170 - 650 nm
NASA NSSDC Master Catalog Description The Swift Gamma Ray Burst Explorer is a three-telescope space observatory for studying gamma ray bursts (GRBs) and monitoring the afterglow in X-ray, and UV/Visible light at the location of a burst. The burst detection rate is 100 per year, with a sensitivity ~3 times fainter than the BATSE detector aboard the Compton Gamma-Ray Observatory. The Swift mission was launched with a nominal on-orbit lifetime of two years. Swift is a NASA Midex (medium-class Explorer) mission. It was the third to be launched, following IMAGE and WMAP.
Family: Astronomy, Gamma ray astronomy satellite. Country: USA. Launch Vehicles: Thor, Delta, Delta 7320-10C. Launch Sites: Cape Canaveral, Cape Canaveral LC17A. Agency: NASA. More at: 6962, 13243. Bibliography: 2, 4131, 4132, 4133, 4134.
2004 November 20 - . 17:16 GMT - . Launch Site: Cape Canaveral. Launch Complex: Cape Canaveral LC17A. Launch Pad: SLC17A. LV Family: Thor. Launch Vehicle: Delta 7320-10C.
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