The final date in the observing calendar
Source note on this page: NASA’s Swift Mission Ends, Leaves Behind Scientific Bonanza
Source note on this page: NASA’s Swift Mission Ends Ahead of Re-Entry
NASA’s announcement dated 23 October reports the end of the Neil Gehrels Swift Observatory’s science mission. The final observation took place on 20 October 2026. Launched on 20 November 2004, the spacecraft leaves nearly 22 years of observations.
According to the agency’s separate operations record, Swift entered safe mode on 20 October at an altitude of 275 kilometres when it could no longer compensate for increased atmospheric drag. The team at Penn State subsequently sent the command ending operations. That altitude belongs to the day described in the record; it is not a measurement of today’s orbit.
Back to section list ↑The science behind a one-minute response
Source note on this page: NASA’s Swift Mission Ends, Leaves Behind Scientific Bonanza
Swift’s task went beyond noticing a burst. Locating a gamma-ray burst, relaying its position to other observatories and turning its own X-ray and ultraviolet/optical telescopes toward the target before the afterglow faded formed one chain. NASA says this typically took about a minute. Different wavelengths provided separate observing records of the same brief event.
NASA’s mission account includes more than 2,000 gamma-ray bursts, studies of more than 1,400 supernovae and about 7,000 published scientific papers to which Swift data contributed.
Back to section list ↑For readers who want to find the data
Source note on this page: NASA’s Swift Mission Ends, Leaves Behind Scientific Bonanza
Source note on this page: Swift Archive Download Portal
The agency describes an open archive of approximately 12 terabytes. It includes more than 1.5 million images from the Ultraviolet/Optical Telescope, alongside brightness measurements and spectra at different wavelengths. The end of new observations does not erase earlier measurements; the records available to researchers and the satellite’s production of new measurements are separate matters.
The UK Swift Science Data Centre at the University of Leicester explains how its download portal finds data by target-name search or date selection. The portal has a stated limit: quick-look data less than a week old are not supplied on that download page. It points readers to a separate catalogue tool for more advanced positional and observation-catalogue queries.
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