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NASA’s Swift space telescope heads for fiery atmospheric reentry after 22 years

The storied Neil Gehrels Swift Observatory ended science operations after atmospheric drag degraded its orbit and a private robotic rescue mission failed to boost the spacecraft.

Swift Observatory spacecraft model
NASA E/PO, Sonoma State University/Aurore Simonnet / Wikimedia Commons, Public domain

A pioneering NASA space telescope that revolutionized the study of cosmic explosions has concluded its scientific mission and will soon burn up in Earth’s atmosphere, space agency officials confirmed. The Neil Gehrels Swift Observatory ceased science operations on Oct. 20 after falling to an altitude of roughly 171 miles, where atmospheric drag made it impossible to reliably steer its instruments toward cosmic targets.

The spacecraft, which spent nearly 22 years in low Earth orbit chasing gamma-ray bursts, is projected to reenter the atmosphere in the coming weeks, according to reports from Live Science and Interesting Engineering. Its demise follows an unsuccessful attempt earlier this year to prolong its flight using a commercial servicing vehicle.

A failed orbital rescue

Swift’s gradual descent accelerated due to heightened solar activity. When the sun enters an active phase, solar radiation warms Earth’s upper atmosphere, causing the atmospheric layer to expand outward. That expansion created extra aerodynamic friction against the spacecraft, steadily sapping its velocity and pulling it closer to the planet.

To save the mission, NASA contracted the Arizona-based firm Katalyst Space Technologies to build an orbital servicing spacecraft named LINK. Launched on July 3 on a Northrop Grumman Pegasus XL rocket, the robotic craft was designed to dock with Swift and nudge it into a higher, safer orbit. However, an attitude-control malfunction struck LINK, rendering the docking and boost attempt impossible, Science News reported. NASA announced in August that the rescue plan had been abandoned.

The spacecraft entered safe mode on Oct. 20 after conducting final observations of Earth’s atmosphere and tracking a distant comet, Interesting Engineering reported.

More than two decades of cosmic tracking

Swift launched on Nov. 20, 2004, designed for an initial primary mission of two years. Instead, it operated for more than a decade beyond its planned lifetime, observing the most energetic phenomena known since the Big Bang. Its key breakthrough was speed: while earlier telescopes took hours or days to pivot, Swift’s Burst Alert Telescope could identify a gamma-ray burst and allow the spacecraft to swing its optical and X-ray sensors toward the coordinates within about a minute.

“Swift was designed as a satellite dedicated to studying gamma-ray bursts, outbursts that came and went so quickly that no one could target them with large telescopes to learn more,” S. Bradley Cenko, the mission’s principal investigator at NASA’s Goddard Space Flight Center, said in a NASA statement quoted by Live Science.

Over its tenure, Swift logged more than 2,000 gamma-ray bursts and studied more than 1,400 supernovae. In 2022, it played a central role in measuring an extraordinarily intense blast designated GRB 221009A, widely known among astronomers as the “brightest of all time,” or BOAT. The telescope also contributed to landmark multiobservatory detections in 2017 involving gravitational waves from colliding neutron stars and high-energy cosmic neutrinos.

Scientific legacy outlives the craft

Although Swift’s physical hardware will soon disintegrate, scientists emphasize that its discoveries are far from finished. The observatory amassed approximately 12 terabytes of public data and captured more than 1.5 million images across visible, ultraviolet and X-ray wavelengths. That archive has supported around 7,000 academic papers, with researchers continuing to mine the repository for unexamined cosmic events.

No identical multiwavelength telescope is currently waiting to replace Swift’s rapid-pointing capabilities, Science News reported, leaving astronomers to rely on a patchwork of other orbital observatories and commercial platforms for time-sensitive transient astronomy.