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Swift's UVOT acquired this image of Comet Garradd (C/2009 P1) on April 1, 2012, when the comet was 142 million miles away

NASA's Swift Monitors Departing Comet Garradd

Outbound comet C/2009 P1 (Garradd) provided a nice show for skywatchers late last year. Now it's the target of an ongoing investigation by NASA's ...

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Three types of systems, illustrated here, may host Type Ia supernovae.

Swift Narrows Down Hosts of Important Supernova Class

Studies using X-ray and ultraviolet observations from NASA's Swift satellite are providing new insights into the elusive origins of an important ...

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Swift Features

Mission Overview

    Swift is a first-of-its-kind multi-wavelength observatory dedicated to the study of gamma-ray burst (GRB) science. Its three instruments will work together to observe GRBs and afterglows in the gamma ray, X-ray, ultraviolet, and optical wavebands. The main mission objectives for Swift are to:

    • Determine the origin of gamma-ray bursts
    • Classify gamma-ray bursts and search for new types
    • Determine how the blastwave evolves and interacts with the surroundings
    • Use gamma-ray bursts to study the early universe
    • Perform the first sensitive hard X-ray survey of the sky

Mission News

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