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Magnetar Flares Confirmed as Key Source of Heavy Elements

New analysis of 2004 gamma-ray data reveals magnetar flares forge up to 10% of the Milky Way’s gold, platinum, and uranium through r-process nucleosynthesis.

This artist's concept depicts a magnetar – a type of neutron star with a strong magnetic field – losing material into space. Shown as thin green lines, the magnetic field lines influence the movement of charged material around the magnetar. NASA/JPL-Caltech
Artist's impression of flares bursting from a rupture in a magnetar.
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Overview

  • Researchers identified magnetar giant flares as a second confirmed site of r-process nucleosynthesis, supplementing neutron star mergers in producing heavy elements.
  • The study analyzed gamma-ray data from the 2004 SGR 1806–20 magnetar flare, linking delayed emissions to radioactive decay of newly formed heavy elements.
  • Magnetar flares, which occur early in galactic history, may account for 1-10% of the Milky Way's heavy elements, including gold and uranium.
  • The 2004 flare alone produced approximately one-millionth of a solar mass in heavy elements, equivalent to 27 lunar masses or a third of Earth’s mass.
  • NASA’s upcoming COSI mission, launching in 2027, is expected to further characterize r-process signals from future magnetar flares, enhancing our understanding of cosmic chemical evolution.