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Magnetar Flares Confirmed as Key Source of Heavy Elements in Milky Way

New research reveals that up to 10% of the galaxy’s heavy elements, including gold and uranium, originate from rare, powerful eruptions of highly magnetized neutron stars.

Image
An artist’s impression of a magnetar. Image credit: NASA’s Goddard Space Flight Center / S. Wiessinger.

Overview

  • Analysis of the 2004 SGR 1806-20 magnetar flare confirms radioactive decay signals consistent with the creation of heavy elements through the r-process.
  • Magnetar flares, caused by extreme magnetic activity in neutron stars, are now estimated to contribute up to 10% of the Milky Way's heavy elements.
  • This discovery complements the 2017 neutron star merger findings, addressing gaps in explaining the early universe's heavy-element abundance.
  • Future missions, like NASA’s COSI launching in 2027, aim to directly identify individual elements from magnetar flares and validate these findings.
  • The study highlights the role of magnetar flares in galactic chemical evolution, influencing the formation of stars, planets, and potentially habitable environments.