A massive eruption from a magnetar in 2004 revealed a new understanding of the universe's heaviest elements like gold and platinum.
The afterglow following the gamma-ray burst from the magnetar indicated the creation of heavy elements through rapid neutron capture, reshaping theories on their origins.
Heavy elements like gold and platinum are primarily formed in extreme environments through rapid neutron capture, a process that requires abundant free neutrons.
Scientists previously believed that such heavy elements were only formed in supernovae or neutron star collisions, until the discovery of magnetar flares as additional contributors.
Magnetars, highly magnetized stars born from massive star cores, can release enormous energy in giant flares, creating conditions for the formation of heavy elements like gold.
Detailed nuclear reaction simulations confirmed that gold and other heavy nuclei can form in the ejected material from magnetar giant flares.
The delayed gamma-ray signal observed after the 2004 magnetar flare matched the expected profile of radioactive decay from newly formed heavy elements like gold.
Researchers estimated that up to 10 percent of the heavy elements in the galaxy could be attributed to magnetar flares, providing valuable insights into galactic enrichment.
Magnetar flares could explain the abundance of heavy elements in ancient galaxies with low metallicity, offering a solution to a longstanding astronomical mystery.
Ongoing research and upcoming missions aim to detect gamma-ray glows in real time, enhancing our understanding of the production of heavy elements in the universe.