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'Space archaeology' reveals first dynamic history of a giant spiral galaxy

Using chemical fingerprints, astronomers traced NGC 1365's growth through repeated mergers and star formation, analyzing over 4,500 regions to reconstruct 12 billion years of evolution.

  • On March 23, researchers published in Nature Astronomy a reconstruction of NGC 1365's 12 billion-year growth by reading chemical fingerprints beyond the Milky Way.
  • Using TYPHOON survey data from the Irénée du Pont telescope at Las Campanas Observatory, researchers isolated individual star-forming regions in NGC 1365 for detailed chemical mapping.
  • Researchers measured oxygen abundance across more than 4,500 regions of NGC 1365 and compared those patterns to roughly 20,000 IllustrisTNG simulations to infer the galaxy's assembly.
  • The method offers a way to test whether the Milky Way's growth is typical, and researchers said the project was 50 percent theory and 50 percent observations.
  • Its core formed early and became oxygen-rich, while outer regions grew through dwarf galaxy mergers that later built the spiral arms.
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Phys.org broke the news in United Kingdom on Monday, March 23, 2026.
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