Updated
Updated · ScienceAlert · Jun 16
Researchers Link Pacific Plutonium-244 to 100-Million-Year-Old Cosmic Blast
Updated
Updated · ScienceAlert · Jun 16

Researchers Link Pacific Plutonium-244 to 100-Million-Year-Old Cosmic Blast

3 articles · Updated · ScienceAlert · Jun 16

Summary

  • Pacific ferromanganese crust from 4,830 meters deep contains Plutonium-244 that researchers say most likely came from a rare r-process explosion more than 100 million years ago, with a kilonova among the leading candidates.
  • No convincing curium-247 was found alongside the plutonium, a key clue because that isotope’s 16-million-year half-life means a recent source should still have left detectable traces.
  • The team also compared iron-60 — tied to supernovae about 2.5 million and 7 million years ago — and concluded the plutonium did not come from those more recent blasts.
  • Plutonium-244’s 81-million-year half-life rules out a primordial Earth source, suggesting the Solar System is still moving through ancient interstellar debris from a long-dispersed explosion.
  • The Nature Astronomy study could help map the Milky Way’s explosion history and test whether past cosmic events influenced Earth’s supply of heavy elements or even life.

Insights

What other exotic stardust from ancient cosmic collisions is currently raining down on our planet, completely undetected until now?
Could a 100-million-year-old cosmic explosion, still raining on Earth, have shaped the evolution of life during the age of dinosaurs?

Landmark Detection of Cosmic Plutonium-244 in Deep-Sea Crusts Points to Kilonovae as Dominant Heavy Element Source

Overview

In June 2026, an international team led by Helmholtz-Zentrum Dresden-Rossendorf (HZDR) discovered cosmic plutonium-244 (Pu-244) in deep-sea ferromanganese crusts using advanced accelerator mass spectrometry. Unlike iron-60, which shows spikes linked to supernovae, Pu-244 was found evenly spread across millions of years, suggesting a continuous cosmic influx rather than bursts from nearby stellar explosions. This breakthrough, published in Nature Astronomy, challenges previous ideas about the origins of heavy elements and highlights the power of new detection technologies to reveal the universe’s history hidden in Earth’s geological archives.

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