Ancient Supernovae and Kilonovae Deposits Found in Deep-Sea Sediments

March 31, 2025
4 mins read
Representative Image: ESO/M. Kornmesser( CC BY 4.0)
Representative Image: ESO/M. Kornmesser( CC BY 4.0)

Scientists have uncovered compelling evidence of ancient stellar explosions that rained debris onto Earth and the Moon, with deep-sea sediments revealing traces of radioactive isotopes from both supernovae and kilonovae events.

Star Explosions Left Traces in Our Backyard

Research led by Brian Fields, an astronomer at the University of Illinois Urbana-Champaign, has found that Earth contains the remnants of cosmic explosions dating back millions of years.

“We live in a supernova graveyard,” Fields stated during his presentation at the 2025 American Physical Society Global Physics Summit. His team discovered that radioactive isotopes from these stellar explosions “accumulate in the depths of the ocean, and they’ll also hang onto the moon.”

Two Key Discoveries Rewriting Cosmic History

The research centers on two major findings:

1. Plutonium-244: Evidence of a Nearby Kilonova

Scientists detected plutonium-244, a long-lived radioactive isotope with an 80-million-year half-life, in deep-sea sediments. This isotope forms primarily during the rapid neutron-capture process (r-process) that occurs when neutron stars collide in kilonovae events.

The presence of plutonium-244 suggests a kilonova explosion occurred relatively close to our solar system approximately 10 million years ago—much closer than the GW170817 kilonova observed in 2017 at a distance of 130 million light-years.

2. Iron-60: Supernova Fingerprints

Researchers also found elevated levels of iron-60, a radioactive isotope with a 2.6-million-year half-life that forms during supernova explosions. This indicates that separate supernova events occurred around 100,000 and 1 million years ago.

“This is direct observational evidence that supernovas are radioactivity factories,” Fields explained.

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The Cosmic Elements Factory

These stellar explosions are crucial for creating heavy elements throughout the universe:

  • Supernovae primarily produce elements up to iron
  • Kilonovae generate elements heavier than iron through the r-process, including gold, platinum, and plutonium

As Fields described the process: “We had a kilonova that made plutonium—like it loves to do—and blasted it all over the place. Then, with the stirring of material by a supernova, it got all mixed up, and some of that fell to Earth.”

Moon Samples: The Next Research Frontier

While Earth samples have yielded valuable data, researchers believe lunar soil could provide even clearer evidence due to the Moon’s lack of atmosphere, weather, and geological activity.

“On Earth, things sink to the bottom of the ocean, and you have to worry about currents and the atmosphere,” Fields told Live Science. “But the moon is awesome because when stuff lands, it just lands.”

The research team hopes that upcoming Artemis missions will provide access to lunar samples that could confirm their findings and offer more precise dating of these cosmic events.

“We’re writing papers to prove to the Artemis community that this is something to seriously think about,” Fields said. “The samples are coming back anyway. We just want to piggyback off of it.”

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Local Bubble: Our Cosmic Neighborhood

These discoveries provide insight into our local cosmic environment, known as the Local Bubble—a region of low-density, hot gas surrounded by denser, cooler gas. Scientists believe this bubble formed from a series of supernova explosions within the last few million years.

The radioactive isotopes found on Earth likely came from supernovae that exploded within this Local Bubble, helping astronomers better understand our galactic neighborhood’s history.

Frequently Asked Questions

What evidence suggests ancient stellar explosions affected Earth? +
Scientists have discovered radioactive isotopes in deep-sea sediments that could only have come from cosmic explosions. These include plutonium-244 (from kilonovae) and iron-60 (from supernovae), which have been found in Earth’s oceans, providing direct evidence that material from these stellar explosions reached our planet.
How do scientists know the age of these stellar explosions? +
Scientists determine the age of stellar explosions by analyzing the radioactive isotopes they leave behind. Using the known half-lives of these isotopes (80 million years for plutonium-244 and 2.6 million years for iron-60), researchers can calculate when the explosions occurred. The findings suggest a kilonova happened about 10 million years ago, while separate supernovae occurred approximately 100,000 and 1 million years ago.
What’s the difference between a supernova and a kilonova? +
A supernova is the explosive death of a massive star, which primarily produces elements up to iron on the periodic table. A kilonova is a different type of explosion that occurs when two neutron stars collide. Kilonovae generate much heavier elements through the rapid neutron-capture process (r-process), including gold, platinum, and plutonium. Both types of explosions disperse these elements throughout space.
How close were these stellar explosions to our solar system? +
The research suggests these explosions occurred relatively close to our solar system in cosmic terms. The kilonova that left plutonium-244 traces appears to have happened about 10 million years ago at a much closer distance than the GW170817 kilonova observed in 2017 (which was 130 million light-years away). The supernovae that left iron-60 traces occurred within what astronomers call the Local Bubble, a region of space surrounding our solar system.
Why are scientists looking at the Moon for evidence of these explosions? +
The Moon provides a more pristine environment for studying cosmic debris compared to Earth. With no atmosphere, weather, or geological activity, material from space that lands on the lunar surface stays there undisturbed. This makes the Moon an ideal “recorder” of cosmic events. Scientists hope the upcoming Artemis missions will collect lunar samples that contain clearer evidence of these stellar explosions.
How do these findings affect our understanding of the universe? +
These discoveries provide crucial insights into how heavy elements are created and distributed throughout the universe. They confirm theoretical models about element formation in stellar explosions and help explain the presence of heavy elements on Earth. The findings also improve our understanding of the Local Bubble—our cosmic neighborhood—and its formation through a series of supernova explosions over the past few million years. This research connects Earth’s geological record with astronomical events, creating a more complete picture of our cosmic history.

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