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Earth Continues to Receive Radioactive “Rain” from Distant Supernova Collisions

New research suggests Earth has been bombarded by radioactive material from ancient supernova events for over 100 million years, with implications for planetary science and our understanding of cosmic history.

News Published 21 June 2026 4 min read Maya Turner
Artist's impression of two neutron stars colliding, or a cross-section of deep-sea manganese crust showing layers of deposition.
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German scientists have uncovered compelling evidence that Earth has been continuously receiving radioactive “rain” for over 100 million years, a phenomenon stemming from the violent collision of two supernovas. This ongoing cosmic bombardment, previously thought to be a more recent event, is shedding new light on the long-term processes shaping our planet and the universe.

The discovery hinges on the analysis of deep-sea ferromanganese crusts, which act as geological time capsules, preserving a record of materials that have settled on the ocean floor over eons. These crusts form slowly, accumulating metals like iron and manganese from seawater, and in doing so, trap other substances that fall into the ocean.

Cosmic Origins of Radioactive Isotopes

At the heart of this finding is the detection of plutonium-244, a radioactive isotope that does not occur naturally on Earth. Plutonium-244 is primarily formed during extreme cosmic events known as the “r-process,” where light atoms rapidly absorb neutrons. The most common source of this process is the kilonova, an explosion resulting from the merger of two neutron stars.

Scientists also examined levels of curium-247, another isotope formed during such mergers, which has a significantly shorter half-life than plutonium-244. The absence of curium-247 in the analyzed deep-sea crust samples indicates that it has completely decayed, a process that would take more than 100 million years. This absence, coupled with the presence of plutonium-244, points to an event that occurred well over 100 million years ago, but less than a billion years ago.

A Persistent “Rain”

While the initial supernova event may have occurred millions of years ago, the study suggests that the radioactive fallout has not ceased. The uniform presence of plutonium in the upper layers of the crust indicates a continuous, albeit likely low-level, deposition of this material. This ongoing “rain” means Earth continues to be influenced by these ancient cosmic cataclysms, even today.

Previous analyses of similar deep-sea crusts had identified iron-60, another radioisotope associated with supernova explosions. Iron-60 has a much shorter half-life of 2.6 million years. The earlier conclusion, based on the presence of iron-60, was that the radioactive shower originated from a supernova event around 3 million years ago. However, the new research, by incorporating the analysis of curium-247, refines this timeline considerably and establishes a much longer duration for the radioactive fallout.

The researchers explain that the iron-60 detected in the samples likely originated from different, distinct cosmic events than the plutonium-244 and curium-247. The varying levels of iron-60 do not align with the deposition patterns of the plutonium isotopes, supporting the idea of multiple cosmic sources contributing to Earth’s radioactive inventory.

Implications for Earth Science and Astrobiology

The continuous influx of extraterrestrial radioactive material has long-term implications for planetary science. While the levels detected are not considered a threat to life on Earth, they contribute to the planet’s overall elemental composition and can provide insights into the history of cosmic events and their impact on our solar system.

The researchers speculate that the immense cataclysm that triggered this prolonged radioactive shower might have had a more significant impact on Earth than currently understood, potentially even affecting life. However, further investigation is required to confirm any such connections. This discovery underscores the dynamic and interconnected nature of the cosmos, where ancient stellar events continue to influence our planet in subtle yet profound ways.

Key facts

Isotope Half-life Origin Significance for Study
Plutonium-244 81 million years Merger of neutron stars (r-process) Presence indicates a cosmic event >100 million years ago; continuous fallout detected.
Curium-247 6 million years Merger of neutron stars (r-process) Absence in samples suggests complete decay, confirming event predates 100 million years.
Iron-60 6 million years Supernova explosions Indicates separate, more recent cosmic events; deposition patterns differ from plutonium.

This research highlights how studying the deep ocean can unlock secrets of the universe, connecting the seemingly disparate fields of geology and astrophysics. By analyzing the chemical signatures left in the Earth’s crust, scientists can piece together a history of cosmic events that have shaped our planet over billions of years.

Source: Científicos alemanes han descubierto que la Tierra lleva más de 100 millones de años recibiendo lluvia radiactiva por el violento “beso” de dos supernovas – Xataka (https://www.xataka.com/espacio/cientificos-alemanes-han-descubierto-que-tierra-lleva-100-millones-anos-recibiendo-lluvia-radiactiva-violento-beso-dos-supernovas)

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Xataka IA Publicacion original: 2026-06-21T12:31:07+00:00