# Increased and varied radiation during the Sun’s encounters with cold clouds in the last 10 million years

**Authors:** Merav Opher, Joe Giacalone, Abraham Loeb, Evan P. Economo, Alan Cummings, Jennifer Middleton, Catherine Zucker, Jesse A. Miller, Anna Nica, Maria Hatzaki

PMC · DOI: 10.1038/s41598-026-36926-z · 2026-02-11

## TL;DR

The Sun's encounters with cold clouds over the last 10 million years exposed Earth to intense and prolonged high-energy radiation, affecting climate and biodiversity.

## Contribution

This study identifies and characterizes Heliospheric Energetic Particles (HEPs) during past solar system encounters with interstellar clouds.

## Key findings

- Earth experienced prolonged exposure to high-energy protons during heliosphere shrinkage, much more intense than current solar events.
- Galactic cosmic ray radiation during Earth's excursion outside the heliosphere was significantly stronger than today.
- These radiation variations could have influenced Earth's climate and biodiversity over extended periods.

## Abstract

Recent research raises the possibility that 2–3 and 6–7 million years ago, the Sun encountered massive clouds that shrank the heliosphere —the solar cocoon protecting our solar system— exposing Earth to its interstellar environment, in agreement with geological evidence from 60Fe and 244Pu isotopes. Here we show that during such encounters Earth was exposed to increased radiation in the form of high-energy particles. During periods of Earth’s immersion in the heliosphere, it received particle radiation that we name Heliospheric Energetic Particles (HEPs). The intensity of < 10 MeV protons was at least an order of magnitude more intense than today’s most extreme solar energetic particle (SEP) events. SEPs today last minutes to hours, but HEP exposure then lasted for extensive periods of several months, making it a prolonged external driver. During Earth’s excursion outside the heliosphere, it was exposed to a galactic cosmic ray radiation with the intensity of < 1 GeV protons at least an order of magnitude more intense than today. Therefore, the space surrounding Earth was permeated by a variable high-energy radiation. We discuss the implications for Earth’s climate and biodiversity.

## Full-text entities

- **Chemicals:** 60Fe (MESH:C000615389), HEP (-)

## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12966331/full.md

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Source: https://tomesphere.com/paper/PMC12966331