Interstellar

Increased And Varied Radiation During The Sun’s Encounters With Cold Clouds In The Last 10 Million Years

By Keith Cowing
Status Report
astro-ph.EP
January 27, 2026
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Increased And Varied Radiation During The Sun’s Encounters With Cold Clouds In The Last 10 Million Years
Heliosphere 2-3 Myr ago –speed. (a) meridional plane (b) equatorial plane showing the trajectory of Earth. When Earth will be inside the heliosphere the Galactic Cosmic Rays will be filtered by the heliosphere and there will be an increase of HEPs. (c) zoom of panel b on the termination shock. The termination shock at these small distances is a parallel shock. — astro-ph.EP

Recent research raises the possibility that 3 and 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.

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

Comments: 34 pages, 4 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2601.11785 [astro-ph.EP] (or arXiv:2601.11785v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2601.11785
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Submission history
From: Anna Nica
[v1] Fri, 16 Jan 2026 21:17:47 UTC (898 KB)
https://arxiv.org/abs/2601.11785
Astrobiology,

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