Terrestrial Effects Of Nearby Supernovae In The Early Pleistocene
Brian C. Thomas (Washburn Univ.), E. E. Engler (Washburn Univ.), M., Kachelrie{\ss} (NTNU), A. L. Melott (Univ. Kansas), A. C. Overholt, (MidAmerica Univ.), and D.V. Semikoz (U. Paris Diderot, Nat. Res. Nuclear U.)

TL;DR
This study assesses the potential impact of nearby supernovae in the early Pleistocene on Earth's atmosphere and life, finding limited chemical effects but significant increases in radiation exposure that could influence climate and biological mutations.
Contribution
It provides a detailed analysis of the terrestrial atmospheric and biological effects of supernovae at 100 pc, highlighting radiation increases and their possible ecological implications.
Findings
Weak ozone depletion from supernova photon effects
Significant increase in ground-level muon radiation
Potential link to Pliocene-Pleistocene boundary extinction
Abstract
Recent results have strongly confirmed that multiple supernovae happened at distances ~100 pc consisting of two main events: one at 1.7 to 3.2 million years ago, and the other at 6.5 to 8.7 million years ago. These events are said to be responsible for excavating the Local Bubble in the interstellar medium and depositing 60Fe on Earth and the Moon. Other events are indicated by effects in the local cosmic ray (CR) spectrum. Given this updated and refined picture, we ask whether such supernovae are expected to have had substantial effects on the terrestrial atmosphere and biota. In a first cut at the most probable cases, combining photon and cosmic ray effects, we find that a supernova at 100 pc can have only a small effect on terrestrial organisms from visible light and that chemical changes such as ozone depletion are weak. However, tropospheric ionization right down to the ground due…
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