2021
DOI: 10.48550/arxiv.2109.11242
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Simulations of $^{60}$Fe entrained in ejecta from a near-Earth supernova: Effects of observer motion

Evgenii Chaikin,
Alexander A. Kaurov,
Brian D. Fields
et al.

Abstract: Recent studies have shown that live (not decayed) radioactive 60 Fe is present in deep-ocean samples, Antarctic snow, lunar regolith, and cosmic rays. 60 Fe represents supernova (SN) ejecta deposited in the Solar System around 3 Myr ago, and recently an earlier pulse β‰ˆ 7 Myr ago has been found. These data point to one or multiple near-Earth SN explosions that presumably participated in the formation of the Local Bubble. We explore this theory using 3D high-resolution smooth-particle hydrodynamical simulation… Show more

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“…At late times, the blast speed slows and Earth's speed could become important; these effects are discussed in (Chaikin et al 2021) in the context of 60 Fe deposition and the local environment encountered by the solar system. It remains for future work to model such effects on the heliosphere, including the possibility that the Earth's velocity is misaligned with that of the supernova blast.…”
Section: Effects Of Solar Motionmentioning
confidence: 99%
“…At late times, the blast speed slows and Earth's speed could become important; these effects are discussed in (Chaikin et al 2021) in the context of 60 Fe deposition and the local environment encountered by the solar system. It remains for future work to model such effects on the heliosphere, including the possibility that the Earth's velocity is misaligned with that of the supernova blast.…”
Section: Effects Of Solar Motionmentioning
confidence: 99%