Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample

Unusual explosive activity occasionally occurs from the Sun, releasing large amounts of solar energetic particles. Extreme solar particle ejection events in the past 11,000 yr have been detected by sharp increases of cosmogenic isotopes in annual tree rings and ice cores. However, quantitative estim...

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Main Authors: Tomoya Obase, Ken-ichi Bajo, Yuta Otsuki, Hisayoshi Yurimoto
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad9919
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author Tomoya Obase
Ken-ichi Bajo
Yuta Otsuki
Hisayoshi Yurimoto
author_facet Tomoya Obase
Ken-ichi Bajo
Yuta Otsuki
Hisayoshi Yurimoto
author_sort Tomoya Obase
collection DOAJ
description Unusual explosive activity occasionally occurs from the Sun, releasing large amounts of solar energetic particles. Extreme solar particle ejection events in the past 11,000 yr have been detected by sharp increases of cosmogenic isotopes in annual tree rings and ice cores. However, quantitative estimation of the event magnitudes is not straightforward, as the cosmogenic isotopes are indirect records of solar particles. Similar solar particle ejection events may also accumulate records in surface materials of airless bodies such as the Moon and asteroids. Samples from the asteroid 25143 Itokawa have been irradiated by solar winds for tens to hundreds of years at some points in the last few million years. Here, we report implantation profiles of solar particle He from an Itokawa regolith grain that trace an extreme solar particle ejection event. The implantation profiles indicate that the fluences of suprathermal solar particles were 250–1300 times larger than that expected from the current normal solar activity. Since the degrees of excesses are inversely related to the solar wind irradiation periods, the high-energy particle fluence would have been derived from a single event. The event was approximately 40 times larger than the 2003 Halloween solar storms, which is one of the largest solar particle ejection events observed since the space-based measurement of solar activity began. The event magnitude is similar to the largest events inferred from the cosmogenic isotope records in terrestrial samples. Our result provides direct evidence of an extreme solar particle ejection event in the last few million years.
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spelling doaj-art-de0faddfefe240efae16db61b3c72f812025-01-07T17:50:37ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01978214210.3847/1538-4357/ad9919Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa SampleTomoya Obase0https://orcid.org/0000-0003-4755-1179Ken-ichi Bajo1https://orcid.org/0000-0002-9013-2730Yuta Otsuki2Hisayoshi Yurimoto3https://orcid.org/0000-0003-0702-0533Department of Natural History Sciences, Hokkaido University , Sapporo, Hokkaido 060-0810, Japan; Department of Earth and Planetary Sciences, Institute of Science Tokyo , Tokyo 152-8551, JapanDepartment of Natural History Sciences, Hokkaido University , Sapporo, Hokkaido 060-0810, JapanDepartment of Natural History Sciences, Hokkaido University , Sapporo, Hokkaido 060-0810, JapanDepartment of Natural History Sciences, Hokkaido University , Sapporo, Hokkaido 060-0810, Japan; Isotope Imaging Laboratory (IIL), Creative Research Institution, Hokkaido University , Sapporo, Hokkaido 001-0021, JapanUnusual explosive activity occasionally occurs from the Sun, releasing large amounts of solar energetic particles. Extreme solar particle ejection events in the past 11,000 yr have been detected by sharp increases of cosmogenic isotopes in annual tree rings and ice cores. However, quantitative estimation of the event magnitudes is not straightforward, as the cosmogenic isotopes are indirect records of solar particles. Similar solar particle ejection events may also accumulate records in surface materials of airless bodies such as the Moon and asteroids. Samples from the asteroid 25143 Itokawa have been irradiated by solar winds for tens to hundreds of years at some points in the last few million years. Here, we report implantation profiles of solar particle He from an Itokawa regolith grain that trace an extreme solar particle ejection event. The implantation profiles indicate that the fluences of suprathermal solar particles were 250–1300 times larger than that expected from the current normal solar activity. Since the degrees of excesses are inversely related to the solar wind irradiation periods, the high-energy particle fluence would have been derived from a single event. The event was approximately 40 times larger than the 2003 Halloween solar storms, which is one of the largest solar particle ejection events observed since the space-based measurement of solar activity began. The event magnitude is similar to the largest events inferred from the cosmogenic isotope records in terrestrial samples. Our result provides direct evidence of an extreme solar particle ejection event in the last few million years.https://doi.org/10.3847/1538-4357/ad9919Solar windSolar energetic particlesSolar stormRegolithMass spectrometryAsteroids
spellingShingle Tomoya Obase
Ken-ichi Bajo
Yuta Otsuki
Hisayoshi Yurimoto
Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
The Astrophysical Journal
Solar wind
Solar energetic particles
Solar storm
Regolith
Mass spectrometry
Asteroids
title Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
title_full Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
title_fullStr Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
title_full_unstemmed Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
title_short Extreme Solar Particle Ejection Event in the Last Few Million Years from Asteroid Itokawa Sample
title_sort extreme solar particle ejection event in the last few million years from asteroid itokawa sample
topic Solar wind
Solar energetic particles
Solar storm
Regolith
Mass spectrometry
Asteroids
url https://doi.org/10.3847/1538-4357/ad9919
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AT kenichibajo extremesolarparticleejectioneventinthelastfewmillionyearsfromasteroiditokawasample
AT yutaotsuki extremesolarparticleejectioneventinthelastfewmillionyearsfromasteroiditokawasample
AT hisayoshiyurimoto extremesolarparticleejectioneventinthelastfewmillionyearsfromasteroiditokawasample