日本地球惑星科学連合2024年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT16] 惑星中心核:内部構造・形成・進化

2024年5月29日(水) 13:45 〜 15:00 102 (幕張メッセ国際会議場)

コンビーナ:飯塚 理子(早稲田大学教育学部理学科地球科学専修)、中島 陽一(熊本大学大学院先端科学研究部物理科学講座)、新名 良介(明治大学)、河口 沙織(高輝度光科学研究センター)、座長:飯塚 理子(早稲田大学教育学部理学科地球科学専修)、河口 沙織(高輝度光科学研究センター)

13:45 〜 14:00

[SIT16-01] Helium in the Earth’s core

*William F McDonough1 (1.Department of Earth Science, Sendai, Miyagi 980-8578, Japan)

キーワード:Earth's core, helium, volcanic gases, core--mantle exchange

To explain the often observed occurrence of 3He-enriched isotopic compositions in some ocean island basalts (OIB) the Earth's core is often invoked as a source of primitive helium gas with a solar, or nearly so, isotopic composition (i.e., Rcore/RA > 120, where RA = (3He/4He) of the atmosphere (i.e., 1.340 ± 0.006)). Here we examine this assumption and consider a number of likely scenarios where the core might or might not be a supplier of isotopically primitive helium gas. Given experimentally determined solubilities for He in a core forming metallic melt and compositional models for the core, we show here that alpha emitting radioisotopes of platinum group elements alone can reduce by about half the original primitive solar isotopic composition of helium. Moreover, adding about 1 picogram/gram of U into the core further reduces the core's 3He/4He value (<50). These observations should motivate further studies on the nature of helium in the core.