Highest terrestrial <sup>3</sup>He/<sup>4</sup>He credibly from the core.
basic_science · Level V
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- Record sourced from PubMed, PMID 37853120.
- Also identified by DOI 10.1038/s41586-023-06590-8.
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Abstract
The observation that many lavas associated with mantle plumes have higher <sup>3</sup>He/<sup>4</sup>He ratios than the upper convecting mantle underpins geophysical, geodynamic and geochemical models of Earth's deep interior. High <sup>3</sup>He/<sup>4</sup>He ratios are thought to derive from the solar nebula or from solar-wind-irradiated material that became incorporated into Earth during early planetary accretion. Traditionally, this high-<sup>3</sup>He/<sup>4</sup>He component has been considered intrinsic to the mantle, having avoided outgassing caused by giant impacts and billions of years of mantle convection<sup>1-4</sup>. Here we report the highest magmatic <sup>3</sup>He/<sup>4</sup>He ratio(67.2 ± 1.8 times the atmospheric ratio) yet measured in terrestrial igneous rocks, in olivines from Baffin Island lavas. We argue that the extremely high-<sup>3</sup>He/<sup>4</sup>He helium in these lavas might derive from Earth's core<sup>5-9</sup>. The viability of the core hypothesis relaxes the long-standing constraint-based on noble gases in lavas associated with mantle plumes globally-that volatile elements from the solar nebula have survived in the mantle since the early stages of accretion.