How Hydrogen & Helium Shape Planets: From Embryos to Earth & Neptune | Astrobiology Explained (2026)

The Quest for Understanding Hydrogen and Helium's Journey: From Planetary Embryos to Earth-like Worlds

Hydrogen and helium, the fundamental building blocks of planets, remain enigmatic in their chemical interactions, especially within the context of rocky and gas-rich worlds. This study delves into the fascinating dynamics of these elements, utilizing advanced computational methods to unravel their secrets.

Through the application of first-principles molecular dynamics and thermodynamic integration, researchers have quantified the partitioning of hydrogen and helium between molten silicate mantles and metallic cores across a range of planetary masses, from Earth to Neptune. The findings reveal intriguing trends: hydrogen exhibits a strong affinity for metallic cores under pressures exceeding 25 GPa, but this behavior diminishes beyond 200 GPa. Conversely, helium remains attracted to the silicate mantle, yet its solubility in metal increases with pressure. These insights are integrated into coupled structure-chemistry models, offering a comprehensive understanding of the planetary interior.

The implications of these volatile exchanges are far-reaching. They may influence the redox states of secondary atmospheres, the longevity of primordial envelopes, and the predicted abundances of CHNOPS elements. Furthermore, the emergence of helium-enriched atmospheres could be a significant outcome. The study highlights the potential of observing He 1083 nm and H Lyman-α lines as indicators of atmosphere-interior exchange, bridging the gap between atomic-scale interactions and planetary-scale phenomena.

This research not only enhances our understanding of the origins of Earth-to-Neptune-sized worlds but also opens up new avenues for exploration in astrobiology and planetary science. By linking atomic-scale interactions to observable planetary phenomena, it provides valuable constraints for further investigation.

Akash Gupta, Haiyang Luo, Jie Deng, and Adam Burrows

Key Details:
- 38 pages, 9 figures
- Subjects: Earth and Planetary Astrophysics, Materials Science, Atmospheric and Oceanic Physics, Computational Physics
- Cite as: arXiv:2510.24956 [astro-ph.EP]
- Explore More: arXiv:2510.24956v1 [astro-ph.EP]
- DOI: 10.48550/arXiv.2510.24956

This groundbreaking research invites further exploration and discussion, encouraging scientists and enthusiasts alike to delve into the mysteries of our planetary formation and the role of these essential elements.

How Hydrogen & Helium Shape Planets: From Embryos to Earth & Neptune | Astrobiology Explained (2026)

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