Evolution of Volatiles in the Moons Permanently Shadowed Regions | Dr. James Green | H2M2 2025 @ExploreMarsOrg
Evolution of Volatiles in the Moons Permanently Shadowed Regions | Dr. James Green | H2M2 2025  @ExploreMarsOrg
Uploaded June 2025 | Updated September 2026, 1 day ago
Delve into the mysteries of the Moon's permanently shadowed regions (PSRs) with Dr. James Green, Chair of the Explore Mars, Inc. Advisory Board and former NASA Chief Scientist. In this enlightening session from the 2025 Humans to the Moon and Mars Summit (H2M2), Dr. Green explores the origin, composition, and significance of volatiles—such as water ice—trapped in the Moon's coldest and darkest craters.
arXiv

Key Topics:

The formation and preservation of volatiles in lunar PSRs.

Insights from missions like LCROSS and Lunar Reconnaissance Orbiter on detecting water ice.

The role of PSRs in understanding the history of the solar system and the potential for prebiotic chemistry.

Implications for future lunar exploration and in-situ resource utilization (ISRU).
Wikipedia
National Academies Press

About Dr. James Green:
Dr. James Green is a distinguished planetary scientist who served as NASA's Chief Scientist, where he provided strategic guidance on the agency's science programs. With a career spanning over four decades, Dr. Green has been instrumental in advancing our understanding of planetary atmospheres, magnetospheres, and the potential for life beyond Earth.

Additional Resources:

Explore Mars Summit Details: exploremars.org/summit

Dr. James Green's LinkedIn: linkedin.com/in/james-green-planetary-scientist

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Evolution of Volatiles in the Moon's Permanently Shadowed Regions | Dr. James Green | H2M2 2025

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