Many studies exist on magmatic volatiles (H, C, N, F, S, Cl) in and on the Moon, within the last several years, that have cast into question the post-Apollo view of lunar formation, the …
The distribution of water in the Moon's interior carries implications for the origin of the Moon, the crystallization of the lunar magma ocean and the duration of lunar volcanism. The …
Although sunlight-driven water splitting is a promising route to sustainable hydrogen fuel production, widespread implementation is hampered by the expense of the necessary …
Earth's water, intrinsic oxidation state and metal core density are fundamental chemical features of our planet. Studies of exoplanets provide a useful context for elucidating the …
Y Xu, HC Tian, C Zhang… - Proceedings of the …, 2022 - National Acad Sciences
Remote sensing data revealed that the presence of water (OH/H2O) on the Moon is latitude- dependent and probably time-of-day variation, suggesting a solar wind (SW)-originated …
Identifying the source of Earth's water is central to understanding the origins of life-fostering environments and to assessing the prevalence of such environments in space. Water …
Geochemical data for H 2 O and other volatiles, as well as major and trace elements, are reported for 377 samples of lunar volcanic glass from three chemical groups (A15 green …
The Moon formed 4.5 Ga ago through a collision between proto-Earth and a planetesimal known as Theia. The compositional similarity of Earth and Moon puts tight limits on the …
Determining the origin of water and the timing of its accretion within the inner solar system is important for understanding the dynamics of planet formation. The timing of water accretion …