Magmatic volatiles (H, C, N, F, S, Cl) in the lunar mantle, crust, and regolith: Abundances, distributions, processes, and reservoirs
FM McCubbin, KEV Kaaden, R Tartèse… - American …, 2015 - degruyter.com
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 …
last several years, that have cast into question the post-Apollo view of lunar formation, the …
Origin of the lunar highlands Mg-suite: An integrated petrology, geochemistry, chronology, and remote sensing perspective
The Mg-suite represents an enigmatic episode of lunar highlands magmatism that
presumably represents the first stage of crustal building following primordial differentiation …
presumably represents the first stage of crustal building following primordial differentiation …
A dry lunar mantle reservoir for young mare basalts of Chang'e-5
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 …
the crystallization of the lunar magma ocean and the duration of lunar volcanism. The …
A solar wind-derived water reservoir on the Moon hosted by impact glass beads
The past two decades of lunar exploration have seen the detection of substantial quantities
of water on the Moon's surface. It has been proposed that a hydrated layer exists at depth in …
of water on the Moon's surface. It has been proposed that a hydrated layer exists at depth in …
Water on the surface of the Moon as seen by the Moon Mineralogy Mapper: Distribution, abundance, and origins
S Li, RE Milliken - Science advances, 2017 - science.org
A new thermal correction model and experimentally validated relationships between
absorption strength and water content have been used to construct the first global …
absorption strength and water content have been used to construct the first global …
[HTML][HTML] Water in the Moon's interior: Truth and consequences
EH Hauri, AE Saal, MJ Rutherford… - Earth and Planetary …, 2015 - Elsevier
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 …
reported for 377 samples of lunar volcanic glass from three chemical groups (A15 green …
Early accretion of water in the inner solar system from a carbonaceous chondrite–like source
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 …
important for understanding the dynamics of planet formation. The timing of water accretion …
Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources
FM McCubbin, JW Boyce, P Srinivasan… - … & Planetary Science, 2016 - Wiley Online Library
We conducted a petrologic study of apatite within 12 Martian meteorites, including 11
shergottites and one basaltic regolith breccia. These data were combined with previously …
shergottites and one basaltic regolith breccia. These data were combined with previously …
The evolution of the lunar crust
1609 AD marked the beginning of the modern scientific exploration of the Moon's crust when
Thomas Harriot and later Galileo Galilei made the first recorded maps of the nearside with …
Thomas Harriot and later Galileo Galilei made the first recorded maps of the nearside with …
Evidence for an early wet Moon from experimental crystallization of the lunar magma ocean
Y Lin, EJ Tronche, ES Steenstra… - Nature Geoscience, 2017 - nature.com
The Moon is thought to have been covered initially by a deep magma ocean, its gradual
solidification leading to the formation of the plagioclase-rich highland crust. We performed a …
solidification leading to the formation of the plagioclase-rich highland crust. We performed a …