[HTML][HTML] The diverse planetary ingassing/outgassing paths produced over billions of years of magmatic activity
The CHONS elements that constitute the outgassed atmosphere and exosphere have likely
been delivered by chondritic materials to the Earth during planetary accretion and …
been delivered by chondritic materials to the Earth during planetary accretion and …
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 …
[HTML][HTML] Evidence of a hydrated mineral enriched in water and ammonium molecules in the Chang'e-5 lunar sample
S Jin, M Hao, Z Guo, B Yin, Y Ma, L Deng, X Chen… - Nature …, 2024 - nature.com
The presence and distribution of water on the Moon are fundamental to our understanding of
the Earth–Moon system. Despite extensive laboratory research and remote sensing …
the Earth–Moon system. Despite extensive laboratory research and remote sensing …
Magmatic chlorine isotope fractionation recorded in apatite from Chang'e-5 basalts
The Moon can have elevated chlorine (Cl) isotope ratios, much higher than any other Solar
System objects. Deciphering the Cl isotope compositions of volcanic lunar samples is critical …
System objects. Deciphering the Cl isotope compositions of volcanic lunar samples is critical …
Origin and abundances of H2O in the terrestrial planets, Moon, and asteroids
FM McCubbin, JJ Barnes - Earth and Planetary Science Letters, 2019 - Elsevier
The presence of H 2 O within differentiated terrestrial bodies in the inner Solar System is
well established; however, the source (s) of this H 2 O and the time of its arrival to the inner …
well established; however, the source (s) of this H 2 O and the time of its arrival to the inner …
[HTML][HTML] Solubility of water in peridotite liquids and the prevalence of steam atmospheres on rocky planets
Atmospheres are products of time-integrated mass exchange between the surface of a
planet and its interior. On Earth and other planetary bodies, magma oceans likely marked …
planet and its interior. On Earth and other planetary bodies, magma oceans likely marked …
Nitrogen and carbon fractionation in planetary magma oceans and origin of the superchondritic C/N ratio in the bulk silicate Earth
Y Li, M Wiedenbeck, B Monteleone, R Dasgupta… - Earth and Planetary …, 2023 - Elsevier
Volatiles are important for planetary geodynamics, climate, and habitability. The C/N ratio of
the bulk silicate Earth (BSE) is superchondritic, which provides a useful tool for …
the bulk silicate Earth (BSE) is superchondritic, which provides a useful tool for …
The H2O content of the ureilite parent body
The fate of highly volatile elements (H, C, F, Cl and S) during planetary accretion and
differentiation is debated. Recent analyses of water in non-carbonaceous chondrites (RC …
differentiation is debated. Recent analyses of water in non-carbonaceous chondrites (RC …
Internal or external magma oceans in the earliest protoplanets–Perspectives from nitrogen and carbon fractionation
Protoplanets growing within∼ 1 Ma of the Solar System's formation underwent large-scale
melting due to heat released by the decay of 26 Al. When the extent of protoplanetary …
melting due to heat released by the decay of 26 Al. When the extent of protoplanetary …
[HTML][HTML] Multiple reservoirs of volatiles in the Moon revealed by the isotopic composition of chlorine in lunar basalts
JJ Barnes, IA Franchi, FM McCubbin… - … et Cosmochimica Acta, 2019 - Elsevier
The isotopes of chlorine (37 Cl and 35 Cl) are highly fractionated in lunar samples
compared to most other Solar System materials. Recently, the chlorine isotope signatures of …
compared to most other Solar System materials. Recently, the chlorine isotope signatures of …