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 …
Mineral processing and metal extraction on the lunar surface-challenges and opportunities
The lunar surface is extremely harsh and current mineral processing and metal extraction
technologies are not adequately equipped to address this environment. In this paper, we …
technologies are not adequately equipped to address this environment. In this paper, we …
Evaporation of moderately volatile elements from silicate melts: experiments and theory
Moderately volatile elements (MVEs) are sensitive tracers of vaporisation in geological and
cosmochemical processes owing to their balanced partitioning between vapour and …
cosmochemical processes owing to their balanced partitioning between vapour and …
Plausible constraints on the range of bulk terrestrial exoplanet compositions in the solar neighborhood
Rocky planet compositions regulate planetary evolution by affecting core sizes, mantle
properties, and melting behaviors. Yet, quantitative treatments of this aspect of exoplanet …
properties, and melting behaviors. Yet, quantitative treatments of this aspect of exoplanet …
Vertically Resolved Magma Ocean–Protoatmosphere Evolution: H2, H2O, CO2, CH4, CO, O2, and N2 as Primary Absorbers
The earliest atmospheres of rocky planets originate from extensive volatile release during
magma ocean epochs that occur during assembly of the planet. These establish the initial …
magma ocean epochs that occur during assembly of the planet. These establish the initial …
Atmosphere origins for exoplanet sub-neptunes
Abstract Planets with 2 R⊕< R< 3 R⊕ and orbital period< 100 days are abundant; these
sub-Neptune exoplanets are not well understood. For example, Kepler sub-Neptunes are …
sub-Neptune exoplanets are not well understood. For example, Kepler sub-Neptunes are …
Shining a hot light on emerging photoabsorber materials: The Power of rapid radiative heating in developing oxide thin-film photoelectrodes
R Gottesman, I Peracchi, JL Gerke, R Irani… - ACS Energy …, 2022 - ACS Publications
The unique possibilities of rapid thermal processing (RTP) for overcoming two significant
challenges in the development of oxide thin-film photoelectrodes are demonstrated. The first …
challenges in the development of oxide thin-film photoelectrodes are demonstrated. The first …
Volatility of sodium in carbonaceous chondrites at temperatures consistent with low-perihelion asteroids
JR Masiero, BJR Davidsson, Y Liu… - The Planetary …, 2021 - iopscience.iop.org
Solar system bodies with surface and subsurface volatiles will show observational evidence
of activity when they reach a temperature where those volatiles change from solid to gas and …
of activity when they reach a temperature where those volatiles change from solid to gas and …
Loss and fractionation of noble gas isotopes and moderately volatile elements from planetary embryos and early Venus, Earth and Mars
Here we discuss the current state of knowledge on how atmospheric escape processes can
fractionate noble gas isotopes and moderately volatile rock-forming elements that populate …
fractionate noble gas isotopes and moderately volatile rock-forming elements that populate …
New approach to prepare the highly pure ceramic precursor for the sapphire synthesis
IV Kozerozhets, GP Panasyuk, EA Semenov… - Ceramics …, 2020 - Elsevier
In the present work, a new method for the synthesis of a highly pure ceramic precursor for
the synthesis of sapphire has been developed. The method consists in hydrothermal …
the synthesis of sapphire has been developed. The method consists in hydrothermal …