A framework for the origin and deep cycles of volatiles in rocky exoplanets
R Dasgupta, D Pathak… - Reviews in Mineralogy …, 2024 - pubs.geoscienceworld.org
Since the first discovery of planets in another solar system of our galaxy in the early 90s and
the discovery of 51 Pegassi b, a Jovian-type planet around a Sun-like star in 1995 (Mayor …
the discovery of 51 Pegassi b, a Jovian-type planet around a Sun-like star in 1995 (Mayor …
Magma ocean evolution at arbitrary redox state
Interactions between magma oceans and overlying atmospheres on young rocky planets
leads to an evolving feedback of outgassing, greenhouse forcing, and mantle melt fraction …
leads to an evolving feedback of outgassing, greenhouse forcing, and mantle melt fraction …
Role of magma oceans in controlling carbon and oxygen of sub-Neptune atmospheres
C Seo, Y Ito, Y Fujii - The Astrophysical Journal, 2024 - iopscience.iop.org
Most exoplanets with a few Earth radii are more inflated than bare-rock planets with the
same mass, indicating a substantial volatile amount. Neither the origin of the volatiles nor …
same mass, indicating a substantial volatile amount. Neither the origin of the volatiles nor …
The fate of nitrogen during early silicate differentiation of rocky bodies constrained by experimental mineral-melt partitioning
A Pal, R Dasgupta - Geochimica et Cosmochimica Acta, 2024 - Elsevier
Nitrogen (N) is an essential element for life. Yet the processes of planet formation and early
planetary evolution through which rocky planets like Earth obtained their atmospheric and …
planetary evolution through which rocky planets like Earth obtained their atmospheric and …