A 3-Dimension Model of Volcanism Volatiles Contribution on Atmospheric Chemical Abundance of Habitable Planets

TL;DR

This paper develops a 3D model to understand how volcanic volatiles influence the atmospheric chemical composition of habitable planets by simulating volatile generation, diffusion, and mixing processes.

Contribution

It introduces a novel 3D diffusion model for volcanic volatiles, linking magma composition to atmospheric element abundance at various altitudes.

Findings

Quantitative models of element abundance at different heights.

Identification of key volatile species and their distribution.

Insights into volcanic contribution to planetary atmospheres.

Abstract

The volcanism plays an important part in mass exchange circle to bring matter from core of planet to atmosphere. Thus, it is a possible method to research the change of elements abundance in atmosphere by modeling the process of volatiles from volcanism get through and mix in atmosphere, which is the focused point of this article. This article penetrates from the generation of volatiles, talks the species, mass, and mole fractions of different typical elements in magma. Then a diffusion progress model of volatiles was built to quantify the abundance of elements with altitude. And the quantitative models of element abundance at different heights are obtained.