Water UV-Shielding in the Terrestrial Planet-Forming Zone: Implications for Oxygen-18 Isotope Anomalies in H2-18O Infrared Emission and Meteorites
Jenny K. Calahan, Edwin A. Bergin, Arthur D. Bosman

TL;DR
This study models water vapor distribution in protoplanetary disks, revealing how water self-shielding affects isotopic ratios and potentially explains oxygen isotope anomalies in meteorites.
Contribution
It introduces a model accounting for water self-shielding, showing its impact on H2-18O distribution and implications for interpreting isotopic anomalies in planetary formation.
Findings
H2-18O is enhanced in the upper layers of the disk within 0.1-10 au due to self-shielding.
Most JWST-observable H2-18O transitions originate from this enriched layer.
Self-shielding may explain oxygen isotope anomalies in meteoritic material.
Abstract
An understanding of the abundance and distribution of water vapor in the innermost region of protoplanetary disks is key to understanding the origin of habitable worlds and planetary systems. Past observations have shown H2O to be abundant and a major carrier of elemental oxygen in disk surface layers that lie within the inner few au of the disk. The combination of high abundance and strong radiative transitions leads to emission lines that are optically thick across the infrared spectral range. Its rarer isotopologue H2-18O traces deeper into this layer and will trace the full content of the planet forming zone. In this work, we explore the relative distribution of H2-16O and H2-18O within a model that includes water self-shielding from the destructive effects of ultraviolet radiation. In this Letter we show that there is an enhancement in the relative H2-18O abundance high up in the…
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Taxonomy
TopicsAstro and Planetary Science · Isotope Analysis in Ecology · Planetary Science and Exploration
