Radial and vertical dust transport inhibit refractory carbon depletion in protoplanetary disks

TL;DR

This study evaluates how vertical and radial dust transport in protoplanetary disks affects refractory carbon removal, finding that radial transport prevents depletion and other mechanisms are needed for observed carbon levels.

Contribution

It provides a detailed model of dust transport and assesses the effectiveness of oxidation and photolysis in depleting refractory carbon in disks.

Findings

Vertical transport can enable carbon removal in certain conditions.

Radial transport prevents depletion, maintaining uniform carbon distribution.

Surface mechanisms alone are insufficient to explain observed carbon depletion.

Abstract

The Earth is strongly depleted in carbon compared to the dust in the ISM, implying efficient removal of refractory carbon before parent body formation. It has been argued that grains get rid of their carbon through oxidation and photolysis in the exposed upper disk layers. We assess the efficacy of these C-removal mechanisms accounting for the vertical and radial transport of grains. We obtain the carbon and carbon free mass budget of solids by solving two 1D advection-diffusion equations, accounting for the dust grain size distribution and radial transport. The carbon removal acts on the fraction of the grains that are in the exposed layer and requires efficient vertical transport. In models without radial transport, oxidation and photolysis can destroy most of the refractory carbon in terrestrial planet formation region. But it only reaches the observed depletion levels for extreme parameter combinations and requires that parent body formation was delayed by 1 Myr. Adding radial transport of solids prevents the depletion entirely, leaving refractory carbon equally distributed throughout the disk. It is unlikely that the observed carbon depletion can ultimately be attributed to mechanisms operating on small grains in the disk surface layers. Other mechanisms need to be studied, for example flash heating events or FU Ori outbursts in order to remove carbon quickly and deeply. However, a sustained drift barrier or strongly reduced radial grain mobility are necessary to prevent replenishment of carbon from the outer disk.