Nebular dead zone effects on the D/H ratio in chondrites and comets
Mohamad Ali-Dib, Rebecca G. Martin, Jean-Marc Petit, Olivier Mousis,, Pierre Vernazza, and Jonathan I. Lunine

TL;DR
This study explores how a protoplanetary disk with a dead zone and non-monotonic temperature structure can explain the diverse D/H ratios observed in comets and chondrites, challenging classical models.
Contribution
It demonstrates that a dead zone in the disk causes temperature peaks that account for the non-monotonic D/H ratios in different small Solar System bodies.
Findings
Temperature peaks explain D/H diversity in chondritic families.
Non-monotonic D/H evolution occurs due to thermal profile.
Reversal of thermal profile is too close to the Sun to affect comets.
Abstract
Comets and chondrites show non-monotonic behaviour of their Deuterium to Hydrogen (D/H) ratio as a function of their formation location from the Sun. This is difficult to explain with a classical protoplanetary disk model that has a decreasing temperature structure with radius from the Sun. We want to understand if a protoplanetary disc with a dead zone, a region of zero or low turbulence, can explain the measured D/H values in comets and chondrites. We use time snapshots of a vertically layered disk model with turbulent surface layers and a dead zone at the midplane. The disc has a non-monotonic temperature structure due to increased heating from self-gravity in the outer parts of the dead zone. We couple this to a D/H ratio evolution model in order to quantify the effect of such thermal profiles on D/H enrichment in the nebula. We find that the local temperature peak in the disk…
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Taxonomy
TopicsAstro and Planetary Science · Molecular Spectroscopy and Structure · Spacecraft and Cryogenic Technologies
