Sulfuric acid as a cryofluid and oxygen isotope reservoir of planetesimals
Akihiko Hashimoto, Yuki Nakano

TL;DR
This paper proposes that sulfuric acid in planetesimals, formed from oxygen-enriched sulfur compounds in molecular clouds, served as a cryofluid and reservoir for oxygen isotopes, explaining isotopic anomalies in meteorites.
Contribution
It introduces a novel pathway linking molecular cloud chemistry to isotopic anomalies in meteorites via sulfuric acid formation and its role in planetesimal evolution.
Findings
Sulfuric acid in planetesimals is enriched in $^{17,18}$O by 24%.
Sulfuric acid acted as a cryofluid and reacted with iron to form specific mineral structures.
The isotopic composition of meteorite symplectites is linked to sulfuric acid derived from molecular cloud chemistry.
Abstract
The Sun exhibits a depletion in O relative to O by 6 % compared to the Earth and Moon. The origin of such a non-mass-dependent isotope fractionation has been extensively debated since the three-isotope-analysis became available in 1970's. Self-shielding of CO molecules against UV photons in the solar system's parent molecular cloud has been suggested as a source of the non-mass-dependent effect, in which a O-enriched oxygen was trapped by ice and selectively incorporated as water into planet-forming materials. The truth is that the Earth-Moon and other planetary objects deviate positively from the Sun by ~6 % in their isotopic compositions. A stunning exception is the magnetite/sulfide symplectite found in Acfer 094 meteorite, which shows 24 % enrichment in O relative to the Sun. Water does not explain the enrichment…
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Taxonomy
TopicsAstro and Planetary Science · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
