Meteoritic Tutton salt, a naturally inspired reservoir of cometary and asteroidal ammonium

TL;DR

This study identifies a naturally occurring mineral, nickeloan boussingaultite, as a reservoir of ammonium in meteorites, providing new insights into the composition of cometary and asteroidal bodies.

Contribution

It reports the discovery of a mineral carrier of meteoritic ammonium, linking it to cometary and asteroidal compositions and spectral characteristics.

Findings

Nickeloan boussingaultite occurs in the Orgueil meteorite.

It is chemically related to Tutton salts and acts as an ammonium reservoir.

Spectroscopic data support its role in cometary and asteroid environments.

Abstract

The lack of benchmark data on the real minerals, native ammonium carriers in Solar System gives rise to controversial opinions on extraterrestrial ammonium reservoirs. We herein report on discovery of the first mineral carrier of meteoritic ammonium and show its relevance to the compositional and spectral characteristics of cometary and asteroidal bodies. Chemically distant from previously inferred volatile organics or ammoniated phyllosilicates, it is an aqueous metal-ammonium sulfate related to a family of so-called Tutton salts. Nickeloan boussingaultite, (NH4)2(Mg,Ni)(SO4)2 6H2O, occurs in Orgueil, a primitive carbonaceous chondrite closely related to (162173) Ryugu and (101955) Bennu, the C-type asteroids. The available spectroscopic, chemical and mineralogical data signify that natural Tutton salts perfectly fit into the role of ammonium reservoir under conditions of cometary nuclei and carbonaceous asteroids.