All chondrites accreted∼ 3.5 wt.% C in their matrices, the bulk of which was in a
macromolecular solvent and acid insoluble organic material (IOM). Similar material to IOM is …

From the frontiers of research on ice dynamics in its broadest sense, this review surveys the
structures of ice, the patterns or morphologies it may assume, and the physical and chemical …

Presented here are the observations and interpretations from a comprehensive analysis of
16 representative particles returned from the C-type asteroid Ryugu by the Hayabusa2 …

Here we introduce the interstellar dust modelling framework THEMIS (The Heterogeneous
dust Evolution Model for Interstellar Solids), which takes a global view of dust and its …

A brief introduction and overview of the astrochemistry of dust, ice and gas and their
interplay is presented. The importance of basic chemical physics studies of critical reactions …

We have analyzed the chemically and isotopically well‐characterized insoluble organic
matter (IOM) extracted from 51 unequilibrated chondrites (8 CR, 9 CM, 1 CI, 3 ungrouped C …

The space environment is regularly used for experiments addressing astrobiology research
goals. The specific conditions prevailing in Earth orbit and beyond, notably the radiative …

Insoluble Organic Matter (IOM) found in primitive meteorites was formed in the Early Solar
System and subsequently processed on the parent asteroids. The location, temporal …

Context. The properties of hydrogenated amorphous carbon (aC: H) dust are known to
evolve in response to the local conditions. Aims. We present an adaptable model for the …

Simple Summary Organic matter is an integral part of all living things on our planet, but
abiotic (not relating to life) organic matter can be found throughout the Solar System within …