The nature, origin and modification of insoluble organic matter in chondrites, the major source of Earth's C and N

CMOD Alexander, GD Cody, BT De Gregorio, LR Nittler… - Geochemistry, 2017 - Elsevier
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 …

On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective

E Nakamura, K Kobayashi, R Tanaka… - Proceedings of the …, 2022 - jstage.jst.go.jp
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 …

Macromolecular organic matter in samples of the asteroid (162173) Ryugu

H Yabuta, GD Cody, C Engrand, Y Kebukawa… - Science, 2023 - science.org
Samples of the carbonaceous asteroid (162173) Ryugu were collected and brought to Earth
by the Hayabusa2 spacecraft. We investigated the macromolecular organic matter in Ryugu …

Accretion of water in carbonaceous chondrites: Current evidence and implications for the delivery of water to early Earth

JM Trigo-Rodríguez, A Rimola, S Tanbakouei… - Space Science …, 2019 - Springer
Protoplanetary disks are dust-rich structures around young stars. The crystalline and
amorphous materials contained within these disks are variably thermally processed and …

Classification of hydrous meteorites (CR, CM and C2 ungrouped) by phyllosilicate fraction: PSD-XRD modal mineralogy and planetesimal environments

KT Howard, CMOD Alexander, DL Schrader… - … et Cosmochimica Acta, 2015 - Elsevier
The relative differences in the degree of hydration should be reflected in any classification
scheme for aqueously altered meteorites. Here we report the bulk mineralogies and degree …

Evolution of organic matter in Orgueil, Murchison and Renazzo during parent body aqueous alteration: In situ investigations

C Le Guillou, S Bernard, AJ Brearley… - … et Cosmochimica Acta, 2014 - Elsevier
Chondrites accreted the oldest solid materials in the solar system including dust processed
in the protoplanetary disk and diverse organic compounds. After accretion, asteroidal …

The key role of meteorites in the formation of relevant prebiotic molecules in a formamide/water environment

L Rotelli, JM Trigo-Rodríguez, CE Moyano-Cambero… - Scientific reports, 2016 - nature.com
We show that carbonaceous chondrite meteorites actively and selectively catalyze the
formation of relevant prebiotic molecules from formamide in aqueous media. Specific …

GEMS-like material in the matrix of the Paris meteorite and the early stages of alteration of CM chondrites

H Leroux, P Cuvillier, B Zanda, RH Hewins - Geochimica et Cosmochimica …, 2015 - Elsevier
The Paris meteorite is a weakly altered CM chondrite that has been discovered recently
(Hewins et al., 2014). Its matrix offers the opportunity to search for well-preserved pristine …

Nonequilibrium spherulitic magnetite in the Ryugu samples

E Dobrică, HA Ishii, JP Bradley, K Ohtaki… - … et Cosmochimica Acta, 2023 - Elsevier
We have investigated several particles collected during each of two touchdowns of the
Hayabusa2 spacecraft at the surface of the C-type asteroid 162173 Ryugu using various …

Carbonate abundances and isotopic compositions in chondrites

CMOD Alexander, R Bowden, ML Fogel… - … & Planetary Science, 2015 - Wiley Online Library
We report the bulk C abundances, and C and O isotopic compositions of carbonates in 64
CM chondrites, 14 CR chondrites, 2 CI chondrites, LEW 85332 (C2), Kaba (CV 3), and …