ArticleChemie der Erde : Beitrage zur chemischen Mineralogie, Petrographie und Geologie2017
The nature, origin and modification of insoluble organic matter in chondrites, the possibly interstellar source of Earth's C and N.
Article in Chemie der Erde : Beitrage zur chemischen Mineralogie, Petrographie und Geologie, 2017. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 37 papers.
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Who cites it
37 citing papers in PubMed.
- Gradual Destruction of Refractory Stardust in Alkali Brines on Asteroid Bennu.Nature communications · 2026Article
- Spatially distributed complex organic matter detected in an ancient river valley in Jezero crater, Mars.Science advances · 2026Article
- Phosphorus-nitrogen systematics of first-generation planetesimals constrain life-essential element delivery to Earth.Science advances · 2026Article
- Abiotic sugar enantiomers in the CI carbonaceous chondrite Orgueil.Nature communications · 2026Article
- Direct Samples of Interstellar and Interplanetary Material with IMAP.Space science reviews · 2026Review
- Prebiotic organic compounds in samples of asteroid Bennu indicate heterogeneous aqueous alteration.Proceedings of the National Academy of Sciences of the United States of America · 2025Article
- Carbon and oxygen isotope evidence for a protoplanetary disk origin of organic solids in meteorites.Proceedings of the National Academy of Sciences of the United States of America · 2025Article
- Low-Temperature Aqueous Alteration of Chondrites.Space science reviews · 2025Review
- The variety and origin of materials accreted by Bennu's parent asteroid.Nature astronomy · 2025Article
- Variations of organic functional chemistry in carbonaceous matter from the asteroid 162173 Ryugu.Nature communications · 2024Article
- High-spatial resolution functional chemistry of nitrogen compounds in the observed UK meteorite fall Winchcombe.Nature communications · 2024Article
- Abundant presolar grains and primordial organics preserved in carbon-rich exogenous clasts in asteroid Ryugu.Science advances · 2023Article
- Review
- Gastrointestinal microbiota profile and clinical correlations in advanced EGFR-WT and EGFR-mutant non-small cell lung cancer.BMC cancer · 2022Article
- Deuterium Isotope Fractionation of Polycyclic Aromatic Hydrocarbons in Meteorites as an Indicator of Interstellar/Protosolar Processing History.Life (Basel, Switzerland) · 2022Article
- Identification and characterization of a new ensemble of cometary organic molecules.Nature communications · 2022Article
- Glycine amino acid transformation under impacts by small solar system bodies, simulated via high-pressure torsion method.Scientific reports · 2022Article
- Visualization and identification of single meteoritic organic molecules by atomic force microscopy.Meteoritics & planetary science · 2022Article
- Exploring the link between molecular cloud ices and chondritic organic matter in laboratory.Nature communications · 2021Article
- Earth's carbon deficit caused by early loss through irreversible sublimation.Science advances · 2021Article
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Abstract
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 found in interplanetary dust particles (IDPs) and comets. The IOM accounts for almost all of the C and N in chondrites, and a significant fraction of the H. Chondrites and, to a lesser extent, comets were probably the major sources of volatiles for the Earth and the other terrestrial planets. Hence, IOM was both the major source of Earth's volatiles and a potential source of complex prebiotic molecules. Large enrichments in D and
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