The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Organic Compounds in Meteorites: They may have formed in the solar nebula, by catalytic reactions of carbon monoxide, hydrogen, and ammonia.
Abstract
Organic compounds in meteorites seem to have formed by catalytic reactions of CO, H 2 , and NH 3 in the solar nebula, at 360° to 400°K and (4 to 10) × 10 -6 atm. The onset of these reactions was triggered by the formation of suitable catalysts (magnetite, hydrated silicates) at these temperatures. These reactions may be a source of prebiotic carbon compounds on the inner planets, and interstellar molecules.
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Citations
Cites
A Production of Amino Acids Under Possible Primitive Earth Conditions
Miller, S. L. (1953) · Science · doi:10.1126/science.117.3046.528 · Cited by 3,522
Production of Some Organic Compounds under Possible Primitive Earth Conditions1
Miller, S. L. (1955) · Journal of the American Chemical Society · doi:10.1021/ja01614a001 · Cited by 827
Wolman, Y., Haverland, W. J., & Miller, S. L. (1972) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.69.4.809 · Cited by 198
Cited by
Pre-biotic organic matter from comets and asteroids
Anders, E. (1989) · Nature · doi:10.1038/342255a0 · Cited by 421
Self-citationDeamer, D. W., & Pashley, R. M. (1989) · Origins of life and evolution of the biosphere · doi:10.1007/bf01808285 · Cited by 272
Boundary structures are formed by organic-components of the Murchison carbonaceous chondrite
Deamer, D. W. (1985) · Nature · doi:10.1038/317792a0 · Cited by 270
Peltzer, E. T., Bada, J. L., Schlesinger, G., & Miller, S. L. (1984) · Advances in Space Research · doi:10.1016/0273-1177(84)90546-5 · Cited by 262
Serpentinization and the Formation of H 2 and CH 4 on Celestial Bodies (Planets, Moons, Comets)
Holm, N. G., Oze, C., Mousis, O., Waite, J. H., & Guilbert-Lepoutre, A. (2015) · Astrobiology · doi:10.1089/ast.2014.1188 · Cited by 187
Metadata
- Authors
- Anders, E., Hayatsu, R., & Studier, M. H.
- Venue
- Science
- Published
- 1973-11-23
- Volume
- 182
- Issue
- 4114
- Pages
- 781-790
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W1967822922
- Cited by
- 230
- References
- 3
- FWCI
- 15.19
- Type
- journal article
- Language
- en
- Open access
- closed
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- The paper
- Anders, E., Hayatsu, R., & Studier, M. H. (1973). Organic Compounds in Meteorites: They may have formed in the solar nebula, by catalytic reactions of carbon monoxide, hydrogen, and ammonia. Science. https://doi.org/10.1126/science.182.4114.781
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
