Results 61 to 70 of about 441 (171)
Over the possible role of metal atom clusters in cosmochemistry and in the origin of life
We present here the hypothesis of a possible relationship between metal atom clusters and the formation of organic molecules in the interstellar medium and on small bodies as a possible pathway to the origin of such molecules.
Silvio Dioses Castro, Richard Korswagen
doaj
Oxygen Isotope Exchange between Dust Aggregates and Ambient Nebular Gas
Meteorites and their components exhibit a diverse range of oxygen isotope compositions, and the isotopic exchange timescale between dust grains and ambient gas is a key parameter for understanding the spatiotemporal evolution of the solar nebula. As dust
Sota Arakawa +4 more
doaj +1 more source
The discovery of extreme strontium isotope anomalies ( μ ^84 Sr) in refractory leachates from Allende fine-grained calcium-aluminum-rich inclusions (CAIs) is at odds with long-standing predictions regarding the homogenization of presolar components in ...
R. T. C. Marquez +2 more
doaj +1 more source
Revisiting a Chemical Route to the Formation of CN− in the Interstellar Medium
We discuss the HCN + H ^− reaction as a path to the formation of CN ^− , the smallest cyanopolyyne anion observed in several interstellar environments.
Pablo del Mazo-Sevillano +5 more
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The analysis of samples returned from the C-type asteroid Ryugu has drastically advanced our knowledge of the evolution of early solar system materials.
Ryoji Tanaka +25 more
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87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source
Automated identification of soil functional components based on NanoSIMS data
NanoSIMS technique allows to investigate the micro-spatial organization in complex structures in multiple scientific fields such as material science, cosmochemistry, and biogeochemistry. In soil biogeochemistry applications, NanoSIMS-based approaches aim
Yahan Hu +4 more
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Compositions of carbonaceous-type asteroidal cores in the early solar system. [PDF]
Zhang B, Chabot NL, Rubin AE.
europepmc +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
The bulk planetary compositions are thought to be consistent with the chemical abundances of their host stars. The abundances of eight key rock-forming elements and the key planetary abundance ratios in G- and F-type main sequence stars located in the ...
Futó Péter, Gucsik Arnold
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