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Compositional and spectroscopic investigation of three ungrouped carbonaceous chondrites
Meteoritics & Planetary Science, 2022Ungrouped carbonaceous chondrites are not easily classified into one of the well‐established groups due to compositional/petrological differences and geochemical anomalies.
M. Yeşiltaş +6 more
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RAMAN-GEOTHERMOMETER FOR CARBONACEOUS CHONDRITES
Доклады Российской академии наук. Физика, технические науки, 2023Samples of the Murchison meteorite (carbonaceous chondrite, type CM2) were kept isothermally in a specially designed device at temperatures of 200, 500 and 800°C. After the samples cooled down in an inert helium atmosphere, Raman scattering spectra were taken.
S. A. Voropaev +2 more
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The surprising thermal properties of CM carbonaceous chondrites
Meteoritics and Planetary Science, 2020Measurements of the low‐temperature thermodynamic and physical properties of meteorites provide fundamental data for the study and understanding of asteroids and other small bodies.
C. Opeil +3 more
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Amino acids in carbonaceous chondrites
Origins of Life, 1974For almost 20 years laboratory experiments have advanced the concepts of chemical evolution, particularly with regard to formation of the amino acids. What has been generally lacking is concrete natural evidence for this chemical evolution hypothesis.
J G, Lawless, E, Peterson
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Meteoritics and Planetary Science, 2020
Evaluating the water‐soluble organic composition of carbonaceous chondrites is key to understanding the inventory of organic matter present at the origins of the solar system and the subsequent processes that took place inside asteroid parent bodies ...
J. Aponte +9 more
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Evaluating the water‐soluble organic composition of carbonaceous chondrites is key to understanding the inventory of organic matter present at the origins of the solar system and the subsequent processes that took place inside asteroid parent bodies ...
J. Aponte +9 more
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Carbonaceous Chondrites and the Condensation of Elements from the Solar Nebula
Astrophysical Journal, 2020Common features of all carbonaceous chondrite groups are invariant refractory element ratios, depletions of moderately volatile elements as a function of their condensation temperature (TC), and strongly depleted highly volatile element concentrations ...
H. Vollstaedt, K. Mezger, Y. Alibert
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Deuterium in carbonaceous chondrites
Earth and Planetary Science Letters, 1980Hydrogen isotopic compositions in seven carbonaceous chondrites lie in the range -70 to +771 per thousand relative to standard mean ocean water. These values decrease, to a range from -145 to +219 per thousand, after low-temperature oxidation in an oxygen plasma.
Y KOLODNY, J KERRIDGE, I KAPLAN
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Xenon in Carbonaceous Chondrites
Nature Physical Science, 1972Carbonaceous chondrites contain two isotopically distinct components of trapped xenon which cannot be explained by the occurrence of nuclear or fractionation processes within these meteorites.
O. K. MANUEL, E. W. HENNECKE, D. D. SABU
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Matrices of Carbonaceous Chondrite Meteorites
Annual Review of Earth and Planetary Sciences, 1993The morphology, classification, and chemistry of the matrices of carbonaceous chondrite (CC) meteorites is reviewed based on recent research results. The various kinds of CCs are examined in terms of their matrix mineralogy. Alteration processes in CCs are discussed.
P R Buseck, X Hua
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The ultraviolet spectra of carbonaceous chondrites
Celestial Mechanics and Dynamical Astronomy, 1992Optical spectroscopy of meteorites is an important laboratory tool for the study of the origin and evolution of solar and galactic interstellar minor bodies. In the region from the visible to the ultraviolet, the absorption spectra have hitherto been measured on the Bruderheim (Egan and Hilgeman, 1975), the Orgueil (Huffman, 1977), the Murchison ...
T. Inagaki, S. Yabushita, K. Wada
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