Results 131 to 140 of about 43,521 (279)
Correlated analyses of D- and 15N-rich carbon grains from CR2 chondrite EET 92042 [PDF]
Extract from introduction: Insoluble organic matter (IOM) and matrix from primitive carbonaceous chondrites carry isotope enrichments (?D?20000', ?15N?3200�) that are comparable to those in interplanetary dust particles [1, this work]. Hence, primitive
Alexander, C. M. O'D. +7 more
core
Primitive meteorite groups such as the Vigarano, Mighei, and Karoonda carbonaceous chondrites have enigmatic patterns of elemental abundances, with moderately volatile elements—those that transition from vapor to condensate between ∼400 and ∼900 K ...
Jeremy W. Boyce +3 more
doaj +1 more source
Pułtusk H5 Chondrite—A Compilation of Chemical, Physical, and Thermophysical Data
The Pułtusk meteorite, classified as an H5 ordinary chondrite, is one of the best documented Polish falls, yet some important data on its physical and thermophysical properties remain limited.
Katarzyna Łuszczek, Radosław A. Wach
doaj +1 more source
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
doaj +1 more source
Variations in the nucleosynthetic isotope compositions of meteorites have been suggested to result from variable destruction of some presolar grains through thermal processing.
Rayssa Martins +5 more
doaj +1 more source
Non-equilibrium condensation of the first Solar System solids. [PDF]
Charnoz S +5 more
europepmc +1 more source
Method Development for the Analysis of Carbonaceous Chondrites by Laser Desorption/Ionization and Secondary Ion Time-of-Flight Mass Spectrometry. [PDF]
Rados E, Frank J, Pittenauer E.
europepmc +1 more source
Data-driven classification of ordinary chondrites and asteroidal metal potential evaluation. [PDF]
Liu TY +5 more
europepmc +1 more source

