Engineering Papers⌕ Search

SEARCH · Engineering Papers

Results for “Co3S”

Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.

Materials Data on Co3S by Materials Project

Co3S is beta Cu3Ti-like structured and crystallizes in the hexagonal P6_3/mmc space group. The structure is three-dimensional. Co is bonded to eight equivalent Co and four equivalent S atoms to form distorted CoCo8S4 cuboctahedra that share corners with four equivalent SCo12 cuboctahedra, corners with fourteen equivalent CoCo8S4 cuboctahedra, edges with six equivalent SCo12 cuboctahedra, edges with twelve equivalent CoCo8S4 cuboctahedra, faces with four equivalent SCo12 cuboctahedra, and faces with sixteen equivalent CoCo8S4 cuboctahedra. There are a spread of Co–Co bond distances ranging from 2.47–2.60 Å. There are two shorter (2.46 Å) and two longer (2.58 Å) Co–S bond lengths. S is bonded to twelve equivalent Co atoms to form SCo12 cuboctahedra that share corners with six equivalent SCo12 cuboctahedra, corners with twelve equivalent CoCo8S4 cuboctahedra, edges with eighteen equivalent CoCo8S4 cuboctahedra, faces with eight equivalent SCo12 cuboctahedra, and faces with twelve equivalent CoCo8S4 cuboctahedra.

36 MATERIALS SCIENCE↗

Cosmic Ray Exposure Ages, Bulk and Isotopic H, C, and N Compositions of Dominion Range (DOM) CO3 Carbonaceous Chondrites and Implications for Pairing

Over 20 CO3 chondrites have been re-covered in the Dominion Range (DOM) dense collection area (DCA) of the Transantarctic Mountains by ANSMET (Antarctic Search for Meteorites) across 6 field seasons. Because of the significant masses involved and huge community interest in the most primitive samples of all carbonaceous chondrite classes such as the CO3s, we have undertaken a de-tailed assessment of the pairings and petrologic types using field relations, macroscopic observations, petrography, olivine compositions, and bulk and isotopic H, C, N compositions, and noble gas abundances and isotopes for cosmic ray exposure (CRE) ages, for all specimens. Most recently, teams during the 2018-19 and 2019-20 seasons recovered 10 new CO3 samples. Here we report new H, C, and N bulk and isotopic data, as well as CRE ages, for these 10 samples and DOM 10900 (which has some unique properties and may not be a CO chondrite). This completes the characterization of all known CO3s from DOM, allowing a thorough assessment of possible pairing relations.

chondrite↗