The stable carbon isotopes in enstatite chondrites and Cumberland Falls
DOI | 10.1016/0016-7037(85)90193-0 |
---|---|
Aasta | 1985 |
Ajakiri | Geochimica et Cosmochimica Acta |
Köide | 49 |
Number | 1 |
Leheküljed | 89-95 |
Tüüp | artikkel ajakirjas |
Keel | inglise |
Id | 23898 |
Abstrakt
The carbon isotopic composition of the total carbon in the enstatite chondrites Indarch, Abee, St. Marks, Pillistfer, Hvittis and Daniel's Kuil and the enstatite achondrite Cumberland Falls has been measured. The empirical relationhip between carbon isotopic composition and total carbon content is distinct from that of carbonaceous and ordinary chondrites. Within the enstatite chondrite group the average 13C content increases with petrographic type: E4 < E5 < E6. Daniel's Kuil shows the largest 13C enrichment in the bulk carbon of any meteorite. The carbon isotopic composition is most clearly correlated with the abundance of the elements Zn, Cd and In. Insofar as these elements may hold the key to the understanding of enstatite chondrites, more detailed combined carbon isotope and trace element studies of these meteorites will play an important role in the deciphering of their history.