Cliftonite in meteorites: A proposed origin

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Abstract

Cliftonite, a polycrystalline aggregate of graphite with cubic morphology, is known in ten meteorites. Some workers have considered it to be a pseudomorph after diamond, and have used the proposed diamond ancestry as evidence of a meteoritic parent body of at least lunar dimensions. We have synthesized cliftonite in Fe-Ni-C alloys in vacuum, as a product of decomposition of cohenite [(Fe,Ni)3C]. We therefore suggest that a high pressure origin is unnecessary for meteorites which contain cliftonite, and that these meteorites were formed at low pressures. This conclusion is in agreement with other recent evidence.

Suggested Citation

Brett, R., and Higgins, G., 1967, Cliftonite in meteorites: A proposed origin: Science, v. 156, no. 3776, p. 819-820, https://doi.org/10.1126/science.156.3776.819.

Publication type Article
Publication Subtype Journal Article
Title Cliftonite in meteorites: A proposed origin
Series title Science
DOI 10.1126/science.156.3776.819
Volume 156
Issue 3776
Year Published 1967
Language English
Publisher American Association for the Advancement of Science
Description 2 p.
First page 819
Last page 820
Additional publication details