| Reference Type | Journal (article/letter/editorial) |
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| Title | Cosmochlore—a new examination |
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| Journal | Mineralogical Magazine | ISSN | 0026-461X |
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| Authors | Couper, A. G. | Author |
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| Hey, M. H. | Author |
| Hutchison, R. | Author |
| Year | 1981 (September) | Volume | 44 |
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| Issue | 335 |
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| Publisher | Mineralogical Society |
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| Download URL | https://rruff.info/doclib/MinMag/Volume_44/44-335-265.pdf+ |
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| DOI | doi:10.1180/minmag.1981.044.335.04Search in ResearchGate |
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| Generate Citation Formats |
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| Mindat Ref. ID | 3269 | Long-form Identifier | mindat:1:5:3269:2 |
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| GUID | 0 |
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| Full Reference | Couper, A. G., Hey, M. H., Hutchison, R. (1981) Cosmochlore—a new examination. Mineralogical Magazine, 44 (335) 265-267 doi:10.1180/minmag.1981.044.335.04 |
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| Plain Text | Couper, A. G., Hey, M. H., Hutchison, R. (1981) Cosmochlore—a new examination. Mineralogical Magazine, 44 (335) 265-267 doi:10.1180/minmag.1981.044.335.04 |
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| In | (1981, September) Mineralogical Magazine Vol. 44 (335) Mineralogical Society |
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| Abstract/Notes | AbstractExamination of cotype cosmochlore from the Toluca meteorite confirms Laspeyres's observations (1897) in every respect, except that what he determined as iron was largely titanium. His data are completed by an electron-probe analysis and by full optical and X-ray data. Accepting the identity of cosmochlore and ureyite, the optical data of Frondel and Klein (1965) for the latter are partly in error or misprinted. |
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