Plessite formation by discontinuous precipitation reaction from γ-Fe,Ni in Richardton (H5) ordinary chondrite / Grokhovsky V.J., Bevan A.W.R. // Nature. - 1983. - V. 301, l. 5898. - P. 322-324.

ISSN:
00280836
Type:
Article
Abstract:
Discontinuous precipitation reactions involve the growth of stable phases behind a grain boundary migrating into a supersaturated solid-solution 1, and have been synthesized in Fe,Ni alloys at temperatures ≥500°C (ref. 2). Axon and Grokhovsky3 have recently described localized, low temperature (350-400°C) discontinuous precipitation reactions of the type α→[α + γ] (ref. 2) occurring naturally in initially slowly cooled α-Fe,Ni (kamacite) in the Richardton H-group ordinary chondrite. In this further study of the same meteorite we describe a complementary discontinuous precipitation reaction in zoned γ-Fe,Ni (taenite) which has produced plessite (α+ γ-Fe,Ni). Microscopic discontinuous precipitation reactions in Richardton metal occurred at lower temperatures (350°C) and, in the case of zoned γ-taenite, at higher Ni contents than those synthesized in the laboratory2. We suggest that discontinuous precipitation may be an important mechanism for the production of plessite in strained then annealed, or shock reheated, meteorites. © 1983 Nature Publishing Group.
Author keywords:
Index keywords:
нет данных
DOI:
10.1038/301322a0
Смотреть в Scopus:
https://www.scopus.com/inward/record.uri?eid=2-s2.0-1542323930&doi=10.1038%2f301322a0&partnerID=40&md5=b3faa873d60275f5ea41be5a12c0d79a
Соавторы в МНС:
Другие поля
Поле Значение
Link https://www.scopus.com/inward/record.uri?eid=2-s2.0-1542323930&doi=10.1038%2f301322a0&partnerID=40&md5=b3faa873d60275f5ea41be5a12c0d79a
Affiliations Physico-Technical Department, Urals Polytechnical Institute, Sverdlovsk 620002, Russian Federation; Department of Mineralogy, British Museum (Natural History), Cromwell Road, London SW7 5BD, United Kingdom
References Williams, D., Butler, E.P., (1981) Int. Metal. Rev, 26, pp. 153-183; Predel, B., Gust, W., (1972) Arch. Bisenhütt, 43, pp. 657-663; Axon, H.J., Grokhovsky, V.J., (1982) Nature, 29, pp. 835-837; Goldstein, J.I., Ogilvie, R.E., (1965) Geochim. Cosmochim. Acta, 29, pp. 893-920; Goldstein, J.I., Axon, H.I., (1973) Naturwissenschaften, 60, pp. 313-321; Wood, J.A., (1964) Icarus, 3, pp. 429-459; Wood, J.A., (1967) Icarus, 6, pp. 1-49; Massalski, T.B., Park, F.R., Vassamillet, L.F., (1966) Geochim. Cosmochim. Acta, 30, pp. 649-662; Lin, L.S., Goldstein, J.I., Williams, D.B., (1979) Geochim. Cosmochim. Acta, 43, pp. 725-737; Buchwald, V.F., (1966) Acta Polytechn. Scand, 51, pp. 1-46; Scott, E.R.D., (1973) Geochim. Cosmochim. Acta, 37, pp. 2283-2294; Romig, A.D., Goldstein, J.I., (1981) Geochim. Cosmochim. Acta, 4 S, pp. 1187-1197; Buchwald, V.F., (1975) Handbook of Iron Meteorites, , (University of California Press, Berkeley; Sears, D.W., Ashworth, J.R., Broadbent, C.P., Bevan, A.W.R., Geochim. Cosmochim. Acta; Taylor, G.J., Heymann, D., (1970) Geochim. Cosmochim. Acta, 34, pp. 677-687; Taylor, G.J., Heymann, D., (1971) J. Geophys. Res, 76, pp. 1879-1893; Fodor, R.V., Keil, K., (1976) Geochim. Cosmochim. Acta, 40, pp. 177-189
Correspondence Address Grokhovsky, V.J.; Physico-Technical Department, Urals Polytechnical Institute, Sverdlovsk 620002, Russian Federation
Language of Original Document English
Source Scopus